Physics – High Energy Physics – High Energy Physics - Theory
Scientific paper
2003-11-26
JHEP 0312 (2003) 041
Physics
High Energy Physics
High Energy Physics - Theory
13 pages, 3 figures; to appear in JHEP
Scientific paper
10.1088/1126-6708/2003/12/041
We calculate the quasinormal modes (QNMs) for gravitational perturbations of the Schwarzschild black hole in the five dimensional (5D) spacetime with a continued fraction method. For all the types of perturbations (scalar-gravitational, vector-gravitational, and tensor-gravitational perturbations), the QNMs associated with l=2, l=3, and l=4 are calculated. Our numerical results are summarized as follows: (i) The three types of gravitational perturbations associated with the same angular quantum number l have a different set of the quasinormal (QN) frequencies; (ii) There is no purely imaginary frequency mode; (iii) The three types of gravitational perturbations have the same asymptotic behavior of the QNMs in the limit of the large imaginary frequencies. In Hawking temperature units these frequencies are given by log3 + i2pi(n+1/2) as n goes to infinity, where n is the mode number.
Cardoso Vitor
Lemos José P. S.
Yoshida Shijun
No associations
LandOfFree
Scalar-gravitational perturbations and quasinormal modes in the five dimensional Schwarzschild black hole does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Scalar-gravitational perturbations and quasinormal modes in the five dimensional Schwarzschild black hole, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Scalar-gravitational perturbations and quasinormal modes in the five dimensional Schwarzschild black hole will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-122480