Astrophysical models for the origin of the positron “excess”
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Physics at the [Formula: see text] linear colliderFirst Result from the Alpha Magnetic Spectrometer on the International Space Station: Precision Measurement of the Positron Fraction in Primary Cosmic Rays of 0.5–350 GeVHigh Statistics Measurement of the Positron Fraction in Primary Cosmic Rays of 0.5–500 GeV with the Alpha Magnetic Spectrometer on the International Space StationElectron and Positron Fluxes in Primary Cosmic Rays Measured with the Alpha Magnetic Spectrometer on the International Space StationNew limits on dark matter annihilation from Alpha Magnetic Spectrometer cosmic ray positron data.Three-dimensional model of cosmic-ray lepton propagation reproduces data from the Alpha Magnetic Spectrometer on the International Space Station.Study of the gamma-ray spectrum from the Galactic Center in view of multi-TeV dark matter candidatesAMS-02 data confront acceleration of cosmic ray secondaries in nearby sourcesOn the magnetohydrodynamic modelling of the Crab nebula radio emissionSearch for dark matter annihilation signatures in H.E.S.S. observations of dwarf spheroidal galaxiesThe origin of galactic cosmic rays
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Astrophysical models for the origin of the positron “excess”
description
article
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im Dezember 2012 veröffentlichter wissenschaftlicher Artikel
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wetenschappelijk artikel
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наукова стаття, опублікована в грудні 2012
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name
Astrophysical models for the origin of the positron “excess”
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Astrophysical models for the origin of the positron “excess”
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type
label
Astrophysical models for the origin of the positron “excess”
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Astrophysical models for the origin of the positron “excess”
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prefLabel
Astrophysical models for the origin of the positron “excess”
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Astrophysical models for the origin of the positron “excess”
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P1476
Astrophysical models for the origin of the positron “excess”
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P356
10.1016/J.ASTROPARTPHYS.2011.08.007
P407
P577
2012-12-01T00:00:00Z