Instability of regular planar black holes in four dimensions arising from an infinite sum of curvature corrections

In four-dimensional scalar-tensor theories derived via dimensional regularization with a conformal rescaling of the metric, we study the stability of planar black holes (BHs) whose horizons are described by two-dimensional compact Einstein spaces with vanishing curvature. By taking an infinite sum of Lovelock curvature invariants, it is possible to construct BH solutions whose metric components remain nonsingular at $r=0$, with a scalar-field derivative given by ${\ensuremath{\phi}}^{\ensuremath{'}}(r)=1/r$, where $r$ is the radial coordinate. We show that such BH solutions suffer from a strong coupling problem, where the kinetic term of the even-parity scalar-field perturbation associated with the timelike coordinate vanishes everywhere. Moreover, we find that these BHs are subject to both ghost and Laplacian instabilities for odd-parity perturbations near $r=0$. Consequently, the presence of these pathological features rules out regular planar BHs with the scalar-field profile ${\ensuremath{\phi}}^{\ensuremath{'}}(r)=1/r$ as physically viable and stable configurations.

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Publication Details

Journal
Physical review. D/Physical review. D.
Published
2025-09-10
DOI
https://doi.org/10.1103/cbyk-b46n
Citations
1
Primary Topic
Black Holes and Theoretical Physics
Type
article
Field-Weighted Citation Impact
1.87
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article

Instability of regular planar black holes in four dimensions arising from an infinite sum of curvature corrections

Shinji Tsujikawa, Antonio De Felice
1 citations
Physical review. D/Physical review. D.
Black Holes and Theoretical Physics
1.87
article

Instability of regular planar black holes in four dimensions arising from an infinite sum of curvature corrections

Shinji Tsujikawa, Antonio De Felice
article en
1 citations

Abstract

In four-dimensional scalar-tensor theories derived via dimensional regularization with a conformal rescaling of the metric, we study the stability of planar black holes (BHs) whose horizons are described by two-dimensional compact Einstein spaces with vanishing curvature. By taking an infinite sum of Lovelock curvature invariants, it is possible to construct BH solutions whose metric components remain nonsingular at $r=0$, with a scalar-field derivative given by ${\ensuremath{\phi}}^{\ensuremath{'}}(r)=1/r$, where $r$ is the radial coordinate. We show that such BH solutions suffer from a strong coupling problem, where the kinetic term of the even-parity scalar-field perturbation associated with the timelike coordinate vanishes everywhere. Moreover, we find that these BHs are subject to both ghost and Laplacian instabilities for odd-parity perturbations near $r=0$. Consequently, the presence of these pathological features rules out regular planar BHs with the scalar-field profile ${\ensuremath{\phi}}^{\ensuremath{'}}(r)=1/r$ as physically viable and stable configurations.

Physical review. D/Physical review. D.Vol. 112(6)
Waseda University (JP), Instituto de Física Teórica (ES), Yukawa Institute for Theoretical Physics (JP)
Openalex Percentile: Top 12%
Black Holes and Theoretical Physics
1.87
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Instability of regular planar black holes in four dimensions arising from an infinite sum of curvature corrections — Shinji Tsujikawa, Antonio De Felice · Physical review. D/Physical review. D. (2025) | TGRS Research Map | TGRS