1
|
Armano M, Audley H, Baird J, Binetruy P, Born M, Bortoluzzi D, Brandt N, Castelli E, Cavalleri A, Cesarini A, Cruise A, Danzmann K, de Deus Silva M, Diepholz I, Dixon G, Dolesi R, Ferraioli L, Ferroni V, Fitzsimons E, Flatscher R, Freschi M, García A, Gerndt R, Gesa L, Giardini D, Gibert F, Giusteri R, Grimani C, Grzymisch J, Guzman F, Harrison I, Hartig MS, Hechenblaikner G, Heinzel G, Hewitson M, Hollington D, Hoyland D, Hueller M, Inchauspé H, Jennrich O, Jetzer P, Johann U, Johlander B, Karnesis N, Kaune B, Killow C, Korsakova N, Lobo J, López-Zaragoza J, Maarschalkerweerd R, Mance D, Martín V, Martin-Polo L, Martin-Porqueras F, Martino J, McNamara P, Mendes J, Mendes L, Meshksar N, Monsky A, Nofrarias M, Paczkowski S, Perreur-Lloyd M, Petiteau A, Plagnol E, Ramos-Castro J, Reiche J, Rivas F, Robertson D, Russano G, Sanjuan J, Slutsky J, Sopuerta C, Steier F, Sumner T, Texier D, Thorpe J, Vetrugno D, Vitale S, Wand V, Wanner G, Ward H, Wass P, Weber W, Wissel L, Wittchen A, Zweifel P. Sensor noise in
LISA Pathfinder
: An extensive in-flight review of the angular and longitudinal interferometric measurement system. Int J Clin Exp Med 2022. [DOI: 10.1103/physrevd.106.082001] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/07/2022]
|
2
|
Pandey S, Krause E, DeRose J, MacCrann N, Jain B, Crocce M, Blazek J, Choi A, Huang H, To C, Fang X, Elvin-Poole J, Prat J, Porredon A, Secco L, Rodriguez-Monroy M, Weaverdyck N, Park Y, Raveri M, Rozo E, Rykoff E, Bernstein G, Sánchez C, Jarvis M, Troxel M, Zacharegkas G, Chang C, Alarcon A, Alves O, Amon A, Andrade-Oliveira F, Baxter E, Bechtol K, Becker M, Camacho H, Campos A, Carnero Rosell A, Carrasco Kind M, Cawthon R, Chen R, Chintalapati P, Davis C, Di Valentino E, Diehl H, Dodelson S, Doux C, Drlica-Wagner A, Eckert K, Eifler T, Elsner F, Everett S, Farahi A, Ferté A, Fosalba P, Friedrich O, Gatti M, Giannini G, Gruen D, Gruendl R, Harrison I, Hartley W, Huff E, Huterer D, Kovacs A, Leget P, McCullough J, Muir J, Myles J, Navarro-Alsina A, Omori Y, Rollins R, Roodman A, Rosenfeld R, Sevilla-Noarbe I, Sheldon E, Shin T, Troja A, Tutusaus I, Varga T, Wechsler R, Yanny B, Yin B, Zhang Y, Zuntz J, Abbott T, Aguena M, Allam S, Annis J, Bacon D, Bertin E, Brooks D, Burke D, Carretero J, Conselice C, Costanzi M, da Costa L, Pereira M, De Vicente J, Dietrich J, Doel P, Evrard A, Ferrero I, Flaugher B, Frieman J, García-Bellido J, Gaztanaga E, Gerdes D, Giannantonio T, Gschwend J, Gutierrez G, Hinton S, Hollowood D, Honscheid K, James D, Jeltema T, Kuehn K, Kuropatkin N, Lahav O, Lima M, Lin H, Maia M, Marshall J, Melchior P, Menanteau F, Miller C, Miquel R, Mohr J, Morgan R, Palmese A, Paz-Chinchón F, Petravick D, Pieres A, Plazas Malagón A, Sanchez E, Scarpine V, Serrano S, Smith M, Soares-Santos M, Suchyta E, Tarle G, Thomas D, Weller J. Dark Energy Survey year 3 results: Constraints on cosmological parameters and galaxy-bias models from galaxy clustering and galaxy-galaxy lensing using the redMaGiC sample. Int J Clin Exp Med 2022. [DOI: 10.1103/physrevd.106.043520] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/07/2022]
|
3
|
Abbott T, Aguena M, Alarcon A, Allam S, Alves O, Amon A, Andrade-Oliveira F, Annis J, Avila S, Bacon D, Baxter E, Bechtol K, Becker M, Bernstein G, Bhargava S, Birrer S, Blazek J, Brandao-Souza A, Bridle S, Brooks D, Buckley-Geer E, Burke D, Camacho H, Campos A, Carnero Rosell A, Carrasco Kind M, Carretero J, Castander F, Cawthon R, Chang C, Chen A, Chen R, Choi A, Conselice C, Cordero J, Costanzi M, Crocce M, da Costa L, da Silva Pereira M, Davis C, Davis T, De Vicente J, DeRose J, Desai S, Di Valentino E, Diehl H, Dietrich J, Dodelson S, Doel P, Doux C, Drlica-Wagner A, Eckert K, Eifler T, Elsner F, Elvin-Poole J, Everett S, Evrard A, Fang X, Farahi A, Fernandez E, Ferrero I, Ferté A, Fosalba P, Friedrich O, Frieman J, García-Bellido J, Gatti M, Gaztanaga E, Gerdes D, Giannantonio T, Giannini G, Gruen D, Gruendl R, Gschwend J, Gutierrez G, Harrison I, Hartley W, Herner K, Hinton S, Hollowood D, Honscheid K, Hoyle B, Huff E, Huterer D, Jain B, James D, Jarvis M, Jeffrey N, Jeltema T, Kovacs A, Krause E, Kron R, Kuehn K, Kuropatkin N, Lahav O, Leget PF, Lemos P, Liddle A, Lidman C, Lima M, Lin H, MacCrann N, Maia M, Marshall J, Martini P, McCullough J, Melchior P, Mena-Fernández J, Menanteau F, Miquel R, Mohr J, Morgan R, Muir J, Myles J, Nadathur S, Navarro-Alsina A, Nichol R, Ogando R, Omori Y, Palmese A, Pandey S, Park Y, Paz-Chinchón F, Petravick D, Pieres A, Plazas Malagón A, Porredon A, Prat J, Raveri M, Rodriguez-Monroy M, Rollins R, Romer A, Roodman A, Rosenfeld R, Ross A, Rykoff E, Samuroff S, Sánchez C, Sanchez E, Sanchez J, Sanchez Cid D, Scarpine V, Schubnell M, Scolnic D, Secco L, Serrano S, Sevilla-Noarbe I, Sheldon E, Shin T, Smith M, Soares-Santos M, Suchyta E, Swanson M, Tabbutt M, Tarle G, Thomas D, To C, Troja A, Troxel M, Tucker D, Tutusaus I, Varga T, Walker A, Weaverdyck N, Wechsler R, Weller J, Yanny B, Yin B, Zhang Y, Zuntz J. Dark Energy Survey Year 3 results: Cosmological constraints from galaxy clustering and weak lensing. Int J Clin Exp Med 2022. [DOI: 10.1103/physrevd.105.023520] [Citation(s) in RCA: 106] [Impact Index Per Article: 53.0] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/07/2022]
|
4
|
Amon A, Gruen D, Troxel M, MacCrann N, Dodelson S, Choi A, Doux C, Secco L, Samuroff S, Krause E, Cordero J, Myles J, DeRose J, Wechsler R, Gatti M, Navarro-Alsina A, Bernstein G, Jain B, Blazek J, Alarcon A, Ferté A, Lemos P, Raveri M, Campos A, Prat J, Sánchez C, Jarvis M, Alves O, Andrade-Oliveira F, Baxter E, Bechtol K, Becker M, Bridle S, Camacho H, Carnero Rosell A, Carrasco Kind M, Cawthon R, Chang C, Chen R, Chintalapati P, Crocce M, Davis C, Diehl H, Drlica-Wagner A, Eckert K, Eifler T, Elvin-Poole J, Everett S, Fang X, Fosalba P, Friedrich O, Gaztanaga E, Giannini G, Gruendl R, Harrison I, Hartley W, Herner K, Huang H, Huff E, Huterer D, Kuropatkin N, Leget P, Liddle A, McCullough J, Muir J, Pandey S, Park Y, Porredon A, Refregier A, Rollins R, Roodman A, Rosenfeld R, Ross A, Rykoff E, Sanchez J, Sevilla-Noarbe I, Sheldon E, Shin T, Troja A, Tutusaus I, Tutusaus I, Varga T, Weaverdyck N, Yanny B, Yin B, Zhang Y, Zuntz J, Aguena M, Allam S, Annis J, Bacon D, Bertin E, Bhargava S, Brooks D, Buckley-Geer E, Burke D, Carretero J, Costanzi M, da Costa L, Pereira M, De Vicente J, Desai S, Dietrich J, Doel P, Ferrero I, Flaugher B, Frieman J, García-Bellido J, Gaztanaga E, Gerdes D, Giannantonio T, Gschwend J, Gutierrez G, Hinton S, Hollowood D, Honscheid K, Hoyle B, James D, Kron R, Kuehn K, Lahav O, Lima M, Lin H, Maia M, Marshall J, Martini P, Melchior P, Menanteau F, Miquel R, Mohr J, Morgan R, Ogando R, Palmese A, Paz-Chinchón F, Petravick D, Pieres A, Romer A, Sanchez E, Scarpine V, Schubnell M, Serrano S, Smith M, Soares-Santos M, Tarle G, Thomas D, To C, Weller J. Dark Energy Survey Year 3 results: Cosmology from cosmic shear and robustness to data calibration. Int J Clin Exp Med 2022. [DOI: 10.1103/physrevd.105.023514] [Citation(s) in RCA: 42] [Impact Index Per Article: 21.0] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/07/2022]
|
5
|
Armano M, Audley H, Baird J, Binetruy P, Born M, Bortoluzzi D, Brandt N, Castelli E, Cavalleri A, Cesarini A, Cruise AM, Danzmann K, de Deus Silva M, Diepholz I, Dixon G, Dolesi R, Ferraioli L, Ferroni V, Fitzsimons ED, Flatscher R, Freschi M, García A, Gerndt R, Gesa L, Giardini D, Gibert F, Giusteri R, Grimani C, Grzymisch J, Guzman F, Harrison I, Hartig MS, Heinzel G, Hewitson M, Hollington D, Hoyland D, Hueller M, Inchauspé H, Jennrich O, Jetzer P, Johann U, Johlander B, Karnesis N, Kaune B, Killow CJ, Korsakova N, Lobo JA, Liu L, López-Zaragoza JP, Maarschalkerweerd R, Mance D, Martín V, Martin-Polo L, Martin-Porqueras F, Martino J, McNamara PW, Mendes J, Mendes L, Meshksar N, Monsky A, Nofrarias M, Paczkowski S, Perreur-Lloyd M, Petiteau A, Pivato P, Plagnol E, Ramos-Castro J, Reiche J, Rivas F, Robertson DI, Russano G, Sanjuan J, Slutsky J, Sopuerta CF, Steier F, Sumner T, Texier D, Thorpe JI, Vetrugno D, Vitale S, Wand V, Wanner G, Ward H, Wass PJ, Weber WJ, Wissel L, Wittchen A, Zweifel P. Sensor Noise in LISA Pathfinder: In-Flight Performance of the Optical Test Mass Readout. Phys Rev Lett 2021; 126:131103. [PMID: 33861094 DOI: 10.1103/physrevlett.126.131103] [Citation(s) in RCA: 5] [Impact Index Per Article: 1.7] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 09/10/2020] [Accepted: 02/12/2021] [Indexed: 06/12/2023]
Abstract
We report on the first subpicometer interferometer flown in space. It was part of ESA's Laser Interferometer Space Antenna (LISA) Pathfinder mission and performed the fundamental measurement of the positional and angular motion of two free-falling test masses. The interferometer worked immediately, stably, and reliably from switch on until the end of the mission with exceptionally low residual noise of 32.0_{-1.7}^{+2.4} fm/sqrt[Hz], significantly better than required. We present an upper limit for the sensor performance at millihertz frequencies and a model for the measured sensitivity above 200 mHz.
Collapse
Affiliation(s)
- M Armano
- European Space Technology Centre, European Space Agency, Keplerlaan 1, 2200 AG Noordwijk, The Netherlands
| | - H Audley
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik und Leibniz Universität Hannover, Callinstraße 38, 30167 Hannover, Germany
| | - J Baird
- APC, Université de Paris, CNRS, Astroparticule et Cosmologie, F-75006 Paris, France
| | - P Binetruy
- APC, Université de Paris, CNRS, Astroparticule et Cosmologie, F-75006 Paris, France
| | - M Born
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik und Leibniz Universität Hannover, Callinstraße 38, 30167 Hannover, Germany
| | - D Bortoluzzi
- Department of Industrial Engineering, University of Trento, via Sommarive 9, 38123 Trento, Italy and Trento Institute for Fundamental Physics and Application/INFN, 38123 Povo, Trento, Italy
| | - N Brandt
- Airbus Defence and Space, Claude-Dornier-Strasse, 88090 Immenstaad, Germany
| | - E Castelli
- Dipartimento di Fisica, Università di Trento and Trento Institute for Fundamental Physics and Application/INFN, 38123 Povo, Trento, Italy
| | - A Cavalleri
- Istituto di Fotonica e Nanotecnologie, CNR-Fondazione Bruno Kessler, I-38123 Povo, Trento, Italy
| | - A Cesarini
- DISPEA, Università di Urbino "Carlo Bo," Via Santa Chiara, 27, 61029 Urbino/INFN, Italy
| | - A M Cruise
- The School of Physics and Astronomy, University of Birmingham, B15 2TT Birmingham, United Kingdom
| | - K Danzmann
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik und Leibniz Universität Hannover, Callinstraße 38, 30167 Hannover, Germany
| | - M de Deus Silva
- European Space Astronomy Centre, European Space Agency, Villanueva de la Cañada, 28692 Madrid, Spain
| | - I Diepholz
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik und Leibniz Universität Hannover, Callinstraße 38, 30167 Hannover, Germany
| | - G Dixon
- The School of Physics and Astronomy, University of Birmingham, B15 2TT Birmingham, United Kingdom
| | - R Dolesi
- Dipartimento di Fisica, Università di Trento and Trento Institute for Fundamental Physics and Application/INFN, 38123 Povo, Trento, Italy
| | - L Ferraioli
- Institut für Geophysik, ETH Zürich, Sonneggstrasse 5, CH-8092 Zürich, Switzerland
| | - V Ferroni
- Dipartimento di Fisica, Università di Trento and Trento Institute for Fundamental Physics and Application/INFN, 38123 Povo, Trento, Italy
| | - E D Fitzsimons
- The UK Astronomy Technology Centre, Royal Observatory, Edinburgh, Blackford Hill, Edinburgh EH9 3HJ, United Kingdom
| | - R Flatscher
- Airbus Defence and Space, Claude-Dornier-Strasse, 88090 Immenstaad, Germany
| | - M Freschi
- European Space Astronomy Centre, European Space Agency, Villanueva de la Cañada, 28692 Madrid, Spain
| | - A García
- City University of Applied Sciences, Flughafenallee 10, 28199 Bremen, Germany
| | - R Gerndt
- Airbus Defence and Space, Claude-Dornier-Strasse, 88090 Immenstaad, Germany
| | - L Gesa
- Institut de Ciències de l'Espai (ICE, CSIC), Campus UAB, Carrer de Can Magrans s/n, 08193 Cerdanyola del Vallès, Spain
- Institut d'Estudis Espacials de Catalunya (IEEC), C/ Gran Capità 2-4, 08034 Barcelona, Spain
| | - D Giardini
- Institut für Geophysik, ETH Zürich, Sonneggstrasse 5, CH-8092 Zürich, Switzerland
| | - F Gibert
- Dipartimento di Fisica, Università di Trento and Trento Institute for Fundamental Physics and Application/INFN, 38123 Povo, Trento, Italy
- isardSAT SL, Marie Curie 8-14, 08042 Barcelona, Catalonia, Spain
| | - R Giusteri
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik und Leibniz Universität Hannover, Callinstraße 38, 30167 Hannover, Germany
| | - C Grimani
- DISPEA, Università di Urbino "Carlo Bo," Via Santa Chiara, 27, 61029 Urbino/INFN, Italy
| | - J Grzymisch
- European Space Technology Centre, European Space Agency, Keplerlaan 1, 2200 AG Noordwijk, The Netherlands
| | - F Guzman
- Texas A&M University, 701 H.R. Bright Building, College Station, Texas 77843-3141, USA
| | - I Harrison
- European Space Operations Centre, European Space Agency, 64293 Darmstadt, Germany
| | - M-S Hartig
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik und Leibniz Universität Hannover, Callinstraße 38, 30167 Hannover, Germany
| | - G Heinzel
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik und Leibniz Universität Hannover, Callinstraße 38, 30167 Hannover, Germany
| | - M Hewitson
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik und Leibniz Universität Hannover, Callinstraße 38, 30167 Hannover, Germany
| | - D Hollington
- Physics Department, Blackett Laboratory, High Energy Physics Group, Imperial College London, Prince Consort Road, London SW7 2BW, United Kingdom
| | - D Hoyland
- The School of Physics and Astronomy, University of Birmingham, B15 2TT Birmingham, United Kingdom
| | - M Hueller
- Dipartimento di Fisica, Università di Trento and Trento Institute for Fundamental Physics and Application/INFN, 38123 Povo, Trento, Italy
| | - H Inchauspé
- APC, Université de Paris, CNRS, Astroparticule et Cosmologie, F-75006 Paris, France
- Department of Mechanical and Aerospace Engineering, MAE-A, P.O. Box 116250, University of Florida, Gainesville, Florida 32611, USA
| | - O Jennrich
- European Space Technology Centre, European Space Agency, Keplerlaan 1, 2200 AG Noordwijk, The Netherlands
| | - P Jetzer
- Physik Institut, Universität Zürich, Winterthurerstrasse 190, CH-8057 Zürich, Switzerland
| | - U Johann
- Airbus Defence and Space, Claude-Dornier-Strasse, 88090 Immenstaad, Germany
| | - B Johlander
- European Space Technology Centre, European Space Agency, Keplerlaan 1, 2200 AG Noordwijk, The Netherlands
| | - N Karnesis
- APC, Université de Paris, CNRS, Astroparticule et Cosmologie, F-75006 Paris, France
| | - B Kaune
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik und Leibniz Universität Hannover, Callinstraße 38, 30167 Hannover, Germany
| | - C J Killow
- SUPA, Institute for Gravitational Research, School of Physics and Astronomy, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - N Korsakova
- Observatoire de la Côte d'Azur, Boulevard de l'Observatoire CS 34229-F 06304 Nice, France
| | - J A Lobo
- Institut de Ciències de l'Espai (ICE, CSIC), Campus UAB, Carrer de Can Magrans s/n, 08193 Cerdanyola del Vallès, Spain
- Institut d'Estudis Espacials de Catalunya (IEEC), C/ Gran Capità 2-4, 08034 Barcelona, Spain
| | - L Liu
- Dipartimento di Fisica, Università di Trento and Trento Institute for Fundamental Physics and Application/INFN, 38123 Povo, Trento, Italy
| | - J P López-Zaragoza
- Institut de Ciències de l'Espai (ICE, CSIC), Campus UAB, Carrer de Can Magrans s/n, 08193 Cerdanyola del Vallès, Spain
| | - R Maarschalkerweerd
- European Space Operations Centre, European Space Agency, 64293 Darmstadt, Germany
| | - D Mance
- Institut für Geophysik, ETH Zürich, Sonneggstrasse 5, CH-8092 Zürich, Switzerland
| | - V Martín
- Institut de Ciències de l'Espai (ICE, CSIC), Campus UAB, Carrer de Can Magrans s/n, 08193 Cerdanyola del Vallès, Spain
- Institut d'Estudis Espacials de Catalunya (IEEC), C/ Gran Capità 2-4, 08034 Barcelona, Spain
| | - L Martin-Polo
- European Space Astronomy Centre, European Space Agency, Villanueva de la Cañada, 28692 Madrid, Spain
| | - F Martin-Porqueras
- European Space Astronomy Centre, European Space Agency, Villanueva de la Cañada, 28692 Madrid, Spain
| | - J Martino
- APC, Université de Paris, CNRS, Astroparticule et Cosmologie, F-75006 Paris, France
| | - P W McNamara
- European Space Technology Centre, European Space Agency, Keplerlaan 1, 2200 AG Noordwijk, The Netherlands
| | - J Mendes
- European Space Operations Centre, European Space Agency, 64293 Darmstadt, Germany
| | - L Mendes
- European Space Astronomy Centre, European Space Agency, Villanueva de la Cañada, 28692 Madrid, Spain
| | - N Meshksar
- Institut für Geophysik, ETH Zürich, Sonneggstrasse 5, CH-8092 Zürich, Switzerland
| | - A Monsky
- OHB System AG, Universitätsallee 27-29, 28359 Bremen, Germany
| | - M Nofrarias
- Institut de Ciències de l'Espai (ICE, CSIC), Campus UAB, Carrer de Can Magrans s/n, 08193 Cerdanyola del Vallès, Spain
- Institut d'Estudis Espacials de Catalunya (IEEC), C/ Gran Capità 2-4, 08034 Barcelona, Spain
| | - S Paczkowski
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik und Leibniz Universität Hannover, Callinstraße 38, 30167 Hannover, Germany
| | - M Perreur-Lloyd
- SUPA, Institute for Gravitational Research, School of Physics and Astronomy, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - A Petiteau
- APC, Université de Paris, CNRS, Astroparticule et Cosmologie, F-75006 Paris, France
| | - P Pivato
- Dipartimento di Fisica, Università di Trento and Trento Institute for Fundamental Physics and Application/INFN, 38123 Povo, Trento, Italy
| | - E Plagnol
- APC, Université de Paris, CNRS, Astroparticule et Cosmologie, F-75006 Paris, France
| | - J Ramos-Castro
- Institut d'Estudis Espacials de Catalunya (IEEC), C/ Gran Capità 2-4, 08034 Barcelona, Spain
- Department d'Enginyeria Electrònica, Universitat Politècnica de Catalunya, 08034 Barcelona, Spain
| | - J Reiche
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik und Leibniz Universität Hannover, Callinstraße 38, 30167 Hannover, Germany
| | - F Rivas
- Dipartimento di Fisica, Università di Trento and Trento Institute for Fundamental Physics and Application/INFN, 38123 Povo, Trento, Italy
| | - D I Robertson
- SUPA, Institute for Gravitational Research, School of Physics and Astronomy, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - G Russano
- Dipartimento di Fisica, Università di Trento and Trento Institute for Fundamental Physics and Application/INFN, 38123 Povo, Trento, Italy
| | - J Sanjuan
- Department of Physics, 2001 Museum Road, University of Florida, Gainesville, Florida 32611, USA
| | - J Slutsky
- Gravitational Astrophysics Laboratory, NASA Goddard Space Flight Center, 8800 Greenbelt Road, Greenbelt, Maryland 20771, USA
