11 pages, 7 figures, uses revtexWe explore the possibility of putting constraints on quintessence models with large-scale structure observations. In particular we compute the linear and second order growth rate of the fluctuations in different flavors of quintessence scenarios. We show that effective models of quintessence (e.g. with a constant equation of state) do not account of the results found in more realistic scenarios. The impact of these results on observational quantities such as the shape of the non-linear power spectrum in weak lensing surveys or the skewness of the convergence field are investigated. It appears that the observational signature of quintessence models are specific and rather large. They clearly cannot be mistaken...
We derive the evolution of the linear bias factor, $b(z)$, in cosmological models driven by an exoti...
International audienceQuintessence has been proposed to account for dark energy (DE) in the Universe...
We apply the Effective Field Theory of Large-Scale Structure (EFTofLSS) to analyze cosmological mod...
We use some of the recently released observational data to test the viability of two classes of mini...
We model the nonlinear growth of cosmic structure in different dark energy models, using large volum...
We carry out a comprehensive study of the dynamics of large-scale perturbations in quintessence scen...
Bibliography: leaves 100-106.v, 107 leaves : ill. ; 30 cm.Studies different models of "quintessence"...
We study the non-linear growth of cosmic structure in different dark energy models, using large volu...
I investigate through simulations the redshift dependence of several lensing measures for two cosmol...
Recent observations indicate that the majority of all matter in the universe is in the form of a d...
We study structure formation in non-minimally coupled dark energy models, where there is a coupling ...
Dark energy as a quintessence component causes a typical modification of the background cosmic expan...
A short review of some of the aspects of quintessence model building is presented. We emphasize the ...
In this work we model the quintessence potential in a Taylor series expansion, up to second order, a...
We investigate the observational consequences of the quintessence field rolling to and oscillating n...
We derive the evolution of the linear bias factor, $b(z)$, in cosmological models driven by an exoti...
International audienceQuintessence has been proposed to account for dark energy (DE) in the Universe...
We apply the Effective Field Theory of Large-Scale Structure (EFTofLSS) to analyze cosmological mod...
We use some of the recently released observational data to test the viability of two classes of mini...
We model the nonlinear growth of cosmic structure in different dark energy models, using large volum...
We carry out a comprehensive study of the dynamics of large-scale perturbations in quintessence scen...
Bibliography: leaves 100-106.v, 107 leaves : ill. ; 30 cm.Studies different models of "quintessence"...
We study the non-linear growth of cosmic structure in different dark energy models, using large volu...
I investigate through simulations the redshift dependence of several lensing measures for two cosmol...
Recent observations indicate that the majority of all matter in the universe is in the form of a d...
We study structure formation in non-minimally coupled dark energy models, where there is a coupling ...
Dark energy as a quintessence component causes a typical modification of the background cosmic expan...
A short review of some of the aspects of quintessence model building is presented. We emphasize the ...
In this work we model the quintessence potential in a Taylor series expansion, up to second order, a...
We investigate the observational consequences of the quintessence field rolling to and oscillating n...
We derive the evolution of the linear bias factor, $b(z)$, in cosmological models driven by an exoti...
International audienceQuintessence has been proposed to account for dark energy (DE) in the Universe...
We apply the Effective Field Theory of Large-Scale Structure (EFTofLSS) to analyze cosmological mod...