On Holographic description of the Kerr-Newman-AdS-dS black holes

Abstract

In this paper, we study the holographic description of the generic four-dimensional non-extremal Kerr-Newman-AdS-dS black holes. We find that if focusing on the near-horizon region, for the massless scalar scattering in the low-frequency limit, there exists hidden conformal symmetry on the solution space. Similar to the Kerr case, this suggests that the Kerr-Newman-AdS-dS black hole is dual to a two-dimensional CFT with central charges $c_L=c_R=\frac{6a(r_{+}+r_{\ast })}{k}$ and temperatures $T_L=\frac{k(r_{+}^2+r_{\ast }^2+2a^2)}{4\pi a\Xi (r_{+}+r_{\ast })},T_R=\frac{k(r_{+}-r_{\ast })}{4\pi a\Xi }$. The macroscopic Bekenstein-Hawking entropy could be recovered from the microscopic counting in dual CFT via the Cardy formula. Using the Minkowski prescription, we compute the real-time correlators of the scalar, photon and graviton in near horizon geometry of near extremal Kerr-AdS-dS black hole. In all these cases, the retarded Green's function and the corresponding absorption cross section are in perfect match with CFT prediction. We further discuss the low-frequency scattering of a charged scalar by a Kerr-Newman-AdS-dS black hole and find the dual CFT description.

22 pages; minor corrections, conlusion unchanged, references added;published version

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