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Charged black holes in effective string theory

S. Mignemi* and N. R. Stewart

  • Laboratoire de Physique Théorique, Gravitation et Cosmologie Relativiste, Université de Paris VI, Centre National de la Recherche Scientifique (CNRS), URA 769, Tour 22, 4e étage, B.C. 142, 4 Place Jussieu, 75252 Paris CEDEX 05, France

  • *Present address: Dipartimento di Scienze Fisiche, Università di Cagliari, via Ospedale 72, 09100 Cagliari, Italy.

Phys. Rev. D 47, 5259 – Published 15 June, 1993

DOI: https://doi.org/10.1103/PhysRevD.47.5259

Abstract

We investigate the qualitative new features of charged dilatonic black holes which emerge when both the Yang-Mills and Gauss-Bonnet curvature corrections are included in the effective action. We consider these perturbative effects by an expansion up to second order in the inverse string tension on the four-dimensional Schwarzschild background and determine the back reaction. We calculate the thermodynamical functions and show that they can behave like those of the Garfinkle-Horowitz-Strominger solution or in a more conventional way, depending on the value of the magnetic charge q. Moreover, we find that for magnetic charge above a critical value, the temperature of the black hole has a maximum and goes to zero for a finite value of the mass. This indicates that the conventional Hawking evaporation law is modified by string theory at a classical level.

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