Search results for "Microwave Background Anisotropies"

showing 2 items of 2 documents

Model independent constraints on mass-varying neutrino scenarios

2009

Models of dark energy in which neutrinos interact with the scalar field supposed to be responsible for the acceleration of the Universe usually imply a variation of the neutrino masses on cosmological time scales. In this work we propose a parametrization for the neutrino mass variation that captures the essentials of those scenarios and allows one to constrain them in a model independent way, that is, without resorting to any particular scalar field model. Using WMAP 5 yr data combined with the matter power spectrum of SDSS and 2dFGRS, the limit on the present value of the neutrino mass is m(0) equivalent to m(nu)(z = 0) 0), totally consistent with no mass variation. These stringent bounds…

Nuclear and High Energy PhysicsParticle physicsAstrophysics and AstronomyAccelerating UniverseCosmology and Nongalactic Astrophysics (astro-ph.CO)Microwave Background Anisotropiesmedia_common.quotation_subjectFOS: Physical sciencesAstrophysicsCosmological constant01 natural sciences[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]High Energy Physics - Phenomenology (hep-ph)0103 physical sciencesPower-SpectrumNeutrino oscillation010303 astronomy & astrophysicsmedia_commonPhysicsMatter010308 nuclear & particles physicsMatter power spectrumHigh Energy Physics::PhenomenologyFísicaHubble-Space-TelescopeDark EnergyCMB cold spotCosmological ConstantUniverseHigh Energy Physics - PhenomenologySupernovaeDark energyHigh Energy Physics::ExperimentNeutrinoScalar fieldAstrophysics - Cosmology and Nongalactic Astrophysics
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Dark radiation and interacting scenarios

2013

An extra dark radiation component can be present in the universe in the form of sterile neutrinos, axions or other very light degrees of freedom which may interact with the dark matter sector. We derive here the cosmological constraints on the dark radiation abundance, on its effective velocity and on its viscosity parameter from current data in dark radiation-dark matter coupled models. The cosmological bounds on the number of extra dark radiation species do not change significantly when considering interacting schemes. We also find that the constraints on the dark radiation effective velocity are degraded by an order of magnitude while the errors on the viscosity parameter are a factor of…

Nuclear and High Energy PhysicsSterile neutrinoCosmology and Nongalactic Astrophysics (astro-ph.CO)Dark matterCosmological parametersCosmic background radiationFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesCosmologyRadiacióPower spectrumsymbols.namesakeHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciences010303 astronomy & astrophysicsAxionTelescopeDigital sky surveyPhysicsCosmologiaHubble constant010308 nuclear & particles physicsSpectral densityMicrowave background anisotropiesHigh Energy Physics - Phenomenology13. Climate actionDark radiationConstraintssymbolsHubble's lawAstrophysics - Cosmology and Nongalactic Astrophysics
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