After primordial inflation

D. V. Nanopoulos, K. A. Olive, M. Srednicki

Research output: Contribution to journalArticlepeer-review

212 Scopus citations

Abstract

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.

Original languageEnglish (US)
Pages (from-to)30-34
Number of pages5
JournalPhysics Letters B
Volume127
Issue number1-2
DOIs
StatePublished - Jul 21 1983
Externally publishedYes

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