The heat kernel approach for calculating the effective action in quantum field theory and quantum gravity

dc.creatorAvramidi, Ivan G.
dc.date1995-09-14
dc.date.accessioned2026-07-07T04:21:28Z
dc.date.available2026-07-07T04:21:28Z
dc.descriptionA short informal overview about recent progress in the calculation of the effective action in quantum gravity is given. I describe briefly the standard heat kernel approach to the calculation of the effective action and discuss the applicability of the Schwinger - De Witt asymptotic expansion in the case of strong background fields. I propose a new ansatz for the heat kernel that generalizes the Schwinger - De Witt one and is always valid. Then I discuss the general structure of the asymptotic expansion and put forward some approximate explicitly covariant methods for calculating the heat kernel, namely, the high-energy approximation as well as the low-energy one. In both cases the explicit formulae for the heat kernel are given.
dc.description21 pages, Plain TeX, 52 KB, no figures
dc.identifierhttps://arxiv.org/abs/hep-th/9509077
dc.identifierhttp://arxiv.org/abs/hep-th/9509077
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/54328
dc.subjectHigh Energy Physics - Theory
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleThe heat kernel approach for calculating the effective action in quantum field theory and quantum gravity
dc.typetext

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