[[abstract]]In this paper we show that the asymptotic iteration method (AIM) allows one to numerically find the quasinormal modes of Schwarzschild and Schwarzschild de Sitter black holes. An added benefit of the method is that it can also be used to calculate the Schwarzschild anti-de Sitter quasinormal modes for the case of spin-zero perturbations. We also discuss an improved version of the AIM, more suitable for numerical implementation.[[journaltype]]國外[[incitationindex]]SCI[[booktype]]紙本[[countrycodes]]GB
Abstract. We establish a Bohr–Sommerfeld type condition for quasi-normal modes of a slowly rotating ...
We calculate the high-order quasinormal modes with large imaginary frequencies for the electromagnet...
We study the quasinormal modes (QNM) for scalar, and electromagnetic perturbations in the Schwarzchi...
[[abstract]]We discuss how to obtain black hole quasinormal modes (QNMs) using the asymptotic iterat...
We revisit the problem of calculating the quasinormal modes of spin 0, 1/2, 1, 3/2, 2, and spin 5/2 ...
We probe into the instabilities of microscopic quantum black holes. For this purpose, we study the q...
The exact computation of asymptotic quasinormal frequencies is a technical problem which involves th...
International audienceThe traditional approach to perturbations of nonrotating black holes in genera...
International audienceThe traditional approach to perturbations of nonrotating black holes in genera...
International audienceThe traditional approach to perturbations of nonrotating black holes in genera...
A conjectured connection to quantum gravity has led to a renewed interest in highly damped black-hol...
International audienceThe traditional approach to perturbations of nonrotating black holes in genera...
International audienceThe traditional approach to perturbations of nonrotating black holes in genera...
We study analytically quasinormal modes in a wide variety of black hole space-times, including d-dim...
W pracy wyznaczone zostały częstości modów kwazinormalnych pola skalarnego oraz wektorowego dla czar...
Abstract. We establish a Bohr–Sommerfeld type condition for quasi-normal modes of a slowly rotating ...
We calculate the high-order quasinormal modes with large imaginary frequencies for the electromagnet...
We study the quasinormal modes (QNM) for scalar, and electromagnetic perturbations in the Schwarzchi...
[[abstract]]We discuss how to obtain black hole quasinormal modes (QNMs) using the asymptotic iterat...
We revisit the problem of calculating the quasinormal modes of spin 0, 1/2, 1, 3/2, 2, and spin 5/2 ...
We probe into the instabilities of microscopic quantum black holes. For this purpose, we study the q...
The exact computation of asymptotic quasinormal frequencies is a technical problem which involves th...
International audienceThe traditional approach to perturbations of nonrotating black holes in genera...
International audienceThe traditional approach to perturbations of nonrotating black holes in genera...
International audienceThe traditional approach to perturbations of nonrotating black holes in genera...
A conjectured connection to quantum gravity has led to a renewed interest in highly damped black-hol...
International audienceThe traditional approach to perturbations of nonrotating black holes in genera...
International audienceThe traditional approach to perturbations of nonrotating black holes in genera...
We study analytically quasinormal modes in a wide variety of black hole space-times, including d-dim...
W pracy wyznaczone zostały częstości modów kwazinormalnych pola skalarnego oraz wektorowego dla czar...
Abstract. We establish a Bohr–Sommerfeld type condition for quasi-normal modes of a slowly rotating ...
We calculate the high-order quasinormal modes with large imaginary frequencies for the electromagnet...
We study the quasinormal modes (QNM) for scalar, and electromagnetic perturbations in the Schwarzchi...