Search results for "Measurement"

showing 10 items of 2918 documents

Atmospheric neutrinos in ice and measurement of neutrino oscillation parameters

2010

The main goal of the IceCube Deep Core array is to search for neutrinos of astrophysical origins. Atmospheric neutrinos are commonly considered as a background for these searches. We show that the very high statistics atmospheric neutrino data can be used to obtain precise measurements of the main oscillation parameters.

AstrofísicaNuclear and High Energy PhysicsParticle physicsPhysics::Instrumentation and DetectorsSolar neutrinoAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysics01 natural sciences7. Clean energyHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)0103 physical sciences010306 general physicsNeutrino oscillationPhysics010308 nuclear & particles physicsHigh Energy Physics::PhenomenologySolar neutrino problemCosmic neutrino backgroundHigh Energy Physics - PhenomenologyNeutrino detector13. Climate actionMeasurements of neutrino speedHigh Energy Physics::ExperimentNeutrinoNeutrino astronomy
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Super-NOvA: a long-baseline neutrino experiment with two off-axis detectors

2005

Establishing the neutrino mass hierarchy is one of the fundamental questions that will have to be addressed in the next future. Its determination could be obtained with long-baseline experiments but typically suffers from degeneracies with other neutrino parameters. We consider here the NOvA experiment configuration and propose to place a second off-axis detector, with a shorter baseline, such that, by exploiting matter effects, the type of neutrino mass hierarchy could be determined with only the neutrino run. We show that the determination of this parameter is free of degeneracies, provided the ratio L/E, where L the baseline and E is the neutrino energy, is the same for both detectors.

AstrofísicaPhysicsNuclear and High Energy PhysicsParticle physicsPhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaHigh Energy Physics::PhenomenologyFOS: Physical sciencesSolar neutrino problemType (model theory)Particle identificationNuclear physicsHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Neutrino detectorMeasurements of neutrino speedInvariant massHigh Energy Physics::ExperimentNeutrinoNeutrino oscillationParticle Physics - Phenomenology
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Disentangling neutrino-nucleon cross section and high energy neutrino flux with akm3neutrino telescope

2007

The energy--zenith angular event distribution in a neutrino telescope provides a unique tool to determine at the same time the neutrino-nucleon cross section at extreme kinematical regions, and the high energy neutrino flux. By using a simple parametrization for fluxes and cross sections, we present a sensitivity analysis for the case of a km^3 neutrino telescope. In particular, we consider the specific case of an under-water Mediterranean telescope placed at the NEMO site, although most of our results also apply to an under-ice detector such as IceCube. We determine the sensitivity to departures from standard values of the cross sections above 1 PeV which can be probed independently from a…

AstrofísicaPhysicsNuclear and High Energy PhysicsParticle physicsPhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaSolar neutrinoAstrophysics (astro-ph)Astrophysics::Instrumentation and Methods for AstrophysicsFOS: Physical sciencesCosmic raySolar neutrino problemAstrophysicslaw.inventionTelescopeHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Neutrino detectorlawMeasurements of neutrino speedHigh Energy Physics::ExperimentNeutrinoNeutrino oscillationPhysical Review D
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Five years of searches for point sources of astrophysical neutrinos with the AMANDA-II neutrino telescope

2007

We report the results of a five-year survey of the northern sky to search for point sources of high energy neutrinos. The search was performed on the data collected with the AMANDA-II neutrino telescope in the years 2000 to 2004, with a live-time of 1001 days. The sample of selected events consists of 4282 upward going muon tracks with high reconstruction quality and an energy larger than about 100 GeV. We found no indication of point sources of neutrinos and set 90% confidence level flux upper limits for an all-sky search and also for a catalog of 32 selected sources. For the all-sky search, our average (over declination and right ascension) experimentally observed upper limit \Phi^{0}=(E/…