| | - C F Sopuerta
- Institut de Ciències de l'Espai (ICE, CSIC), Campus UAB, Carrer de Can Magrans s/n, 08193 Cerdanyola del Vallès, Spain
- Institut d'Estudis Espacials de Catalunya (IEEC), C/ Gran Capità 2-4, 08034 Barcelona, Spain
| | - F Steier
- OHB System AG, Universitätsallee 27-29, 28359 Bremen, Germany
| | - T Sumner
- Physics Department, Blackett Laboratory, High Energy Physics Group, Imperial College London, Prince Consort Road, London SW7 2BW, United Kingdom
| | - D Texier
- European Space Astronomy Centre, European Space Agency, Villanueva de la Cañada, 28692 Madrid, Spain
| | - J I Thorpe
- Gravitational Astrophysics Laboratory, NASA Goddard Space Flight Center, 8800 Greenbelt Road, Greenbelt, Maryland 20771, USA
| | - D Vetrugno
- Dipartimento di Fisica, Università di Trento and Trento Institute for Fundamental Physics and Application/INFN, 38123 Povo, Trento, Italy
| | - S Vitale
- Dipartimento di Fisica, Università di Trento and Trento Institute for Fundamental Physics and Application/INFN, 38123 Povo, Trento, Italy
| | - V Wand
- OHB System AG, Universitätsallee 27-29, 28359 Bremen, Germany
| | - G Wanner
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik und Leibniz Universität Hannover, Callinstraße 38, 30167 Hannover, Germany
| | - H Ward
- SUPA, Institute for Gravitational Research, School of Physics and Astronomy, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - P J Wass
- Physics Department, Blackett Laboratory, High Energy Physics Group, Imperial College London, Prince Consort Road, London SW7 2BW, United Kingdom
- Department of Mechanical and Aerospace Engineering, MAE-A, P.O. Box 116250, University of Florida, Gainesville, Florida 32611, USA
| | - W J Weber
- Dipartimento di Fisica, Università di Trento and Trento Institute for Fundamental Physics and Application/INFN, 38123 Povo, Trento, Italy
| | - L Wissel
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik und Leibniz Universität Hannover, Callinstraße 38, 30167 Hannover, Germany
| | - A Wittchen
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik und Leibniz Universität Hannover, Callinstraße 38, 30167 Hannover, Germany
| | - P Zweifel
- Institut für Geophysik, ETH Zürich, Sonneggstrasse 5, CH-8092 Zürich, Switzerland
| |
Collapse
|
6
|
Armano M, Audley H, Baird J, Born M, Bortoluzzi D, Cardines N, Castelli E, Cavalleri A, Cesarini A, Cruise AM, Danzmann K, de Deus Silva M, Dixon G, Dolesi R, Ferraioli L, Ferroni V, Fitzsimons ED, Freschi M, Gesa L, Giardini D, Gibert F, Giusteri R, Grimani C, Grzymisch J, Harrison I, Hartig MS, Heinzel G, Hewitson M, Hollington D, Hoyland D, Hueller M, Inchauspé H, Jennrich O, Jetzer P, Karnesis N, Kaune B, Killow CJ, Korsakova N, López-Zaragoza JP, Maarschalkerweerd R, Mance D, Martín V, Martin-Polo L, Martino J, Martin-Porqueras F, Mateos I, McNamara PW, Mendes J, Mendes L, Meshksar N, Nofrarias M, Paczkowski S, Perreur-Lloyd M, Petiteau A, Pivato P, Plagnol E, Ramos-Castro J, Reiche J, Rivas F, Robertson DI, Russano G, Slutsky J, Sopuerta CF, Sumner T, Texier D, Ten Pierick J, Thorpe JI, Vetrugno D, Vitale S, Wanner G, Ward H, Wass PJ, Weber WJ, Wissel L, Wittchen A, Zweifel P. Analysis of the accuracy of actuation electronics in the laser interferometer space antenna pathfinder. Rev Sci Instrum 2020; 91:045003. [PMID: 32357757 DOI: 10.1063/1.5140406] [Citation(s) in RCA: 2] [Impact Index Per Article: 0.5] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 12/02/2019] [Accepted: 03/13/2020] [Indexed: 06/11/2023]
Abstract
The Laser Interferometer Space Antenna Pathfinder (LPF) main observable, labeled Δg, is the differential force per unit mass acting on the two test masses under free fall conditions after the contribution of all non-gravitational forces has been compensated. At low frequencies, the differential force is compensated by an applied electrostatic actuation force, which then must be subtracted from the measured acceleration to obtain Δg. Any inaccuracy in the actuation force contaminates the residual acceleration. This study investigates the accuracy of the electrostatic actuation system and its impact on the LPF main observable. It is shown that the inaccuracy is mainly caused by the rounding errors in the waveform processing and also by the random error caused by the analog to digital converter random noise in the control loop. Both errors are one order of magnitude smaller than the resolution of the commanded voltages. We developed a simulator based on the LPF design to compute the close-to-reality actuation voltages and, consequently, the resulting actuation forces. The simulator is applied during post-processing the LPF data.
Collapse
Affiliation(s)
- M Armano
- European Space Technology Centre, European Space Agency, Keplerlaan 1, 2200 AG Noordwijk, The Netherlands
| | - H Audley
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik und Leibniz Universität Hannover, Callinstraße 38, 30167 Hannover, Germany
| | - J Baird
- APC, Univ Paris Diderot, CNRS/IN2P3, CEA/lrfu, Obs de Paris, Sorbonne Paris Cité, 10, rue Alice Domon et Léonie Duquet, 75013 Paris, France
| | - M Born
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik und Leibniz Universität Hannover, Callinstraße 38, 30167 Hannover, Germany
| | - D Bortoluzzi
- Department of Industrial Engineering, University of Trento, via Sommarive 9, 38123 Trento, Italy
| | - N Cardines
- Institut für Geophysik, ETH Zürich, Sonneggstrasse 5, CH-8092 Zürich, Switzerland
| | - E Castelli
- Trento Institute for Fundamental Physics and Application/INFN, 38123 Povo, Trento, Italy
| | - A Cavalleri
- Istituto di Fotonica e Nanotecnologie, CNR-Fondazione Bruno Kessler, I-38123 Povo, Trento, Italy
| | - A Cesarini
- DISPEA, Università di Urbino "Carlo Bo", Via S. Chiara, 27, 61029 Urbino/INFN, Italy
| | - A M Cruise
- The School of Physics and Astronomy, University of Birmingham, B15 2TT Birmingham, United Kingdom
| | - K Danzmann
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik und Leibniz Universität Hannover, Callinstraße 38, 30167 Hannover, Germany
| | - M de Deus Silva
- European Space Astronomy Centre, European Space Agency, Villanueva de la Cañada, 28692 Madrid, Spain
| | - G Dixon
- The School of Physics and Astronomy, University of Birmingham, B15 2TT Birmingham, United Kingdom
| | - R Dolesi
- Trento Institute for Fundamental Physics and Application/INFN, 38123 Povo, Trento, Italy
| | - L Ferraioli
- Institut für Geophysik, ETH Zürich, Sonneggstrasse 5, CH-8092 Zürich, Switzerland
| | - V Ferroni
- Trento Institute for Fundamental Physics and Application/INFN, 38123 Povo, Trento, Italy
| | - E D Fitzsimons
- European Space Technology Centre, European Space Agency, Keplerlaan 1, 2200 AG Noordwijk, The NetherlandsAlbert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik und Leibniz Universität Hannover, Callinstraße 38, 30167 Hannover, GermanyAPC, Univ Paris Diderot, CNRS/IN2P3, CEA/lrfu, Obs de Paris, Sorbonne Paris Cité, 10, rue Alice Domon et Léonie Duquet, 75013 Paris, FranceDepartment of Industrial Engineering, University of Trento, via Sommarive 9, 38123 Trento, ItalyTrento Institute for Fundamental Physics and Application/INFN, 38123 Povo, Trento, ItalyInstitut für Geophysik, ETH Zürich, Sonneggstrasse 5, CH-8092 Zürich, SwitzerlandDipartimento di Fisica, Università di Trento, 38123 Povo, Trento, ItalyIstituto di Fotonica e Nanotecnologie, CNR-Fondazione Bruno Kessler, I-38123 Povo, Trento, ItalyDISPEA, Università di Urbino "Carlo Bo", Via S. Chiara, 27, 61029 Urbino/INFN, ItalyThe School of Physics and Astronomy, University of Birmingham, B15 2TT Birmingham, United KingdomEuropean Space Astronomy Centre, European Space Agency, Villanueva de la Cañada, 28692 Madrid, SpainThe UK Astronomy Technology Centre, Royal Observatory, Edinburgh, Blackford Hill, Edinburgh EH9 3HJ, United KingdomInstitut de Ciències de l'Espai (ICE, CSIC), Campus UAB, Carrer de Can Magrans s/n, 08193 Cerdanyola del Vallès, SpainInstitut d'Estudis Espacials de Catalunya (IEEC), C/Gran Capità 2-4, 08034 Barcelona, SpainisardSAT SL, Marie Curie 8-14, 08042 Barcelona, Catalonia, SpainEuropean Space Operations Centre, European Space Agency, 64293 Darmstadt, GermanyHigh Energy Physics Group, Physics Department, Imperial College London, Blackett Laboratory, Prince Consort Road, London SW7 2BW, United KingdomDepartment of Mechanical and Aerospace Engineering, MAE-A, University of Florida, P.O. Box 116250, Gainesville, Florida 32611, USAPhysik Institut, Universität Zürich, Winterthurerstrasse 190, CH-8057 Zürich, SwitzerlandSUPA, Institute for Gravitational Research, School of Physics and Astronomy, University of Glasgow, Glasgow G12 8QQ, United KingdomObservatoire de la Côte d'Azur, Boulevard de l'Observatoire CS 34229, F 06304 Nice, FranceEscuela Superior de Ingeniería, Universidad de Cádiz, 11519 Cádiz, SpainDepartment d'Enginyeria Electrònica, Universitat Politècnica de Catalunya, 08034 Barcelona, SpainGravitational Astrophysics Lab, NASA Goddard Space Flight Center, 8800 Greenbelt Road, Greenbelt, Maryland 20771, USA
| | - M Freschi
- European Space Astronomy Centre, European Space Agency, Villanueva de la Cañada, 28692 Madrid, Spain
| | - L Gesa
- Institut de Ciències de l'Espai (ICE, CSIC), Campus UAB, Carrer de Can Magrans s/n, 08193 Cerdanyola del Vallès, Spain
| | - D Giardini
- Institut für Geophysik, ETH Zürich, Sonneggstrasse 5, CH-8092 Zürich, Switzerland
| | - F Gibert
- Trento Institute for Fundamental Physics and Application/INFN, 38123 Povo, Trento, Italy
| | - R Giusteri
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik und Leibniz Universität Hannover, Callinstraße 38, 30167 Hannover, Germany
| | - C Grimani
- DISPEA, Università di Urbino "Carlo Bo", Via S. Chiara, 27, 61029 Urbino/INFN, Italy
| | - J Grzymisch
- European Space Technology Centre, European Space Agency, Keplerlaan 1, 2200 AG Noordwijk, The Netherlands
| | - I Harrison
- European Space Operations Centre, European Space Agency, 64293 Darmstadt, Germany
| | - M-S Hartig
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik und Leibniz Universität Hannover, Callinstraße 38, 30167 Hannover, Germany
| | - G Heinzel
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik und Leibniz Universität Hannover, Callinstraße 38, 30167 Hannover, Germany
| | - M Hewitson
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik und Leibniz Universität Hannover, Callinstraße 38, 30167 Hannover, Germany
| | - D Hollington
- High Energy Physics Group, Physics Department, Imperial College London, Blackett Laboratory, Prince Consort Road, London SW7 2BW, United Kingdom
| | - D Hoyland
- The School of Physics and Astronomy, University of Birmingham, B15 2TT Birmingham, United Kingdom
| | - M Hueller
- Trento Institute for Fundamental Physics and Application/INFN, 38123 Povo, Trento, Italy
| | - H Inchauspé
- APC, Univ Paris Diderot, CNRS/IN2P3, CEA/lrfu, Obs de Paris, Sorbonne Paris Cité, 10, rue Alice Domon et Léonie Duquet, 75013 Paris, France
| | - O Jennrich
- European Space Technology Centre, European Space Agency, Keplerlaan 1, 2200 AG Noordwijk, The Netherlands
| | - P Jetzer
- Physik Institut, Universität Zürich, Winterthurerstrasse 190, CH-8057 Zürich, Switzerland
| | - N Karnesis
- APC, Univ Paris Diderot, CNRS/IN2P3, CEA/lrfu, Obs de Paris, Sorbonne Paris Cité, 10, rue Alice Domon et Léonie Duquet, 75013 Paris, France
| | - B Kaune
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik und Leibniz Universität Hannover, Callinstraße 38, 30167 Hannover, Germany
| | - C J Killow
- SUPA, Institute for Gravitational Research, School of Physics and Astronomy, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - N Korsakova
- Observatoire de la Côte d'Azur, Boulevard de l'Observatoire CS 34229, F 06304 Nice, France
| | - J P López-Zaragoza
- Institut de Ciències de l'Espai (ICE, CSIC), Campus UAB, Carrer de Can Magrans s/n, 08193 Cerdanyola del Vallès, Spain
| | - R Maarschalkerweerd
- European Space Operations Centre, European Space Agency, 64293 Darmstadt, Germany
| | - D Mance
- Institut für Geophysik, ETH Zürich, Sonneggstrasse 5, CH-8092 Zürich, Switzerland
| | - V Martín
- Institut de Ciències de l'Espai (ICE, CSIC), Campus UAB, Carrer de Can Magrans s/n, 08193 Cerdanyola del Vallès, Spain
| | - L Martin-Polo
- European Space Astronomy Centre, European Space Agency, Villanueva de la Cañada, 28692 Madrid, Spain
| | - J Martino
- APC, Univ Paris Diderot, CNRS/IN2P3, CEA/lrfu, Obs de Paris, Sorbonne Paris Cité, 10, rue Alice Domon et Léonie Duquet, 75013 Paris, France
| | - F Martin-Porqueras
- European Space Astronomy Centre, European Space Agency, Villanueva de la Cañada, 28692 Madrid, Spain
| | - I Mateos
- Escuela Superior de Ingeniería, Universidad de Cádiz, 11519 Cádiz, Spain
| | - P W McNamara
- European Space Technology Centre, European Space Agency, Keplerlaan 1, 2200 AG Noordwijk, The Netherlands
| | - J Mendes
- European Space Operations Centre, European Space Agency, 64293 Darmstadt, Germany
| | - L Mendes
- European Space Astronomy Centre, European Space Agency, Villanueva de la Cañada, 28692 Madrid, Spain
| | - N Meshksar
- Institut für Geophysik, ETH Zürich, Sonneggstrasse 5, CH-8092 Zürich, Switzerland
| | - M Nofrarias
- Institut de Ciències de l'Espai (ICE, CSIC), Campus UAB, Carrer de Can Magrans s/n, 08193 Cerdanyola del Vallès, Spain
| | - S Paczkowski
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik und Leibniz Universität Hannover, Callinstraße 38, 30167 Hannover, Germany
| | - M Perreur-Lloyd
- SUPA, Institute for Gravitational Research, School of Physics and Astronomy, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - A Petiteau
- APC, Univ Paris Diderot, CNRS/IN2P3, CEA/lrfu, Obs de Paris, Sorbonne Paris Cité, 10, rue Alice Domon et Léonie Duquet, 75013 Paris, France
| | - P Pivato
- Trento Institute for Fundamental Physics and Application/INFN, 38123 Povo, Trento, Italy
| | - E Plagnol
- APC, Univ Paris Diderot, CNRS/IN2P3, CEA/lrfu, Obs de Paris, Sorbonne Paris Cité, 10, rue Alice Domon et Léonie Duquet, 75013 Paris, France
| | - J Ramos-Castro
- Institut d'Estudis Espacials de Catalunya (IEEC), C/Gran Capità 2-4, 08034 Barcelona, Spain
| | - J Reiche
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik und Leibniz Universität Hannover, Callinstraße 38, 30167 Hannover, Germany
| | - F Rivas
- Institut de Ciències de l'Espai (ICE, CSIC), Campus UAB, Carrer de Can Magrans s/n, 08193 Cerdanyola del Vallès, Spain
| | - D I Robertson
- SUPA, Institute for Gravitational Research, School of Physics and Astronomy, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - G Russano
- Trento Institute for Fundamental Physics and Application/INFN, 38123 Povo, Trento, Italy
| | - J Slutsky
- Gravitational Astrophysics Lab, NASA Goddard Space Flight Center, 8800 Greenbelt Road, Greenbelt, Maryland 20771, USA
| | - C F Sopuerta
- Institut de Ciències de l'Espai (ICE, CSIC), Campus UAB, Carrer de Can Magrans s/n, 08193 Cerdanyola del Vallès, Spain
| | - T Sumner
- High Energy Physics Group, Physics Department, Imperial College London, Blackett Laboratory, Prince Consort Road, London SW7 2BW, United Kingdom
| | - D Texier
- European Space Astronomy Centre, European Space Agency, Villanueva de la Cañada, 28692 Madrid, Spain
| | - J Ten Pierick
- Institut für Geophysik, ETH Zürich, Sonneggstrasse 5, CH-8092 Zürich, Switzerland
| | - J I Thorpe
- Gravitational Astrophysics Lab, NASA Goddard Space Flight Center, 8800 Greenbelt Road, Greenbelt, Maryland 20771, USA
| | - D Vetrugno
- Trento Institute for Fundamental Physics and Application/INFN, 38123 Povo, Trento, Italy
| | - S Vitale
- Trento Institute for Fundamental Physics and Application/INFN, 38123 Povo, Trento, Italy
| | - G Wanner
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik und Leibniz Universität Hannover, Callinstraße 38, 30167 Hannover, Germany
| | - H Ward
- SUPA, Institute for Gravitational Research, School of Physics and Astronomy, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - P J Wass
- High Energy Physics Group, Physics Department, Imperial College London, Blackett Laboratory, Prince Consort Road, London SW7 2BW, United Kingdom
| | - W J Weber
- Trento Institute for Fundamental Physics and Application/INFN, 38123 Povo, Trento, Italy
| | - L Wissel
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik und Leibniz Universität Hannover, Callinstraße 38, 30167 Hannover, Germany
| | - A Wittchen
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik und Leibniz Universität Hannover, Callinstraße 38, 30167 Hannover, Germany
| | - P Zweifel
- Institut für Geophysik, ETH Zürich, Sonneggstrasse 5, CH-8092 Zürich, Switzerland
| |
Collapse
|
7
|
Armano M, Audley H, Baird J, Binetruy P, Born M, Bortoluzzi D, Castelli E, Cavalleri A, Cesarini A, Cruise AM, Danzmann K, de Deus Silva M, Diepholz I, Dixon G, Dolesi R, Ferraioli L, Ferroni V, Fitzsimons ED, Freschi M, Gesa L, Gibert F, Giardini D, Giusteri R, Grimani C, Grzymisch J, Harrison I, Hartig MS, Heinzel G, Hewitson M, Hollington D, Hoyland D, Hueller M, Inchauspé H, Jennrich O, Jetzer P, Karnesis N, Kaune B, Korsakova N, Killow CJ, Lobo JA, Liu L, López-Zaragoza JP, Maarschalkerweerd R, Mance D, Meshksar N, Martín V, Martin-Polo L, Martino J, Martin-Porqueras F, Mateos I, McNamara PW, Mendes J, Mendes L, Nofrarias M, Paczkowski S, Perreur-Lloyd M, Petiteau A, Pivato P, Plagnol E, Ramos-Castro J, Reiche J, Robertson DI, Rivas F, Russano G, Slutsky J, Sopuerta CF, Sumner T, Texier D, Thorpe JI, Vetrugno D, Vitale S, Wanner G, Ward H, Wass PJ, Weber WJ, Wissel L, Wittchen A, Zweifel P. LISA Pathfinder Performance Confirmed in an Open-Loop Configuration: Results from the Free-Fall Actuation Mode. Phys Rev Lett 2019; 123:111101. [PMID: 31573236 PMCID: PMC7810161 DOI: 10.1103/physrevlett.123.111101] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Grants] [Track Full Text] [Figures] [Subscribe] [Scholar Register] [Received: 02/19/2019] [Revised: 06/11/2019] [Indexed: 06/10/2023]
Abstract
We report on the results of the LISA Pathfinder (LPF) free-fall mode experiment, in which the control force needed to compensate the quasistatic differential force acting on two test masses is applied intermittently as a series of "impulse" forces lasting a few seconds and separated by roughly 350 s periods of true free fall. This represents an alternative to the normal LPF mode of operation in which this balancing force is applied continuously, with the advantage that the acceleration noise during free fall is measured in the absence of the actuation force, thus eliminating associated noise and force calibration errors. The differential acceleration noise measurement presented here with the free-fall mode agrees with noise measured with the continuous actuation scheme, representing an important and independent confirmation of the LPF result. An additional measurement with larger actuation forces also shows that the technique can be used to eliminate actuation noise when this is a dominant factor.
