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Quasi-normal modes of the scalar hairy black hole

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Alexander Zhidenko

General Relativity and Quantum Cosmology · Submitted 8 Oct 2005

abstract compiled · 2026-09-23 · no language-model review

The authors' main claim Increasing of the scalar field mass does not cause the imaginary part to vanish, it reaches some minimum and then increases, thus in the case under consideration the infinitely long living modes (quasi-resonances) do not appear.

how it is stated · asserted 1.00 read the record →

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arXiv IDgr-qc/0510039 (version 3)
Pith IDKN23VEAY, Pith's permanent record of this paper and its review
CitationAlexander Zhidenko. "Quasi-normal modes of the scalar hairy black hole." arXiv:gr-qc/0510039 (2005). https://pith.science/paper/KN23VEAY
Claim paper

The compiled record

The paper's own sentences, arranged. Each label is drawn from a closed vocabulary; the number beside it is the probability the classifier gave that label. Numbers in the tables are the authors', checked by code. No sentence in this record was written by a model.

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Compiled by classifier-1.13-20260917 via OpenRouter, question bank abstract-p1-20260923, 2026-09-23: 1 request, 2,926 input tokens, $0.0001 reported.

What the abstract itself states, as probabilities: claims first 0.03 · states limitation 0.75 · human participants 0.01 · controlled comparison 0.02 · randomized assignment 0.01 · states quantitative result 0.13 · compares with prior results 0.10 · mentions code or data availability 0.02.

The abstract, sentence by sentence

arXiv listing abstract v3. Results and the main claim are underlined; .

We calculate QNMs of the scalar hairy black hole in the AdS background using Horowitz-Hubeny method for the potential that is not known in analytical form. For some black hole parameters we found pure imaginary frequencies. Increasing of the scalar field mass does not cause the imaginary part to vanish, it reaches some minimum and then increases, thus in the case under consideration the infinitely long living modes (quasi-resonances) do not appear.

background contribution method result interpretation main claim

What the classifier reports for each sentence. The number is the probability it gave the label.
#sentencerolethe authors' own workstates the main conclusionstrength
s0 We calculate QNMs of the scalar hairy black hole in the AdS background using Horowitz-Hubeny method for the potential that is not known in analytical form. contribution 0.73 0.96 0.07 asserted 1.00
s1 For some black hole parameters we found pure imaginary frequencies. result 1.00 0.97 0.12 asserted 1.00
s2 Increasing of the scalar field mass does not cause the imaginary part to vanish, it reaches some minimum and then increases, thus in the case under consideration the infinitely long living modes (quasi-resonances) do not appear. result 0.72 0.93 0.70 asserted 1.00

What kind of paper the classifier reports this is: simulation study 0.87 · evidence from simulation or computation 1.00.

What was examined, and what was not

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  • arXiv listing abstract v3
not examined
  • full text
  • figures and tables
  • references and citing sentences
  • relations to other papers
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  • P abstract
not run
  • S sections
  • T body sentences
  • C citations
  • R cross-paper relations

Every quoted sentence on this record is the authors'. Every label is from Pith's closed vocabulary, with the probability shown beside it. Every number in the measurements table is the authors', checked by code. Record as JSON

The paper
Original abstract

We calculate QNMs of the scalar hairy black hole in the AdS background using Horowitz-Hubeny method for the potential that is not known in analytical form. For some black hole parameters we found pure imaginary frequencies. Increasing of the scalar field mass does not cause the imaginary part to vanish, it reaches some minimum and then increases, thus in the case under consideration the infinitely long living modes (quasi-resonances) do not appear.

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References
How the literature uses it

9 arXiv papers cite this in 11 sentences

Each citing sentence is taken from the citing paper's LaTeX source and typed by Pith's classifier. A label appears at probability 0.8 or more (0.95 for support), a contest at 0.7 or more; the quoted words are the citing authors'. How each label was checked · JSON

Papers citing it · 8 sentences without a confident label

Compares with it 1 paper
  • The signature of symmergent parameters on QNMs is noticeably different from other black hole hairs in different well-studied black hole systems, including the standard Schwarzschild dS/AdS black holes [ref] .

    Quasinormal modes and greybody factors of symmergent black hole · WKB method with Padé Approximation for Quasinormal modes · 0.93

Cites it as background 2 papers
  • A broad body of work has explored QNMs in asymptotically AdS and dS spacetimes, analogue systems, scalar-hairy and regular black holes, charged and nonlinear-electrodynamic backgrounds, phase-transition settings, scale-dependent geometries, and several modified-gravity scenarios, including Einstein–Gauss–Bonnet, Einstein–dilaton–Gauss–Bonnet, slowly rotating vector perturbations, loop-quantum-corrected and Weyl black holes [ref] .

    Echoes of a hairy black hole from gravitational decoupling · Introduction · 0.99

  • The properties of gravitational waves and quasinormal modes of black holes have been extensively explored in various modified gravity theories in recent years [ref] .

    Quasinormal Modes of Black holes in $f(Q)$ gravity · Introduction · 0.98

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