Vacuum polarization in the Schwarzschild black hole with a global monopole

Fuente: arXiv
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Main Authors: Barbosa, Leonardo G., Ramos, Victor H. M., Pitelli, João Paulo M.
Format: Preprint
Published: 2026
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author Barbosa, Leonardo G.
Ramos, Victor H. M.
Pitelli, João Paulo M.
author_facet Barbosa, Leonardo G.
Ramos, Victor H. M.
Pitelli, João Paulo M.
contents We investigate vacuum polarization on the event horizon of a Schwarzschild black hole carrying a global monopole. For a massless scalar field $Ψ$ in the Hartle-Hawking state and with arbitrary curvature coupling, we compute the renormalized vacuum expectation value $\langle Ψ^2 \rangle_{\textrm{ren}}$. The monopole produces a solid-angle deficit and makes the spacetime non-Ricci-flat. Working perturbatively in the monopole parameter $η$ and retaining terms through $O(η^2)$, we find that $\langle Ψ^2 \rangle_{\textrm{ren}}$ on the horizon splits into two contributions: a genuinely monopole-induced term evaluated at the horizon and the usual Schwarzschild result - with the event horizon radius modified by the presence of $η$. Our result parallels earlier analyses for Schwarzschild black holes pierced by a cosmic string.
format Preprint
id arxiv_https___arxiv_org_abs_2602_10899
institution arXiv
publishDate 2026
record_format arxiv
spellingShingle Vacuum polarization in the Schwarzschild black hole with a global monopole
Barbosa, Leonardo G.
Ramos, Victor H. M.
Pitelli, João Paulo M.
General Relativity and Quantum Cosmology
High Energy Physics - Theory
We investigate vacuum polarization on the event horizon of a Schwarzschild black hole carrying a global monopole. For a massless scalar field $Ψ$ in the Hartle-Hawking state and with arbitrary curvature coupling, we compute the renormalized vacuum expectation value $\langle Ψ^2 \rangle_{\textrm{ren}}$. The monopole produces a solid-angle deficit and makes the spacetime non-Ricci-flat. Working perturbatively in the monopole parameter $η$ and retaining terms through $O(η^2)$, we find that $\langle Ψ^2 \rangle_{\textrm{ren}}$ on the horizon splits into two contributions: a genuinely monopole-induced term evaluated at the horizon and the usual Schwarzschild result - with the event horizon radius modified by the presence of $η$. Our result parallels earlier analyses for Schwarzschild black holes pierced by a cosmic string.
title Vacuum polarization in the Schwarzschild black hole with a global monopole
topic General Relativity and Quantum Cosmology
High Energy Physics - Theory
url https://arxiv.org/abs/2602.10899