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First Result from the Alpha Magnetic Spectrometer on the International Space Station: Precision Measurement of the Positron Fraction in Primary Cosmic Rays of 0.5–350 GeV

M. Aguilar32,20, G. Alberti42,43, B. Alpat42, A. Alvino42,43, G. Ambrosi42, K. Andeen28, H. Anderhub54, L. Arruda30, P. Azzarello42,21,* et al. (AMS Collaboration)

P. Azzarello42,21,*, A. Bachlechner1, F. Barao30, B. Baret22, A. Barrau22, L. Barrin20, A. Bartoloni47, L. Basara5, A. Basili11, L. Batalha30, J. Bates25, R. Battiston42,43,46, J. Bazo42, R. Becker11, U. Becker11, M. Behlmann11, B. Beischer1, J. Berdugo32, P. Berges11, B. Bertucci42,43, G. Bigongiari44,45, A. Biland54, V. Bindi24, S. Bizzaglia42, G. Boella36,37, W. de Boer28, K. Bollweg25, J. Bolmont38, B. Borgia47,48, S. Borsini42,43, M. J. Boschini36, G. Boudoul22, M. Bourquin21, P. Brun5, M. Buénerd22, J. Burger11, W. Burger43, F. Cadoux5,21, X. D. Cai11, M. Capell11, D. Casadei9,10, J. Casaus32, V. Cascioli42,43, G. Castellini18, I. Cernuda32, F. Cervelli44, M. J. Chae49, Y. H. Chang12, A. I. Chen11, C. R. Chen26, H. Chen11, G. M. Cheng8, H. S. Chen8, L. Cheng50, N. Chernoplyiokov39, A. Chikanian41, E. Choumilov11, V. Choutko11, C. H. Chung1, C. Clark25, R. Clavero29, G. Coignet5, V. Commichau54, C. Consolandi36,24, A. Contin9,10, C. Corti24, M. T. Costado Dios29, B. Coste22, D. Crespo32, Z. Cui50, M. Dai7, C. Delgado32, S. Della Torre36,37, B. Demirkoz4, P. Dennett11, L. Derome22, S. Di Falco44, X. H. Diao23, A. Diago29, L. Djambazov54, C. Díaz32, P. von Doetinchem1, W. J. Du50, J. M. Dubois5, R. Duperay22, M. Duranti42,43, D. D’Urso42,20, A. Egorov11, A. Eline11, F. J. Eppling11, T. Eronen53, J. van Es17, H. Esser1, A. Falvard38, E. Fiandrini42,43, A. Fiasson5, E. Finch41, P. Fisher11, K. Flood11, R. Foglio22, M. Fohey25, S. Fopp1, N. Fouque5, Y. Galaktionov11, M. Gallilee11, L. Gallin-Martel22, G. Gallucci44, B. García32, J. García32, R. García-López29, L. García-Tabares32, C. Gargiulo47,11, H. Gast1, I. Gebauer28, S. Gentile47,48, M. Gervasi36,37, W. Gillard22, F. Giovacchini32, L. Girard5, P. Goglov11, J. Gong40, C. Goy-Henningsen5, D. Grandi36, M. Graziani42,43, A. Grechko39, A. Gross1, I. Guerri44,45, C. de la Guía32, K. H. Guo23, M. Habiby21, S. Haino42,12, F. Hauler28, Z. H. He23, M. Heil28, J. Heilig25, R. Hermel5, H. Hofer54, Z. C. Huang23, W. Hungerford11,25, M. Incagli44,11, M. Ionica42,43, A. Jacholkowska38, W. Y. Jang16, H. Jinchi31, M. Jongmanns54,†, L. Journet5, L. Jungermann28, W. Karpinski1, G. N. Kim16, K. S. Kim16, Th. Kirn1, R. Kossakowski5, A. Koulemzine11, O. Kounina11, A. Kounine11, V. Koutsenko11, M. S. Krafczyk11, E. Laudi42,43,‡, G. Laurenti9, C. Lauritzen25, A. Lebedev11, M. W. Lee16, S. C. Lee52, C. Leluc21, H. León Vargas33, V. Lepareur5, J. Q. Li40, Q. Li40, T. X. Li23, W. Li6, Z. H. Li8, P. Lipari47, C. H. Lin52, D. Liu52, H. Liu40, T. Lomtadze44, Y. S. Lu8, S. Lucidi42, K. Lübelsmeyer1, J. Z. Luo40, W. Lustermann54, S. Lv23, J. Madsen2, R. Majka41, A. Malinin14, C. Mañá32, J. Marín32, T. Martin25, G. Martínez32, F. Masciocchi21, N. Masi9,10, D. Maurin22, A. McInturff15, P. McIntyre15, A. Menchaca-Rocha33, Q. Meng40, M. Menichelli42, I. Mereu42,43, M. Millinger1, D. C. Mo23, M. Molina§, P. Mott25, A. Mujunen27, S. Natale1,52, P. Nemeth25, J. Q. Ni23, N. Nikonov28, F. Nozzoli42,19, P. Nunes30, A. Obermeier28, S. Oh49, A. Oliva42,43,32, F. Palmonari9,10, C. Palomares32, M. Paniccia5,21, A. Papi42, W. H. Park16, M. Pauluzzi42,43, F. Pauss54, A. Pauw17, E. Pedreschi44, S. Pensotti36,37, R. Pereira30, E. Perrin21, G. Pessina36,37, G. Pierschel1, F. Pilo44, A. Piluso42,43, C. Pizzolotto42,19, V. Plyaskin11, J. Pochon5,29, M. Pohl21, V. Poireau5, S. Porter25, J. Pouxe22, A. Putze1, L. Quadrani9,10, X. N. Qi23, P. G. Rancoita36, D. Rapin21, Z. L. Ren52, J. S. Ricol22, E. Riihonen53, I. Rodríguez32, U. Roeser54, S. Rosier-Lees5, L. Rossi35,20, A. Rozhkov11, D. Rozza36,37,20, A. Sabellek28, R. Sagdeev13, J. Sandweiss41, B. Santos30, P. Saouter21, M. Sarchioni42, S. Schael1, D. Schinzel11, M. Schmanau28, G. Schwering1, A. Schulz von Dratzig1, G. Scolieri42, E. S. Seo14, B. S. Shan6, J. Y. Shi40, Y. M. Shi51, T. Siedenburg1, R. Siedling1, D. Son16, F. Spada47, F. Spinella44, M. Steuer11, K. Stiff15, W. Sun11, W. H. Sun40, X. H. Sun23, M. Tacconi36,37, C. P. Tang23, X. W. Tang8, Z. C. Tang8, L. Tao5, J. Tassan-Viol5, Samuel C. C. Ting11, S. M. Ting11, C. Titus11, N. Tomassetti42,43, F. Toral32, J. Torsti53, J. R. Tsai26, J. C. Tutt25, J. Ulbricht54, T. Urban25, V. Vagelli28, E. Valente47, C. Vannini44, E. Valtonen53, M. Vargas Trevino22, S. Vaurynovich11, M. Vecchi12, M. Vergain11, B. Verlaat3, C. Vescovi22, J. P. Vialle5, G. Viertel54, G. Volpini34,35, D. Wang26, N. H. Wang50, Q. L. Wang7, R. S. Wang51, X. Wang11, Z. X. Wang23, W. Wallraff1, Z. L. Weng23,52, M. Willenbrock11, M. Wlochal1, H. Wu40, K. Y. Wu6,52, Z. S. Wu23, W. J. Xiao23, S. Xie51, R. Q. Xiong40, G. M. Xin50, N. S. Xu23, W. Xu8, Q. Yan8, J. Yang49, M. Yang8, Q. H. Ye51, H. Yi40, Y. J. Yu7, Z. Q. Yu8, S. Zeissler28, J. G. Zhang40, Z. Zhang23, M. M. Zhang23, Z. M. Zheng6, H. L. Zhuang8, V. Zhukov1, A. Zichichi9,10, P. Zuccon42,11, and C. Zurbach38 (AMS Collaboration)

