arXiv Analytics

Sign in

arXiv:hep-ph/0504021AbstractReferencesReviewsResources

Natural gravitino dark matter in SO(10) gauge mediated supersymmetry breaking

Martin Lemoine, Gilbert Moultaka, Karsten Jedamzik

Published 2005-04-04, updated 2006-12-11Version 2

It is shown that gravitinos with mass m_{3/2} ~ 0.1-1 MeV may provide suitable cold dark matter candidates in scenarios of gauge mediated supersymmetry breaking (GMSB) under SO(10) grand unification coupled to supergravity, which accommodate a messenger sector of mass scale M_X ~ 10^6 GeV. This is due to the combined effects of renormalizable loop-suppressed operators and generic non-renormalizable ones governing the dilution of a pre-existing equilibrium gravitino abundance via messenger decay. The above range of gravitino and messenger masses can be accommodated in indirect GMSB scenarios. The gravitino abundance does not depend on the post-inflationary reheat temperature and it is shown that leptogenesis can generate successfully the baryon asymmetry.

Comments: 8 pages - version to appear in Phys.Lett.B ; discussion of one loop annihilation cross-section modified, conclusions unchanged
Journal: Phys.Lett.B645:222-227,2007
Categories: hep-ph, astro-ph, gr-qc, hep-th
Related articles: Most relevant | Search more
arXiv:hep-ph/0506129 (Published 2005-06-14, updated 2006-05-09)
Gravitino dark matter in gauge mediated supersymmetry breaking
arXiv:hep-ph/0208191 (Published 2002-08-21, updated 2002-10-27)
Natural Gravitino Dark Matter and Thermal Leptogenesis in Gauge-Mediated Supersymmetry Breaking Models
arXiv:hep-ph/9511381 (Published 1995-11-21)
Particle Production and Gravitino Abundance after Inflation