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Asymptotic Reissner-Nordström solution within nonlinear electrodynamics

S. I. KruglovDepartment of Chemical and Physical Sciences, University of Toronto, 3359 Mississauga Road North, Mississauga, Ontario L5L 1C6, Canada
2016en
ABI

Аннотация

A model of nonlinear electrodynamics coupled with the gravitational field is studied. We obtain the asymptotic black hole solutions at $r\ensuremath{\rightarrow}0$ and $r\ensuremath{\rightarrow}\ensuremath{\infty}$. The asymptotic at $r\ensuremath{\rightarrow}0$ is shown, and we find corrections to the Reissner-Nordstr\"om solution and Coulomb's law at $r\ensuremath{\rightarrow}\ensuremath{\infty}$. The mass of the black hole is evaluated having the electromagnetic origin. We investigate the thermodynamics of charged black holes and their thermal stability. The critical point corresponding to the second-order phase transition (where heat capacity diverges) is found. If the mass of the black hole is greater than the critical mass, the black hole becomes unstable.

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