Renormalization of nonequilibrium dynamics in FRW cosmology
- 15 November 1997
- journal article
- research article
- Published by American Physical Society (APS) in Physical Review D
- Vol. 56 (10) , 6556-6565
- https://doi.org/10.1103/physrevd.56.6556
Abstract
We derive the renormalized nonequilibrium equations of motion for a scalar field and its quantum back reaction in a conformally flat Friedmann-Robertson-Walker universe. We use a fully covariant formalism proposed by us recently for handling numerically and analytically nonequilibrium dynamics in the one-loop approximation. The system is assumed to be in a conformal vacuum state initially. We use dimensional regularization; we find that the counterterms can be chosen independent of the initial conditions though the divergent leading order graphs do depend on them. [S0556-2821(97)00822-9].All Related Versions
This publication has 26 references indexed in Scilit:
- Towards the theory of reheating after inflationPhysical Review D, 1997
- Scalar field dynamics in Friedmann-Robertson-Walker spacetimesPhysical Review D, 1997
- Universe reheating after inflationPhysical Review D, 1995
- Reheating after InflationPhysical Review Letters, 1994
- Nonequilibrium evolution of scalar fields in FRW cosmologiesPhysical Review D, 1994
- Particle Physics and Inflationary CosmologyPublished by Taylor & Francis ,1990
- Closed-time-path functional formalism in curved spacetime: Application to cosmological back-reaction problemsPhysical Review D, 1987
- Effective field equations for expectation valuesPhysical Review D, 1986
- Particle production in the new inflationary cosmologyPhysics Letters B, 1982
- Baryon asymmetry in the inflationary universePhysics Letters B, 1982