Home > Publications database > Towards Understanding the Origin of Cosmic-Ray Positrons > print

001     861500
005     20210130000833.0
024 7 _ |a 10.1103/PhysRevLett.122.041102
|2 doi
024 7 _ |a 0031-9007
|2 ISSN
024 7 _ |a 1079-7114
|2 ISSN
024 7 _ |a 1092-0145
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024 7 _ |a 2128/21861
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024 7 _ |a pmid:30768313
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024 7 _ |a WOS:000457061400002
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024 7 _ |a altmetric:54663511
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037 _ _ |a FZJ-2019-01961
082 _ _ |a 530
100 1 _ |a Aguilar, M.
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245 _ _ |a Towards Understanding the Origin of Cosmic-Ray Positrons
260 _ _ |a College Park, Md.
|c 2019
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336 7 _ |a article
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336 7 _ |a Output Types/Journal article
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336 7 _ |a Journal Article
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336 7 _ |a ARTICLE
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336 7 _ |a JOURNAL_ARTICLE
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336 7 _ |a Journal Article
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520 _ _ |a Precision measurements of cosmic ray positrons are presented up to 1 TeV based on 1.9 million positrons collected by the Alpha Magnetic Spectrometer on the International Space Station. The positron flux exhibits complex energy dependence. Its distinctive properties are (a) a significant excess starting from 25.2±1.8  GeV compared to the lower-energy, power-law trend, (b) a sharp dropoff above $284^{+91}_{−64}  GeV$, (c) in the entire energy range the positron flux is well described by the sum of a term associated with the positrons produced in the collision of cosmic rays, which dominates at low energies, and a new source term of positrons, which dominates at high energies, and (d) a finite energy cutoff of the source term of $E_s =810^{+310}_{−180}  GeV$ is established with a significance of more than 4σ. These experimental data on cosmic ray positrons show that, at high energies, they predominantly originate either from dark matter annihilation or from other astrophysical sources.
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536 _ _ |a Cosmic-ray physics with the AMS experiment on the International Space Station (jara0052_20150501)
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773 _ _ |a 10.1103/PhysRevLett.122.041102
|g Vol. 122, no. 4, p. 041102
|0 PERI:(DE-600)1472655-5
|n 4
|p 041102
|t Physical review letters
|v 122
|y 2019
|x 1079-7114
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Marc 21