We investigate future constraints on early dark energy (EDE) achievable by the Planck and CMBPol experiments, including cosmic microwave background (CMB) lensing. For the dark energy, we include the possibility of clustering through a sound speed cs2<1 (cold dark energy) and anisotropic stresses parametrized with a viscosity parameter cvis2. We discuss the degeneracies between cosmological parameters and EDE parameters. In particular we show that the presence of anisotropic stresses in EDE models can substantially undermine the determination of the EDE sound speed parameter cs2. The constraints on EDE primordial energy density are however unaffected. We also calculate the future CMB constraints on neutrino masses and find that they are weak...
We perform a detailed forecast on how well a Euclid-like survey will be able to constrain dark energ...
International audienceCosmological data still allow for the presence of a non-negligible amount of d...
We forecast the expected cosmological constraints from a combination of probes of both the universal...
We investigate future constraints on early dark energy (EDE) achievable by the Planck and CMBPol exp...
We investigate future constraints on early dark energy (EDE) achievable by the Planck and CMBPol exp...
We investigate future constraints on early dark energy (EDE) achievable by the Planck and CMBPol exp...
We consider an Early Dark Energy (EDE) cosmological model, and perform an analysis which takes into ...
We perform a detailed forecast on how well a Euclid-like survey will be able to constrain dark energ...
Anisotropies in the angular power spectra of the Cosmic Microwave Background (CMB) temperature and p...
International audienceThe early dark energy (EDE) scenario aims to increase the value of the Hubble ...
A dark energy–like component in the early universe, known as early dark energy (EDE), is a proposed ...
International audienceThe early dark energy (EDE) scenario aims to increase the value of the Hubble ...
Despite the great progress of current cosmological measurements, the nature of the dominant componen...
Despite the great progress of current cosmological measurements, the nature of the dominant componen...
We perform a detailed forecast on how well a Euclid-like survey will be able to constrain dark energ...
We perform a detailed forecast on how well a Euclid-like survey will be able to constrain dark energ...
International audienceCosmological data still allow for the presence of a non-negligible amount of d...
We forecast the expected cosmological constraints from a combination of probes of both the universal...
We investigate future constraints on early dark energy (EDE) achievable by the Planck and CMBPol exp...
We investigate future constraints on early dark energy (EDE) achievable by the Planck and CMBPol exp...
We investigate future constraints on early dark energy (EDE) achievable by the Planck and CMBPol exp...
We consider an Early Dark Energy (EDE) cosmological model, and perform an analysis which takes into ...
We perform a detailed forecast on how well a Euclid-like survey will be able to constrain dark energ...
Anisotropies in the angular power spectra of the Cosmic Microwave Background (CMB) temperature and p...
International audienceThe early dark energy (EDE) scenario aims to increase the value of the Hubble ...
A dark energy–like component in the early universe, known as early dark energy (EDE), is a proposed ...
International audienceThe early dark energy (EDE) scenario aims to increase the value of the Hubble ...
Despite the great progress of current cosmological measurements, the nature of the dominant componen...
Despite the great progress of current cosmological measurements, the nature of the dominant componen...
We perform a detailed forecast on how well a Euclid-like survey will be able to constrain dark energ...
We perform a detailed forecast on how well a Euclid-like survey will be able to constrain dark energ...
International audienceCosmological data still allow for the presence of a non-negligible amount of d...
We forecast the expected cosmological constraints from a combination of probes of both the universal...