Accurate quasinormal modes of the analogue black holes
Jerzy Matyjasek, Kristian Benda, Maja Stafi\'nska

TL;DR
This paper accurately computes quasinormal modes of analogue black holes in (2+1) and (3+1) dimensions using multiple numerical methods, improving precision and extending previous results.
Contribution
It introduces refined computational techniques and cross-validates results for quasinormal modes of analogue black holes, achieving higher accuracy than prior studies.
Findings
Achieved up to 9 decimal place accuracy in quasinormal mode calculations.
Validated consistency of multiple numerical methods for these computations.
Extended existing literature with more precise mode data.
Abstract
We study the quasinormal modes of the spherically-symmetric -dimensional analogue black hole, modeled by the ``draining bathtub'' fluid flow, and the -dimensional canonical acoustic black hole. In the both cases the emphasis is on the accuracy. Formally, the radial equation describing perturbations of the -dimensional black hole is a special case of the general master equation of the 5-dimensional Tangherlini black hole. Similarly, the -dimensional equation can be obtained from the master equation of the 7-dimensional Tangherlini black hole. For the -dimensional analogue black hole we used three major techniques: the higher-order WKB method with the Pad\'e summation, the Hill-determinant method and the continued fraction method, the latter two with the convergence acceleration. In the -dimensional case, we propose the simpler recurrence…
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Taxonomy
TopicsBlack Holes and Theoretical Physics · Geophysics and Sensor Technology · Pulsars and Gravitational Waves Research
