1
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Psaltis A, Chen AA, Longland R, Connolly DS, Brune CR, Davids B, Fallis J, Giri R, Greife U, Hutcheon DA, Kroll L, Lennarz A, Liang J, Lovely M, Luo M, Marshall C, Paneru SN, Parikh A, Ruiz C, Shotter AC, Williams M. Direct Measurement of Resonances in ^{7}Be(α,γ)^{11}C Relevant to νp-Process Nucleosynthesis. Phys Rev Lett 2022; 129:162701. [PMID: 36306775 DOI: 10.1103/physrevlett.129.162701] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 12/31/2021] [Revised: 07/01/2022] [Accepted: 08/24/2022] [Indexed: 06/16/2023]
Abstract
We have performed the first direct measurement of two resonances of the ^{7}Be(α,γ)^{11}C reaction with unknown strengths using an intense radioactive ^{7}Be beam and the DRAGON recoil separator. We report on the first measurement of the 1155 and 1110 keV resonance strengths of 1.73±0.25(stat)±0.40(syst) eV and 125_{-25}^{+27}(stat)±15(syst) meV, respectively. The present results have reduced the uncertainty in the ^{7}Be(α,γ)^{11}C reaction rate to ∼9.4%-10.7% over T=1.5-3 GK, which is relevant for nucleosynthesis in the neutrino-driven outflows of core-collapse supernovae (νp process). We find no effect of the new, constrained reaction rate on νp-process nucleosynthesis.
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Affiliation(s)
- A Psaltis
- Department of Physics and Astronomy, McMaster University, Hamilton, Ontario L8S 4M1, Canada
- The NuGrid Collaboration
| | - A A Chen
- Department of Physics and Astronomy, McMaster University, Hamilton, Ontario L8S 4M1, Canada
- The NuGrid Collaboration
| | - R Longland
- Department of Physics, North Carolina State University, Raleigh, North Carolina 27695, USA
- Triangle Universities Nuclear Laboratory, Duke University, Durham, North Carolina 27710, USA
| | - D S Connolly
- TRIUMF, 4004 Wesbrook Mall, Vancouver, British Columbia V6T 2A3, Canada
| | - C R Brune
- Department of Physics and Astronomy, Ohio University, Athens, Ohio 45701, USA
| | - B Davids
- TRIUMF, 4004 Wesbrook Mall, Vancouver, British Columbia V6T 2A3, Canada
- Department of Physics, Simon Fraser University, Burnaby, British Columbia V5A 1S6, Canada
| | - J Fallis
- North Island College, 2300 Ryan Road, Courtenay, British Columbia V9N 8N6, Canada
| | - R Giri
- Department of Physics and Astronomy, Ohio University, Athens, Ohio 45701, USA
| | - U Greife
- Department of Physics, Colorado School of Mines, Golden, Colorado 80401, USA
| | - D A Hutcheon
- TRIUMF, 4004 Wesbrook Mall, Vancouver, British Columbia V6T 2A3, Canada
| | - L Kroll
- Department of Physics and Astronomy, McMaster University, Hamilton, Ontario L8S 4M1, Canada
- The NuGrid Collaboration
| | - A Lennarz
- TRIUMF, 4004 Wesbrook Mall, Vancouver, British Columbia V6T 2A3, Canada
| | - J Liang
- Department of Physics and Astronomy, McMaster University, Hamilton, Ontario L8S 4M1, Canada
| | - M Lovely
- Department of Physics, Colorado School of Mines, Golden, Colorado 80401, USA
| | - M Luo
- Department of Physics and Astronomy, University of British Columbia, Vancouver, British Columbia V6T 1Z4, Canada
| | - C Marshall
- Department of Physics, North Carolina State University, Raleigh, North Carolina 27695, USA
- Triangle Universities Nuclear Laboratory, Duke University, Durham, North Carolina 27710, USA
| | - S N Paneru
- Department of Physics and Astronomy, Ohio University, Athens, Ohio 45701, USA
| | - A Parikh
- Department de Física, Universitat Politècnica de Catalunya, E-08036 Barcelona, Spain
| | - C Ruiz
- TRIUMF, 4004 Wesbrook Mall, Vancouver, British Columbia V6T 2A3, Canada
- Department of Physics and Astronomy, University of Victoria, Victoria, British Columbia V8W 2Y2, Canada
| | - A C Shotter
- School of Physics, University of Edinburgh EH9 3JZ Edinburgh, United Kingdom
| | - M Williams
- TRIUMF, 4004 Wesbrook Mall, Vancouver, British Columbia V6T 2A3, Canada
- Department of Physics, University of York, Heslington, York YO10 5DD, United Kingdom
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2
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Mahajan R, Adams A, Allmond J, Alvarez Pol H, Argo E, Ayyad Y, Bardayan D, Bazin D, Budner T, Chen A, Chipps K, Davids B, Dopfer J, Friedman M, Fynbo H, Grzywacz R, Jose J, Liang J, Pain S, Perez-Loureiro D, Pollacco E, Psaltis A, Ravishankar S, Rogers A, Schaedig L, Sun LJ, Surbrook J, Wheeler T, Weghorn L, Wrede C. Measuring the 15O( α, γ) 19Ne Reaction in Type I X-ray Bursts using the GADGET II TPC: Software. EPJ Web Conf 2022. [DOI: 10.1051/epjconf/202226011034] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/14/2022] Open
Abstract
15O(α,γ)19Ne is regarded as one of the most important thermonuclear reactions in type I X-ray bursts. For studying the properties of the key resonance in this reaction using β decay, the existing Proton Detector component of the Gaseous Detector with Germanium Tagging (GADGET) assembly is being upgraded to operate as a time projection chamber (TPC) at FRIB. This upgrade includes the associated hardware as well as software and this paper mainly focusses on the software upgrade. The full detector set up is simulated using the ATTPCROOTv 2 data analysis framework for 20Mg and 241Am.
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3
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Wheeler T, Adams A, Allmond J, Alvarez Pol H, Argo E, Ayyad Y, Bardayan D, Bazin D, Budner T, Chen A, Chipps K, Davids B, Dopfer J, Friedman M, Fynbo H, Grzywacz R, Jose J, Liang J, Mahajan R, Pain S, Pérez-Loureiro D, Pollacco E, Psaltis A, Ravishankar S, Rogers A, Schaedig L, Sun LJ, Surbrook J, Weghorn L, Wrede C. Measuring the 15O(α, γ) 19Ne reaction in Type I X-ray bursts using the GADGET II TPC: Hardware. EPJ Web Conf 2022. [DOI: 10.1051/epjconf/202226011046] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/14/2022] Open
Abstract
Sensitivity studies have shown that the 15O(α, γ)19Ne reaction is the most important reaction rate uncertainty affecting the shape of light curves from Type I X-ray bursts. This reaction is dominated by the 4.03 MeV resonance in 19Ne. Previous measurements by our group have shown that this state is populated in the decay sequence of 20Mg. A single 20Mg(βp α)15O event through the key 15O(α, γ)19Ne resonance yields a characteristic signature: the emission of a proton and alpha particle. To achieve the granularity necessary for the identification of this signature, we have upgraded the Proton Detector of the Gaseous Detector with Germanium Tagging (GADGET) into a time projection chamber to form the GADGET II detection system. GADGET II has been fully constructed, and is entering the testing phase.