Astroparticle physicsPhysicsNuclear and High Energy PhysicsMuonAstrophysics::High Energy Astrophysical Phenomenamedia_common.quotation_subjectSolar neutrinoAstrophysics (astro-ph)High Energy Physics::PhenomenologyAstrophysics::Instrumentation and Methods for AstrophysicsFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsSolar neutrino problemAstrophysicsSkyAstronomiaMeasurements of neutrino speedHigh Energy Physics::Experimentddc:530NeutrinoNeutrino astronomymedia_common
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The frontiers of the virtual photons program at MAMI

2012

The most recent results and the future physics program of the high precision electron-scattering experiment at MAMI are briefly outlined. The A1 high-resolution spectrometers facility allows for a unique quality of virtual photon experiments. High precision form factor measurements, few-baryon systems highresolution structure studies and the innovative way in the search of dark photons illustrate the interplay between such diverse fields as precision atomic physics, nuclear astrophysics and astroparticle physics, where hadron physics plays a central and connecting role.

Astroparticle physicsPhysicsParticle physicsPhotonSpectrometerPhysicsQC1-999Form factor (quantum field theory)Virtual particleEngineering physicsHadron physicsNuclear astrophysicsvirtual photon; form factor measurements; dark photon; precision spectroscopy of light hypernucleiNuclear Experiment
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"Table 29" of "Properties of hadronic Z decays and test of QCD generators"

1992

N-jet production rates (in percent) corrected for charged and neutral particles.

Astrophysics::High Energy Astrophysical PhenomenaE+ E- --> HADRONSE+ E- --> Z0Integrated Cross Section91.2Jet Productionrespiratory systemCross Sectionequipment and suppliesSIGcomplex mixturesDijet ProductionE+ E- ScatteringExclusiveHigh Energy Physics::ExperimentE+ E- --> 2JETR measurementhuman activitiescirculatory and respiratory physiology
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"Table 25" of "Properties of hadronic Z decays and test of QCD generators"

1992

N-jet production rates (in percent) corrected for charged particles only.

Astrophysics::High Energy Astrophysical PhenomenaE+ E- --> HADRONSE+ E- --> Z0Integrated Cross Section91.2Jet Productionrespiratory systemCross Sectionequipment and suppliesSIGcomplex mixturesDijet ProductionE+ E- ScatteringExclusiveHigh Energy Physics::ExperimentE+ E- --> 2JETR measurementhuman activitiescirculatory and respiratory physiology
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"Table 26" of "Properties of hadronic Z decays and test of QCD generators"

1992

N-jet production rates (in percent) corrected for charged particles only.

Astrophysics::High Energy Astrophysical PhenomenaE+ E- --> HADRONSE+ E- --> Z0Integrated Cross Section91.2Jet Productionrespiratory systemCross Sectionequipment and suppliesSIGcomplex mixturesE+ E- --> 3JETE+ E- ScatteringExclusiveHigh Energy Physics::ExperimentR measurementhuman activitiescirculatory and respiratory physiology
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"Table 30" of "Properties of hadronic Z decays and test of QCD generators"

1992

N-jet production rates (in percent) corrected for charged and neutral particles.

Astrophysics::High Energy Astrophysical PhenomenaE+ E- --> HADRONSE+ E- --> Z0Integrated Cross Section91.2Jet Productionrespiratory systemCross Sectionequipment and suppliesSIGcomplex mixturesE+ E- --> 3JETE+ E- ScatteringExclusiveHigh Energy Physics::ExperimentR measurementhuman activitiescirculatory and respiratory physiology
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"Table 31" of "Properties of hadronic Z decays and test of QCD generators"

1992

N-jet production rates (in percent) corrected for charged and neutral particles.

Astrophysics::High Energy Astrophysical PhenomenaE+ E- --> HADRONSE+ E- --> Z0Integrated Cross Section91.2Jet Productionrespiratory systemCross Sectionequipment and suppliesSIGcomplex mixturesE+ E- --> 4JETE+ E- ScatteringExclusiveHigh Energy Physics::ExperimentR measurementhuman activitiescirculatory and respiratory physiology
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