Scalar fields in a five-dimensional Lovelock black hole spacetime
arXiv:2001.08690 · doi:10.1016/j.aop.2020.168197
Abstract
We study the interaction between massive scalar fields and the gravitational field produced by a higher dimensional Schwarzschild solution in a string cloud model. Exact analytical solutions of both angular and radial parts of the Klein--Gordon equation are obtained in terms of the three-dimensional spherical harmonics and general Heun functions, respectively. From these solutions, we examine the interesting physical phenomena related to the Hawking radiation and resonant frequencies.
arXiv comment19 pages, 4 figures, 4 tables
References in corpus (19)
- Hawking temperature in the tunneling picture
- Subtleties in the quasi-classical calculation of Hawking radiation
- Local Quantum Gravity
- Thermal radiation of various gravitational backgrounds
- Black holes in Einstein-Gauss-Bonnet gravity with a string cloud background
- Confluent Heun functions and the physics of black holes: resonant frequencies, Hawking radiation and scattering of scalar waves
- Problems with Tunneling of Thin Shells from Black Holes
- The portrait of eikonal instability in Lovelock theories
- Exact solutions of the Klein-Gordon equation in the Kerr-Newman background and Hawking radiation
- Analytical solutions in rotating linear dilaton black holes: resonant frequencies, quantization, greybody factor, and Hawking radiation
- Black Hole Hair from Scalar Dark Matter
- On the growth of massive scalar hair around a Schwarzschild black hole
- The background scale Ward identity in quantum gravity
- Analytical Solutions in a Cosmic String Born-Infeld-dilaton Black Hole Geometry: Quasinormal Modes and Quantization
- Scalar scattering in Schwarzschild spacetime: Integral equation method
- Coherent states in quantum gravity: a construction based on the flux representation of LQG
- Quantum Gravity and Inflation
- Charged scalar fields in a Kerr-Sen black hole: exact solutions, Hawking radiation, and resonant frequencies
- Resonant frequencies of a charged scalar field in the Garfinkle-Horowitz-Strominger dilaton black hole