Search results for "Physics of the early Universe"

showing 2 items of 12 documents

On the full Boltzmann equations for leptogenesis

2009

We consider the full Boltzmann equations for standard and soft leptogenesis, instead of the usual integrated Boltzmann equations which assume kinetic equilibrium for all species. Decays and inverse decays may be inefficient for thermalising the heavy-(s)neutrino distribution function, leading to significant deviations from kinetic equilibrium. We analyse the impact of using the full kinetic equations in the case of a previously generated lepton asymmetry, and find that the washout of this initial asymmetry due to the interactions of the right-handed neutrino is larger than when calculated via the integrated equations. We also solve the full Boltzmann equations for soft leptogenesis, where t…

PhysicsleptogenesisParticle physicsmedia_common.quotation_subjectHigh Energy Physics::PhenomenologyFOS: Physical sciencesInverseFísicaAstronomy and AstrophysicsKinetic energyAsymmetrysymbols.namesakeHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Distribution functionneutrino theoryLeptogenesisBoltzmann constantsymbolsphysics of the early universeHigh Energy Physics::ExperimentNeutrinomedia_commonLepton
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Testing effects of Lorentz invariance violation in the propagation of astroparticles with the Pierre Auger Observatory

2021

The successful installation, commissioning, and operation of the Pierre Auger Observatory would not have been possible without the strong commitment and effort from the technical and administrative staff in Malargüe. We are very grateful to the following agencies and organizations for financial support: Argentina — Comisión Nacional de Energía Atómica; Agencia Nacional de Promoción Científica y Tecnológica (ANPCyT); Consejo Nacional de Investigaciones Científicas y Técnicas (CONICET); Gobierno de la Provincia de Mendoza; Municipalidad de Malargüe; NDM Holdings and Valle Las Leñas; in gratitude for their continuing cooperation over land access; Australia — the Australian Research Council; Be…

interaction [cosmic radiation]mass spectrum [cosmic radiation]dispersion relationAstronomyAstrophysics::High Energy Astrophysical Phenomenaenergy spectrumcosmic ray experimentFOS: Physical sciencesultra high energy cosmic rayscosmic radiation: interactioninvariance: Lorentz01 natural sciences530UHEultra high energy cosmic rayenergy: thresholdFundamental physics gravitational waves LISA Tests of general relativityCosmic ray experiments0103 physical sciencespropagationddc:530physics of the early universeHigh Energy PhysicsLorentz [invariance]010303 astronomy & astrophysicsphoton: fluxflux [photon]Lorentz [violation]High Energy Astrophysical Phenomena (astro-ph.HE)astro-ph.HEenergy: high010308 nuclear & particles physicscosmic radiation: mass spectrumcosmic ray experiments; ultra high energy cosmic rays; physics of the early universeSettore FIS/01 - Fisica SperimentaleAstronomy and AstrophysicsASTROFÍSICAUltra-high energy cosmic raysthreshold [energy]violation: LorentzAugerobservatoryelectromagnetickinematicsExperimental High Energy Physicshigh [energy]cosmic ray experimentsAstrophysics - High Energy Astrophysical PhenomenaPhysics of the early universe
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