中文

Towards a unified string supergravity model

高能物理 - 唯象学 2009-08-25 v2

摘要

We present a unified string supergravity model based on a string-derived SU(5)×U(1)SU(5)\times U(1) model and a string-inspired supersymmetry breaking scenario triggered by the FF-term of the universally present dilaton field. This model can be described by three parameters: mtm_t, tanβ\tan\beta, and mg~m_{\tilde g}. We work out the predictions for all sparticle and Higgs masses and discuss the prospects for their detection at the Tevatron, LEPI,II, and HERA. We find that the cosmological neutralino relic density is always within current expectations (\ie, Ωχh02\lsim0.9\Omega_\chi h^2_0\lsim0.9). We also consider a more constrained version of this supersymmetry breaking scenario where the BB-term is specified. In this case tanβ\tan\beta can be determined (tanβ1.41.6\tan\beta\approx1.4-1.6) and implies mt\lsim155\GeVm_t\lsim155\GeV and mh\lsim91\GeVm_h\lsim91\GeV. Thus, continuing Tevatron top-quark searches and LEPI,II Higgs searches could probe this restricted scenario completely.

关键词

引用

@article{arxiv.hep-ph/9306226,
  title  = {Towards a unified string supergravity model},
  author = {J. Lopez and D. Nanopoulos and A. Zichichi},
  journal= {arXiv preprint arXiv:hep-ph/9306226},
  year   = {2009}
}

备注

CERN-TH.6903/93, CTP-TAMU-31/93, plain tex with harvmac, 3 figures. A correction is made on the relation between $m_0$ and $m_{1/2}$, numerical results changed significantly. The manuscript ps file and the three ps figures are available via anonymous ftp site tamsun.tamu.edu in directory incoming, filenames: CTP-TAMU-31-93.ps, CTP-TAMU-31-93a.ps, CTP-TAMU-31-93b.ps, CTP-TAMU-31-93c.ps