1
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Habib AF, Manahan GG, Scherkl P, Heinemann T, Sutherland A, Altuiri R, Alotaibi BM, Litos M, Cary J, Raubenheimer T, Hemsing E, Hogan MJ, Rosenzweig JB, Williams PH, McNeil BWJ, Hidding B. Attosecond-Angstrom free-electron-laser towards the cold beam limit. Nat Commun 2023; 14:1054. [PMID: 36828817 PMCID: PMC9958197 DOI: 10.1038/s41467-023-36592-z] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [Track Full Text] [Figures] [Journal Information] [Subscribe] [Scholar Register] [Received: 03/30/2022] [Accepted: 02/08/2023] [Indexed: 02/26/2023] Open
Abstract
Electron beam quality is paramount for X-ray pulse production in free-electron-lasers (FELs). State-of-the-art linear accelerators (linacs) can deliver multi-GeV electron beams with sufficient quality for hard X-ray-FELs, albeit requiring km-scale setups, whereas plasma-based accelerators can produce multi-GeV electron beams on metre-scale distances, and begin to reach beam qualities sufficient for EUV FELs. Here we show, that electron beams from plasma photocathodes many orders of magnitude brighter than state-of-the-art can be generated in plasma wakefield accelerators (PWFAs), and then extracted, captured, transported and injected into undulators without significant quality loss. These ultrabright, sub-femtosecond electron beams can drive hard X-FELs near the cold beam limit to generate coherent X-ray pulses of attosecond-Angstrom class, reaching saturation after only 10 metres of undulator. This plasma-X-FEL opens pathways for advanced photon science capabilities, such as unperturbed observation of electronic motion inside atoms at their natural time and length scale, and towards higher photon energies.
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Affiliation(s)
- A. F. Habib
- grid.11984.350000000121138138Department of Physics, Scottish Universities Physics Alliance, University of Strathclyde, Glasgow, UK ,grid.450757.40000 0004 6085 4374The Cockcroft Institute, Daresbury, UK
| | - G. G. Manahan
- grid.11984.350000000121138138Department of Physics, Scottish Universities Physics Alliance, University of Strathclyde, Glasgow, UK ,grid.450757.40000 0004 6085 4374The Cockcroft Institute, Daresbury, UK
| | - P. Scherkl
- grid.11984.350000000121138138Department of Physics, Scottish Universities Physics Alliance, University of Strathclyde, Glasgow, UK ,grid.450757.40000 0004 6085 4374The Cockcroft Institute, Daresbury, UK ,grid.9026.d0000 0001 2287 2617University Medical Center Hamburg-Eppendorf, University of Hamburg, 20246 Hamburg, Germany
| | - T. Heinemann
- grid.11984.350000000121138138Department of Physics, Scottish Universities Physics Alliance, University of Strathclyde, Glasgow, UK ,grid.450757.40000 0004 6085 4374The Cockcroft Institute, Daresbury, UK
| | - A. Sutherland
- grid.11984.350000000121138138Department of Physics, Scottish Universities Physics Alliance, University of Strathclyde, Glasgow, UK ,grid.450757.40000 0004 6085 4374The Cockcroft Institute, Daresbury, UK
| | - R. Altuiri
- grid.11984.350000000121138138Department of Physics, Scottish Universities Physics Alliance, University of Strathclyde, Glasgow, UK ,grid.449346.80000 0004 0501 7602Physics Department, Princess Nourah Bint Abdulrahman University, Riyadh, Kingdom of Saudi Arabia
| | - B. M. Alotaibi
- grid.11984.350000000121138138Department of Physics, Scottish Universities Physics Alliance, University of Strathclyde, Glasgow, UK ,grid.449346.80000 0004 0501 7602Physics Department, Princess Nourah Bint Abdulrahman University, Riyadh, Kingdom of Saudi Arabia
| | - M. Litos
- grid.266190.a0000000096214564Department of Physics, Center for Integrated Plasma Studies, University of Colorado, Boulder, CO USA
| | - J. Cary
- grid.266190.a0000000096214564Department of Physics, Center for Integrated Plasma Studies, University of Colorado, Boulder, CO USA ,grid.448325.c0000 0004 0556 1325Tech-X Corporation, Boulder, USA
| | - T. Raubenheimer
- grid.445003.60000 0001 0725 7771SLAC National Accelerator Laboratory, Menlo Park, CA USA
| | - E. Hemsing
- grid.445003.60000 0001 0725 7771SLAC National Accelerator Laboratory, Menlo Park, CA USA
| | - M. J. Hogan
- grid.445003.60000 0001 0725 7771SLAC National Accelerator Laboratory, Menlo Park, CA USA
| | - J. B. Rosenzweig
- grid.19006.3e0000 0000 9632 6718Department of Physics and Astronomy, University of California Los Angeles, Los Angeles, CA USA
| | - P. H. Williams
- grid.450757.40000 0004 6085 4374The Cockcroft Institute, Daresbury, UK ,grid.482271.a0000 0001 0727 2226ASTeC, STFC Daresbury Laboratory, Warrington, UK
| | - B. W. J. McNeil
- grid.11984.350000000121138138Department of Physics, Scottish Universities Physics Alliance, University of Strathclyde, Glasgow, UK ,grid.450757.40000 0004 6085 4374The Cockcroft Institute, Daresbury, UK
| | - B. Hidding
- grid.11984.350000000121138138Department of Physics, Scottish Universities Physics Alliance, University of Strathclyde, Glasgow, UK ,grid.450757.40000 0004 6085 4374The Cockcroft Institute, Daresbury, UK ,grid.411327.20000 0001 2176 9917Institute for Laser and Plasma Physics, Heinrich Heine University Düsseldorf, Düsseldorf, Germany
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2
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Zgadzaj R, Silva T, Khudyakov VK, Sosedkin A, Allen J, Gessner S, Li Z, Litos M, Vieira J, Lotov KV, Hogan MJ, Yakimenko V, Downer MC. Dissipation of electron-beam-driven plasma wakes. Nat Commun 2020; 11:4753. [PMID: 32958741 PMCID: PMC7506535 DOI: 10.1038/s41467-020-18490-w] [Citation(s) in RCA: 8] [Impact Index Per Article: 2.0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [Grants] [Track Full Text] [Download PDF] [Figures] [Journal Information] [Subscribe] [Scholar Register] [Received: 08/16/2019] [Accepted: 08/24/2020] [Indexed: 11/09/2022] Open
Abstract
Metre-scale plasma wakefield accelerators have imparted energy gain approaching 10 gigaelectronvolts to single nano-Coulomb electron bunches. To reach useful average currents, however, the enormous energy density that the driver deposits into the wake must be removed efficiently between shots. Yet mechanisms by which wakes dissipate their energy into surrounding plasma remain poorly understood. Here, we report picosecond-time-resolved, grazing-angle optical shadowgraphic measurements and large-scale particle-in-cell simulations of ion channels emerging from broken wakes that electron bunches from the SLAC linac generate in tenuous lithium plasma. Measurements show the channel boundary expands radially at 1 million metres-per-second for over a nanosecond. Simulations show that ions and electrons that the original wake propels outward, carrying 90 percent of its energy, drive this expansion by impact-ionizing surrounding neutral lithium. The results provide a basis for understanding global thermodynamics of multi-GeV plasma accelerators, which underlie their viability for applications demanding high average beam current.
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Affiliation(s)
- Rafal Zgadzaj
- University of Texas at Austin, 1 University Station C1600, Austin, TX, 78712-1081, USA
| | - T Silva
- GoLP/Instituto de Plasmas e Fusão Nuclear-Laboratório Associado, Insituto Superior Técnico, Lisboa, Portugal
| | - V K Khudyakov
- Budker Institute of Nuclear Physics, 630090, Novosibirsk, Russia
- Novosibirsk State University, 630090, Novosibirsk, Russia
| | - A Sosedkin
- Budker Institute of Nuclear Physics, 630090, Novosibirsk, Russia
- Novosibirsk State University, 630090, Novosibirsk, Russia
| | - J Allen
- SLAC National Accelerator Laboratory, Menlo Park, CA, 94025, USA
| | - S Gessner
- SLAC National Accelerator Laboratory, Menlo Park, CA, 94025, USA
| | - Zhengyan Li
- University of Texas at Austin, 1 University Station C1600, Austin, TX, 78712-1081, USA
- Huazhong University of Science and Technology, Wuhan, China
| | - M Litos
- SLAC National Accelerator Laboratory, Menlo Park, CA, 94025, USA
- Center for Integrated Plasma Studies, University of Colorado Boulder, Boulder, CO, 80309, USA
| | - J Vieira
- GoLP/Instituto de Plasmas e Fusão Nuclear-Laboratório Associado, Insituto Superior Técnico, Lisboa, Portugal
| | - K V Lotov
- Budker Institute of Nuclear Physics, 630090, Novosibirsk, Russia
- Novosibirsk State University, 630090, Novosibirsk, Russia
| | - M J Hogan
- SLAC National Accelerator Laboratory, Menlo Park, CA, 94025, USA
| | - V Yakimenko
- SLAC National Accelerator Laboratory, Menlo Park, CA, 94025, USA
| | - M C Downer
- University of Texas at Austin, 1 University Station C1600, Austin, TX, 78712-1081, USA.
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3
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San Miguel Claveria P, Adli E, Amorim LD, An W, Clayton CE, Corde S, Gessner S, Hogan MJ, Joshi C, Kononenko O, Litos M, Lu W, Marsh KA, Mori WB, O'Shea B, Raj G, Storey D, Vafaei-Najafabadi N, White G, Xu X, Yakimenko V. Betatron radiation and emittance growth in plasma wakefield accelerators. Philos Trans A Math Phys Eng Sci 2019; 377:20180173. [PMID: 31230577 PMCID: PMC6602914 DOI: 10.1098/rsta.2018.0173] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [Grants] [Track Full Text] [Figures] [Subscribe] [Scholar Register] [Accepted: 03/20/2019] [Indexed: 06/09/2023]
Abstract
Beam-driven plasma wakefield acceleration (PWFA) has demonstrated significant progress during the past two decades of research. The new Facility for Advanced Accelerator Experimental Tests (FACET) II, currently under construction, will provide 10 GeV electron beams with unprecedented parameters for the next generation of PWFA experiments. In the context of the FACET II facility, we present simulation results on expected betatron radiation and its potential application to diagnose emittance preservation and hosing instability in the upcoming PWFA experiments. This article is part of the Theo Murphy meeting issue 'Directions in particle beam-driven plasma wakefield acceleration'.
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Affiliation(s)
- P. San Miguel Claveria
- LOA, ENSTA ParisTech, CNRS, Ecole Polytechnique, Institut Polytechnique de Paris, 91762 Palaiseau, France
| | - E. Adli
- University of Oslo, NO-0316 Oslo, Norway
| | - L. D. Amorim
- Stonybrook University, Stony Brook, NY 11794, USA
| | - W. An
- University of California Los Angeles, Los Angeles, CA 90095, USA
| | - C. E. Clayton
- University of California Los Angeles, Los Angeles, CA 90095, USA
| | - S. Corde
- LOA, ENSTA ParisTech, CNRS, Ecole Polytechnique, Institut Polytechnique de Paris, 91762 Palaiseau, France
| | | | - M. J. Hogan
- SLAC National Accelerator Laboratory, Menlo Park, CA 94025, USA
| | - C. Joshi
- University of California Los Angeles, Los Angeles, CA 90095, USA
| | - O. Kononenko
- LOA, ENSTA ParisTech, CNRS, Ecole Polytechnique, Institut Polytechnique de Paris, 91762 Palaiseau, France
| | - M. Litos
- University of Colorado Boulder, Boulder, CO 80309, USA
| | - W. Lu
- Tsinghua University, Beijing 10084, People's Republic of China
| | - K. A. Marsh
- University of California Los Angeles, Los Angeles, CA 90095, USA
| | - W. B. Mori
- University of California Los Angeles, Los Angeles, CA 90095, USA
| | - B. O'Shea
- SLAC National Accelerator Laboratory, Menlo Park, CA 94025, USA
| | - G. Raj
- LOA, ENSTA ParisTech, CNRS, Ecole Polytechnique, Institut Polytechnique de Paris, 91762 Palaiseau, France
| | - D. Storey
- SLAC National Accelerator Laboratory, Menlo Park, CA 94025, USA
| | | | - G. White
- SLAC National Accelerator Laboratory, Menlo Park, CA 94025, USA
| | - Xinlu Xu
- University of California Los Angeles, Los Angeles, CA 90095, USA
- SLAC National Accelerator Laboratory, Menlo Park, CA 94025, USA
| | - V. Yakimenko
- SLAC National Accelerator Laboratory, Menlo Park, CA 94025, USA
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4
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Vafaei-Najafabadi N, Amorim LD, Adli E, An W, Clarke CI, Clayton CE, Corde S, Gessner S, Green SZ, Hogan MJ, Joshi C, Kononenko O, Lindstrøm CA, Litos M, Lu W, Marsh KA, Mori WB, San Miguel Claveria P, O'Shea B, Raj G, Storey D, White G, Xu X, Yakimenko V. Producing multi-coloured bunches through beam-induced ionization injection in plasma wakefield accelerator. Philos Trans A Math Phys Eng Sci 2019; 377:20180184. [PMID: 31230576 PMCID: PMC6602915 DOI: 10.1098/rsta.2018.0184] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [Grants] [Track Full Text] [Subscribe] [Scholar Register] [Accepted: 03/20/2019] [Indexed: 06/09/2023]
Abstract
This paper discusses the properties of electron beams formed in plasma wakefield accelerators through ionization injection. In particular, the potential for generating a beam composed of co-located multi-colour beamlets is demonstrated in the case where the ionization is initiated by the evolving charge field of the drive beam itself. The physics of the processes of ionization and injection are explored through OSIRIS simulations. Experimental evidence showing similar features are presented from the data obtained in the E217 experiment at the FACET facility of the SLAC National Laboratory. This article is part of the Theo Murphy meeting issue 'Directions in particle beam-driven plasma wakefield acceleration'.