Collapse
Affiliation(s)
- M. Armano
- European Space Technology Centre, European Space Agency, Keplerlaan 1, 2200 AG Noordwijk, The Netherlands
| | - H. Audley
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik und Leibniz Universität Hannover, Callinstraße 38, 30167 Hannover, Germany
| | - J. Baird
- APC, Univ Paris Diderot, CNRS/IN2P3, CEA/lrfu, Obs de Paris, Sorbonne Paris Cité, France
| | - P. Binetruy
- APC, Univ Paris Diderot, CNRS/IN2P3, CEA/lrfu, Obs de Paris, Sorbonne Paris Cité, France
| | - M. Born
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik und Leibniz Universität Hannover, Callinstraße 38, 30167 Hannover, Germany
| | - D. Bortoluzzi
- epartment of Industrial Engineering, University of Trento, via Sommarive 9, 38123 Trento, and Trento Institute for Fundamental Physics and Application / INFN
| | - E. Castelli
- Dipartimento di Fisica, Università di Trento and Trento Institute for Fundamental Physics and Application / INFN, 38123 Povo, Trento, Italy
| | - A. Cavalleri
- Istituto di Fotonica e Nanotecnologie, CNR-Fondazione Bruno Kessler, I-38123 Povo, Trento, Italy
| | - A. Cesarini
- DISPEA, Università di Urbino “Carlo Bo,” Via S. Chiara, 27 61029 Urbino/INFN, Italy
| | - A. M. Cruise
- The School of Physics and Astronomy, University of Birmingham, Birmingham, United Kingdom
| | - K. Danzmann
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik und Leibniz Universität Hannover, Callinstraße 38, 30167 Hannover, Germany
| | - M. de Deus Silva
- European Space Astronomy Centre, European Space Agency, Villanueva de la Cañada, 28692 Madrid, Spain
| | - I. Diepholz
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik und Leibniz Universität Hannover, Callinstraße 38, 30167 Hannover, Germany
| | - G. Dixon
- The School of Physics and Astronomy, University of Birmingham, Birmingham, United Kingdom
| | - R. Dolesi
- Dipartimento di Fisica, Università di Trento and Trento Institute for Fundamental Physics and Application / INFN, 38123 Povo, Trento, Italy
| | - L. Ferraioli
- Institut für Geophysik, ETH Zürich, Sonneggstrasse 5, CH-8092, Zürich, Switzerland
| | - V. Ferroni
- Dipartimento di Fisica, Università di Trento and Trento Institute for Fundamental Physics and Application / INFN, 38123 Povo, Trento, Italy
| | - E. D. Fitzsimons
- The UK Astronomy Technology Centre, Royal Observatory, Edinburgh, Blackford Hill, Edinburgh, EH9 3HJ, United Kingdom
| | - M. Freschi
- European Space Astronomy Centre, European Space Agency, Villanueva de la Cañada, 28692 Madrid, Spain
| | - L. Gesa
- Institut de Ciències de l’Espai (ICE, CSIC), Campus UAB, Carrer de Can Magrans s/n, 08193 Cerdanyola del Vallès, Spain
- Institut d’Estudis Espacials de Catalunya (IEEC), C/ Gran Capità 2-4, 08034 Barcelona, Spain
| | - F. Gibert
- Dipartimento di Fisica, Università di Trento and Trento Institute for Fundamental Physics and Application / INFN, 38123 Povo, Trento, Italy
- isardSAT SL, Marie Curie 8-14, 08042 Barcelona, Catalonia, Spain
| | - D. Giardini
- Institut für Geophysik, ETH Zürich, Sonneggstrasse 5, CH-8092, Zürich, Switzerland
| | - R. Giusteri
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik und Leibniz Universität Hannover, Callinstraße 38, 30167 Hannover, Germany
- Dipartimento di Fisica, Università di Trento and Trento Institute for Fundamental Physics and Application / INFN, 38123 Povo, Trento, Italy
| | - C. Grimani
- DISPEA, Università di Urbino “Carlo Bo,” Via S. Chiara, 27 61029 Urbino/INFN, Italy
| | - J. Grzymisch
- European Space Technology Centre, European Space Agency, Keplerlaan 1, 2200 AG Noordwijk, The Netherlands
| | - I. Harrison
- European Space Operations Centre, European Space Agency, 64293 Darmstadt, Germany
| | - M-S. Hartig
- European Space Operations Centre, European Space Agency, 64293 Darmstadt, Germany
| | - G. Heinzel
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik und Leibniz Universität Hannover, Callinstraße 38, 30167 Hannover, Germany
| | - M. Hewitson
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik und Leibniz Universität Hannover, Callinstraße 38, 30167 Hannover, Germany
| | - D. Hollington
- High Energy Physics Group, Physics Department, Imperial College London, Blackett Laboratory, Prince Consort Road, London, SW7 2BW, United Kingdom
| | - D. Hoyland
- The School of Physics and Astronomy, University of Birmingham, Birmingham, United Kingdom
| | - M. Hueller
- Dipartimento di Fisica, Università di Trento and Trento Institute for Fundamental Physics and Application / INFN, 38123 Povo, Trento, Italy
| | - H. Inchauspé
- APC, Univ Paris Diderot, CNRS/IN2P3, CEA/lrfu, Obs de Paris, Sorbonne Paris Cité, France
- Department of Mechanical and Aerospace Engineering, MAE-A, P.O. Box 116250, University of Florida, Gainesville, Florida 32611, USA
| | - O. Jennrich
- European Space Technology Centre, European Space Agency, Keplerlaan 1, 2200 AG Noordwijk, The Netherlands
| | - P. Jetzer
- Physik Institut, Universität Zürich, Winterthurerstrasse 190, CH-8057 Zürich, Switzerland
| | - N. Karnesis
- APC, Univ Paris Diderot, CNRS/IN2P3, CEA/lrfu, Obs de Paris, Sorbonne Paris Cité, France
| | - B. Kaune
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik und Leibniz Universität Hannover, Callinstraße 38, 30167 Hannover, Germany
| | - N. Korsakova
- SUPA, Institute for Gravitational Research, School of Physics and Astronomy, University of Glasgow, Glasgow, G12 8QQ, United Kingdom
| | - C. J. Killow
- SUPA, Institute for Gravitational Research, School of Physics and Astronomy, University of Glasgow, Glasgow, G12 8QQ, United Kingdom
| | - J. A. Lobo
- Institut de Ciències de l’Espai (ICE, CSIC), Campus UAB, Carrer de Can Magrans s/n, 08193 Cerdanyola del Vallès, Spain
- Institut d’Estudis Espacials de Catalunya (IEEC), C/ Gran Capità 2-4, 08034 Barcelona, Spain
| | - L. Liu
- Dipartimento di Fisica, Università di Trento and Trento Institute for Fundamental Physics and Application / INFN, 38123 Povo, Trento, Italy
| | - J. P. López-Zaragoza
- Institut de Ciències de l’Espai (ICE, CSIC), Campus UAB, Carrer de Can Magrans s/n, 08193 Cerdanyola del Vallès, Spain
| | - R. Maarschalkerweerd
- European Space Operations Centre, European Space Agency, 64293 Darmstadt, Germany
| | - D. Mance
- Institut für Geophysik, ETH Zürich, Sonneggstrasse 5, CH-8092, Zürich, Switzerland
| | - N. Meshksar
- Institut für Geophysik, ETH Zürich, Sonneggstrasse 5, CH-8092, Zürich, Switzerland
| | - V. Martín
- Institut de Ciències de l’Espai (ICE, CSIC), Campus UAB, Carrer de Can Magrans s/n, 08193 Cerdanyola del Vallès, Spain
- Institut d’Estudis Espacials de Catalunya (IEEC), C/ Gran Capità 2-4, 08034 Barcelona, Spain
| | - L. Martin-Polo
- European Space Astronomy Centre, European Space Agency, Villanueva de la Cañada, 28692 Madrid, Spain
| | - J. Martino
- APC, Univ Paris Diderot, CNRS/IN2P3, CEA/lrfu, Obs de Paris, Sorbonne Paris Cité, France
| | - F. Martin-Porqueras
- European Space Astronomy Centre, European Space Agency, Villanueva de la Cañada, 28692 Madrid, Spain
| | - I. Mateos
- Institut de Ciències de l’Espai (ICE, CSIC), Campus UAB, Carrer de Can Magrans s/n, 08193 Cerdanyola del Vallès, Spain
- Institut d’Estudis Espacials de Catalunya (IEEC), C/ Gran Capità 2-4, 08034 Barcelona, Spain
| | - P. W. McNamara
- European Space Technology Centre, European Space Agency, Keplerlaan 1, 2200 AG Noordwijk, The Netherlands
| | - J. Mendes
- European Space Operations Centre, European Space Agency, 64293 Darmstadt, Germany
| | - L. Mendes
- European Space Astronomy Centre, European Space Agency, Villanueva de la Cañada, 28692 Madrid, Spain
| | - M. Nofrarias
- Institut de Ciències de l’Espai (ICE, CSIC), Campus UAB, Carrer de Can Magrans s/n, 08193 Cerdanyola del Vallès, Spain
- Institut d’Estudis Espacials de Catalunya (IEEC), C/ Gran Capità 2-4, 08034 Barcelona, Spain
| | - S. Paczkowski
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik und Leibniz Universität Hannover, Callinstraße 38, 30167 Hannover, Germany
| | - M. Perreur-Lloyd
- SUPA, Institute for Gravitational Research, School of Physics and Astronomy, University of Glasgow, Glasgow, G12 8QQ, United Kingdom
| | - A. Petiteau
- APC, Univ Paris Diderot, CNRS/IN2P3, CEA/lrfu, Obs de Paris, Sorbonne Paris Cité, France
| | - P. Pivato
- Dipartimento di Fisica, Università di Trento and Trento Institute for Fundamental Physics and Application / INFN, 38123 Povo, Trento, Italy
| | - E. Plagnol
- APC, Univ Paris Diderot, CNRS/IN2P3, CEA/lrfu, Obs de Paris, Sorbonne Paris Cité, France
| | - J. Ramos-Castro
- Institut d’Estudis Espacials de Catalunya (IEEC), C/ Gran Capità 2-4, 08034 Barcelona, Spain
- Department d’Enginyeria Electrònica, Universitat Politècnica de Catalunya, 08034 Barcelona, Spain
| | - J. Reiche
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik und Leibniz Universität Hannover, Callinstraße 38, 30167 Hannover, Germany
| | - D. I. Robertson
- SUPA, Institute for Gravitational Research, School of Physics and Astronomy, University of Glasgow, Glasgow, G12 8QQ, United Kingdom
| | - F. Rivas
- Institut de Ciències de l’Espai (ICE, CSIC), Campus UAB, Carrer de Can Magrans s/n, 08193 Cerdanyola del Vallès, Spain
- Institut d’Estudis Espacials de Catalunya (IEEC), C/ Gran Capità 2-4, 08034 Barcelona, Spain
| | - G. Russano
- Dipartimento di Fisica, Università di Trento and Trento Institute for Fundamental Physics and Application / INFN, 38123 Povo, Trento, Italy
| | - J. Slutsky
- Gravitational Astrophysics Lab, NASA Goddard Space Flight Center, 8800 Greenbelt Road, Greenbelt, Maryland 20771, USA
| | - C. F. Sopuerta
- Institut de Ciències de l’Espai (ICE, CSIC), Campus UAB, Carrer de Can Magrans s/n, 08193 Cerdanyola del Vallès, Spain
- Institut d’Estudis Espacials de Catalunya (IEEC), C/ Gran Capità 2-4, 08034 Barcelona, Spain
| | - T. Sumner
- High Energy Physics Group, Physics Department, Imperial College London, Blackett Laboratory, Prince Consort Road, London, SW7 2BW, United Kingdom
| | - D. Texier
- European Space Astronomy Centre, European Space Agency, Villanueva de la Cañada, 28692 Madrid, Spain
| | - J. I. Thorpe
- Gravitational Astrophysics Lab, NASA Goddard Space Flight Center, 8800 Greenbelt Road, Greenbelt, Maryland 20771, USA
| | - D. Vetrugno
- Dipartimento di Fisica, Università di Trento and Trento Institute for Fundamental Physics and Application / INFN, 38123 Povo, Trento, Italy
| | - S. Vitale
- Dipartimento di Fisica, Università di Trento and Trento Institute for Fundamental Physics and Application / INFN, 38123 Povo, Trento, Italy
| | - G. Wanner
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik und Leibniz Universität Hannover, Callinstraße 38, 30167 Hannover, Germany
| | - H. Ward
- SUPA, Institute for Gravitational Research, School of Physics and Astronomy, University of Glasgow, Glasgow, G12 8QQ, United Kingdom
| | - P. J. Wass
- High Energy Physics Group, Physics Department, Imperial College London, Blackett Laboratory, Prince Consort Road, London, SW7 2BW, United Kingdom
- Department of Mechanical and Aerospace Engineering, MAE-A, P.O. Box 116250, University of Florida, Gainesville, Florida 32611, USA
| | - W. J. Weber
- Dipartimento di Fisica, Università di Trento and Trento Institute for Fundamental Physics and Application / INFN, 38123 Povo, Trento, Italy
| | - L. Wissel
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik und Leibniz Universität Hannover, Callinstraße 38, 30167 Hannover, Germany
| | - A. Wittchen
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik und Leibniz Universität Hannover, Callinstraße 38, 30167 Hannover, Germany
| | - P. Zweifel
- Institut für Geophysik, ETH Zürich, Sonneggstrasse 5, CH-8092, Zürich, Switzerland
| |
Collapse
|
8
|
Croxford S, Miller RF, Post FA, Harding R, Lucas SB, Figueroa J, Harrison I, Delpech VC, Dhoot S, Sullivan AK. Cause of death among HIV patients in London in 2016. HIV Med 2019; 20:628-633. [PMID: 31274241 DOI: 10.1111/hiv.12761] [Citation(s) in RCA: 3] [Impact Index Per Article: 0.6] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Accepted: 04/29/2019] [Indexed: 11/30/2022]
Abstract
OBJECTIVES Since 2013, the London HIV Mortality Review Group has conducted annual reviews of deaths among people with HIV to reduce avoidable mortality. METHODS All London HIV care Trusts reported data on 2016 patient deaths in 2017. Deaths were submitted using a modified Causes of Death in HIV reporting form and categorized by a specialist HIV pathologist and two HIV clinicians. RESULTS There were 206 deaths reported; 77% were among men. Median age at death was 56 years. Cause was established for 82% of deaths, with non-AIDS-related malignancies and AIDS-defining illnesses being the most common causes reported. Risk factors in the year before death included: tobacco smoking (37%), excessive alcohol consumption (19%), non-injecting drug use (10%), injecting drug use (7%) and opioid substitution therapy (6%). Thirty-nine per cent of patients had a history of depression, 33% chronic hypertension, 27% dyslipidaemia, 17% coinfection with hepatitis B virus and/or hepatitis C virus and 14% diabetes mellitus. At the time of death, 81% of patients were on antiretroviral therapy (ART), 61% had a CD4 count < 350 cells/μL, and 24% had a viral load ≥ 200 HIV-1 RNA copies/mL. Thirty-six per cent of deaths were unexpected; 61% of expected deaths were in hospital. Two-thirds of expected deaths had a prior end-of-life care discussion documented. CONCLUSIONS In 2016, most deaths were attributable to non-AIDS-related conditions and the majority of patients were on ART and virally suppressed. However, several potentially preventable deaths were identified and underlying risk factors were common. As London HIV patients are not representative of people with HIV in the UK, a national mortality review is warranted.
Collapse
Affiliation(s)
- S Croxford
- National Infection Service, Public Health England, London, UK
| | - R F Miller
- Central and North West London NHS Foundation Trust, Mortimer Market Centre, London, UK
| | - F A Post
- King's College Hospital NHS Foundation Trust, London, UK
| | - R Harding
- Florence Nightingale Faculty of Nursing Midwifery and Palliative Care, King's College London, London, UK
| | - S B Lucas
- Guy's & St Thomas' NHS Foundation Trust, London, UK
| | - J Figueroa
- National Infection Service, Public Health England, London, UK.,NHS England London, London, UK
| | | | - V C Delpech
- National Infection Service, Public Health England, London, UK
| | - S Dhoot
- Directorate of HIV and Sexual Health, Chelsea and Westminster Hospital NHS Foundation Trust, London, UK
| | - A K Sullivan
- National Infection Service, Public Health England, London, UK.,Directorate of HIV and Sexual Health, Chelsea and Westminster Hospital NHS Foundation Trust, London, UK
| |
Collapse
|
9
|
Armano M, Audley H, Baird J, Binetruy P, Born M, Bortoluzzi D, Castelli E, Cavalleri A, Cesarini A, Cruise A, Danzmann K, de Deus Silva M, Diepholz I, Dixon G, Dolesi R, Ferraioli L, Ferroni V, Fitzsimons E, Freschi M, Gesa L, Gibert F, Giardini D, Giusteri R, Grimani C, Grzymisch J, Harrison I, Heinzel G, Hewitson M, Hollington D, Hoyland D, Hueller M, Inchauspé H, Jennrich O, Jetzer P, Karnesis N, Kaune B, Korsakova N, Killow C, Lobo J, Lloro I, Liu L, López-Zaragoza J, Maarschalkerweerd R, Mance D, Meshksar N, Martín V, Martin-Polo L, Martino J, Martin-Porqueras F, Mateos I, McNamara P, Mendes J, Mendes L, Nofrarias M, Paczkowski S, Perreur-Lloyd M, Petiteau A, Pivato P, Plagnol E, Ramos-Castro J, Reiche J, Robertson D, Rivas F, Russano G, Slutsky J, Sopuerta C, Sumner T, Texier D, Thorpe J, Vetrugno D, Vitale S, Wanner G, Ward H, Wass P, Weber W, Wissel L, Wittchen A, Zweifel P. Calibrating the system dynamics of LISA Pathfinder. Int J Clin Exp Med 2018. [DOI: 10.1103/physrevd.97.122002] [Citation(s) in RCA: 13] [Impact Index Per Article: 2.2] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/07/2022]
|
10
|
Armano M, Audley H, Baird J, Binetruy P, Born M, Bortoluzzi D, Castelli E, Cavalleri A, Cesarini A, Cruise AM, Danzmann K, de Deus Silva M, Diepholz I, Dixon G, Dolesi R, Ferraioli L, Ferroni V, Fitzsimons ED, Freschi M, Gesa L, Gibert F, Giardini D, Giusteri R, Grimani C, Grzymisch J, Harrison I, Heinzel G, Hewitson M, Hollington D, Hoyland D, Hueller M, Inchauspé H, Jennrich O, Jetzer P, Karnesis N, Kaune B, Korsakova N, Killow CJ, Lobo JA, Lloro I, Liu L, López-Zaragoza JP, Maarschalkerweerd R, Mance D, Meshksar N, Martín V, Martin-Polo L, Martino J, Martin-Porqueras F, Mateos I, McNamara PW, Mendes J, Mendes L, Nofrarias M, Paczkowski S, Perreur-Lloyd M, Petiteau A, Pivato P, Plagnol E, Ramos-Castro J, Reiche J, Robertson DI, Rivas F, Russano G, Slutsky J, Sopuerta CF, Sumner T, Texier D, Thorpe JI, Vetrugno D, Vitale S, Wanner G, Ward H, Wass PJ, Weber WJ, Wissel L, Wittchen A, Zweifel P. Beyond the Required LISA Free-Fall Performance: New LISA Pathfinder Results down to 20 μHz. Phys Rev Lett 2018; 120:061101. [PMID: 29481269 DOI: 10.1103/physrevlett.120.061101] [Citation(s) in RCA: 17] [Impact Index Per Article: 2.8] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 12/11/2017] [Revised: 01/12/2018] [Indexed: 06/08/2023]
Abstract
In the months since the publication of the first results, the noise performance of LISA Pathfinder has improved because of reduced Brownian noise due to the continued decrease in pressure around the test masses, from a better correction of noninertial effects, and from a better calibration of the electrostatic force actuation. In addition, the availability of numerous long noise measurement runs, during which no perturbation is purposely applied to the test masses, has allowed the measurement of noise with good statistics down to 20 μHz. The Letter presents the measured differential acceleration noise figure, which is at (1.74±0.05) fm s^{-2}/sqrt[Hz] above 2 mHz and (6±1)×10 fm s^{-2}/sqrt[Hz] at 20 μHz, and discusses the physical sources for the measured noise. This performance provides an experimental benchmark demonstrating the ability to realize the low-frequency science potential of the LISA mission, recently selected by the European Space Agency.
