Quasinormal modes of the spherical bumblebee black holes with a global monopole
arXiv:2308.01575 · doi:10.1140/epjc/s10052-023-11899-9
Abstract
The bumblebee model is an extension of the Einstein-Maxwell theory that allows for the spontaneous breaking of the Lorentz symmetry of the spacetime. In this paper, we study the quasinormal modes of the spherical black holes in this model that are characterized by a global monopole. We analyze the two cases with a vanishing cosmological constant or a negative one (the anti-de Sitter case). We find that the black holes are stable under the perturbation of a massless scalar field. However, both the Lorentz symmetry breaking and the global monopole have notable impacts on the evolution of the perturbation. The Lorentz symmetry breaking may prolong or shorten the decay of the perturbation according to the sign of the breaking parameter. The global monopole, on the other hand, has different effects depending on whether a nonzero cosmological constant presences: it reduces the damping of the perturbations for the case with a vanishing cosmological constant, but has little influence for the anti-de Sitter case.
arXiv commentaccepted by Eur. Phys. J. C
References in corpus (41)
- Gravity, Lorentz Violation, and the Standard Model
- Modern tests of Lorentz invariance
- Noncommutative Field Theory and Lorentz Violation
- Nonstandard optics from quantum spacetime
- Quasinormal Modes of AdS Black Holes and the Approach to Thermal Equilibrium
- Ghost Condensation and a Consistent Infrared Modification of Gravity
- Quantum Spacetime Phenomenology
- Electrodynamics with Lorentz-violating operators of arbitrary dimension
- Spontaneous Lorentz Violation, Nambu-Goldstone Modes, and Gravity
- An exact Schwarzschild-like solution in a bumblebee gravity model
- Black holes with a cosmological constant in bumblebee gravity
- Quantum-Gravitational Diffusion and Stochastic Fluctuations in the Velocity of Light
- Mining information from binary black hole mergers: a comparison of estimation methods for complex exponentials in noise
- Gravitational Lensing Under the Effect of Weyl and Bumblebee Gravities: Applications of Gauss-Bonnet Theorem
- Exact Kerr-like solution and its shadow in a gravity model with spontaneous Lorentz symmetry breaking
- Loop-Generated Bounds on Changes to the Graviton Dispersion Relation
- Evolving of a massless scalar field in Reissner--Nordström Anti--de Sitter spacetimes
- Schwarzschild-like black hole with a topological defect in bumblebee gravity
- QNMs of slowly rotating Einstein-Bumblebee Black Hole
- Quasinormal frequencies for a black hole in a bumblebee gravity
- Bumblebee gravity with a Kerr-Sen-like solution and its Shadow
- The gravitational field of a global monopole
- Greybody Radiation and Quasinormal Modes of Kerr-like Black Hole in Bumblebee Gravity Model
- String Theoretic Bounds on Lorentz-Violating Warped Compactification
- Einstein-Gauss-Bonnet gravity coupled to bumblebee field in four dimensional spacetime
- Magnetic Reconnection and Energy Extraction from a Spinning Black Hole with Broken Lorentz Symmetry
- Constraint on parameters of a rotating black hole in Einstein-bumblebee theory by quasi-periodic oscillations
- Slowly rotating Einstein-bumblebee black hole solution and its greybody factor in a Lorentz violation model
- Holographic superconductors in the AdS black hole spacetime with a global monopole
- Black Hole Superradiance in the Presence of Lorentz Symmetry Violation
- Asymmetrically warped compactifications and gravitational Lorentz violation
- Black holes in massive gravity: Quasi-normal modes of scalar perturbations
- Phase transition of a charged AdS black hole with a global monopole through geometrical thermodynamics
- Global Monopole in Asymptotically dS/AdS Spacetime
- Decay of massive scalar hair in the background of a black hole with a global monopole
- Reply to "Comment on 'Greybody radiation and quasinormal modes of Kerr-like black hole in Bumblebee gravity model' "
- Selfgravitating magnetic monopoles, global monopoles and black holes
- Comment on "Greybody radiation and quasinormal modes of Kerr-like black hole in Bumblebee gravity model"
- Superradiant instability of the Kerr-like black hole in Einstein-bumblebee gravity
- Effects of a global monopole on thermodynamic phase transition of the charged AdS black hole
- Perturbations of global monopoles as a black hole's hair
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