Search results for "Particle physics"

showing 10 items of 6826 documents

Neutrino cosmology and Planck

2014

Relic neutrinos play an important role in the evolution of the Universe, modifying some of the cosmological observables. We summarize the main aspects of cosmological neutrinos and describe how the precision of present cosmological data can be used to learn about neutrino properties. In particular, we discuss how cosmology provides information on the absolute scale of neutrino masses, complementary to beta decay and neutrinoless double-beta decay experiments. We explain why the combination of Planck temperature data with measurements of the baryon acoustic oscillation angular scale provides a strong bound on the sum of neutrino masses, 0.23 eV at the 95% confidence level, while the lensing …

Particle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)General Physics and AstronomyFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic AstrophysicsCosmologydark matterHigh Energy Physics - Experimentsymbols.namesakeHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)PlanckAbsolute scaleParticle Physics - PhenomenologyPhysicsOscillationneutrino massesHigh Energy Physics::PhenomenologyFísicaObservablePlanck temperatureBaryonHigh Energy Physics - Phenomenology13. Climate action[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]symbolsHigh Energy Physics::ExperimentNeutrinocosmologyAstrophysics - Cosmology and Nongalactic Astrophysics
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Evidence for High-Energy Extraterrestrial Neutrinos at the IceCube Detector

2013

We report on results of an all-sky search for high-energy neutrino events interacting within the IceCube neutrino detector conducted between May 2010 and May 2012. The search follows up on the previous detection of two PeV neutrino events, with improved sensitivity and extended energy coverage down to approximately 30 TeV. Twenty-six additional events were observed, substantially more than expected from atmospheric backgrounds. Combined, both searches reject a purely atmospheric origin for the twenty-eight events at the $4\sigma$ level. These twenty-eight events, which include the highest energy neutrinos ever observed, have flavors, directions, and energies inconsistent with those expected…

Particle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)General Science & TechnologyPhysics::Instrumentation and DetectorsSolar neutrinoAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesddc:500.2AstrophysicsIceCube Collaboration01 natural sciences7. Clean energyHigh Energy Physics - ExperimentIceCube Neutrino ObservatoryIceCubeHigh Energy Physics - Experiment (hep-ex)MD Multidisciplinary0103 physical sciences010303 astronomy & astrophysicsastro-ph.HEPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Multidisciplinaryhep-ex010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyneutrinosSolar neutrino problemKM3NeTNeutrino detector13. Climate actionastro-ph.COMeasurements of neutrino speedHigh Energy Physics::Experimentddc:500NeutrinoNeutrino astronomyAstrophysics - High Energy Astrophysical PhenomenaphysicsAstrophysics - Cosmology and Nongalactic AstrophysicsScience
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Lattice Calculation of the Decay of Primordial Higgs Condensate

2015

We study the resonant decay of the primordial Standard Model Higgs condensate after inflation into $SU(2)$ gauge bosons on the lattice. We find that the non-Abelian interactions between the gauge bosons quickly extend the momentum distribution towards high values, efficiently destroying the condensate after the onset of backreaction. For the inflationary scale $H = 10^8$ GeV, we find that 90% of the Higgs condensate has decayed after $n \sim 10$ oscillation cycles. This differs significantly from the Abelian case where, given the same coupling strengths, most of the condensate would persist after the resonance.

Particle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)High Energy Physics::LatticeLattice field theoryFOS: Physical sciences01 natural sciencesHigh Energy Physics - Phenomenology (hep-ph)High Energy Physics - LatticeLattice (order)0103 physical sciences010306 general physicsSpecial unitary groupBosonCoupling constantPhysicsCondensed Matter::Quantum GasesGauge boson010308 nuclear & particles physicsHigh Energy Physics - Lattice (hep-lat)High Energy Physics::PhenomenologyAstronomy and AstrophysicsHigh Energy Physics - PhenomenologyHiggs bosonBack-reactionHigh Energy Physics::ExperimentAstrophysics - Cosmology and Nongalactic Astrophysics
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Postinflationary vacuum instability and Higgs-inflaton couplings

