SUSY dark matter in nonuniversal gaugino mass models

18th International Symposium on Particles Strings and Cosmology

Roy, D.P.^1

Homi Bhabha Centre for Science Education, Tata Institute of Fundamental Research, Mumbai 400088, India^1

关键词: Dark matter;    Model prediction;    Non-universal gaugino mass;    Parameter spaces;    Predictive models;   

Others  :  https://iopscience.iop.org/article/10.1088/1742-6596/485/1/012003/pdf
DOI  :  10.1088/1742-6596/485/1/012003

来源: IOP

【 摘 要 】

We discuss the SUSY dark matter phenomenology in some simple and predictive models of nonuniversal gaugino masses at the GUT scale. Assuming the gaugino masses to transform as a sum of singlet and a nonsinglet representation of the GUT group SU(5), one can evade the LEP constraints to access the bulk annihilation region of the bino dark matter relic density. Besides, with this assumption one can also have a mixed gaugino-higgsino dark matter, giving the right relic density over large parts of the parameter space. We consider the model predictions for LHC and dark matter experiments in both the cases. Finally we consider the AMSB model prediction of wino dark matter giving the right relic density for TeV scale wino mass. Assuming this wino dark matter mass to be at the first Sommerfeld resonance of ∼ 4 TeV one can simultaneously reproduce the right relic density as well as the hard positron spectrum observed by the PAMELA experiment. -