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Title The Alpha Magnetic Spectrometer (AMS) on the international space station: Part II — Results from the first seven years
Author(s)

Aguilar, M (Madrid, CIEMAT) ; Ali Cavasonza, L (Aachen, Tech. Hochsch.) ; Ambrosi, G (INFN, Perugia) ; Arruda, L (LIP, Lisbon ; Lisbon, CFTP) ; Attig, N (IAS, Julich ; JCHP, Julich) ; Barao, F (LIP, Lisbon ; Lisbon, CFTP) ; Barrin, L (CERN) ; Bartoloni, A (INFN, Rome) ; Başeğmez-du Pree, S (Kapteyn Astron. Inst., Groningen) ; Bates, J (NASA, Houston) ; Battiston, R (TIFPA-INFN, Trento ; Trento U.) ; Behlmann, M (MIT) ; Beischer, B (Aachen, Tech. Hochsch.) ; Berdugo, J (Madrid, CIEMAT) ; Bertucci, B (INFN, Perugia ; Perugia U.) ; Bindi, V (Hawaii U.) ; de Boer, W (KIT, Karlsruhe, ETP) ; Bollweg, K (NASA, Houston) ; Borgia, B (INFN, Rome ; U. Rome La Sapienza (main)) ; Boschini, M J (INFN, Milan Bicocca) ; Bourquin, M (Geneva U.) ; Bueno, E F (Kapteyn Astron. Inst., Groningen) ; Burger, J (MIT) ; Burger, W J (TIFPA-INFN, Trento) ; Burmeister, S (Kiel U.) ; Cai, X D (MIT) ; Capell, M (MIT) ; Casaus, J (Madrid, CIEMAT) ; Castellini, G (INOA, Florence) ; Cervelli, F (INFN, Pisa) ; Chang, Y H (Taiwan, Inst. Phys. ; Taiwan, Natl. Central U.) ; Chen, G M (Beijing, Inst. High Energy Phys. ; Beijing, GUCAS) ; Chen, H S (Beijing, Inst. High Energy Phys. ; Beijing, GUCAS) ; Chen, Y (Geneva U.) ; Cheng, L (Shandong U.) ; Chou, H Y (Taiwan, Natl. Central U.) ; Chouridou, S (Aachen, Tech. Hochsch.) ; Choutko, V (MIT) ; Chung, C H (Aachen, Tech. Hochsch.) ; Clark, C (MIT ; NASA, Houston) ; Coignet, G (Annecy, LAPP) ; Consolandi, C (Hawaii U.) ; Contin, A (INFN, Bologna ; Bologna U.) ; Corti, C (Hawaii U.) ; Cui, Z (Shandong U. ; Shandong U.) ; Dadzie, K (MIT) ; Dai, Y M (Inst. Electr. Engin., Beijing) ; Delgado, C (Madrid, CIEMAT) ; Della Torre, S (INFN, Milan Bicocca) ; Demirköz, M B (Middle East Tech. U., Ankara) ; Derome, L (LPSC, Grenoble) ; Di Falco, S (INFN, Pisa) ; Di Felice, V (INFN, Rome2) ; Díaz, C (Madrid, CIEMAT) ; Dimiccoli, F (TIFPA-INFN, Trento) ; von Doetinchem, P (Hawaii U.) ; Dong, F (Southeast U., Nanjing) ; Donnini, F (INFN, Rome2) ; Duranti, M (INFN, Perugia) ; Egorov, A (MIT) ; Eline, A (MIT) ; Feng, J (MIT) ; Fiandrini, E (INFN, Perugia ; Perugia U.) ; Fisher, P (MIT) ; Formato, V (INFN, Rome2) ; Freeman, C (Hawaii U.) ; Galaktionov, Y (MIT) ; Gámez, C (Madrid, CIEMAT) ; García-López, R J (IAC, La Laguna ; Laguna U., Tenerife) ; Gargiulo, C (CERN) ; Gast, H (Aachen, Tech. Hochsch.) ; Gebauer, I (KIT, Karlsruhe, ETP) ; Gervasi, M (INFN, Milan Bicocca ; Milan Bicocca U.) ; Giovacchini, F (Madrid, CIEMAT) ; Gómez-Coral, D M (Hawaii U.) ; Gong, J (Southeast U., Nanjing) ; Goy, C (Annecy, LAPP) ; Grabski, V (Mexico U.) ; Grandi, D (INFN, Milan Bicocca ; Milan Bicocca U.) ; Graziani, M (INFN, Perugia ; Perugia U.) ; Guo, K H (SYSU, Guangzhou) ; Haino, S (Taiwan, Inst. Phys.) ; Han, K C (CSIST, Taiwan) ; Hashmani, R K (Middle East Tech. U., Ankara) ; He, Z H (SYSU, Guangzhou) ; Heber, B (Kiel U.) ; Hsieh, T H (MIT) ; Hu, J Y (Beijing, Inst. High Energy