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@ARTICLE{Aguilar:861498,
author = {Aguilar, M. and Ali Cavasonza, L. and Alpat, B. and
Ambrosi, G. and Arruda, L. and Attig, N. and Azzarello, P.
and Bachlechner, A. and Barao, F. and Barrau, A. and Barrin,
L. and Bartoloni, A. and Basara, L. and Başeğmez-du Pree,
S. and Battiston, R. and Becker, U. and Behlmann, M. and
Beischer, B. and Berdugo, J. and Bertucci, B. and Bindi, V.
and de Boer, W. and Bollweg, K. and Borgia, B. and Boschini,
M. J. and Bourquin, M. and Bueno, E. F. and Burger, J. and
Burger, W. J. and Cai, X. D. and Capell, M. and Caroff, S.
and Casaus, J. and Castellini, G. and Cervelli, F. and
Chang, Y. H. and Chen, G. M. and Chen, H. S. and Chen, Y.
and Cheng, L. and Chou, H. Y. and Choutko, V. and Chung, C.
H. and Clark, C. and Coignet, G. and Consolandi, C. and
Contin, A. and Corti, C. and Crispoltoni, M. and Cui, Z. and
Dadzie, K. and Dai, Y. M. and Datta, A. and Delgado, C. and
Della Torre, S. and Demirköz, M. B. and Derome, L. and Di
Falco, S. and Di Felice, V. and Dimiccoli, F. and Díaz, C.
and von Doetinchem, P. and Dong, F. and Donnini, F. and
Duranti, M. and Egorov, A. and Eline, A. and Eronen, T. and
Feng, J. and Fiandrini, E. and Fisher, P. and Formato, V.
and Galaktionov, Y. and García-López, R. J. and Gargiulo,
C. and Gast, H. and Gebauer, I. and Gervasi, M. and
Giovacchini, F. and Gómez-Coral, D. M. and Gong, J. and
Goy, C. and Grabski, V. and Grandi, D. and Graziani, M. and
Guo, K. H. and Haino, S. and Han, K. C. and He, Z. H. and
Heil, M. and Hsieh, T. H. and Huang, H. and Huang, Z. C. and
Incagli, M. and Jia, Yi and Jinchi, H. and Kanishev, K. and
Khiali, B. and Kirn, Th. and Konak, C. and Kounina, O. and
Kounine, A. and Koutsenko, V. and Kulemzin, A. and La Vacca,
G. and Laudi, E. and Laurenti, G. and Lazzizzera, I. and
Lebedev, A. and Lee, H. T. and Lee, S. C. and Leluc, C. and
Li, J. Q. and Li, Q. and Li, T. X. and Li, Z. H. and Light,
C. and Lin, C. H. and Lippert, T. and Liu, F. Z. and Liu, Hu
and Liu, Z. and Lu, S. Q. and Lu, Y. S. and Luebelsmeyer, K.
and Luo, F. and Luo, J. Z. and Luo, Xi and Lyu, S. S. and
Machate, F. and Mañá, C. and Marín, J. and Martin, T. and
Martínez, G. and Masi, N. and Maurin, D. and
Menchaca-Rocha, A. and Meng, Q. and Mo, D. C. and Molero, M.
and Mott, P. and Mussolin, L. and Nelson, T. and Ni, J. Q.
and Nikonov, N. and Nozzoli, F. and Oliva, A. and Orcinha,
M. and Palermo, M. and Palmonari, F. and Paniccia, M. and
Pashnin, A. and Pauluzzi, M. and Pensotti, S. and Perrina,
C. and Phan, H. D. and Picot-Clemente, N. and Plyaskin, V.
and Pohl, M. and Poireau, V. and Popkow, A. and Quadrani, L.
and Qi, X. M. and Qin, X. and Qu, Z. Y. and Rancoita, P. G.
and Rapin, D. and Conde, A. Reina and Rosier-Lees, S. and
Rozhkov, A. and Rozza, D. and Sagdeev, R. and Solano, C. and
Schael, S. and Schmidt, Sebastian M. and von Dratzig, A.
Schulz and Schwering, G. and Seo, E. S. and Shan, B. S. and
Shi, J. Y. and Siedenburg, T. and Song, J. W. and Sun, Z. T.
and Tacconi, M. and Tang, X. W. and Tang, Z. C. and Tian, J.
and Ting, Samuel C. C. and Ting, S. M. and Tomassetti, N.
and Torsti, J. and Urban, T. and Vagelli, V. and Valente, E.
and Valtonen, E. and Acosta, M. Vázquez and Vecchi, M. and
Velasco, M. and Vialle, J. P. and Vizán, J. and Wang, L. Q.
and Wang, N. H. and Wang, Q. L. and Wang, X. and Wang, X. Q.
and Wang, Z. X. and Wei, J. and Weng, Z. L. and Wu, H. and
Xiong, R. Q. and Xu, W. and Yan, Q. and Yang, Y. and Yi, H.
and Yu, Y. J. and Yu, Z. Q. and Zannoni, M. and Zeissler, S.
and Zhang, C. and Zhang, F. and Zhang, J. H. and Zhang, Z.
and Zhao, F. and Zheng, Z. M. and Zhuang, H. L. and Zhukov,
V. and Zichichi, A. and Zimmermann, N. and Zuccon, P.},
title = {{T}owards {U}nderstanding the {O}rigin of {C}osmic-{R}ay
{E}lectrons},
journal = {Physical review letters},
volume = {122},
number = {10},
issn = {1079-7114},
address = {College Park, Md.},
publisher = {APS},
reportid = {FZJ-2019-01959},
pages = {101101},
year = {2019},
abstract = {Precision results on cosmic-ray electrons are presented in
the energy range from 0.5 GeV to 1.4 TeV based on
$28.1×10^6$ electrons collected by the Alpha Magnetic
Spectrometer on the International Space Station. In the
entire energy range the electron and positron spectra have
distinctly different magnitudes and energy dependences. The
electron flux exhibits a significant excess starting from
$42.1^{+5.4}_{−5.2} GeV$ compared to the lower energy
trends, but the nature of this excess is different from the
positron flux excess above 25.2±1.8 GeV. Contrary to
the positron flux, which has an exponential energy cutoff of
$810^{+310}_{−180} GeV$, at the 5σ level the
electron flux does not have an energy cutoff below 1.9 TeV.
In the entire energy range the electron flux is well
described by the sum of two power law components. The
different behavior of the cosmic-ray electrons and positrons
measured by the Alpha Magnetic Spectrometer is clear
evidence that most high energy electrons originate from
different sources than high energy positrons.},
cin = {JSC / VS-I / JARA-HPC},
ddc = {530},
cid = {I:(DE-Juel1)JSC-20090406 / I:(DE-Juel1)VS-I-20090406 /
$I:(DE-82)080012_20140620$},
pnm = {513 - Supercomputer Facility (POF3-513) / Cosmic-ray
physics with the AMS experiment on the International Space
Station $(jara0052_20150501)$},
pid = {G:(DE-HGF)POF3-513 / $G:(DE-Juel1)jara0052_20150501$},
typ = {PUB:(DE-HGF)16},
pubmed = {pmid:30932626},
UT = {WOS:000461070200003},
doi = {10.1103/PhysRevLett.122.101101},
url = {https://juser.fz-juelich.de/record/861498},
}
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