We introduce a 'quasi-topological` term [1] in D=1+1 dimensions and the entropy for black holes is calculated [2]. The source of entropy in this case is justified by a non-null stress-energy tensor
We obtain the dilaton solution in the background of a spherically symmetric black hole with curvatu...
Recent derivations of Cardy-like formulae in higher dimensional field theories have opened up a way ...
We derive an extension of the Ryu-Takayanagi prescription for curvature squared theories of gravity ...
We study the contribution to entropy of Black Holes in D=2+1 dimensions from an extension of the Che...
The near extremal Reissner-Nordstrom black holes in arbitrary dimensions ca be modeled by the Jackiw...
AbstractWe find the entropy of Kehagias–Sfetsos black hole in the deformed Hořava–Lifshitz gravity b...
Following the derivation of the Green function for the massless scalar field satisfying the Dirichle...
In this pedagogical note, we discuss obstacles to the usual Palatini formulations of gauge and gravi...
By an extension of the methods used for the reduction of the two body problem in 2+1 dimensional gra...
The theory of resurgence connects high order terms of perturbative series to low order terms in non-...
In the standard methodology for evaluating the Hawking radiation emanating from a black hole, the ba...
AbstractAxially symmetric gravitating multi-skyrmion configurations are obtained using the harmonic ...
Though entropy production is forbidden in standard FRW Cosmology, Berman and Som presented a simple ...
There would be a perfect correspondence between the laws of classical thermodynamics and black hole ...
The flat anisotropic model of the early Universe is considered. Two interacting scalar fields with s...
We obtain the dilaton solution in the background of a spherically symmetric black hole with curvatu...
Recent derivations of Cardy-like formulae in higher dimensional field theories have opened up a way ...
We derive an extension of the Ryu-Takayanagi prescription for curvature squared theories of gravity ...
We study the contribution to entropy of Black Holes in D=2+1 dimensions from an extension of the Che...
The near extremal Reissner-Nordstrom black holes in arbitrary dimensions ca be modeled by the Jackiw...
AbstractWe find the entropy of Kehagias–Sfetsos black hole in the deformed Hořava–Lifshitz gravity b...
Following the derivation of the Green function for the massless scalar field satisfying the Dirichle...
In this pedagogical note, we discuss obstacles to the usual Palatini formulations of gauge and gravi...
By an extension of the methods used for the reduction of the two body problem in 2+1 dimensional gra...
The theory of resurgence connects high order terms of perturbative series to low order terms in non-...
In the standard methodology for evaluating the Hawking radiation emanating from a black hole, the ba...
AbstractAxially symmetric gravitating multi-skyrmion configurations are obtained using the harmonic ...
Though entropy production is forbidden in standard FRW Cosmology, Berman and Som presented a simple ...
There would be a perfect correspondence between the laws of classical thermodynamics and black hole ...
The flat anisotropic model of the early Universe is considered. Two interacting scalar fields with s...
We obtain the dilaton solution in the background of a spherically symmetric black hole with curvatu...
Recent derivations of Cardy-like formulae in higher dimensional field theories have opened up a way ...
We derive an extension of the Ryu-Takayanagi prescription for curvature squared theories of gravity ...