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Affiliation(s)
| | - L. D. Amorim
- Stony Brook University, Stony Brook, NY 11794, USA
| | - E. Adli
- University of Oslo, Oslo 0316, Norway
| | - W. An
- University of California Los Angeles, Los Angeles, CA 90095, USA
| | - C. I. Clarke
- SLAC National Accelerator Laboratory, Menlo Park, CA 94025, USA
| | - C. E. Clayton
- University of California Los Angeles, Los Angeles, CA 90095, USA
| | - S. Corde
- LOA, ENSTA ParisTech, CNRS, Ecole Polytechnique, Université Paris-Saclay, Palaiseau 91762, France
| | | | - S. Z. Green
- SLAC National Accelerator Laboratory, Menlo Park, CA 94025, USA
| | - M. J. Hogan
- SLAC National Accelerator Laboratory, Menlo Park, CA 94025, USA
| | - C. Joshi
- University of California Los Angeles, Los Angeles, CA 90095, USA
| | - O. Kononenko
- LOA, ENSTA ParisTech, CNRS, Ecole Polytechnique, Université Paris-Saclay, Palaiseau 91762, France
| | | | - M. Litos
- University of Colorado Boulder, Boulder, CO 80309, USA
| | - W. Lu
- Tsinghua University, Beijing 10084, People's Republic of China
| | - K. A. Marsh
- University of California Los Angeles, Los Angeles, CA 90095, USA
| | - W. B. Mori
- University of California Los Angeles, Los Angeles, CA 90095, USA
| | - P. San Miguel Claveria
- LOA, ENSTA ParisTech, CNRS, Ecole Polytechnique, Université Paris-Saclay, Palaiseau 91762, France
| | - B. O'Shea
- SLAC National Accelerator Laboratory, Menlo Park, CA 94025, USA
| | - G. Raj
- LOA, ENSTA ParisTech, CNRS, Ecole Polytechnique, Université Paris-Saclay, Palaiseau 91762, France
| | - D. Storey
- SLAC National Accelerator Laboratory, Menlo Park, CA 94025, USA
| | - G. White
- SLAC National Accelerator Laboratory, Menlo Park, CA 94025, USA
| | - Xinlu Xu
- University of California Los Angeles, Los Angeles, CA 90095, USA
| | - V. Yakimenko
- SLAC National Accelerator Laboratory, Menlo Park, CA 94025, USA
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5
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Lindstrøm CA, Adli E, Allen JM, An W, Beekman C, Clarke CI, Clayton CE, Corde S, Doche A, Frederico J, Gessner SJ, Green SZ, Hogan MJ, Joshi C, Litos M, Lu W, Marsh KA, Mori WB, O'Shea BD, Vafaei-Najafabadi N, Yakimenko V. Measurement of Transverse Wakefields Induced by a Misaligned Positron Bunch in a Hollow Channel Plasma Accelerator. Phys Rev Lett 2018; 120:124802. [PMID: 29694092 DOI: 10.1103/physrevlett.120.124802] [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: 11/07/2017] [Indexed: 06/08/2023]
Abstract
Hollow channel plasma wakefield acceleration is a proposed method to provide high acceleration gradients for electrons and positrons alike: a key to future lepton colliders. However, beams which are misaligned from the channel axis induce strong transverse wakefields, deflecting beams and reducing the collider luminosity. This undesirable consequence sets a tight constraint on the alignment accuracy of the beam propagating through the channel. Direct measurements of beam misalignment-induced transverse wakefields are therefore essential for designing mitigation strategies. We present the first quantitative measurements of transverse wakefields in a hollow plasma channel, induced by an off-axis 20 GeV positron bunch, and measured with another 20 GeV lower charge trailing positron probe bunch. The measurements are largely consistent with theory.
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Affiliation(s)
- C A Lindstrøm
- Department of Physics, University of Oslo, 0316 Oslo, Norway
| | - E Adli
- Department of Physics, University of Oslo, 0316 Oslo, Norway
| | - J M Allen
- SLAC National Accelerator Laboratory, Menlo Park, California 94025, USA
| | - W An
- Department of Electrical Engineering, University of California-Los Angeles, Los Angeles, California 90095, USA
| | - C Beekman
- LOA, ENSTA ParisTech, CNRS, Ecole Polytechnique, Université Paris-Saclay, 91762 Palaiseau, France
| | - C I Clarke
- SLAC National Accelerator Laboratory, Menlo Park, California 94025, USA
| | - C E Clayton
- Department of Electrical Engineering, University of California-Los Angeles, Los Angeles, California 90095, USA
| | - S Corde
- LOA, ENSTA ParisTech, CNRS, Ecole Polytechnique, Université Paris-Saclay, 91762 Palaiseau, France
| | - A Doche
- LOA, ENSTA ParisTech, CNRS, Ecole Polytechnique, Université Paris-Saclay, 91762 Palaiseau, France
| | - J Frederico
- SLAC National Accelerator Laboratory, Menlo Park, California 94025, USA
| | - S J Gessner
- SLAC National Accelerator Laboratory, Menlo Park, California 94025, USA
| | - S Z Green
- SLAC National Accelerator Laboratory, Menlo Park, California 94025, USA
| | - M J Hogan
- SLAC National Accelerator Laboratory, Menlo Park, California 94025, USA
| | - C Joshi
- Department of Electrical Engineering, University of California-Los Angeles, Los Angeles, California 90095, USA
| | - M Litos
- Department of Physics, University of Colorado Boulder, Boulder, Colorado 80309, USA
| | - W Lu
- IFSA Collaborative Innovation Center, Department of Engineering Physics, Tsinghua University, Beijing 100084, China
| | - K A Marsh
- Department of Electrical Engineering, University of California-Los Angeles, Los Angeles, California 90095, USA
| | - W B Mori
- Department of Physics and Astronomy, University of California-Los Angeles, Los Angeles, California 90095, USA
| | - B D O'Shea
- SLAC National Accelerator Laboratory, Menlo Park, California 94025, USA
| | - N Vafaei-Najafabadi
- Department of Electrical Engineering, University of California-Los Angeles, Los Angeles, California 90095, USA
| | - V Yakimenko
- SLAC National Accelerator Laboratory, Menlo Park, California 94025, USA
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6
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Clayton CE, Adli E, Allen J, An W, Clarke CI, Corde S, Frederico J, Gessner S, Green SZ, Hogan MJ, Joshi C, Litos M, Lu W, Marsh KA, Mori WB, Vafaei-Najafabadi N, Xu X, Yakimenko V. Self-mapping the longitudinal field structure of a nonlinear plasma accelerator cavity. Nat Commun 2016; 7:12483. [PMID: 27527569 PMCID: PMC4990705 DOI: 10.1038/ncomms12483] [Citation(s) in RCA: 16] [Impact Index Per Article: 2.0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Download PDF] [Figures] [Journal Information] [Subscribe] [Scholar Register] [Received: 02/20/2016] [Accepted: 07/05/2016] [Indexed: 11/09/2022] Open
Abstract
The preservation of emittance of the accelerating beam is the next challenge for plasma-based accelerators envisioned for future light sources and colliders. The field structure of a highly nonlinear plasma wake is potentially suitable for this purpose but has not been yet measured. Here we show that the longitudinal variation of the fields in a nonlinear plasma wakefield accelerator cavity produced by a relativistic electron bunch can be mapped using the bunch itself as a probe. We find that, for much of the cavity that is devoid of plasma electrons, the transverse force is constant longitudinally to within ±3% (r.m.s.). Moreover, comparison of experimental data and simulations has resulted in mapping of the longitudinal electric field of the unloaded wake up to 83 GV m(-1) to a similar degree of accuracy. These results bode well for high-gradient, high-efficiency acceleration of electron bunches while preserving their emittance in such a cavity.
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Affiliation(s)
- C E Clayton
- Department of Electrical Engineering, University of California Los Angeles, Los Angeles, California 90095, USA
| | - E Adli
- SLAC National Accelerator Laboratory, Menlo Park, California 94025, USA.,Department of Physics, University of Oslo, Oslo 0316, Norway
| | - J Allen
- SLAC National Accelerator Laboratory, Menlo Park, California 94025, USA
| | - W An
- Department of Electrical Engineering, University of California Los Angeles, Los Angeles, California 90095, USA.,Department of Physics and Astronomy, University of California Los Angeles, Los Angeles, California 90095, USA
| | - C I Clarke
- SLAC National Accelerator Laboratory, Menlo Park, California 94025, USA
| | - S Corde
- SLAC National Accelerator Laboratory, Menlo Park, California 94025, USA.,LOA, ENSTA ParisTech, CNRS, Ecole Polytechnique, Université Paris-Saclay, Palaiseau 91762, France
| | - J Frederico
- SLAC National Accelerator Laboratory, Menlo Park, California 94025, USA
| | - S Gessner
- SLAC National Accelerator Laboratory, Menlo Park, California 94025, USA
| | - S Z Green
- SLAC National Accelerator Laboratory, Menlo Park, California 94025, USA
| | - M J Hogan
- SLAC National Accelerator Laboratory, Menlo Park, California 94025, USA
| | - C Joshi
- Department of Electrical Engineering, University of California Los Angeles, Los Angeles, California 90095, USA
| | - M Litos
- SLAC National Accelerator Laboratory, Menlo Park, California 94025, USA
| | - W Lu
- Department of Engineering Physics, Tsinghua University, Beijing 100084, China
| | - K A Marsh
- Department of Electrical Engineering, University of California Los Angeles, Los Angeles, California 90095, USA
| | - W B Mori
- Department of Electrical Engineering, University of California Los Angeles, Los Angeles, California 90095, USA.,Department of Physics and Astronomy, University of California Los Angeles, Los Angeles, California 90095, USA
| | - N Vafaei-Najafabadi
- Department of Electrical Engineering, University of California Los Angeles, Los Angeles, California 90095, USA
| | - X Xu
- Department of Electrical Engineering, University of California Los Angeles, Los Angeles, California 90095, USA.,Department of Physics and Astronomy, University of California Los Angeles, Los Angeles, California 90095, USA
| | - V Yakimenko
- SLAC National Accelerator Laboratory, Menlo Park, California 94025, USA
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7
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Corde S, Adli E, Allen JM, An W, Clarke CI, Clayton CE, Delahaye JP, Frederico J, Gessner S, Green SZ, Hogan MJ, Joshi C, Lipkowitz N, Litos M, Lu W, Marsh KA, Mori WB, Schmeltz M, Vafaei-Najafabadi N, Walz D, Yakimenko V, Yocky G. Multi-gigaelectronvolt acceleration of positrons in a self-loaded plasma wakefield. Nature 2015; 524:442-5. [PMID: 26310764 DOI: 10.1038/nature14890] [Citation(s) in RCA: 112] [Impact Index Per Article: 12.4] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 03/29/2015] [Accepted: 06/30/2015] [Indexed: 11/09/2022]
Abstract
Electrical breakdown sets a limit on the kinetic energy that particles in a conventional radio-frequency accelerator can reach. New accelerator concepts must be developed to achieve higher energies and to make future particle colliders more compact and affordable. The plasma wakefield accelerator (PWFA) embodies one such concept, in which the electric field of a plasma wake excited by a bunch of charged particles (such as electrons) is used to accelerate a trailing bunch of particles. To apply plasma acceleration to electron-positron colliders, it is imperative that both the electrons and their antimatter counterpart, the positrons, are efficiently accelerated at high fields using plasmas. Although substantial progress has recently been reported on high-field, high-efficiency acceleration of electrons in a PWFA powered by an electron bunch, such an electron-driven wake is unsuitable for the acceleration and focusing of a positron bunch. Here we demonstrate a new regime of PWFAs where particles in the front of a single positron bunch transfer their energy to a substantial number of those in the rear of the same bunch by exciting a wakefield in the plasma. In the process, the accelerating field is altered--'self-loaded'--so that about a billion positrons gain five gigaelectronvolts of energy with a narrow energy spread over a distance of just 1.3 metres. They extract about 30 per cent of the wake's energy and form a spectrally distinct bunch with a root-mean-square energy spread as low as 1.8 per cent. This ability to transfer energy efficiently from the front to the rear within a single positron bunch makes the PWFA scheme very attractive as an energy booster to an electron-positron collider.
