Strong cosmic censorship conjecture for a charged AdS black hole

TL;DR

This paper investigates the validity of the strong cosmic censorship conjecture in charged anti-de Sitter black holes by analyzing quasinormal modes and finds conditions under which the conjecture is violated.

Contribution

It provides an analytical and numerical analysis of quasinormal modes to determine the validity or violation of SCCC in charged AdS black holes, highlighting the role of the parameter 2.

Findings

2 > 1/2 indicates SCCC violation

SCCC is violated for charged AdS black holes with dissipative boundary conditions in the near extremal region

The study combines analytical and numerical methods to assess SCCC validity

Abstract

The strong cosmic censorship conjecture states (SCCC) that one cannot extend spacetime beyond the Cauchy horizon with a square-integrable connection. This conjecture was postulated to save the deterministic nature of the most successful theory of gravitation, general relativity. In order to explore the validation/violation of the SCCC for the charged anti-de Sitter black hole spacetime, we compute the ratio of the imaginary part of the quasinormal mode frequencies and the surface gravity at the Cauchy horizon both analytically and numerically. The lowest value of which defines the key parameter $\beta$ determining the fate of SCCC where $\beta < 1/2$ indicates validation and else violation. We show that $\beta > 1/2$ for a charged AdS black hole with the dissipative boundary conditions in the near extremal region. Thus the SCCC is violated for this spacetime.