Collapse
Affiliation(s)
- M Armano
- European Space Astronomy Centre, European Space Agency, Villanueva de la Cañada, 28692 Madrid, Spain
| | - H Audley
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik und Leibniz Universität Hannover, Callinstraße 38, 30167 Hannover, Germany
| | - J Baird
- High Energy Physics Group, Physics Department, Imperial College London, Blackett Laboratory, Prince Consort Road, London, SW7 2BW, United Kingdom
| | - P Binetruy
- APC, Université Paris Diderot, CNRS/IN2P3, CEA/lrfu, Observatoire de Paris, Sorbonne Paris Cité, France
| | - M Born
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik und Leibniz Universität Hannover, Callinstraße 38, 30167 Hannover, Germany
| | - D Bortoluzzi
- Department of Industrial Engineering, University of Trento, via Sommarive 9, 38123 Trento, and Trento Institute for Fundamental Physics and Application/INFN, Italy
| | - E Castelli
- Dipartimento di Fisica, Università di Trento and Trento Institute for Fundamental Physics and Application/INFN, 38123 Povo, Trento, Italy
| | - A Cavalleri
- Istituto di Fotonica e Nanotecnologie, CNR-Fondazione Bruno Kessler, I-38123 Povo, Trento, Italy
| | - A Cesarini
- DISPEA, Università di Urbino "Carlo Bo," Via S. Chiara, 27 61029 Urbino/INFN, Italy
| | - A M Cruise
- The School of Physics and Astronomy, University of Birmingham, Birmingham, United Kingdom
| | - K Danzmann
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik und Leibniz Universität Hannover, Callinstraße 38, 30167 Hannover, Germany
| | - M de Deus Silva
- European Space Astronomy Centre, European Space Agency, Villanueva de la Cañada, 28692 Madrid, Spain
| | - I Diepholz
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik und Leibniz Universität Hannover, Callinstraße 38, 30167 Hannover, Germany
| | - G Dixon
- The School of Physics and Astronomy, University of Birmingham, Birmingham, United Kingdom
| | - R Dolesi
- Dipartimento di Fisica, Università di Trento and Trento Institute for Fundamental Physics and Application/INFN, 38123 Povo, Trento, Italy
| | - L Ferraioli
- Institut für Geophysik, ETH Zürich, Sonneggstrasse 5, CH-8092, Zürich, Switzerland
| | - V Ferroni
- Dipartimento di Fisica, Università di Trento and Trento Institute for Fundamental Physics and Application/INFN, 38123 Povo, Trento, Italy
| | - E D Fitzsimons
- The UK Astronomy Technology Centre, Royal Observatory, Edinburgh, Blackford Hill, Edinburgh, EH9 3HJ, United Kingdom
| | - M Freschi
- European Space Astronomy Centre, European Space Agency, Villanueva de la Cañada, 28692 Madrid, Spain
| | - L Gesa
- Institut de Ciències de l'Espai (ICE, CSIC), Campus UAB, Carrer de Can Magrans s/n, 08193 Cerdanyola del Vallès, and Institut d'Estudis Espacials de Catalunya (IEEC), Gran Capità, 2-4, 08034 Barcelona, Spain
| | - F Gibert
- Dipartimento di Fisica, Università di Trento and Trento Institute for Fundamental Physics and Application/INFN, 38123 Povo, Trento, Italy
| | - D Giardini
- Institut für Geophysik, ETH Zürich, Sonneggstrasse 5, CH-8092, Zürich, Switzerland
| | - R Giusteri
- Dipartimento di Fisica, Università di Trento and Trento Institute for Fundamental Physics and Application/INFN, 38123 Povo, Trento, Italy
| | - C Grimani
- DISPEA, Università di Urbino "Carlo Bo," Via S. Chiara, 27 61029 Urbino/INFN, Italy
| | - J Grzymisch
- European Space Technology Centre, European Space Agency, Keplerlaan 1, 2200 AG Noordwijk, Netherlands
| | - I Harrison
- European Space Operations Centre, European Space Agency, 64293 Darmstadt, Germany
| | - G Heinzel
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik und Leibniz Universität Hannover, Callinstraße 38, 30167 Hannover, Germany
| | - M Hewitson
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik und Leibniz Universität Hannover, Callinstraße 38, 30167 Hannover, Germany
| | - D Hollington
- High Energy Physics Group, Physics Department, Imperial College London, Blackett Laboratory, Prince Consort Road, London, SW7 2BW, United Kingdom
| | - D Hoyland
- The School of Physics and Astronomy, University of Birmingham, Birmingham, United Kingdom
| | - M Hueller
- Dipartimento di Fisica, Università di Trento and Trento Institute for Fundamental Physics and Application/INFN, 38123 Povo, Trento, Italy
| | - H Inchauspé
- APC, Université Paris Diderot, CNRS/IN2P3, CEA/lrfu, Observatoire de Paris, Sorbonne Paris Cité, France
| | - O Jennrich
- European Space Technology Centre, European Space Agency, Keplerlaan 1, 2200 AG Noordwijk, Netherlands
| | - P Jetzer
- Physik Institut, Universität Zürich, Winterthurerstrasse 190, CH-8057 Zürich, Switzerland
| | - N Karnesis
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik und Leibniz Universität Hannover, Callinstraße 38, 30167 Hannover, Germany
| | - B Kaune
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik und Leibniz Universität Hannover, Callinstraße 38, 30167 Hannover, Germany
| | - N Korsakova
- SUPA, Institute for Gravitational Research, School of Physics and Astronomy, University of Glasgow, Glasgow, G12 8QQ, United Kingdom
| | - C J Killow
- SUPA, Institute for Gravitational Research, School of Physics and Astronomy, University of Glasgow, Glasgow, G12 8QQ, United Kingdom
| | - J A Lobo
- Institut de Ciències de l'Espai (ICE, CSIC), Campus UAB, Carrer de Can Magrans s/n, 08193 Cerdanyola del Vallès, and Institut d'Estudis Espacials de Catalunya (IEEC), Gran Capità, 2-4, 08034 Barcelona, Spain
| | - I Lloro
- Institut de Ciències de l'Espai (ICE, CSIC), Campus UAB, Carrer de Can Magrans s/n, 08193 Cerdanyola del Vallès, and Institut d'Estudis Espacials de Catalunya (IEEC), Gran Capità, 2-4, 08034 Barcelona, Spain
| | - L Liu
- Dipartimento di Fisica, Università di Trento and Trento Institute for Fundamental Physics and Application/INFN, 38123 Povo, Trento, Italy
| | - J P López-Zaragoza
- Institut de Ciències de l'Espai (ICE, CSIC), Campus UAB, Carrer de Can Magrans s/n, 08193 Cerdanyola del Vallès, and Institut d'Estudis Espacials de Catalunya (IEEC), Gran Capità, 2-4, 08034 Barcelona, Spain
| | - R Maarschalkerweerd
- European Space Operations Centre, European Space Agency, 64293 Darmstadt, Germany
| | - D Mance
- Institut für Geophysik, ETH Zürich, Sonneggstrasse 5, CH-8092, Zürich, Switzerland
| | - N Meshksar
- Institut für Geophysik, ETH Zürich, Sonneggstrasse 5, CH-8092, Zürich, Switzerland
| | - V Martín
- Institut de Ciències de l'Espai (ICE, CSIC), Campus UAB, Carrer de Can Magrans s/n, 08193 Cerdanyola del Vallès, and Institut d'Estudis Espacials de Catalunya (IEEC), Gran Capità, 2-4, 08034 Barcelona, Spain
| | - L Martin-Polo
- European Space Astronomy Centre, European Space Agency, Villanueva de la Cañada, 28692 Madrid, Spain
| | - J Martino
- APC, Université Paris Diderot, CNRS/IN2P3, CEA/lrfu, Observatoire de Paris, Sorbonne Paris Cité, France
| | - F Martin-Porqueras
- European Space Astronomy Centre, European Space Agency, Villanueva de la Cañada, 28692 Madrid, Spain
| | - I Mateos
- Institut de Ciències de l'Espai (ICE, CSIC), Campus UAB, Carrer de Can Magrans s/n, 08193 Cerdanyola del Vallès, and Institut d'Estudis Espacials de Catalunya (IEEC), Gran Capità, 2-4, 08034 Barcelona, Spain
| | - P W McNamara
- European Space Technology Centre, European Space Agency, Keplerlaan 1, 2200 AG Noordwijk, Netherlands
| | - J Mendes
- European Space Operations Centre, European Space Agency, 64293 Darmstadt, Germany
| | - L Mendes
- European Space Astronomy Centre, European Space Agency, Villanueva de la Cañada, 28692 Madrid, Spain
| | - M Nofrarias
- Institut de Ciències de l'Espai (ICE, CSIC), Campus UAB, Carrer de Can Magrans s/n, 08193 Cerdanyola del Vallès, and Institut d'Estudis Espacials de Catalunya (IEEC), Gran Capità, 2-4, 08034 Barcelona, Spain
| | - S Paczkowski
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik und Leibniz Universität Hannover, Callinstraße 38, 30167 Hannover, Germany
| | - M Perreur-Lloyd
- SUPA, Institute for Gravitational Research, School of Physics and Astronomy, University of Glasgow, Glasgow, G12 8QQ, United Kingdom
| | - A Petiteau
- APC, Université Paris Diderot, CNRS/IN2P3, CEA/lrfu, Observatoire de Paris, Sorbonne Paris Cité, France
| | - P Pivato
- Dipartimento di Fisica, Università di Trento and Trento Institute for Fundamental Physics and Application/INFN, 38123 Povo, Trento, Italy
| | - E Plagnol
- APC, Université Paris Diderot, CNRS/IN2P3, CEA/lrfu, Observatoire de Paris, Sorbonne Paris Cité, France
| | - J Ramos-Castro
- Department d'Enginyeria Electrònica, Universitat Politècnica de Catalunya, and Institut d'Estudis Espacials de Catalunya (IEEC), Gran Capità, 2-4, 08034 Barcelona, Spain
| | - J Reiche
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik und Leibniz Universität Hannover, Callinstraße 38, 30167 Hannover, Germany
| | - D I Robertson
- SUPA, Institute for Gravitational Research, School of Physics and Astronomy, University of Glasgow, Glasgow, G12 8QQ, United Kingdom
| | - F Rivas
- Institut de Ciències de l'Espai (ICE, CSIC), Campus UAB, Carrer de Can Magrans s/n, 08193 Cerdanyola del Vallès, and Institut d'Estudis Espacials de Catalunya (IEEC), Gran Capità, 2-4, 08034 Barcelona, Spain
| | - G Russano
- Dipartimento di Fisica, Università di Trento and Trento Institute for Fundamental Physics and Application/INFN, 38123 Povo, Trento, Italy
| | - J Slutsky
- Gravitational Astrophysics Lab, NASA Goddard Space Flight Center, 8800 Greenbelt Road, Greenbelt, Maryland 20771, USA
| | - C F Sopuerta
- Institut de Ciències de l'Espai (ICE, CSIC), Campus UAB, Carrer de Can Magrans s/n, 08193 Cerdanyola del Vallès, and Institut d'Estudis Espacials de Catalunya (IEEC), Gran Capità, 2-4, 08034 Barcelona, Spain
| | - T Sumner
- High Energy Physics Group, Physics Department, Imperial College London, Blackett Laboratory, Prince Consort Road, London, SW7 2BW, United Kingdom
| | - D Texier
- European Space Astronomy Centre, European Space Agency, Villanueva de la Cañada, 28692 Madrid, Spain
| | - J I Thorpe
- Gravitational Astrophysics Lab, NASA Goddard Space Flight Center, 8800 Greenbelt Road, Greenbelt, Maryland 20771, USA
| | - D Vetrugno
- Dipartimento di Fisica, Università di Trento and Trento Institute for Fundamental Physics and Application/INFN, 38123 Povo, Trento, Italy
| | - S Vitale
- Dipartimento di Fisica, Università di Trento and Trento Institute for Fundamental Physics and Application/INFN, 38123 Povo, Trento, Italy
| | - G Wanner
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik und Leibniz Universität Hannover, Callinstraße 38, 30167 Hannover, Germany
| | - H Ward
- SUPA, Institute for Gravitational Research, School of Physics and Astronomy, University of Glasgow, Glasgow, G12 8QQ, United Kingdom
| | - P J Wass
- High Energy Physics Group, Physics Department, Imperial College London, Blackett Laboratory, Prince Consort Road, London, SW7 2BW, United Kingdom
- Department of Mechanical and Aerospace Engineering, MAE-A, P.O. Box 116250, University of Florida, Gainesville, Florida 32611, USA
| | - W J Weber
- Dipartimento di Fisica, Università di Trento and Trento Institute for Fundamental Physics and Application/INFN, 38123 Povo, Trento, Italy
| | - L Wissel
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik und Leibniz Universität Hannover, Callinstraße 38, 30167 Hannover, Germany
| | - A Wittchen
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik und Leibniz Universität Hannover, Callinstraße 38, 30167 Hannover, Germany
| | - P Zweifel
- Institut für Geophysik, ETH Zürich, Sonneggstrasse 5, CH-8092, Zürich, Switzerland
| |
Collapse
|
11
|
Lau S, Lim H, Ravoof T, Yaacob M, Grant D, MacKenzie R, Harrison I, Huang N. A three-electrode integrated photo-supercapacitor utilizing graphene-based intermediate bifunctional electrode. Electrochim Acta 2017. [DOI: 10.1016/j.electacta.2017.04.003] [Citation(s) in RCA: 31] [Impact Index Per Article: 4.4] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 10/19/2022]
|
12
|
Armano M, Audley H, Auger G, Baird JT, Binetruy P, Born M, Bortoluzzi D, Brandt N, Bursi A, Caleno M, Cavalleri A, Cesarini A, Cruise M, Danzmann K, de Deus Silva M, Diepholz I, Dolesi R, Dunbar N, Ferraioli L, Ferroni V, Fitzsimons ED, Flatscher R, Freschi M, Gallegos J, García Marirrodriga C, Gerndt R, Gesa L, Gibert F, Giardini D, Giusteri R, Grimani C, Grzymisch J, Harrison I, Heinzel G, Hewitson M, Hollington D, Hueller M, Huesler J, Inchauspé H, Jennrich O, Jetzer P, Johlander B, Karnesis N, Kaune B, Killow CJ, Korsakova N, Lloro I, Liu L, López-Zaragoza JP, Maarschalkerweerd R, Madden S, Mance D, Martín V, Martin-Polo L, Martino J, Martin-Porqueras F, Mateos I, McNamara PW, Mendes J, Mendes L, Moroni A, Nofrarias M, Paczkowski S, Perreur-Lloyd M, Petiteau A, Pivato P, Plagnol E, Prat P, Ragnit U, Ramos-Castro J, Reiche J, Romera Perez JA, Robertson DI, Rozemeijer H, Rivas F, Russano G, Sarra P, Schleicher A, Slutsky J, Sopuerta C, Sumner TJ, Texier D, Thorpe JI, Trenkel C, Vetrugno D, Vitale S, Wanner G, Ward H, Wass PJ, Wealthy D, Weber WJ, Wittchen A, Zanoni C, Ziegler T, Zweifel P. Charge-Induced Force Noise on Free-Falling Test Masses: Results from LISA Pathfinder. Phys Rev Lett 2017; 118:171101. [PMID: 28498710 DOI: 10.1103/physrevlett.118.171101] [Citation(s) in RCA: 4] [Impact Index Per Article: 0.6] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 02/16/2017] [Indexed: 06/07/2023]
Abstract
We report on electrostatic measurements made on board the European Space Agency mission LISA Pathfinder. Detailed measurements of the charge-induced electrostatic forces exerted on free-falling test masses (TMs) inside the capacitive gravitational reference sensor are the first made in a relevant environment for a space-based gravitational wave detector. Employing a combination of charge control and electric-field compensation, we show that the level of charge-induced acceleration noise on a single TM can be maintained at a level close to 1.0 fm s^{-2} Hz^{-1/2} across the 0.1-100 mHz frequency band that is crucial to an observatory such as the Laser Interferometer Space Antenna (LISA). Using dedicated measurements that detect these effects in the differential acceleration between the two test masses, we resolve the stochastic nature of the TM charge buildup due to interplanetary cosmic rays and the TM charge-to-force coupling through stray electric fields in the sensor. All our measurements are in good agreement with predictions based on a relatively simple electrostatic model of the LISA Pathfinder instrument.