Phys. ; Beijing, GUCAS) ; Huang, Z C (SYSU, Guangzhou) ; Hungerford, W (NASA, Houston) ; Incagli, M (INFN, Pisa) ; Jang, W Y (CHEP, Taegu) ; Jia, Yi (MIT) ; Jinchi, H (CSIST, Taiwan) ; Kanishev, K (TIFPA-INFN, Trento) ; Khiali, B (INFN, Rome2) ; Kim, G N (CHEP, Taegu) ; Kirn, Th (Aachen, Tech. Hochsch.) ; Konyushikhin, M (MIT) ; Kounina, O (MIT) ; Kounine, A (MIT) ; Koutsenko, V (MIT) ; Kuhlman, A (Hawaii U.) ; Kulemzin, A (MIT) ; La Vacca, G (INFN, Milan Bicocca ; Milan Bicocca U.) ; Laudi, E (CERN) ; Laurenti, G (INFN, Bologna) ; Lazzizzera, I (TIFPA-INFN, Trento ; Trento U.) ; Lebedev, A (MIT) ; Lee, H T (Taipei, Computing Ctr.) ; Lee, S C (Taiwan, Inst. Phys.) ; Leluc, C (Geneva U.) ; Li, J Q (Southeast U., Nanjing) ; Li, M (Aachen, Tech. Hochsch.) ; Li, Q (Southeast U., Nanjing) ; Li, S (Aachen, Tech. Hochsch.) ; Li, T X (SYSU, Guangzhou) ; Li, Z H (Beijing, Inst. High Energy Phys.) ; Light, C (Hawaii U.) ; Lin, C H (Taiwan, Inst. Phys.) ; Lippert, T (IAS, Julich ; JCHP, Julich) ; Liu, Z (Geneva U.) ; Lu, S Q (SYSU, Guangzhou) ; Lu, Y S (Beijing, Inst. High Energy Phys.) ; Luebelsmeyer, K (Aachen, Tech. Hochsch.) ; Luo, J Z (Southeast U., Nanjing) ; Lyu, S S (SYSU, Guangzhou) ; Machate, F (Aachen, Tech. Hochsch.) ; Mañá, C (Madrid, CIEMAT) ; Marín, J (Madrid, CIEMAT) ; Marquardt, J (Kiel U.) ; Martin, T (MIT ; NASA, Houston) ; Martínez, G (Madrid, CIEMAT) ; Masi, N (INFN, Bologna ; Bologna U.) ; Maurin, D (LPSC, Grenoble) ; Menchaca-Rocha, A (Mexico U.) ; Meng, Q (Southeast U., Nanjing) ; Mo, D C (SYSU, Guangzhou) ; Molero, M (Madrid, CIEMAT) ; Mott, P (MIT ; NASA, Houston) ; Mussolin, L (INFN, Perugia ; Perugia U.) ; Ni, J Q (SYSU, Guangzhou) ; Nikonov, N (Aachen, Tech. Hochsch.) ; Nozzoli, F (TIFPA-INFN, Trento) ; Oliva, A (INFN, Bologna) ; Orcinha, M (LIP, Lisbon ; Lisbon, CFTP) ; Palermo, M (Hawaii U.) ; Palmonari, F (INFN, Bologna ; Bologna U.) ; Paniccia, M (Geneva U.) ; Pashnin, A (MIT) ; Pauluzzi, M (INFN, Perugia ; Perugia U.) ; Pensotti, S (INFN, Milan Bicocca ; Milan Bicocca U.) ; Phan, H D (MIT) ; Plyaskin, V (MIT) ; Pohl, M (Geneva U.) ; Porter, S (NASA, Houston) ; Qi, X M (SYSU, Guangzhou) ; Qin, X (MIT) ; Qu, Z Y (Taiwan, Inst. Phys.) ; Quadrani, L (INFN, Bologna ; Bologna U.) ; Rancoita, P G (INFN, Milan Bicocca) ; Rapin, D (Geneva U.) ; Reina Conde, A (IAC, La Laguna ; Laguna U., Tenerife) ; Rosier-Lees, S (Annecy, LAPP) ; Rozhkov, A (MIT) ; Rozza, D (INFN, Milan Bicocca ; Milan Bicocca U.) ; Sagdeev, R (Maryland U.) ; Schael, S (Aachen, Tech. Hochsch.) ; Schmidt, S M (IAS, Julich ; JCHP, Julich) ; Schulz von Dratzig, A (Aachen, Tech. Hochsch.) ; Schwering, G (Aachen, Tech. Hochsch.) ; Seo, E S (Maryland U.) ; Shan, B S (Beihang U.) ; Shi, J Y (Southeast U., Nanjing) ; Siedenburg, T (Aachen, Tech. Hochsch.) ; Solano, C (MIT) ; Song, J W (Shandong U.) ; Sonnabend, R (Aachen, Tech. Hochsch.) ; Sun, Q (Shandong U.) ; Sun, Z T (Beijing, Inst. High Energy Phys. ; Beijing, GUCAS) ; Tacconi, M (INFN, Milan Bicocca ; Milan Bicocca U.) ; Tang, X W (Beijing, Inst. High Energy Phys.) ; Tang, Z C (Beijing, Inst. High Energy Phys.) ; Tian, J (INFN, Perugia ; Perugia U.) ; Ting, Samuel C C (MIT ; CERN) ; Ting, S M (MIT) ; Tomassetti, N (INFN, Perugia ; Perugia U.) ; Torsti, J (Turku U.) ; Tüysüz, C (Middle East Tech. U., Ankara) ; Urban, T (MIT ; NASA, Houston) ; Usoskin, I (Oulu U.) ; Vagelli, V (ASI, Rome ; INFN, Perugia) ; Vainio, R (Turku U.) ; Valente, E (INFN, Rome ; U. Rome La Sapienza (main)) ; Valtonen, E (Turku U.) ; Vázquez Acosta, M (IAC, La Laguna ; Laguna U., Tenerife) ; Vecchi, M (Kapteyn Astron. Inst., Groningen) ; Velasco, M (Madrid, CIEMAT) ; Vialle, J P (Annecy, LAPP) ; Wang, L Q (Shandong U.) ; Wang, N H (Shandong U.) ; Wang, Q L (Inst. Electr. Engin., Beijing) ; Wang, S (Hawaii U.) ; Wang, X (MIT) ; Wang, Z X (SYSU, Guangzhou) ; Wei, J (Geneva U.) ; Weng, Z L (MIT) ; Wu, H (Southeast U., Nanjing) ; Xiong, R Q (Southeast U., Nanjing) ; Xu, W (Shandong U. ; Shandong U.) ; Yan, Q (MIT) ; Yang, Y (Taiwan, Natl. Cheng Kung U.) ; Yi, H (Southeast U., Nanjing) ; Yu, Y J (Inst. Electr. Engin., Beijing) ; Yu, Z Q (Beijing, Inst. High Energy Phys.) ; Zannoni, M (INFN, Milan Bicocca ; Milan Bicocca U.) ; Zhang, C (Beijing, Inst. High Energy Phys.) ; Zhang, F (Beijing, Inst. High Energy Phys.) ; Zhang, F Z (Beijing, Inst. High Energy Phys. ; Beijing, GUCAS) ; Zhang, J H (Southeast U., Nanjing) ; Zhang, Z (MIT) ; Zhao, F (Beijing, Inst. High Energy Phys. ; Beijing, GUCAS) ; Zheng, Z M (Beihang U.) ; Zhuang, H L (Beijing, Inst. High Energy Phys.) ; Zhukov, V (Aachen, Tech. Hochsch.) ; Zichichi, A (INFN, Bologna ; Bologna U.) ; Zimmermann, N (Aachen, Tech. Hochsch.) ; Zuccon, P (TIFPA-INFN, Trento ; Trento U.)

Publication 2021
Number of pages 116
In: Phys. Rep. 894 (2021) 1-116
DOI 10.1016/j.physrep.2020.09.003
Subject category Astrophysics and Astronomy
Accelerator/Facility, Experiment AMS
Abstract The Alpha Magnetic Spectrometer (AMS) is a precision particle physics detector on the International Space Station (ISS) conducting a unique, long-duration mission of fundamental physics research in space. The physics objectives include the precise studies of the origin of dark matter, antimatter, and cosmic rays as well as the exploration of new phenomena. Following a 16-year period of construction and testing, and a precursor flight on the Space Shuttle, AMS was installed on the ISS on May 19, 2011. In this report we present results based on 120 billion charged cosmic ray events up to multi-TeV energies. This includes the fluxes of positrons, electrons, antiprotons, protons, and nuclei. These results provide unexpected information, which cannot be explained by the current theoretical models. The accuracy and characteristics of the data, simultaneously from many different types of cosmic rays, provide unique input to the understanding of origins, acceleration, and propagation of cosmic rays.
Related document Part I: Phys. Rep. 366 (2002) 331-405
Copyright/License © 2020-2025 The Authors (License: CC-BY-NC-ND-4.0)

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 Notice créée le 2021-02-09, modifiée le 2021-02-10


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