Sparticle spectroscopy with neutralino dark matter from t-b-tau quasi-Yukawa unification

Dar S., Gogoladze I., Shafi Q., Uen C. S.

PHYSICAL REVIEW D, vol.84, no.8, 2011 (SCI-Expanded) identifier identifier

  • Publication Type: Article / Article
  • Volume: 84 Issue: 8
  • Publication Date: 2011
  • Doi Number: 10.1103/physrevd.84.085015
  • Journal Name: PHYSICAL REVIEW D
  • Journal Indexes: Science Citation Index Expanded (SCI-EXPANDED), Scopus
  • Bursa Uludag University Affiliated: No

Abstract

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 nonuniversal Higgs model with m(Hu) = m(Hd) not equal m(0) and the constrained minimal sumersymmetric model frameworks, and they yield a variety of sparticle spectra with Wilkinson Microwave Anisotropy Probe compatible neutralino dark matter. In the nonuniversal Higgs model with m(Hu) = m(Hd) not equal m(0), we find bino-Higgsino dark matter as well as the stau coannihilation and A-funnel solutions. The constrained minimal sumersymmetric model case yields the stau coannihilation and A-funnel solutions. The gluino and squark masses are found to lie in the TeV range.