Collapse
Affiliation(s)
- M Armano
- European Space Astronomy Centre, European Space Agency, Villanueva de la Cañada, 28692 Madrid, Spain
| | - H Audley
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik und Universität Hannover, 30167 Hannover, Germany
| | - G Auger
- APC UMR7164, Université Paris Diderot, 10, rue Alice Domon et Léonie Duquet, 75205 Paris Cedex 13, France
| | - J T Baird
- High Energy Physics Group, Department of Physics, Imperial College London, Blackett Laboratory, Prince Consort Road, London SW7 2BW, United Kingdom
| | - P Binetruy
- APC UMR7164, Université Paris Diderot, 10, rue Alice Domon et Léonie Duquet, 75205 Paris Cedex 13, France
| | - M Born
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik und Universität Hannover, 30167 Hannover, Germany
| | - D Bortoluzzi
- Department of Industrial Engineering, University of Trento, via Sommarive 9, 38123 Trento, Italy and Trento Institute for Fundamental Physics and Application/INFN, Italy
| | - N Brandt
- Airbus Defence and Space, Claude-Dornier-Strasse, 88090 Immenstaad, Germany
| | - A Bursi
- CGS S.p.A, Compagnia Generale per lo Spazio, Via Gallarate, 150-20151 Milano, Italy
| | - M Caleno
- European Space Technology Centre, European Space Agency, Keplerlaan 1, 2200 AG Noordwijk, Netherlands
| | - A Cavalleri
- Dipartimento di Fisica, Università di Trento and Trento Institute for Fundamental Physics and Application/INFN, 38123 Povo, Trento, Italy
| | - A Cesarini
- Dipartimento di Fisica, Università di Trento and Trento Institute for Fundamental Physics and Application/INFN, 38123 Povo, Trento, Italy
| | - M Cruise
- Department of Physics and Astronomy, University of Birmingham, Birmingham, Edgbaston Park Road, Birmingham B15 2TT, United Kingdom
| | - K Danzmann
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik und Universität Hannover, 30167 Hannover, Germany
| | - M de Deus Silva
- European Space Astronomy Centre, European Space Agency, Villanueva de la Cañada, 28692 Madrid, Spain
| | - I Diepholz
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik und Universität Hannover, 30167 Hannover, Germany
| | - R Dolesi
- Dipartimento di Fisica, Università di Trento and Trento Institute for Fundamental Physics and Application/INFN, 38123 Povo, Trento, Italy
| | - N Dunbar
- Airbus Defence and Space, Gunnels Wood Road, Stevenage, Hertfordshire SG1 2AS, United Kingdom
| | - L Ferraioli
- Institut für Geophysik, ETH Zürich, Sonneggstrasse 5, CH-8092, Zürich, Switzerland
| | - V Ferroni
- Dipartimento di Fisica, Università di Trento and Trento Institute for Fundamental Physics and Application/INFN, 38123 Povo, Trento, Italy
| | - E D Fitzsimons
- United Kingdom Astronomy Technology Centre, Royal Observatory, Edinburgh EH9 3HJ, United Kingdom
| | - R Flatscher
- Airbus Defence and Space, Claude-Dornier-Strasse, 88090 Immenstaad, Germany
| | - M Freschi
- European Space Astronomy Centre, European Space Agency, Villanueva de la Cañada, 28692 Madrid, Spain
| | - J Gallegos
- European Space Astronomy Centre, European Space Agency, Villanueva de la Cañada, 28692 Madrid, Spain
| | - C García Marirrodriga
- European Space Technology Centre, European Space Agency, Keplerlaan 1, 2200 AG Noordwijk, Netherlands
| | - R Gerndt
- Airbus Defence and Space, Claude-Dornier-Strasse, 88090 Immenstaad, Germany
| | - L Gesa
- Institut de Ciències de l'Espai (CSIC-IEEC), Campus UAB, Carrer de Can Magrans s/n, 08193 Cerdanyola del Vallès, Spain
| | - F Gibert
- Dipartimento di Fisica, Università di Trento and Trento Institute for Fundamental Physics and Application/INFN, 38123 Povo, Trento, Italy
| | - D Giardini
- Institut für Geophysik, ETH Zürich, Sonneggstrasse 5, CH-8092, Zürich, Switzerland
| | - R Giusteri
- Dipartimento di Fisica, Università di Trento and Trento Institute for Fundamental Physics and Application/INFN, 38123 Povo, Trento, Italy
| | - C Grimani
- DiSPeA, Università di Urbino "Carlo Bo", Via S. Chiara, 27 61029 Urbino/INFN, Italy
| | - J Grzymisch
- European Space Technology Centre, European Space Agency, Keplerlaan 1, 2200 AG Noordwijk, Netherlands
| | - I Harrison
- European Space Operations Centre, European Space Agency, 64293 Darmstadt, Germany
| | - G Heinzel
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik und Universität Hannover, 30167 Hannover, Germany
| | - M Hewitson
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik und Universität Hannover, 30167 Hannover, Germany
| | - D Hollington
- High Energy Physics Group, Department of Physics, Imperial College London, Blackett Laboratory, Prince Consort Road, London SW7 2BW, United Kingdom
| | - M Hueller
- Dipartimento di Fisica, Università di Trento and Trento Institute for Fundamental Physics and Application/INFN, 38123 Povo, Trento, Italy
| | - J Huesler
- European Space Technology Centre, European Space Agency, Keplerlaan 1, 2200 AG Noordwijk, Netherlands
| | - H Inchauspé
- APC UMR7164, Université Paris Diderot, 10, rue Alice Domon et Léonie Duquet, 75205 Paris Cedex 13, France
| | - O Jennrich
- European Space Technology Centre, European Space Agency, Keplerlaan 1, 2200 AG Noordwijk, Netherlands
| | - P Jetzer
- Physik Institut, Universität Zürich, Winterthurerstrasse 190, CH-8057 Zürich, Switzerland
| | - B Johlander
- European Space Technology Centre, European Space Agency, Keplerlaan 1, 2200 AG Noordwijk, Netherlands
| | - N Karnesis
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik und Universität Hannover, 30167 Hannover, Germany
| | - B Kaune
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik und Universität Hannover, 30167 Hannover, Germany
| | - C J Killow
- SUPA, Institute for Gravitational Research, School of Physics and Astronomy, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - N Korsakova
- SUPA, Institute for Gravitational Research, School of Physics and Astronomy, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - I Lloro
- Institut de Ciències de l'Espai (CSIC-IEEC), Campus UAB, Carrer de Can Magrans s/n, 08193 Cerdanyola del Vallès, Spain
| | - L Liu
- Dipartimento di Fisica, Università di Trento and Trento Institute for Fundamental Physics and Application/INFN, 38123 Povo, Trento, Italy
| | - J P López-Zaragoza
- Institut de Ciències de l'Espai (CSIC-IEEC), Campus UAB, Carrer de Can Magrans s/n, 08193 Cerdanyola del Vallès, Spain
| | - R Maarschalkerweerd
- European Space Operations Centre, European Space Agency, 64293 Darmstadt, Germany
| | - S Madden
- European Space Technology Centre, European Space Agency, Keplerlaan 1, 2200 AG Noordwijk, Netherlands
| | - D Mance
- Institut für Geophysik, ETH Zürich, Sonneggstrasse 5, CH-8092, Zürich, Switzerland
| | - V Martín
- Institut de Ciències de l'Espai (CSIC-IEEC), Campus UAB, Carrer de Can Magrans s/n, 08193 Cerdanyola del Vallès, Spain
| | - L Martin-Polo
- European Space Astronomy Centre, European Space Agency, Villanueva de la Cañada, 28692 Madrid, Spain
| | - J Martino
- APC UMR7164, Université Paris Diderot, 10, rue Alice Domon et Léonie Duquet, 75205 Paris Cedex 13, France
| | - F Martin-Porqueras
- European Space Astronomy Centre, European Space Agency, Villanueva de la Cañada, 28692 Madrid, Spain
| | - I Mateos
- Institut de Ciències de l'Espai (CSIC-IEEC), Campus UAB, Carrer de Can Magrans s/n, 08193 Cerdanyola del Vallès, Spain
| | - P W McNamara
- European Space Technology Centre, European Space Agency, Keplerlaan 1, 2200 AG Noordwijk, Netherlands
| | - J Mendes
- European Space Operations Centre, European Space Agency, 64293 Darmstadt, Germany
| | - L Mendes
- European Space Astronomy Centre, European Space Agency, Villanueva de la Cañada, 28692 Madrid, Spain
| | - A Moroni
- CGS S.p.A, Compagnia Generale per lo Spazio, Via Gallarate, 150-20151 Milano, Italy
| | - M Nofrarias
- Institut de Ciències de l'Espai (CSIC-IEEC), Campus UAB, Carrer de Can Magrans s/n, 08193 Cerdanyola del Vallès, Spain
| | - S Paczkowski
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik und Universität Hannover, 30167 Hannover, Germany
| | - M Perreur-Lloyd
- SUPA, Institute for Gravitational Research, School of Physics and Astronomy, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - A Petiteau
- APC UMR7164, Université Paris Diderot, 10, rue Alice Domon et Léonie Duquet, 75205 Paris Cedex 13, France
| | - P Pivato
- Dipartimento di Fisica, Università di Trento and Trento Institute for Fundamental Physics and Application/INFN, 38123 Povo, Trento, Italy
| | - E Plagnol
- APC UMR7164, Université Paris Diderot, 10, rue Alice Domon et Léonie Duquet, 75205 Paris Cedex 13, France
| | - P Prat
- APC UMR7164, Université Paris Diderot, 10, rue Alice Domon et Léonie Duquet, 75205 Paris Cedex 13, France
| | - U Ragnit
- European Space Technology Centre, European Space Agency, Keplerlaan 1, 2200 AG Noordwijk, Netherlands
| | - J Ramos-Castro
- Department d'Enginyeria Electrònica, Universitat Politècnica de Catalunya, 08034 Barcelona, Spain
- Institut d'Estudis Espacials de Catalunya (IEEC), C/ Gran Capità 2-4, 08034 Barcelona, Spain
| | - J Reiche
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik und Universität Hannover, 30167 Hannover, Germany
| | - J A Romera Perez
- European Space Technology Centre, European Space Agency, Keplerlaan 1, 2200 AG Noordwijk, Netherlands
| | - D I Robertson
- SUPA, Institute for Gravitational Research, School of Physics and Astronomy, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - H Rozemeijer
- European Space Technology Centre, European Space Agency, Keplerlaan 1, 2200 AG Noordwijk, Netherlands
| | - F Rivas
- Institut de Ciències de l'Espai (CSIC-IEEC), Campus UAB, Carrer de Can Magrans s/n, 08193 Cerdanyola del Vallès, Spain
| | - G Russano
- Dipartimento di Fisica, Università di Trento and Trento Institute for Fundamental Physics and Application/INFN, 38123 Povo, Trento, Italy
| | - P Sarra
- CGS S.p.A, Compagnia Generale per lo Spazio, Via Gallarate, 150-20151 Milano, Italy
| | - A Schleicher
- Airbus Defence and Space, Claude-Dornier-Strasse, 88090 Immenstaad, Germany
| | - J Slutsky
- NASA Goddard Space Flight Center, 8800 Greenbelt Road, Greenbelt, Maryland 20771, USA
| | - C Sopuerta
- Institut de Ciències de l'Espai (CSIC-IEEC), Campus UAB, Carrer de Can Magrans s/n, 08193 Cerdanyola del Vallès, Spain
| | - T J Sumner
- High Energy Physics Group, Department of Physics, Imperial College London, Blackett Laboratory, Prince Consort Road, London SW7 2BW, United Kingdom
| | - D Texier
- European Space Astronomy Centre, European Space Agency, Villanueva de la Cañada, 28692 Madrid, Spain
| | - J I Thorpe
- NASA Goddard Space Flight Center, 8800 Greenbelt Road, Greenbelt, Maryland 20771, USA
| | - C Trenkel
- Airbus Defence and Space, Gunnels Wood Road, Stevenage, Hertfordshire SG1 2AS, United Kingdom
| | - D Vetrugno
- Dipartimento di Fisica, Università di Trento and Trento Institute for Fundamental Physics and Application/INFN, 38123 Povo, Trento, Italy
| | - S Vitale
- Dipartimento di Fisica, Università di Trento and Trento Institute for Fundamental Physics and Application/INFN, 38123 Povo, Trento, Italy
| | - G Wanner
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik und Universität Hannover, 30167 Hannover, Germany
| | - H Ward
- SUPA, Institute for Gravitational Research, School of Physics and Astronomy, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - P J Wass
- High Energy Physics Group, Department of Physics, Imperial College London, Blackett Laboratory, Prince Consort Road, London SW7 2BW, United Kingdom
| | - D Wealthy
- Airbus Defence and Space, Gunnels Wood Road, Stevenage, Hertfordshire SG1 2AS, United Kingdom
| | - W J Weber
- Dipartimento di Fisica, Università di Trento and Trento Institute for Fundamental Physics and Application/INFN, 38123 Povo, Trento, Italy
| | - A Wittchen
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik und Universität Hannover, 30167 Hannover, Germany
| | - C Zanoni
- Department of Industrial Engineering, University of Trento, via Sommarive 9, 38123 Trento, Italy and Trento Institute for Fundamental Physics and Application/INFN, Italy
| | - T Ziegler
- Airbus Defence and Space, Claude-Dornier-Strasse, 88090 Immenstaad, Germany
| | - P Zweifel
- Institut für Geophysik, ETH Zürich, Sonneggstrasse 5, CH-8092, Zürich, Switzerland
| |
Collapse
|
13
|
Chee WK, Lim HN, Zainal Z, Harrison I, Huang N, Andou Y, Chong KF, Pandikumar A. Electrospun nanofiber membranes as ultrathin flexible supercapacitors. RSC Adv 2017. [DOI: 10.1039/c7ra00406k] [Citation(s) in RCA: 27] [Impact Index Per Article: 3.9] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/21/2022] Open
Abstract
A highly flexible electrochemical supercapacitor electrode was developed with a novel metal oxide-reinforced nanofiber electrode by utilizing a solution-based electrospinning technique.
Collapse
Affiliation(s)
- W. K. Chee
- Department of Chemistry
- Faculty of Science
- Universiti Putra Malaysia
- Malaysia
| | - H. N. Lim
- Department of Chemistry
- Faculty of Science
- Universiti Putra Malaysia
- Malaysia
- Functional Device Laboratory
| | - Z. Zainal
- Department of Chemistry
- Faculty of Science
- Universiti Putra Malaysia
- Malaysia
| | - I. Harrison
- Department of Electrical and Electronic Engineering
- Faculty of Engineering
- University of Nottingham
- Nottingham NG7 2RD
- UK
| | - N. M. Huang
- Centre of Printable Electronics
- Deputy Vice Chancellor Office (Research & Innovation)
- University of Malaya
- 50603 Kuala Lumpur
- Malaysia
| | - Y. Andou
- Graduate School of Life Science and Systems Engineering
- Eco-Town Collaborative R&D Center for the Environment and Recycling
- Kyushu Institute of Technology
- Kitakyushu-city
- Japan
| | - K. F. Chong
- Faculty of Industrial Sciences & Technology
- Universiti Malaysia Pahang
- Kuantan
- Malaysia
| | - A. Pandikumar
- Research Institute & Department of Chemistry
- SRM University
- Chennai
- India
| |
Collapse
|
14
|
Armano M, Audley H, Auger G, Baird JT, Bassan M, Binetruy P, Born M, Bortoluzzi D, Brandt N, Caleno M, Carbone L, Cavalleri A, Cesarini A, Ciani G, Congedo G, Cruise AM, Danzmann K, de Deus Silva M, De Rosa R, Diaz-Aguiló M, Di Fiore L, Diepholz I, Dixon G, Dolesi R, Dunbar N, Ferraioli L, Ferroni V, Fichter W, Fitzsimons ED, Flatscher R, Freschi M, García Marín AF, García Marirrodriga C, Gerndt R, Gesa L, Gibert F, Giardini D, Giusteri R, Guzmán F, Grado A, Grimani C, Grynagier A, Grzymisch J, Harrison I, Heinzel G, Hewitson M, Hollington D, Hoyland D, Hueller M, Inchauspé H, Jennrich O, Jetzer P, Johann U, Johlander B, Karnesis N, Kaune B, Korsakova N, Killow CJ, Lobo JA, Lloro I, Liu L, López-Zaragoza JP, Maarschalkerweerd R, Mance D, Martín V, Martin-Polo L, Martino J, Martin-Porqueras F, Madden S, Mateos I, McNamara PW, Mendes J, Mendes L, Monsky A, Nicolodi D, Nofrarias M, Paczkowski S, Perreur-Lloyd M, Petiteau A, Pivato P, Plagnol E, Prat P, Ragnit U, Raïs B, Ramos-Castro J, Reiche J, Robertson DI, Rozemeijer H, Rivas F, Russano G, Sanjuán J, Sarra P, Schleicher A, Shaul D, Slutsky J, Sopuerta CF, Stanga R, Steier F, Sumner T, Texier D, Thorpe JI, Trenkel C, Tröbs M, Tu HB, Vetrugno D, Vitale S, Wand V, Wanner G, Ward H, Warren C, Wass PJ, Wealthy D, Weber WJ, Wissel L, Wittchen A, Zambotti A, Zanoni C, Ziegler T, Zweifel P. Sub-Femto-g Free Fall for Space-Based Gravitational Wave Observatories: LISA Pathfinder Results. Phys Rev Lett 2016; 116:231101. [PMID: 27341221 DOI: 10.1103/physrevlett.116.231101] [Citation(s) in RCA: 79] [Impact Index Per Article: 9.9] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 05/04/2016] [Indexed: 05/27/2023]
Abstract
We report the first results of the LISA Pathfinder in-flight experiment. The results demonstrate that two free-falling reference test masses, such as those needed for a space-based gravitational wave observatory like LISA, can be put in free fall with a relative acceleration noise with a square root of the power spectral density of 5.2±0.1 fm s^{-2}/sqrt[Hz], or (0.54±0.01)×10^{-15} g/sqrt[Hz], with g the standard gravity, for frequencies between 0.7 and 20 mHz. This value is lower than the LISA Pathfinder requirement by more than a factor 5 and within a factor 1.25 of the requirement for the LISA mission, and is compatible with Brownian noise from viscous damping due to the residual gas surrounding the test masses. Above 60 mHz the acceleration noise is dominated by interferometer displacement readout noise at a level of (34.8±0.3) fm/sqrt[Hz], about 2 orders of magnitude better than requirements. At f≤0.5 mHz we observe a low-frequency tail that stays below 12 fm s^{-2}/sqrt[Hz] down to 0.1 mHz. This performance would allow for a space-based gravitational wave observatory with a sensitivity close to what was originally foreseen for LISA.
