Relic density of dark matter in mSUGRA and non-universal SUGRA

Details Relic density of dark matter in mSUGRA and non-universal SUGRA Relic density of dark matter in mSUGRA and non-universal SUGRA

2004-12-21

arxiv.org/abs/hep-ph/0412309v1

Czech.J.Phys. 55 (2005) B205-B212

Physics

High Energy Physics

High Energy Physics - Phenomenology

8 pages, 3 figures, Invited talk at Physics at LHC, Vienna, July 2004

Scientific paper

The measurements of WMAP on the relic density of dark matter strongly
constrain supersymmetric models. In mSUGRA where the neutralino LSP is mostly a
bino only rather fine-tuned models survive. On the other hand the relic density
upper limit can be easily satisfied in models with a Higgsino or wino LSP.

Affiliated with

Also associated with

No associations

Rating

Relic density of dark matter in mSUGRA and non-universal SUGRA 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 Relic density of dark matter in mSUGRA and non-universal SUGRA, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Relic density of dark matter in mSUGRA and non-universal SUGRA will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-121557