%0 Journal Article
%A Ruiz Cembranos, José Alberto
%A Cruz-Dombriz, Álvaro
%A Jarillo Díaz, Javier
%T Thermodynamic Analysis of Non-Linear Reissner-Nordström Black Holes
%D 2015
%@ 2218-1997
%U https://hdl.handle.net/20.500.14352/23862
%X In the present article we study the Inverse Electrodynamics Model. This model is a gauge and parity invariant non-linear Electrodynamics theory, which respects the conformal invariance of standard Electrodynamics. This modified Electrodynamics model, when minimally coupled to General Relativity, is compatible with static and spherically symmetric Reissner-Nordström-like black-hole solutions. However, these black-hole solutions present more complex thermodynamic properties than their Reissner-Nordström black-hole solutions counterparts in standard Electrodynamics. In particular, in the Inverse Model a new stability region, with both the heat capacity and the free energy negative, arises. Moreover, unlike the scenario in standard Electrodynamics, a sole transition phase is possible for a suitable choice in the set of parameters of these solutions.
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