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4
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Lotay G, Lennarz A, Ruiz C, Akers C, Chen AA, Christian G, Connolly D, Davids B, Davinson T, Fallis J, Hutcheon DA, Machule P, Martin L, Mountford DJ, Murphy ASJ. Radiative Capture on Nuclear Isomers: Direct Measurement of the ^{26m}Al(p,γ)^{27}Si Reaction. Phys Rev Lett 2022; 128:042701. [PMID: 35148128 DOI: 10.1103/physrevlett.128.042701] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 10/07/2021] [Revised: 12/10/2021] [Accepted: 12/24/2021] [Indexed: 06/14/2023]
Abstract
We present the first direct measurement of an astrophysical reaction using a radioactive beam of isomeric nuclei. In particular, we have measured the strength of the key 447-keV resonance in the ^{26m}Al(p,γ)^{27}Si reaction to be 432_{-226}^{+146} meV and find that this resonance dominates the thermally averaged reaction rate for temperatures between 0.3 and 2.5 GK. This work represents a critical development in resolving one of the longest standing issues in nuclear astrophysics research, relating to the measurement of proton capture reactions on excited quantum levels, and offers unique insight into the destruction of isomeric ^{26}Al in astrophysical plasmas.
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Affiliation(s)
- G Lotay
- Department of Physics, University of Surrey, Guildford GU2 7XH, United Kingdom
| | - A Lennarz
- TRIUMF, Vancouver, British Columbia V6T 2A3, Canada
- Department of Physics and Astronomy, McMaster University, Hamilton, Ontario L8S 4M1, Canada
| | - C Ruiz
- TRIUMF, Vancouver, British Columbia V6T 2A3, Canada
- Department of Physics and Astronomy, University of Victoria, Victoria, BC V8W 2Y2, Canada
| | - C Akers
- TRIUMF, Vancouver, British Columbia V6T 2A3, Canada
- Department of Physics, University of York, Heslington, York YO10 5DD, United Kingdom
| | - A A Chen
- Department of Physics and Astronomy, McMaster University, Hamilton, Ontario L8S 4M1, Canada
| | - G Christian
- TRIUMF, Vancouver, British Columbia V6T 2A3, Canada
| | - D Connolly
- TRIUMF, Vancouver, British Columbia V6T 2A3, Canada
| | - B Davids
- TRIUMF, Vancouver, British Columbia V6T 2A3, Canada
- Department of Physics, Simon Fraser University, Burnaby, British Columbia V5A 1S6, Canada
| | - T Davinson
- School of Physics and Astronomy, University of Edinburgh, Edinburgh EH9 3JZ, United Kingdom
| | - J Fallis
- TRIUMF, Vancouver, British Columbia V6T 2A3, Canada
| | - D A Hutcheon
- TRIUMF, Vancouver, British Columbia V6T 2A3, Canada
| | - P Machule
- TRIUMF, Vancouver, British Columbia V6T 2A3, Canada
| | - L Martin
- TRIUMF, Vancouver, British Columbia V6T 2A3, Canada
| | - D J Mountford
- School of Physics and Astronomy, University of Edinburgh, Edinburgh EH9 3JZ, United Kingdom
| | - A St J Murphy
- School of Physics and Astronomy, University of Edinburgh, Edinburgh EH9 3JZ, United Kingdom
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5
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Lotay G, Gillespie SA, Williams M, Rauscher T, Alcorta M, Amthor AM, Andreoiu CA, Baal D, Ball GC, Bhattacharjee SS, Behnamian H, Bildstein V, Burbadge C, Catford WN, Doherty DT, Esker NE, Garcia FH, Garnsworthy AB, Hackman G, Hallam S, Hudson KA, Jazrawi S, Kasanda E, Kennington ARL, Kim YH, Lennarz A, Lubna RS, Natzke CR, Nishimura N, Olaizola B, Paxman C, Psaltis A, Svensson CE, Williams J, Wallis B, Yates D, Walter D, Davids B. First Direct Measurement of an Astrophysical p-Process Reaction Cross Section Using a Radioactive Ion Beam. Phys Rev Lett 2021; 127:112701. [PMID: 34558922 DOI: 10.1103/physrevlett.127.112701] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 05/14/2021] [Revised: 07/19/2021] [Accepted: 08/11/2021] [Indexed: 06/13/2023]
Abstract
We have performed the first direct measurement of the ^{83}Rb(p,γ) radiative capture reaction cross section in inverse kinematics using a radioactive beam of ^{83}Rb at incident energies of 2.4 and 2.7A MeV. The measured cross section at an effective relative kinetic energy of E_{cm}=2.393 MeV, which lies within the relevant energy window for core collapse supernovae, is smaller than the prediction of statistical model calculations. This leads to the abundance of ^{84}Sr produced in the astrophysical p process being higher than previously calculated. Moreover, the discrepancy of the present data with theoretical predictions indicates that further experimental investigation of p-process reactions involving unstable projectiles is clearly warranted.
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Affiliation(s)
- G Lotay
- Department of Physics, University of Surrey, Guildford GU2 7XH, United Kingdom
| | - S A Gillespie
- TRIUMF, 4004 Wesbrook Mall, Vancouver, British Columbia V6T 2A3, Canada
| | - M Williams
- TRIUMF, 4004 Wesbrook Mall, Vancouver, British Columbia V6T 2A3, Canada
- Department of Physics, University of York, Heslington, York YO10 5DD, United Kingdom
| | - T Rauscher
- Department of Physics, University of Basel, Klingelbergstrasse 82, CH-4056 Basel, Switzerland
- Centre for Astrophysics Research, University of Hertfordshire, Hatfield AL10 9AB, United Kingdom
| | - M Alcorta
- TRIUMF, 4004 Wesbrook Mall, Vancouver, British Columbia V6T 2A3, Canada
| | - A M Amthor
- Department of Physics and Astronomy, Bucknell University, Lewisburg, Pennsylvania 17837, USA
| | - C A Andreoiu
- Department of Chemistry, Simon Fraser University, Burnaby, British Columbia V5A 1S6, Canada
| | - D Baal
- TRIUMF, 4004 Wesbrook Mall, Vancouver, British Columbia V6T 2A3, Canada
| | - G C Ball
- TRIUMF, 4004 Wesbrook Mall, Vancouver, British Columbia V6T 2A3, Canada
| | - S S Bhattacharjee
- TRIUMF, 4004 Wesbrook Mall, Vancouver, British Columbia V6T 2A3, Canada
| | - H Behnamian
- Department of Physics, University of Guelph, Guelph, Ontario N1G 2W1, Canada
| | - V Bildstein
- Department of Physics, University of Guelph, Guelph, Ontario N1G 2W1, Canada
| | - C Burbadge
- Department of Physics, University of Guelph, Guelph, Ontario N1G 2W1, Canada
| | - W N Catford
- Department of Physics, University of Surrey, Guildford GU2 7XH, United Kingdom
| | - D T Doherty
- Department of Physics, University of Surrey, Guildford GU2 7XH, United Kingdom
| | - N E Esker
- TRIUMF, 4004 Wesbrook Mall, Vancouver, British Columbia V6T 2A3, Canada
| | - F H Garcia
- Department of Chemistry, Simon Fraser University, Burnaby, British Columbia V5A 1S6, Canada
| | - A B Garnsworthy
- TRIUMF, 4004 Wesbrook Mall, Vancouver, British Columbia V6T 2A3, Canada
| | - G Hackman
- TRIUMF, 4004 Wesbrook Mall, Vancouver, British Columbia V6T 2A3, Canada
| | - S Hallam
- Department of Physics, University of Surrey, Guildford GU2 7XH, United Kingdom
| | - K A Hudson
- TRIUMF, 4004 Wesbrook Mall, Vancouver, British Columbia V6T 2A3, Canada
- Department of Physics, Simon Fraser University, Burnaby, British Columbia V5A 1S6, Canada
| | - S Jazrawi
