Search results for " Big Bang Nucleosynthesis"

showing 3 items of 3 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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Bounds on very low reheating scenarios after Planck

2015

9 pages.- 9 figures

Nuclear and High Energy PhysicsParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Astrophysics::High Energy Astrophysical PhenomenaEarly universeFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic AstrophysicsUpper and lower boundsCosmologysymbols.namesakeGeneral Relativity and Quantum CosmologyHigh Energy Physics - Phenomenology (hep-ph)Big Bang nucleosynthesisPlanckPhysicsCosmology Big Bang NucleosynthesisOscillationHigh Energy Physics::PhenomenologyFísicaHigh Energy Physics - PhenomenologysymbolsProduction (computer science)High Energy Physics::ExperimentNeutrinoAstrophysics - Cosmology and Nongalactic AstrophysicsPrimordial abundance
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New reaction rates for the destruction of $^7$Be during big bang nucleosynthesis measured at CERN/n_TOF and their implications on the cosmological li…

2019

New measurements of the7Be(n,α)4He and7Be(n,p)7Li reaction cross sections from thermal to keV neutron energies have been recently performed at CERN/n_TOF. Based on the new experimental results, astrophysical reaction rates have been derived for both reactions, including a proper evaluation of their uncertainties in the thermal energy range of interest for big bang nucleosynthesis studies. The new estimate of the7Be destruction rate, based on these new results, yields a decrease of the predicted cosmological7Li abundance insufficient to provide a viable solution to the cosmological lithium problem.

PhysicsRange (particle radiation)Large Hadron Collidern_TOF 7Be big bang nucleosynthesis cosmological lithium problem010308 nuclear & particles physicsPhysicsQC1-999chemistry.chemical_element[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]7. Clean energy01 natural sciencesReaction rateNuclear physicsBig Bang nucleosynthesischemistry13. Climate action0103 physical sciencesThermalNeutronLithiumNuclear Physics - Experiment010306 general physicsNuclear Experiment
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