Calculations of relic densities in the early universe

Details Calculations of relic densities in the early universe Calculations of relic densities in the early universe

Dec 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988nuphb.310..693s&link_type=abstract

Nuclear Physics B, Volume 310, Issue 3-4, p. 693-713.

Physics

Nuclear Physics

160

Scientific paper

The cosmological relic densities of stable particles are calculated to
high precision. The results depend on assumptions made about the
quark-hadron phase transition. We discuss in detail the calculation of
the thermally averaged annihilation cross section. We consider the
specific cases of photinos, higgsinos, and Dirac and Majorana neutrinos.

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