Search results for " early Universe"

showing 6 items of 16 documents

Early Universe Higgs dynamics in the presence of the Higgs-inflaton and non-minimal Higgs-gravity couplings

2017

Apparent metastability of the electroweak vacuum poses a number of cosmological questions. These concern evolution of the Higgs field to the current vacuum, and its stability during and after inflation. Higgs-inflaton and non-minimal Higgs-gravity interactions can make a crucial impact on these considerations potentially solving the problems. In this work, we allow for these couplings to be present simultaneously and study their interplay. We find that different combinations of the Higgs-inflaton and non-minimal Higgs-gravity couplings induce effective Higgs mass during and after inflation. This crucially affects the Higgs stability considerations during preheating. In particular, a wide ra…

Particle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Physics beyond the Standard Modelmedia_common.quotation_subjectHigh Energy Physics::LatticeFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciences114 Physical sciencesGeneral Relativity and Quantum CosmologyHigh Energy Physics - Phenomenology (hep-ph)Metastability0103 physical sciencesphysics of the early universeinflationparticle physicscosmology connectionELECTROWEAK VACUUM010306 general physicscosmology of theories beyond the SMmedia_commonInflation (cosmology)PhysicsSTABILITY010308 nuclear & particles physicsElectroweak interactionHigh Energy Physics::PhenomenologyAstronomy and AstrophysicsBOSONInflaton115 Astronomy Space scienceUniverseHigh Energy Physics - PhenomenologyHiggs fieldHiggs bosonHigh Energy Physics::ExperimentAstrophysics - Cosmology and Nongalactic Astrophysics
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New cosmological bounds on hot relics: Axions $\&$ Neutrinos

2020

Axions, if realized in nature, can be copiously produced in the early universe via thermal processes, contributing to the mass-energy density of thermal hot relics. In light of the most recent cosmological observations, we analyze two different thermal processes within a realistic mixed hot-dark-matter scenario which includes also massive neutrinos. Considering the axion-gluon thermalization channel we derive our most constraining bounds on the hot relic masses $m_a < 7.46$ eV and $\sum m_��< 0.114$ eV both at 95 per cent CL; while studying the axion-pion scattering, without assuming any specific model for the axion-pion interactions and remaining in the range of validity of the chira…

Particle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Physics::Instrumentation and Detectorsmedia_common.quotation_subjectDark matterCosmic background radiationFOS: Physical sciencescosmic background radiation; cosmological parameters; dark matter; early Universe; cosmology: observations;7. Clean energy01 natural sciencesHigh Energy Physics - Phenomenology (hep-ph)Double beta decay0103 physical sciences010306 general physicsAxionmedia_commonPhysics010308 nuclear & particles physicsHot dark matterHigh Energy Physics::PhenomenologyAstronomy and AstrophysicsUniverseHigh Energy Physics - Phenomenology13. Climate actionSpace and Planetary ScienceStrong CP problemNeutrinoAstrophysics - Cosmology and Nongalactic Astrophysics
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Observational signatures of Higgs inflation

2016

We investigate the dependency of Higgs inflation on the non-renormalisable matching between the low energy Standard Model limit and the inflationary regime at high energies. We show that for the top mass range $m_t \gtrsim 171.8$ GeV the scenario robustly predicts the spectral index $n_s \simeq 0.97$ and the tensor-to-scalar ratio $r\simeq 0.003$. The matching is however non-trivial, even the best-fit values $m_h=125.09$ GeV and $m_t=173.21$ GeV require a jump $\delta \lambda \sim 0.01$ in the Higgs coupling below the inflationary scale. For $m_t\lesssim 171.8$ GeV, the matching may generate a feature in the inflationary potential. In this case the predicted values of $n_s$ and $r$ vary but…

Particle physicsMatching (statistics)Cosmology and Nongalactic Astrophysics (astro-ph.CO)STANDARD MODELFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic Astrophysics114 Physical sciences01 natural sciencesStandard ModelHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesphysics of the early universeinflationELECTROWEAK VACUUM010306 general physicscosmology of theories beyond the SMBosonInflation (cosmology)PhysicsSpectral index010308 nuclear & particles physicsINDUCED GRAVITY INFLATIONHigh Energy Physics::PhenomenologySpectral densityBOSONAstronomy and Astrophysics115 Astronomy Space scienceHigh Energy Physics - Phenomenologyparticle physics - cosmology connectionJumpHiggs bosonHigh Energy Physics::ExperimentAstrophysics - Cosmology and Nongalactic Astrophysics
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Reexamination of the Power Spectrum in De Sitter Inflation

2008

4 pages, 1 table.-- PACS nrs.: 98.80.Cq, 04.62.+v.-- PMID: 18999735 [PubMed].

PhysicsQuantum field theory in curved spacetime010308 nuclear & particles physicsVacuum stateGeneral Physics and AstronomySpectral densityAstrophysics::Cosmology and Extragalactic AstrophysicsInflaton01 natural sciences[PACS] Quantum fields in curved spacetimeMassless particleGeneral Relativity and Quantum CosmologyAmplitude[PACS] Particle-theory and field-theory models of the early UniverseDe Sitter universeQuantum mechanicsQuantum electrodynamics0103 physical sciences010306 general physicsQuantum fluctuationPhysical Review Letters
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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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