Cosmological Coleman-Weinberg potentials and inflation

J. H. Liao, Shun-Pei Miao, R. P. Woodard

Research output: Contribution to journalArticle

Abstract

We consider an additional fine-tuning problem which afflicts scalar-driven models of inflation. The problem is that successful reheating requires the inflaton be coupled to ordinary matter, and quantum fluctuations of this matter induce Coleman-Weinberg potentials which are not Planck suppressed. Unlike the flat space case, these potentials depend upon a still-unknown, nonlocal functional of the metric which reduces to the Hubble parameter for de Sitter. Such a potential cannot be completely subtracted off by any local action. In a simple model we numerically consider one possible subtraction scheme in which the correction is locally subtracted at the beginning of inflation. For fermions the effect is to make the Universe approach de Sitter with a smaller Hubble parameter. For gauge bosons the effect is to make inflation end almost instantly unless the gauge charge is unacceptably small.

Original languageEnglish
Article number103522
JournalPhysical Review D
Volume99
Issue number10
DOIs
Publication statusPublished - 2019 May 15

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subtraction
bosons
universe
fermions
tuning
scalars
heating

All Science Journal Classification (ASJC) codes

  • Physics and Astronomy (miscellaneous)

Cite this

Liao, J. H. ; Miao, Shun-Pei ; Woodard, R. P. / Cosmological Coleman-Weinberg potentials and inflation. In: Physical Review D. 2019 ; Vol. 99, No. 10.
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Cosmological Coleman-Weinberg potentials and inflation. / Liao, J. H.; Miao, Shun-Pei; Woodard, R. P.

In: Physical Review D, Vol. 99, No. 10, 103522, 15.05.2019.

Research output: Contribution to journalArticle

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