Pulsars as the sources of high energy cosmic ray positrons
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Constraining the origin of the rising cosmic ray positron fraction with the boron-to-carbon ratioImplications of CoGeNT and DAMA for light WIMP dark matterFirst 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 StationDirect detection of a break in the teraelectronvolt cosmic-ray spectrum of electrons and positrons.Time Dependence of the Electron and Positron Components of the Cosmic Radiation Measured by the PAMELA Experiment between July 2006 and December 2015.Superexponential cutoff as a probe of annihilating dark matter.New 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.Dark matter annihilation in the first galaxy haloesStudy of the gamma-ray spectrum from the Galactic Center in view of multi-TeV dark matter candidatesCan the Morphology ofγ-Ray Emission Distinguish Annihilating from Decaying Dark Matter?Can the WIMP annihilation boost factor be boosted by the Sommerfeld enhancement?Pulsar-Wind Nebulae and Magnetar Outflows: Observations at Radio, X-Ray, and Gamma-Ray WavelengthsSearches for cosmic-ray electron anisotropies with the Fermi Large Area TelescopeAll-flavour search for neutrinos from dark matter annihilations in the Milky Way with IceCube/DeepCoreCosmic ray acceleration in supernova remnants and the FERMI/PAMELA dataTesting Astrophysical Models for the PAMELA Positron Excess with Cosmic Ray NucleiHigh-Energy Antiprotons from Old Supernova RemnantsPossible causes of a rise with energy of the cosmic ray positron fractionOrigin of the Positron Excess in Cosmic RaysAbout detection of precessing circumpulsar discsThe PAMELA experiment and antimatter in the universeThe PAMELA space mission for antimatter and dark matter searches in spaceDark matter through the axion portal
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P2860
Pulsars as the sources of high energy cosmic ray positrons
description
im Januar 2009 veröffentlichter wissenschaftlicher Artikel
@de
wetenschappelijk artikel
@nl
наукова стаття, опублікована в січні 2009
@uk
name
Pulsars as the sources of high energy cosmic ray positrons
@en
Pulsars as the sources of high energy cosmic ray positrons
@nl
type
label
Pulsars as the sources of high energy cosmic ray positrons
@en
Pulsars as the sources of high energy cosmic ray positrons
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prefLabel
Pulsars as the sources of high energy cosmic ray positrons
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Pulsars as the sources of high energy cosmic ray positrons
@nl
P356
P1476
Pulsars as the sources of high energy cosmic ray positrons
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P2093
Dan Hooper
P304
P356
10.1088/1475-7516/2009/01/025
P407
P577
2009-01-12T00:00:00Z