We give a pedagogical introduction to black holes (BHs) greybody factors (GFs) and quasinormal modes (QNMs) and share the recent developments on those subjects. In this study, our primary focus will be on the bosonic and fermionic GFs and QNMs of various BH and brane geometries and reveal the fingerprints of the invisibles with the radiation spectra to be obtained by the WKB approximation and bounding the Bogoliubov coefficients (together with the Miller-Good transformation) methods. (*Due to the notification of arXiv "The Abstract field cannot be longer than 1,920 characters", the appeared Abstract is shortened. For the full Abstract, please download the Article.)Comment: Published in Turkish Journal of Physics. 69 pages. For original ar...
Greybody factors are transmission probabilities of the Hawking radiation, which are emitted from bla...
We study the propagation of massless scalar fields non-minimally coupled to gravity in the backgroun...
We study the greybody factors, quasinormal modes, and shadow of the higher dimensional de-Sitter (dS...
Quasinormal modes are eigenmodes of dissipative systems. Perturbations of classical gravitational ba...
We consider perturbations of the massless Dirac field in the background of a black hole solution fou...
Quasinormal mode(QNM) is a characteristic "sound" for a black hole which can provide us with a new m...
Bardeen de-Sitter (BdS) black hole is a spherically symmetric solution of Einstein's equation which ...
The Effective Field Theory (EFT) of perturbations on an arbitrary background geometry with a timelik...
In this work, we investigate the quasinormal frequencies of a class of regular black hole solutions ...
We investigate the scalar, gravitational, and electromagnetic quasinormal mode spectra of Schwarzsch...
Symmergent gravity is an emergent gravity framework in which gravity emerges guided by gauge invaria...
Quasinormal modes (QNMs) are the damped vibrations of black hole (BH) spacetimes, characterising m...
The WKB approach for finding quasinormal modes of black holes, suggested in Schutz and Will (1985 As...
We study the quasi-normal modes for scalar, electromagnetic, and gravitational axial perturbations i...
This is an unconventional review article on spectral problems in black hole perturbation theory. Our...
Greybody factors are transmission probabilities of the Hawking radiation, which are emitted from bla...
We study the propagation of massless scalar fields non-minimally coupled to gravity in the backgroun...
We study the greybody factors, quasinormal modes, and shadow of the higher dimensional de-Sitter (dS...
Quasinormal modes are eigenmodes of dissipative systems. Perturbations of classical gravitational ba...
We consider perturbations of the massless Dirac field in the background of a black hole solution fou...
Quasinormal mode(QNM) is a characteristic "sound" for a black hole which can provide us with a new m...
Bardeen de-Sitter (BdS) black hole is a spherically symmetric solution of Einstein's equation which ...
The Effective Field Theory (EFT) of perturbations on an arbitrary background geometry with a timelik...
In this work, we investigate the quasinormal frequencies of a class of regular black hole solutions ...
We investigate the scalar, gravitational, and electromagnetic quasinormal mode spectra of Schwarzsch...
Symmergent gravity is an emergent gravity framework in which gravity emerges guided by gauge invaria...
Quasinormal modes (QNMs) are the damped vibrations of black hole (BH) spacetimes, characterising m...
The WKB approach for finding quasinormal modes of black holes, suggested in Schutz and Will (1985 As...
We study the quasi-normal modes for scalar, electromagnetic, and gravitational axial perturbations i...
This is an unconventional review article on spectral problems in black hole perturbation theory. Our...
Greybody factors are transmission probabilities of the Hawking radiation, which are emitted from bla...
We study the propagation of massless scalar fields non-minimally coupled to gravity in the backgroun...
We study the greybody factors, quasinormal modes, and shadow of the higher dimensional de-Sitter (dS...