Topical Review: Greybody Factors and Quasinormal Modes for Black Holes in Various Theories -- Fingerprints of Invisibles
arXiv:2205.01771 · doi:10.55730/1300-0101.2691
Abstract
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.)
Published in Turkish Journal of Physics. 69 pages. For original article, please follow the link: https://journals.tubitak.gov.tr/physics/issues/fiz-22-46-2/fiz-46-2-1-2203-15.pdf
References in corpus (29)
- Observation of a new particle in the search for the Standard Model Higgs boson with the ATLAS detector at the LHC
- Observation of a new boson at a mass of 125 GeV with the CMS experiment at the LHC
- GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral
- The physical interpretation of the spectrum of black hole quasinormal modes
- A Short Review of Loop Quantum Gravity
- Bounding the greybody factors for Schwarzschild black holes
- Black hole entropy quantization
- Greybody Factors for Brane Scalar Fields in a Rotating Black-Hole Background
- Graviton Emission in the Bulk from a Higher-Dimensional Schwarzschild Black Hole
- Superradiant Instability of Five-Dimensional Rotating Charged AdS Black Holes
- Quasinormal modes, shadow and greybody factors of 5D electrically charged Bardeen black holes
- Greybody factors for rotating black holes in higher dimensions
- Quasinormal modes for tensor and vector type perturbation of Gauss Bonnet black holes using third order WKB approach
- Evaporation of a black hole off of a tense brane
- Brane-World Black Hole Solutions via a Confining Potential
- Quantization of Black Hole Entropy from Quasinormal Modes
- Holographic Isotropisation in Gauss-Bonnet Gravity
- Greybody factors at large imaginary frequencies
- Greybody Factors for Rotating Black Holes on Codimension-2 Branes
- Superradiance and black hole bomb in five-dimensional minimal ungauged supergravity
- Spectroscopy of Rotating Linear Dilaton Black Holes From Boxed Quasinormal Modes
- Quasinormal modes of magnetized black hole
- Comment on "Greybody radiation and quasinormal modes of Kerr-like black hole in Bumblebee gravity model"
- Greybody factor for massive fermion emitted by a black hole in dRGT massive gravity theory
- Emissivities for the various Graviton Modes in the Background of the Higher-Dimensional Black Hole
- Resonance Spectra of Caged Stringy Black Hole and Its Spectroscopy
- Low-lying quasinormal modes of topological AdS black holes and hydrodynamics
- Quasinormal modes of charged fermions in linear dilaton black hole spacetime: Exact frequencies
- Bulk versus Brane Emissivities of Photon Fields: For the case of Higher-Dimensional Schwarzschild Phase
Cited by in corpus (9)
- Probing the Lorentz Invariance Violation via Gravitational Lensing and Analytical Eigenmodes of Perturbed Slowly Rotating Bumblebee Black Holes
- Noncommutative Schwarzschild black hole surrounded by quintessence: Thermodynamics, Shadows and Quasinormal modes
- Thermal fluctuations of (non)linearly charged BTZ black hole in massive gravity
- Greybody factors emitted by a regular black hole in a non-minimally coupled Einstein-Yang-Mills theory
- Weak Deflection Angle, Greybody Bound and Shadow for Charged Massive BTZ Black Hole
- Novel charged black hole solutions of Born-Infeld type: General properties, Smarr formula and Quasinormal frequencies
- Fermionic greybody factors in Schwarzschild acoustic black holes
- The Dirac and Klein-Gordon equations and Greybody Radiation for the Regular Hayward Black Hole
- Dimensionally-dependent uncertainty relations, or why we (probably) won't see micro-black holes at the LHC, even if large extra dimensions exist