  • 1I. Physikalisches Institut B, RWTH, D-52056 Aachen, Germany∥
  • 2Department of Physics and Astronomy, University of Aarhus, DK-8000 Aarhus C, Denmark
  • 3National Institute for Nuclear Physics and High Energy Physics, NIKHEF, NL-1098 SJ Amsterdam, Netherlands
  • 4Department of Physics, Middle East Technical University, METU, 06800 Ankara, Turkey
  • 5Laboratoire d’Annecy-Le-Vieux de Physique des Particules, LAPP, IN2P3/CNRS and Université de Savoie, F-74941 Annecy-le-Vieux, France
  • 6Beihang University, BUAA, Beijing, 100191, China
  • 7Institute of Electrical Engineering, IEE, Chinese Academy of Sciences, Beijing, 100080, China
  • 8Institute of High Energy Physics, IHEP, Chinese Academy of Sciences, Beijing, 100039, China¶
  • 9INFN-Sezione di Bologna, I-40126 Bologna, Italy**
  • 10Università di Bologna, I-40126 Bologna, Italy
  • 11Massachusetts Institute of Technology, MIT, Cambridge, Massachusetts 02139, USA
  • 12National Central University, NCU, Chung-Li, Tao Yuan 32054, Taiwan
  • 13East-West Center for Space Science, University of Maryland, College Park, Maryland 20742, USA
  • 14IPST, University of Maryland, College Park, Maryland 20742, USA
  • 15Department of Physics, Texas A&M University, College Station, Texas 77843, USA
  • 16CHEP, Kyungpook National University, 702-701 Daegu, Korea
  • 17National Aerospace Laboratory, NLR, NL-8300 AD Emmeloord, Netherlands
  • 18CNR–IROE, I-50125 Firenze, Italy
  • 19ASDC ESRIN, I-00044 Frascati, Italy
  • 20European Organization for Nuclear Research, CERN, CH-1211 Geneva 23, Switzerland
  • 21DPNC, Université de Genève, CH-1211 Genève 4, Switzerland
  • 22Laboratoire de Physique subatomique et de cosmologie, LPSC, IN2P3/CNRS and Université Joseph Fourier, Grenoble INP, F-38026 Grenoble, France
  • 23Sun Yat-sen University, SYSU, Guangzhou, 510275, China
  • 24University of Hawaii, Physics and Astronomy Department, 2505 Correa Road, WAT 432; Honolulu, Hawaii 96822, USA
  • 25NASA, National Aeronautics and Space Administration, Johnson Space Center, JSC, and Jacobs-Sverdrup, Houston, Texas 77058, USA
  • 26National Space Organization, Hsin-Chu City, 300, Taiwan
  • 27Metsahovi Radio Observatory, Helsinki University of Technology, FIN-02540 Kylmala, Finland
  • 28Institut für Experimentelle Kernphysik, Karlsruhe Institute of Technology, KIT, D-76128 Karlsruhe, Germany∥
  • 29Instituto de Astrofísica de Canarias, IAC, E-38205, La Laguna, Tenerife, Spain
  • 30Laboratório de Instrumentação e Física Experimental de Partículas, LIP, P-1000 Lisboa, Portugal
  • 31Chung-Shan Institute of Science and Technology, Lung-Tan, Tao Yuan 325, Taiwan
  • 32Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas, CIEMAT, E-28040 Madrid, Spain††
  • 33Instituto de Física, Universidad Nacional Autónoma de México, UNAM, México, D. F., 01000 México
  • 34INFN-Sezione di Milano, I-20090 Milano, Italy
  • 35Università di Milano, I-20090 Milano, Italy
  • 36INFN-Sezione di Milano–Bicocca, I-20126 Milano, Italy**
  • 37Università di Milano–Bicocca, I-20126 Milano, Italy**
  • 38Laboratoire Univers et Particules de Montpellier, LUPM (ex LPTA), IN2P3/CNRS and Université de Montpellier II, F-34095 Montpellier, France
  • 39Kurchatov Institute, Russian Research Centre, Moscow, 123182, Russia
  • 40Southeast University, SEU, Nanjing, 210096, China
  • 41Physics Department, Yale University, New Haven, Connecticut 06520, USA
  • 42INFN-Sezione di Perugia, I-06100 Perugia, Italy**
  • 43Università di Perugia, I-06100 Perugia, Italy**
  • 44INFN-Sezione di Pisa, I-56100 Pisa, Italy**
  • 45Università di Pisa, I-56100 Pisa, Italy**
  • 46INFN-TIFPA and Università di Trento, I-38123 Povo, Trento, Italy**
  • 47INFN-Sezione di Roma 1, I-00185 Roma, Italy**
  • 48Università di Roma La Sapienza, I-00185 Roma, Italy**
  • 49Department of Physics, Ewha Womans University, Seoul, 120-750, Korea
  • 50Shandong University, SDU, Jinan, Shandong, 250100, China
  • 51Shanghai Jiaotong University, SJTU, Shanghai, 200030, China
  • 52Institute of Physics, Academia Sinica, Nankang, Taipei 11529, Taiwan
  • 53Space Research Laboratory, Department of Physics, University of Turku, FIN-20014 Turku, Finland
  • 54Institute for Particle Physics, ETH Zürich, CH-8093 Zürich, Switzerland

