English

Proton Decay and Cosmology Strongly Constrain the Minimal SU(5) Supergravity Model

High Energy Physics - Phenomenology 2011-06-08 v1

Abstract

We present the results of an extensive exploration of the five-dimensional parameter space of the minimal SU(5)SU(5) supergravity model, including the constraints of a long enough proton lifetime (τp>1×1032\y\tau_p>1\times10^{32}\y) and a small enough neutralino cosmological relic density (Ωχh021\Omega_\chi h^2_0\le1). We find that the combined effect of these two constraints is quite severe, although still leaving a small region of parameter space with mg~,q~<1\TeVm_{\tilde g,\tilde q}<1\TeV. The allowed values of the proton lifetime extend up to τp1×1033\y\tau_p\approx1\times10^{33}\y and should be fully explored by the SuperKamiokande experiment. The proton lifetime cut also entails the following mass correlations and bounds: mh\lsim100\GeVm_h\lsim100\GeV, mχ12mχ200.15\gluinom_\chi\approx{1\over2}m_{\chi^0_2}\approx0.15\gluino, mχ20mχ1+m_{\chi^0_2}\approx m_{\chi^+_1}, and mχ<85(115)\GeVm_\chi<85\,(115)\GeV, mχ20,χ1+<165(225)\GeVm_{\chi^0_2,\chi^+_1}<165\,(225)\GeV for α3=0.113(0.120)\alpha_3=0.113\,(0.120). Finally, the {\it combined} proton decay and cosmology constraints predict that if mh\gsim75(80)\GeVm_h\gsim75\,(80)\GeV then mχ1+\lsim90(110)\GeVm_{\chi^+_1}\lsim90\,(110)\GeV for α3=0.113(0.120)\alpha_3=0.113\,(0.120). Thus, if this model is correct, at least one of these particles will likely be observed at LEPII.

Keywords

Cite

@article{arxiv.hep-ph/9209220,
  title  = {Proton Decay and Cosmology Strongly Constrain the Minimal SU(5) Supergravity Model},
  author = {J. Lopez and D. Nanopoulos and H. Pois},
  journal= {arXiv preprint arXiv:hep-ph/9209220},
  year   = {2011}
}

Comments

11 pages plus 5 figures (not included). CERN-TH.6628/92, CTP-TAMU-61/92. A condensed version of this paper will appear in the Proceedings of the XXVI International Conference on High Energy Physics, Dallas--Texas, August 5--12, 1992