After primordial inflation

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

doi:10.1016/0370-2693(83)91624-6

After primordial inflation

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

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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 language	English (US)
Pages (from-to)	30-34
Number of pages	5
Journal	Physics Letters B
Volume	127
Issue number	1-2
DOIs	https://doi.org/10.1016/0370-2693(83)91624-6
State	Published - Jul 21 1983
Externally published	Yes

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10.1016/0370-2693(83)91624-6

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title = "After primordial inflation",

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.",

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AU - Olive, K. A.

AU - Srednicki, M.

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After primordial inflation

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