Accès ouvert déclaré
2018
article
Observation of New Properties of Secondary Cosmic Rays Lithium, Beryllium, and Boron by the Alpha Magnetic Spectrometer on the International Space Station
M. Aguilar, L. Ali Cavasonza, G. Ambrosi, L. Arruda, N. Attig, S. Aupetit, P. Azzarello, A. Bachlechner, F. Barão, Aurélien Barrau, L. Barrin, A. Bartoloni, L. Basara, Seth Pree, Markus Battarbee, R. Battiston, U. Becker, M. Behlmann, B. Beischer, J. Berdugo, B. Bertucci, K. F. Bindel, V. Bindi, W. De Boer, K. Bollweg, V. Bonnivard, B. Borgia, M. J. Boschini, M. Bourquin, E. F. Bueno, J.D. Burger, W. J. Burger, F. Cadoux, X.D. Cai, M. Capell, Sami Caroff, J. Casaus, G. Castellini, F. Cervelli, M. J. Chae, Y. H. Chang, A. I. Chen, G. M. Chen, H. S. Chen, Lin Cheng, H. Y. Chou, E. Choumilov, V. Choutko, C. H. Chung, C. Clark, R. Clavero, G. Coignet, C. Consolandi, A. Contin, C. Corti, W. Creus, M. Crispoltoni, Z. Cui, S. Kokou Dadzie, Ye Dai, A. Datta, S. Della Torre, B. Demirköz, L. Derome, S. Di Falco, F. Dimiccoli, C. Díaz, P. von Doetinchem, Fei Dong, F. Donnini, M. Duranti, D. D’Urso, A. I. Egorov, A. Eline, T. Eronen, J. H. Feng, E. Fiandrini, P.H. Fisher, V. Formato, Yu. Galaktionov, G. Gallucci, R. J. Garcı́a López, Corrado Gargiulo, H. Gast, Iris Gebauer, M. Gervasi, A. Ghelfi, F. Giovacchini, D. M. Gómez-Coral, J. Gong, C. Goy, Varlen Grabski, D. Grandi, M. Graziani, K. H. Guo, S. Haino, K. C. Han, Z. H. He, M. Heil, Timothy H. Hsieh, H. Huang, Z. C. Huang, C. Huh, M. Incagli, M. Ionica, W. Jang, Yi Jia, H. Jinchi, S.C. Kang, K. Kanishev, B. Khiali, G. N. Kim, K. S. Kim, Th. Kirn, O. Kounina, A. Kounine, V. Koutsenko, A. Kulemzin, G. La Vacca, E. Laudi, G. Laurenti, I. Lazzizzera, A. Lebedev, H. T. Lee, S.C. Lee, C. Leluc, H. S. Li, J. Q. Li, Q. Li, T. X. Li, Yang Li, Zongshu Li, Z. Y. Li, Soobin Lim, Chao‐Hung Lin, P. Lipari, Thomas Lippert, D. Liu, Hu Liu, V. D. Lordello, S. Q. Lu, Y.S. Lu, K. Luebelsmeyer, Feng Luo, J. Luo, Shaoyu Lyu, F. Machate, C. Mañá, J. Marín, T. Martin, G. Martı́nez, N. Masi, D. Maurin, A. Menchaca-Rocha, Q. Meng, V. M. Mikuni, Dong-Chuan Mo, P. Mott, T. Nelson, J. Q. Ni, N. Nikonov, F. Nozzoli, A. Oliva, M. Orcinha, M. Palermo, F. Palmonari, C. Palomares, M. Paniccia, M. Pauluzzi, S. Pensotti, C. Perrina, H. D. Phan, N. Picot-Clémente, F. Pilo, C. Pizzolotto, V. Plyaskin, M. Pohl, V. Poireau, L. Quadrani, X. M. Qi, X. Qin, Z. H. Qu, T. Räihä, P.G. Rancoita, D. Rapin, Jean-Stephane Ricol, S. Rosier-Lees, A. Rozhkov, D. Rozza, R. Z. Sagdeev, S. Schael, Susann Schmidt, A. Schulz von Dratzig, G. Schwering, E. S. Seo, B. S. Shan, Jianzheng Shi, T. Siedenburg, D. Son, Jiwei Song, M. Tacconi, Xiao Tang, Zhi-Cheng Tang, D. Tescaro, Samuel C.C. Ting, S. M. Ting, Nicola Tomassetti, J. Torsti, C. Türkoğlu, T. Urban, V. Vagelli, E. Valente, E. Valtonen, M. Vázquez Acosta, M. Vecchi, M. Velasco, J. P. Vialle, V. Vitale, L. Q. Wang, N. H. Wang, Qiuliang Wang, X. Wang, X. Q. Wang, Z. X. Wang, Chuncheng Wei, Z. Weng, Kathryn Whitman, H. Wu, X. Wu, R. Q. Xiong, W. Xu, Qi Yan, J. Yang, Mao Yang, Y. Yang, Hemian Yi, Yaxin Yu, Z. Q. Yu, M. Zannoni, S. Zeissler, Cheng Zhang, Fei Zhang, J. Zhang, J. H. Zhang, S. W. Zhang, Z. Zhang, Z. M. Zheng, H. L. Zhuang, V. Zhukov, A. Zichichi, N. Zimmermann, P. Zuccon
267Citations signalées, ce qui n’est pas une note de qualité
52Institutions déclarées
14Pays d’affiliation déclarés
Rattachement africain : es, de, it, pt, fr, ch, cn, fi, us, br, kr, tw, tr, mx.