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Affiliation(s)
- S Corde
- SLAC National Accelerator Laboratory, Menlo Park, California 94025, USA.,LOA, ENSTA ParisTech, CNRS, Ecole Polytechnique, Université Paris-Saclay, 91762 Palaiseau, France
| | - E Adli
- SLAC National Accelerator Laboratory, Menlo Park, California 94025, USA.,Department of Physics, University of Oslo, 0316 Oslo, Norway
| | - J M Allen
- SLAC National Accelerator Laboratory, Menlo Park, California 94025, USA
| | - W An
- Department of Electrical Engineering, University of California Los Angeles, Los Angeles, California 90095, USA.,Department of Physics and Astronomy, University of California Los Angeles, Los Angeles, California 90095, USA
| | - C I Clarke
- SLAC National Accelerator Laboratory, Menlo Park, California 94025, USA
| | - C E Clayton
- Department of Electrical Engineering, University of California Los Angeles, Los Angeles, California 90095, USA
| | - J P Delahaye
- SLAC National Accelerator Laboratory, Menlo Park, California 94025, USA
| | - J Frederico
- SLAC National Accelerator Laboratory, Menlo Park, California 94025, USA
| | - S Gessner
- SLAC National Accelerator Laboratory, Menlo Park, California 94025, USA
| | - S Z Green
- SLAC National Accelerator Laboratory, Menlo Park, California 94025, USA
| | - M J Hogan
- SLAC National Accelerator Laboratory, Menlo Park, California 94025, USA
| | - C Joshi
- Department of Electrical Engineering, University of California Los Angeles, Los Angeles, California 90095, USA
| | - N Lipkowitz
- SLAC National Accelerator Laboratory, Menlo Park, California 94025, USA
| | - M Litos
- SLAC National Accelerator Laboratory, Menlo Park, California 94025, USA
| | - W Lu
- Department of Engineering Physics, Tsinghua University, Beijing 100084, China
| | - K A Marsh
- Department of Electrical Engineering, University of California Los Angeles, Los Angeles, California 90095, USA
| | - W B Mori
- Department of Electrical Engineering, University of California Los Angeles, Los Angeles, California 90095, USA.,Department of Physics and Astronomy, University of California Los Angeles, Los Angeles, California 90095, USA
| | - M Schmeltz
- SLAC National Accelerator Laboratory, Menlo Park, California 94025, USA
| | - N Vafaei-Najafabadi
- Department of Electrical Engineering, University of California Los Angeles, Los Angeles, California 90095, USA
| | - D Walz
- SLAC National Accelerator Laboratory, Menlo Park, California 94025, USA
| | - V Yakimenko
- SLAC National Accelerator Laboratory, Menlo Park, California 94025, USA
| | - G Yocky
- SLAC National Accelerator Laboratory, Menlo Park, California 94025, USA
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8
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Abe K, Hayato Y, Iida T, Ishihara K, Kameda J, Koshio Y, Minamino A, Mitsuda C, Miura M, Moriyama S, Nakahata M, Obayashi Y, Ogawa H, Sekiya H, Shiozawa M, Suzuki Y, Takeda A, Takeuchi Y, Ueshima K, Watanabe H, Higuchi I, Ishihara C, Ishitsuka M, Kajita T, Kaneyuki K, Mitsuka G, Nakayama S, Nishino H, Okumura K, Saji C, Takenaga Y, Clark S, Desai S, Dufour F, Herfurth A, Kearns E, Likhoded S, Litos M, Raaf J, Stone J, Sulak L, Wang W, Goldhaber M, Casper D, Cravens J, Dunmore J, Griskevich J, Kropp W, Liu D, Mine S, Regis C, Smy M, Sobel H, Vagins M, Ganezer K, Hartfiel B, Hill J, Keig W, Jang J, Jeoung I, Kim J, Lim I, Scholberg K, Tanimoto N, Walter C, Wendell R, Ellsworth R, Tasaka S, Guillian G, Learned J, Matsuno S, Messier M, Ichikawa A, Ishida T, Ishii T, Iwashita T, Kobayashi T, Nakadaira T, Nakamura K, Nishikawa K, Nitta K, Oyama Y, Suzuki A, Hasegawa M, Maesaka H, Nakaya T, Sasaki T, Sato H, Tanaka H, Yamamoto S, Yokoyama M, Haines T, Dazeley S, Hatakeyama S, Svoboda R, Sullivan G, Gran R, Habig A, Fukuda Y, Itow Y, Koike T, Jung C, Kato T, Kobayashi K, McGrew C, Sarrat A, Terri R, Yanagisawa C, Tamura N, Ikeda M, Sakuda M, Kuno Y, Yoshida M, Kim S, Yang B, Ishizuka T, Okazawa H, Choi Y, Seo H, Gando Y, Hasegawa T, Inoue K, Ishii H, Nishijima K, Ishino H, Watanabe Y, Koshiba M, Totsuka Y, Chen S, Deng Z, Liu Y, Kielczewska D, Berns H, Shiraishi K, Thrane E, Washburn K, Wilkes R. Search forn−n¯oscillation in Super-Kamiokande. Int J Clin Exp Med 2015. [DOI: 10.1103/physrevd.91.072006] [Citation(s) in RCA: 66] [Impact Index Per Article: 7.3] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/07/2022]
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9
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Litos M, Adli E, An W, Clarke CI, Clayton CE, Corde S, Delahaye JP, England RJ, Fisher AS, Frederico J, Gessner S, Green SZ, Hogan MJ, Joshi C, Lu W, Marsh KA, Mori WB, Muggli P, Vafaei-Najafabadi N, Walz D, White G, Wu Z, Yakimenko V, Yocky G. High-efficiency acceleration of an electron beam in a plasma wakefield accelerator. Nature 2014; 515:92-5. [DOI: 10.1038/nature13882] [Citation(s) in RCA: 346] [Impact Index Per Article: 34.6] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 07/20/2014] [Accepted: 09/01/2014] [Indexed: 11/09/2022]
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10
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Abe K, Hayato Y, Iida T, Iyogi K, Kameda J, Koshio Y, Kozuma Y, Marti L, Miura M, Moriyama S, Nakahata M, Nakayama S, Obayashi Y, Sekiya H, Shiozawa M, Suzuki Y, Takeda A, Takenaga Y, Ueno K, Ueshima K, Yamada S, Yokozawa T, Ishihara C, Kaji H, Kajita T, Kaneyuki K, Lee KP, McLachlan T, Okumura K, Shimizu Y, Tanimoto N, Labarga L, Kearns E, Litos M, Raaf JL, Stone JL, Sulak LR, Goldhaber M, Bays K, Kropp WR, Mine S, Regis C, Renshaw A, Smy MB, Sobel HW, Ganezer KS, Hill J, Keig WE, Jang JS, Kim JY, Lim IT, Albert JB, Scholberg K, Walter CW, Wendell R, Wongjirad TM, Ishizuka T, Tasaka S, Learned JG, Matsuno S, Smith SN, Hasegawa T, Ishida T, Ishii T, Kobayashi T, Nakadaira T, Nakamura K, Nishikawa K, Oyama Y, Sakashita K, Sekiguchi T, Tsukamoto T, Suzuki AT, Takeuchi Y, Ikeda M, Minamino A, Nakaya T, Fukuda Y, Itow Y, Mitsuka G, Tanaka T, Jung CK, Lopez GD, Taylor I, Yanagisawa C, Ishino H, Kibayashi A, Mino S, Mori T, Sakuda M, Toyota H, Kuno Y, Yoshida M, Kim SB, Yang BS, Okazawa H, Choi Y, Nishijima K, Koshiba M, Yokoyama M, Totsuka Y, Martens K, Schuemann J, Vagins MR, Chen S, Heng Y, Yang Z, Zhang H, Kielczewska D, Mijakowski P, Connolly K, Dziomba M, Thrane E, Wilkes RJ. Search for nucleon decay via n→ν[over ¯]π0 and p→ν[over ¯]π+ in Super-Kamiokande. Phys Rev Lett 2014; 113:121802. [PMID: 25279622 DOI: 10.1103/physrevlett.113.121802] [Citation(s) in RCA: 7] [Impact Index Per Article: 0.7] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 05/21/2013] [Indexed: 06/03/2023]
Abstract
We present the results of searches for nucleon decay via n→ν[over ¯]π0 and p→ν[over ¯]π+ using data from a combined 172.8 kt·yr exposure of Super-Kamiokande-I,-II, and-III. We set lower limits on the partial lifetime for each of these modes: τn→ν[over ¯]π0>1.1×10(33) years and τp→ν[over ¯]π+>3.9×10(32) years at a 90% confidence level.
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Affiliation(s)
- K Abe
- Kamioka Observatory, Institute for Cosmic Ray Research, University of Tokyo, Kamioka, Gifu 506-1205, Japan and Kavli Institute for the Physics and Mathematics of the Universe (WPI), Todai Institutes for Advanced Study, University of Tokyo, Kashiwa, Chiba 277-8583, Japan
| | - Y Hayato
- Kamioka Observatory, Institute for Cosmic Ray Research, University of Tokyo, Kamioka, Gifu 506-1205, Japan and Kavli Institute for the Physics and Mathematics of the Universe (WPI), Todai Institutes for Advanced Study, University of Tokyo, Kashiwa, Chiba 277-8583, Japan
| | - T Iida
- Kamioka Observatory, Institute for Cosmic Ray Research, University of Tokyo, Kamioka, Gifu 506-1205, Japan
| | - K Iyogi
- Kamioka Observatory, Institute for Cosmic Ray Research, University of Tokyo, Kamioka, Gifu 506-1205, Japan
| | - J Kameda
- Kamioka Observatory, Institute for Cosmic Ray Research, University of Tokyo, Kamioka, Gifu 506-1205, Japan and Kavli Institute for the Physics and Mathematics of the Universe (WPI), Todai Institutes for Advanced Study, University of Tokyo, Kashiwa, Chiba 277-8583, Japan
| | - Y Koshio
- Kamioka Observatory, Institute for Cosmic Ray Research, University of Tokyo, Kamioka, Gifu 506-1205, Japan and Kavli Institute for the Physics and Mathematics of the Universe (WPI), Todai Institutes for Advanced Study, University of Tokyo, Kashiwa, Chiba 277-8583, Japan
| | - Y Kozuma
- Kamioka Observatory, Institute for Cosmic Ray Research, University of Tokyo, Kamioka, Gifu 506-1205, Japan
| | - Ll Marti
- Kamioka Observatory, Institute for Cosmic Ray Research, University of Tokyo, Kamioka, Gifu 506-1205, Japan
| | - M Miura
- Kamioka Observatory, Institute for Cosmic Ray Research, University of Tokyo, Kamioka, Gifu 506-1205, Japan and Kavli Institute for the Physics and Mathematics of the Universe (WPI), Todai Institutes for Advanced Study, University of Tokyo, Kashiwa, Chiba 277-8583, Japan
| | - S Moriyama
- Kamioka Observatory, Institute for Cosmic Ray Research, University of Tokyo, Kamioka, Gifu 506-1205, Japan and Kavli Institute for the Physics and Mathematics of the Universe (WPI), Todai Institutes for Advanced Study, University of Tokyo, Kashiwa, Chiba 277-8583, Japan
| | - M Nakahata
- Kamioka Observatory, Institute for Cosmic Ray Research, University of Tokyo, Kamioka, Gifu 506-1205, Japan and Kavli Institute for the Physics and Mathematics of the Universe (WPI), Todai Institutes for Advanced Study, University of Tokyo, Kashiwa, Chiba 277-8583, Japan
| | - S Nakayama
- Kamioka Observatory, Institute for Cosmic Ray Research, University of Tokyo, Kamioka, Gifu 506-1205, Japan and Kavli Institute for the Physics and Mathematics of the Universe (WPI), Todai Institutes for Advanced Study, University of Tokyo, Kashiwa, Chiba 277-8583, Japan
| | - Y Obayashi
- Kamioka Observatory, Institute for Cosmic Ray Research, University of Tokyo, Kamioka, Gifu 506-1205, Japan and Kavli Institute for the Physics and Mathematics of the Universe (WPI), Todai Institutes for Advanced Study, University of Tokyo, Kashiwa, Chiba 277-8583, Japan
| | - H Sekiya
- Kamioka Observatory, Institute for Cosmic Ray Research, University of Tokyo, Kamioka, Gifu 506-1205, Japan and Kavli Institute for the Physics and Mathematics of the Universe (WPI), Todai Institutes for Advanced Study, University of Tokyo, Kashiwa, Chiba 277-8583, Japan
| | - M Shiozawa
- Kamioka Observatory, Institute for Cosmic Ray Research, University of Tokyo, Kamioka, Gifu 506-1205, Japan and Kavli Institute for the Physics and Mathematics of the Universe (WPI), Todai Institutes for Advanced Study, University of Tokyo, Kashiwa, Chiba 277-8583, Japan
| | - Y Suzuki
- Kamioka Observatory, Institute for Cosmic Ray Research, University of Tokyo, Kamioka, Gifu 506-1205, Japan and Kavli Institute for the Physics and Mathematics of the Universe (WPI), Todai Institutes for Advanced Study, University of Tokyo, Kashiwa, Chiba 277-8583, Japan
| | - A Takeda
- Kamioka Observatory, Institute for Cosmic Ray Research, University of Tokyo, Kamioka, Gifu 506-1205, Japan and Kavli Institute for the Physics and Mathematics of the Universe (WPI), Todai Institutes for Advanced Study, University of Tokyo, Kashiwa, Chiba 277-8583, Japan
| | - Y Takenaga
- Kamioka Observatory, Institute for Cosmic Ray Research, University of Tokyo, Kamioka, Gifu 506-1205, Japan
| | - K Ueno
- Kamioka Observatory, Institute for Cosmic Ray Research, University of Tokyo, Kamioka, Gifu 506-1205, Japan
| | - K Ueshima
- Kamioka Observatory, Institute for Cosmic Ray Research, University of Tokyo, Kamioka, Gifu 506-1205, Japan
| | - S Yamada
- Kamioka Observatory, Institute for Cosmic Ray Research, University of Tokyo, Kamioka, Gifu 506-1205, Japan
| | - T Yokozawa
- Kamioka Observatory, Institute for Cosmic Ray Research, University of Tokyo, Kamioka, Gifu 506-1205, Japan
