arXiv · gr-qc/0502115
Semiclassical ultraextremal horizons
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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Jerzy Matyjasek, O. B. Zaslavskii. 2005-03-04. Semiclassical ultraextremal horizons. https://doi.org/10.1103/physrevd.71.087501
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