Cited by 116Black Holes and Theoretical PhysicsPulsars and Gravitational Waves ResearchCosmology and Gravitation Theories

Gravitational instability of Einstein–Gauss–Bonnet black holes under tensor mode perturbations

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Dotti, Gustavo, Gleiser, Reinaldo J·2005·Classical and Quantum Gravity

Abstract

We analyse the tensor mode perturbations of static, spherically symmetric solutions of the Einstein equations with a quadratic Gauss–Bonnet term in dimension D > 4. We show that the evolution equations for this type of perturbation can be cast in a Regge–Wheeler–Zerilli form, and obtain the exact potential for the corresponding Schrödinger-like stability equation. As an immediate application we prove that for D ≠ 6 and α > 0, the sign choice for the Gauss–Bonnet coefficient suggested by string theory, all positive mass black holes of this type are stable. In the exceptional case D = 6, we find a range of parameters where positive mass asymptotically flat black holes, with regular horizon, are unstable. This feature is found also in general for α < 0.

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Crossref · 10.1088/0264-9381/22/1/l01

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  • For bad modes, V_l is negative for r <= r_bad and admits negative energy bound states.

    “But for the bad modes, V r ( ) l is negative for ⩽ r r bad , and admits negative energy bound states [18].”

    From Causality and hyperbolicity of Lovelock theories (2014) · cites this paper as [18]

    Section 3 gives a negative-potential-integral criterion for negative-energy bound states and shows it holds for sufficiently small mass and large angular eigenvalue in the exceptional n = 4 case. The copy does not define r_bad or establish that the potential is negative throughout r ≤ r_bad. No page number is available for these passages in the indexed copy. (LLM, conf=0.83)

    Experimental — accuracy not yet measured
  • For a d = 6 small spherical black hole with Λ = 0, the tensors have V_eff < 0 near the horizon, giving the instability of [18,19]; this is a failure of hyperbolicity.

    “Similarly, for the d = 6 example the tensors have < V 0 eff near the horizon, which gives the instability of [18,19].But again, this is much worse than an instability, it is a failure of hyperbolicity of the theory.”

    From Causality and hyperbolicity of Lovelock theories (2014) · cites this paper as [18]

  • For static spherically or planar symmetric black hole solutions of Lovelock theories, there exist effective metrics G_S, G_V and G_T such that characteristic hypersurfaces are null hypersurfaces with respect to one of these metrics.

    “From this one can infer that there exist 'effective metrics' G ab S , G ab V and G ab T such that characteristic hypersurfaces are null hypersurfaces with respect to one of these metrics.”

    From Causality and hyperbolicity of Lovelock theories (2014) · cites this paper as [18]

    Section 2 (pp. L2–L3) studies tensor perturbations of spherically symmetric Einstein–Gauss–Bonnet solutions, and Section 4 (p. L6) summarizes a stability analysis. Our copy does not address effective metrics for scalar, vector, and tensor modes or say that characteristic hypersurfaces are null with respect to them (searched: effective metrics, characteristic hypersurfaces, and propagation cones). (LLM, conf=0.76)

    Experimental — accuracy not yet measured

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Authors
Dotti, G., & Gleiser, R. J.
Affiliations
Universidad Nacional de Córdoba (AR)
Venue
Classical and Quantum Gravity
Published
2004-12-10
Volume
22
Issue
1
Pages
L1-L6
ISSN
  • 0264-9381 (ISSN-L)
  • 1361-6382
OpenAlex
W1984446792
Cited by
116
References
1
Citations by year
2026: 16 · 2025: 9 · 2024: 7 · 2023: 2 · 2021: 2 · 2020: 3 · 2019: 6 · 2018: 3 · 2017: 4 · 2016: 4 · 2015: 2 · 2014: 4 · 2013: 5 · 2012: 3
FWCI
2.97
Type
journal article
Language
en
Open access
Locations
  • Classical and Quantum Gravity (publishedVersion)
  • arXiv (Cornell University) (submittedVersion)
  • CERN Document Server (European Organization for Nuclear Research) (submittedVersion)
  • arXiv (Cornell University)
Funders
  • National Science Foundation (0204937)
  • Agencia Córdoba Ciencia
  • Consejo Nacional de Investigaciones Científicas y Técnicas
  • Universidad de Córdoba
Topics
  • Physical Sciences › Physics and Astronomy › Nuclear and High Energy Physics › Black Holes and Theoretical Physics
  • Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Pulsars and Gravitational Waves Research
  • Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Cosmology and Gravitation Theories
Keywords
gravitational instability, Einstein-Gauss-Bonnet gravity, black holes, higher-dimensional black holes, six-dimensional black holes, asymptotically flat black holes, static spherically symmetric solutions

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