Thermal properties of an inflationary universe

Arjun Berera*

*Corresponding author for this work

Research output: Contribution to journalArticlepeer-review

Abstract / Description of output

An energetic justification of a thermal component during inflation is given. The thermal component can act as a heat reservoir which induces thermal fluctuations on the inflaton field system. We showed previously that such thermal fluctuations could dominate quantum fluctuations in producing the initial seeds of density perturbations. A Langevin-like rate equation is derived from quantum field theory which describes the production of fluctuations in the inflaton field when acted upon by a simple modeled heat reservoir. In a certain limit this equation is shown to reduce to the standard Langevin equation, which we used to construct "warm inflation" scenarios in previous work. A particle physics interpretation of our system-reservoir model is offered.

Original languageEnglish
Pages (from-to)2519-2534
Number of pages16
JournalPhysical Review D, particles, fields, gravitation, and cosmology
Volume54
Issue number4
Publication statusPublished - 15 Aug 1996

Fingerprint

Dive into the research topics of 'Thermal properties of an inflationary universe'. Together they form a unique fingerprint.

Cite this