Dynamical evolution of scalar perturbation in Horava-Lifshitz black-hole spacetimes
Abstract
We study the dynamical evolution of a massless scalar perturbation in the Horava-Lifshitz black-hole spacetimes with the coupling constants λ=1/3, λ=1/2 and λ=3, respectively. Our calculation shows that, for the three cases, the scalar perturbations decay without any oscillation in which the decay rate imprints the parameter of the Horava-Lifshitz black hole. The results are quite different from those in the Schwarzschild AdS black hole and can help us understand more about the Horava-Lifshitz gravity.
0
Turn this paper into a lesson
ArcXiv compiles a structured reading guide from this paper's metadata: plain-English importance, contributions, prerequisite concepts, which sections to read first, flashcards, and a quiz. Grounded in the abstract, never invented.