| | - C Ishihara
- Research Center for Cosmic Neutrinos, Institute for Cosmic Ray Research, University of Tokyo, Kashiwa, Chiba 277-8582, Japan
| | - H Kaji
- Research Center for Cosmic Neutrinos, Institute for Cosmic Ray Research, University of Tokyo, Kashiwa, Chiba 277-8582, Japan
| | - T Kajita
- Research Center for Cosmic Neutrinos, Institute for Cosmic Ray Research, University of Tokyo, Kashiwa, Chiba 277-8582, Japan and Kavli Institute for the Physics and Mathematics of the Universe (WPI), Todai Institutes for Advanced Study, University of Tokyo, Kashiwa, Chiba 277-8583, Japan
| | - K Kaneyuki
- Research Center for Cosmic Neutrinos, Institute for Cosmic Ray Research, University of Tokyo, Kashiwa, Chiba 277-8582, Japan and Kavli Institute for the Physics and Mathematics of the Universe (WPI), Todai Institutes for Advanced Study, University of Tokyo, Kashiwa, Chiba 277-8583, Japan
| | - K P Lee
- Research Center for Cosmic Neutrinos, Institute for Cosmic Ray Research, University of Tokyo, Kashiwa, Chiba 277-8582, Japan
| | - T McLachlan
- Research Center for Cosmic Neutrinos, Institute for Cosmic Ray Research, University of Tokyo, Kashiwa, Chiba 277-8582, Japan
| | - K Okumura
- Research Center for Cosmic Neutrinos, Institute for Cosmic Ray Research, University of Tokyo, Kashiwa, Chiba 277-8582, Japan
| | - Y Shimizu
- Research Center for Cosmic Neutrinos, Institute for Cosmic Ray Research, University of Tokyo, Kashiwa, Chiba 277-8582, Japan
| | - N Tanimoto
- Research Center for Cosmic Neutrinos, Institute for Cosmic Ray Research, University of Tokyo, Kashiwa, Chiba 277-8582, Japan
| | - L Labarga
- Department of Theoretical Physics, University Autonoma Madrid, 28049 Madrid, Spain
| | - E Kearns
- Department of Physics, Boston University, Boston, Massachusetts 02215, USA and Kavli Institute for the Physics and Mathematics of the Universe (WPI), Todai Institutes for Advanced Study, University of Tokyo, Kashiwa, Chiba 277-8583, Japan
| | - M Litos
- Department of Physics, Boston University, Boston, Massachusetts 02215, USA
| | - J L Raaf
- Department of Physics, Boston University, Boston, Massachusetts 02215, USA
| | - J L Stone
- Department of Physics, Boston University, Boston, Massachusetts 02215, USA and Kavli Institute for the Physics and Mathematics of the Universe (WPI), Todai Institutes for Advanced Study, University of Tokyo, Kashiwa, Chiba 277-8583, Japan
| | - L R Sulak
- Department of Physics, Boston University, Boston, Massachusetts 02215, USA
| | - M Goldhaber
- Physics Department, Brookhaven National Laboratory, Upton, New York 11973, USA
| | - K Bays
- Department of Physics and Astronomy, University of California, Irvine, Irvine, California 92697-4575, USA
| | - W R Kropp
- Department of Physics and Astronomy, University of California, Irvine, Irvine, California 92697-4575, USA
| | - S Mine
- Department of Physics and Astronomy, University of California, Irvine, Irvine, California 92697-4575, USA
| | - C Regis
- Department of Physics and Astronomy, University of California, Irvine, Irvine, California 92697-4575, USA
| | - A Renshaw
- Department of Physics and Astronomy, University of California, Irvine, Irvine, California 92697-4575, USA
| | - M B Smy
- Department of Physics and Astronomy, University of California, Irvine, Irvine, California 92697-4575, USA and Kavli Institute for the Physics and Mathematics of the Universe (WPI), Todai Institutes for Advanced Study, University of Tokyo, Kashiwa, Chiba 277-8583, Japan
| | - H W Sobel
- Department of Physics and Astronomy, University of California, Irvine, Irvine, California 92697-4575, USA and Kavli Institute for the Physics and Mathematics of the Universe (WPI), Todai Institutes for Advanced Study, University of Tokyo, Kashiwa, Chiba 277-8583, Japan
| | - K S Ganezer
- Department of Physics, California State University, Dominguez Hills, Carson, California 90747, USA
| | - J Hill
- Department of Physics, California State University, Dominguez Hills, Carson, California 90747, USA
| | - W E Keig
- Department of Physics, California State University, Dominguez Hills, Carson, California 90747, USA
| | - J S Jang
- Department of Physics, Chonnam National University, Kwangju 500-757, Korea
| | - J Y Kim
- Department of Physics, Chonnam National University, Kwangju 500-757, Korea
| | - I T Lim
- Department of Physics, Chonnam National University, Kwangju 500-757, Korea
| | - J B Albert
- Department of Physics, Duke University, Durham, North Carolina 27708, USA
| | - K Scholberg
- Department of Physics, Duke University, Durham, North Carolina 27708, USA and Kavli Institute for the Physics and Mathematics of the Universe (WPI), Todai Institutes for Advanced Study, University of Tokyo, Kashiwa, Chiba 277-8583, Japan
| | - C W Walter
- Department of Physics, Duke University, Durham, North Carolina 27708, USA and Kavli Institute for the Physics and Mathematics of the Universe (WPI), Todai Institutes for Advanced Study, University of Tokyo, Kashiwa, Chiba 277-8583, Japan
| | - R Wendell
- Department of Physics, Duke University, Durham, North Carolina 27708, USA
| | - T M Wongjirad
- Department of Physics, Duke University, Durham, North Carolina 27708, USA
| | - T Ishizuka
- Junior College, Fukuoka Institute of Technology, Fukuoka 811-0214, Japan
| | - S Tasaka
- Information and Multimedia Center, Gifu University, Gifu, Gifu 501-1193, Japan
| | - J G Learned
- Department of Physics and Astronomy, University of Hawaii, Honolulu, Hawaii 96822, USA
| | - S Matsuno
- Department of Physics and Astronomy, University of Hawaii, Honolulu, Hawaii 96822, USA
| | - S N Smith
- Department of Physics and Astronomy, University of Hawaii, Honolulu, Hawaii 96822, USA
| | - T Hasegawa
- High Energy Accelerator Research Organization (KEK), Tsukuba, Ibaraki 305-0801, Japan
| | - T Ishida
- High Energy Accelerator Research Organization (KEK), Tsukuba, Ibaraki 305-0801, Japan
| | - T Ishii
- High Energy Accelerator Research Organization (KEK), Tsukuba, Ibaraki 305-0801, Japan
| | - T Kobayashi
- High Energy Accelerator Research Organization (KEK), Tsukuba, Ibaraki 305-0801, Japan
| | - T Nakadaira
- High Energy Accelerator Research Organization (KEK), Tsukuba, Ibaraki 305-0801, Japan
| | - K Nakamura
- High Energy Accelerator Research Organization (KEK), Tsukuba, Ibaraki 305-0801, Japan and Kavli Institute for the Physics and Mathematics of the Universe (WPI), Todai Institutes for Advanced Study, University of Tokyo, Kashiwa, Chiba 277-8583, Japan
| | - K Nishikawa
- High Energy Accelerator Research Organization (KEK), Tsukuba, Ibaraki 305-0801, Japan
| | - Y Oyama
- High Energy Accelerator Research Organization (KEK), Tsukuba, Ibaraki 305-0801, Japan
| | - K Sakashita
- High Energy Accelerator Research Organization (KEK), Tsukuba, Ibaraki 305-0801, Japan
| | - T Sekiguchi
- High Energy Accelerator Research Organization (KEK), Tsukuba, Ibaraki 305-0801, Japan
| | - T Tsukamoto
- High Energy Accelerator Research Organization (KEK), Tsukuba, Ibaraki 305-0801, Japan
| | - A T Suzuki
- Department of Physics, Kobe University, Kobe, Hyogo 657-8501, Japan
| | - Y Takeuchi
- Department of Physics, Kobe University, Kobe, Hyogo 657-8501, Japan and Kavli Institute for the Physics and Mathematics of the Universe (WPI), Todai Institutes for Advanced Study, University of Tokyo, Kashiwa, Chiba 277-8583, Japan
| | - M Ikeda
- Department of Physics, Kyoto University, Kyoto, Kyoto 606-8502, Japan
| | - A Minamino
- Department of Physics, Kyoto University, Kyoto, Kyoto 606-8502, Japan
| | - T Nakaya
- Department of Physics, Kyoto University, Kyoto, Kyoto 606-8502, Japan and Kavli Institute for the Physics and Mathematics of the Universe (WPI), Todai Institutes for Advanced Study, University of Tokyo, Kashiwa, Chiba 277-8583, Japan
| | - Y Fukuda
- Department of Physics, Miyagi University of Education, Sendai, Miyagi 980-0845, Japan
| | - Y Itow
- Solar Terrestrial Environment Laboratory, Nagoya University, Nagoya, Aichi 464-8602, Japan and Kobayashi-Maskawa Institute for the Origin of Particles and the Universe, Nagoya University, Nagoya, Aichi 464-8602, Japan
| | - G Mitsuka
- Solar Terrestrial Environment Laboratory, Nagoya University, Nagoya, Aichi 464-8602, Japan
| | - T Tanaka
- Solar Terrestrial Environment Laboratory, Nagoya University, Nagoya, Aichi 464-8602, Japan
| | - C K Jung
- Department of Physics and Astronomy, State University of New York, Stony Brook, New York 11794-3800, USA
| | - G D Lopez
- Department of Physics and Astronomy, State University of New York, Stony Brook, New York 11794-3800, USA
| | - I Taylor
- Department of Physics and Astronomy, State University of New York, Stony Brook, New York 11794-3800, USA
| | - C Yanagisawa
- Department of Physics and Astronomy, State University of New York, Stony Brook, New York 11794-3800, USA
| | - H Ishino
- Department of Physics, Okayama University, Okayama, Okayama 700-8530, Japan
| | - A Kibayashi
- Department of Physics, Okayama University, Okayama, Okayama 700-8530, Japan
| | - S Mino
- Department of Physics, Okayama University, Okayama, Okayama 700-8530, Japan
| | - T Mori
- Department of Physics, Okayama University, Okayama, Okayama 700-8530, Japan
| | - M Sakuda
- Department of Physics, Okayama University, Okayama, Okayama 700-8530, Japan
| | - H Toyota
- Department of Physics, Okayama University, Okayama, Okayama 700-8530, Japan
| | - Y Kuno
- Department of Physics, Osaka University, Toyonaka, Osaka 560-0043, Japan
| | - M Yoshida
- Department of Physics, Osaka University, Toyonaka, Osaka 560-0043, Japan
| | - S B Kim
- Department of Physics, Seoul National University, Seoul 151-742, Korea
| | - B S Yang
- Department of Physics, Seoul National University, Seoul 151-742, Korea
| | - H Okazawa
- Department of Informatics in Social Welfare, Shizuoka University of Welfare, Yaizu, Shizuoka, 425-8611, Japan
| | - Y Choi
- Department of Physics, Sungkyunkwan University, Suwon 440-746, Korea
| | - K Nishijima
- Department of Physics, Tokai University, Hiratsuka, Kanagawa 259-1292, Japan
| | - M Koshiba
- The University of Tokyo, Bunkyo, Tokyo 113-0033, Japan
| | - M Yokoyama
- The University of Tokyo, Bunkyo, Tokyo 113-0033, Japan and Kavli Institute for the Physics and Mathematics of the Universe (WPI), Todai Institutes for Advanced Study, University of Tokyo, Kashiwa, Chiba 277-8583, Japan
| | - Y Totsuka
- The University of Tokyo, Bunkyo, Tokyo 113-0033, Japan
| | - K Martens
- Kavli Institute for the Physics and Mathematics of the Universe (WPI), Todai Institutes for Advanced Study, University of Tokyo, Kashiwa, Chiba 277-8583, Japan
| | - J Schuemann
- Kavli Institute for the Physics and Mathematics of the Universe (WPI), Todai Institutes for Advanced Study, University of Tokyo, Kashiwa, Chiba 277-8583, Japan
| | - M R Vagins
- Department of Physics and Astronomy, University of California, Irvine, Irvine, California 92697-4575, USA and Kavli Institute for the Physics and Mathematics of the Universe (WPI), Todai Institutes for Advanced Study, University of Tokyo, Kashiwa, Chiba 277-8583, Japan
| | - S Chen
- Department of Engineering Physics, Tsinghua University, Beijing 100084, China
| | - Y Heng
- Department of Engineering Physics, Tsinghua University, Beijing 100084, China
| | - Z Yang
- Department of Engineering Physics, Tsinghua University, Beijing 100084, China
| | - H Zhang
- Department of Engineering Physics, Tsinghua University, Beijing 100084, China
| | - D Kielczewska
- Institute of Experimental Physics, Warsaw University, 00-681 Warsaw, Poland
| | - P Mijakowski
- Institute of Experimental Physics, Warsaw University, 00-681 Warsaw, Poland
| | - K Connolly
- Department of Physics, University of Washington, Seattle, Washington 98195-1560, USA
| | - M Dziomba
- Department of Physics, University of Washington, Seattle, Washington 98195-1560, USA
| | - E Thrane
