English

Yukawa Unification in SO(10)

High Energy Physics - Phenomenology 2009-07-09 v3

Abstract

In simple SO(10) SUSY GUTs the top, bottom and tau Yukawa couplings unify at the GUT scale. A naive renormalization group analysis, neglecting weak scale threshold corrections, leads to moderate agreement with the low energy data. However it is known that intrinsically large threshold corrections proportional to tanβmt(MZ)/mb(MZ)50\tan\beta \sim m_t(M_Z)/m_b(M_Z) \sim 50 can nullify these t,bt, b, τ\tau mass predictions. In this paper we turn the argument around. Instead of predicting fermion masses, we use the constraint of Yukawa unification and the observed values Mt,mb(mb),MτM_t, m_b(m_b), M_\tau to constrain SUSY parameter space. We find a narrow region survives for μ>0\mu > 0 with μ,M1/2<<m16\mu, M_{1/2} << m_{16}, A01.9m16A_0 \approx - 1.9 m_{16} and m16>1200m_{16} > 1200 \gev. Demanding Yukawa unification thus makes definite predictions for Higgs and sparticle masses. In particular we find a light higgs with mass mh0=114±5±3m_h^0 = 114 \pm 5 \pm 3 GeV and a light stop with (mt~1)MIN450(m_{\tilde t_1})_{MIN} \sim 450 GeV and mt~1<<mb~1m_{\tilde t_1} << m_{\tilde b_1}. In addition, we find a light chargino and a neutralino LSP. It is also significant that in this region of parameter space the SUSY contribution to the muon anomalous magnetic moment aμSUSY<16×1010a_\mu^{SUSY} < 16 \times 10^{-10}.

Keywords

Cite

@article{arxiv.hep-ph/0201081,
  title  = {Yukawa Unification in SO(10)},
  author = {T. Blazek and R. Dermisek and S. Raby},
  journal= {arXiv preprint arXiv:hep-ph/0201081},
  year   = {2009}
}

Comments

30 pages, 20 figures, revised version to be published in Phys. Rev. D

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