Abstract

The thermodynamics and weak cosmic censorship conjecture in Reissner-Nordström anti-de Sitter black holes are investigated by the scattering of the scalar field. The first law of thermodynamics in the non-extremal Reissner-Nordström anti-de Sitter black hole is recovered by the scattering. The increase of the horizon radius indicates that the singularity is not naked in this black hole. For the near-extremal and extremal black holes, the validity is tested by the minimum values of the function f at their final states. It is found that both of the near-extremal and extremal black holes can not be overcharged. When ω=qϕ, the final state of the extremal black hole is still an extremal black hole. When ω≠qϕ, it becomes a near-extremal black hole with new mass and charge.

Highlights

  • It is widely believed that spacetime singularities arise from gravitational collapse

  • We investigate the thermodynamics and weak cosmic censorship conjecture (WCCC) in Reissner-Nordstrom anti-de Sitter (RN-AdS) black holes by the scattering of a complex scalar field

  • We investigated the thermodynamics and WCCC in the RN-AdS black holes by the scattering of the scalar field

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Summary

Introduction

It is widely believed that spacetime singularities arise from gravitational collapse. Considering the interaction between a complex scalar field and a charged black hole, Semiz found that the WCCC was not violated in the dyonic Kerr-Newman black holes This result was gotten again in [19]. We investigate the thermodynamics and WCCC in Reissner-Nordstrom anti-de Sitter (RN-AdS) black holes by the scattering of a complex scalar field. For the near-extremal and extremal RN-AdS black holes, due to the divergence of Eq(3.21), the validity is tested by the minimum value of the function f at the final state after the scattering. This value is evaluated by adjusting values of ω and q.

The wave function in the RN-AdS black hole
Thermodynamics of the non-extremal RN-AdS black hole
The WCCC in the near-extremal and extremal RNAdS black holes
Discussion and Conclusion
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