- Department of Physics, University of Washington, Seattle, Washington 98195-1560, USA
| | - R J Wilkes
- Department of Physics, University of Washington, Seattle, Washington 98195-1560, USA
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11
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Litos M, Abe K, Hayato Y, Iida T, Ikeda M, Iyogi K, Kameda J, Kobayashi K, Koshio Y, Kozuma Y, Miura M, Moriyama S, Nakahata M, Nakayama S, Obayashi Y, Ogawa H, Sekiya H, Shiozawa M, Suzuki Y, Takeda A, Takenaga Y, Takeuchi Y, Ueno K, Ueshima K, Watanabe H, Yamada S, Yokozawa T, Hazama S, Ishihara C, Kaji H, Kajita T, Kaneyuki K, McLachlan T, Okumura K, Shimizu Y, Tanimoto N, Vagins MR, Kearns E, Stone JL, Sulak LR, Dufour F, Raaf JL, Henning B, Goldhaber M, Bays K, Casper D, Cravens JP, Kropp WR, Mine S, Regis C, Smy MB, Sobel HW, Ganezer KS, Hill J, Keig WE, Jang JS, Kim JY, Lim IT, Albert JB, Wongjirad T, Wendell R, Scholberg K, Walter CW, Tasaka S, Learned JG, Matsuno S, Watanabe Y, Hasegawa T, Ishida T, Ishii T, Kobayashi T, Nakadaira T, Nakamura K, Nishikawa K, Nishino H, Oyama Y, Sakashita K, Sekiguchi T, Tsukamoto T, Suzuki AT, Minamino A, Nakaya T, Fukuda Y, Itow Y, Mitsuka G, Tanaka T, Jung CK, Lopez G, McGrew C, Terri R, Yanagisawa C, Tamura N, Ishino H, Kibayashi A, Mino S, Mori T, Sakuda M, Toyota H, Kuno Y, Yoshida M, Kim SB, Yang BS, Ishizuka T, Okazawa H, Choi Y, Nishijima K, Yokosawa Y, Koshiba M, Yokoyama M, Totsuka Y, Chen S, Heng Y, Yang Z, Zhang H, Kielczewska D, Mijakowski P, Connolly K, Dziomba M, Thrane E, Wilkes RJ. Search for dinucleon decay into kaons in Super-Kamiokande. Phys Rev Lett 2014; 112:131803. [PMID: 24745406 DOI: 10.1103/physrevlett.112.131803] [Citation(s) in RCA: 6] [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: 10/10/2013] [Indexed: 06/03/2023]
Abstract
A search for the dinucleon decay pp → K+ K+ has been performed using 91.6 kton·yr data from Super-Kamiokande-I. This decay provides a sensitive probe of the R-parity-violating parameter λ112''. A boosted decision tree analysis found no signal candidates in the data. The expected background was 0.28±0.19 atmospheric neutrino induced events and the estimated signal detection efficiency was 12.6%±3.2%. A lower limit of 1.7×10(32) years has been placed on the partial lifetime of the decay O16 → C14K+ K+ at 90% C.L. A corresponding upper limit of 7.8×10(-9) has been placed on the parameter λ112''.
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Affiliation(s)
- M Litos
- Department of Physics, Boston University, Boston, Massachusetts 02215, USA
| | - K Abe
- Kamioka Observatory, Institute for Cosmic Ray Research, University of Tokyo, Kamioka, Gifu 506-1205, Japan
| | - Y Hayato
- Kamioka Observatory, Institute for Cosmic Ray Research, University of Tokyo, Kamioka, Gifu 506-1205, Japan and Institute for the Physics and Mathematics of the Universe (WPI), University of Tokyo, Kashiwa, Chiba 277-8583, Japan
| | - T Iida
- Kamioka Observatory, Institute for Cosmic Ray Research, University of Tokyo, Kamioka, Gifu 506-1205, Japan
| | - M Ikeda
- Kamioka Observatory, Institute for Cosmic Ray Research, University of Tokyo, Kamioka, Gifu 506-1205, Japan
| | - K Iyogi
- Kamioka Observatory, Institute for Cosmic Ray Research, University of Tokyo, Kamioka, Gifu 506-1205, Japan
| | - J Kameda
- Kamioka Observatory, Institute for Cosmic Ray Research, University of Tokyo, Kamioka, Gifu 506-1205, Japan
| | - K Kobayashi
- Kamioka Observatory, Institute for Cosmic Ray Research, University of Tokyo, Kamioka, Gifu 506-1205, Japan
| | - Y Koshio
- Kamioka Observatory, Institute for Cosmic Ray Research, University of Tokyo, Kamioka, Gifu 506-1205, Japan
| | - Y Kozuma
- Kamioka Observatory, Institute for Cosmic Ray Research, University of Tokyo, Kamioka, Gifu 506-1205, Japan
| | - M Miura
- Kamioka Observatory, Institute for Cosmic Ray Research, University of Tokyo, Kamioka, Gifu 506-1205, Japan
| | - S Moriyama
- Kamioka Observatory, Institute for Cosmic Ray Research, University of Tokyo, Kamioka, Gifu 506-1205, Japan and Institute for the Physics and Mathematics of the Universe (WPI), University of Tokyo, Kashiwa, Chiba 277-8583, Japan
| | - M Nakahata
- Kamioka Observatory, Institute for Cosmic Ray Research, University of Tokyo, Kamioka, Gifu 506-1205, Japan and Institute for the Physics and Mathematics of the Universe (WPI), University of Tokyo, Kashiwa, Chiba 277-8583, Japan
| | - S Nakayama
- Kamioka Observatory, Institute for Cosmic Ray Research, University of Tokyo, Kamioka, Gifu 506-1205, Japan
| | - Y Obayashi
- Kamioka Observatory, Institute for Cosmic Ray Research, University of Tokyo, Kamioka, Gifu 506-1205, Japan
| | - H Ogawa
- Kamioka Observatory, Institute for Cosmic Ray Research, University of Tokyo, Kamioka, Gifu 506-1205, Japan
| | - H Sekiya
- Kamioka Observatory, Institute for Cosmic Ray Research, University of Tokyo, Kamioka, Gifu 506-1205, Japan
| | - M Shiozawa
- Kamioka Observatory, Institute for Cosmic Ray Research, University of Tokyo, Kamioka, Gifu 506-1205, Japan and Institute for the Physics and Mathematics of the Universe (WPI), University of Tokyo, Kashiwa, Chiba 277-8583, Japan
| | - Y Suzuki
- Kamioka Observatory, Institute for Cosmic Ray Research, University of Tokyo, Kamioka, Gifu 506-1205, Japan and Institute for the Physics and Mathematics of the Universe (WPI), University of Tokyo, Kashiwa, Chiba 277-8583, Japan
| | - A Takeda
- Kamioka Observatory, Institute for Cosmic Ray Research, University of Tokyo, Kamioka, Gifu 506-1205, Japan
| | - Y Takenaga
- Kamioka Observatory, Institute for Cosmic Ray Research, University of Tokyo, Kamioka, Gifu 506-1205, Japan
| | - Y Takeuchi
- Kamioka Observatory, Institute for Cosmic Ray Research, University of Tokyo, Kamioka, Gifu 506-1205, Japan and Institute for the Physics and Mathematics of the Universe (WPI), University of Tokyo, Kashiwa, Chiba 277-8583, Japan
| | - K Ueno
- Kamioka Observatory, Institute for Cosmic Ray Research, University of Tokyo, Kamioka, Gifu 506-1205, Japan
| | - K Ueshima
- Kamioka Observatory, Institute for Cosmic Ray Research, University of Tokyo, Kamioka, Gifu 506-1205, Japan
| | - H Watanabe
- Kamioka Observatory, Institute for Cosmic Ray Research, University of Tokyo, Kamioka, Gifu 506-1205, Japan
| | - S Yamada
- Kamioka Observatory, Institute for Cosmic Ray Research, University of Tokyo, Kamioka, Gifu 506-1205, Japan
| | - T Yokozawa
- Kamioka Observatory, Institute for Cosmic Ray Research, University of Tokyo, Kamioka, Gifu 506-1205, Japan
| | - S Hazama
- Research Center for Cosmic Neutrinos, Institute for Cosmic Ray Research, University of Tokyo, Kashiwa, Chiba 277-8582, Japan
| | - C Ishihara
- Research Center for Cosmic Neutrinos, Institute for Cosmic Ray Research, University of Tokyo, Kashiwa, Chiba 277-8582, Japan
| | - H Kaji
- Research Center for Cosmic Neutrinos, Institute for Cosmic Ray Research, University of Tokyo, Kashiwa, Chiba 277-8582, Japan
| | - T Kajita
- Institute for the Physics and Mathematics of the Universe (WPI), University of Tokyo, Kashiwa, Chiba 277-8583, Japan and Research Center for Cosmic Neutrinos, Institute for Cosmic Ray Research, University of Tokyo, Kashiwa, Chiba 277-8582, Japan
| | - K Kaneyuki
- Institute for the Physics and Mathematics of the Universe (WPI), University of Tokyo, Kashiwa, Chiba 277-8583, Japan and Research Center for Cosmic Neutrinos, Institute for Cosmic Ray Research, University of Tokyo, Kashiwa, Chiba 277-8582, Japan
| | - T McLachlan
- Research Center for Cosmic Neutrinos, Institute for Cosmic Ray Research, University of Tokyo, Kashiwa, Chiba 277-8582, Japan
| | - K Okumura
- Research Center for Cosmic Neutrinos, Institute for Cosmic Ray Research, University of Tokyo, Kashiwa, Chiba 277-8582, Japan
| | - Y Shimizu
- Research Center for Cosmic Neutrinos, Institute for Cosmic Ray Research, University of Tokyo, Kashiwa, Chiba 277-8582, Japan
| | - N Tanimoto
- Research Center for Cosmic Neutrinos, Institute for Cosmic Ray Research, University of Tokyo, Kashiwa, Chiba 277-8582, Japan
| | - M R Vagins
- Institute for the Physics and Mathematics of the Universe (WPI), University of Tokyo, Kashiwa, Chiba 277-8583, Japan and Department of Physics and Astronomy, University of California, Irvine, Irvine, California 92697-4575, USA
| | - E Kearns
- Department of Physics, Boston University, Boston, Massachusetts 02215, USA and Institute for the Physics and Mathematics of the Universe (WPI), University of Tokyo, Kashiwa, Chiba 277-8583, Japan
| | - J L Stone
- Department of Physics, Boston University, Boston, Massachusetts 02215, USA and Institute for the Physics and Mathematics of the Universe (WPI), University of Tokyo, Kashiwa, Chiba 277-8583, Japan
| | - L R Sulak
- Department of Physics, Boston University, Boston, Massachusetts 02215, USA
| | - F Dufour
- Department of Physics, Boston University, Boston, Massachusetts 02215, USA
| | - J L Raaf
- Department of Physics, Boston University, Boston, Massachusetts 02215, USA
| | - B Henning
- Department of Physics, Boston University, Boston, Massachusetts 02215, USA
| | - M Goldhaber
- Physics Department, Brookhaven National Laboratory, Upton, New York 11973, USA
| | - K Bays
- Department of Physics and Astronomy, University of California, Irvine, Irvine, California 92697-4575, USA
| | - D Casper
- Department of Physics and Astronomy, University of California, Irvine, Irvine, California 92697-4575, USA
| | - J P Cravens
- Department of Physics and Astronomy, University of California, Irvine, Irvine, California 92697-4575, USA
| | - W R Kropp
- Department of Physics and Astronomy, University of California, Irvine, Irvine, California 92697-4575, USA
| | - S Mine
- Department of Physics and Astronomy, University of California, Irvine, Irvine, California 92697-4575, USA
| | - C Regis
- Department of Physics and Astronomy, University of California, Irvine, Irvine, California 92697-4575, USA
| | - M B Smy
- Institute for the Physics and Mathematics of the Universe (WPI), University of Tokyo, Kashiwa, Chiba 277-8583, Japan and Department of Physics and Astronomy, University of California, Irvine, Irvine, California 92697-4575, USA
| | - H W Sobel
- Institute for the Physics and Mathematics of the Universe (WPI), University of Tokyo, Kashiwa, Chiba 277-8583, Japan and Department of Physics and Astronomy, University of California, Irvine, Irvine, California 92697-4575, USA
| | - K S Ganezer
- Department of Physics, California State University, Dominguez Hills, Carson, California 90747, USA
| | - J Hill
- Department of Physics, California State University, Dominguez Hills, Carson, California 90747, USA
| | - W E Keig
- Department of Physics, California State University, Dominguez Hills, Carson, California 90747, USA
| | - J S Jang
- Department of Physics, Chonnam National University, Kwangju 500-757, Korea
| | - J Y Kim
- Department of Physics, Chonnam National University, Kwangju 500-757, Korea
| | - I T Lim
- Department of Physics, Chonnam National University, Kwangju 500-757, Korea
| | - J B Albert
- Department of Physics, Duke University, Durham, North Carolina 27708, USA
| | - T Wongjirad
- Department of Physics, Duke University, Durham, North Carolina 27708, USA
| | - R Wendell
- Department of Physics, Duke University, Durham, North Carolina 27708, USA
| | - K Scholberg
- Institute for the Physics and Mathematics of the Universe (WPI), University of Tokyo, Kashiwa, Chiba 277-8583, Japan and Department of Physics, Duke University, Durham, North Carolina 27708, USA
| | - C W Walter
- Institute for the Physics and Mathematics of the Universe (WPI), University of Tokyo, Kashiwa, Chiba 277-8583, Japan and Department of Physics, Duke University, Durham, North Carolina 27708, USA
| | - S Tasaka
- Department of Physics, Gifu University, Gifu, Gifu 501-1193, Japan
| | - J G Learned
- Department of Physics and Astronomy, University of Hawaii, Honolulu, Hawaii 96822, USA
