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• W1966490192 abstract "We calculate the dissipation rate of a coherently oscillating scalar field in a thermal environment using nonequilibrium quantum field theory and apply it to the reheating stage after cosmic inflation. It is shown that the rate is nonvanishing even when particles coupled to the oscillating inflaton field have a larger thermal mass than it, and therefore the cosmic temperature can be much higher than inflaton's mass even in the absence of preheating. Its cosmological implications are also discussed." @default.
• W1966490192 created "2016-06-24" @default.
• W1966490192 creator A5050762792 @default.
• W1966490192 date "2006-04-01" @default.
• W1966490192 modified "2023-10-17" @default.
• W1966490192 title "Can oscillating scalar fields decay into particles with a large thermal mass?" @default.
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• W1966490192 doi "https://doi.org/10.1016/j.physletb.2006.02.039" @default.
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