2017
DOI: 10.1016/j.physletb.2017.06.012
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Magnetic brane solutions in Gauss–Bonnet–Maxwell massive gravity

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Cited by 14 publications
(9 citation statements)
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“…Finally, it is worthwhile to think about the physical interpretation of abnormal behavior which was seen in this paper. It is notable that, one can generalize obtained linear solutions in this paper to nonlinear case of electrodynamics and investigate the effects of nonlinearity [139]. In addition, one may investigate the extended phase space and thermodynamic criticality in higher order Lovelock-Maxwell gravity's rainbow as well as Lovelock-nonlinear electrodynamics [140,141].…”
Section: Discussionmentioning
confidence: 95%
“…Finally, it is worthwhile to think about the physical interpretation of abnormal behavior which was seen in this paper. It is notable that, one can generalize obtained linear solutions in this paper to nonlinear case of electrodynamics and investigate the effects of nonlinearity [139]. In addition, one may investigate the extended phase space and thermodynamic criticality in higher order Lovelock-Maxwell gravity's rainbow as well as Lovelock-nonlinear electrodynamics [140,141].…”
Section: Discussionmentioning
confidence: 95%
“…In addition, it was shown that this model is ghost free and stable [12]. The static black hole solutions and magnetic solutions in the presence of this model of massive gravity have been investigated in [13][14][15][16] and [17,18], respectively. Moreover, the thermodynamic properties and van der Waals like phase transition of black holes have been studied [14,[19][20][21][22].…”
Section: Jhep10(2019)207mentioning
confidence: 99%
“…Within this framework, a black hole solution with negative cosmological constant was proven to exist in the massive gravity theory [35][36]. The study of the thermodynamic properties of massive gravity black holes has attracted the attention of many researchers [36][37][38][39][40][41]. In this paper, we extend the PW method to a four-dimensional massive gravity black hole to investigate the emission rate of a particle from the event horizon.…”
Section: Introductionmentioning
confidence: 99%