RT Journal Article
T1 Thermodynamic Analysis of Non-Linear Reissner-Nordström Black Holes
A1 Ruiz Cembranos, José Alberto
A1 Cruz-Dombriz, Álvaro
A1 Jarillo Díaz, Javier
AB 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.
PB MDPI
SN 2218-1997
YR 2015
FD 2015-11-16
LK https://hdl.handle.net/20.500.14352/23862
UL https://hdl.handle.net/20.500.14352/23862
LA eng
NO Ministerio de Economía y Competitividad (MINECO)
DS Docta Complutense
RD 6 abr 2025