Search results for "High Energy Physics::Phenomenology"

showing 10 items of 5791 documents

Radiative neutrino masses: A window to new physics

2021

Currently, the Standard Model of particle physics (SM) is the best theory we have to describe particles and their interactions. However, there is evidence of physics beyond it, which motivates us to seek for a more complete theory. Neutrino oscillations constitute the first experimental confirmation of new physics, as they require a new piece that is absent in the SM, non-zero neutrino masses. Neutrino masses brought new theoretical challenges, for instance questions as how these masses are generated or why are they so small compared to other masses, are still under investigation. In this thesis, we aim to study radiative neutrino mass models, a class of models where small neutrino masses a…

bsm physicsHigh Energy Physics::Phenomenology:FÍSICA::Física de altas energías::Física teórica altas energías [UNESCO]neutrinosphenomenologyUNESCO::FÍSICA::Física de altas energías::Física teórica altas energías
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Single electron yields from semileptonic charm and bottom hadron decays in Au+Au collisions at √sNN = 200 GeV

2016

The PHENIX Collaboration at the Relativistic Heavy Ion Collider has measured open heavy flavor production in minimum bias Au + Au collisions at √sNN = 200 GeV via the yields of electrons from semileptonic decays of charm and bottom hadrons. Previous heavy flavor electron measurements indicated substantial modification in the momentum distribution of the parent heavy quarks owing to the quark-gluon plasma created in these collisions. For the first time, using the PHENIX silicon vertex detector to measure precision displaced tracking, the relative contributions from charm and bottom hadrons to these electrons as a function of transverse momentum are measured in Au + Au collisions. We compare …

charm hadronsHigh Energy Physics::PhenomenologyAu+Au collisionskvarkki-gluoniplasmaHigh Energy Physics::ExperimentNuclear Experimentelektronitbottom hadrons
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LC-Polymers with Axial Chirality

1991

Abstract Liquid crystalline polymers with axial chirality are prepared. These polymers are chiral, not due to a single asymmetric carbon atom, but due to a larger molecular fragment, which is chiral as a whole. They exhibit cholesteric and chiral smectic C* phases. Dielectric spectroscopy proves strong ferroelectric properties in the chiral smectic C* phases of these polymers.

chemistry.chemical_classificationQuantitative Biology::BiomoleculesMaterials scienceStereochemistryLiquid crystallineHigh Energy Physics::LatticeHigh Energy Physics::PhenomenologyPolymerFerroelectricityDielectric spectroscopyCondensed Matter::Soft Condensed MatterCondensed Matter::Materials ScienceCrystallographychemistryAsymmetric carbonAxial chiralityChirality (chemistry)Molecular Crystals and Liquid Crystals
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The effective cross section for double parton scattering within a holographic AdS/QCD approach

2017

A first attempt to apply the AdS/QCD framework for a bottom-up approach to the evaluation of the effective cross section for double parton scattering in proton-proton collisions is presented. The main goal is the analytic evaluation of the dependence of the effective cross section on the longitudinal momenta of the involved partons, obtained within the holographic Soft-Wall model. If measured in high-energy processes at hadron colliders, this momentum dependence could open a new window on 2-parton correlations in a proton.

correlation: two-particleNuclear and High Energy PhysicsParticle physicsp p: scatteringNuclear TheoryProton[PHYS.NUCL]Physics [physics]/Nuclear Theory [nucl-th]Nuclear TheoryHadronFOS: Physical sciencesParton01 natural sciences[ PHYS.HTHE ] Physics [physics]/High Energy Physics - Theory [hep-th]quantum chromodynamics: holographyNuclear Theory (nucl-th)Nuclear physicsMomentumCross section (physics)12.38.AwHigh Energy Physics - Phenomenology (hep-ph)parton: multiple scattering0103 physical sciencesparton: correlation010306 general physicsNuclear Experimentparton: interaction[ PHYS.NUCL ] Physics [physics]/Nuclear Theory [nucl-th]Quantum chromodynamicsPhysicsAdS/CFT correspondence010308 nuclear & particles physicsScattering[PHYS.HTHE]Physics [physics]/High Energy Physics - Theory [hep-th]High Energy Physics::Phenomenology12.39.Kilcsh:QC1-999High Energy Physics - PhenomenologyAdS/CFT correspondence[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]14.20.DhPhysics::Accelerator Physics[ PHYS.HPHE ] Physics [physics]/High Energy Physics - Phenomenology [hep-ph]High Energy Physics::Experimentlcsh:Physics
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A strong electroweak phase transition from the inflaton field

