Quasinormal modes and hidden conformal symmetry of warpeddS3black hole

Abstract

In this paper, we analytically calculate the quasinormal modes of scalar, vector, tensor, and spinor perturbations of the warped ${\mathrm{dS}}_{3}$ black hole. There are two horizons for the warped ${\mathrm{dS}}_{3}$ black hole, namely, the black hole horizon ${r}_{b}$ and the cosmological horizon ${r}_{c}$. In the calculation, we impose the ingoing boundary condition at the black hole horizon and the outgoing boundary condition at the cosmological horizon. We also investigate the hidden conformal symmetry of the warped ${\mathrm{dS}}_{3}$ black hole in the region between the black hole horizon and the cosmological horizon ${r}_{b}<r<{r}_{c}$. We use the hidden conformal symmetry to construct the quasinormal modes in an algebraic way and find that the results agree with the analytically ones. It turns out that the frequencies of the quasinormal modes could be identified with the poles in the thermal boundary-boundary correlators.