- Department of Physics, University of Surrey, Guildford GU2 7XH, United Kingdom
| | - E Kasanda
- Department of Physics, University of Guelph, Guelph, Ontario N1G 2W1, Canada
| | - A R L Kennington
- Department of Physics, University of Surrey, Guildford GU2 7XH, United Kingdom
| | - Y H Kim
- Department of Nuclear Engineering, Hanyang University, Seoul 04763, Republic of Korea
| | - A Lennarz
- TRIUMF, 4004 Wesbrook Mall, Vancouver, British Columbia V6T 2A3, Canada
| | - R S Lubna
- TRIUMF, 4004 Wesbrook Mall, Vancouver, British Columbia V6T 2A3, Canada
| | - C R Natzke
- TRIUMF, 4004 Wesbrook Mall, Vancouver, British Columbia V6T 2A3, Canada
- Department of Physics, Colorado School of Mines, Golden, Colorado 80401, USA
| | - N Nishimura
- Astrophysical Big Bang Laboratory, CPR, RIKEN, Wako, Saitama 351-0198, Japan
| | - B Olaizola
- TRIUMF, 4004 Wesbrook Mall, Vancouver, British Columbia V6T 2A3, Canada
| | - C Paxman
- Department of Physics, University of Surrey, Guildford GU2 7XH, United Kingdom
- TRIUMF, 4004 Wesbrook Mall, Vancouver, British Columbia V6T 2A3, Canada
| | - A Psaltis
- Department of Physics and Astronomy, McMaster University, Hamilton, Ontario L8S 4L8, Canada
| | - C E Svensson
- Department of Physics, University of Guelph, Guelph, Ontario N1G 2W1, Canada
| | - J Williams
- TRIUMF, 4004 Wesbrook Mall, Vancouver, British Columbia V6T 2A3, Canada
| | - B Wallis
- Department of Physics, University of York, Heslington, York YO10 5DD, United Kingdom
| | - D Yates
- TRIUMF, 4004 Wesbrook Mall, Vancouver, British Columbia V6T 2A3, Canada
- Department of Physics and Astronomy, University of British Columbia, Vancouver BC V6T 1Z4, Canada
| | - D Walter
- TRIUMF, 4004 Wesbrook Mall, Vancouver, British Columbia V6T 2A3, Canada
| | - B Davids
- TRIUMF, 4004 Wesbrook Mall, Vancouver, British Columbia V6T 2A3, Canada
- Department of Physics, Simon Fraser University, Burnaby, British Columbia V5A 1S6, Canada
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6
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Wilkinson R, Lotay G, Lennarz A, Ruiz C, Christian G, Akers C, Catford WN, Chen AA, Connolly D, Davids B, Hutcheon DA, Jedrejcic D, Laird AM, Martin L, McNeice E, Riley J, Williams M. Direct Measurement of the Key E_{c.m.}=456 keV Resonance in the Astrophysical ^{19}Ne(p,γ)^{20}Na Reaction and Its Relevance for Explosive Binary Systems. Phys Rev Lett 2017; 119:242701. [PMID: 29286739 DOI: 10.1103/physrevlett.119.242701] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 08/24/2017] [Indexed: 06/07/2023]
Abstract
We have performed a direct measurement of the ^{19}Ne(p,γ)^{20}Na reaction in inverse kinematics using a beam of radioactive ^{19}Ne. The key astrophysical resonance in the ^{19}Ne+p system has been definitely measured for the first time at E_{c.m.}=456_{-2}^{+5} keV with an associated strength of 17_{-5}^{+7} meV. The present results are in agreement with resonance strength upper limits set by previous direct measurements, as well as resonance energies inferred from precision (^{3}He, t) charge exchange reactions. However, both the energy and strength of the 456 keV resonance disagree with a recent indirect study of the ^{19}Ne(d, n)^{20}Na reaction. In particular, the new ^{19}Ne(p,γ)^{20}Na reaction rate is found to be factors of ∼8 and ∼5 lower than the most recent evaluation over the temperature range of oxygen-neon novae and astrophysical x-ray bursts, respectively. Nevertheless, we find that the ^{19}Ne(p,γ)^{20}Na reaction is likely to proceed fast enough to significantly reduce the flux of ^{19}F in nova ejecta and does not create a bottleneck in the breakout from the hot CNO cycles into the rp process.
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Affiliation(s)
- R Wilkinson
- Department of Physics, University of Surrey, Guildford GU2 7XH, United Kingdom
| | - G Lotay
- Department of Physics, University of Surrey, Guildford GU2 7XH, United Kingdom
- National Physical Laboratory, Teddington, Middlesex TW11 0LW, United Kingdom
| | - A Lennarz
- TRIUMF, Vancouver, British Columbia V6T 2A3, Canada
| | - C Ruiz
- TRIUMF, Vancouver, British Columbia V6T 2A3, Canada
| | - G Christian
- Cyclotron Institute, Texas A&M University, College Station, Texas 77843-3366, USA
- Department of Physics and Astronomy, Texas A&M University, College Station, Texas 77843-3366, USA
- Nuclear Solutions Institute, Texas A&M University, College Station, Texas 77843-3366, USA
| | - C Akers
- TRIUMF, Vancouver, British Columbia V6T 2A3, Canada
| | - W N Catford
- Department of Physics, University of Surrey, Guildford GU2 7XH, United Kingdom
| | - A A Chen
- Department of Physics and Astronomy, McMaster University, Hamilton, Ontario L8S 4M1, Canada
| | - D Connolly
- TRIUMF, Vancouver, British Columbia V6T 2A3, Canada
| | - B Davids
- TRIUMF, Vancouver, British Columbia V6T 2A3, Canada
| | - D A Hutcheon
- TRIUMF, Vancouver, British Columbia V6T 2A3, Canada
| | - D Jedrejcic
- Colorado School of Mines, Golden, Colorado 80401, USA
| | - A M Laird
- Department of Physics, The University of York, York YO10 5DD, United Kingdom
| | - L Martin
- TRIUMF, Vancouver, British Columbia V6T 2A3, Canada
| | - E McNeice
- Department of Physics and Astronomy, McMaster University, Hamilton, Ontario L8S 4M1, Canada
| | - J Riley
- Department of Physics, The University of York, York YO10 5DD, United Kingdom
| | - M Williams
- TRIUMF, Vancouver, British Columbia V6T 2A3, Canada
- Department of Physics, The University of York, York YO10 5DD, United Kingdom
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7
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Kumar A, Kanungo R, Calci A, Navrátil P, Sanetullaev A, Alcorta M, Bildstein V, Christian G, Davids B, Dohet-Eraly J, Fallis J, Gallant AT, Hackman G, Hadinia B, Hupin G, Ishimoto S, Krücken R, Laffoley AT, Lighthall J, Miller D, Quaglioni S, Randhawa JS, Rand ET, Rojas A, Roth R, Shotter A, Tanaka J, Tanihata I, Unsworth C. Nuclear Force Imprints Revealed on the Elastic Scattering of Protons with ^{10}C. Phys Rev Lett 2017; 118:262502. [PMID: 28707906 DOI: 10.1103/physrevlett.118.262502] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 03/08/2017] [Indexed: 06/07/2023]
Abstract
How does nature hold together protons and neutrons to form the wide variety of complex nuclei in the Universe? Describing many-nucleon systems from the fundamental theory of quantum chromodynamics has been the greatest challenge in answering this question. The chiral effective field theory description of the nuclear force now makes this possible but requires certain parameters that are not uniquely determined. Defining the nuclear force needs identification of observables sensitive to the different parametrizations. From a measurement of proton elastic scattering on ^{10}C at TRIUMF and ab initio nuclear reaction calculations, we show that the shape and magnitude of the measured differential cross section is strongly sensitive to the nuclear force prescription.