Collapse
Affiliation(s)
- M Armano
- European Space Astronomy Centre, European Space Agency, Villanueva de la Cañada, 28692 Madrid, Spain
| | - H Audley
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik und Leibniz Universität Hannover, Callinstraße 38, 30167 Hannover, Germany
| | - G Auger
- APC, Université Paris Diderot, CNRS/IN2P3, CEA/lrfu, Obs de Paris, Sorbonne Paris Cité, France
| | - J T Baird
- High Energy Physics Group, Physics Department, Imperial College London, Blackett Laboratory, Prince Consort Road, London, SW7 2BW, United Kingdom
| | - M Bassan
- Dipartimento di Fisica, Università di Roma "Tor Vergata", and INFN, sezione Roma Tor Vergata, I-00133 Roma, Italy
| | - P Binetruy
- APC, Université Paris Diderot, CNRS/IN2P3, CEA/lrfu, Obs de Paris, Sorbonne Paris Cité, France
| | - M Born
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik und Leibniz Universität Hannover, Callinstraße 38, 30167 Hannover, Germany
| | - D Bortoluzzi
- Department of Industrial Engineering, University of Trento, via Sommarive 9, 38123 Trento, and Trento Institute for Fundamental Physics and Applications/INFN, Italy
| | - N Brandt
- Airbus Defence and Space, Claude-Dornier-Strasse, 88090 Immenstaad, Germany
| | - M Caleno
- European Space Technology Centre, European Space Agency, Keplerlaan 1, 2200 AG Noordwijk, Netherlands
| | - L Carbone
- Dipartimento di Fisica, Università di Trento and Trento Institute for Fundamental Physics and Applications/INFN, 38123 Povo, Trento, Italy
| | - A Cavalleri
- Istituto di Fotonica e Nanotecnologie, CNR-Fondazione Bruno Kessler, I-38123 Povo, Trento, Italy
| | - A Cesarini
- Dipartimento di Fisica, Università di Trento and Trento Institute for Fundamental Physics and Applications/INFN, 38123 Povo, Trento, Italy
| | - G Ciani
- Dipartimento di Fisica, Università di Trento and Trento Institute for Fundamental Physics and Applications/INFN, 38123 Povo, Trento, Italy
| | - G Congedo
- Dipartimento di Fisica, Università di Trento and Trento Institute for Fundamental Physics and Applications/INFN, 38123 Povo, Trento, Italy
| | - A M Cruise
- The School of Physics and Astronomy, University of Birmingham, Birmingham, United Kingdom
| | - K Danzmann
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik und Leibniz Universität Hannover, Callinstraße 38, 30167 Hannover, Germany
| | - M de Deus Silva
- European Space Astronomy Centre, European Space Agency, Villanueva de la Cañada, 28692 Madrid, Spain
| | - R De Rosa
- Dipartimento di Fisica, Università di Napoli "Federico II" and INFN-Sezione di Napoli, I-80126, Napoli, Italy
| | - M Diaz-Aguiló
- Institut de Ciències de l'Espai (CSIC-IEEC), Campus UAB, Carrer de Can Magrans s/n, 08193 Cerdanyola del Vallès, Spain
| | - L Di Fiore
- INFN-Sezione di Napoli, I-80126, Napoli, Italy
| | - I Diepholz
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik und Leibniz Universität Hannover, Callinstraße 38, 30167 Hannover, Germany
| | - G Dixon
- The School of Physics and Astronomy, University of Birmingham, Birmingham, United Kingdom
| | - R Dolesi
- Dipartimento di Fisica, Università di Trento and Trento Institute for Fundamental Physics and Applications/INFN, 38123 Povo, Trento, Italy
| | - N Dunbar
- Airbus Defence and Space, Gunnels Wood Road, Stevenage, Hertfordshire, SG1 2AS, United Kingdom
| | - L Ferraioli
- Institut für Geophysik, ETH Zürich, Sonneggstrasse 5, CH-8092, Zürich, Switzerland
| | - V Ferroni
- Dipartimento di Fisica, Università di Trento and Trento Institute for Fundamental Physics and Applications/INFN, 38123 Povo, Trento, Italy
| | - W Fichter
- Universitt Stuttgart, Institut fr Flugmechanik und Flugregelung, Pfaffenwaldring 27, 70569 Stuttgart, Germany
| | - E D Fitzsimons
- The UK Astronomy Technology Centre, Royal Observatory, Edinburgh, Blackford Hill, Edinburgh, EH9 3HJ, United Kingdom
| | - R Flatscher
- Airbus Defence and Space, Claude-Dornier-Strasse, 88090 Immenstaad, Germany
| | - M Freschi
- European Space Astronomy Centre, European Space Agency, Villanueva de la Cañada, 28692 Madrid, Spain
| | - A F García Marín
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik und Leibniz Universität Hannover, Callinstraße 38, 30167 Hannover, Germany
| | - C García Marirrodriga
- European Space Technology Centre, European Space Agency, Keplerlaan 1, 2200 AG Noordwijk, Netherlands
| | - R Gerndt
- Airbus Defence and Space, Claude-Dornier-Strasse, 88090 Immenstaad, Germany
| | - L Gesa
- Institut de Ciències de l'Espai (CSIC-IEEC), Campus UAB, Carrer de Can Magrans s/n, 08193 Cerdanyola del Vallès, Spain
| | - F Gibert
- Dipartimento di Fisica, Università di Trento and Trento Institute for Fundamental Physics and Applications/INFN, 38123 Povo, Trento, Italy
| | - D Giardini
- Institut für Geophysik, ETH Zürich, Sonneggstrasse 5, CH-8092, Zürich, Switzerland
| | - R Giusteri
- Dipartimento di Fisica, Università di Trento and Trento Institute for Fundamental Physics and Applications/INFN, 38123 Povo, Trento, Italy
| | - F Guzmán
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik und Leibniz Universität Hannover, Callinstraße 38, 30167 Hannover, Germany
| | - A Grado
- INAF Osservatorio Astronomico di Capodimonte, I-80131 Napoli, Italy and INFN sezione di Napoli, I-80126 Napoli, Italy
| | - C Grimani
- DISPEA, Università di Urbino "Carlo Bo", Via S. Chiara, 27 61029 Urbino/INFN, Italy
| | - A Grynagier
- Universitt Stuttgart, Institut fr Flugmechanik und Flugregelung, Pfaffenwaldring 27, 70569 Stuttgart, Germany
| | - J Grzymisch
- European Space Technology Centre, European Space Agency, Keplerlaan 1, 2200 AG Noordwijk, Netherlands
| | - I Harrison
- European Space Operations Centre, European Space Agency, 64293 Darmstadt, Germany
| | - G Heinzel
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik und Leibniz Universität Hannover, Callinstraße 38, 30167 Hannover, Germany
| | - M Hewitson
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik und Leibniz Universität Hannover, Callinstraße 38, 30167 Hannover, Germany
| | - D Hollington
- High Energy Physics Group, Physics Department, Imperial College London, Blackett Laboratory, Prince Consort Road, London, SW7 2BW, United Kingdom
| | - D Hoyland
- The School of Physics and Astronomy, University of Birmingham, Birmingham, United Kingdom
| | - M Hueller
- Dipartimento di Fisica, Università di Trento and Trento Institute for Fundamental Physics and Applications/INFN, 38123 Povo, Trento, Italy
| | - H Inchauspé
- APC, Université Paris Diderot, CNRS/IN2P3, CEA/lrfu, Obs de Paris, Sorbonne Paris Cité, France
| | - O Jennrich
- European Space Technology Centre, European Space Agency, Keplerlaan 1, 2200 AG Noordwijk, Netherlands
| | - P Jetzer
- Physik Institut, Universität Zürich, Winterthurerstrasse 190, CH-8057 Zürich, Switzerland
| | - U Johann
- Airbus Defence and Space, Claude-Dornier-Strasse, 88090 Immenstaad, Germany
| | - B Johlander
- European Space Technology Centre, European Space Agency, Keplerlaan 1, 2200 AG Noordwijk, Netherlands
| | - N Karnesis
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik und Leibniz Universität Hannover, Callinstraße 38, 30167 Hannover, Germany
| | - B Kaune
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik und Leibniz Universität Hannover, Callinstraße 38, 30167 Hannover, Germany
| | - N Korsakova
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik und Leibniz Universität Hannover, Callinstraße 38, 30167 Hannover, Germany
| | - C J Killow
- SUPA, Institute for Gravitational Research, School of Physics and Astronomy, University of Glasgow, Glasgow, G12 8QQ, United Kingdom
| | - J A Lobo
- Institut de Ciències de l'Espai (CSIC-IEEC), Campus UAB, Carrer de Can Magrans s/n, 08193 Cerdanyola del Vallès, Spain
| | - I Lloro
- Institut de Ciències de l'Espai (CSIC-IEEC), Campus UAB, Carrer de Can Magrans s/n, 08193 Cerdanyola del Vallès, Spain
| | - L Liu
- Dipartimento di Fisica, Università di Trento and Trento Institute for Fundamental Physics and Applications/INFN, 38123 Povo, Trento, Italy
| | - J P López-Zaragoza
- Institut de Ciències de l'Espai (CSIC-IEEC), Campus UAB, Carrer de Can Magrans s/n, 08193 Cerdanyola del Vallès, Spain
| | - R Maarschalkerweerd
- European Space Operations Centre, European Space Agency, 64293 Darmstadt, Germany
| | - D Mance
- Institut für Geophysik, ETH Zürich, Sonneggstrasse 5, CH-8092, Zürich, Switzerland
| | - V Martín
- Institut de Ciències de l'Espai (CSIC-IEEC), Campus UAB, Carrer de Can Magrans s/n, 08193 Cerdanyola del Vallès, Spain
| | - L Martin-Polo
- European Space Astronomy Centre, European Space Agency, Villanueva de la Cañada, 28692 Madrid, Spain
| | - J Martino
- APC, Université Paris Diderot, CNRS/IN2P3, CEA/lrfu, Obs de Paris, Sorbonne Paris Cité, France
| | - F Martin-Porqueras
- European Space Astronomy Centre, European Space Agency, Villanueva de la Cañada, 28692 Madrid, Spain
| | - S Madden
- European Space Technology Centre, European Space Agency, Keplerlaan 1, 2200 AG Noordwijk, Netherlands
| | - I Mateos
- Institut de Ciències de l'Espai (CSIC-IEEC), Campus UAB, Carrer de Can Magrans s/n, 08193 Cerdanyola del Vallès, Spain
| | - P W McNamara
- European Space Technology Centre, European Space Agency, Keplerlaan 1, 2200 AG Noordwijk, Netherlands
| | - J Mendes
- European Space Operations Centre, European Space Agency, 64293 Darmstadt, Germany
| | - L Mendes
- European Space Astronomy Centre, European Space Agency, Villanueva de la Cañada, 28692 Madrid, Spain
| | - A Monsky
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik und Leibniz Universität Hannover, Callinstraße 38, 30167 Hannover, Germany
| | - D Nicolodi
- Dipartimento di Fisica, Università di Trento and Trento Institute for Fundamental Physics and Applications/INFN, 38123 Povo, Trento, Italy
| | - M Nofrarias
- Institut de Ciències de l'Espai (CSIC-IEEC), Campus UAB, Carrer de Can Magrans s/n, 08193 Cerdanyola del Vallès, Spain
| | - S Paczkowski
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik und Leibniz Universität Hannover, Callinstraße 38, 30167 Hannover, Germany
| | - M Perreur-Lloyd
- SUPA, Institute for Gravitational Research, School of Physics and Astronomy, University of Glasgow, Glasgow, G12 8QQ, United Kingdom
| | - A Petiteau
- APC, Université Paris Diderot, CNRS/IN2P3, CEA/lrfu, Obs de Paris, Sorbonne Paris Cité, France
| | - P Pivato
- Dipartimento di Fisica, Università di Trento and Trento Institute for Fundamental Physics and Applications/INFN, 38123 Povo, Trento, Italy
| | - E Plagnol
- APC, Université Paris Diderot, CNRS/IN2P3, CEA/lrfu, Obs de Paris, Sorbonne Paris Cité, France
| | - P Prat
- APC, Université Paris Diderot, CNRS/IN2P3, CEA/lrfu, Obs de Paris, Sorbonne Paris Cité, France
| | - U Ragnit
- European Space Technology Centre, European Space Agency, Keplerlaan 1, 2200 AG Noordwijk, Netherlands
| | - B Raïs
- APC, Université Paris Diderot, CNRS/IN2P3, CEA/lrfu, Obs de Paris, Sorbonne Paris Cité, France
| | - J Ramos-Castro
- Departament d'Enginyeria Electrònica, Universitat Politècnica de Catalunya, 08034 Barcelona, Spain
| | - J Reiche
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik und Leibniz Universität Hannover, Callinstraße 38, 30167 Hannover, Germany
| | - D I Robertson
- SUPA, Institute for Gravitational Research, School of Physics and Astronomy, University of Glasgow, Glasgow, G12 8QQ, United Kingdom
| | - H Rozemeijer
- European Space Technology Centre, European Space Agency, Keplerlaan 1, 2200 AG Noordwijk, Netherlands
| | - F Rivas
- Institut de Ciències de l'Espai (CSIC-IEEC), Campus UAB, Carrer de Can Magrans s/n, 08193 Cerdanyola del Vallès, Spain
| | - G Russano
- Dipartimento di Fisica, Università di Trento and Trento Institute for Fundamental Physics and Applications/INFN, 38123 Povo, Trento, Italy
| | - J Sanjuán
- Institut de Ciències de l'Espai (CSIC-IEEC), Campus UAB, Carrer de Can Magrans s/n, 08193 Cerdanyola del Vallès, Spain
| | - P Sarra
- CGS S.p.A, Compagnia Generale per lo Spazio, Via Gallarate, 150-20151 Milano, Italy
| | - A Schleicher
- Airbus Defence and Space, Claude-Dornier-Strasse, 88090 Immenstaad, Germany
| | - D Shaul
- High Energy Physics Group, Physics Department, Imperial College London, Blackett Laboratory, Prince Consort Road, London, SW7 2BW, United Kingdom
| | - J Slutsky
- Gravitational Astrophysics Lab, NASA Goddard Space Flight Center, 8800 Greenbelt Road, Greenbelt, Maryland 20771, USA
| | - C F Sopuerta
- Institut de Ciències de l'Espai (CSIC-IEEC), Campus UAB, Carrer de Can Magrans s/n, 08193 Cerdanyola del Vallès, Spain
| | - R Stanga
- Dipartimento di Fisica ed Astronomia, Università degli Studi di Firenze and INFN-Sezione di Firenze, I-50019 Firenze, Italy
| | - F Steier
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik und Leibniz Universität Hannover, Callinstraße 38, 30167 Hannover, Germany
| | - T Sumner
- High Energy Physics Group, Physics Department, Imperial College London, Blackett Laboratory, Prince Consort Road, London, SW7 2BW, United Kingdom
| | - D Texier
- European Space Astronomy Centre, European Space Agency, Villanueva de la Cañada, 28692 Madrid, Spain
| | - J I Thorpe
- Gravitational Astrophysics Lab, NASA Goddard Space Flight Center, 8800 Greenbelt Road, Greenbelt, Maryland 20771, USA
| | - C Trenkel
- Airbus Defence and Space, Gunnels Wood Road, Stevenage, Hertfordshire, SG1 2AS, United Kingdom
| | - M Tröbs
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik und Leibniz Universität Hannover, Callinstraße 38, 30167 Hannover, Germany
| | - H B Tu
- Dipartimento di Fisica, Università di Trento and Trento Institute for Fundamental Physics and Applications/INFN, 38123 Povo, Trento, Italy
| | - D Vetrugno
- Dipartimento di Fisica, Università di Trento and Trento Institute for Fundamental Physics and Applications/INFN, 38123 Povo, Trento, Italy
| | - S Vitale
- Dipartimento di Fisica, Università di Trento and Trento Institute for Fundamental Physics and Applications/INFN, 38123 Povo, Trento, Italy
| | - V Wand
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik und Leibniz Universität Hannover, Callinstraße 38, 30167 Hannover, Germany
| | - G Wanner
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik und Leibniz Universität Hannover, Callinstraße 38, 30167 Hannover, Germany
| | - H Ward
- SUPA, Institute for Gravitational Research, School of Physics and Astronomy, University of Glasgow, Glasgow, G12 8QQ, United Kingdom
| | - C Warren
- Airbus Defence and Space, Gunnels Wood Road, Stevenage, Hertfordshire, SG1 2AS, United Kingdom
| | - P J Wass
- High Energy Physics Group, Physics Department, Imperial College London, Blackett Laboratory, Prince Consort Road, London, SW7 2BW, United Kingdom
| | - D Wealthy
- Airbus Defence and Space, Gunnels Wood Road, Stevenage, Hertfordshire, SG1 2AS, United Kingdom
| | - W J Weber
- Dipartimento di Fisica, Università di Trento and Trento Institute for Fundamental Physics and Applications/INFN, 38123 Povo, Trento, Italy
| | - L Wissel
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik und Leibniz Universität Hannover, Callinstraße 38, 30167 Hannover, Germany
| | - A Wittchen
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik und Leibniz Universität Hannover, Callinstraße 38, 30167 Hannover, Germany
| | - A Zambotti
- Department of Industrial Engineering, University of Trento, via Sommarive 9, 38123 Trento, and Trento Institute for Fundamental Physics and Applications/INFN, Italy
| | - C Zanoni
- Department of Industrial Engineering, University of Trento, via Sommarive 9, 38123 Trento, and Trento Institute for Fundamental Physics and Applications/INFN, Italy
| | - T Ziegler
- Airbus Defence and Space, Claude-Dornier-Strasse, 88090 Immenstaad, Germany
| | - P Zweifel
- Institut für Geophysik, ETH Zürich, Sonneggstrasse 5, CH-8092, Zürich, Switzerland
| |
Collapse
|
15
|
Winemiller KO, McIntyre PB, Castello L, Fluet-Chouinard E, Giarrizzo T, Nam S, Baird IG, Darwall W, Lujan NK, Harrison I, Stiassny MLJ, Silvano RAM, Fitzgerald DB, Pelicice FM, Agostinho AA, Gomes LC, Albert JS, Baran E, Petrere M, Zarfl C, Mulligan M, Sullivan JP, Arantes CC, Sousa LM, Koning AA, Hoeinghaus DJ, Sabaj M, Lundberg JG, Armbruster J, Thieme ML, Petry P, Zuanon J, Torrente Vilara G, Snoeks J, Ou C, Rainboth W, Pavanelli CS, Akama A, van Soesbergen A, Sáenz L. Balancing hydropower and biodiversity in the Amazon, Congo, and Mekong. Science 2016; 351:128-9. [PMID: 26744397 DOI: 10.1126/science.aac7082] [Citation(s) in RCA: 346] [Impact Index Per Article: 43.3] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [MESH Headings] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/02/2022]
Affiliation(s)
| | - P B McIntyre
- See supplementary materials for author affiliations
| | - L Castello
- See supplementary materials for author affiliations
| | | | - T Giarrizzo
- See supplementary materials for author affiliations
| | - S Nam
- See supplementary materials for author affiliations
| | - I G Baird
- See supplementary materials for author affiliations
| | - W Darwall
- See supplementary materials for author affiliations
| | - N K Lujan
- See supplementary materials for author affiliations
| | - I Harrison
- See supplementary materials for author affiliations
| | | | | | | | - F M Pelicice
- See supplementary materials for author affiliations
| | | | - L C Gomes
- See supplementary materials for author affiliations
| | - J S Albert
- See supplementary materials for author affiliations
| | - E Baran
- See supplementary materials for author affiliations
| | - M Petrere
- See supplementary materials for author affiliations
| | - C Zarfl
- See supplementary materials for author affiliations
| | - M Mulligan
- See supplementary materials for author affiliations
| | - J P Sullivan
- See supplementary materials for author affiliations
| | - C C Arantes
- See supplementary materials for author affiliations
| | - L M Sousa
- See supplementary materials for author affiliations
| | - A A Koning
- See supplementary materials for author affiliations
| | | | - M Sabaj
- See supplementary materials for author affiliations
| | - J G Lundberg
- See supplementary materials for author affiliations
| | - J Armbruster
- See supplementary materials for author affiliations
| | - M L Thieme
- See supplementary materials for author affiliations
| | - P Petry
- See supplementary materials for author affiliations
| | - J Zuanon
- See supplementary materials for author affiliations
| | | | - J Snoeks
- See supplementary materials for author affiliations
| | - C Ou
- See supplementary materials for author affiliations
| | - W Rainboth
- See supplementary materials for author affiliations
| | | | - A Akama
- See supplementary materials for author affiliations
| | | | - L Sáenz
- See supplementary materials for author affiliations
| |
Collapse
|
16
|
Nurzulaikha R, Lim H, Harrison I, Lim S, Pandikumar A, Huang N, Lim S, Thien G, Yusoff N, Ibrahim I. Graphene/SnO 2 nanocomposite-modified electrode for electrochemical detection of dopamine. Sensing and Bio-Sensing Research 2015. [DOI: 10.1016/j.sbsr.2015.06.002] [Citation(s) in RCA: 60] [Impact Index Per Article: 6.7] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Submit a Manuscript] [Subscribe] [Scholar Register] [Indexed: 01/24/2023] Open
|
17
|
Chee W, Lim H, Harrison I, Chong K, Zainal Z, Ng C, Huang N. Performance of Flexible and Binderless Polypyrrole/Graphene Oxide/Zinc Oxide Supercapacitor Electrode in a Symmetrical Two-Electrode Configuration. Electrochim Acta 2015. [DOI: 10.1016/j.electacta.2015.01.080] [Citation(s) in RCA: 140] [Impact Index Per Article: 15.6] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 10/24/2022]
|
18
|
Abstract
Graphene-based nanofillers and their applications. Fabrication methods of graphene-based nanocomposites. Interaction and dispersion of graphene-based fillers in polymer matrices. Current trends and prospects of graphene-based nanocomposites.
Collapse
Affiliation(s)
- W. K. Chee
- Department of Chemistry
- Faculty of Science
- Universiti Putra Malaysia
- Malaysia
| | - H. N. Lim
- Department of Chemistry
- Faculty of Science
- Universiti Putra Malaysia
- Malaysia
- Functional Device Laboratory
| | - N. M. Huang
- Low Dimension Materials Research Centre
- Department of Physics
- Faculty of Science
- University of Malaya
- Kuala Lumpur 50603
| | - I. Harrison
- Faculty of Engineering
- The University of Nottingham Malaysia Campus
- Malaysia
| |
Collapse
|
19
|
Donald SB, Navin JK, Harrison I. Methane dissociative chemisorption and detailed balance on Pt(111): dynamical constraints and the modest influence of tunneling. J Chem Phys 2014; 139:214707. [PMID: 24320394 DOI: 10.1063/1.4837697] [Citation(s) in RCA: 12] [Impact Index Per Article: 1.2] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/14/2022] Open
Abstract
A dynamically biased (d-) precursor mediated microcanonical trapping (PMMT) model of the activated dissociative chemisorption of methane on Pt(111) is applied to a wide range of dissociative sticking experiments, and, by detailed balance, to the methane product state distributions from the thermal associative desorption of adsorbed hydrogen with coadsorbed methyl radicals. Tunneling pathways were incorporated into the d-PMMT model to better replicate the translational energy distribution of the desorbing methane product from the laser induced thermal reaction of coadsorbed hydrogen and methyl radicals occurring near T(s) = 395 K. Although tunneling is predicted to be inconsequential to the thermal dissociative chemisorption of CH4 on Pt(111) at the high temperatures of catalytic interest, once the temperature drops to 395 K the tunneling fraction of the reactive thermal flux reaches 15%, and as temperatures drop below 275 K the tunneling fraction exceeds 50%. The d-PMMT model parameters of {E0 = 58.9 kJ/mol, s = 2, η(v) = 0.40} describe the apparent threshold energy for CH4/Pt(111) dissociative chemisorption, the number of surface oscillators involved in the precursor complex, and the efficacy of molecular vibrational energy to promote reaction, relative to translational energy directed along the surface normal. Molecular translations parallel to the surface and rotations are treated as spectator degrees of freedom. Transition state vibrational frequencies are derived from generalized gradient approximation-density functional theory electronic structure calculations. The d-PMMT model replicates the diverse range of experimental data available with good fidelity, including some new effusive molecular beam and ambient gas dissociative sticking measurements. Nevertheless, there are some indications that closer agreement between theory and experiments could be achieved if a surface efficacy less than one was introduced into the modeling as an additional dynamical constraint.
Collapse
Affiliation(s)
- S B Donald
- Department of Chemistry, University of Virginia, Charlottesville, Virginia 22904-4319, USA
| | | | | |
Collapse
|
20
|
Huddy VC, Clark L, Harrison I, Ron MA, Moutoussis M, Barnes TRE, Joyce EM. Multifaceted impairments of impulsivity in cannabis users? A reply. Psychol Med 2013; 43:2238-2239. [PMID: 24137768 DOI: 10.1017/s0033291713001645] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [MESH Headings] [Track Full Text] [Journal Information] [Submit a Manuscript] [Subscribe] [Scholar Register] [Indexed: 11/06/2022]
|
21
|
Huddy VC, Clark L, Harrison I, Ron MA, Moutoussis M, Barnes TRE, Joyce EM. Reflection impulsivity and response inhibition in first-episode psychosis: relationship to cannabis use. Psychol Med 2013; 43:2097-2107. [PMID: 23339857 DOI: 10.1017/s0033291712003054] [Citation(s) in RCA: 15] [Impact Index Per Article: 1.4] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Grants] [Track Full Text] [Journal Information] [Submit a Manuscript] [Subscribe] [Scholar Register] [Indexed: 11/06/2022]
Abstract
BACKGROUND People with psychosis demonstrate impaired response inhibition on the Stop Signal Task (SST). It is less clear if this impairment extends to reflection impulsivity, a form of impulsivity that has been linked to substance use in non-psychotic samples. METHOD We compared 49 patients with first-episode psychosis (FEP) and 30 healthy control participants on two forms of impulsivity measured using the Information Sampling Test (IST) and the SST, along with clinical and IQ assessments. We also compared those patients who used cannabis with those who had either given up or never used. RESULTS Patients with FEP had significantly greater impairment in response inhibition but not in reflection impulsivity compared with healthy controls. By contrast, patients who reported current cannabis use demonstrated greater reflection impulsivity than those that had either given up or never used, whereas there were no differences in response inhibition. CONCLUSIONS These data suggest that abnormal reflection impulsivity is associated with substance use in psychosis but not psychosis itself ; the opposite relationship may hold for response inhibition.
