Quantum stress tensor in the three-dimensional black hole

Details Quantum stress tensor in the three-dimensional black hole Quantum stress tensor in the three-dimensional black hole

Jan 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994phrvd..49..585s&link_type=abstract

Physical Review D (Particles, Fields, Gravitation, and Cosmology), Volume 49, Issue 2, 15 January 1994, pp.R585-R589

Physics

44

Quantum Aspects Of Black Holes, Evaporation, Thermodynamics, Lower Dimensional Models, Minisuperspace Models

Scientific paper

The quantum stress tensor is calculated in the (2+1)-dimensional black hole found by Banados, Teitelboim, and Zanelli. The Green's function, from which is derived, is obtained by the method of images. For the nonrotating black hole, it is shown that is finite on the event horizon, but diverges at the singularity. For the rotating solution, the stress tensor is finite at the outer horizon, but diverges near the inner horizon. This suggests that the inner horizon is quantum mechanically unstable against the formation of a singularity.

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