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Semiclassical ultraextremal horizons

Jerzy Matyjasek*

O. B. Zaslavskii

  • Institute of Physics, Maria Curie-Skłodowska University, pl. Marii Skłodowskiej-Curie 1, 20-031 Lublin, Poland

  • Department of Mechanics and Mathematics, Kharkov V. N. Karazin’s National University, Svoboda Sq.4, Kharkov 61077, Ukraine

  • *Electronic address: matyjase@tytan.umcs.lublin.pl jurek@kft.umcs.lublin.pl
  • Electronic address: ozaslav@kharkov.ua

Phys. Rev. D 71, 087501 – Published 22 April, 2005

DOI: https://doi.org/10.1103/PhysRevD.71.087501

Abstract

We examine backreaction of quantum massive fields on multiply-degenerate (ultraextremal) horizons. It is shown that, under influence of the quantum backreaction, the horizon of such a kind moves to a new position near which the metric does not change its asymptotics, so the ultraextremal black holes and cosmological spacetimes do exist as self-consistent solutions of the semiclassical field equations.

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