AbstractA cosmological scenario is proposed, which simultaneously solves the mass hierarchy and the small dark energy problem. In the present scenario an effective gravity mass scale (inverse of the Newton's constant) increases during the inflationary period. The small cosmological constant or the dark energy density in the present universe is dynamically realized by introducing two, approximately O(2) symmetric dilatons, taking the fundamental mass scale at TeV
A pedagogical introduction to aspects of string cosmology, including the landscape (BPBT) solution t...
The early cosmic inflation, when taken along with the recent observations that the universe is curre...
AbstractThe cosmological constant problem is studied in a two component cosmological model. The univ...
AbstractA cosmological scenario is proposed, which simultaneously solves the mass hierarchy and the ...
We discuss the cosmological phenomenology of biscalar-tensor models displaying a maximally symmetric...
We discuss the cosmological phenomenology of biscalar-tensor models displaying a maximally symmetric...
AbstractRecent cosmological data favor R2-inflation and some amount of non-standard dark radiation i...
Recent cosmological data favor R2 -inflation and some amount of non-standard dark radiation in the U...
I describe the phenomenology of a model of supersymmetry breaking in the presence of a tiny (tuneabl...
AbstractWe show that holographic dark energy could explain why the current dark energy density is so...
One of the most pressing, modern cosmological mysteries is the cause of the accelerated expansion o...
AbstractWe construct a class of theories which are scale-invariant on quantum level in all orders of...
I describe the phenomenology of a model of supersymmetry breaking in the presence of a tiny (tuneabl...
URL: http://www-spht.cea.fr/articles/T03/162 (sur invitation).International audienceObservational ev...
The early cosmic inflation, when taken along with the recent observations that the universe is curre...
A pedagogical introduction to aspects of string cosmology, including the landscape (BPBT) solution t...
The early cosmic inflation, when taken along with the recent observations that the universe is curre...
AbstractThe cosmological constant problem is studied in a two component cosmological model. The univ...
AbstractA cosmological scenario is proposed, which simultaneously solves the mass hierarchy and the ...
We discuss the cosmological phenomenology of biscalar-tensor models displaying a maximally symmetric...
We discuss the cosmological phenomenology of biscalar-tensor models displaying a maximally symmetric...
AbstractRecent cosmological data favor R2-inflation and some amount of non-standard dark radiation i...
Recent cosmological data favor R2 -inflation and some amount of non-standard dark radiation in the U...
I describe the phenomenology of a model of supersymmetry breaking in the presence of a tiny (tuneabl...
AbstractWe show that holographic dark energy could explain why the current dark energy density is so...
One of the most pressing, modern cosmological mysteries is the cause of the accelerated expansion o...
AbstractWe construct a class of theories which are scale-invariant on quantum level in all orders of...
I describe the phenomenology of a model of supersymmetry breaking in the presence of a tiny (tuneabl...
URL: http://www-spht.cea.fr/articles/T03/162 (sur invitation).International audienceObservational ev...
The early cosmic inflation, when taken along with the recent observations that the universe is curre...
A pedagogical introduction to aspects of string cosmology, including the landscape (BPBT) solution t...
The early cosmic inflation, when taken along with the recent observations that the universe is curre...
AbstractThe cosmological constant problem is studied in a two component cosmological model. The univ...