Renormalized Vacuum Polarization and Stress Tensor on the Horizon of a Schwarzschild Black Hole Threaded by a Cosmic String
Adrian C. Ottewill, Peter Taylor

TL;DR
This paper computes the renormalized vacuum polarization and stress tensor for a scalar field near a Schwarzschild black hole with a cosmic string, using a novel mathematical identity for Legendre functions.
Contribution
It introduces a generalized Heine identity for non-integer Legendre functions to facilitate calculations in curved spacetime with cosmic strings.
Findings
Derived a new identity for Legendre functions applicable to black hole spacetimes.
Calculated vacuum polarization and stress tensor on the horizon of a black hole threaded by a cosmic string.
Provides insights into quantum field effects in black hole geometries with topological defects.
Abstract
We calculate the renormalized vacuum polarization and stress tensor for a massless, arbitrarily coupled scalar field in the Hartle-Hawking vacuum state on the horizon of a Schwarzschild black hole threaded by an infinte straight cosmic string. This calculation relies on a generalized Heine identity for non-integer Legendre functions which we derive without using specific properties of the Legendre functions themselves.
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