General Framework for the Spontaneous Scalarization of Regular Black Holes

Fuente: arXiv
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Autori principali: Contreras, Ernesto, Carrasco-Hidalgo, Mikaela, Bargueño, Pedro, Suvorov, Arthur G.
Natura: Preprint
Pubblicazione: 2025
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author Contreras, Ernesto
Carrasco-Hidalgo, Mikaela
Bargueño, Pedro
Suvorov, Arthur G.
author_facet Contreras, Ernesto
Carrasco-Hidalgo, Mikaela
Bargueño, Pedro
Suvorov, Arthur G.
contents We investigate the spontaneous scalarization of generic, static, and spherically symmetric regular black holes supported by nonlinear electrodynamics. Starting from an arbitrary seed metric, we employ the P-dual formalism to reconstruct the electromagnetic sector and subsequently couple a real scalar field nonminimally. As a worked example, we apply the framework to the regular Balart-Vagenas black hole, showing that scalarized and scalar-free branches can coexist in a region where the scalarized configurations are entropically preferred. We further assess possible observational imprints, finding percent-level deviations in both the shadow size and the fundamental scalar quasi-normal modes ($< 10\%$ for small charge-to-mass ratios), indicating that current electromagnetic and gravitational-wave observations do not rule out these solutions. Our construction thus provides a general route to explore scalarization on top of nonlinear-electrodynamics-supported spacetimes, extending beyond specific Reissner-Nordström-like cases.
format Preprint
id arxiv_https___arxiv_org_abs_2511_01544
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle General Framework for the Spontaneous Scalarization of Regular Black Holes
Contreras, Ernesto
Carrasco-Hidalgo, Mikaela
Bargueño, Pedro
Suvorov, Arthur G.
General Relativity and Quantum Cosmology
High Energy Astrophysical Phenomena
We investigate the spontaneous scalarization of generic, static, and spherically symmetric regular black holes supported by nonlinear electrodynamics. Starting from an arbitrary seed metric, we employ the P-dual formalism to reconstruct the electromagnetic sector and subsequently couple a real scalar field nonminimally. As a worked example, we apply the framework to the regular Balart-Vagenas black hole, showing that scalarized and scalar-free branches can coexist in a region where the scalarized configurations are entropically preferred. We further assess possible observational imprints, finding percent-level deviations in both the shadow size and the fundamental scalar quasi-normal modes ($< 10\%$ for small charge-to-mass ratios), indicating that current electromagnetic and gravitational-wave observations do not rule out these solutions. Our construction thus provides a general route to explore scalarization on top of nonlinear-electrodynamics-supported spacetimes, extending beyond specific Reissner-Nordström-like cases.
title General Framework for the Spontaneous Scalarization of Regular Black Holes
topic General Relativity and Quantum Cosmology
High Energy Astrophysical Phenomena
url https://arxiv.org/abs/2511.01544