Precision measurement of the (e++e-) flux in primary cosmic rays from 0.5 GeV to 1 TeV with the alpha magnetic spectrometer on the international space station

Please use this identifier to cite or link to this item: https://ir.lib.ncu.edu.tw/handle/987654321/105592

Title:	Precision measurement of the (e++e-) flux in primary cosmic rays from 0.5 GeV to 1 TeV with the alpha magnetic spectrometer on the international space station
Authors:	張元翰;Beischer, B;Bizzaglia, S;Barrau, A;Shan, Y H;Yu, Y J;Consolandi, C;Nozzoli, F;Schmidt, S M;Battarbee, M;Lee, H T;Lee, S C;Xin, G M;Vecchi, M;Wang, Z X;Bachlechner, A;He, Z H;Chen, H;Berdugo, J;Yan, Q;García, B;Hsieh, T H;Battiston, R;Yi, H;Corti, C;Cui, Z;Luo, J Z;Rancoita, P G;Chou, H Y;Sbarra, C;Heil, M;Tang, X W;Gargiulo, C;Fiasson, A;Grandi, D;Li, H L;Paniccia, M;Choumilov, E;Aisa, D;Spinella, F;Zhuang, H L;Guo, K H;Gillard, W;Ionica, M;von Doetinchem, P;Shi, Y M;Huang, Z C;Xu, W;Bizzarri, M;Lim, S;Du, W J;Wienkenhöver, J;Cheng, G M;Kunz, S;Di Masso, L;Lv, S S;García-López, R;Xu, N S;Zhang, M T;Crispoltoni, M;Pereira, R;Zichichi, A;Kim, G N;Mo, D C;Li, Z H;Lin, C H;Marín, J;Quadrani, L;Eronen, T;Sagdeev, R;Rosier-Lees, S;Eline, A;Bartoloni, A;Fan, Y Y;Galaktionov, Y;Martínez, G;Putze, A;Gebauer, I;Li, W;Velasco, M;Li, Q;Lippert, T;Bollweg, K;Schuckardt, D;de Boer, W;Nunes, P;Menchaca-Rocha, A;Müller, M;Jang, W Y;Poireau, V;Lu, Y S;Tao, L;Alpat, B;Li, T X;Tang, C P;Rozza, D;Finch, E;Lebedev, A;Schael, S;Barao, F;Zurbach, C
Contributors:	理學院物理學系
Keywords:	Alpha Magnetic Spectrometer;Astrophysics;Astrophysics and Astronomy;Cosmic rays;Cosmology and Extra-Galactic Astrophysics;Experiment;Flux;International Space Station;Particle Physics;Physics;Power law;Primary cosmic rays;Spectra;Statistics
Date:	2014-11-26
Issue Date:	2026-04-23 12:40:22 (UTC+8)
Publisher:	American Physical Society;United States: American Physical Society
Abstract:	摘要： We present a measurement of the cosmic ray ($e^+ + e^−$) flux in the range 0.5 GeV to 1 TeV based on the analysis of 10.6 million ($e^+ + e^−$) events collected by AMS. The statistics and the resolution of AMS provide a precision measurement of the flux. The flux is smooth and reveals new and distinct information. Above 30.2 GeV, the flux can be described by a single power law with a spectral index γ=−3.170±0.008(stat+syst)±0.008(energy scale). 其他題名： Phys Rev Lett 出版者： United States: American Physical Society 出版日期： 2014-11-28 出處： Physical review letters, 2014-11, Vol.113 (22), p.221102, Article 221102 資源來源： American Physical Society Journals 版權： licence_http://creativecommons.org/publicdomain/zero 識別號： ISSN: 0031-9007 識別號： ISSN: 1079-7114 識別號： EISSN: 1079-7114 識別號： DOI: 10.1103/PhysRevLett.113.221102 識別號： PMID: 25494065
Appears in Collections:	[Department of Physics] journal & Dissertation

Files in This Item:

File	Description	Size	Format
index.html		0Kb	HTML	16	View/Open

社群 sharing

Loading...