Perturbative construction of stationary Randall-Sundrum II black holes on a 5-brane

Abstract

We numerically construct large Randall-Sundrum II brane black holes in 4 and 5 dimensions from associated AdS/CFT spacetimes. Our solutions are leading order perturbations of a representative of the boundary conformal structure of the AdS spacetime sourced by the dual CFT stress tensor. The 4-dimensional solutions are static perturbations of the Euclidean Schwarzschild metric, while the 5-dimensional solutions are perturbations of the Myers-Perry metric with equal angular momenta. We compare the former with previous numerical results for Randall-Sundrum bulk black holes and find good agreement down to a horizon radius of about r H ∼ 30 . The latter are the first numerical results pertaining to rotating Randall-Sundrum black holes. They have the same entropy, but a larger horizon area than Myers-Perry black holes of the same mass and angular momentum.

Quantum work and information geometry of a quantum Myers-Perry black hole

“…The thermodynamics of such a five dimensional Myers-Perry black hole has been investigated [37,38]. The effect of perturbative quantum corrections to the thermodynamics of the Myers-Perry black hole has also been studied [40]. So, we will analyze the effects of non-perturbative corrections to a five dimensional quantum Myers-Perry black hole.…”