We analyze the thermodynamical properties of the regular static and spherically symmetric black hole interior model presented by Mbonye and Kazanas. Equations for the thermodynamical quantities valid for an arbitrary density profile are deduced, and from them we show that the model is thermodynamically unstable. Evidence is also presented pointing to its dynamical instability. The gravitational entropy of this solution based on the Weyl curvature conjecture is calculated, following the recipe given by Rudjord, Grøn and Sigbjørn, and it is shown to have the expected behavior.Facultad de Ciencias Astronómicas y Geofísica
We consider the thermodynamic properties of the constant curvature black hole solution recently foun...
The geometry of thermodynamic state space is studied for asymptotically anti-de Sitter black holes ...
The geometry of thermodynamic state space is studied for asymptotically anti-de Sitter black holes i...
We analyze the thermodynamical properties of the regular static and spherically symmetric black hole...
We analyze the thermodynamical properties of the regular static and spherically symmetric black hole...
We analyze the thermodynamical properties of the regular static and spherically symmetric black hole...
In this work we address the issue of the thermodynamic behavior of a non-singular spherically-symmet...
In this work we address the issue of the thermodynamic behavior of a non-singular spherically-symmet...
We study the thermodynamics of spherically symmetric, neutral and non-rotating black holes in confor...
In this paper we present a non-singular black hole model as a possible end-product of gravitational ...
A family of spacetimes suitable for describing the interior of a non-rotational black hole is constr...
In this paper we present a non-singular black hole model as a possible end-product of gravitational ...
The geometry of thermodynamic state space is studied for asymptotically anti-de Sitter black holes ...
Along this review, we focus on the study of several properties of modified gravity theories, in part...
We study the interior metric of 4D spherically symmetric static black holes by using the semi-classi...
We consider the thermodynamic properties of the constant curvature black hole solution recently foun...
The geometry of thermodynamic state space is studied for asymptotically anti-de Sitter black holes ...
The geometry of thermodynamic state space is studied for asymptotically anti-de Sitter black holes i...
We analyze the thermodynamical properties of the regular static and spherically symmetric black hole...
We analyze the thermodynamical properties of the regular static and spherically symmetric black hole...
We analyze the thermodynamical properties of the regular static and spherically symmetric black hole...
In this work we address the issue of the thermodynamic behavior of a non-singular spherically-symmet...
In this work we address the issue of the thermodynamic behavior of a non-singular spherically-symmet...
We study the thermodynamics of spherically symmetric, neutral and non-rotating black holes in confor...
In this paper we present a non-singular black hole model as a possible end-product of gravitational ...
A family of spacetimes suitable for describing the interior of a non-rotational black hole is constr...
In this paper we present a non-singular black hole model as a possible end-product of gravitational ...
The geometry of thermodynamic state space is studied for asymptotically anti-de Sitter black holes ...
Along this review, we focus on the study of several properties of modified gravity theories, in part...
We study the interior metric of 4D spherically symmetric static black holes by using the semi-classi...
We consider the thermodynamic properties of the constant curvature black hole solution recently foun...
The geometry of thermodynamic state space is studied for asymptotically anti-de Sitter black holes ...
The geometry of thermodynamic state space is studied for asymptotically anti-de Sitter black holes i...