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• W1593042512 abstract "It is shown how quantum field theory at finite temperature can be used to set up selfconsistent and gauge invariant equations for cosmological perturbations sustained by an ultrarelativistic plasma. While in the collisionless case, the results are equivalent to those obtained from the Einstein-Vlasov equations, weak self-interactions in the plasma turn out to require the full machinery of perturbative thermal field theories such as resummation of hard thermal loops. Nevertheless it is still possible to use the same methods that yielded exact solutions in the collisionless case." @default.
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• W1593042512 date "1996-01-01" @default.
• W1593042512 modified "2023-09-23" @default.
• W1593042512 title "Quantum Field Theory at Finite Temperature and Cosmological Perturbations" @default.
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• W1593042512 doi "https://doi.org/10.1007/978-3-663-01204-7_26" @default.
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