Search results for " cosmological parameters from CMBR"

showing 2 items of 2 documents

Cosmological bounds on neutrino statistics

2018

We consider the phenomenological implications of the violation of the Pauli exclusion principle for neutrinos, focusing on cosmological observables such as the spectrum of Cosmic Microwave Background anisotropies, Baryon Acoustic Oscillations and the primordial abundances of light elements. Neutrinos that behave (at least partly) as bosonic particles have a modified equilibrium distribution function that implies a different influence on the evolution of the Universe that, in the case of massive neutrinos, can not be simply parametrized by a change in the effective number of neutrinos. Our results show that, despite the precision of the available cosmological data, only very weak bounds can …

AstrofísicaCosmology and Nongalactic Astrophysics (astro-ph.CO)Astrophysics::High Energy Astrophysical PhenomenaCosmic microwave backgroundFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic AstrophysicsNeutrino properties01 natural sciencesPartícules (Física nuclear)symbols.namesakePauli exclusion principleHigh Energy Physics - Phenomenology (hep-ph)Big Bang nucleosynthesis0103 physical sciencesStatisticsAnisotropy010303 astronomy & astrophysicsPhysicsCosmologia010308 nuclear & particles physicsBig bang nucleosynthesisSpectrum (functional analysis)High Energy Physics::PhenomenologyObservableAstronomy and AstrophysicsCosmological neutrinos neutrino properties big bang nucleosynthesis cosmological parameters from CMBRCosmological parameters from CMBRHigh Energy Physics - Phenomenologysymbolsastro-ph.COBig bang nucleosynthesis; Cosmological neutrinos; Cosmological parameters from CMBR; Neutrino properties; astro-ph.CO; astro-ph.CO; High Energy Physics - Phenomenology; Astronomy and AstrophysicsCosmological neutrinosHigh Energy Physics::ExperimentBaryon acoustic oscillationsNeutrinoAstrophysics - Cosmology and Nongalactic Astrophysics
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Cosmic microwave background constraints on secret interactions among sterile neutrinos

2017

Secret contact interactions among eV sterile neutrinos, mediated by a massive gauge boson $X$ (with $M_X \ll M_W$), and characterized by a gauge coupling $g_X$, have been proposed as a mean to reconcile cosmological observations and short-baseline laboratory anomalies. We constrain this scenario using the latest Planck data on Cosmic Microwave Background anisotropies, and measurements of baryon acoustic oscillations (BAO). We consistently include the effect of secret interactions on cosmological perturbations, namely the increased density and pressure fluctuations in the neutrino fluid, and still find a severe tension between the secret interaction framework and cosmology. In fact, taking i…

Sterile neutrinoParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)cosmological neutrinosDark matterCosmic microwave backgroundFOS: Physical sciencescosmological neutrinos; cosmological parameters from CMBR; neutrino masses from cosmology; neutrino properties; Astronomy and AstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesNOsymbols.namesakeHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesPlanck010303 astronomy & astrophysicsneutrino propertiesPhysicsGauge bosoncosmological neutrino010308 nuclear & particles physicsHigh Energy Physics::Phenomenologycosmological parameters from CMBRAstronomy and Astrophysicsneutrino masses from cosmologyCoupling (probability)3. Good healthHigh Energy Physics - Phenomenology13. Climate actionsymbolsHigh Energy Physics::ExperimentBaryon acoustic oscillationsNeutrinoAstrophysics - Cosmology and Nongalactic Astrophysics
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