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Affiliation(s)
- A Kumar
- Astronomy and Physics Department, Saint Mary's University, Halifax, Nova Scotia B3H 3C3, Canada
| | - R Kanungo
- Astronomy and Physics Department, Saint Mary's University, Halifax, Nova Scotia B3H 3C3, Canada
| | - A Calci
- TRIUMF, Vancouver, British Columbia V6T2A3, Canada
| | - P Navrátil
- TRIUMF, Vancouver, British Columbia V6T2A3, Canada
| | - A Sanetullaev
- Astronomy and Physics Department, Saint Mary's University, Halifax, Nova Scotia B3H 3C3, Canada
- TRIUMF, Vancouver, British Columbia V6T2A3, Canada
| | - M Alcorta
- TRIUMF, Vancouver, British Columbia V6T2A3, Canada
| | - V Bildstein
- Department of Physics, University of Guelph, Guelph, Ontario N1G 2W1, Canada
| | - G Christian
- TRIUMF, Vancouver, British Columbia V6T2A3, Canada
| | - B Davids
- TRIUMF, Vancouver, British Columbia V6T2A3, Canada
| | - J Dohet-Eraly
- TRIUMF, Vancouver, British Columbia V6T2A3, Canada
- Istituto Nazionale di Fisica Nucleare, Sezione di Pisa, Largo B. Pontecorvo 3, I-56127 Pisa, Italy
| | - J Fallis
- TRIUMF, Vancouver, British Columbia V6T2A3, Canada
| | - A T Gallant
- TRIUMF, Vancouver, British Columbia V6T2A3, Canada
| | - G Hackman
- TRIUMF, Vancouver, British Columbia V6T2A3, Canada
| | - B Hadinia
- Department of Physics, University of Guelph, Guelph, Ontario N1G 2W1, Canada
| | - G Hupin
- Institut de Physique Nucléaire, Université Paris-Sud, IN2P3/CNRS, F-91406 Orsay Cedex, France
- CEA, DAM, DIF, F-91297 Arpajon, France
| | - S Ishimoto
- High Energy Accelerator Research Organization (KEK), Ibaraki 305-0801, Japan
| | - R Krücken
- TRIUMF, Vancouver, British Columbia V6T2A3, Canada
- Department of Physics and Astronomy, University of British Columbia, Vancouver, British Columbia V6T 1Z1, Canada
| | - A T Laffoley
- Department of Physics, University of Guelph, Guelph, Ontario N1G 2W1, Canada
| | - J Lighthall
- TRIUMF, Vancouver, British Columbia V6T2A3, Canada
| | - D Miller
- TRIUMF, Vancouver, British Columbia V6T2A3, Canada
| | - S Quaglioni
- Lawrence Livermore National Laboratory, P.O. Box 808, L-414, Livermore, California 94551, USA
| | - J S Randhawa
- Astronomy and Physics Department, Saint Mary's University, Halifax, Nova Scotia B3H 3C3, Canada
| | - E T Rand
- Department of Physics, University of Guelph, Guelph, Ontario N1G 2W1, Canada
| | - A Rojas
- TRIUMF, Vancouver, British Columbia V6T2A3, Canada
| | - R Roth
- Institut fur Kernphysik, Technische Universitat Darmstadt, 64289 Darmstadt, Germany
| | - A Shotter
- School of Physics and Astronomy, University of Edinburgh, JCMB, Mayfield Road, Edinburgh EH9 3JZ, United Kingdom
| | - J Tanaka
- RCNP, Osaka University, Mihogaoka, Ibaraki, Osaka 567 0047, Japan
| | - I Tanihata
- RCNP, Osaka University, Mihogaoka, Ibaraki, Osaka 567 0047, Japan
- School of Physics and Nuclear Energy Engineering and IRCNPC, Beihang University, Beijing 100191, China
| | - C Unsworth
- TRIUMF, Vancouver, British Columbia V6T2A3, Canada
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8
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Cavallaro M, De Napoli M, Cappuzzello F, Orrigo SEA, Agodi C, Bondí M, Carbone D, Cunsolo A, Davids B, Davinson T, Foti A, Galinski N, Kanungo R, Lenske H, Ruiz C, Sanetullaev A. Investigation of the ^{10}Li shell inversion by neutron continuum transfer reaction. Phys Rev Lett 2017; 118:012701. [PMID: 28106447 DOI: 10.1103/physrevlett.118.012701] [Citation(s) in RCA: 1] [Impact Index Per Article: 0.1] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 01/26/2016] [Indexed: 06/06/2023]
Abstract
This Letter reports a study of the highly debated ^{10}Li structure through the d(^{9}Li,p)^{10}Li one-neutron transfer reaction at 100 MeV. The ^{10}Li energy spectrum is measured up to 4.6 MeV and angular distributions corresponding to different excitation energy regions are reported for the first time. The comparison between data and theoretical predictions, including pairing correlation effects, shows the existence of a p_{1/2} resonance at 0.45±0.03 MeV excitation energy, while no evidence for a significant s-wave contribution close to the threshold energy is observed. Moreover, two high-lying structures are populated at 1.5 and 2.9 MeV. The corresponding angular distributions suggest a significant s_{1/2} partial-wave contribution for the 1.5 MeV structure and a mixing of configurations at higher energy, with the d_{5/2} partial-wave contributing the most to the cross section.
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Affiliation(s)
- M Cavallaro
- INFN-Laboratori Nazionali del Sud, I-95123 Catania, Italy
| | - M De Napoli
- INFN-Sezione di Catania, I-95123 Catania, Italy
| | - F Cappuzzello
- INFN-Laboratori Nazionali del Sud, I-95123 Catania, Italy
- Dipartimento di Fisica e Astronomia, Universitá di Catania, I-95123 Catania, Italy
| | - S E A Orrigo
- Instituto de Física Corpuscular, CSIC-Universidad de Valencia, E-46071 Valencia, Spain
| | - C Agodi
- INFN-Laboratori Nazionali del Sud, I-95123 Catania, Italy
| | - M Bondí
- INFN-Sezione di Catania, I-95123 Catania, Italy
| | - D Carbone
- INFN-Laboratori Nazionali del Sud, I-95123 Catania, Italy
| | - A Cunsolo
- INFN-Laboratori Nazionali del Sud, I-95123 Catania, Italy
| | - B Davids
- TRIUMF, Vancouver, British Columbia V6T2A3, Canada
| | - T Davinson
- School of Physics and Astronomy, University of Edinburgh, EH9 3FD Edinburgh, United Kingdom
| | - A Foti
- INFN-Sezione di Catania, I-95123 Catania, Italy
- Dipartimento di Fisica e Astronomia, Universitá di Catania, I-95123 Catania, Italy
| | - N Galinski
- TRIUMF, Vancouver, British Columbia V6T2A3, Canada
| | - R Kanungo
- Astronomy and Physics Department, Saint Marys University, Halifax, Nova Scotia B3H 3C3, Canada
| | - H Lenske
- Institut für Theoretische Physik, Universität Giessen, D-35392 Giessen, Germany
| | - C Ruiz
- TRIUMF, Vancouver, British Columbia V6T2A3, Canada
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9
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Wilkinson R, Lotay G, Lennarz A, Ruiz C, Christian G, Akers C, Catford WN, Chen AA, Connolly D, Davids B, Hutcheon DA, Jedrejcic D, Laird AM, Martin L, McNeice E, Riley J, Williams M. Constraining the 19Ne(p,γ) 20Na Reaction Rate Using a Direct Measurement at DRAGON. EPJ Web Conf 2017. [DOI: 10.1051/epjconf/201716501054] [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: 11/14/2022] Open
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10
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Lotay G, Christian G, Ruiz C, Akers C, Burke DS, Catford WN, Chen AA, Connolly D, Davids B, Fallis J, Hager U, Hutcheon DA, Mahl A, Rojas A, Sun X. Direct Measurement of the Astrophysical ^{38}K(p,γ)^{39}Ca Reaction and Its Influence on the Production of Nuclides toward the End Point of Nova Nucleosynthesis. Phys Rev Lett 2016; 116:132701. [PMID: 27081974 DOI: 10.1103/physrevlett.116.132701] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 11/19/2015] [Indexed: 06/05/2023]
Abstract
We have performed the first direct measurement of the ^{38}K(p,γ)^{39}Ca reaction using a beam of radioactive ^{38}K. A proposed ℓ=0 resonance in the ^{38}K+p system has been identified at 679(2) keV with an associated strength of 120_{-30}^{+50} meV. Upper limits of 1.16 (3.5) and 8.6 (26) meV at the 68% (95%) confidence level were also established for two further expected ℓ=0 resonances at 386 and 515 keV, respectively. The present results have reduced uncertainties in the ^{38}K(p,γ)^{39}Ca reaction rate at temperatures of 0.4 GK by more than 2 orders of magnitude and indicate that Ar and Ca may be ejected in observable quantities by oxygen-neon novae. However, based on the newly evaluated rate, the ^{38}K(p,γ)^{39}Ca path is unlikely to be responsible for the production of Ar and Ca in significantly enhanced quantities relative to solar abundances.
