Vaidya-like exact solutions with torsion
arXiv:1502.07105 · doi:10.1007/JHEP05(2015)101
Abstract
Starting from the Oliva--Tempo--Troncoso black hole, a solution of the Bergshoeff--Hohm--Townsend massive gravity, a class of the Vaidya-like exact vacuum solutions with torsion is constructed in the three-dimensional Poincaré gauge theory. A particular subclass of these solutions is shown to possess the asymptotic conformal symmetry. The related canonical energy contains a contribution stemming from torsion.
LaTeX, 15 pages, 2 figures; v2 minor revisions
References in corpus (8)
- Massive Gravity in Three Dimensions
- Three-dimensional black holes, gravitational solitons, kinks and wormholes for BHT massive gravity
- Static spherically symmetric solutions for conformal gravity in three dimensions
- Extra gauge symmetries in BHT gravity
- Conserved charges in 3D gravity
- Black-hole dynamics in BHT massive gravity
- Siklos waves with torsion in 3D
- Gravitational waves with torsion in 3D
Cited by in corpus (9)
- Dynamic wormhole solutions in Einstein-Cartan gravity
- Gravitational waves in Poincaré gauge gravity theory
- Generalized plane waves in Poincaré gauge theory of gravity
- Conformally flat black holes in Poincaré gauge theory
- Gravitational waves in metric-affine gravity theory
- Review of gravitational wave solutions in quadratic metric-affine gravity
- Static Vacuum Solutions on Curved Spacetimes with Torsion
- Drude weight and Mazur-Suzuki bounds in holography
- Torsion as a Gauge Field in a Lorentz-Chern-Simons Theory