Charged three-dimensions black holes in Weitzenböck geometry
DOI10.1142/S0219887817501055zbMath1376.83025MaRDI QIDQ5370970
Publication date: 20 October 2017
Published in: International Journal of Geometric Methods in Modern Physics (Search for Journal in Brave)
black holeaxially symmetric solutionWeitzenböck geometrytotal conserved charge\(f(T)\) theories of gravityKomar formulaMaxwell-teleparallel gravity
Black holes (83C57) Applications of differential geometry to physics (53Z05) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Analogues of general relativity in lower dimensions (83C80) Einstein-Maxwell equations (83C22)
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Cites Work
- Topologically massive gravity at the chiral point is not unitary
- Constraint dynamics and gravitons in three dimensions
- Invariant conserved currents for gravity
- Topologically massive AdS gravity
- Charged axially symmetric solution and energy in teleparallel theory equivalent to general relativity
- Variational principles for gravity and fluids
- Trace-anomaly driven inflation in \(f(T)\) gravity and in minimal massive bigravity
- Covariant Conservation Laws in General Relativity
- Asymptotic Covariant Conservation Laws for Gravitational Radiation
- Cosmological topologically massive gravitons and photons
- Black hole in three-dimensional spacetime
- String theory formulation of the three-dimensional black hole
- The (2 + 1)-dimensional black hole
- Conformal field theory, (2 + 1)-dimensional gravity and the BTZ black hole
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