0000000000388735

AUTHOR

Matteo Martinelli

0000-0002-6943-7732

showing 3 related works from this author

Future constraints on the Hu-Sawicki modified gravity scenario

2011

We present current and future constraints on the Hu and Sawicki modified gravity scenario. This model can reproduce a late time accelerated universe and evade solar system constraints. While current cosmological data still allows for distinctive deviations from the cosmological constant picture, future measurements of the growth of structure combined with Supernova Ia luminosity distance data will greatly improve present constraints.

PhysicsNuclear and High Energy PhysicsGravity (chemistry)Solar SystemCosmology and Nongalactic Astrophysics (astro-ph.CO)media_common.quotation_subjectFOS: Physical sciencesFísicaAstrophysicsCosmological constantAstrophysics::Cosmology and Extragalactic AstrophysicsCosmologyUniverseSupernovaLuminosity distancemedia_commonAstrophysics - Cosmology and Nongalactic Astrophysics
researchProduct

Future weak lensing constraints in a dark coupled universe

2011

Coupled cosmologies can predict values for the cosmological parameters at low redshifts which may differ substantially from the parameters values within non-interacting cosmologies. Therefore, low redshift probes, as the growth of structure and the dark matter distribution via galaxy and weak lensing surveys constitute a unique tool to constrain interacting dark sector models. We focus here on weak lensing forecasts from future Euclid and LSST-like surveys combined with the ongoing Planck cosmic microwave background experiment. We find that these future data could constrain the dimensionless coupling to be smaller than a few $\times 10^{-2}$. The coupling parameter $\xi$ is strongly degener…

PhysicsNuclear and High Energy PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Hot dark matterDark matterScalar field dark matterFísicaFOS: Physical sciencesLambda-CDM modelAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsCoupling (probability)High Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Dark energyWeak gravitational lensingDark fluidAstrophysics - Cosmology and Nongalactic Astrophysics
researchProduct

Future CMB cosmological constraints in a dark coupled universe

2010

Cosmic microwave background satellite missions as the ongoing Planck experiment are expected to provide the strongest constraints on a wide set of cosmological parameters. Those constraints, however, could be weakened when the assumption of a cosmological constant as the dark energy component is removed. Here we show that it will indeed be the case when there exists a coupling among the dark energy and the dark matter fluids. In particular, the expected errors on key parameters as the cold dark matter density and the angular diameter distance at decoupling are significantly larger when a dark coupling is introduced. We show that it will be the case also for future satellite missions as EPIC…

AstrofísicaAstrophysics and AstronomyNuclear and High Energy PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Cold dark matterDark matterScalar field dark matterFOS: Physical sciencesLambda-CDM modelGeneral Relativity and Quantum Cosmology (gr-qc)Astrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics01 natural sciencesGeneral Relativity and Quantum CosmologyThermodynamics of the universeHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciences010303 astronomy & astrophysicsPhysics010308 nuclear & particles physicsHot dark matterAstronomyHigh Energy Physics - PhenomenologyDark energyDark fluidAstrophysics - Cosmology and Nongalactic AstrophysicsPhysical Review D
researchProduct