Search results for "NEUTRINO"

showing 10 items of 1752 documents

Feasibility and physics potential of detecting 8B solar neutrinos at JUNO

2021

The Jiangmen Underground Neutrino Observatory (JUNO) features a 20 kt multi-purpose underground liquid scintillator sphere as its main detector. Some of JUNO's features make it an excellent location for B-8 solar neutrino measurements, such as its low-energy threshold, high energy resolution compared with water Cherenkov detectors, and much larger target mass compared with previous liquid scintillator detectors. In this paper, we present a comprehensive assessment of JUNO's potential for detecting B solar neutrinos via the neutrino-electron elastic scattering process. A reduced 2 MeV threshold for the recoil electron energy is found to be achievable, assuming that the intrinsic radioactive …

JUNOneutriino-oskillaatiosolar neutrinoPhysics::Instrumentation and DetectorsilmaisimettutkimuslaitteetneutriinotHigh Energy Physics::Experimenthiukkasfysiikkaydinfysiikka
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Deep sea tests of a prototype of the KM3NeT digital optical module

2014

SIRE(opens in a new window)|View at Publisher| Export | Download | Add to List | More... European Physical Journal C Volume 74, Issue 9, 1 September 2014, 8p Deep sea tests of a prototype of the KM3NeT digital optical module: KM3NeT Collaboration (Article) Adrián-Martínez, S.a, Ageron, M.b, Aharonian, F.c, Aiello, S.d, Albert, A.e, Ameli, F.f, Anassontzis, E.G.g, Anghinolfi, M.h, Anton, G.i, Anvar, S.j, Ardid, M.a, de Asmundis, R.k, Balasi, K.l, Band, H.m, Barbarino, G.kn, