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Effective Lagrangian and the back-reaction problem in a self-interacting O(N) scalar theory in curved spacetime

E. Elizalde

K. Kirsten and S. D. Odintsov

  • Departament d’Estructura i Constituents de la Matèria i Institut de Física d’Altes Energies, Faculty of Physics, University of Barcelona, Diagonal 647, 08028 Barcelona, Catalonia, Spain
  • Center for Advanced Studies, Consejo Superior de Investigaciones Científicás, Camí de Santa Bàrbara, 17300 Blanes, Catalonia, Spain

  • Departament d’Estructura i Constituents de la Matèria, Faculty of Physics, University of Barcelona, Diagonal 647, 08028 Barcelona, Catalonia, Spain

Phys. Rev. D 50, 5137 – Published 15 October, 1994

DOI: https://doi.org/10.1103/PhysRevD.50.5137

Abstract

A derivation of the one-loop effective Lagrangian in the self-interacting O(N) scalar theory, in slowly varying gravitational fields, is presented (using ζ-function regularization and heat-kernel techniques). The result is given in terms of the expansion in powers of the curvature tensors (up to quadratic terms) and their derivatives, as well as in derivatives of the background scalar field (up to second derivatives). The renormalization group improved effective Lagrangian is studied, which gives the leading-log approach of the whole perturbation theory. An analysis of the effective equations (back-reaction problem) on the static hyperbolic spacetime openR2×H2/Γ is carried out for the simplest version of the theory: m2=0 and N=1. The possibility of the existence of the solution openR2×H2/Γ, induced by purely quantum effects, is discussed.

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