Finite temperature effects in primordial inflation

G. B. Gelmini; D. V. Nanopoulos; K. A. Olive

doi:10.1016/0370-2693(83)91090-0

Finite temperature effects in primordial inflation

G. B. Gelmini, D. V. Nanopoulos, K. A. Olive

Physics and Astronomy (Twin Cities)

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Abstract

We present a detailed study of a recently proposed model for primordial inflation based on an N=1 locally supersymmetric potential. For a large class of parameters with which all cosmological constraints are satisfied, the temperature corrections can be neglected during the inflation period. At higher temperatures, the minimum is not at the origin, but very close to it.

Original language	English (US)
Pages (from-to)	53-58
Number of pages	6
Journal	Physics Letters B
Volume	131
Issue number	1-3
DOIs	https://doi.org/10.1016/0370-2693(83)91090-0
State	Published - Nov 10 1983

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title = "Finite temperature effects in primordial inflation",

abstract = "We present a detailed study of a recently proposed model for primordial inflation based on an N=1 locally supersymmetric potential. For a large class of parameters with which all cosmological constraints are satisfied, the temperature corrections can be neglected during the inflation period. At higher temperatures, the minimum is not at the origin, but very close to it.",

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AU - Gelmini, G. B.

AU - Nanopoulos, D. V.

AU - Olive, K. A.

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AB - We present a detailed study of a recently proposed model for primordial inflation based on an N=1 locally supersymmetric potential. For a large class of parameters with which all cosmological constraints are satisfied, the temperature corrections can be neglected during the inflation period. At higher temperatures, the minimum is not at the origin, but very close to it.

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Finite temperature effects in primordial inflation

Abstract

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