On the Global Casimir Effect in the Schwarzschild Spacetime

TL;DR

This paper calculates the Casimir energy of a scalar field around a Schwarzschild black hole, revealing how spacetime topology influences vacuum fluctuations and thermodynamic properties without artificial boundaries.

Contribution

It provides an analytic, convergent series calculation of the Casimir energy in Schwarzschild spacetime considering vacuum topology effects and thermal corrections.

Findings

Casimir energy is regularized using Riemann zeta function.

Vacuum tension manifests on the event horizon.

System exhibits thermodynamic instability at low and high temperatures.

Abstract

In this paper we study the vacuum quantum fluctuations of the stationary modes of an uncharged scalar field with mass $m$ around a Schwarzschild black hole with mass $M$, at zero and non-zero temperatures. The procedure consists of calculating the energy eigenvalues starting from the exact solutions found for the dynamics of the scalar field, considering a frequency cutoff in which the particle is not absorbed by the black hole. From this result, we obtain the exterior contributions for the vacuum energy associated to the stationary states of the scalar field, by considering the half-summing of the levels of energy and taking into account the respective degeneracies, in order to better capture the nontrivial topology of the black hole spacetime. Then we use the Riemann's zeta function to regularize the vacuum energy thus found. Such a regularized quantity is the Casimir energy, whose analytic computation we show to yield a convergent series. The Casimir energy obtained does not take into account any boundaries artificially imposed on the system, just the nontrivial spacetime topology associated to the source and its singularity. We suggest that this latter manifests itself through the vacuum tension calculated on the event horizon. We also investigate the problem by considering the thermal corrections via Helmholtz free energy calculation, computing the Casimir internal energy, the corresponding tension on the event horizon, the Casimir entropy, and the thermal capacity of the regularized quantum vacuum, analyzing their behavior at low and high temperatures, pointing out the thermodynamic instability of the system in the considered regime, i.e., $mM\ll 1$.