We study the possibility of non-singular black hole solutions in the theory of general relativity coupled to a non-linear scalar field with a positive potential possessing two minima: a `false vacuum' with positive energy and a `true vacuum' with zero energy. Assuming that the scalar field starts at the false vacuum at the origin and comes to the true vacuum at spatial infinity, we prove a no-go theorem by extending a no-hair theorem to the black hole interior: no smooth solutions exist which interpolate between the local de Sitter solution near the origin and the asymptotic Schwarzschild solution through a regular event horizon or several horizons
We consider static, spherically symmetric, electrically or/and magnetically charged configurations o...
We argue the existence of solutions of the Euclidean Einstein equations that correspond to a vortex ...
In this paper we present a non-singular black hole model as a possible end-product of gravitational ...
We enumerate all possible types of spacetime causal structures that can appear in static, sphericall...
We prove some theorems characterizing the global properties of static, spherically symmetric configu...
I enumerate all possible types of spacetime causal structures that can appear in static, spherically...
I enumerate all possible types of spacetime causal structures that can appear in static, spherically...
This paper is concerned with several not-quantum aspects of black holes, with emphasis on theoretica...
A static spherically symmetric metric in Einstein-scalar-tensor gravity theory with a scalar field p...
The static spherically symmetric ``black hole solution" of the Einstein - conformally invariant mass...
We study the thermodynamics of n -dimensional static asymptotically AdS black holes in Einstein grav...
Abstract With the back reaction of the vacuum energy-momentum tensor consistently taken into account...
When a potential for a scalar field has two local minima, there arises structure of spherical shells...
In this paper we study the properties of black holes and scalarons in Einstein gravity when it is mi...
As an example of a black hole in a non-flat background a composite static spacetime is constructed. ...
We consider static, spherically symmetric, electrically or/and magnetically charged configurations o...
We argue the existence of solutions of the Euclidean Einstein equations that correspond to a vortex ...
In this paper we present a non-singular black hole model as a possible end-product of gravitational ...
We enumerate all possible types of spacetime causal structures that can appear in static, sphericall...
We prove some theorems characterizing the global properties of static, spherically symmetric configu...
I enumerate all possible types of spacetime causal structures that can appear in static, spherically...
I enumerate all possible types of spacetime causal structures that can appear in static, spherically...
This paper is concerned with several not-quantum aspects of black holes, with emphasis on theoretica...
A static spherically symmetric metric in Einstein-scalar-tensor gravity theory with a scalar field p...
The static spherically symmetric ``black hole solution" of the Einstein - conformally invariant mass...
We study the thermodynamics of n -dimensional static asymptotically AdS black holes in Einstein grav...
Abstract With the back reaction of the vacuum energy-momentum tensor consistently taken into account...
When a potential for a scalar field has two local minima, there arises structure of spherical shells...
In this paper we study the properties of black holes and scalarons in Einstein gravity when it is mi...
As an example of a black hole in a non-flat background a composite static spacetime is constructed. ...
We consider static, spherically symmetric, electrically or/and magnetically charged configurations o...
We argue the existence of solutions of the Euclidean Einstein equations that correspond to a vortex ...
In this paper we present a non-singular black hole model as a possible end-product of gravitational ...