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Affiliation(s)
- G Lotay
- Department of Physics, University of Surrey, Guildford GU2 7XH, United Kingdom
- National Physical Laboratory, Teddington, Middlesex TW11 0LW, United Kingdom
| | - G Christian
- TRIUMF, Vancouver, British Columbia V6T 2A3, Canada
| | - C Ruiz
- TRIUMF, Vancouver, British Columbia V6T 2A3, Canada
| | - C Akers
- TRIUMF, Vancouver, British Columbia V6T 2A3, Canada
- Department of Physics, The University of York, York YO10 5DD, United Kingdom
| | - D S Burke
- Department of Physics and Astronomy, McMaster University, Hamilton, Ontario L8S 4M1, Canada
| | - W N Catford
- Department of Physics, University of Surrey, Guildford GU2 7XH, United Kingdom
| | - A A Chen
- Department of Physics and Astronomy, McMaster University, Hamilton, Ontario L8S 4M1, Canada
| | - D Connolly
- Colorado School of Mines, Golden, Colorado 80401, USA
| | - B Davids
- TRIUMF, Vancouver, British Columbia V6T 2A3, Canada
| | - J Fallis
- TRIUMF, Vancouver, British Columbia V6T 2A3, Canada
| | - U Hager
- Colorado School of Mines, Golden, Colorado 80401, USA
| | - D A Hutcheon
- TRIUMF, Vancouver, British Columbia V6T 2A3, Canada
| | - A Mahl
- Colorado School of Mines, Golden, Colorado 80401, USA
| | - A Rojas
- TRIUMF, Vancouver, British Columbia V6T 2A3, Canada
| | - X Sun
- TRIUMF, Vancouver, British Columbia V6T 2A3, Canada
- McGill University, Montreal, Quebec H3A 0G4, Canada
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11
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Cavallaro M, De Napoli M, Cappuzzello F, Agodi C, Bondí M, Carbone D, Cunsolo A, Davids B, Davinson T, Foti A, Galinski N, Kanungo R, Lenske H, Orrigo S, Ruiz C, Sanetullaev A. Preliminary study of the 10Li nucleus via one-neutron transfer. EPJ Web of Conferences 2016. [DOI: 10.1051/epjconf/201611706009] [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: 11/15/2022] Open
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12
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Margerin V, Lotay G, Woods PJ, Aliotta M, Christian G, Davids B, Davinson T, Doherty DT, Fallis J, Howell D, Kirsebom OS, Mountford DJ, Rojas A, Ruiz C, Tostevin JA. Inverse Kinematic Study of the (26g)Al(d,p)(27)Al Reaction and Implications for Destruction of (26)Al in Wolf-Rayet and Asymptotic Giant Branch Stars. Phys Rev Lett 2015; 115:062701. [PMID: 26296114 DOI: 10.1103/physrevlett.115.062701] [Citation(s) in RCA: 1] [Impact Index Per Article: 0.1] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 03/27/2015] [Indexed: 06/04/2023]
Abstract
In Wolf-Rayet and asymptotic giant branch (AGB) stars, the (26g)Al(p,γ)(27)Si reaction is expected to govern the destruction of the cosmic γ-ray emitting nucleus (26)Al. The rate of this reaction, however, is highly uncertain due to the unknown properties of key resonances in the temperature regime of hydrogen burning. We present a high-resolution inverse kinematic study of the (26g)Al(d,p)(27)Al reaction as a method for constraining the strengths of key astrophysical resonances in the (26g)Al(p,γ)(27)Si reaction. In particular, the results indicate that the resonance at E(r)=127 keV in (27)Si determines the entire (26g)Al(p,γ)(27)Si reaction rate over almost the complete temperature range of Wolf-Rayet stars and AGB stars.
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Affiliation(s)
- V Margerin
- School of Physics and Astronomy, University of Edinburgh, Edinburgh, EH9 3FD, United Kingdom
| | - G Lotay
- School of Physics and Astronomy, University of Edinburgh, Edinburgh, EH9 3FD, United Kingdom
- Department of Physics, University of Surrey, Guildford GU2 7XH, United Kingdom
- National Physical Laboratory, Teddington, Middlesex TW11 0LW, United Kingdom
| | - P J Woods
- School of Physics and Astronomy, University of Edinburgh, Edinburgh, EH9 3FD, United Kingdom
| | - M Aliotta
- School of Physics and Astronomy, University of Edinburgh, Edinburgh, EH9 3FD, United Kingdom
| | - G Christian
- TRIUMF, Vancouver, British Columbia V6T 2A3, Canada
| | - B Davids
- TRIUMF, Vancouver, British Columbia V6T 2A3, Canada
| | - T Davinson
- School of Physics and Astronomy, University of Edinburgh, Edinburgh, EH9 3FD, United Kingdom
| | - D T Doherty
- School of Physics and Astronomy, University of Edinburgh, Edinburgh, EH9 3FD, United Kingdom
| | - J Fallis
- TRIUMF, Vancouver, British Columbia V6T 2A3, Canada
| | - D Howell
- TRIUMF, Vancouver, British Columbia V6T 2A3, Canada
| | - O S Kirsebom
- TRIUMF, Vancouver, British Columbia V6T 2A3, Canada
| | - D J Mountford
- School of Physics and Astronomy, University of Edinburgh, Edinburgh, EH9 3FD, United Kingdom
| | - A Rojas
- TRIUMF, Vancouver, British Columbia V6T 2A3, Canada
| | - C Ruiz
- TRIUMF, Vancouver, British Columbia V6T 2A3, Canada
| | - J A Tostevin
- Department of Physics, University of Surrey, Guildford GU2 7XH, United Kingdom
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13
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Tomlinson JR, Fallis J, Laird AM, Fox SP, Akers C, Alcorta M, Bentley MA, Christian G, Davids B, Davinson T, Fulton BR, Galinski N, Rojas A, Ruiz C, de Séréville N, Shen M, Shotter AC. Measurement of 23Na(α,p)26Mg at Energies Relevant to 26Al Production in Massive Stars. Phys Rev Lett 2015; 115:052702. [PMID: 26274415 DOI: 10.1103/physrevlett.115.052702] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 04/22/2015] [Indexed: 06/04/2023]
Abstract
26Al is an important radioisotope in astrophysics that provides evidence of ongoing nucleosynthesis in the Galaxy. The 23Na(α, p)26Mg reaction has been identified by a sensitivity study as being one of the most important reactions for the production of 26Al in the convective C/Ne burning shell of massive stars. Owing to large uncertainties in previous experimental data, model calculations are used for the reaction rate of 23Na(α, p)26Mg in this sensitivity study. Current experimental data suggest a reaction rate a factor of ∼40 higher than model calculations. However, a new measurement of this reaction cross section has been made in inverse kinematics in the energy range E(c.m.)=1.28-3.15 MeV at TRIUMF, and found to be in reasonable agreement with the model calculation. A new reaction rate is calculated and tight constraints on the uncertainty in the production of 26Al, due to this reaction, are determined.
