We study the interior metric of 4D spherically symmetric static black holes by using the semi-classical Einstein equation and find a consistent class of geometries with large curvatures. We approximate the matter fields by conformal fields and consider the contribution of 4D Weyl anomaly, giving a state-independent constraint. Combining this with an equation of state yields an equation that determines the interior geometry completely. We explore the solution space of the equation in a non-perturbative manner for $\hbar$. First, we find three types of asymptotic behaviors and examine the general features of the solutions. Then, by imposing physical conditions, we obtain approximately a general class of interior geometries: various combinatio...
We revamp the constructive enumeration of 1/16-BPS states in the maximally supersymmetric Yang-Mills...
Black-hole solutions to general relativity carry a thermodynamic entropy, discovered by Bekenstein a...
A family of spacetimes suitable for describing the interior of a non-rotational black hole is constr...
We analyze the thermodynamical properties of the regular static and spherically symmetric black hole...
We solve the Wheeler DeWitt equation for the planar Reissner-Nordstr\"om-AdS black hole in a minisup...
We consider numerical black hole solutions in the Weyl conformal geometry, and its associated confor...
Indexación: SpringerWe consider the role of the type-A trace anomaly in static black hole solutions ...
The thermodynamic properties of black holes -- temperature, entropy and radiation rates -- are usual...
We study the quantum error correction properties of the black hole interior in a toy model for an ev...
We systematically calculate the quantum extremal surface (QES) associated with Hawking radiation for...
We analyze the thermodynamical properties of the regular static and spherically symmetric black hole...
In general, a finite metric function at the center of a black hole describes a non-singular spacetim...
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 regularized 4-dimensional Einstein-Gauss-Bonnet (EGB) gravity derived from a Kaluza-Klein reducti...
We revamp the constructive enumeration of 1/16-BPS states in the maximally supersymmetric Yang-Mills...
Black-hole solutions to general relativity carry a thermodynamic entropy, discovered by Bekenstein a...
A family of spacetimes suitable for describing the interior of a non-rotational black hole is constr...
We analyze the thermodynamical properties of the regular static and spherically symmetric black hole...
We solve the Wheeler DeWitt equation for the planar Reissner-Nordstr\"om-AdS black hole in a minisup...
We consider numerical black hole solutions in the Weyl conformal geometry, and its associated confor...
Indexación: SpringerWe consider the role of the type-A trace anomaly in static black hole solutions ...
The thermodynamic properties of black holes -- temperature, entropy and radiation rates -- are usual...
We study the quantum error correction properties of the black hole interior in a toy model for an ev...
We systematically calculate the quantum extremal surface (QES) associated with Hawking radiation for...
We analyze the thermodynamical properties of the regular static and spherically symmetric black hole...
In general, a finite metric function at the center of a black hole describes a non-singular spacetim...
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 regularized 4-dimensional Einstein-Gauss-Bonnet (EGB) gravity derived from a Kaluza-Klein reducti...
We revamp the constructive enumeration of 1/16-BPS states in the maximally supersymmetric Yang-Mills...
Black-hole solutions to general relativity carry a thermodynamic entropy, discovered by Bekenstein a...
A family of spacetimes suitable for describing the interior of a non-rotational black hole is constr...