We consider scalar perturbations in the time dependent Horava-Witten model in order to probe its stability. We show that during the nonsingular epoque the model evolves without instabilities until it encounters the curvature singularity where a big crunch is supposed to occur. We compute the frequencies of the scalar field oscillation during the stable period and show how the oscillations can be used to prove the presence of such a singularity
Many and very general arguments indicate that the event horizon behaves as a stretched membrane. We ...
General-relativistic stable spacetimes can be made unstable under the presence of certain nonminimal...
We explore nonequilibrium dynamics of inhomogeneous nonlinearly interacting scalar fields in several...
We consider scalar perturbations in the time dependent Horava-Witten model in order to probe its sta...
We consider scalar perturbations in the time dependent Horava-Witten model in order to probe its sta...
Horava-Witten spacetimes necessarily include two branes of opposite tension. If these branes are BPS...
© 2017 IOP Publishing Ltd and Sissa Medialab srl. In expanding FRW spacetimes, it is usually the cas...
We present a detailed study of a simple scalar field model that yields non-singular cosmological sol...
Horava-Lifshitz gravity is a potentially UV complete theory with important implications for the very...
We consider here the dynamics of some homogeneous and isotropic cosmological models with N interacti...
Bouncing solutions are obtained from a generally covariant action characterized by a potential which...
Bouncing solutions are obtained from a generally covariant action characterized by a potential which...
Bouncing solutions are obtained from a generally covariant action characterized by a potential which...
In this paper, we introduce a non-minimally conformally coupled scalar field and dark matter in F(T)...
The behavior of fundamental fields in strong gravity or nontrivial environments is important for our...
Many and very general arguments indicate that the event horizon behaves as a stretched membrane. We ...
General-relativistic stable spacetimes can be made unstable under the presence of certain nonminimal...
We explore nonequilibrium dynamics of inhomogeneous nonlinearly interacting scalar fields in several...
We consider scalar perturbations in the time dependent Horava-Witten model in order to probe its sta...
We consider scalar perturbations in the time dependent Horava-Witten model in order to probe its sta...
Horava-Witten spacetimes necessarily include two branes of opposite tension. If these branes are BPS...
© 2017 IOP Publishing Ltd and Sissa Medialab srl. In expanding FRW spacetimes, it is usually the cas...
We present a detailed study of a simple scalar field model that yields non-singular cosmological sol...
Horava-Lifshitz gravity is a potentially UV complete theory with important implications for the very...
We consider here the dynamics of some homogeneous and isotropic cosmological models with N interacti...
Bouncing solutions are obtained from a generally covariant action characterized by a potential which...
Bouncing solutions are obtained from a generally covariant action characterized by a potential which...
Bouncing solutions are obtained from a generally covariant action characterized by a potential which...
In this paper, we introduce a non-minimally conformally coupled scalar field and dark matter in F(T)...
The behavior of fundamental fields in strong gravity or nontrivial environments is important for our...
Many and very general arguments indicate that the event horizon behaves as a stretched membrane. We ...
General-relativistic stable spacetimes can be made unstable under the presence of certain nonminimal...
We explore nonequilibrium dynamics of inhomogeneous nonlinearly interacting scalar fields in several...