| | - S Matsuno
- Department of Physics and Astronomy, University of Hawaii, Honolulu, Hawaii 96822, USA
| | - Y Watanabe
- Physics Division, Department of Engineering, Kanagawa University, Kanagawa, Yokohama 221-8686, Japan
| | - T Hasegawa
- High Energy Accelerator Research Organization (KEK), Tsukuba, Ibaraki 305-0801, Japan
| | - T Ishida
- High Energy Accelerator Research Organization (KEK), Tsukuba, Ibaraki 305-0801, Japan
| | - T Ishii
- High Energy Accelerator Research Organization (KEK), Tsukuba, Ibaraki 305-0801, Japan
| | - T Kobayashi
- High Energy Accelerator Research Organization (KEK), Tsukuba, Ibaraki 305-0801, Japan
| | - T Nakadaira
- High Energy Accelerator Research Organization (KEK), Tsukuba, Ibaraki 305-0801, Japan
| | - K Nakamura
- Institute for the Physics and Mathematics of the Universe (WPI), University of Tokyo, Kashiwa, Chiba 277-8583, Japan and High Energy Accelerator Research Organization (KEK), Tsukuba, Ibaraki 305-0801, Japan
| | - K Nishikawa
- High Energy Accelerator Research Organization (KEK), Tsukuba, Ibaraki 305-0801, Japan
| | - H Nishino
- High Energy Accelerator Research Organization (KEK), Tsukuba, Ibaraki 305-0801, Japan
| | - Y Oyama
- High Energy Accelerator Research Organization (KEK), Tsukuba, Ibaraki 305-0801, Japan
| | - K Sakashita
- High Energy Accelerator Research Organization (KEK), Tsukuba, Ibaraki 305-0801, Japan
| | - T Sekiguchi
- High Energy Accelerator Research Organization (KEK), Tsukuba, Ibaraki 305-0801, Japan
| | - T Tsukamoto
- High Energy Accelerator Research Organization (KEK), Tsukuba, Ibaraki 305-0801, Japan
| | - A T Suzuki
- Department of Physics, Kobe University, Kobe, Hyogo 657-8501, Japan
| | - A Minamino
- Department of Physics, Kyoto University, Kyoto, Kyoto 606-8502, Japan
| | - T Nakaya
- Institute for the Physics and Mathematics of the Universe (WPI), University of Tokyo, Kashiwa, Chiba 277-8583, Japan and Department of Physics, Kyoto University, Kyoto, Kyoto 606-8502, Japan
| | - Y Fukuda
- Department of Physics, Miyagi University of Education, Sendai, Miyagi 980-0845, Japan
| | - Y Itow
- Solar Terrestrial Environment Laboratory, Nagoya University, Nagoya, Aichi 464-8602, Japan
| | - G Mitsuka
- Solar Terrestrial Environment Laboratory, Nagoya University, Nagoya, Aichi 464-8602, Japan
| | - T Tanaka
- Solar Terrestrial Environment Laboratory, Nagoya University, Nagoya, Aichi 464-8602, Japan
| | - C K Jung
- Department of Physics and Astronomy, State University of New York, Stony Brook, New York 11794-3800, USA
| | - G Lopez
- Department of Physics and Astronomy, State University of New York, Stony Brook, New York 11794-3800, USA
| | - C McGrew
- Department of Physics and Astronomy, State University of New York, Stony Brook, New York 11794-3800, USA
| | - R Terri
- Department of Physics and Astronomy, State University of New York, Stony Brook, New York 11794-3800, USA
| | - C Yanagisawa
- Department of Physics and Astronomy, State University of New York, Stony Brook, New York 11794-3800, USA
| | - N Tamura
- Department of Physics, Niigata University, Niigata, Niigata 950-2181, Japan
| | - H Ishino
- Department of Physics, Okayama University, Okayama, Okayama 700-8530, Japan
| | - A Kibayashi
- Department of Physics, Okayama University, Okayama, Okayama 700-8530, Japan
| | - S Mino
- Department of Physics, Okayama University, Okayama, Okayama 700-8530, Japan
| | - T Mori
- Department of Physics, Okayama University, Okayama, Okayama 700-8530, Japan
| | - M Sakuda
- Department of Physics, Okayama University, Okayama, Okayama 700-8530, Japan
| | - H Toyota
- Department of Physics, Okayama University, Okayama, Okayama 700-8530, Japan
| | - Y Kuno
- Department of Physics, Osaka University, Toyonaka, Osaka 560-0043, Japan
| | - M Yoshida
- Department of Physics, Osaka University, Toyonaka, Osaka 560-0043, Japan
| | - S B Kim
- Department of Physics, Seoul National University, Seoul 151-742, Korea
| | - B S Yang
- Department of Physics, Seoul National University, Seoul 151-742, Korea
| | - T Ishizuka
- Department of Systems Engineering, Shizuoka University, Hamamatsu, Shizuoka 432-8561, Japan
| | - H Okazawa
- Department of Informatics in Social Welfare, Shizuoka University of Welfare, Yaizu, Shizuoka 425-8611, Japan
| | - Y Choi
- Department of Physics, Sungkyunkwan University, Suwon 440-746, Korea
| | - K Nishijima
- Department of Physics, Tokai University, Hiratsuka, Kanagawa 259-1292, Japan
| | - Y Yokosawa
- Department of Physics, Tokai University, Hiratsuka, Kanagawa 259-1292, Japan
| | - M Koshiba
- The University of Tokyo, Bunkyo, Tokyo 113-0033, Japan
| | - M Yokoyama
- The University of Tokyo, Bunkyo, Tokyo 113-0033, Japan
| | - Y Totsuka
- The University of Tokyo, Bunkyo, Tokyo 113-0033, Japan
| | - S Chen
- Department of Engineering Physics, Tsinghua University, Beijing 100084, China
| | - Y Heng
- Department of Engineering Physics, Tsinghua University, Beijing 100084, China
| | - Z Yang
- Department of Engineering Physics, Tsinghua University, Beijing 100084, China
| | - H Zhang
- Department of Engineering Physics, Tsinghua University, Beijing 100084, China
| | - D Kielczewska
- Institute of Experimental Physics, Warsaw University, 00-681 Warsaw, Poland
| | - P Mijakowski
- Institute of Experimental Physics, Warsaw University, 00-681 Warsaw, Poland
| | - K Connolly
- Department of Physics, University of Washington, Seattle, Washington 98195-1560, USA
| | - M Dziomba
- Department of Physics, University of Washington, Seattle, Washington 98195-1560, USA
| | - E Thrane
- Department of Physics, University of Washington, Seattle, Washington 98195-1560, USA
| | - R J Wilkes
- Department of Physics, University of Washington, Seattle, Washington 98195-1560, USA
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12
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Vafaei-Najafabadi N, Marsh KA, Clayton CE, An W, Mori WB, Joshi C, Lu W, Adli E, Corde S, Litos M, Li S, Gessner S, Frederico J, Fisher AS, Wu Z, Walz D, England RJ, Delahaye JP, Clarke CI, Hogan MJ, Muggli P. Beam loading by distributed injection of electrons in a plasma wakefield accelerator. Phys Rev Lett 2014; 112:025001. [PMID: 24484020 DOI: 10.1103/physrevlett.112.025001] [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: 05/17/2013] [Indexed: 06/03/2023]
Abstract
We show through experiments and supporting simulations that propagation of a highly relativistic and dense electron bunch through a plasma can lead to distributed injection of electrons, which depletes the accelerating field, i.e., beam loads the wake. The source of the injected electrons is ionization of the second electron of rubidium (Rb II) within the wake. This injection of excess charge is large enough to severely beam load the wake, and thereby reduce the transformer ratio T. The reduction of the average T with increasing beam loading is quantified for the first time by measuring the ratio of peak energy gain and loss of electrons while changing the beam emittance. Simulations show that beam loading by Rb II electrons contributes to the reduction of the peak accelerating field from its weakly loaded value of 43 GV/m to a strongly loaded value of 26 GV/m.
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Affiliation(s)
- N Vafaei-Najafabadi
- Department of Electrical Engineering, University of California Los Angeles, Los Angeles, California 90095, USA
| | - K A Marsh
- Department of Electrical Engineering, University of California Los Angeles, Los Angeles, California 90095, USA
| | - C E Clayton
- Department of Electrical Engineering, University of California Los Angeles, Los Angeles, California 90095, USA
| | - W An
- Department of Electrical Engineering, University of California Los Angeles, Los Angeles, California 90095, USA
| | - W B Mori
- Department of Electrical Engineering, University of California Los Angeles, Los Angeles, California 90095, USA and Department of Physics and astronomy, University of California Los Angeles, Los Angeles, California 90095, USA
| | | | - W Lu
- Department of Physics and astronomy, University of California Los Angeles, Los Angeles, California 90095, USA and Department of Engineering Physics, Tsinghua University, Beijing 100084, China
| | - E Adli
- SLAC National Accelerator Laboratory, Menlo Park, California 94025, USA and Department of Physics, University of Oslo, 0316 Oslo, Norway
| | - S Corde
- SLAC National Accelerator Laboratory, Menlo Park, California 94025, USA
| | - M Litos
- SLAC National Accelerator Laboratory, Menlo Park, California 94025, USA
| | - S Li
- SLAC National Accelerator Laboratory, Menlo Park, California 94025, USA
| | - S Gessner
- SLAC National Accelerator Laboratory, Menlo Park, California 94025, USA
| | - J Frederico
- SLAC National Accelerator Laboratory, Menlo Park, California 94025, USA
| | - A S Fisher
- SLAC National Accelerator Laboratory, Menlo Park, California 94025, USA
| | - Z Wu
- SLAC National Accelerator Laboratory, Menlo Park, California 94025, USA
| | - D Walz
- SLAC National Accelerator Laboratory, Menlo Park, California 94025, USA
| | - R J England
- SLAC National Accelerator Laboratory, Menlo Park, California 94025, USA
| | - J P Delahaye
- SLAC National Accelerator Laboratory, Menlo Park, California 94025, USA
| | - C I Clarke
- SLAC National Accelerator Laboratory, Menlo Park, California 94025, USA
| | - M J Hogan
- SLAC National Accelerator Laboratory, Menlo Park, California 94025, USA
| | - P Muggli
- Max Planck Institute for Physics, 80805 Munich, Germany
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13
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Abe K, Hayato Y, Iida T, Iyogi K, Kameda J, Koshio Y, Kozuma Y, Marti L, Miura M, Moriyama S, Nakahata M, Nakayama S, Obayashi Y, Sekiya H, Shiozawa M, Suzuki Y, Takeda A, Takenaga Y, Ueno K, Ueshima K, Yamada S, Yokozawa T, Ishihara C, Kaji H, Kajita T, Kaneyuki K, Lee KP, McLachlan T, Okumura K, Shimizu Y, Tanimoto N, Labarga L, Kearns E, Litos M, Raaf JL, Stone JL, Sulak LR, Goldhaber M, Bays K, Kropp WR, Mine S, Regis C, Renshaw A, Smy MB, Sobel HW, Ganezer KS, Hill J, Keig WE, Jang JS, Kim JY, Lim IT, Albert JB, Scholberg K, Walter CW, Wendell R, Wongjirad TM, Ishizuka T, Tasaka S, Learned JG, Matsuno S, Smith SN, Hasegawa T, Ishida T, Ishii T, Kobayashi T, Nakadaira T, Nakamura K, Nishikawa K, Oyama Y, Sakashita K, Sekiguchi T, Tsukamoto T, Suzuki AT, Takeuchi Y, Ikeda M, Minamino A, Nakaya T, Fukuda Y, Itow Y, Mitsuka G, Tanaka T, Jung CK, Lopez GD, Taylor I, Yanagisawa C, Ishino H, Kibayashi A, Mino S, Mori T, Sakuda M, Toyota H, Kuno Y, Yoshida M, Kim SB, Yang BS, Okazawa H, Choi Y, Nishijima K, Koshiba M, Yokoyama M, Totsuka Y, Martens K, Schuemann J, Vagins MR, Chen S, Heng Y, Yang Z, Zhang H, Kielczewska D, Mijakowski P, Connolly K, Dziomba M, Thrane E, Wilkes RJ. Evidence for the appearance of atmospheric tau neutrinos in super-Kamiokande. Phys Rev Lett 2013; 110:181802. [PMID: 23683190 DOI: 10.1103/physrevlett.110.181802] [Citation(s) in RCA: 5] [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: 06/05/2012] [Indexed: 06/02/2023]
Abstract
Super-Kamiokande atmospheric neutrino data were fit with an unbinned maximum likelihood method to search for the appearance of tau leptons resulting from the interactions of oscillation-generated tau neutrinos in the detector. Relative to the expectation of unity, the tau normalization is found to be 1.42 ± 0.35(stat)(-0.12)(+0.14)(syst) excluding the no-tau-appearance hypothesis, for which the normalization would be zero, at the 3.8σ level. We estimate that 180.1 ± 44.3(stat)(-15.2)(+17.8) (syst) tau leptons were produced in the 22.5 kton fiducial volume of the detector by tau neutrinos during the 2806 day running period. In future analyses, this large sample of selected tau events will allow the study of charged current tau neutrino interaction physics with oscillation produced tau neutrinos.
