Search results for " Neutrino"

showing 10 items of 727 documents

Neutral-Current Neutrino-Nucleus Scattering off Xe Isotopes

2018

Large liquid xenon detectors aiming for dark matter direct detection will soon become viable tools also for investigating neutrino physics. Information on the effects of nuclear structure in neutrino-nucleus scattering can be important in distinguishing neutrino backgrounds in such detectors. We perform calculations for differential and total cross sections of neutral-current neutrino scattering off the most abundant xenon isotopes. The nuclear structure calculations are made in the nuclear shell model for elastic scattering, and also in the quasiparticle random-phase approximation (QRPA) and microscopic quasiparticle phonon model (MQPM) for both elastic and inelastic scattering. Using suit…

Computer Science::Machine LearningNuclear and High Energy PhysicsArticle SubjectNuclear TheoryPhysics::Instrumentation and DetectorsSolar neutrinoAstrophysics::High Energy Astrophysical PhenomenaDark matterNuclear TheoryFOS: Physical sciencesInelastic scatteringComputer Science::Digital Libraries01 natural sciencesNuclear Theory (nucl-th)Nuclear physicsStatistics::Machine LearningHigh Energy Physics - Phenomenology (hep-ph)neutrino physics0103 physical sciencesIsotopes of xenonsironta010306 general physicsPhysicsElastic scatteringneutrino-nucleus scatteringta114010308 nuclear & particles physicsScatteringHigh Energy Physics::PhenomenologyNuclear shell modelneutriinotlcsh:QC1-999High Energy Physics - PhenomenologyComputer Science::Mathematical SoftwareHigh Energy Physics::ExperimentNeutrinolcsh:PhysicsAdvances in High Energy Physics
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Characteristics of the diffuse astrophysical electron and Tau neutrino flux with six years of IceCube high energy cascade data

2020

We report on the first measurement of the astrophysical neutrino flux using particle showers (cascades) in IceCube data from 2010-2015. Assuming standard oscillations, the astrophysical neutrinos in this dedicated cascade sample are dominated (∼90%) by electron and tau flavors. The flux, observed in the sensitive energy range from 16 TeV to 2.6 PeV, is consistent with a single power-law model as expected from Fermi-type acceleration of high energy particles at astrophysical sources. We find the flux spectral index to be γ=2.53±0.07 and a flux normalization for each neutrino flavor of φastro=1.66-0.27+0.25 at E0=100 TeV, in agreement with IceCube's complementary muon neutrino results and wit…

Cosmology and Nongalactic Astrophysics (astro-ph.CO)Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesGeneral Physics and AstronomyElectronpower spectrumflux [electron]energy [particle]01 natural sciencesIceCubeNuclear physics5/3Tau neutrinomuon0103 physical scienceslow [energy]Muon neutrinoddc:530010303 astronomy & astrophysicsastro-ph.HEHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsSPECTRUMSpectral indexMuon010308 nuclear & particles physicsHigh Energy Physics::Phenomenologyflavor [neutrino]RAYSflux [neutrino]accelerationshowersoscillationPhysics and Astronomy13. Climate actionEnergy cascadePhysique des particules élémentairesastro-ph.COhigh [energy]cascade [energy]High Energy Physics::ExperimentNeutrinoAstrophysics - High Energy Astrophysical PhenomenaFermi Gamma-ray Space TelescopeAstrophysics - Cosmology and Nongalactic Astrophysics
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Euclid preparation XIX. Impact of magnification on photometric galaxy clustering

2022

Aims. We investigate the importance of lensing magnification for estimates of galaxy clustering and its cross-correlation with shear for the photometric sample of Euclid. Using updated specifications, we study the impact of lensing magnification on the constraints and the shift in the estimation of the best fitting cosmological parameters that we expect if this effect is neglected.

