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Gravitino dark matter in R-parity breaking vacua

  • Wilfried Buchmüller
  • , Laura Covi
  • , Koichi Hamaguchi
  • , Alejandro Ibarra
  • , Tsutomu T. Yanagida
  • Deutsches Elektronen-Synchrotron (DESY)
  • University of Tokyo

Research output: Contribution to journalArticlepeer-review

218 Scopus citations

Abstract

We show that in the case of small R-parity and lepton number breaking couplings, primordial nucleosynthesis, thermal leptogenesis and gravitino dark matter are naturally consistent for gravitino masses m3/25 GeV. We present a model where R-parity breaking is tied to B-L breaking, which predicts the needed small couplings. The metastable next-to-lightest superparticle has a decay length that is typically larger than a few centimeters, with characteristic signatures at the LHC. The photon flux produced by relic gravitino decays may be part of the apparent excess in the extragalactic diffuse gamma-ray flux obtained from the EGRET data for a gravitino mass m 3/2 ∼ 10 GeV. In this case, a clear signal can be expected from GLAST in the near future.

Original languageEnglish
Article number037
JournalJournal of High Energy Physics
Volume2007
Issue number3
DOIs
StatePublished - 1 Mar 2007
Externally publishedYes

Keywords

  • Cosmology of theories beyond the SM
  • Supergravity models
  • Supersymmetry phenomenology

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