Yukawa Unification, b --> s gamma and Bino-Stau Coannihilation

Physics – High Energy Physics – High Energy Physics - Phenomenology

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

16 pages including 3 figures, Revtex, major revisions are made

Scientific paper

10.1016/S0370-2693(00)00841-8

The minimal supersymmetric standard model with universal boundary conditions and "asymptotic" Yukawa unification is considered. The full one-loop effective potential for radiative electroweak symmetry breaking as well as the one-loop corrections to the charged Higgs boson, b-quark and tau lepton masses are included. The CP-even Higgs boson masses are corrected to two-loops. The relic abundance of the lightest supersymmetric particle (bino) is calculated by including its coannihilations with the next-to-lightest supersymmetric particle (lightest stau) consistently with Yukawa unification. The branching ratio of b --> s gamma is evaluated by incorporating all the applicable next-to-leading order QCD corrections. The bino-stau coannihilations reduce the bino relic abundance below the upper bound from cold dark matter considerations in a sizable fraction of the parameter space allowed by b --> s gamma for mu>0. Thus, the mu>0 case, which also predicts an acceptable b-quark mass, is perfectly compatible with data.

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

Yukawa Unification, b --> s gamma and Bino-Stau Coannihilation 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 Yukawa Unification, b --> s gamma and Bino-Stau Coannihilation, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Yukawa Unification, b --> s gamma and Bino-Stau Coannihilation will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-73102

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