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Affiliation(s)
- J R Tomlinson
- The University of York, Heslington, York YO10 5DD, United Kingdom
| | - J Fallis
- TRIUMF, 4004 Westbrook Mall, Vancouver, British Columbia V6T 2A3, Canada
| | - A M Laird
- The University of York, Heslington, York YO10 5DD, United Kingdom
| | - S P Fox
- The University of York, Heslington, York YO10 5DD, United Kingdom
| | - C Akers
- The University of York, Heslington, York YO10 5DD, United Kingdom
- TRIUMF, 4004 Westbrook Mall, Vancouver, British Columbia V6T 2A3, Canada
| | - M Alcorta
- TRIUMF, 4004 Westbrook Mall, Vancouver, British Columbia V6T 2A3, Canada
| | - M A Bentley
- The University of York, Heslington, York YO10 5DD, United Kingdom
| | - G Christian
- TRIUMF, 4004 Westbrook Mall, Vancouver, British Columbia V6T 2A3, Canada
| | - B Davids
- TRIUMF, 4004 Westbrook Mall, Vancouver, British Columbia V6T 2A3, Canada
| | - T Davinson
- School of Physics and Astronomy, The University of Edinburgh, James Clerk Maxwell Building, Mayfield Road, Edinburgh EH9 3FD, United Kingdom
| | - B R Fulton
- The University of York, Heslington, York YO10 5DD, United Kingdom
| | - N Galinski
- TRIUMF, 4004 Westbrook Mall, Vancouver, British Columbia V6T 2A3, Canada
| | - A Rojas
- TRIUMF, 4004 Westbrook Mall, Vancouver, British Columbia V6T 2A3, Canada
| | - C Ruiz
- TRIUMF, 4004 Westbrook Mall, Vancouver, British Columbia V6T 2A3, Canada
| | - N de Séréville
- Institut de Physique Nucléaire d'Orsay, IN2P3-CNRS and Univ Paris-Sud, F-91405 Orsay Cedex, France
| | - M Shen
- TRIUMF, 4004 Westbrook Mall, Vancouver, British Columbia V6T 2A3, Canada
| | - A C Shotter
- School of Physics and Astronomy, The University of Edinburgh, James Clerk Maxwell Building, Mayfield Road, Edinburgh EH9 3FD, United Kingdom
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14
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Kanungo R, Sanetullaev A, Tanaka J, Ishimoto S, Hagen G, Myo T, Suzuki T, Andreoiu C, Bender P, Chen AA, Davids B, Fallis J, Fortin JP, Galinski N, Gallant AT, Garrett PE, Hackman G, Hadinia B, Jansen G, Keefe M, Krücken R, Lighthall J, McNeice E, Miller D, Otsuka T, Purcell J, Randhawa JS, Roger T, Rojas A, Savajols H, Shotter A, Tanihata I, Thompson IJ, Unsworth C, Voss P, Wang Z. Evidence of soft dipole resonance in ^{11}li with isoscalar character. Phys Rev Lett 2015; 114:192502. [PMID: 26024166 DOI: 10.1103/physrevlett.114.192502] [Citation(s) in RCA: 1] [Impact Index Per Article: 0.1] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 12/24/2014] [Indexed: 06/04/2023]
Abstract
The first conclusive evidence of a dipole resonance in ^{11}Li having isoscalar character observed from inelastic scattering with a novel solid deuteron target is reported. The experiment was performed at the newly commissioned IRIS facility at TRIUMF. The results show a resonance peak at an excitation energy of 1.03±0.03 MeV with a width of 0.51±0.11 MeV (FWHM). The angular distribution is consistent with a dipole excitation in the distorted-wave Born approximation framework. The observed resonance energy together with shell model calculations show the first signature that the monopole tensor interaction is important in ^{11}Li. The first ab initio calculations in the coupled cluster framework are also presented.
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Affiliation(s)
- R Kanungo
- Astronomy and Physics Department, Saint Mary's University, Halifax, Nova Scotia B3H 3C3, Canada
| | - A Sanetullaev
- Astronomy and Physics Department, Saint Mary's University, Halifax, Nova Scotia B3H 3C3, Canada
- TRIUMF, Vancouver, British Columbia V6T2A3, Canada
| | - J Tanaka
- RCNP, Osaka University, Mihogaoka, Ibaraki, Osaka 567 0047, Japan
| | - S Ishimoto
- High Energy Accelerator Research Organization (KEK), Ibaraki 305-0801, Japan
| | - G Hagen
- Physics Division, Oak Ridge National Laboratory, Oak Ridge, Tennessee 37831, USA
- Department of Physics and Astronomy, University of Tennessee, Knoxville, Tennessee 37996, USA
| | - T Myo
- General Education, Faculty of Engineering, Osaka Institute of Technology, Osaka, Osaka 535-8585, Japan
| | - T Suzuki
- Department of Physics, Nihon University, Setagaya-ku, Tokyo 156-8550, Japan
| | - C Andreoiu
- Department of Chemistry, Simon Fraser University, Burnaby, British Columbia V5A 1S6, Canada
| | - P Bender
- TRIUMF, Vancouver, British Columbia V6T2A3, Canada
| | - A A Chen
- Department of Physics and Astronomy, McMaster University, Hamilton, Ontario L8S 4M1, Canada
| | - B Davids
- TRIUMF, Vancouver, British Columbia V6T2A3, Canada
| | - J Fallis
- TRIUMF, Vancouver, British Columbia V6T2A3, Canada
| | - J P Fortin
- Astronomy and Physics Department, Saint Mary's University, Halifax, Nova Scotia B3H 3C3, Canada
- Department of Physics, University of Laval, Quebec City, Quebec G1V 0A8, Canada
| | - N Galinski
- TRIUMF, Vancouver, British Columbia V6T2A3, Canada
| | - A T Gallant
- TRIUMF, Vancouver, British Columbia V6T2A3, Canada
| | - P E Garrett
- Department of Physics, University of Guelph, Guelph, Ontario N1G 2W1, Canada
| | - G Hackman
- TRIUMF, Vancouver, British Columbia V6T2A3, Canada
| | - B Hadinia
- Department of Physics, University of Guelph, Guelph, Ontario N1G 2W1, Canada
| | - G Jansen
- Physics Division, Oak Ridge National Laboratory, Oak Ridge, Tennessee 37831, USA
- Department of Physics and Astronomy, University of Tennessee, Knoxville, Tennessee 37996, USA
| | - M Keefe
- Astronomy and Physics Department, Saint Mary's University, Halifax, Nova Scotia B3H 3C3, Canada
| | - R Krücken
- TRIUMF, Vancouver, British Columbia V6T2A3, Canada
- Department of Physics and Astronomy, University of British Columbia, Vancouver, British Columbia V6T 1Z1, Canada
| | - J Lighthall
- TRIUMF, Vancouver, British Columbia V6T2A3, Canada
| | - E McNeice
- Department of Physics and Astronomy, McMaster University, Hamilton, Ontario L8S 4M1, Canada
| | - D Miller
- TRIUMF, Vancouver, British Columbia V6T2A3, Canada
| | - T Otsuka
- Department of Physics and Center of Nuclear Studies, University of Tokyo, Bunky-ku, Tokyo 113-0033, Japan
| | - J Purcell
- Astronomy and Physics Department, Saint Mary's University, Halifax, Nova Scotia B3H 3C3, Canada
| | - J S Randhawa
- Astronomy and Physics Department, Saint Mary's University, Halifax, Nova Scotia B3H 3C3, Canada
| | - T Roger
- Grand Accélérateur National dIons Lourds, CEA/DSM-CNRS/IN2P3, B.P. 55027, F-14076 Caen Cedex 5, France
| | - A Rojas
- TRIUMF, Vancouver, British Columbia V6T2A3, Canada
| | - H Savajols
- Grand Accélérateur National dIons Lourds, CEA/DSM-CNRS/IN2P3, B.P. 55027, F-14076 Caen Cedex 5, France
| | - A Shotter
- School of Physics and Astronomy, University of Edinburgh, EH9 3JZ, Edinburgh, United Kingdom
| | - I Tanihata
- RCNP, Osaka University, Mihogaoka, Ibaraki, Osaka 567 0047, Japan
