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
Summary
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.
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have