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Cosmological Vacuum Decays from Schwinger-Keldysh Formalism
In this work, we take a first step to a stochastic real-time description of the vacuum phase transitions in a radiation-dominated FLRW universe from the Schwinger-Keldysh formalism. By splitting the phase transition field $Φ$ into the long-wavelength mode $ϕ$ and the short-wavelength mode $σ$ and tr
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