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Affiliation(s)
- K Abe
- Kamioka Observatory, Institute for Cosmic Ray Research, University of Tokyo, Kamioka, Gifu 506-1205, Japan
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14
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Hidding B, Rosenzweig JB, Xi Y, O'Shea B, Andonian G, Schiller D, Barber S, Williams O, Pretzler G, Königstein T, Kleeschulte F, Hogan MJ, Litos M, Corde S, White WW, Muggli P, Bruhwiler DL, Lotov K. Beyond injection: Trojan horse underdense photocathode plasma wakefield acceleration. ACTA ACUST UNITED AC 2013. [DOI: 10.1063/1.4773760] [Citation(s) in RCA: 14] [Impact Index Per Article: 1.3] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/14/2022]
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15
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Abe K, Hayato Y, Iida T, Ikeda M, Iyogi K, Kameda J, Koshio Y, Kozuma Y, Miura M, Moriyama S, Nakahata M, Nakayama S, Obayashi Y, Sekiya H, Shiozawa M, Suzuki Y, Takeda A, Takenaga Y, Takeuchi Y, Ueno K, Ueshima K, Watanabe H, Yamada S, Yokozawa T, Ishihara C, Kaji H, Lee KP, Kajita T, Kaneyuki K, McLachlan T, Okumura K, Shimizu Y, Tanimoto N, Martens K, Vagins MR, Labarga L, Magro LM, Dufour F, Kearns E, Litos M, Raaf JL, Stone JL, Sulak LR, Goldhaber M, Bays K, Kropp WR, Mine S, Regis C, Smy MB, Sobel HW, Ganezer KS, Hill J, Keig WE, Jang JS, Kim JY, Lim IT, Albert JB, Scholberg K, Walter CW, Wendell R, Wongjirad TM, Tasaka S, Learned JG, Matsuno S, Hasegawa T, Ishida T, Ishii T, Kobayashi T, Nakadaira T, Nakamura K, Nishikawa K, Nishino H, Oyama Y, Sakashita K, Sekiguchi T, Tsukamoto T, Suzuki AT, Minamino A, Nakaya T, Fukuda Y, Itow Y, Mitsuka G, Tanaka T, Jung CK, Taylor I, Yanagisawa C, Ishino H, Kibayashi A, Mino S, Mori T, Sakuda M, Toyota H, Kuno Y, Kim SB, Yang BS, Ishizuka T, Okazawa H, Choi Y, Nishijima K, Koshiba M, Yokoyama M, Totsuka Y, Chen S, Heng Y, Yang Z, Zhang H, Kielczewska D, Mijakowski P, Connolly K, Dziomba M, Wilkes RJ. Search for differences in oscillation parameters for atmospheric neutrinos and antineutrinos at Super-Kamiokande. Phys Rev Lett 2011; 107:241801. [PMID: 22242990 DOI: 10.1103/physrevlett.107.241801] [Citation(s) in RCA: 6] [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: 09/09/2011] [Indexed: 05/31/2023]
Abstract
We present a search for differences in the oscillations of antineutrinos and neutrinos in the Super-Kamiokande-I, -II, and -III atmospheric neutrino sample. Under a two-flavor disappearance model with separate mixing parameters between neutrinos and antineutrinos, we find no evidence for a difference in oscillation parameters. Best-fit antineutrino mixing is found to be at (Δm2,sin2 2θ)=(2.0×10(-3) eV2, 1.0) and is consistent with the overall Super-K measurement.
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Affiliation(s)
- K Abe
- Kamioka Observatory, Institute for Cosmic Ray Research, University of Tokyo, Kamioka, Gifu 506-1205, Japan
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Abe K, Abgrall N, Ajima Y, Aihara H, Albert JB, Andreopoulos C, Andrieu B, Aoki S, Araoka O, Argyriades J, Ariga A, Ariga T, Assylbekov S, Autiero D, Badertscher A, Barbi M, Barker GJ, Barr G, Bass M, Bay F, Bentham S, Berardi V, Berger BE, Bertram I, Besnier M, Beucher J, Beznosko D, Bhadra S, Blaszczyk FDMM, Blondel A, Bojechko C, Bouchez J, Boyd SB, Bravar A, Bronner C, Brook-Roberge DG, Buchanan N, Budd H, Calvet D, Cartwright SL, Carver A, Castillo R, Catanesi MG, Cazes A, Cervera A, Chavez C, Choi S, Christodoulou G, Coleman J, Coleman W, Collazuol G, Connolly K, Curioni A, Dabrowska A, Danko I, Das R, Davies GS, Davis S, Day M, De Rosa G, de André JPAM, de Perio P, Delbart A, Densham C, Di Lodovico F, Di Luise S, Dinh Tran P, Dobson J, Dore U, Drapier O, Dufour F, Dumarchez J, Dytman S, Dziewiecki M, Dziomba M, Emery S, Ereditato A, Escudero L, Esposito LS, Fechner M, Ferrero A, Finch AJ, Frank E, Fujii Y, Fukuda Y, Galymov V, Gannaway FC, Gaudin A, Gendotti A, George MA, Giffin S, Giganti C, Gilje K, Golan T, Goldhaber M, Gomez-Cadenas JJ, Gonin M, Grant N, Grant A, Gumplinger P, Guzowski P, Haesler A, Haigh MD, Hamano K, Hansen C, Hansen D, Hara T, Harrison PF, Hartfiel B, Hartz M, Haruyama T, Hasegawa T, Hastings NC, Hastings S, Hatzikoutelis A, Hayashi K, Hayato Y, Hearty C, Helmer RL, Henderson R, Higashi N, Hignight J, Hirose E, Holeczek J, Horikawa S, Hyndman A, Ichikawa AK, Ieki K, Ieva M, Iida M, Ikeda M, Ilic J, Imber J, Ishida T, Ishihara C, Ishii T, Ives SJ, Iwasaki M, Iyogi K, Izmaylov A, Jamieson B, Johnson RA, Joo KK, Jover-Manas GV, Jung CK, Kaji H, Kajita T, Kakuno H, Kameda J, Kaneyuki K, Karlen D, Kasami K, Kato I, Kearns E, Khabibullin M, Khanam F, Khotjantsev A, Kielczewska D, Kikawa T, Kim J, Kim JY, Kim SB, Kimura N, Kirby B, Kisiel J, Kitching P, Kobayashi T, Kogan G, Koike S, Konaka A, Kormos LL, Korzenev A, Koseki K, Koshio Y, Kouzuma Y, Kowalik K, Kravtsov V, Kreslo I, Kropp W, Kubo H, Kudenko Y, Kulkarni N, Kurjata R, Kutter T, Lagoda J, Laihem K, Laveder M, Lee KP, Le PT, Levy JM, Licciardi C, Lim IT, Lindner T, Litchfield RP, Litos M, Longhin A, Lopez GD, Loverre PF, Ludovici L, Lux T, Macaire M, Mahn K, Makida Y, Malek M, Manly S, Marchionni A, Marino AD, Marteau J, Martin JF, Maruyama T, Maryon T, Marzec J, Masliah P, Mathie EL, Matsumura C, Matsuoka K, Matveev V, Mavrokoridis K, Mazzucato E, McCauley N, McFarland KS, McGrew C, McLachlan T, Messina M, Metcalf W, Metelko C, Mezzetto M, Mijakowski P, Miller CA, Minamino A, Mineev O, Mine S, Missert AD, Mituka G, Miura M, Mizouchi K, Monfregola L, Moreau F, Morgan B, Moriyama S, Muir A, Murakami A, Murdoch M, Murphy S, Myslik J, Nakadaira T, Nakahata M, Nakai T, Nakajima K, Nakamoto T, Nakamura K, Nakayama S, Nakaya T, Naples D, Navin ML, Nelson B, Nicholls TC, Nishikawa K, Nishino H, Nowak JA, Noy M, Obayashi Y, Ogitsu T, Ohhata H, Okamura T, Okumura K, Okusawa T, Oser SM, Otani M, Owen RA, Oyama Y, Ozaki T, Pac MY, Palladino V, Paolone V, Paul P, Payne D, Pearce GF, Perkin JD, Pettinacci V, Pierre F, Poplawska E, Popov B, Posiadala M, Poutissou JM, Poutissou R, Przewlocki P, Qian W, Raaf JL, Radicioni E, Ratoff PN, Raufer TM, Ravonel M, Raymond M, Retiere F, Robert A, Rodrigues PA, Rondio E, Roney JM, Rossi B, Roth S, Rubbia A, Ruterbories D, Sabouri S, Sacco R, Sakashita K, Sánchez F, Sarrat A, Sasaki K, Scholberg K, Schwehr J, Scott M, Scully DI, Seiya Y, Sekiguchi T, Sekiya H, Shibata M, Shimizu Y, Shiozawa M, Short S, Siyad M, Smith RJ, Smy M, Sobczyk JT, Sobel H, Sorel M, Stahl A, Stamoulis P, Steinmann J, Still B, Stone J, Strabel C, Sulak LR, Sulej R, Sutcliffe P, Suzuki A, Suzuki K, Suzuki S, Suzuki SY, Suzuki Y, Suzuki Y, Szeglowski T, Szeptycka M, Tacik R, Tada M, Takahashi S, Takeda A, Takenaga Y, Takeuchi Y, Tanaka K, Tanaka HA, Tanaka M, Tanaka MM, Tanimoto N, Tashiro K, Taylor I, Terashima A, Terhorst D, Terri R, Thompson LF, Thorley A, Toki W, Tomaru T, Totsuka Y, Touramanis C, Tsukamoto T, Tzanov M, Uchida Y, Ueno K, Vacheret A, Vagins M, Vasseur G, Wachala T, Walding JJ, Waldron AV, Walter CW, Wanderer PJ, Wang J, Ward MA, Ward GP, Wark D, Wascko MO, Weber A, Wendell R, West N, Whitehead LH, Wikström G, Wilkes RJ, Wilking MJ, Wilson JR, Wilson RJ, Wongjirad T, Yamada S, Yamada Y, Yamamoto A, Yamamoto K, Yamanoi Y, Yamaoka H, Yanagisawa C, Yano T, Yen S, Yershov N, Yokoyama M, Zalewska A, Zalipska J, Zambelli L, Zaremba K, Ziembicki M, Zimmerman ED, Zito M, Żmuda J. Indication of electron neutrino appearance from an accelerator-produced off-axis muon neutrino beam. Phys Rev Lett 2011; 107:041801. [PMID: 21866992 DOI: 10.1103/physrevlett.107.041801] [Citation(s) in RCA: 65] [Impact Index Per Article: 5.0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 06/13/2011] [Indexed: 05/31/2023]
Abstract
The T2K experiment observes indications of ν(μ) → ν(e) appearance in data accumulated with 1.43×10(20) protons on target. Six events pass all selection criteria at the far detector. In a three-flavor neutrino oscillation scenario with |Δm(23)(2)| = 2.4×10(-3) eV(2), sin(2)2θ(23) = 1 and sin(2)2θ(13) = 0, the expected number of such events is 1.5±0.3(syst). Under this hypothesis, the probability to observe six or more candidate events is 7×10(-3), equivalent to 2.5σ significance. At 90% C.L., the data are consistent with 0.03(0.04) < sin(2)2θ(13) < 0.28(0.34) for δ(CP) = 0 and a normal (inverted) hierarchy.
