29 research outputs found
Gravitational quasinormal modes of black holes in Einstein-aether theory
The local Lorentz violation (LV) in gravity sector should show itself in
derivation of the characteristic quasinormal modes (QNMs) of black hole mergers
from their general relativity case. In this paper, I study QNMs of the
gravitational field perturbations to Einstein-aether black holes and, at first
compare them to those in Schwarzschild black hole, and then some other known LV
gravity theories. By comparing to Schwarzschild black hole, the first kind
aether black holes have larger damping rate and the second ones have lower
damping rate. And they all have smaller real oscillation frequency of QNMs. By
comparing to some other LV theories, the QNMs of the first kind aether black
hole are similar to that of the QED-extension limit of standard model
extension, non-minimal coupling to Einstein's tensor and massive gravity
theories. While as to the second kind aether black hole, they are similar to
those of the noncommutative gravity theories and Einstein-Born-Infeld theories.
These similarities may imply that LV in gravity sector and LV in matter sector
have some intrinsic connections.Comment: 14 pages,8 figures, accepted by Nucl. Phys. B. arXiv admin note:
substantial text overlap with arXiv:1707.0674
Particle energy and Hawking temperature
Some authors have recently found that the tunneling approach gives a
different Hawking temperature for a Schwarzschild black hole in a different
coordinate system. In this paper, we find that to work out the Hawking
temperature in a different coordinate system by the tunneling approach, we must
use the correct definition of the energy of the radiating particles. By using a
new definition of the particle energy, we obtain the correct Hawking
temperature for a Schwarzschild black hole in two dynamic coordinate systems,
the Kruskal-Szekers and dynamic Lemaitre coordinate systems.Comment: 11 pages; Accepted by PL