2016

The Higgs-inflaton coupling plays an important role in the Higgs field dynamics in the early Universe. Even a tiny coupling generated at loop level can have a dramatic effect on the fate of the electroweak vacuum. Such Higgs-inflaton interaction is present both at the trilinear and quartic levels in realistic reheating models. In this work, we examine the Higgs dynamics during the preheating epoch, focusing on the effects of the parametric and tachyonic resonances. We use lattice simulations and other numerical tools in our studies. We find that the resonances can induce large fluctuations of the Higgs field which destabilize the electroweak vacuum. Our considerations thus provide an upper …

Particle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)High Energy Physics::LatticePhysics beyond the Standard ModeleducationFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic Astrophysics114 Physical sciences01 natural sciencesUpper and lower boundsInstabilityGeneral Relativity and Quantum CosmologyHigh Energy Physics - Phenomenology (hep-ph)inflation Higgs0103 physical sciences010306 general physicsPhysicsCoupling010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyElectroweak interactionAstronomy and AstrophysicsInflatonHigh Energy Physics - PhenomenologyHiggs fieldHiggs bosonHigh Energy Physics::ExperimentAstrophysics - Cosmology and Nongalactic AstrophysicsJournal of Cosmology and Astroparticle Physics
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Baryogenesis and dark matter from B mesons

2019

We present a new mechanism of Baryogenesis and dark matter production in which both the dark matter relic abundance and the baryon asymmetry arise from neutral $B$ meson oscillations and subsequent decays. This set-up is testable at hadron colliders and $B$-factories. In the early Universe, decays of a long lived particle produce $B$ mesons and anti-mesons out of thermal equilibrium. These mesons/anti-mesons then undergo CP violating oscillations before quickly decaying into visible and dark sector particles. Dark matter will be charged under Baryon number so that the visible sector baryon asymmetry is produced without violating the total baryon number of the Universe. The produced baryon a…

Particle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)MesonProton decayDark matterHadronNuclear TheoryFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciences7. Clean energyHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)Baryon asymmetry0103 physical sciences010306 general physicsNuclear ExperimentPhysics010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyBaryonBaryogenesisHigh Energy Physics - PhenomenologyHigh Energy Physics::ExperimentBaryon numberAstrophysics - Cosmology and Nongalactic Astrophysics
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Higgs-like spectator field as the origin of structure

2021

We show that the observed primordial perturbations can be entirely sourced by a light spectator scalar field with a quartic potential, akin to the Higgs boson, provided that the field is sufficiently displaced from vacuum during inflation. The framework relies on the indirect modulation of reheating, which is implemented without any direct coupling between the spectator field and the inflaton and does not require non-renormalisable interactions. The scenario gives rise to local non-Gaussianity with $f_{\rm NL}\simeq 5$ as the typical signal. As an example model where the indirect modulation mechanism is realised for the Higgs boson, we study the Standard Model extended with right-handed neu…

Particle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Physics and Astronomy (miscellaneous)Field (physics)FOS: Physical sciencesQC770-798Astrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicskosmologia01 natural sciences7. Clean energy114 Physical sciencesPhysics Particles & FieldsStandard ModelHigh Energy Physics - Phenomenology (hep-ph)Nuclear and particle physics. Atomic energy. RadioactivityQuartic function0103 physical sciences0206 Quantum Physics010303 astronomy & astrophysicsEngineering (miscellaneous)kosminen inflaatioInflation (cosmology)PhysicsScience & Technology010308 nuclear & particles physicsPhysicsHiggsin bosoniHigh Energy Physics::Phenomenologyhiukkasfysiikan standardimallihep-phInflatonPERTURBATIONSNuclear & Particles PhysicsQB460-466High Energy Physics - Phenomenologykosminen taustasäteilyPhysical Sciences0202 Atomic Molecular Nuclear Particle and Plasma Physicsastro-ph.COHiggs bosonNeutrinoScalar fieldAstrophysics - Cosmology and Nongalactic AstrophysicsThe European Physical Journal C
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Flavor versus mass eigenstates in neutrino asymmetries: implications for cosmology