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Affiliation(s)
- K Abe
- University of Tokyo, Institute for Cosmic Ray Research, Kamioka Observatory, Kamioka, Japan
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Nishino H, Clark S, Abe K, Hayato Y, Iida T, Ikeda M, Kameda J, Kobayashi K, Koshio Y, Miura M, Moriyama S, Nakahata M, Nakayama S, Obayashi Y, Ogawa H, Sekiya H, Shiozawa M, Suzuki Y, Takeda A, Takenaga Y, Takeuchi Y, Ueno K, Ueshima K, Watanabe H, Yamada S, Hazama S, Higuchi I, Ishihara C, Kajita T, Kaneyuki K, Mitsuka G, Okumura K, Tanimoto N, Vagins MR, Dufour F, Kearns E, Litos M, Raaf JL, Stone JL, Sulak LR, Wang W, Goldhaber M, Dazeley S, Svoboda R, Bays K, Casper D, Cravens JP, Kropp WR, Mine S, Regis C, Smy MB, Sobel HW, Ganezer KS, Hill J, Keig WE, Jang JS, Kim JY, Lim IT, Fechner M, Scholberg K, Walter CW, Wendell R, Tasaka S, Learned JG, Matsuno S, Watanabe Y, Hasegawa T, Ishida T, Ishii T, Kobayashi T, Nakadaira T, Nakamura K, Nishikawa K, Oyama Y, Sakashita K, Sekiguchi T, Tsukamoto T, Suzuki AT, Minamino A, Nakaya T, Yokoyama M, Fukuda Y, Itow Y, Tanaka T, Jung CK, Lopez G, McGrew C, Terri R, Yanagisawa C, Tamura N, Idehara Y, Sakuda M, Kuno Y, Yoshida M, Kim SB, Yang BS, Ishizuka T, Okazawa H, Choi Y, Seo HK, Furuse Y, Nishijima K, Yokosawa Y, Koshiba M, Totsuka Y, Chen S, Heng Y, Yang Z, Zhang H, Kielczewska D, Thrane E, Wilkes RJ. Search for proton decay via p-->e+pi0 and p-->micro+pi0 in a large water Cherenkov detector. Phys Rev Lett 2009; 102:141801. [PMID: 19392425 DOI: 10.1103/physrevlett.102.141801] [Citation(s) in RCA: 10] [Impact Index Per Article: 0.7] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 01/09/2009] [Indexed: 05/27/2023]
Abstract
We have searched for proton decays via p-->e;{+}pi;{0} and p-->micro;{+}pi;{0} using data from a 91.7 kt.yr exposure of Super-Kamiokande-I and a 49.2 kt.yr exposure of Super-Kamiokande-II. No candidate events were observed with expected backgrounds induced by atmospheric neutrinos of 0.3 events for each decay mode. From these results, we set lower limits on the partial lifetime of 8.2 x 10;{33} and 6.6 x 10;{33} years at 90% confidence level for p-->e;{+}pi;{0} and p-->micro;{+}pi;{0} modes, respectively.
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Affiliation(s)
- H Nishino
- Research Center for Cosmic Neutrinos, Institute for Cosmic Ray Research, University of Tokyo, Kashiwa, Chiba 277-8582, Japan
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Sarris I, Litos M, Bewley S, Okpala I, Seed P, Oteng-Ntim E. Platelet count as a predictor of the severity of sickle cell disease during pregnancy. J OBSTET GYNAECOL 2009; 28:688-91. [PMID: 19065361 DOI: 10.1080/01443610802462977] [Citation(s) in RCA: 2] [Impact Index Per Article: 0.1] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 10/21/2022]
Abstract
Recent evidence implicates the immune system and the clotting mechanisms in the pathophysiology of sickle cell disease (SCD). This study investigates the association of steady state platelet count with the severity of SCD in pregnancy. A total of 40 SCD women who were asymptomatic early in pregnancy were studied retrospectively: 14 remained asymptomatic throughout pregnancy and 26 developed at least one SCD-related complication. The early pregnancy platelet count was compared between the two groups using t-test and its ability to predict SCD-related complications in pregnancy was investigated using Receiver-Operator Characteristics (ROC) curve. Compared with asymptomatic patients, women who developed SCD-related complications had significantly higher early-pregnancy platelet count [328x10(9)/l (95% CI: 268-389) vs 210x10(9)/l (146-275), p < 0.01]. The area under the ROC curve was 76.4% (95% CI 59.7-93.2). These indicate that the platelet count in early pregnancy is significantly higher in SCD patients who subsequently develop SCD-related complications and may be used for screening.
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Affiliation(s)
- I Sarris
- Department of Obstetrics and Gynaecology, Guy's and St Thomas' NHS Trust, London, UK
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Abe K, Hayato Y, Iida T, Ikeda M, Kameda J, Koshio Y, Minamino A, Miura M, Moriyama S, Nakahata M, Nakayama S, Obayashi Y, Ogawa H, Sekiya H, Shiozawa M, Suzuki Y, Takeda A, Takeuchi Y, Ueshima K, Watanabe H, Yamada S, Higuchi I, Ishihara C, Kajita T, Kaneyuki K, Mitsuka G, Nishino H, Okumura K, Saji C, Takenaga Y, Clark S, Desai S, Dufour F, Kearns E, Likhoded S, Litos M, Raaf JL, Stone JL, Sulak LR, Wang W, Goldhaber M, Casper D, Cravens JP, Dunmore J, Kropp WR, Liu DW, Mine S, Regis C, Smy MB, Sobel HW, Vagins MR, Ganezer KS, Hartfield B, Hill J, Keig WE, Jang JS, Jeong IS, Kim JY, Lim IT, Scholberg K, Fechner M, Tanimoto N, Walter CW, Wendell R, Tasaka S, Guillian G, Learned JG, Matsuno S, Messier MD, Hasegawa T, Ishida T, Ishii T, Kobayashi T, Nakadaira T, Nakamura K, Nishikawa K, Oyama Y, Totsuka Y, Suzuki AT, Nakaya T, Tanaka H, Yokoyama M, Haines TJ, Dazeley S, Svoboda R, Habig A, Fukuda Y, Sato T, Itow Y, Koike T, Tanaka T, Jung CK, Kato T, Kobayashi K, McGrew C, Sarrat A, Terri R, Yanagisawa C, Tamura N, Idehara Y, Sakuda M, Sugihara M, Kuno Y, Yoshida M, Kim SB, Yang BS, Ishizuka T, Okazawa H, Choi Y, Seo HK, Gando Y, Inoue K, Furuse Y, Ishii H, Nishijima K, Watanabe Y, Koshiba M, Chen S, Deng Z, Liu Y, Kielczewska D, Berns H, Shiraishi KK, Thrane E, Wilkes RJ. Search for matter-dependent atmospheric neutrino oscillations in Super-Kamiokande. Int J Clin Exp Med 2008. [DOI: 10.1103/physrevd.77.052001] [Citation(s) in RCA: 12] [Impact Index Per Article: 0.8] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/07/2022]
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Abe K, Hayato Y, Iida T, Ishihara K, Kameda J, Koshio Y, Minamino A, Mitsuda C, Miura M, Moriyama S, Nakahata M, Obayashi Y, Ogawa H, Shiozawa M, Suzuki Y, Takeda A, Takeuchi Y, Ueshima K, Higuchi I, Ishihara C, Ishitsuka M, Kajita T, Kaneyuki K, Mitsuka G, Nakayama S, Nishino H, Okumura K, Saji C, Takenaga Y, Totsuka Y, Clark S, Desai S, Dufour F, Kearns E, Likhoded S, Litos M, Raaf JL, Stone JL, Sulak LR, Wang W, Goldhaber M, Casper D, Cravens JP, Kropp WR, Liu DW, Mine S, Regis C, Smy MB, Sobel HW, Vagins MR, Ganezer KS, Hill JE, Keig WE, Jang JS, Kim JY, Lim IT, Scholberg K, Tanimoto N, Walter CW, Wendell R, Ellsworth RW, Tasaka S, Guillian E, Learned JG, Matsuno S, Messier MD, Ichikawa AK, Ishida T, Ishii T, Iwashita T, Kobayashi T, Nakadaira T, Nakamura K, Nitta K, Oyama Y, Suzuki AT, Hasegawa M, Kato I, Maesaka H, Nakaya T, Nishikawa K, Sasaki T, Sato H, Yamamoto S, Yokoyama M, Haines TJ, Dazeley S, Hatakeyama S, Svoboda R, Sullivan GW, Habig A, Gran R, Fukuda Y, Sato T, Itow Y, Koike T, Jung CK, Kato T, Kobayashi K, Malek M, McGrew C, Sarrat A, Terri R, Yanagisawa C, Tamura N, Sakuda M, Sugihara M, Kuno Y, Yoshida M, Kim SB, Yoo J, Ishizuka T, Okazawa H, Choi Y, Seo HK, Gando Y, Hasegawa T, Inoue K, Ishii H, Nishijima K, Ishino H, Watanabe Y, Koshiba M, Kielczewska D, Zalipska J, Berns HG, Shiraishi KK, Washburn K, Wilkes RJ. Measurement of atmospheric neutrino flux consistent with tau neutrino appearance. Phys Rev Lett 2006; 97:171801. [PMID: 17155460 DOI: 10.1103/physrevlett.97.171801] [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: 07/25/2006] [Indexed: 05/12/2023]
Abstract
A search for the appearance of tau neutrinos from nu(mu) <--> nu(tau) oscillations in the atmospheric neutrinos has been performed using 1489.2 days of atmospheric neutrino data from the Super-Kamiokande-I experiment. A best fit tau neutrino appearance signal of 138+/-48(stat)-32(+15)(syst) events is obtained with an expectation of 78+/-26(syst). The hypothesis of no tau neutrino appearance is disfavored by 2.4 sigma.
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Affiliation(s)
- K Abe
- Kamioka Observatory, Institute for Cosmic Ray Research, University of Tokyo, Kamioka, Gifu 506-1205, Japan
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Galani E, Skarlos D, Sgouros J, Litos M, Gonos E, Dionyssiou-Asteriou A. Correlation of MDR 1 expression and CA 125 in ovarian cancer. In Vivo 2005; 19:797-800. [PMID: 15999552] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 05/03/2023]
Abstract
BACKGROUND The serum CA 125 marker is elevated in 80% of patients with ovarian adenocarcinoma. MDR 1 gene expression has been identified in a variety of tumor types and its expression has been correlated with multidrug resistance. Whether there is a correlation between CA 125 levels and MDR 1 expression has not been sufficiently investigated. Therefore, the aim of this study was to examine whether an association between serum CA 125 levels and MDR 1 expression exists. PATIENTS AND METHODS Serum CA 125 levels were measured during the diagnosis of ovarian cancer. Fresh tumor specimens or ascitic fluid samples were studied for MDR 1 expression by the polymerase chain reaction method (PCR). RESULTS Forty patients with ovarian cancer were studied, 34 (85%) of whom had elevated CA 125. Twenty-eight out of the 40 patients were tested for MDR 1 expression; 20 expressed the gene and 8 did not. The median level of CA 125 in specimens expressing the MDR1 gene was 327, and in specimens that did not it was 376. There was no correlation between the CA 125 levels and MDR 1 expression (p = 0.484). CONCLUSION There does not seem to be an association between CA 125 levels and expression of the MDR1 gene in patients with ovarian cancer.
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Affiliation(s)
- E Galani
- Department of Clinical Biochemistry, School of Medicine, University of Athens, Mikras Asias 75, 11527, Athens, Greece.
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Abstract
Histamine receptors of the H2 type are found on mature hemopoetic cells such as lymphocytes and monocytes. Since little is known about histamine receptors on immature cells, we studied histamine-induced cAMP synthesis in leukemic cells of 51 patients using 73 samples of peripheral blood and/or bone marrow. Histamine-induced cAMP synthesis was found in all cALL (FAB L1, L2), but only occasionally in AML. In 1 out of 11 myelomonocytic leukemias (M4), and also in 2 out of 5 monocytic leukemias (FAB M5), histamine-inducible cAMP synthesis was found, but no induction of cAMP synthesis by histamine was found in 19 cases from the remaining subgroups (FAB M1-M3, M6). The inhibiting action of H2 antagonists on cAMP synthesis indicates that the receptor is of the H2 type. Since H2 receptors were found in all cALL blasts, we assume a compulsory expression of this receptor on immature cells of the B-lymphocytic lineage.
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