Diffuse gamma ray constraints on annihilating or decaying dark matter after Fermi

DOI10.1016/j.nuclphysb.2010.07.010zbMath1206.85014arXiv0912.0663OpenAlexW2147869517WikidataQ58022520 ScholiaQ58022520MaRDI QIDQ627898

Marco Cirelli, Paolo Panci, Pasquale D. Serpico

Publication date: 4 March 2011

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

Full work available at URL: https://arxiv.org/abs/0912.0663

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Radiative transfer in astronomy and astrophysics (85A25)

Related Items (8)

RELIC DENSITY AND PAMELA EVENTS IN A HEAVY WINO DARK MATTER MODEL WITH SOMMERFELD EFFECT ⋮ A warped model of dark matter ⋮ Decaying dark matter in supersymmetric model and cosmic-ray observations ⋮ Decaying dark matter in the supersymmetric standard model with freeze-in and seesaw mechanims ⋮ Phenomenology of dark matter from \(A_{4}\) flavor symmetry ⋮ Goldstini as the decaying dark matter ⋮ Cosmic ray anomalies from the MSSM? ⋮ 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
• Inverse compton constraints on the dark matter \(e^{\pm }\) excesses

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