The interplay of WGC and WCCC via charged scalar field fluxes in the RPST framework

TL;DR

This paper explores how charged scalar field fluxes influence the weak cosmic censorship conjecture and weak gravity conjecture in Reissner-Nordstrom AdS black holes within a restricted phase space thermodynamics framework, revealing conditions for stability and conjecture validity.

Contribution

It introduces a novel analysis of WCCC and WGC interplay using energy flux and thermodynamics in RPST, highlighting effects near extremality and superradiance.

Findings

WCCC holds near extremality with radiation and particle absorption.

Superradiance particles obey WGC when black hole radiates and charge exceeds scaled electric charge.

Black holes become closer or further from extremality depending on particle attraction and charge conditions.

Abstract

In this paper, we investigate the weak cosmic censorship conjecture (WCCC) for the Reissner-Nordstrom (R-N) AdS black hole in a restricted phase space thermodynamics (RPST). Also here, we consider energy flux and equivalence mass-energy principle and examine the weak gravity conjecture (WGC) and the weak cosmic censorship conjecture. The incoming and outgoing energy flux leads to changes in the black hole. In that case, by applying the first law, we examined whether the second law of thermodynamics is valid. And also one can say that, in the case where absorption and superradiance are in the saturated to an equilibrium. Also, by using the thermodynamics of black holes in the restricted phase space, we show that if the black hole is in an extreme or close to an extreme state with radiation and particle absorption, the weak cosmic censorship conjecture is established. In addition, with the help of equivalence mass and energy principle and second-order approximation, in the near extremity, we find that when the black hole radiates and its central charge is greater than the scaled electric charge, the superradiance particles obey the weak gravity conjecture, and this causes the black hole to move further away from its extreme state. But when the particles that obey the weak gravity conjecture are attracted to the black hole when the black hole is very small. Then, in this case, we note that the black hole becomes closer to its extreme state.