- School of Physics and Nuclear Energy Engineering and IRCNPC, Beihang University, Beijing 100191, China
| | - I J Thompson
- Lawrence Livermore National Laboratory, L-414, Livermore, California 94551, USA
| | - C Unsworth
- TRIUMF, Vancouver, British Columbia V6T2A3, Canada
| | - P Voss
- Department of Chemistry, Simon Fraser University, Burnaby, British Columbia V5A 1S6, Canada
| | - Z Wang
- TRIUMF, Vancouver, British Columbia V6T2A3, Canada
- Department of Chemistry, Simon Fraser University, Burnaby, British Columbia V5A 1S6, Canada
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15
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Carmona-Gallardo M, Rojas A, Borge M, Davids B, Fulton B, Hass M, Nara Singh B, Ruiz C, Tengblad O. 3He(α,γ)7Be cross section measured using complementary techniques. EPJ Web of Conferences 2014. [DOI: 10.1051/epjconf/20146607003] [Citation(s) in RCA: 6] [Impact Index Per Article: 0.6] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/14/2022] Open
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16
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Akers C, Laird AM, Fulton BR, Ruiz C, Bardayan DW, Buchmann L, Christian G, Davids B, Erikson L, Fallis J, Hager U, Hutcheon D, Martin L, Murphy ASJ, Nelson K, Spyrou A, Stanford C, Ottewell D, Rojas A. Measurement of radiative proton capture on 18F and implications for oxygen-neon novae. Phys Rev Lett 2013; 110:262502. [PMID: 23848867 DOI: 10.1103/physrevlett.110.262502] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 01/21/2013] [Indexed: 06/02/2023]
Abstract
The rate of the 18F(p,γ)19Ne reaction affects the final abundance of the γ-ray observable radioisotope 18F, produced in novae. However, no successful measurement of this reaction exists and the rate used is calculated from incomplete information on the contributing resonances. Of the two resonances thought to play a significant role, one has a radiative width estimated from the assumed analogue state in the mirror nucleus, 19F. The second does not have an analogue state assignment at all, resulting in an arbitrary radiative width being assumed. Here, we report the first successful direct measurement of the 18F(p,γ)^19Ne reaction. The strength of the 665 keV resonance (Ex=7.076 MeV) is found to be over an order of magnitude weaker than currently assumed in nova models. Reaction rate calculations show that this resonance therefore plays no significant role in the destruction of ^{18}F at any astrophysical energy.
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Affiliation(s)
- C Akers
- TRIUMF, Vancouver, British Columbia V6T 2A3, Canada
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17
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Salter PJC, Aliotta M, Davinson T, Al Falou H, Chen A, Davids B, Fulton BR, Galinski N, Howell D, Lotay G, Machule P, Murphy AS, Ruiz C, Sjue S, Taggart M, Walden P, Woods PJ. Measurement of the 18Ne(α,p0) 21Na reaction cross section in the burning energy region for x-ray bursts. Phys Rev Lett 2012; 108:242701. [PMID: 23004266 DOI: 10.1103/physrevlett.108.242701] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 02/16/2012] [Indexed: 06/01/2023]
Abstract
The 18Ne(α,p) 21Na reaction provides one of the main HCNO-breakout routes into the rp process in x-ray bursts. The 18Ne(α,p0) 21Na reaction cross section has been determined for the first time in the Gamow energy region for peak temperatures T∼2 GK by measuring its time-reversal reaction 21Na(p,α) 18Ne in inverse kinematics. The astrophysical rate for ground-state to ground-state transitions was found to be a factor of 2 lower than Hauser-Feshbach theoretical predictions. Our reduced rate will affect the physical conditions under which breakout from the HCNO cycles occurs via the 18Ne(α,p) 21Na reaction.
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Affiliation(s)
- P J C Salter
- SUPA, School of Physics and Astronomy, University of Edinburgh, Edinburgh EH9 3JZ, United Kingdom
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18
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Kanungo R, Nociforo C, Prochazka A, Aumann T, Boutin D, Cortina-Gil D, Davids B, Diakaki M, Farinon F, Geissel H, Gernhäuser R, Gerl J, Janik R, Jonson B, Kindler B, Knöbel R, Krücken R, Lantz M, Lenske H, Litvinov Y, Lommel B, Mahata K, Maierbeck P, Musumarra A, Nilsson T, Otsuka T, Perro C, Scheidenberger C, Sitar B, Strmen P, Sun B, Szarka I, Tanihata I, Utsuno Y, Weick H, Winkler M. One-neutron removal measurement reveals 24O as a new doubly magic nucleus. Phys Rev Lett 2009; 102:152501. [PMID: 19518623 DOI: 10.1103/physrevlett.102.152501] [Citation(s) in RCA: 30] [Impact Index Per Article: 2.0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 11/08/2008] [Indexed: 05/27/2023]
Abstract
The first measurement of the momentum distribution for one-neutron removal from (24)O at 920A MeV performed at GSI, Darmstadt is reported. The observed distribution has a width (FWHM) of 99 +/- 4 MeV/c in the projectile rest frame and a one-neutron removal cross section of 63 +/- 7 mb. The results are well explained with a nearly pure 2s_{1/2} neutron spectroscopic factor of 1.74 +/- 0.19 within the eikonal model. This large s-wave probability shows a spherical shell closure thereby confirming earlier suggestions that (24)O is a new doubly magic nucleus.
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Affiliation(s)
- R Kanungo
- Astronomy and Physics Department, Saint Mary's University, Halifax, NS B3H 3C3, Canada.
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19
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Tanihata I, Alcorta M, Bandyopadhyay D, Bieri R, Buchmann L, Davids B, Galinski N, Howell D, Mills W, Mythili S, Openshaw R, Padilla-Rodal E, Ruprecht G, Sheffer G, Shotter AC, Trinczek M, Walden P, Savajols H, Roger T, Caamano M, Mittig W, Roussel-Chomaz P, Kanungo R, Gallant A, Notani M, Savard G, Thompson IJ. Measurement of the two-halo neutron transfer reaction (1)H((11)Li, (9)Li)(3)H at 3A MeV. Phys Rev Lett 2008; 100:192502. [PMID: 18518445 DOI: 10.1103/physrevlett.100.192502] [Citation(s) in RCA: 5] [Impact Index Per Article: 0.3] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 01/22/2008] [Indexed: 05/26/2023]
Abstract
The p((11)Li, (9)Li)t reaction has been studied for the first time at an incident energy of 3A MeV at the new ISAC-2 facility at TRIUMF. An active target detector MAYA, built at GANIL, was used for the measurement. The differential cross sections have been determined for transitions to the (9)Li ground and first excited states in a wide range of scattering angles. Multistep transfer calculations using different (11)Li model wave functions show that wave functions with strong correlations between the halo neutrons are the most successful in reproducing the observation.
