The Sagnac effect on a scale-dependent rotating BTZ black hole background
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Publication:5161863
DOI10.1088/1361-6382/ABA17FzbMath1479.83164arXiv1902.03704OpenAlexW3105769209MaRDI QIDQ5161863
Ángel Rincón, J. R. Villanueva
Publication date: 1 November 2021
Published in: Classical and Quantum Gravity (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1902.03704
Black holes (83C57) Quantum optics (81V80) Analogues of general relativity in lower dimensions (83C80) Motion of the gyroscope (70E05)
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Cites Work
- On the thermal description of the BTZ black holes
- Particle creation by black holes
- Greybody factors for \(d\)-dimensional black holes
- \(2+1\)-dimensional gravity as an exactly soluble system
- Quasinormal modes of the BTZ black hole under scalar perturbations with a non-minimal coupling: exact spectrum
- The Sagnac phase shift suggested by the Aharonov-Bohm effect for relativistic matter beams
- A direct kinematical derivation of the relativistic Sagnac effect for light or matter beams
- Black hole entropy from near-horizon microstates
- Quasinormal modes of modified gravity (MOG) black holes
- The large-\(N\) limit of superconformal field theories and supergravity
- A stress tensor for anti-de Sitter gravity
- The Sagnac effect in conformal Weyl gravity
- Large \(N\) field theories, string theory and gravity
- Static circularly symmetric perfect fluid solutions with an exterior BTZ metric
- The Sagnac effect in curved space-times from an analogy with the Aharonov-Bohm effect
- THE SCATTERING MATRIX APPROACH FOR THE QUANTUM BLACK HOLE: AN OVERVIEW
- Quasinormal modes of extremal BTZ black hole
- Quasinormal modes of black holes and black branes
- Motion and trajectories of particles around three-dimensional black holes
- Perfect fluid sources in 2+1 dimensions
- Black hole in three-dimensional spacetime
- Stellar equilibrium in 2+1 dimensions
- Geodesic structure of the (2 + 1)-dimensional BTZ black hole
- The (2 + 1)-dimensional black hole
- A regular scale-dependent black hole solution
- A self-sustained traversable scale-dependent wormhole
- A scale dependent black hole in three-dimensional space–time
- Black hole explosions?
- SAGNAC EFFECT IN (2+1)-DIMENSIONAL GRAVITATIONAL FIELD
- Quasi-normal modes of stars and black holes
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