International audienceFollowing recent claims relative to the question of large anisotropy production in regular bouncing scenarios, we study the evolution of such anisotropies in a model where an ekpyrotic phase of contraction is followed by domination of a Galileon-type Lagrangian which generates a non-singular bounce. We show that the anisotropies decrease during the phase of ekpyrotic contraction (as expected) and that they can be constrained to remain small during the non-singular bounce phase (a non-trivial result). Specifically, we derive the e-folding number of the phase of ekpyrotic contraction which leads to a present-day anisotropy in agreement with current observational bounds. Communicated by P Sing
AbstractWe recently showed how it is possible to use a cubic Galileon action to construct classical ...
International audienceThe simplest possible classical model leading to a cosmological bounce is exam...
International audienceWe compute the level of non-gaussianities produced by a cosmological bouncing ...
We analyze the Galileon ghost condensate implementation of a bouncing cosmological model in the pres...
We consider a simple cosmological model that includes a long ekpyrotic contraction stage and smooth ...
Bouncing cosmologies are often proposed as alternatives to standard inflation for the explanation of...
We study the behaviour of Bianchi class A universes containing an ultra-stiff isotropic ghost field ...
Martin J, Peter P, Pinto-Neto N, Schwarz D. Passing through the bounce in the ekpyrotic models. PHYS...
We show that it is possible to realize a cosmological bouncing solution in an anisotropic but homoge...
In bouncing cosmology, the primordial fluctuations are generated in a cosmic contraction phase befor...
We investigate bouncing solutions in the framework of the nonsingular gravity model of Brandenberger...
A period of slow contraction with equation of state w>1, known as an ekpyrotic phase, has been shown...
We study a model for a non-singular cosmic bounce in N=1 supergravity, based on supergravity version...
In the context of a ghost free f(R,G) model, we present a non-singular cosmological scenario in whic...
We recently showed how it is possible to use a cubic Galileon action to construct classical cosmolog...
AbstractWe recently showed how it is possible to use a cubic Galileon action to construct classical ...
International audienceThe simplest possible classical model leading to a cosmological bounce is exam...
International audienceWe compute the level of non-gaussianities produced by a cosmological bouncing ...
We analyze the Galileon ghost condensate implementation of a bouncing cosmological model in the pres...
We consider a simple cosmological model that includes a long ekpyrotic contraction stage and smooth ...
Bouncing cosmologies are often proposed as alternatives to standard inflation for the explanation of...
We study the behaviour of Bianchi class A universes containing an ultra-stiff isotropic ghost field ...
Martin J, Peter P, Pinto-Neto N, Schwarz D. Passing through the bounce in the ekpyrotic models. PHYS...
We show that it is possible to realize a cosmological bouncing solution in an anisotropic but homoge...
In bouncing cosmology, the primordial fluctuations are generated in a cosmic contraction phase befor...
We investigate bouncing solutions in the framework of the nonsingular gravity model of Brandenberger...
A period of slow contraction with equation of state w>1, known as an ekpyrotic phase, has been shown...
We study a model for a non-singular cosmic bounce in N=1 supergravity, based on supergravity version...
In the context of a ghost free f(R,G) model, we present a non-singular cosmological scenario in whic...
We recently showed how it is possible to use a cubic Galileon action to construct classical cosmolog...
AbstractWe recently showed how it is possible to use a cubic Galileon action to construct classical ...
International audienceThe simplest possible classical model leading to a cosmological bounce is exam...
International audienceWe compute the level of non-gaussianities produced by a cosmological bouncing ...