One-loop Quantum Gravity in Schwarzschild Spacetime
arXiv:gr-qc/9412075 · doi:10.1103/PhysRevD.51.5676
Abstract
The quantum theory of linearized perturbations of the gravitational field of a Schwarzschild black hole is presented. The fundamental operators are seen to be the perturbed Weyl scalars and associated with the Newman-Penrose description of the classical theory. Formulae are obtained for the expectation values of the modulus squared of these operators in the Boulware, Unruh and Hartle-Hawking quantum states. Differences between the renormalized expectation values of both and in the three quantum states are evaluated numerically.
39 pages, 11 Postscript figures, using revtex
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