Accelerating black holes in the low energy heterotic string theory
arXiv:1805.07790 · doi:10.1016/j.physletb.2018.06.004
Abstract
We present a new solution describing a pair of rotating, charged, and accelerating black holes in in the low energy limit of heterotic string theory. To obtain the solution, we apply the Hassan-Sen transformation to the neutral accelerating Kerr spacetime as the seed solution. Some properties of the black hole solutions are discussed.
15 pages, no figures; v2: refs fixed
References in corpus (10)
- Interpreting the C-metric
- Holographic Thermodynamics of Accelerating Black Holes
- Kerr-Sen dilaton-axion black hole lensing in the strong deflection limit
- Thermodynamics of Regular Accelerating Black Holes
- The Event Horizon Telescope: exploring strong gravity and accretion physics
- Null Geodesics and Observables around Kerr-Sen Black Hole
- Stationary Charged Scalar Clouds around Black Holes in String Theory
- Quasi-local conserved charges and holography
- Scalar clouds around Kerr-Sen black holes
- Analytical Study of a Kerr-Sen Black Hole and a Charged Massive Scalar Field
Cited by in corpus (12)
- Aspects of the dyonic Kerr-Sen-AdS black hole and its ultraspinning version
- Solutions and basic properties of regularized Maxwell theory
- Merger estimates for Kerr-Sen black holes
- Kerr-Sen-Taub-NUT spacetime and circular geodesics
- Charged scalar fields in a Kerr-Sen black hole: exact solutions, Hawking radiation, and resonant frequencies
- Pair production of scalars around near-extremal Kerr-Sen black holes
- Black Remnants from T-Duality
- Accelerating Kaluza-Klein black hole and Kerr/CFT correspondence
- Validity of black hole complementarity in an accelerating Schwarzschild black hole
- Null hypersurface caustics and super-entropic black holes
- Shadows for Kerr-Sen-Taub-NUT black holes with Manko-Ruiz parameter
- Three Dimensional Black Hole in the Low Energy Heterotic String Theory