Search results for "Dark energy experiments"

showing 2 items of 2 documents

Testing LTB void models without the cosmic microwave background or large scale structure: new constraints from galaxy ages

2012

We present new observational constraints on inhomogenous models based on observables independent of the CMB and large-scale structure. Using Bayesian evidence we find very strong evidence for homogeneous LCDM model, thus disfavouring inhomogeneous models. Our new constraints are based on quantities independent of the growth of perturbations and rely on cosmic clocks based on atomic physics and on the local density of matter.

AstrofísicaVoid (astronomy)Cosmology and Nongalactic Astrophysics (astro-ph.CO)dark energy experimentsCosmic microwave backgroundgalaxy evolutionFOS: Physical sciencesAstrophysicsBayesian evidenceAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics01 natural sciences0103 physical sciencesScale structuredark energy theory010303 astronomy & astrophysicsPhysicsCOSMIC cancer databaseCosmologia010308 nuclear & particles physicsAstronomy and AstrophysicsObservableGalaxiesGalaxyGalàxiesCosmologyHomogeneousAstrophysics - Cosmology and Nongalactic Astrophysics
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The dark side of curvature

2009

Geometrical tests such as the combination of the Hubble parameter H(z) and the angular diameter distance d(A)(z) can, in principle, break the degeneracy between the dark energy equation of state parameter w(z), and the spatial curvature Omega(k) in a direct, model-independent way. In practice, constraints on these quantities achievable from realistic experiments, such as those to be provided by Baryon Acoustic Oscillation (BAO) galaxy surveys in combination with CMB data, can resolve the cosmic confusion between the dark energy equation of state parameter and curvature only statistically and within a parameterized model for w(z). Combining measurements of both H(z) and d(A)(z) up to suffici…

Equation of stateCosmology and Nongalactic Astrophysics (astro-ph.CO)Cosmic microwave backgroundFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsCurvature01 natural sciencessymbols.namesakeHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesDark energy experiments010303 astronomy & astrophysicsPhysics010308 nuclear & particles physicsAngular diameter distanceAstronomy and AstrophysicsRedshiftCosmological parameters from CMBRHigh Energy Physics - PhenomenologysymbolsDark energyBaryon acoustic-oscillationsBaryon acoustic oscillationsHubble's lawAstrophysics - Cosmology and Nongalactic Astrophysics
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