Abstract:Recent studies based on the notion of black hole pseudospectrum indicated substantial instability of the fundamental and high-overtone quasinormal modes. Besides its theoretical novelty, the details about the migration of the quasinormal mode spectrum due to specific perturbations may furnish valuable information on the properties of associated gravitational waves in a more realistic context. This work generalizes the matrix method for black hole quasinormal modes to cope with a specific class of perturbations… Show more
“…It is also noted that even though, in principle, equation ( 15) might introduce additional irrelevant roots, it does not pose a serious problem, as long as they stay away from the low-lying quasinormal frequencies. Furthermore, it was proposed [59] that the above algorithm can be adapted for the effective potential possessing discontinuity. To proceed, one assigns the point of discontinuity to one of the grid points x = x c .…”
Section: The Matrix Methodsmentioning
confidence: 99%
“…The matrix method [54][55][56][57][58][59] is an approach that reformulates the QNM problem into a matrix equation for the complex frequencies. The approach is reminiscent of the continued fraction method, and their main difference resides in the choice of the grid points where the expansion of the waveform is performed [54].…”
Section: Introductionmentioning
confidence: 99%
“…It has been generalized to deal with dynamic black hole spacetimes [58]. More recently, the original method was generalized [59] to handle effective potentials containing discontinuity. These features indicate that the method is a promising alternative in the toolkit for black hole QNMs.…”
Motivated by the substantial instability of the fundamental and high-overtone quasinormal modes, recent developments regarding the notion of black hole pseudospectrum call for numerical results with unprecedented precision.
This work generalizes and improves the matrix method for black hole quasinormal modes to higher orders, specifically aiming at a class of perturbations to the metric featured by discontinuity intimately associated with the quasinormal mode structural instability.
The approach is based on the mock-Chebyshev grid, which guarantees its convergence in the degree of the interpolant.
In practice, solving for black hole quasinormal modes is a formidable task.
The presence of discontinuity poses a further difficulty so that many well-known approaches cannot be employed straightforwardly.
Compared with other viable methods, the modified matrix method is competent in speed and accuracy. 
Therefore, the method serves as a helpful gadget for relevant studies.
“…It is also noted that even though, in principle, equation ( 15) might introduce additional irrelevant roots, it does not pose a serious problem, as long as they stay away from the low-lying quasinormal frequencies. Furthermore, it was proposed [59] that the above algorithm can be adapted for the effective potential possessing discontinuity. To proceed, one assigns the point of discontinuity to one of the grid points x = x c .…”
Section: The Matrix Methodsmentioning
confidence: 99%
“…The matrix method [54][55][56][57][58][59] is an approach that reformulates the QNM problem into a matrix equation for the complex frequencies. The approach is reminiscent of the continued fraction method, and their main difference resides in the choice of the grid points where the expansion of the waveform is performed [54].…”
Section: Introductionmentioning
confidence: 99%
“…It has been generalized to deal with dynamic black hole spacetimes [58]. More recently, the original method was generalized [59] to handle effective potentials containing discontinuity. These features indicate that the method is a promising alternative in the toolkit for black hole QNMs.…”
Motivated by the substantial instability of the fundamental and high-overtone quasinormal modes, recent developments regarding the notion of black hole pseudospectrum call for numerical results with unprecedented precision.
This work generalizes and improves the matrix method for black hole quasinormal modes to higher orders, specifically aiming at a class of perturbations to the metric featured by discontinuity intimately associated with the quasinormal mode structural instability.
The approach is based on the mock-Chebyshev grid, which guarantees its convergence in the degree of the interpolant.
In practice, solving for black hole quasinormal modes is a formidable task.
The presence of discontinuity poses a further difficulty so that many well-known approaches cannot be employed straightforwardly.
Compared with other viable methods, the modified matrix method is competent in speed and accuracy. 
Therefore, the method serves as a helpful gadget for relevant studies.
“…Proposed by some of us, the matrix method [26][27][28][29][30][31][32] is an approach that turns the problem of solving the master equation for the quasinormal frequencies into a non-standard matrix eigenvalue problem. Like the well-known continued fraction method [22], Taylor expansion is utilized to rewrite the wave function.…”
Section: Introductionmentioning
confidence: 99%
“…It can be adapted to different boundary conditions [29] and dynamic black hole spacetimes [30]. More recently, the method was generalized [31] to the potentials containing discontinuity and aimed to the higher orders [32]. The approach provides reasonable accuracy and efficiency and has been utilized in various studies [6,[34][35][36][37][38][39][40][41][42][43][44][45][46].…”
In this work, we explore the properties of the matrix method for black hole quasinormal modes on the nonuniform grid.In particular, the method is implemented to be adapted to the Chebyshev grid, aimed at effectively suppressing Runge's phenomenon.It is found that while such an implementation is favorable from a mathematical point of view, in practice, the increase in precision does not necessarily compensate for the penalty in computational time.On the other hand, the original matrix method, though subject to Runge's phenomenon, is shown to be reasonably robust and suffices for most applications with a moderate grid number.In terms of computational time and obtained significant figures, we carried out an analysis regarding the trade-off between the two aspects.The implications of the present study are also addressed.
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