| Article ID | Journal | Published Year | Pages | File Type |
|---|---|---|---|---|
| 8193367 | Physics Letters B | 2010 | 5 Pages |
Abstract
We study the quasinormal modes of the massless scalar perturbation in the background of a deformed black hole in the HoÅava-Lifshitz gravity with coupling constant λ=1. Our results show that the quasinormal frequencies depend on the parameter in the HoÅava-Lifshitz gravity and the behavior of the quasinormal modes is different from those in the Reissner-Norström and Einstein-Born-Infeld black hole spacetimes. The absolute value of imaginary parts is smaller and the scalar perturbations decay more slowly in the deformed HoÅava-Lifshitz black hole spacetime. This information can help us understand more about the HoÅava-Lifshitz gravity.
Keywords
Related Topics
Physical Sciences and Engineering
Physics and Astronomy
Nuclear and High Energy Physics
Authors
Songbai Chen, Jiliang Jing,