Journal
ASTROPHYSICS AND SPACE SCIENCE
Volume 350, Issue 2, Pages 721-726Publisher
SPRINGER
DOI: 10.1007/s10509-013-1761-2
Keywords
Black hole; Quasinormal Modes; WKB approximation
Categories
Ask authors/readers for more resources
In this paper, we evaluate quasinormal modes (QNMs) of scalar perturbations around a quantum-corrected Schwarzschild black hole by using the third order Wentzel-Kramers-Brillouin (WKB) approximation method. The results show that due to the quantum fluctuations in the background of the Schwarzschild black hole, the QNMs of the black hole damp more slowly when increasing the quantum correction factor (a), and oscillate more slowly.
Authors
I am an author on this paper
Click your name to claim this paper and add it to your profile.
Reviews
Recommended
No Data Available