Sparticle Spectroscopy with Neutralino Dark matter from t-b-tau Quasi-Yukawa Unification

Details Sparticle Spectroscopy with Neutralino Dark matter from t-b-tau Quasi-Yukawa Unification Sparticle Spectroscopy with Neutralino Dark matter from t-b-tau Quasi-Yukawa Unification

2011-05-25

arxiv.org/abs/1105.5122v2

Physics

High Energy Physics

High Energy Physics - Phenomenology

21 pages, 12 figures, 2 tables

Scientific paper

We consider two classes of t-b-tau quasi-Yukawa unification scenarios which can arise from realistic supersymmetric SO(10) and SU(4)_C X SU(2)_L X SU(2)_R models. We show that these scenarios can be successfully implemented in the CMSSM and NUHM1 frameworks, and yields a variety of sparticle spectra with WMAP compatible neutralino dark matter. In NUHM1 we find bino-higgsino dark matter as well as the stau coannihilation and A-funnel solutions. The CMSSM case yields the stau coannihilation and A-funnel solutions. The gluino and squark masses are found to lie in the TeV range.

Affiliated with

Also associated with

No associations

Rating

Sparticle Spectroscopy with Neutralino Dark matter from t-b-tau Quasi-Yukawa Unification 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 Sparticle Spectroscopy with Neutralino Dark matter from t-b-tau Quasi-Yukawa Unification, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Sparticle Spectroscopy with Neutralino Dark matter from t-b-tau Quasi-Yukawa Unification will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-192460