Fermion pair generation in isotropic cosmology

Details Fermion pair generation in isotropic cosmology Fermion pair generation in isotropic cosmology

Mar 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976svphj..19..310m&link_type=abstract

Soviet Physics Journal, Volume 19, Issue 3, pp.310-313

Physics

Scientific paper

The generation of particles with a spin of 1/2 in a nonstationary gravitational field corresponding to the quasi-Euclidian Friedman model is considered. Particle generation probability and particle density are evaluated for both the present epoch and near the cosmological singularity. It is shown that the effect is most significant at t ˜ m-1, where m is the particle mass.

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