| Literature DB >> 25494065 |
M Aguilar1, D Aisa2, B Alpat3, A Alvino3, G Ambrosi3, K Andeen4, L Arruda5, N Attig6, P Azzarello7, A Bachlechner8, F Barao5, A Barrau9, L Barrin10, A Bartoloni11, L Basara12, M Battarbee13, R Battiston14, J Bazo3, U Becker15, M Behlmann15, B Beischer8, J Berdugo1, B Bertucci2, G Bigongiari16, V Bindi17, S Bizzaglia3, M Bizzarri2, G Boella18, W de Boer4, K Bollweg19, V Bonnivard9, B Borgia20, S Borsini3, M J Boschini21, M Bourquin22, J Burger15, F Cadoux22, X D Cai15, M Capell15, S Caroff23, J Casaus1, V Cascioli3, G Castellini24, I Cernuda1, F Cervelli25, M J Chae26, Y H Chang27, A I Chen15, H Chen15, G M Cheng28, H S Chen28, L Cheng29, A Chikanian30, H Y Chou27, E Choumilov15, V Choutko15, C H Chung8, C Clark19, R Clavero31, G Coignet23, C Consolandi17, A Contin32, C Corti17, B Coste14, M Crispoltoni2, Z Cui29, M Dai33, C Delgado1, S Della Torre21, M B Demirköz34, L Derome9, S Di Falco25, L Di Masso2, F Dimiccoli14, C Díaz1, P von Doetinchem17, F Donnini2, W J Du29, M Duranti3, D D'Urso3, A Eline15, F J Eppling15, T Eronen13, Y Y Fan35, L Farnesini3, J Feng23, E Fiandrini2, A Fiasson23, E Finch30, P Fisher15, Y Galaktionov15, G Gallucci36, B García1, R García-López31, C Gargiulo10, H Gast8, I Gebauer4, M Gervasi18, A Ghelfi9, W Gillard27, F Giovacchini1, P Goglov15, J Gong37, C Goy23, V Grabski38, D Grandi21, M Graziani39, C Guandalini32, I Guerri16, K H Guo40, M Habiby22, S Haino41, K C Han42, Z H He40, M Heil15, J Hoffman27, T H Hsieh15, Z C Huang40, C Huh43, M Incagli25, M Ionica3, W Y Jang43, H Jinchi42, K Kanishev14, G N Kim43, K S Kim43, Th Kirn8, R Kossakowski23, O Kounina15, A Kounine15, V Koutsenko15, M S Krafczyk15, S Kunz4, G La Vacca44, E Laudi2, G Laurenti32, I Lazzizzera14, A Lebedev15, H T Lee35, S C Lee35, C Leluc22, H L Li35, J Q Li37, Q Li15, Q Li15, T X Li40, W Li45, Y Li22, Z H Li28, Z Y Li35, S Lim26, C H Lin35, P Lipari11, T Lippert6, D Liu35, H Liu37, T Lomtadze25, M J Lu14, Y S Lu28, K Luebelsmeyer8, F Luo29, J Z Luo37, S S Lv40, R Majka30, A Malinin46, C Mañá1, J Marín1, T Martin19, G Martínez1, N Masi32, D Maurin9, A Menchaca-Rocha38, Q Meng37, D C Mo40, L Morescalchi25, P Mott19, M Müller8, J Q Ni40, N Nikonov4, F Nozzoli3, P Nunes5, A Obermeier8, A Oliva1, M Orcinha5, F Palmonari32, C Palomares1, M Paniccia22, A Papi3, M Pauluzzi2, E Pedreschi25, S Pensotti18, R Pereira47, F Pilo25, A Piluso2, C Pizzolotto3, V Plyaskin15, M Pohl22, V Poireau23, E Postaci34, A Putze23, L Quadrani32, X M Qi40, T Räihä8, P G Rancoita21, D Rapin22, J S Ricol9, I Rodríguez1, S Rosier-Lees23, A Rozhkov15, D Rozza21, R Sagdeev48, J Sandweiss30, P Saouter22, C Sbarra32, S Schael8, S M Schmidt6, D Schuckardt4, A Schulz von Dratzig8, G Schwering8, G Scolieri3, E S Seo46, B S Shan45, Y H Shan45, J Y Shi37, X Y Shi15, Y M Shi49, T Siedenburg8, D Son43, F Spada11, F Spinella25, W Sun15, W H Sun15, M Tacconi18, C P Tang40, X W Tang28, Z C Tang28, L Tao23, D Tescaro31, Samuel C C Ting15, S M Ting15, N Tomassetti9, J Torsti13, C Türkoğlu34, T Urban19, V Vagelli4, E Valente20, C Vannini25, E Valtonen13, S Vaurynovich15, M Vecchi23, M Velasco1, J P Vialle23, L Q Wang29, Q L Wang33, R S Wang49, X Wang15, Z X Wang40, Z L Weng15, K Whitman17, J Wienkenhöver8, H Wu37, X Xia1, M Xie15, S Xie49, R Q Xiong37, G M Xin29, N S Xu40, W Xu50, Q Yan28, J Yang26, M Yang28, Q H Ye49, H Yi37, Y J Yu33, Z Q Yu28, S Zeissler4, J H Zhang37, M T Zhang40, X B Zhang40, Z Zhang40, Z M Zheng45, H L Zhuang28, V Zhukov8, A Zichichi32, N Zimmermann8, P Zuccon15, C Zurbach51.
Abstract
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).Entities:
Year: 2014 PMID： 25494065 DOI： 10.1103/PhysRevLett.113.221102
Source DB: PubMed Journal: Phys Rev Lett ISSN： 0031-9007 Impact factor: 9.161