Perturbations and quasi-normal modes of black holes in Einstein-Aether theory
arXiv:gr-qc/0605082 · doi:10.1016/j.physletb.2006.11.036
Abstract
We develop a new method for calculation of quasi-normal modes of black holes, when the effective potential, which governs black hole perturbations, is known only numerically in some region near the black hole. This method can be applied to perturbations of a wide class of numerical black hole solutions. We apply it to the black holes in the Einstein-Aether theory, a theory where general relativity is coupled to a unit time-like vector field, in order to observe local Lorentz symmetry violation. We found that in the non-reduced Einstein-Aether theory, real oscillation frequency and damping rate of quasi-normal modes are larger than those of Schwarzschild black holes in the Einstein theory.
6 pages, 3 figures, RevTex, to be published in Phys. Lett. B
References in corpus (2)
Cited by in corpus (40)
- Horizon-scale tests of gravity theories and fundamental physics from the Event Horizon Telescope image of Sagittarius A
- Black holes in Einstein-aether and Horava-Lifshitz gravity
- New parametrization for spherically symmetric black holes in metric theories of gravity
- Towards constraining of the Horava-Lifshitz gravities
- Quasinormal modes, scattering and Hawking radiation in the vicinity of Einstein-dilaton-Gauss-Bonnet black hole
- Detecting a Lorentz-Violating Field in Cosmology
- Quasinormal modes of black holes immersed in a strong magnetic field
- Perturbations of spinning black holes beyond General Relativity: Modified Teukolsky equation
- Arbitrarily long-lived quasinormal modes in a wormhole background
- Gravitational spectrum of black holes in the Einstein-Aether theory
- Superradiant instability for black holes immersed in a magnetic field
- Generic features of Einstein-Aether black holes
- Quasinormal modes, shadow and greybody factors of 5D electrically charged Bardeen black holes
- Thin Accretion Disk onto slowly rotating black holes in Einstein-Æther theory
- Correspondence between quasinormal modes and grey-body factors of spherically symmetric traversable wormholes
- Einstein-aether gravity: a status report
- Quasinormal modes in higher derivative gravity: testing the black hole parametrization and sensitivity of overtones
- Quasinormal ringing of black holes in Einstein aether theory
- Quasinormal modes of Einstein--scalar--Gauss--Bonnet black holes
- Quasinormal modes of the bumblebee black holes with a global monopole
- Quasinormal modes of black holes with a scalar hair in Einstein-Maxwell-dilaton theory
- Exact theory for the Rezzolla-Zhidenko metric and self-consistent calculation of quasinormal modes
- Cosmological evolution of interacting dark energy in Lorentz violation
- Quantum gravitational corrections to the Schwarzschild spacetime and quasinormal frequencies
- Analytic expressions for quasinormal modes of the general parametrized spherically symmetric black holes and the Hod's proposal
- Fermions Analysis of IR modified Horava-Lifshitz gravity: Tunneling and Perturbation Perspectives
- Perturbations of Schwarzschild black holes in laboratories
- An Effective Model for the Quantum Schwarzschild Black Hole: Weak Deflection Angle, Quasinormal Modes and Bounding of Greybody Factor
- Thermodynamics of Einstein-Aether Black Holes
- Fermion perturbations in string-theory black holes
- Is Birkhoff's Theorem Valid in Einstein-Aether Theory?
- On optical appearance of Einstein-Maxwell-Æther black holes surrounded by various accretions
- Quasinormal modes of semiclassical electrically charged black holes
- Revisiting linear stability of black hole odd-parity perturbations in Einstein-Aether gravity
- Noncommutative quasinormal modes of Schwarzschild black hole
- Buchdahl bound, photon ring, ISCO and radial acceleration in Einstein-æther theory
- Black holes surrounded by massive vector fields in Kaluza-Klein gravity
- Gravitino perturbations in Schwarzschild black holes
- Hawking Emission from Black Holes Evaporating toward Wormholes and the Accuracy of the WKB Approximation
- The radial metric function does not identify null surfaces