Collapse
Affiliation(s)
- V C Huddy
- Department of Psychosis Studies, Institute of Psychiatry, King's College London, UK
| | | | | | | | | | | | | |
Collapse
|
22
|
Navin JK, Donald SB, Tinney DG, Cushing GW, Harrison I. Communication: Angle-resolved thermal dissociative sticking of CH4 on Pt(111): Further indication that rotation is a spectator to the gas-surface reaction dynamics. J Chem Phys 2012; 136:061101. [DOI: 10.1063/1.3685833] [Citation(s) in RCA: 10] [Impact Index Per Article: 0.8] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/15/2022] Open
Affiliation(s)
- J. K. Navin
- Department of Chemistry, University of Virginia, Charlottesville, Virginia 22904-4319, USA
| | - S. B. Donald
- Department of Chemistry, University of Virginia, Charlottesville, Virginia 22904-4319, USA
| | - D. G. Tinney
- Department of Chemistry, University of Virginia, Charlottesville, Virginia 22904-4319, USA
| | - G. W. Cushing
- Department of Chemistry, University of Virginia, Charlottesville, Virginia 22904-4319, USA
| | - I. Harrison
- Department of Chemistry, University of Virginia, Charlottesville, Virginia 22904-4319, USA
| |
Collapse
|
23
|
Lim HN, Huang NM, Lim SS, Harrison I, Chia CH. Fabrication and characterization of graphene hydrogel via hydrothermal approach as a scaffold for preliminary study of cell growth. Int J Nanomedicine 2011; 6:1817-23. [PMID: 21931479 PMCID: PMC3173046 DOI: 10.2147/ijn.s23392] [Citation(s) in RCA: 149] [Impact Index Per Article: 11.5] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [MESH Headings] [Track Full Text] [Download PDF] [Figures] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 12/23/2022] Open
Abstract
BACKGROUND Three-dimensional assembly of graphene hydrogel is rapidly attracting the interest of researchers because of its wide range of applications in energy storage, electronics, electrochemistry, and waste water treatment. Information on the use of graphene hydrogel for biological purposes is lacking, so we conducted a preliminary study to determine the suitability of graphene hydrogel as a substrate for cell growth, which could potentially be used as building blocks for biomolecules and tissue engineering applications. METHODS A three-dimensional structure of graphene hydrogel was prepared via a simple hydrothermal method using two-dimensional large-area graphene oxide nanosheets as a precursor. RESULTS The concentration and lateral size of the graphene oxide nanosheets influenced the structure of the hydrogel. With larger-area graphene oxide nanosheets, the graphene hydrogel could be formed at a lower concentration. X-ray diffraction patterns revealed that the oxide functional groups on the graphene oxide nanosheets were reduced after hydrothermal treatment. The three-dimensional graphene hydrogel matrix was used as a scaffold for proliferation of a MG63 cell line. CONCLUSION Guided filopodia protrusions of MG63 on the hydrogel were observed on the third day of cell culture, demonstrating compatibility of the graphene hydrogel structure for bioapplications.
Collapse
Affiliation(s)
- HN Lim
- Centre for Ionics University of Malaya, Physics Department, Faculty of Science, University of Malaya, Kuala Lumpur
| | - NM Huang
- Low Dimensional Materials Research Centre, Physics Department, Faculty of Science, University of Malaya, Kuala Lumpur
| | - SS Lim
- School of Chemical and Environmental Engineering, Faculty of Engineering, The University of Nottingham Malaysia Campus, Jalan Broga, Semenyih, Selangor
| | - I Harrison
- School of Chemical and Environmental Engineering, Faculty of Engineering, The University of Nottingham Malaysia Campus, Jalan Broga, Semenyih, Selangor
| | - CH Chia
- School of Applied Physics, Faculty of Science and Technology, Universiti Kebangsaan Malaysia, Selangor, Malaysia
| |
Collapse
|
24
|
Cushing GW, Navin JK, Valadez L, Johánek V, Harrison I. An effusive molecular beam technique for studies of polyatomic gas-surface reactivity and energy transfer. Rev Sci Instrum 2011; 82:044102. [PMID: 21529024 DOI: 10.1063/1.3577076] [Citation(s) in RCA: 2] [Impact Index Per Article: 0.2] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 05/30/2023]
Abstract
An effusive molecular beam technique is described to measure alkane dissociative sticking coefficients, S(T(g), T(s); ϑ), on metal surfaces for which the impinging gas temperature, T(g), and surface temperature, T(s), can be independently varied, along with the angle of incidence, ϑ, of the impinging gas. Effusive beam experiments with T(g) = T(s) = T allow for determination of angle-resolved dissociative sticking coefficients, S(T; ϑ), which when averaged over the cos (ϑ)/π angular distribution appropriate to the impinging flux from a thermal ambient gas yield the thermal dissociative sticking coefficient, S(T). Nonequilibrium S(T(g), T(s); ϑ) measurements for which T(g) ≠ T(s) provide additional opportunities to characterize the transition state and gas-surface energy transfer at reactive energies. A resistively heated effusive molecular beam doser controls the T(g) of the impinging gas striking the surface. The flux of molecules striking the surface from the effusive beam is determined from knowledge of the dosing geometry, chamber pressure, and pumping speed. Separate experiments with a calibrated leak serve to fix the chamber pumping speed. Postdosing Auger electron spectroscopy is used to measure the carbon of the alkyl radical reaction product that is deposited on the surface as a result of alkane dissociative sticking. As implemented in a typical ultrahigh vacuum chamber for surface analysis, the technique has provided access to a dynamic range of roughly 6 orders of magnitude in the initial dissociative sticking coefficient for small alkanes on Pt(111).
Collapse
Affiliation(s)
- G W Cushing
- Department of Chemistry, University of Virginia, Charlottesville, Virginia 22904-4319, USA
| | | | | | | | | |
Collapse
|
25
|
Vane CH, Chenery SR, Harrison I, Kim AW, Moss-Hayes V, Jones DG. Chemical signatures of the Anthropocene in the Clyde estuary, UK: sediment-hosted Pb, (207/206)Pb, total petroleum hydrocarbon, polyaromatic hydrocarbon and polychlorinated biphenyl pollution records. Philos Trans A Math Phys Eng Sci 2011; 369:1085-111. [PMID: 21282161 DOI: 10.1098/rsta.2010.0298] [Citation(s) in RCA: 31] [Impact Index Per Article: 2.4] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 05/25/2023]
Abstract
The sediment concentrations of total petroleum hydrocarbons (TPHs), polyaromatic hydrocarbons (PAHs), polychlorinated biphenyls (PCBs), Pb and (207/206)Pb isotope ratios were measured in seven cores from the middle Clyde estuary (Scotland, UK) with an aim of tracking the late Anthropocene. Concentrations of TPHs ranged from 34 to 4386 mg kg(-1), total PAHs from 19 to 16,163 μg kg(-1) and total PCBs between less than 4.3 to 1217 μg kg(-1). Inventories, distributions and isomeric ratios of the organic pollutants were used to reconstruct pollutant histories. Pre-Industrial Revolution and modern non-polluted sediments were characterized by low TPH and PAH values as well as high relative abundance of biogenic-sourced phenanthrene and naphthalene. The increasing industrialization of the Clyde gave rise to elevated PAH concentrations and PAH isomeric ratios characteristic of both grass/wood/coal and petroleum and combustion (specifically petroleum combustion). Overall, PAHs had the longest history of any of the organic contaminants. Increasing TPH concentrations and a concomitant decline in PAHs mirrored the lessening of coal use and increasing reliance on petroleum fuels from about the 1950s. Thereafter, declining hydrocarbon pollution was followed by the onset (1950s), peak (1965-1977) and decline (post-1980s) in total PCB concentrations. Lead concentrations ranged from 6 to 631 mg kg(-1), while (207/206)Pb isotope ratios spanned 0.838-0.876, indicative of various proportions of 'background', British ore/coal and Broken Hill type petrol/industrial lead. A chronology was established using published Pb isotope data for aerosol-derived Pb and applied to the cores.
Collapse
Affiliation(s)
- C H Vane
- British Geological Survey, Kingsley Dunham Centre, Keyworth, Nottingham NG12 5GG, UK.
| | | | | | | | | | | |
Collapse
|
26
|
Abstract
The ability of two differing marine sediments (one clayey, the other sandy) to attenuate the explosive 2,4,6-trinitrotoluene (TNT), dissolved in intertidal seawater from the eastern English coast of the North Sea, was examined using aerobic microcosms. Analysis of the seawater from the microcosms revealed an initial sharp decline in TNT concentration with clayey sediment in both sterilized (to prevent microbial activity) and unsterilized microcosms. This effect did not occur to such a marked extent in similar sterile and non-sterile sandy sediment microcosms and was attributed mainly to sorption of TNT to the fine clay particles of the clayey sediment. As time progressed, the attenuation of TNT in microcosms containing either type of sediment was found to be less in those that had been sterilized compared with those where microbial action proceeded unhindered. Feeding the microcosms, (i.e. supplying extra carbon sources for the microbial communities), appeared to have a small, but perceptible, enhancing effect upon TNT dissipation. The attenuation of TNT was also measured in large microcosms containing 2.5 L of seawater and no sediment. Analysis of the seawater revealed a gradual decline in TNT concentration in non-sterile and fed microcosms compared to their sterile counterpart. Overall, this laboratory study showed that the attenuation of TNT is slow (half-life in seawater ca.1900 days; half-life sand sediment <700 days; half life in clay sediment 130 days) under conditions commonly encountered in coastal waters of the North Sea.
Collapse
Affiliation(s)
- I Harrison
- Kingsley Dunham Centre, Keyworth, Nottingham, UK
| | | |
Collapse
|
27
|
Leeson VC, Robbins TW, Franklin C, Harrison M, Harrison I, Ron MA, Barnes TRE, Joyce EM. Dissociation of long-term verbal memory and fronto-executive impairment in first-episode psychosis. Psychol Med 2009; 39:1799-1808. [PMID: 19419594 PMCID: PMC2758301 DOI: 10.1017/s0033291709005935] [Citation(s) in RCA: 25] [Impact Index Per Article: 1.7] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [MESH Headings] [Grants] [Track Full Text] [Download PDF] [Figures] [Journal Information] [Submit a Manuscript] [Subscribe] [Scholar Register] [Received: 11/07/2008] [Revised: 03/03/2009] [Accepted: 03/18/2009] [Indexed: 11/10/2022]
Abstract
BACKGROUND Verbal memory is frequently and severely affected in schizophrenia and has been implicated as a mediator of poor clinical outcome. Whereas encoding deficits are well demonstrated, it is unclear whether retention is impaired. This distinction is important because accelerated forgetting implies impaired consolidation attributable to medial temporal lobe (MTL) dysfunction whereas impaired encoding and retrieval implicates involvement of prefrontal cortex. METHOD We assessed a group of healthy volunteers (n=97) and pre-morbid IQ- and sex-matched first-episode psychosis patients (n=97), the majority of whom developed schizophrenia. We compared performance of verbal learning and recall with measures of visuospatial working memory, planning and attentional set-shifting, and also current IQ. RESULTS All measures of performance, including verbal memory retention, a memory savings score that accounted for learning impairments, were significantly impaired in the schizophrenia group. The difference between groups for delayed recall remained even after the influence of learning and recall was accounted for. Factor analyses showed that, in patients, all variables except verbal memory retention loaded on a single factor, whereas in controls verbal memory and fronto-executive measures were separable. CONCLUSIONS The results suggest that IQ, executive function and verbal learning deficits in schizophrenia may reflect a common abnormality of information processing in prefrontal cortex rather than specific impairments in different cognitive domains. Verbal memory retention impairments, however, may have a different aetiology.
Collapse
Affiliation(s)
- V C Leeson
- Institute of Neurology, University College London, UK.
| | | | | | | | | | | | | | | |
Collapse
|
28
|
Vane CH, Harrison I, Kim AW, Moss-Hayes V, Vickers BP, Hong K. Organic and metal contamination in surface mangrove sediments of South China. Mar Pollut Bull 2009; 58:134-144. [PMID: 18990413 DOI: 10.1016/j.marpolbul.2008.09.024] [Citation(s) in RCA: 25] [Impact Index Per Article: 1.7] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [MESH Headings] [Track Full Text] [Subscribe] [Scholar Register] [Received: 07/08/2008] [Revised: 09/22/2008] [Accepted: 09/24/2008] [Indexed: 05/27/2023]
Affiliation(s)
- C H Vane
- British Geological Survey, Kingsley Dunham Centre, Keyworth, Nottingham, UK.
| | | | | | | | | | | |
Collapse
|
29
|
Vane CH, Harrison I, Kim AW, Moss-Hayes V, Vickers BP, Horton BP. Status of organic pollutants in surface sediments of Barnegat Bay-Little Egg Harbor Estuary, New Jersey, USA. Mar Pollut Bull 2008; 56:1802-1808. [PMID: 18715597 DOI: 10.1016/j.marpolbul.2008.07.004] [Citation(s) in RCA: 7] [Impact Index Per Article: 0.4] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [MESH Headings] [Track Full Text] [Subscribe] [Scholar Register] [Received: 06/03/2008] [Revised: 07/03/2008] [Accepted: 07/08/2008] [Indexed: 05/26/2023]
Affiliation(s)
- C H Vane
- British Geological Survey, Kingsley Dunham Centre, Keyworth, Nottingham, NG12 5GG, United Kingdom.
| | | | | | | | | | | |
Collapse
|
30
|
Harrison I, Joyce E, Mutsatsa S, Hutton S, Huddy V, Kapasi M, Barnes T. Naturalistic follow-up of co-morbid substance use in schizophrenia: the West London first-episode study. Psychol Med 2008; 38:79-88. [PMID: 17532864 PMCID: PMC2577143 DOI: 10.1017/s0033291707000797] [Citation(s) in RCA: 62] [Impact Index Per Article: 3.9] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [MESH Headings] [Grants] [Track Full Text] [Download PDF] [Figures] [Journal Information] [Submit a Manuscript] [Subscribe] [Scholar Register] [Received: 04/21/2006] [Revised: 04/05/2007] [Accepted: 04/12/2007] [Indexed: 11/06/2022]
Abstract
BACKGROUND The impact of co-morbid substance use in first-episode schizophrenia has not been fully explored. METHOD This naturalistic follow-up of a cohort of 152 people with first-episode schizophrenia examined substance use and clinical outcome in terms of symptoms and social and neuropsychological function. RESULTS Data were collected on 85 (56%) of the patient cohort after a median period of 14 months. Over the follow-up period, the proportion of smokers rose from 60% at baseline to 64%. While 30% reported lifetime problem drinking of alcohol at baseline, only 15% had problem drinking at follow-up. Furthermore, while at baseline 63% reported lifetime cannabis use and 32% were currently using the drug, by the follow-up assessment the latter figure had fallen to 18.5%. At follow-up, persistent substance users had significantly more severe positive and depressive symptoms and greater overall severity of illness. A report of no lifetime substance use at baseline was associated with greater improvement in spatial working memory (SWM) at follow-up. CONCLUSIONS Past substance use may impede recovery of SWM performance in people with schizophrenia in the year or so following first presentation to psychiatric services. The prevalence of substance use other than tobacco tends to diminish over this period, in the absence of specific interventions. Persistent substance use in first-episode schizophrenia is associated with more severe positive and depressive symptoms but not negative symptoms, and should be a target for specific treatment intervention.
Collapse
Affiliation(s)
- I. Harrison
- Department of Psychological Medicine, Imperial College
Faculty of Medicine, London, UK
| | - E. M. Joyce
- Institute of Neurology, University College London,
London, UK
| | - S. H. Mutsatsa
- Department of Psychological Medicine, Imperial College
Faculty of Medicine, London, UK
| | - S. B. Hutton
- Department of Psychology, University of Sussex,
Brighton, UK
| | - V. Huddy
- Department of Psychological Medicine, Imperial College
Faculty of Medicine, London, UK
| | - M. Kapasi
- Department of Psychological Medicine, Imperial College
Faculty of Medicine, London, UK
| | - T. R. E. Barnes
- Department of Psychological Medicine, Imperial College
Faculty of Medicine, London, UK
| |
Collapse
|
31
|
Connell PP, Saddak T, Harrison I, Kelly S, Bobart A, McGettrick P, Collum LTM. Construction-related eye injuries in Irish nationals and non-nationals: attitudes and strategies for prevention. Ir J Med Sci 2007; 176:11-4. [PMID: 17849517 DOI: 10.1007/s11845-007-0002-5] [Citation(s) in RCA: 6] [Impact Index Per Article: 0.4] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/25/2022]
Abstract
BACKGROUND Construction-related ocular injuries are an important cause of vision loss but few studies on the incidence, epidemiology and nature of these injuries exist. AIMS Due to the perceived increase in occupation-related eye injuries in non-nationals we aimed to investigate the nature of such injuries presenting to a single eye unit over a two-month period. METHODS One hundred and fifty-five patients presenting to the accident and emergency department with construction related ocular injury were examined. RESULTS Of 155 patients, 80 were Irish and 75 nonnational, of whom 60, 21.3 and 6.7% were Polish, Lithuanian and Romanian, respectively. Common causative factors included hammering, grinding, drilling and splash injury. Average rate of eyewear protection usage was 35%, with attendance at safety courses highest in Irish nationals. A penetrating eye injury rate of 4.9% overall was observed, all in non-nationals. CONCLUSION Construction related ocular injury is a serious cause of visual loss in non-nationals. Greater adherence to safety regulations and training is required.
Collapse
Affiliation(s)
- P P Connell
- Royal Victoria Eye and Ear Hospital, Adelaide Road, Dublin 2, Ireland.
| | | | | | | | | | | | | |
Collapse
|
32
|
Gooddy DC, Mathias SA, Harrison I, Lapworth DJ, Kim AW. The significance of colloids in the transport of pesticides through Chalk. Sci Total Environ 2007; 385:262-71. [PMID: 17673277 DOI: 10.1016/j.scitotenv.2007.06.043] [Citation(s) in RCA: 9] [Impact Index Per Article: 0.5] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Track Full Text] [Subscribe] [Scholar Register] [Received: 02/14/2007] [Revised: 06/19/2007] [Accepted: 06/21/2007] [Indexed: 05/16/2023]
Abstract
Agrochemical contamination in groundwater poses a significant long term threat to water quality and is of concern for legislators, water utilities and consumers alike. In the dual porosity, dual permeability aquifers such as the Chalk aquifer, movement of pesticides and their metabolites through the unsaturated zone to groundwater is generally considered to be through one of two pathways; a rapid by-pass flow and a slower 'piston-flow' route via the rock matrix. However, the dissolved form or 'colloidal species' in which pesticides move within the water body is poorly understood. Following heavy rainfall, very high peaks in pesticide concentration have been observed in shallow Chalk aquifers. These concentrations might be well explained by colloidal transport of pesticides. We have sampled a Chalk groundwater beneath a deep (30 m) unsaturated zone known to be contaminated with the pesticide diuron. Using a tangential flow filtration technique we have produced colloidal fractions from 0.45 microm to 1 kDa. In addition, we have applied agricultural grade diuron to a typical Chalk soil and created a soil water suspension which was also subsequently fractionated using the same filtration system. The deep groundwater sample showed no evidence of association between colloidal material and pesticide concentration. In comparison, despite some evidence of particle trapping or sorption to the filters, the soil water clearly showed an association between the <0.45 microm and <0.1 microm colloidal fractions which displayed significantly higher pesticide concentrations than the unfiltered sample. Degradation products were also observed and found to behave in a similar manner to the parent compound. Although relatively large colloids can be generated in the Chalk soil zone, it appears transport to depth in a colloidal-bound form does not occur. Comparison with other field and monitoring studies suggests that rapid by-pass flow is unlikely to occur beneath 4-5 m. Therefore, shallow groundwaters are most at risk from rapid transport of high concentrations of pesticide-colloidal complexes. The presence of a deep unsaturated zone will mean that most of the colloidal-complexes will be filtered by the narrow Chalk pores and the majority of pesticide transport will occur in a 'dissolved' form through the more gradual 'piston-flow' route.
