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000861500 005__ 20210130000833.0
000861500 0247_ $$2doi$$a10.1103/PhysRevLett.122.041102
000861500 0247_ $$2ISSN$$a0031-9007
000861500 0247_ $$2ISSN$$a1079-7114
000861500 0247_ $$2ISSN$$a1092-0145
000861500 0247_ $$2Handle$$a2128/21861
000861500 0247_ $$2pmid$$apmid:30768313
000861500 0247_ $$2WOS$$aWOS:000457061400002
000861500 0247_ $$2altmetric$$aaltmetric:54663511
000861500 037__ $$aFZJ-2019-01961
000861500 082__ $$a530
000861500 1001_ $$0P:(DE-HGF)0$$aAguilar, M.$$b0$$eCorresponding author
000861500 245__ $$aTowards Understanding the Origin of Cosmic-Ray Positrons
000861500 260__ $$aCollege Park, Md.$$bAPS$$c2019
000861500 3367_ $$2DRIVER$$aarticle
000861500 3367_ $$2DataCite$$aOutput Types/Journal article
000861500 3367_ $$0PUB:(DE-HGF)16$$2PUB:(DE-HGF)$$aJournal Article$$bjournal$$mjournal$$s1582019974_521
000861500 3367_ $$2BibTeX$$aARTICLE
000861500 3367_ $$2ORCID$$aJOURNAL_ARTICLE
000861500 3367_ $$00$$2EndNote$$aJournal Article
000861500 520__ $$aPrecision 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.
000861500 536__ $$0G:(DE-HGF)POF3-513$$a513 - Supercomputer Facility (POF3-513)$$cPOF3-513$$fPOF III$$x0
000861500 536__ $$0G:(DE-Juel1)jara0052_20150501$$aCosmic-ray physics with the AMS experiment on the International Space Station (jara0052_20150501)$$cjara0052_20150501$$fCosmic-ray physics with the AMS experiment on the International Space Station$$x1
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