A Matrix Method for Quasinormal Modes: Kerr and Kerr-Sen Black Holes
TLDR
In this paper, a matrix method is employed to study the scalar quasinormal modes of Kerr as well as Kerr-Sen black holes, where discretization is applied to transfer the perturbation equation into a matrix form eigenvalue problem, where the resulting radial and angular equations are derived by the method of separation of variables.Abstract:
In this letter, a matrix method is employed to study the scalar quasinormal modes of Kerr as well as Kerr-Sen black holes. Discretization is applied to transfer the scalar perturbation equation into a matrix form eigenvalue problem, where the resulting radial and angular equations are derived by the method of separation of variables. The eigenvalues, quasinormal frequencies $\omega$ and angular quantum numbers $\lambda$, are then obtained by numerically solving the resultant homogeneous matrix equation. This work shows that the present approach is an accurate as well as efficient method for investigating quasinormal modes.read more
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Proceedings of the royal society.
George Rennie,T.Wharton Jones,A.F. Chambers,James Copland,John Webster,Robert J. Lee,James H. Clark,Richard Bright,Marshall Hall,JamesR. Martin,RobertE. Grant,George Gulliver +11 more
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A New Approach to Black Hole Quasinormal Modes: A Review of the Asymptotic Iteration Method
TL;DR: In this article, an approach to obtaining black hole quasinormal modes (QNMs) using the asymptotic iteration method (AIM) was discussed, initially developed to solve second order ordinary differential equations.
Journal ArticleDOI
The matrix method for black hole quasinormal modes
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Journal ArticleDOI
Stability under scalar perturbations and quasinormal modes of 4D Einstein-Born-Infeld dilaton spacetime: Exact spectrum
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Journal ArticleDOI
Charged scalar fields around Einstein-power-Maxwell black holes
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