Cosmology and Nongalactic Astrophysics (astro-ph.CO)FOS: Physical sciencesAstrophysics::Cosmology and Extragalactic Astrophysicsshearkosmologiapower spectragalaksijoukotredshift-space distortionscosmology: theorycosmological parameterstheorydark energyAstrophysics::Galaxy Astrophysicstheory large-scale structure of Universe [cosmological parameters cosmology]theory [cosmology]massive neutrinosunified pipelineAstronomy and Astrophysics115 Astronomy Space scienceangular cross-correlationshalo-modelSpace and Planetary Science[SDU]Sciences of the Universe [physics]fotometriacosmological parametercosmic magnificationlarge-scale structure of UniversecosmologydipoleAstrophysics - Cosmology and Nongalactic Astrophysics
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Probing long-range leptonic forces with solar and reactor neutrinos

2006

In this work we study the phenomenological consequences of the existence of long-range forces coupled to lepton flavour numbers in solar neutrino oscillations. We study electronic forces mediated by scalar, vector or tensor neutral bosons and analyze their effect on the propagation of solar neutrinos as a function of the force strength and range. Under the assumption of one mass scale dominance, we perform a global analysis of solar and KamLAND neutrino data which depends on the two standard oscillation parameters, \Delta m^2_{21} and \tan^2\theta_{12}, the force coupling constant, its range and, for the case of scalar-mediated interactions, on the neutrino mass scale as well. We find that,…

Coupling constantPhysicsParticle physics010308 nuclear & particles physicsOscillationSolar neutrinoHigh Energy Physics::PhenomenologyScalar (mathematics)FOS: Physical sciencesAstronomy and Astrophysics7. Clean energy01 natural sciencesHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesHigh Energy Physics::ExperimentTensorNeutrino010306 general physicsLeptonBosonJournal of Cosmology and Astroparticle Physics
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Measurement of the Atmospheric ve flux in IceCube

2012

We report the first measurement of the atmospheric electron neutrino flux in the energy range between approximately 80 GeV and 6 TeV, using data recorded during the first year of operation of IceCube's DeepCore low energy extension. Techniques to identify neutrinos interacting within the DeepCore volume and veto muons originating outside the detector are demonstrated. A sample of 1029 events is observed in 281 days of data, of which 496 $\pm$ 66(stat.) $\pm$ 88(syst.) are estimated to be cascade events, including both electron neutrino and neutral current events. The rest of the sample includes residual backgrounds due to atmospheric muons and charged current interactions of atmospheric muo…

DEEPCOREParticle physicsAMANDAPhysics::Instrumentation and DetectorsSolar neutrinoAstrophysics::High Energy Astrophysical PhenomenaGeneral Physics and Astronomyddc:500.201 natural sciences7. Clean energyHigh Energy Physics - ExperimentNuclear physicsSEARCH0103 physical sciencesddc:550010306 general physicsNeutrino oscillationDETECTORPhysics010308 nuclear & particles physicsHigh Energy Physics::PhenomenologySolar neutrino problemCosmic neutrino backgroundNeutrino detectorPhysics and Astronomy13. Climate actionMeasurements of neutrino speedHigh Energy Physics::ExperimentNeutrino astronomyNeutrinoNEUTRINO-INDUCED CASCADESAstrophysics - High Energy Astrophysical PhenomenaPhysical Review Letters
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South Pole glacial climate reconstruction from multi-borehole laser particulate stratigraphy

2013

AbstractThe IceCube Neutrino Observatory and its prototype, AMANDA, were built in South Pole ice, using powerful hot-water drills to cleanly bore>100 holes to depths up to 2500 m. The construction of these particle physics detectors provided a unique opportunity to examine the deep ice sheet using a variety of novel techniques. We made high-resolution particulate profiles with a laser dust logger in eight of the boreholes during detector commissioning between 2004 and 2010. The South Pole laser logs are among the most clearly resolved measurements of Antarctic dust strata during the last glacial period and can be used to reconstruct paleoclimate records in exceptional detail. Here we use…

