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The Mystery of the Asymptotic Quasinormal Modes of Gauss-Bonnet Black Holes

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R. G. Daghigh, G. Kunstatter, J. Ziprick

General Relativity and Quantum Cosmology · Submitted 27 Nov 2006

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

The authors' main claim We show that for this damping region the famous $\ln(3)$ appears in the real part of the quasinormal mode frequency.

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arXiv IDgr-qc/0611139 (version 1)
Pith IDWXU7AL23, Pith's permanent record of this paper and its review
CitationG. Kunstatter, J. Ziprick, R. G. Daghigh. "The Mystery of the Asymptotic Quasinormal Modes of Gauss-Bonnet Black Holes." arXiv:gr-qc/0611139 (2006). https://pith.science/paper/WXU7AL23
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Compiled by classifier-1.13-20260917 via OpenRouter, question bank abstract-p1-20260923, 2026-09-23: 1 request, 3,697 input tokens, $0.0002 reported.

What the abstract itself states, as probabilities: claims first 0.04 · states limitation 0.93 · human participants 0.01 · controlled comparison 0.03 · randomized assignment 0.01 · states quantitative result 0.84 · compares with prior results 0.35 · mentions code or data availability 0.02.

The abstract, sentence by sentence

arXiv listing abstract v1. Results and the main claim are underlined; .

We analyze the quasinormal modes of $D$-dimensional Schwarzschild black holes with the Gauss-Bonnet correction in the large damping limit and show that standard analytic techniques cannot be applied in a straightforward manner to the case of infinite damping. However, by using a combination of analytic and numeric techniques we are able to calculate the quasinormal mode frequencies in a range where the damping is large but finite. We show that for this damping region the famous $\ln(3)$ appears in the real part of the quasinormal mode frequency. In our calculations, the Gauss-Bonnet coupling, $\alpha$, is taken to be much smaller than the parameter $\mu$, which is related to the black hole mass.

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 analyze the quasinormal modes of $D$-dimensional Schwarzschild black holes with the Gauss-Bonnet correction in the large damping limit and show that standard analytic techniques cannot be applied in a straightforward manner to the case of infinite damping. contribution 0.61 0.92 0.23 asserted 1.00
s1 However, by using a combination of analytic and numeric techniques we are able to calculate the quasinormal mode frequencies in a range where the damping is large but finite. method 0.82 0.96 0.14 asserted 1.00
s2 We show that for this damping region the famous $\ln(3)$ appears in the real part of the quasinormal mode frequency. result 1.00 0.93 0.48 asserted 1.00
s3 In our calculations, the Gauss-Bonnet coupling, $\alpha$, is taken to be much smaller than the parameter $\mu$, which is related to the black hole mass. method 0.72 0.84 0.04 asserted 1.00

What kind of paper the classifier reports this is: theoretical result 0.93 · evidence from simulation or computation 0.70.

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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 analyze the quasinormal modes of $D$-dimensional Schwarzschild black holes with the Gauss-Bonnet correction in the large damping limit and show that standard analytic techniques cannot be applied in a straightforward manner to the case of infinite damping. However, by using a combination of analytic and numeric techniques we are able to calculate the quasinormal mode frequencies in a range where the damping is large but finite. We show that for this damping region the famous $\ln(3)$ appears in the real part of the quasinormal mode frequency. In our calculations, the Gauss-Bonnet coupling, $\alpha$, is taken to be much smaller than the parameter $\mu$, which is related to the black hole mass.

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4 arXiv papers cite this in 4 sentences

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