A slowly rotating black hole solution in Einstein–Maxwell-dilaton gravity is considered. Using the obtained solution we investigate thermodynamic functions such as the black hole’s temperature, entropy and heat capacity. In addition, to examine the thermodynamic properties of the black hole an extended technique is applied. The equation of state of Van der Waals type is obtained and investigated. It has been shown that the given system has phase transitions of the first and of the zeroth order below a critical temperature, which is a notable feature of the black hole. A coexistence relation for two phases is also considered and the latent heat is calculated. In the end, critical exponents are calculated
We derive a singular solution for the rotating counterpart of Lee-Wick gravity having a point source...
In this review we summarize, expand, and set in context recent developments on the thermodynamics of...
Considering de Rham–Gabadadze–Tolley theory of massive gravity coupled with (ghost free) higher curv...
The exact solutions of coupled scalar, electromagnetic and gravitational field equations have been o...
In this paper, we take into account the dilaton black hole solutions of Einstein gravity in the pres...
In this paper, the three-dimensional Einstein–Maxwell theory in the presence of a dilatonic scalar f...
In this paper, we present charged dilatonic black holes in gravity’s rainbow. We study the geometric...
Abstract Thermodynamics of rotating black holes described by the Rényi formula as equilibrium and ze...
The thermodynamics of a three-dimensional Einstein–Maxwell-dilaton black hole is investigated using ...
This paper is devoted to an investigation of nonlinearly charged dilatonic black holes in the contex...
The critical phenomena of dilaton black holes are probed from a totally different perspective other ...
We construct a class of charged, rotating solutions of (n+1)-dimensional Einstein-Maxwell-dilaton gr...
Abstract We present a spinning black hole solution in d dimensions with a maximal number of rotation...
Abstract In the context of dilaton coupled Einstein gravity with a negative cosmological constant an...
A thermodynamic analysis of the black hole solutions coming from the Einstein-Maxwell-Dilaton theory...
We derive a singular solution for the rotating counterpart of Lee-Wick gravity having a point source...
In this review we summarize, expand, and set in context recent developments on the thermodynamics of...
Considering de Rham–Gabadadze–Tolley theory of massive gravity coupled with (ghost free) higher curv...
The exact solutions of coupled scalar, electromagnetic and gravitational field equations have been o...
In this paper, we take into account the dilaton black hole solutions of Einstein gravity in the pres...
In this paper, the three-dimensional Einstein–Maxwell theory in the presence of a dilatonic scalar f...
In this paper, we present charged dilatonic black holes in gravity’s rainbow. We study the geometric...
Abstract Thermodynamics of rotating black holes described by the Rényi formula as equilibrium and ze...
The thermodynamics of a three-dimensional Einstein–Maxwell-dilaton black hole is investigated using ...
This paper is devoted to an investigation of nonlinearly charged dilatonic black holes in the contex...
The critical phenomena of dilaton black holes are probed from a totally different perspective other ...
We construct a class of charged, rotating solutions of (n+1)-dimensional Einstein-Maxwell-dilaton gr...
Abstract We present a spinning black hole solution in d dimensions with a maximal number of rotation...
Abstract In the context of dilaton coupled Einstein gravity with a negative cosmological constant an...
A thermodynamic analysis of the black hole solutions coming from the Einstein-Maxwell-Dilaton theory...
We derive a singular solution for the rotating counterpart of Lee-Wick gravity having a point source...
In this review we summarize, expand, and set in context recent developments on the thermodynamics of...
Considering de Rham–Gabadadze–Tolley theory of massive gravity coupled with (ghost free) higher curv...