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20
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Ruiz C, Parikh A, José J, Buchmann L, Caggiano JA, Chen AA, Clark JA, Crawford H, Davids B, D'Auria JM, Davis C, Deibel C, Erikson L, Fogarty L, Frekers D, Greife U, Hussein A, Hutcheon DA, Huyse M, Jewett C, Laird AM, Lewis R, Mumby-Croft P, Olin A, Ottewell DF, Ouellet CV, Parker P, Pearson J, Ruprecht G, Trinczek M, Vockenhuber C, Wrede C. Measurement of the Ec.m. = 184 keV resonance strength in the 26gAl (p, gamma)27 Si reaction. Phys Rev Lett 2006; 96:252501. [PMID: 16907298 DOI: 10.1103/physrevlett.96.252501] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 04/13/2006] [Indexed: 05/11/2023]
Abstract
The strength of the Ec.m. = 184 keV resonance in the 26gAl(p, gamma)27 reaction has been measured in inverse kinematics using the DRAGON recoil separator at TRIUMF's ISAC facility. We measure a value of omega gamma = 35 +/- 7 microeV and a resonance energy of Ec.m. = 184 +/- 1 keV, consistent with p-wave proton capture into the 7652(3) keV state in 27Si, and discuss the implications of these values for 26GAl nucleosynthesis in typical oxygen-neon white-dwarf novae.
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Affiliation(s)
- C Ruiz
- TRIUMF, Vancouver, BC V6T 2A3, Canada.
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Davids B, Anthony DW, Aumann T, Austin SM, Baumann T, Bazin D, Clement RR, Davids CN, Esbensen H, Lofy PA, Nakamura T, Sherrill BM, Yurkon J. S17(0) determined from the Coulomb breakup of 83 MeV /nucleon 8B. Phys Rev Lett 2001; 86:2750-2753. [PMID: 11290030 DOI: 10.1103/physrevlett.86.2750] [Citation(s) in RCA: 1] [Impact Index Per Article: 0.0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 09/08/2000] [Indexed: 05/23/2023]
Abstract
A kinematically complete measurement was made of the Coulomb dissociation of 8B nuclei on a Pb target at 83 MeV/nucleon. The cross section was measured at low relative energies in order to infer the astrophysical S factor for the 7Be(p,gamma)8B reaction. A first-order perturbation theory analysis including E1, E2, and M1 transitions was employed to extract the E1 strength relevant to neutrino-producing reactions in the solar interior. By fitting the measured cross section from E(rel) = 130 to 400 keV, we find S17(0) = 17.8(+1.4)(-1.2) eV b.
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Affiliation(s)
- B Davids
- National Superconducting Cyclotron Laboratory, Michigan State University, East Lansing, MI 48824, USA.
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Aumann T, Navin A, Balamuth DP, Bazin D, Blank B, Brown BA, Bush JE, Caggiano JA, Davids B, Glasmacher T, Guimaraes V, Hansen PG, Ibbotson RW, Karnes D, Kolata JJ, Maddalena V, Pritychenko B, Scheit H, Sherrill BM, Tostevin JA. One-neutron knockout from individual single-particle states of 11Be. Phys Rev Lett 2000; 84:35-38. [PMID: 11015828 DOI: 10.1103/physrevlett.84.35] [Citation(s) in RCA: 4] [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] [Received: 06/01/1999] [Indexed: 05/23/2023]
Abstract
The structure of the halo nucleus 11Be has been studied using the reaction 9Be(11Be,10Be+gamma)X at 60 MeV/nucleon. The ground state structure of 11Be is determined by comparing the experimental cross sections to a calculation combining spectroscopic factors from the shell model with l-dependent single-particle cross sections obtained in an eikonal model. This experiment shows the dominant 1s single-particle character of the 11Be ground state and indicates a small contribution of 0d admixture in the wave function. After correction for the approximately 22% intensity to excited levels, a clean and precise distribution of parallel momentum for knockout from the 1s halo wave function is obtained for the first time.
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Affiliation(s)
- T Aumann
- National Superconducting Cyclotron Laboratory, Michigan State University, East Lansing, Michigan 48824 and Gesellschaft fur Schwerionenforschung, Planckstrasse 1, 64291 Darmstadt, Germany
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Collon P, Cole D, Davids B, Fauerbachs M, Harkewicz R, Kutschera W, Morrissey DJ, Pardo RC, Paul M, Sherrill BM, Steiner M. Measurement of the Long-lived Radionuclide 81Kr in Pre-nuclear and Present-day Atmospheric Krypton. ACTA ACUST UNITED AC 1999. [DOI: 10.1524/ract.1999.85.12.13] [Citation(s) in RCA: 9] [Impact Index Per Article: 0.4] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/24/2022]
Affiliation(s)
- P. Collon
- Vienna Environmental Research Accelerator, Institut für Radiumforschung und Kernphysik, Universität Wien, Währingerstr. 17, A-1090 Wien, Austria
| | - D. Cole
- National Superconducting Cyclotron Laboratory, Michigan State University, East Lansing, Michigan 48824, USA
| | - B. Davids
- National Superconducting Cyclotron Laboratory, Michigan State University, East Lansing, Michigan 48824, USA
| | - M. Fauerbachs
- National Superconducting Cyclotron Laboratory, Michigan State University, East Lansing, Michigan 48824, USA
| | - R. Harkewicz
- National Superconducting Cyclotron Laboratory, Michigan State University, East Lansing, Michigan 48824, USA
| | | | - D. J. Morrissey
- National Superconducting Cyclotron Laboratory, Michigan State University, East Lansing, Michigan 48824, USA
| | - R. C. Pardo
- Physics Division, Argonne National Laboratory, Argonne, IL 60439, USA
| | - M. Paul
- Racah Institute for Physics, Hebrew University of Jerusalem, 91904 Jerusalem, Israel
| | - B. M. Sherrill
- National Superconducting Cyclotron Laboratory, Michigan State University, East Lansing, Michigan 48824, USA
| | - M. Steiner
- National Superconducting Cyclotron Laboratory, Michigan State University, East Lansing, Michigan 48824, USA
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Abstract
Magnetic resonance imaging of the brain was undertaken in women with obsessive-compulsive disorder (n = 13), trichotillomania (n = 17), and healthy controls (n = 12). Caudate volume and ventricular-brain ratio (VBR) (variables that have previously been highlighted as abnormal in studies of OCD) were compared in the three subject groups and were correlated with neuropsychological and neurological soft sign findings. No significant differences were found between women with OCD, trichotillomania and normal controls on caudate volume or VBR. Decreased left caudate volume was significantly correlated with impairment on neuropsychological testing and with increased neurological soft signs. The negative findings here may indicate that in women with OCD and related disorders structural brain abnormalities are less obvious or less common than in men with these conditions, or they may reflect inadequate sensitivity of the brain measures employed.
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Affiliation(s)
- D J Stein
- Department of Psychiatry, University of Stellenbosch, Tygerberg, South Africa
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Davids B. [Direction of gene activity or gene action through other genes? A contribution to the research of melanosarcoma]. Med Welt 1968; 3:187-8. [PMID: 5728928] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [MESH Headings] [Subscribe] [Scholar Register] [Indexed: 01/16/2023]
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