Abstract
In theories with spontaneous symmetry breaking, the exact effective potential V(φc,T) is real, but its loop expansion can be complex. A generalization of the effective potential is developed that is real and that can be computed perturbatively. For the theory with the classical potential V(φ)=(λ/4)(φ2-σ2 )2, this real effective potential closely tracks the usual effective potential where the latter is real, ‖φc‖≥σ/ √3 , and at finite temperatures displays at φc=0 a local minimum, which may have astrophysical implications. The critical temperature at the one-loop level runs from TC≊1.81σ for λ=0.1 to TC≊1.74σ for λ=1.

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