2017

We show that, if they exist, lepton number asymmetries ($L_\alpha$) of neutrino flavors should be distinguished from the ones ($L_i$) of mass eigenstates, since Big Bang Nucleosynthesis (BBN) bounds on the flavor eigenstates cannot be directly applied to the mass eigenstates. Similarly, Cosmic Microwave Background (CMB) constraints on mass eigenstates do not directly constrain flavor asymmetries. Due to the difference of mass and flavor eigenstates, the cosmological constraint on the asymmetries of neutrino flavors can be much stronger than conventional expectation, but not uniquely determined unless at least the asymmetry of the heaviest neutrino is well constrained. Cosmological constrain…

Particle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Physics and Astronomy (miscellaneous)media_common.quotation_subjectHigh Energy Physics::LatticeCosmic microwave backgroundCosmic background radiationFOS: Physical scienceslcsh:AstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesAsymmetryCosmologyHigh Energy Physics - Phenomenology (hep-ph)Big Bang nucleosynthesislcsh:QB460-4660103 physical scienceslcsh:Nuclear and particle physics. Atomic energy. Radioactivity010306 general physicsEngineering (miscellaneous)Eigenvalues and eigenvectorsmedia_commonPhysics010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyLepton numberHigh Energy Physics - Phenomenologylcsh:QC770-798High Energy Physics::ExperimentNeutrinoAstrophysics - Cosmology and Nongalactic Astrophysics
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Toward (finally!) ruling out Z and Higgs mediated dark matter models

2016

In recent years, direct detection, indirect detection, and collider experiments have placed increasingly stringent constraints on particle dark matter, exploring much of the parameter space associated with the WIMP paradigm. In this paper, we focus on the subset of WIMP models in which the dark matter annihilates in the early universe through couplings to either the Standard Model $Z$ or the Standard Model Higgs boson. Considering fermionic, scalar, and vector dark matter candidates within a model-independent context, we find that the overwhelming majority of these dark matter candidates are already ruled out by existing experiments. In the case of $Z$ mediated dark matter, the only scenari…

Particle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Physics beyond the Standard Modelmedia_common.quotation_subjectDark matterScalar (mathematics)FOS: Physical sciencesAstrophysics::Cosmology and Extragalactic Astrophysics7. Clean energy01 natural sciencesStandard ModelHigh Energy Physics - Phenomenology (hep-ph)WIMP0103 physical sciences010306 general physicsmedia_commonPhysics010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyAstronomy and AstrophysicsUniversePseudoscalarHigh Energy Physics - PhenomenologyHiggs bosonHigh Energy Physics::ExperimentAstrophysics - Cosmology and Nongalactic AstrophysicsJournal of Cosmology and Astroparticle Physics
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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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Limits on a muon flux from neutralino annihilations in the sun with the IceCube 22-string detector.

2009

A search for muon neutrinos from neutralino annihilations in the Sun has been performed with the IceCube 22-string neutrino detector using data collected in 104.3 days of live-time in 2007. No excess over the expected atmospheric background has been observed. Upper limits have been obtained on the annihilation rate of captured neutralinos in the Sun and converted to limits on the WIMP-proton cross-sections for WIMP masses in the range 250 - 5000 GeV. These results are the most stringent limits to date on neutralino annihilation in the Sun.

Particle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Physics::Instrumentation and DetectorsDark matterFOS: Physical sciencesGeneral Physics and Astronomy01 natural sciences7. Clean energyNuclear physicsWIMP0103 physical sciencesddc:550010306 general physicsNeutrino oscillationNeutrino TelescopeHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsMuonAnnihilation010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyNeutrino detector13. Climate actionNeutralinoHigh Energy Physics::ExperimentNeutrinoAstrophysics - High Energy Astrophysical PhenomenaAstrophysics - Cosmology and Nongalactic AstrophysicsPhysical review letters
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