Non-Universalities In Dark Matter Detection

Details Non-Universalities In Dark Matter Detection Non-Universalities In Dark Matter Detection

Jan 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997nuphs..52..229a&link_type=abstract

Nuclear Physics B Proceedings Supplements, v. 52, p. 229-234.

Physics

Nuclear Physics

Scientific paper

The existence of dark matter, both on the cosmological scale and locally in the Milky Way is reviewed. Models of cold dark matter (CDM) based on supergravity grand unification with R-partity invariance are examined. In these models, the CDM particles are the lightest neutralino, Z~1. The parameter space for SU(5) and SO(10) models with non-universal soft breaking is examined. It is seen that the minimum event rates can be increased or decreased by a factor of 10-100 (depending on the sign of the non-universal corrections) if 2mZ~1 is in the vicinity of the Z or Higgs mass.

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