Inverse compton constraints on the dark matter \(e^{\pm }\) excesses

DOI10.1016/j.nuclphysb.2009.06.034zbMath1196.83035arXiv0904.3830OpenAlexW2065820329MaRDI QIDQ1960088

Paolo Panci, Marco Cirelli

Publication date: 12 October 2010

Published in: Nuclear Physics. B (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/0904.3830

zbMATH Keywords

PAMELAgalactic halo at large

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Galactic and stellar structure (85A15) Radiative transfer in astronomy and astrophysics (85A25)

Related Items (4)

Diffuse gamma ray constraints on annihilating or decaying dark matter after Fermi ⋮ Constraining dark matter properties with gamma-rays from the Galactic Center with \(Fermi\)-LAT ⋮ Radiative bound-state-formation cross-sections for dark matter interacting via a Yukawa potential ⋮ ELECTRON/POSITRON EXCESSES IN THE COSMIC RAY SPECTRUM AND POSSIBLE INTERPRETATIONS

Cites Work

• Model-independent implications of the \(e^{\pm }\), \(\bar{p}\) cosmic ray spectra on properties of Dark Matter

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