2016

We study a singlet scalar extension of the Standard Model. The singlet scalar is coupled non-minimally to gravity and assumed to drive inflation, and also couple sufficiently strongly with the SM Higgs field in order to provide for a strong first order electroweak phase transition. Requiring the model to describe inflation successfully, be compatible with the LHC data, and yield a strong first order electroweak phase transition, we identify the regions of the parameter space where the model is viable. We also include a singlet fermion with scalar coupling to the singlet scalar to probe the sensitivity of the constraints on additional degrees of freedom and their couplings in the singlet sec…

cosmological inflationParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Physics beyond the Standard ModelScalar (mathematics)Degrees of freedom (physics and chemistry)FOS: Physical sciences01 natural sciences7. Clean energyStandard ModelGeneral Relativity and Quantum CosmologyHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciences010306 general physicsPhysicsInflation (cosmology)010308 nuclear & particles physicsElectroweak interactionHigh Energy Physics::PhenomenologyAstronomy and AstrophysicsInflatonextensions of the Standard ModelHiggs fieldHigh Energy Physics - Phenomenologyelectroweak phase transitionAstrophysics - Cosmology and Nongalactic Astrophysics
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Probing the origin of ultra-high-energy cosmic rays with neutrinos in the EeV energy range using the Pierre Auger Observatory

2019

Neutrinos with energies above 1017 eV are detectable with the Surface Detector Array of the Pierre Auger Observatory. The identification is efficiently performed for neutrinos of all flavors interacting in the atmosphere at large zenith angles, as well as for Earth-skimming τ neutrinos with nearly tangential trajectories relative to the Earth. No neutrino candidates were found in ∼ 14.7 years of data taken up to 31 August 2018. This leads to restrictive upper bounds on their flux. The 90% C.L. single-flavor limit to the diffuse flux of ultra-high-energy neutrinos with an Eν -2 spectrum in the energy range 1.0 × 1017 eV -2.5 × 1019 eV is E2 dNν/dEν < 4.4 × 10-9 GeV cm-2 s-1 sr-1, placing str…

cosmological neutrinosAstronomyFluxAstrophysics01 natural sciences7. Clean energycosmic ray experiments; cosmological neutrinos; neutrino astronomy; ultra high energy cosmic rayssurface [detector]Ultra-high-energy cosmic rayPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)cosmological neutrinoSettore FIS/01 - Fisica SperimentaleDETETORESneutrino: UHEUHE [neutrino]Augerobservatorytrajectoryneutrino: flavorProduction (computer science)NeutrinoAstrophysics - High Energy Astrophysical PhenomenaAstrophysics::High Energy Astrophysical PhenomenaUHE [cosmic radiation]FOS: Physical sciencescosmic ray experimentCosmic rayultra high energy cosmic raysneutrino: productionneutrino astronomyproduction [neutrino]TheoryofComputation_ANALYSISOFALGORITHMSANDPROBLEMCOMPLEXITY0103 physical sciencesddc:530model [neutrino]High Energy Physicscosmic radiation: UHEZenithAstrophysiqueneutrino: modelPierre Auger ObservatorySPECTRUM010308 nuclear & particles physicsdetector: surfaceHigh Energy Physics::Phenomenologyflavor [neutrino]Astronomy and AstrophysicsAstronomiefluxExperimental High Energy PhysicsatmosphereHigh Energy Physics::Experimentcosmic ray experiments[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Energy (signal processing)
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Measurement of the cosmic ray proton spectrum from 40 GeV to 100 TeV with the DAMPE satellite

2019

DAMPE satellite has directly measured the cosmic ray proton spectrum from 40 GeV to 100 TeV and revealed a new feature at about 13.6 TeV.

dark matter cosmic rays spaceProtonMilky WayAstrophysics::High Energy Astrophysical PhenomenaDark matterFOS: Physical sciencesCosmic rayAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsKinetic energy01 natural sciences0103 physical sciences010306 general physicsNuclear ExperimentResearch ArticlesPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Spectral indexMultidisciplinary010308 nuclear & particles physicsPhysicsHigh Energy Physics::PhenomenologySettore FIS/01 - Fisica SperimentaleSciAdv r-articlesPhysics::Accelerator PhysicsHigh Energy Physics::ExperimentAstrophysics - High Energy Astrophysical PhenomenaResearch Article
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Measurements of the top quark branching ratios into channels with leptons and quarks with the ATLAS detector

2015

Measurements of the branching ratios of top quark decays into leptons and jets using events with t[bar over t] (top antitop) pairs are reported. Events were recorded with the ATLAS detector at the LHC in pp collisions at a center-of-mass energy of 7 TeV. The collected data sample corresponds to an integrated luminosity of 4.6  fb[superscript −1]. The measured top quark branching ratios agree with the Standard Model predictions within the measurement uncertainties of a few percent.