  • *Present address: ISDC, CH-1290 Versoix, Switzerland.
  • †Deceased.
  • ‡Present address: OHB, D-28359 Bremen, Germany.
  • §Present address: Selex ES, I–20014 Nerviano MI, Italy.
  • ∥Supported by the Deutsches Zentrum für Luft- und Raumfahrt, DLR.
  • Supported by the National Natural Science Foundation of China.
  • **Also supported by the Italian Space Agency, ASI.
  • ††Also supported by SEIDI and CPAN.

Phys. Rev. Lett. 110, 141102 – Published 3 April, 2013

DOI: https://doi.org/10.1103/PhysRevLett.110.141102

Abstract

A precision measurement by the Alpha Magnetic Spectrometer on the International Space Station of the positron fraction in primary cosmic rays in the energy range from 0.5 to 350 GeV based on 6.8×106 positron and electron events is presented. The very accurate data show that the positron fraction is steadily increasing from 10 to ∼250  GeV, but, from 20 to 250 GeV, the slope decreases by an order of magnitude. The positron fraction spectrum shows no fine structure, and the positron to electron ratio shows no observable anisotropy. Together, these features show the existence of new physical phenomena.

Viewpoint

Positrons Galore

Published 3 April, 2013

The first results from the space-borne Alpha Magnetic Spectrometer confirm an unexplained excess of high-energy positrons in Earth-bound cosmic rays.

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