The reently proposed proof by Jensen and Stein-Schabes of the No Hair Theorem for inhomogeneous spacetimes is analyzed, putting a special emphasis on the asymptotic behavior of the shear and curvature. It is concluded that the theorem only holds locally, and the minimum size a region should be is estimated in order for it to inflate. The assumptions used in the theorem are discussed in detail. The last section speculates about the possible measure of the set of spacetimes that would undergo inflation
According to the `Cosmological Central Dogma', de Sitter space can be viewed as a quantum mechanical...
We conjecture the following entropy bound to be valid in all space-times admitted by Einstein's equa...
The no-boundary wave function (NBWF) specifies a measure for prediction in cosmology that selects in...
Interest in the attracting property of de Sitter space-time has grown during the 'infla-tionary...
We study the asymptotic stability of de Sitter spacetime with respect to non-linear perturbations, b...
An introduction to the physics of inflation and to the no-hair theorem is presented, raising the uns...
Theses (M.Sc.)-University of Natal, 1996.Interest in the attracting property of de Sitter space-time...
We show that under very general conditions any inhomogeneous cosmological model with a positive cosm...
The possibility of having inflation in a renormalizable cosmological model is investigated. The Cosm...
We present results on the nonlinear dynamics of inhomogeneous cosmological models with irrotational ...
The gravitational entropy and no-hair conjectures seem to predict contradictory future states of our...
We study how the initial inhomogeneities of the spatial curvature affect the onset of inflation in t...
The simplicity of black holes, as characterized by no-hair theorems, is one of the most important ma...
The Cohen–Kaplan–Nelson (CKN) bound formulates the condition that black hole is not produced by the ...
We consider landscape models that admit several regions where the conditions for eternal inflation h...
According to the `Cosmological Central Dogma', de Sitter space can be viewed as a quantum mechanical...
We conjecture the following entropy bound to be valid in all space-times admitted by Einstein's equa...
The no-boundary wave function (NBWF) specifies a measure for prediction in cosmology that selects in...
Interest in the attracting property of de Sitter space-time has grown during the 'infla-tionary...
We study the asymptotic stability of de Sitter spacetime with respect to non-linear perturbations, b...
An introduction to the physics of inflation and to the no-hair theorem is presented, raising the uns...
Theses (M.Sc.)-University of Natal, 1996.Interest in the attracting property of de Sitter space-time...
We show that under very general conditions any inhomogeneous cosmological model with a positive cosm...
The possibility of having inflation in a renormalizable cosmological model is investigated. The Cosm...
We present results on the nonlinear dynamics of inhomogeneous cosmological models with irrotational ...
The gravitational entropy and no-hair conjectures seem to predict contradictory future states of our...
We study how the initial inhomogeneities of the spatial curvature affect the onset of inflation in t...
The simplicity of black holes, as characterized by no-hair theorems, is one of the most important ma...
The Cohen–Kaplan–Nelson (CKN) bound formulates the condition that black hole is not produced by the ...
We consider landscape models that admit several regions where the conditions for eternal inflation h...
According to the `Cosmological Central Dogma', de Sitter space can be viewed as a quantum mechanical...
We conjecture the following entropy bound to be valid in all space-times admitted by Einstein's equa...
The no-boundary wave function (NBWF) specifies a measure for prediction in cosmology that selects in...