Thermodynamic Analysis of Non-Linear Reissner-Nordström Black Holes
AbstractIn 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. View Full-Text
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Cembranos, J.A.R.; Cruz-Dombriz, Á.; Jarillo, J. Thermodynamic Analysis of Non-Linear Reissner-Nordström Black Holes. Universe 2015, 1, 412-421.
Cembranos JAR, Cruz-Dombriz Á, Jarillo J. Thermodynamic Analysis of Non-Linear Reissner-Nordström Black Holes. Universe. 2015; 1(3):412-421.Chicago/Turabian Style
Cembranos, Jose A.R.; Cruz-Dombriz, Álvaro ; Jarillo, Javier. 2015. "Thermodynamic Analysis of Non-Linear Reissner-Nordström Black Holes." Universe 1, no. 3: 412-421.