Leaver's method has been the standard for computing the quasinormal mode (QNM) frequencies for a Kerr black hole (BH) for a few decades. We start with a spectral variant of Leaver's method introduced by Cook and Zalutskiy (arXiv: 1410.7698) and propose improvements in the form of computing the necessary derivatives analytically, rather than by numerical finite differencing. We also incorporate this derivative information into qnm, a Python package which finds the QNM frequencies via the spectral variant of Leaver's method. We confine ourselves to first derivatives only.Comment: 6 pages, 1 figur
We investigate the scalar, gravitational, and electromagnetic quasinormal mode spectra of Schwarzsch...
There is a well-known, intuitive geometric correspondence between high-frequency quasinormal modes o...
The excitation factors of black hole quasinormal modes quantify the $\textit{ease of excitation}$ of...
We compute the quasinormal frequencies of rotating black holes using the continued fraction method f...
We present numerical results from three-dimensional evolutions of scalar perturbations of Kerr black...
The quasinormal modes (QNMs) of a black hole spacetime are the free, decaying oscillations of the sp...
We present numerical results from three-dimensional evolutions of scalar perturbations of Kerr black...
[[abstract]]We discuss how to obtain black hole quasinormal modes (QNMs) using the asymptotic iterat...
We study the gravito-electromagnetic perturbations of the Kerr-Newman (KN) black hole metric and ide...
We use physics-informed neural networks (PINNs) to compute the first quasi-normal modes of the Kerr ...
We study the spectrum of quasinormal mode frequencies for a Proca field on a rotating black hole spa...
We show that the linear perturbations of any spin field in the near-zone limit of the Kerr black hol...
Quasinormal modes characterize the final stage of a black hole merger. In this regime, spacetime cur...
In modified theories of gravity, the potentials appearing in the Schr\"odinger-like equations that d...
The resonant mode spectrum of the Kerr-Newman spacetime is presently unknown. These modes, called th...
We investigate the scalar, gravitational, and electromagnetic quasinormal mode spectra of Schwarzsch...
There is a well-known, intuitive geometric correspondence between high-frequency quasinormal modes o...
The excitation factors of black hole quasinormal modes quantify the $\textit{ease of excitation}$ of...
We compute the quasinormal frequencies of rotating black holes using the continued fraction method f...
We present numerical results from three-dimensional evolutions of scalar perturbations of Kerr black...
The quasinormal modes (QNMs) of a black hole spacetime are the free, decaying oscillations of the sp...
We present numerical results from three-dimensional evolutions of scalar perturbations of Kerr black...
[[abstract]]We discuss how to obtain black hole quasinormal modes (QNMs) using the asymptotic iterat...
We study the gravito-electromagnetic perturbations of the Kerr-Newman (KN) black hole metric and ide...
We use physics-informed neural networks (PINNs) to compute the first quasi-normal modes of the Kerr ...
We study the spectrum of quasinormal mode frequencies for a Proca field on a rotating black hole spa...
We show that the linear perturbations of any spin field in the near-zone limit of the Kerr black hol...
Quasinormal modes characterize the final stage of a black hole merger. In this regime, spacetime cur...
In modified theories of gravity, the potentials appearing in the Schr\"odinger-like equations that d...
The resonant mode spectrum of the Kerr-Newman spacetime is presently unknown. These modes, called th...
We investigate the scalar, gravitational, and electromagnetic quasinormal mode spectra of Schwarzsch...
There is a well-known, intuitive geometric correspondence between high-frequency quasinormal modes o...
The excitation factors of black hole quasinormal modes quantify the $\textit{ease of excitation}$ of...