Magnetic brane solutions in Gauss–Bonnet–Maxwell massive gravity

Hendi, S. H.; Panah, B. Eslam; Panahiyan, S.; Momennia, Mehrab

doi:10.1016/j.physletb.2017.06.012

Cited by 14 publications

(9 citation statements)

References 57 publications

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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%

Charged dilatonic black holes in gravity’s rainbow

et al. 2016

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In this paper, we present charged dilatonic black holes in gravity's rainbow. We study the geometric and thermodynamic properties of black hole solutions. We also investigate the effects of rainbow functions on different thermodynamic quantities for these charged black holes in dilatonic gravity's rainbow. Then we demonstrate that the first law of thermodynamics is valid for these solutions. After that, we investigate thermal stability of the solutions using the canonical ensemble and analyze the effects of different rainbow functions on the thermal stability. In addition, we present some arguments regarding the bound and phase transition points in context of geometrical thermodynamics. We also study the phase transition in extended phase space in which the cosmological constant is treated as the thermodynamic pressure. Finally, we use another approach to calculate and demonstrate that the obtained critical points in extended phase space represent a second order phase transition for these black holes.

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Section: Discussionmentioning

confidence: 95%

Charged dilatonic black holes in gravity’s rainbow

et al. 2016

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“…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%

Thermodynamic description and quasinormal modes of adS black holes in Born-lnfeld massive gravity with a non-abelian hair

Hendi

Momennia

2019

J. High Energ. Phys.

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We construct a new class of asymptotically (a)dS black hole solutions of Einstein-Yang-Mills massive gravity in the presence of Born-Infeld nonlinear electrodynamics. The obtained solutions possess a Coulomb electric charge, massive term and a non-abelian hair as well. We calculate the conserved and thermodynamic quantities, and investigate the validity of the first law of thermodynamics. Also, we investigate thermal stability conditions by using the sign of heat capacity through canonical ensemble. Next, we consider the cosmological constant as a thermodynamical pressure and study the van der Waals like phase transition of black holes in the extended phase space thermodynamics. Our results indicate the existence of a phase transition which is affected by the parameters of theory. Finally, we consider a massless scalar perturbation in the background of asymptotically adS solutions and calculate the quasinormal modes by employing the pseudospectral method. The imaginary part of quasinormal frequencies is the time scale of a thermal state (in the conformal field theory) for the approach to thermal equilibrium.

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“…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%

Tunneling radiation and quantum entropy of a massive gravity black hole

Li¹,

Zhuang²

2020

Turk J Phys

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By using the Parikh-Wilczek (PW) quantum tunneling method, the Hawking radiation of black holes inmassive gravity is investigated, the emission rate of particles and the black hole entropy are calculated. It is shownthat the emission spectrum is not purely thermal, depends on the increment of the black hole entropy, consists with anaccurate unitary theory and supports the standpoint of information conservation. Unlike other modified gravities, theentropy of the massive gravity black hole unexpectedly conforms to the area law just as that of Einstein gravity blackhole.

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Magnetic brane solutions in Gauss–Bonnet–Maxwell massive gravity

Cited by 14 publications

References 57 publications

Charged dilatonic black holes in gravity’s rainbow

Charged dilatonic black holes in gravity’s rainbow

Thermodynamic description and quasinormal modes of adS black holes in Born-lnfeld massive gravity with a non-abelian hair

Tunneling radiation and quantum entropy of a massive gravity black hole

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