Warm inflation and its microphysical basis

被引:254
作者
Berera, Arjun [1 ]
Moss, Ian G. [2 ]
Ramos, Rudnei O. [3 ]
机构
[1] Univ Edinburgh, Sch Phys & Astron, Edinburgh EH9 3JZ, Midlothian, Scotland
[2] Newcastle Univ, Sch Math & Stat, Newcastle Upon Tyne NE1 7RU, Tyne & Wear, England
[3] Univ Estado Rio de Janeiro, Dept Fis Teor, BR-20550013 Rio De Janeiro, Brazil
关键词
EXPECTATION VALUE FORMALISM; FINITE-TEMPERATURE; HYBRID INFLATION; DENSITY PERTURBATIONS; EVOLUTION EQUATION; SCALAR FIELD; HIGGS FIELD; SUPERSYMMETRIC INFLATION; PARTICLE-PRODUCTION; EARLY UNIVERSE;
D O I
10.1088/0034-4885/72/2/026901
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
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.
引用
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页数:25
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