After primordial inflation

Details After primordial inflation After primordial inflation

Jul 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983phlb..127...30n&link_type=abstract

Physics Letters B, Volume 127, Issue 1-2, p. 30-34.

Physics

163

Scientific paper

We consider the history of the early universe in the locally supersymmetric model we have previously discussed. We pay particular attention to the requirement of converting the quanta of the field which drives primordial inflation (inflatons) to ordinary particles which can produce the cosmological baryon asymmetry without producing too many gravitinos. An inflaton mass of about 1013 GeV (a natural value in our model) produces a completely acceptable scenario.

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