Search results for "solar and atmospheric neutrinos"

showing 5 items of 5 documents

Updated determination of the solar neutrino fluxes from solar neutrino data

2016

Journal of High Energy Physics 2016.3 (2016): 132 reproduced by permission of Scuola Internazionale Superiore di Studi Avanzati (SISSA)

Normalization (statistics)Particle physicsNuclear and High Energy PhysicsSolar and atmospheric neutrinosSolar neutrinoAstrophysics::High Energy Astrophysical PhenomenaBayesian probabilityPosterior probabilitySolar neutrinosFOS: Physical sciences7. Clean energy01 natural sciencesHigh Energy Physics - Experimentsymbols.namesakeHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)Neutrins solars0103 physical sciencesAstrophysics::Solar and Stellar Astrophysics010306 general physicsNeutrino oscillationSolar and Stellar Astrophysics (astro-ph.SR)Physics010308 nuclear & particles physicsParticle physicsFísicaMarkov chain Monte CarloNeutrino physicsHigh Energy Physics - PhenomenologyDistribution functionAstrophysics - Solar and Stellar Astrophysics13. Climate actionPhysics::Space PhysicssymbolsAstrophysics::Earth and Planetary AstrophysicsNeutrinoFísica de partícules
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Searches for atmospheric long-lived particles

2020

Long-lived particles are predicted in extensions of the Standard Model that involve relatively light but very weakly interacting sectors. In this paper we consider the possibility that some of these particles are produced in atmospheric cosmic ray showers, and their decay intercepted by neutrino detectors such as IceCube or Super-Kamiokande. We present the methodology and evaluate the sensitivity of these searches in various scenarios, including extensions with heavy neutral leptons in models of massive neutrinos, models with an extra $U(1)$ gauge symmetry, and a combination of both in a $U(1)_{B-L}$ model. Our results are shown as a function of the production rate and the lifetime of the c…

Nuclear and High Energy PhysicsParticle physicsAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesCosmic ray01 natural sciences7. Clean energyHigh Energy Physics - ExperimentStandard ModelHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)0103 physical sciencesNeutrino Physicslcsh:Nuclear and particle physics. Atomic energy. Radioactivity010306 general physicsGauge symmetryPhysics010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyFunction (mathematics)High Energy Physics - PhenomenologyNeutrino detectorBeyond Standard Modellcsh:QC770-798High Energy Physics::ExperimentSolar and Atmospheric NeutrinosNeutrinoProduction rateLeptonJournal of High Energy Physics
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DARWIN: Towards the ultimate dark matter detector

2016

DARk matter WImp search with liquid xenoN (DARWIN) will be an experiment for the direct detection of dark matter using a multi-ton liquid xenon time projection chamber at its core. Its primary goal will be to explore the experimentally accessible parameter space for Weakly Interacting Massive Particles (WIMPs) in a wide mass-range, until neutrino interactions with the target become an irreducible background. The prompt scintillation light and the charge signals induced by particle interactions in the xenon will be observed by VUV sensitive, ultra-low background photosensors. Besides its excellent sensitivity to WIMPs above a mass of 5 GeV/c2, such a detector with its large mass, low-energy …

Physics - Instrumentation and DetectorsPhysics::Instrumentation and Detectorsdouble beta decay7. Clean energy01 natural sciencesHigh Energy Physics - ExperimentPhysics Particles & FieldsNeutrino detectorHigh Energy Physics - Experiment (hep-ex)XenonWIMPPHOTOMULTIPLIERAXIONSphysics.ins-detsolar and atmospheric neutrinosPhysicsDark matter detectorTime projection chamberdark matter detectorsPhysicsSolar and atmospheric neutrinoInstrumentation and Detectors (physics.ins-det)Nuclear & Particles PhysicsNeutrino detectorSOLAR NEUTRINOSGASPhysical SciencesNeutrinoAstrophysics - Instrumentation and Methods for AstrophysicsGRAN SASSODark matter detectors; Double beta decay; Neutrino detectors; Solar and atmospheric neutrinosDark matterchemistry.chemical_elementFOS: Physical sciencesAstronomy & AstrophysicsLIQUID-XENON DETECTOR0202 Atomic Molecular Nuclear Particle And Plasma PhysicsSettore FIS/05 - Astronomia e AstrofisicaSEARCH0103 physical sciencesIsotopes of xenonZEPLIN-III[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsAxionInstrumentation and Methods for Astrophysics (astro-ph.IM)Science & Technology010308 nuclear & particles physicshep-exAstronomyAstronomy and Astrophysics0201 Astronomical And Space ScienceschemistryHigh Energy Physics::ExperimentSCINTILLATIONneutrino detectorsastro-ph.IMJournal of Cosmology and Astroparticle Physics
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Sensitivity on earth core and mantle densities using atmospheric neutrinos

2009

11 pages, 11 figures.-- ISI article identifier:000267776100008 .-- ArXiv pre-print avaible at: http://arxiv.org/abs/0904.0796

PhysicsEarth and Planetary Astrophysics (astro-ph.EP)business.industrysolar and atmospheric neutrinosNeutrino telescopeFísicaFOS: Physical sciencesAstronomy and AstrophysicsGeophysicsMantle (geology)Physics::GeophysicsHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Neutrino detectorNondestructive testingUnderwaterNeutrinoAtmospheric neutrinobusinessAstrophysics - Earth and Planetary Astrophysicsneutrino detectors
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Improved global fit to Non-Standard neutrino Interactions using COHERENT energy and timing data

2020

We perform a global fit to neutrino oscillation and coherent neutrino-nucleus scattering data, using both timing and energy information from the COHERENT experiment. The results are used to set model-independent bounds on four-fermion effective operators inducing non-standard neutral-current neutrino interactions. We quantify the allowed ranges for their Wilson coefficients, as well as the status of the LMA-D solution, for a wide class of new physics models with arbitrary ratios between the strength of the operators involving up and down quarks. Our results are presented for the COHERENT experiment alone, as well as in combination with the global data from oscillation experiments. We also q…

QuarkNuclear and High Energy PhysicsParticle physicsPhysics beyond the Standard ModelFOS: Physical sciences7. Clean energy01 natural sciencesHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)0103 physical scienceslcsh:Nuclear and particle physics. Atomic energy. RadioactivityNeutrino Physics010306 general physicsNeutrino oscillationPhysics010308 nuclear & particles physicsScatteringOscillationForm factor (quantum field theory)High Energy Physics - PhenomenologyBeyond Standard Modellcsh:QC770-798Solar and Atmospheric NeutrinosNeutrinoEnergy (signal processing)
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