decay [top]Top quarkБольшой адронный коллайдерAtlas detectormeasured [cross section]верхние кваркиpair production [top]multiplicity [lepton]High Energy Physics - ExperimentScatteringSubatomär fysikHigh Energy Physics - Experiment (hep-ex)лептоныSubatomic PhysicsJets[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]scattering [p p]CollisionsSUPERSYMMETRYGeneralLiterature_REFERENCE(e.g.dictionariesencyclopediasglossaries)протон-протонные столкновенияQCPhysicsLarge Hadron ColliderSettore FIS/01 - Fisica SperimentaleSupersymmetryATLASTop Quark Branching RatiosCERN LHC CollProton–proton collisions7000 GeV-cmsPAIR CROSS-SECTIONcolliding beams [p p]Particle Physics - Experiment((n)jet lepton) [final state]top quark branching ratios; leptons; quarks; ATLAS detectorQuarkParticle physicsNuclear and High Energy PhysicsCiências Naturais::Ciências Físicas530 Physics:Ciências Físicas [Ciências Naturais]FOS: Physical sciencesPAIR CROSS-SECTION; PARTON DISTRIBUTIONS; PP COLLISIONS; SUPERSYMMETRY; TEVBranching (polymer chemistry)Accelerator Physics and Instrumentation530Nuclear physicsddc:530Science & TechnologyPP COLLISIONSScatteringHigh Energy Physics::PhenomenologyFísicaAcceleratorfysik och instrumenteringLeptons and Quarksbranching ratio: measured [top]PARTON DISTRIBUTIONSExperimental High Energy PhysicsTEVp p --> 2top anythingHigh Energy Physics::ExperimentATLAS детекторhadronic decay [tau]Leptonexperimental results
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Search for heavy neutrinos with the T2K near detector ND280

2019

This paper reports on the search for heavy neutrinos with masses in the range 140<MN<493  MeV/c2 using the off-axis near detector ND280 of the T2K experiment. These particles can be produced from kaon decays in the standard neutrino beam and then subsequently decay in ND280. The decay modes under consideration are N→ℓ±απ∓ and N→ℓ+αℓ−β(−)ν(α,β=e,μ). A search for such events has been made using the Time Projection Chambers of ND280, where the background has been reduced to less than two events in the current dataset in all channels. No excess has been observed in the signal region. A combined Bayesian statistical approach has been applied to extract upper limits on the mixing elements of heav…

decay modes [neutrino]GENERAL-THEORYmixing [neutrino]Physics::Instrumentation and Detectorsneutrino: heavy: search forKAMIOKANDE01 natural sciencesHigh Energy Physics - ExperimentPhysics Particles & FieldsHigh Energy Physics - Experiment (hep-ex)LIMITSsecondary beam [neutrino/mu]neutrino: decay modes[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Particle Physics Experimentsneutrino: massmedia_commonPhysicsVMSMJ-PARC LabPhysicsstatistical analysis: BayesianK: decayheavy neutrinos T2K Experiment Time Projection Chambersmass dependenceGeneral theoryT2K ExperimentTime Projection ChambersPhysical SciencesChristian ministrydata analysis methodFOS: Physical sciencesLibrary scienceheavy: search for [neutrino]Astronomy & AstrophysicsBayesian [statistical analysis]530near detector0103 physical sciencesDARK-MATTERmedia_common.cataloged_instanceddc:530Early careerEuropean unionS077A00010306 general physicsS077A01heavy neutrinosScience & Technology010308 nuclear & particles physicsbackgroundhep-exHigh Energy Physics::PhenomenologyFísicaneutrino/mu: secondary beamtime projection chamberdecay [K]mass [neutrino]Hypothetical particle physics models Particle phenomenaHigh Energy Physics::Experimentneutrino: mixingstatisticalexperimental resultsPhysical Review D
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First real–time detection of solar pp neutrinos by Borexino

2014

International audience; Solar neutrinos have been pivotal to the discovery of neutrino flavour oscillations and are a unique tool to probe the reactions that keep the Sun shine. Although most of solar neutrino components have been directly measured, the neutrinos emitted by the keystone pp reaction, in which two protons fuse to make a deuteron, have so far eluded direct detection. The Borexino experiment, an ultra-pure liquid scintillator detector running at the Laboratori Nazionali del Gran Sasso in Italy, has now filled the gap, providing the first direct real time measurement of pp neutrinos and of the solar neutrino luminosity.

deuteronParticle physicsneutrino: solarPhysics::Instrumentation and DetectorsQC1-999Solar neutrinoAstrophysics::High Energy Astrophysical Phenomenascintillation counter: liquidgap7. Clean energy01 natural sciencesNuclear physicsPhysics and Astronomy (all)0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]ddc:530flavor: oscillation010306 general physicsNuclear ExperimentBorexinoPhysicsICARUSp p: fusion010308 nuclear & particles physicsPhysicsHigh Energy Physics::Phenomenologytalk: Noto 2014/09/30Solar neutrino problemGran SassoNeutrino detectorneutrino: flavorMeasurements of neutrino speedCOUNTING TEST FACILITYHigh Energy Physics::Experimentdirect detectionBorexinoneutrino: oscillationNeutrino astronomyNeutrinoexperimental resultsneutrino: luminosity
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