Collapse
Affiliation(s)
- D C Gooddy
- British Geological Survey, Wallingford, Oxfordshire, OX10 8BB, UK.
| | | | | | | | | |
Collapse
|
33
|
Vane CH, Harrison I, Kim AW. Assessment of polyaromatic hydrocarbons (PAHs) and polychlorinated biphenyls (PCBs) in surface sediments of the Inner Clyde Estuary, UK. Mar Pollut Bull 2007; 54:1301-6. [PMID: 17553529 DOI: 10.1016/j.marpolbul.2007.04.005] [Citation(s) in RCA: 1] [Impact Index Per Article: 0.1] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [MESH Headings] [Track Full Text] [Subscribe] [Scholar Register] [Received: 03/15/2007] [Revised: 04/17/2007] [Accepted: 04/19/2007] [Indexed: 05/15/2023]
Affiliation(s)
- C H Vane
- British Geological Survey, Kingsley Dunham Centre, Keyworth, Nottingham, NG12 5GG, United Kingdom.
| | | | | |
Collapse
|
34
|
Vane CH, Harrison I, Kim AW. Polycyclic aromatic hydrocarbons (PAHs) and polychlorinated biphenyls (PCBs) in sediments from the Mersey Estuary, U.K. Sci Total Environ 2007; 374:112-26. [PMID: 17258286 DOI: 10.1016/j.scitotenv.2006.12.036] [Citation(s) in RCA: 20] [Impact Index Per Article: 1.2] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Track Full Text] [Subscribe] [Scholar Register] [Received: 10/30/2006] [Revised: 12/04/2006] [Accepted: 12/12/2006] [Indexed: 05/07/2023]
Abstract
Sediments from the Mersey Estuary were analysed for polycylic aromatic hydrocarbons (PAHs) and polychlorinated biphenyls (PCBs). Total PAH concentrations ranged from 626 to 3766 microg/kg and total PCB concentrations ranged from 36 to 1409 microg/kg. These concentrations are intermediate in comparison to other U.K estuaries with similar histories of industrialisation and urbanisation. The distribution of individual PAHs were consistent throughout the Mersey Estuary, this together with molecular indices suggests mainly pyrolitic inputs, augmented by a variety of industrial petrogenic sources. Comparison of tri-to-hepta PCB congeners revealed multiple sources and inputs throughout the estuary. A sediment core collected in close proximity to Garston Docks revealed the take-off, peak pollutant input and recent decline of PCB pollution. However, a second depth profile of sediments at Ellesmere Port showed little change in total or individual PCB concentrations due to extensive sediment reworking and mixing.
Collapse
Affiliation(s)
- C H Vane
- British Geological Survey, Kingsley Dunham Centre, Keyworth, Nottingham, NG12 5GG, United Kingdom.
| | | | | |
Collapse
|
35
|
Abbott HL, Harrison I. Seven-dimensional microcanonical treatment of hydrogen dissociation dynamics on Cu(111): Clarifying the essential role of surface phonons. J Chem Phys 2006; 125:24704. [PMID: 16848601 DOI: 10.1063/1.2208362] [Citation(s) in RCA: 7] [Impact Index Per Article: 0.4] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/14/2022] Open
Abstract
A simple picture of the hydrogen dissociation/associative desorption dynamics on Cu(111) emerges from a two-parameter, full dimensionality microcanonical unimolecular rate theory (MURT) model of the gas-surface reactivity. Vibrational frequencies for the reactive transition state were taken from density functional theory calculations of a six-dimensional potential energy surface [Hammer et al., Phys. Rev. Lett. 73, 1400 (1994)]. The two remaining parameters required by the MURT were fixed by simulation of experiments. These parameters are the dissociation threshold energy, E(0)=79 kJmol, and the number of surface oscillators involved in the localized H(2)Cu(111) collision complex, s=1. The two-parameter MURT quantitatively predicts much of the varied behavior observed for the H(2) and D(2)Cu(111) reactive systems, including the temperature-dependent associative desorption angular distributions, mean translational energies of the associatively desorbing hydrogen as a function of rovibrational eigenstate, etc. The divergence of the statistical theory's predictions from experimental results at low rotational quantum numbers, J < or approximately 5, suggests that either (i) rotational steering is important to the dissociation dynamics at low J, an effect that washes out at high J, or (ii) molecular rotation is approximately a spectator degree of freedom to the dissociation dynamics for these low J states, the states that dominate the thermal reactivity. Surface vibrations are predicted to provide approximately 30% of the energy required to surmount the activation barrier to H(2) dissociation under thermal equilibrium conditions. The MURT with s=1 is used to analytically confirm the experimental finding that partial differential "E(a)(T(s))" partial differential E(t)= -1 for eigenstate-resolved dissociative sticking at translational energies E(t)<E(0)-E(v)-E(r). Explicit treatment of the surface motion (i.e., surface not frozen at T(s)=0 K) is a relatively novel aspect of the MURT theoretical approach.
Collapse
Affiliation(s)
- H L Abbott
- Department of Chemistry, University of Virginia, Charlottesville, VA 22904-4319, USA
| | | |
Collapse
|
36
|
Bigelow N, Harrison I, Goodell H, Wolff HG. STUDIES ON PAIN: QUANTITATIVE MEASUREMENTS OF TWO PAIN SENSATIONS OF THE SKIN, WITH REFERENCE TO THE NATURE OF THE "HYPERALGESIA OF PERIPHERAL NEURITIS". J Clin Invest 2006; 24:503-12. [PMID: 16695239 PMCID: PMC435481 DOI: 10.1172/jci101629] [Citation(s) in RCA: 34] [Impact Index Per Article: 1.9] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/17/2022] Open
|
37
|
Bukoski A, Abbott HL, Harrison I. Microcanonical unimolecular rate theory at surfaces. III. Thermal dissociative chemisorption of methane on Pt(111) and detailed balance. J Chem Phys 2005; 123:94707. [PMID: 16164362 DOI: 10.1063/1.2006679] [Citation(s) in RCA: 24] [Impact Index Per Article: 1.3] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/14/2022] Open
Abstract
A local hot spot model of gas-surface reactivity is used to investigate the state-resolved dynamics of methane dissociative chemisorption on Pt(111) under thermal equilibrium conditions. Three Pt surface oscillators, and the molecular vibrations, rotations, and the translational energy directed along the surface normal are treated as active degrees of freedom in the 16-dimensional microcanonical kinetics. Several energy transfer models for coupling a local hot spot to the surrounding substrate are developed and evaluated within the context of a master equation kinetics approach. Bounds on the thermal dissociative sticking coefficient based on limiting energy transfer models are derived. The three-parameter physisorbed complex microcanonical unimolecular rate theory (PC-MURT) is shown to closely approximate the thermal sticking under any realistic energy transfer model. Assuming an apparent threshold energy for CH(4) dissociative chemisorption of E(0)=0.61 eV on clean Pt(111), the PC-MURT is used to predict angle-resolved yield, translational, vibrational, and rotational distributions for the reactive methane flux at thermal equilibrium at 500 K. By detailed balance, these same distributions should be observed for the methane product from methyl radical hydrogenation at 500 K in the zero coverage limit if the methyl radicals are not subject to side reactions. Given that methyl radical hydrogenation can only be experimentally observed when the CH(3) radicals are kinetically stabilized against decomposition by coadsorbed H, the PC-MURT was used to evaluate E(0) in the high coverage limit. A high coverage value of E(0)=2.3 eV adequately reproduced the experimentally observed methane angular and translational energy distributions from thermal hydrogenation of methyl radicals. Although rigorous application of detailed balance arguments to this reactive system cannot be made because thermal decomposition of the methyl radicals competes with hydrogenation, approximate applicability of detailed balance would argue for a strong coverage dependence of E(0) with H coverage--a dependence not seen for methyl radical hydrogenation on Ru(0001), but not yet experimentally explored on Pt(111).
Collapse
Affiliation(s)
- A Bukoski
- Department of Chemistry, University of Virginia, Charlottesville, Virginia 22904-4319, USA
| | | | | |
Collapse
|
38
|
Abbott HL, Bukoski A, Harrison I. Microcanonical unimolecular rate theory at surfaces. II. Vibrational state resolved dissociative chemisorption of methane on Ni(100). J Chem Phys 2004; 121:3792-810. [PMID: 15303948 DOI: 10.1063/1.1777221] [Citation(s) in RCA: 47] [Impact Index Per Article: 2.4] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/14/2022] Open
Abstract
A three-parameter microcanonical theory of gas-surface reactivity is used to investigate the dissociative chemisorption of methane impinging on a Ni(100) surface. Assuming an apparent threshold energy for dissociative chemisorption of E(0)=65 kJ/mol, contributions to the dissociative sticking coefficient from individual methane vibrational states are calculated: (i) as a function of molecular translational energy to model nonequilibrium molecular beam experiments and (ii) as a function of temperature to model thermal equilibrium mbar pressure bulb experiments. Under fairly typical molecular beam conditions (e.g., E(t)>/=25 kJ mol(-1), T(s)>/=475 K, T(n)</=400 K), sticking from methane in the ground vibrational state dominates the overall sticking. In contrast, under thermal equilibrium conditions at temperatures T>/=100 K the dissociative sticking is dominated by methane in vibrationally excited states, particularly those involving excitation of the nu(4) bending mode. Fractional energy uptakes f(j) defined as the fraction of the mean energy of the reacting gas-surface collision complexes that derives from specific degrees of freedom of the reactants (i.e., molecular translation, rotation, vibration, and surface) are calculated for thermal dissociative chemisorption. At 500 K, the fractional energy uptakes are calculated to be f(t)=14%, f(r)=21%, f(v)=40%, and f(s)=25%. Over the temperature range from 500 K to 1500 K relevant to thermal catalysis, the incident gas-phase molecules supply the preponderance of energy used to surmount the barrier to dissociative chemisorption, f(g)=f(t)+f(r)+f(v) approximately 75%, with the highest energy uptake always coming from the molecular vibrational degrees of freedom. The predictions of the statistical, mode-nonspecific microcanonical theory are compared to those of other dynamical theories and to recent experimental data.
Collapse
Affiliation(s)
- H L Abbott
- Department of Chemistry, University of Virginia, Charlottesville, Virginia 22904-4319, USA
| | | | | |
Collapse
|
39
|
Abbott HL, Bukoski A, Kavulak DF, Harrison I. Dissociative chemisorption of methane on Ni(100): Threshold energy from CH4(2ν3) eigenstate-resolved sticking measurements. J Chem Phys 2003. [DOI: 10.1063/1.1613935] [Citation(s) in RCA: 31] [Impact Index Per Article: 1.5] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 12/11/2022] Open
|
40
|
Williams GM, Harrison I, Carlick CA, Crowley O. Changes in enantiomeric fraction as evidence of natural attenuation of mecoprop in a limestone aquifer. J Contam Hydrol 2003; 64:253-67. [PMID: 12814883 DOI: 10.1016/s0169-7722(02)00206-1] [Citation(s) in RCA: 14] [Impact Index Per Article: 0.7] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 05/23/2023]
Abstract
Natural attenuation of the chiral pesticide mecoprop [2-(2-methyl-4-chlorophenoxy)propionic acid] has been studied by determining changes in its enantiomeric fraction in different redox environments down gradient of a landfill in the Lincolnshire Limestone. Previous studies have shown that mecoprop degrades predominantly aerobically and that differences in the biological behaviour of the two enantiomers will change their relative proportions during biodegradation. Originally deposited as a racemic mixture, there has been no change in the enantiomeric fraction in the most polluted part of the landfill plume where conditions are sulphate reducing/methanogenic. In the nitrate-reducing zone, the proportion of (S)-mecoprop increases, suggesting preferential degradation of (R)-mecoprop; while in the aerobic zone, the proportion of (R)-mecoprop increases, suggesting faster degradation of (S)-mecoprop. Mecoprop persistence in the confined Lincolnshire Limestone further downdip is explained by inhibition of degradation in sulphate-reducing conditions, which develop naturally. Laboratory microcosm experiments using up to 10 mg l(-1) of mecoprop confirm these inferences and show that under aerobic conditions, (S)-mecoprop and (R)-mecoprop degrade with zero-order kinetics at rates of 1.90 and 1.32 mg l(-1) day(-1), respectively. Under nitrate-reducing conditions (S)-mecoprop does not degrade, but (R)-mecoprop degrades with zero-order kinetics at 0.65 mg l(-1) day(-1) to produce a stoichiometric equivalent amount of 4-chloro-2-methylphenol. This metabolite only degrades when the (R)-mecoprop has disappeared. The addition of nitrate to a dormant iron-reducing microcosm devoid of nitrate stimulated anaerobic degradation of (R)-mecoprop after a lag period of 21 days. There was no evidence for enantiomeric inversion. The study demonstrates the sensitivity of changes in enantiomeric fraction for detecting natural attenuation, and reveals subtle differences in mecoprop degradation in different redox environments within the Lincolnshire Limestone aquifer.
Collapse
Affiliation(s)
- G M Williams
- British Geological Survey, Keyworth, Nottingham, NG12 5GG, UK.
| | | | | | | |
Collapse
|
41
|
Bukoski A, Harrison I. Assessing a microcanonical theory of gas-surface reactivity: Applicability to thermal equilibrium, nonequilibrium, and eigenstate-resolved dissociation of methane on Ni(100). J Chem Phys 2003. [DOI: 10.1063/1.1570393] [Citation(s) in RCA: 24] [Impact Index Per Article: 1.1] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/14/2022] Open
|
42
|
Affiliation(s)
- I. Harrison
- The Pearlstone Center of Aeronautical Engineering, Department of Mechanical Engineering, Ben–Gurion University of the Negev, Beer–Sheva 84105, Israel
| | - G. deBotton
- The Pearlstone Center of Aeronautical Engineering, Department of Mechanical Engineering, Ben–Gurion University of the Negev, Beer–Sheva 84105, Israel
| |
Collapse
|
43
|
Bukoski A, Blumling D, Harrison I. Microcanonical unimolecular rate theory at surfaces. I. Dissociative chemisorption of methane on Pt(111). J Chem Phys 2003. [DOI: 10.1063/1.1525803] [Citation(s) in RCA: 53] [Impact Index Per Article: 2.5] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/14/2022] Open
|
44
|
Bourdon EBD, Cowin JP, Harrison I, Polanyi JC, Segner J, Stanners CD, Young PA. UV photodissociation and photodesorption of adsorbed molecules. 1. Methyl bromide on lithium fluoride(001). ACTA ACUST UNITED AC 2002. [DOI: 10.1021/j150669a009] [Citation(s) in RCA: 113] [Impact Index Per Article: 5.1] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/29/2022]
|
45
|
Trager-Cowan C, Sweeney F, Hastie J, Manson-Smith SK, Cowan DA, McColl D, Mohammed A, O'Donnell KP, Zubia D, Hersee SD, Foxon CT, Harrison I, Novikov SV. Characterization of nitride thin films by electron backscatter diffraction. J Microsc 2002; 205:226-30. [PMID: 11996185 DOI: 10.1046/j.1365-2818.2002.00996.x] [Citation(s) in RCA: 8] [Impact Index Per Article: 0.4] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/20/2022]
Abstract
Thin films incorporating GaN, InGaN and AlGaN are presently arousing considerable excitement because of their suitability for UV and visible light-emitting diodes and laser diodes. However, because of the lattice mismatch between presently used substrates and epitaxial nitride thin films, the films are of variable quality In this paper we describe our preliminary studies of nitride thin films using electron backscattered diffraction (EBSD). We show that the EBSD technique may be used to reveal the relative orientation of an epitaxial thin film with respect to its substrate (a 90 degrees rotation between a GaN epitaxial thin film and its sapphire substrate is observed) and to determine its tilt (a GaN thin film was found to be tiltedby 13 +/- 1 degrees towards [1010]GaN), where the tilt is due to the inclination of the sapphire substrate (cut off-axis by 10 degrees from (0001)sapphire towards (1010)sapphire). We compare EBSD patterns obtained from As-doped GaN films grown by plasma-assisted molecular beam epitaxy (PA-MBE) with low and high As4 flux, respectively. Higher As4 flux results in sharper, better defined patterns, this observation is consistent with the improved surface morphology observed in AFM studies. Finally, we show that more detail can be discerned in EBSD patterns from GaN thin films when samples are cooled.
Collapse
Affiliation(s)
- C Trager-Cowan
- Department of Physics and Applied Physics, University of Strathclyde, Glasgow, UK.
| | | | | | | | | | | | | | | | | | | | | | | | | |
Collapse
|
46
|
Abstract
A natural groundwater system modified by pollutant phenols and agricultural nitrate has been modelled in the laboratory by a series of sacrificial microcosm experiments. Samples of aquifer sediment and groundwater from the margin of the phenol plume were used to inoculate anaerobic microcosms enriched in nitrate and pollutant phenols. Rapid degradation of phenol and p-cresol was observed over a 35-day period leading to the generation of inorganic carbon and a number of transient intermediates. O-cresol proved to be recalcitrant on the experimental time-scale. A mass balance calculation shows that, during degradation, carbon was conserved in the aqueous phase. Groundwater-sediment interactions were monitored using carbon stable isotope data. A mass balance for solution TIC indicates thatp-cresol degradation stimulated the dissolution of sedimentary carbonate phases due to the formation of carbonic acid. Compound-specific carbon isotope analysis (GC-IRMS) was used to search for 13C enrichment in residual p-cresol. A slight enrichment trend (epsilon = -2.5/1000) was tentatively identified. The potential of this fractionation effect for obtaining in situ degradation rates is discussed. Results from the microcosm experiments help to explain the observed distribution of nitrate and phenols within the polluted aquifer.
Collapse
Affiliation(s)
- M J Spence
- School of Earth Sciences, University of Leeds, UK
| | | | | | | | | |
Collapse
|
47
|
Harrison I, Williams GM, Higgo JJ, Leader RU, Kim AW, Noy DJ. Microcosm studies of microbial degradation in a coal tar distillate plume. J Contam Hydrol 2001; 53:319-340. [PMID: 11820476 DOI: 10.1016/s0169-7722(01)00172-3] [Citation(s) in RCA: 6] [Impact Index Per Article: 0.3] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 05/23/2023]
Abstract
Investigation of a groundwater plume containing up to 24 g l(-1) phenolic compounds suggested that over a period of nearly 50 years, little degradation had occurred despite the presence of a microbial community and electron acceptors within the core of the plume. In order to study the effect of contaminant concentration on degradation behaviour, laboratory microcosm experiments were performed under aerobic and anaerobic conditions at four different concentrations obtained by diluting contaminated with uncontaminated groundwater. The microcosms contained groundwater with total phenols at ca. 200, 250, 660 and 5000 mg l(-1), and aquifer sediment that had been acclimatised within the plume for several months. The microcosms were operated for a period of 390-400 days along with sterile controls to ascertain whether degradation was microbially mediated or abiotic. Under aerobic conditions, degradation only occurred at concentrations up to 660 mg l(-1) total phenols. At phenol concentrations below 250 mg l(-1) a benzoquinone intermediate, thought to originate from the degradation of 2,5-dimethylphenol, was isolated and identified. This suggested an unusual degradative pathway for this compound; its aerobic degradation more commonly proceeding via catecholic intermediates. Under anaerobic conditions, degradation only occurred in the most dilute microcosm (total phenols 195 mg l(-1)) with a loss of p-cresol accompanied by a nonstoichiometric decrease in nitrate and sulphate. By inference, iron(III) from the sediment may also have been used as a terminal electron acceptor, in which case the amount of biologically available iron released was calculated as 1.07 mg Fe(III)/g of sediment. The study shows that natural attenuation is likely to be stimulated by dilution of the plume.
Collapse
Affiliation(s)
- I Harrison
- British Geological Survey, Kinsey Dunham Centre, Keyworth, Nottingham, UK.
| | | | | | | | | | | |
Collapse
|
48
|
Abstract
The concept and regulation of a code of ethics and professional conduct are approached differently in Great Britain and the USA. In Great Britain, the Royal Pharmaceutical Society has no definition of professional conduct, its Code of Ethics covering only those items upon which it believes that it must make a comment or explanation. Individual States in the USA have definitions of professional conduct, which are defined and regulated by the State legal system.
Collapse
|
49
|
Affiliation(s)
- R. Zehr
- Department of Chemistry, University of Virginia, Charlottesville, Virginia 22904
| | - A. Solodukhin
- Department of Chemistry, University of Virginia, Charlottesville, Virginia 22904
| | - B. C. Haynie
- Department of Chemistry, University of Virginia, Charlottesville, Virginia 22904
| | - C. French
- Department of Chemistry, University of Virginia, Charlottesville, Virginia 22904
| | - I. Harrison
- Department of Chemistry, University of Virginia, Charlottesville, Virginia 22904
| |
Collapse
|
50
|
Affiliation(s)
- H. Xu
- Department of Chemistry, University of Virginia, Charlottesville, Virginia 22901
| | - I. Harrison
- Department of Chemistry, University of Virginia, Charlottesville, Virginia 22901
| |
Collapse
|