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Phase Structure and Gravitational-Wave Phenomenology of a Thermal First-Order Phase Transition
We investigate the phase structure and gravitational-wave (GW) phenomenology of a cosmological first-order phase transition described by the finite-temperature effective potential $V(ϕ,T)=D(T^2-T_0^2)ϕ^2-ETϕ^3+λϕ^4/4$. We derive the critical temperature and the broken-phase order parameter and ident
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