Niveau de preuve : code pays fourni par la source.
Le résumé fourni par la source
We report on the observation of new properties of secondary cosmic rays Li, Be, and B measured in the rigidity (momentum per unit charge) range 1.9 GV to 3.3 TV with a total of 5.4×10^{6} nuclei collected by AMS during the first five years of operation aboard the International Space Station. The Li and B fluxes have an identical rigidity dependence above 7 GV and all three fluxes have an identical rigidity dependence above 30 GV with the Li/Be flux ratio of 2.0±0.1. The three fluxes deviate from a single power law above 200 GV in an identical way. This behavior of secondary cosmic rays has also been observed in the AMS measurement of primary cosmic rays He, C, and O but the rigidity dependences of primary cosmic rays and of secondary cosmic rays are distinctly different. In particular, above 200 GV, the secondary cosmic rays harden more than the primary cosmic rays.
Ce résumé expose les affirmations des auteurs. BNTIC ne l’interprète pas comme une validation indépendante des résultats.
Le contrôle bibliographique ouvert
DOI retrouvé dans Crossref DOI retrouvé ; titre concordant.
- Titre Crossref
- Observation of New Properties of Secondary Cosmic Rays Lithium, Beryllium, and Boron by the Alpha Magnetic Spectrometer on the International Space Station
- Date Crossref
- 11/01/2018
- Éditeur
- American Physical Society (APS)
- Type
- journal-article
Ce recoupement confirme des métadonnées liées au DOI. Il ne confirme ni la méthode ni les conclusions de l’étude, et il ne compte pas comme une seconde source scientifique indépendante.
Les institutions déclarées
Centro de Investigaciones Energéticas, Medioambientales y TecnológicasRWTH Aachen UniversityIstituto Nazionale di Fisica Nucleare, Sezione di PerugiaLIP - Laboratory of Instrumentation and Experimental Particle PhysicsJülich Aachen Research AllianceCentre National de la Recherche ScientifiqueInstitut National de Physique Nucléaire et de Physique des ParticulesLaboratoire de Physique Subatomique et de CosmologieUniversité Grenoble AlpesUniversity of GenevaEuropean Organization for Nuclear ResearchIstituto Nazionale di Fisica Nucleare, Sezione di Roma IIstituto Nazionale di Fisica Nucleare, Trento Institute for Fundamental Physics And ApplicationsChinese Academy of SciencesInstitute of High Energy PhysicsUniversity of TurkuUniversity of TrentoMassachusetts Institute of TechnologyUniversity of PerugiaKarlsruhe Institute of TechnologyUniversity of Hawaii SystemNational Aeronautics and Space AdministrationJohnson Space CenterSapienza University of RomeIstituto Nazionale di Fisica Nucleare, Sezione di Milano BicoccaUniversidade Federal de São CarlosUniversidade de São PauloLaboratoire d’Annecy de Physique des ParticulesUniversité Savoie Mont BlancIstituto Nazionale di Fisica Nucleare, Sezione di PisaEwha Womans UniversityNational Central UniversityUniversity of Chinese Academy of SciencesShandong UniversityUniversidad de La LagunaInstituto de Astrofísica de CanariasIstituto Nazionale di Fisica Nucleare, Sezione di BolognaUniversity of BolognaInstitute of Physics, Academia SinicaInstitute of Electrical EngineeringMiddle East Technical UniversitySoutheast UniversityUniversity of Milano-BicoccaUniversidad Nacional Autónoma de MéxicoSun Yat-sen UniversityNational Chung Shan Institute of Science and TechnologyKyungpook National UniversityGenomics Research Center, Academia SinicaNational Cheng Kung UniversityUniversity of Maryland, College ParkEast–West CenterBeihang University
Une affiliation ne permet pas de déduire la nationalité d’un auteur.
Les sujets associés
Dark Matter and Cosmic PhenomenaAstrophysics and Cosmic PhenomenaRadiation Therapy and Dosimetry