EPICA-DOME-C010504 meteorology & atmospheric sciencesDEEP ICEBoreholeAntarctic ice sheetDUSTddc:500.2ANTARCTIC ICE-SHEET01 natural sciencesIceCube Neutrino ObservatoryIceCubePaleontology0103 physical sciencesPaleoclimatologyddc:550COREGlacial period010303 astronomy & astrophysicsSIPLE DOME0105 earth and related environmental sciencesEarth-Surface Processesgeographygeography.geographical_feature_categoryEAST ANTARCTICAVOLCANIC WINTERVOSTOKOPTICAL-PROPERTIESStratigraphy13. Climate actionEarth and Environmental SciencesRadiometric datingIce sheetphysicsGeology
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Probing nonstandard neutrino-electron interactions with solar and reactor neutrinos

2009

Most neutrino mass extensions of the standard electroweak model entail non-standard interactions which, in the low energy limit, can be parametrized in term of effective four-fermion operators $\nu_\alpha \nu_\beta \bar f f $. Typically of sub-weak strength, $\epsilon_{\alpha \beta} G_F$, these are characterized by dimensionless coupling parameters, $\epsilon_{\alpha \beta}$, which may be relatively sizeable in a wide class of schemes. Here we focus on non-universal (NU) flavor conserving couplings ($\alpha = \beta$) with electrons ($f = e$) and analyse their impact on the phenomenology of solar neutrinos. We consistently take into account their effect both at the level of propagation where…

Elastic scatteringPhysicsNuclear and High Energy PhysicsParticle physicsSolar neutrinoHigh Energy Physics::PhenomenologyElectroweak interactionFOS: Physical sciencesFísicaElectronHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)High Energy Physics::ExperimentBeta (velocity)NeutrinoPhenomenology (particle physics)Dimensionless quantityPhysical Review D
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Search for Coherent Elastic Scattering of Solar B8 Neutrinos in the XENON1T Dark Matter Experiment

2021

We report on a search for nuclear recoil signals from solar $^8$B neutrinos elastically scattering off xenon nuclei in XENON1T data, lowering the energy threshold from 2.6 keV to 1.6 keV. We develop a variety of novel techniques to limit the resulting increase in backgrounds near the threshold. No significant $^8$B neutrino-like excess is found in an exposure of 0.6 t $\times$ y. For the first time, we use the non-detection of solar neutrinos to constrain the light yield from 1-2 keV nuclear recoils in liquid xenon, as well as non-standard neutrino-quark interactions. Finally, we improve upon world-leading constraints on dark matter-nucleus interactions for dark matter masses between 3 GeV/…

Elastic scatteringPhysicsPhysics::Instrumentation and DetectorsScatteringAstrophysics::High Energy Astrophysical PhenomenaSolar neutrinoDark matterGeneral Physics and Astronomychemistry.chemical_element01 natural sciences7. Clean energyNuclear physicsXenonRecoilchemistry0103 physical sciencesHigh Energy Physics::ExperimentNeutrinoNuclear Experiment010306 general physicsOrder of magnitudePhysical Review Letters
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"Table 4" of "Search for a right-handed gauge boson decaying into a high-momentum heavy neutrino and a charged lepton in $pp$ collisions with the ATL…

2019

Observed 95% CL exclusion contours in the $(m_{N_R}, m_{W_R})$ plane in the muon channel.

Exclusion limits13000.0WR --> NR lRight-hanedeHeavy neutrinoGauge BosonLeft-Right SymmetricP P --> WR
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"Table 2" of "Search for a right-handed gauge boson decaying into a high-momentum heavy neutrino and a charged lepton in $pp$ collisions with the ATL…

2019

Observed 95% CL exclusion contours in the $(m_{N_R}, m_{W_R})$ plane in the electron channel.

Exclusion limits13000.0WR --> NR lRight-hanedeHeavy neutrinoGauge BosonLeft-Right SymmetricP P --> WR
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