interactions in Galactic jets as a plausible origin of the positron excess
arXiv:1404.4188 · doi:10.1093/mnras/stu770
Abstract
The positron flux measured near Earth shows a rise with energy beyond 30 GeV. We show that this rise may be compatible with the production of positrons in interactions in the jets of microquasars.
5 pages, 1 figure, to be published in MNRAS
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Cited by in corpus (12)
- Extended gamma-ray sources around pulsars constrain the origin of the positron flux at Earth
- The Phase II Murchison Widefield Array: Design Overview
- Gamma-ray halos around pulsars as the key to understanding cosmic ray transport in the Galaxy
- Cosmic-ray positrons from millisecond pulsars
- GeV observations of the extended pulsar wind nebulae constrain the pulsar interpretations of the cosmic-ray positron excess
- Positrons from Primordial Black Hole Microquasars and Gamma-ray Bursts
- Undiscovered pulsar in the Local Bubble as an explanation of the local high energy cosmic ray all-electron spectrum
- Effect of the diffusion parameters on the observed gamma-ray spectrum of sources and their contribution to the local all-electron spectrum: the EDGE code
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- The Contribution of Millisecond Pulsars to the Galactic Cosmic-Ray Lepton Spectrum
- EDGE: a code to calculate diffusion of cosmic-ray electrons and their gamma-ray emission