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Renormalization of \Phi-derivable approximations in scalar field theories

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arxiv hep-ph/0312085 v1 pith:7YP6AQ7G submitted 2003-12-05 hep-ph

classification hep-ph
keywords equationapproximationscountertermsrenormalizationtemperatureauxiliaryeliminatefield
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We discuss the renormalization of \Phi-derivable approximations for scalar field theories. In such approximations, the self-energy is obtained as the solution of a self-consistent equation which effectively resums infinite subsets of diagrams of perturbation theory. We show that a consistent renormalization can be carried out, and we provide an explicit construction of the counterterms needed to eliminate the subdivergences. The counterterms are calculated from the solution of an auxiliary gap equation which determines the leading asymptotic part of the self-energy. This auxiliary gap equation may be chosen as the gap equation of the massless theory at zero temperature. We verify explicitly that the counterterms determined at zero temperature are sufficient to eliminate the divergences which occur in finite temperature calculations.

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Cited by 1 Pith paper

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    A 2PI-Hartree effective potential for two mixing scalars is renormalized and used to show that self-consistent thermal resummation can substantially alter predicted phase transition strengths and gravitational wave spectra.

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