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Warm inflation and its microphysical basis

2008/08/31 by Arjun Berera, Ian G. Moss, Rudnei O. Ramos · 17 citations
Physics and Astronomy · #Advanced Thermodynamics and Statistical Mechanics #Black Holes and Theoretical Physics #Cosmology and Gravitation Theories #Dissipation #Field (mathematics) #Inflation (cosmology) #Physics #Quantum #Quantum field theory #Quantum gravity #Quantum mechanics #Statistical physics #Theoretical physics #Thermal #Thermal quantum field theory #Thermodynamics #astro-ph.CO #gr-qc #hep-ph #hep-th

paper · pdf · doi:10.1088/0034-4885/72/2/026901

published as Rept.Prog.Phys.72:026901,2009 · 34 pages, 8 figures. Invited review article for Reports on Progress in Physics, In Press 2009

openalex publication_date 2009/01/26 · arxiv created 2009/01/28 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/06

Abstract

The microscopic quantum field theory origins of warm inflation dynamics are reviewed. The warm inflation scenario is first described along with its results, predictions and comparison with the standard cold inflation scenario. The basics of thermal field theory required in the study of warm inflation are discussed. Quantum field theory real time calculations at finite temperature are then presented and the derivation of dissipation and stochastic fluctuations are shown from a general perspective. Specific results are given of dissipation coefficients for a variety of quantum field theory interaction structures relevant to warm inflation, in a form that can be readily used by model builders. Different particle physics models realizing warm inflation are presented along with their observational predictions.

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