Quantum scalar field in D-dimensional static black hole space-times

TL;DR

This paper reviews an Euclidean method using near horizon approximation and $\

Contribution

It extends the $\

Findings

Quantum fluctuations are finite on the horizon when cusp singularities are absent.

The $\

Abstract

An Euclidean approach for investigating quantum aspects of a scalar field living on a class of D-dimensional static black hole space-times, including the extremal ones, is reviewed. The method makes use of a near horizon approximation of the metric and $\zeta$-function formalism for evaluating the partition function and the expectation value of the field fluctuations $<\phi^2(x)>$. After a review of the non-extreme black hole case, the extreme one is considered in some details. In this case, there is no conical singularity, but the finite imaginary time compactification introduces a cusp singularity. It is found that the $\zeta$-function regularized partition function can be defined, and the quantum fluctuations are finite on the horizon, as soon as the cusp singularity is absent, and the corresponding temperature is T=0.