0000000000347688

AUTHOR

Laura Lopez Honorez

showing 2 related works from this author

Dark coupling and gauge invariance

2010

We study a coupled dark energy–dark matter model in which the energymomentum exchange is proportional to the Hubble expansion rate. The inclusion of its perturbation is required by gauge invariance. We derive the linear perturbation equations for the gauge invariant energy density contrast and velocity of the coupled fluids, and we determine the initial conditions. The latter turn out to be adiabatic for dark energy, when assuming adiabatic initial conditions for all the standard fluids. We perform a full Monte Carlo Markov Chain likelihood analysis of the model, using WMAP 7-year data.

AstrofísicaAstrophysics and AstronomyCosmology and Nongalactic Astrophysics (astro-ph.CO)Monte Carlo methodFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesCosmologysymbols.namesakeHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesCosmological perturbation theoryGauge theoryAdiabatic process010303 astronomy & astrophysicsPhysics010308 nuclear & particles physicsFísicaAstronomy and AstrophysicsMarkov chain Monte CarloHigh Energy Physics - PhenomenologyQuantum electrodynamicssymbolsDark energyHubble's lawAstrophysics - Cosmology and Nongalactic Astrophysics
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Coupled dark matter-dark energy in light of near Universe observations

2010

Cosmological analysis based on currently available observations are unable to rule out a sizeable coupling among the dark energy and dark matter fluids. We explore a variety of coupled dark matter-dark energy models, which satisfy cosmic microwave background constraints, in light of low redshift and near universe observations. We illustrate the phenomenology of different classes of dark coupling models, paying particular attention in distinguishing between effects that appear only on the expansion history and those that appear in the growth of structure. We find that while a broad class of dark coupling models are effectively models where general relativity (GR) is modified - and thus can b…

Astrophysics and AstronomyCosmology and Nongalactic Astrophysics (astro-ph.CO)General relativityCosmic microwave backgroundDark matterFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsEnergia fosca (Astronomia)01 natural sciencesRedshift-space distortionssymbols.namesake0103 physical sciencesDark energy (Astronomy)010303 astronomy & astrophysicsPhysicsCosmologia010308 nuclear & particles physicsAstronomy and AstrophysicsGalaxyRedshiftCosmologyDark matter (Astronomy)symbolsDark energyMatèria fosca (Astronomia)Astrophysics - Cosmology and Nongalactic AstrophysicsHubble's law
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