Physics – High Energy Physics – High Energy Physics - Theory
Scientific paper
2006-05-12
JHEP0608:087,2006
Physics
High Energy Physics
High Energy Physics - Theory
49 pages, 5 figures
Scientific paper
10.1088/1126-6708/2006/08/087
We study analytically quasinormal modes in a wide variety of black hole spacetimes, including $d$--dimensional asymptotically flat spacetimes and non-asymptotically flat spacetimes (particular attention has been paid to the four dimensional case). We extend the analytical calculation to include first-order corrections to analytical expressions for quasinormal mode frequencies by making use of a monodromy technique. All possible type perturbations are included in this paper. The calculation performed in this paper show that systematic expansions for uncharged black holes include different corrections with the ones for charged black holes. This difference makes them have a different $n$--dependence relation in the first-order correction formulae. The method applied above in calculating the first-order corrections of quasinormal mode frequencies seems to be unavailable for black holes with small charge. This result supports the Neitzke's prediction. On what concerns quantum gravity we confirm the view that the $\ln3$ in $d=4$ Schwarzschild seems to be nothing but some numerical coincidences.
Shen You-Gen
Shu Fu-Wen
No associations
LandOfFree
Perturbative Calculation of Quasinormal Modes of $d$--Dimensional Black Holes 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 Perturbative Calculation of Quasinormal Modes of $d$--Dimensional Black Holes, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Perturbative Calculation of Quasinormal Modes of $d$--Dimensional Black Holes will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-596769