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

Physics – High Energy Physics – High Energy Physics - Phenomenology

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

8 pages - version to appear in Phys.Lett.B ; discussion of one loop annihilation cross-section modified, conclusions unchanged

Scientific paper

10.1016/j.physletb.2006.12.025

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.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Natural gravitino dark matter in SO(10) gauge mediated supersymmetry breaking does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Natural gravitino dark matter in SO(10) gauge mediated supersymmetry breaking, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Natural gravitino dark matter in SO(10) gauge mediated supersymmetry breaking will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-279665

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.