Mass and wave-function renormalization at finite temperature

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Scientific paper

Using the real-time formulation of finite-temperature field theory by Niemi and Semenoff we present a rigorous analysis of how to include radiative QED self-energy corrections for thermal decay and scattering processes into suitable mass wave-function renormalization counterterms. Previous work is examined as a special case in our general framework. Our results have immediate applications in cosmology and astrophysics.

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