Neutralino relic density from minimal supergravity: direct detection vs. collider searches.

Details Neutralino relic density from minimal supergravity: direct detection vs. collider searches. Neutralino relic density from minimal supergravity: direct detection vs. collider searches.

Dec 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998phr...307..201b&link_type=abstract

Physics Reports, Vol. 307, No. 1 - 4, p. 201 - 206

Physics

1

Cosmology: Elementary Particles

Scientific paper

Working within the framework of the minimal supergravity (mSUGRA) model, the author shows regions of model parameter space which lead to cosmologically interesting values of the neutralino relic density Ωh2. In these regions, he also shows expected event rates for direct detection of neutralinos by a germanium detector. The author compares the direct dark matter detection event rates with expected decay rates for b→sγ. He also compares neutralino direct detection rates with the reach of various colliding beam experiments for mSUGRA. He presents results for both small and large values of the parameter tan β.

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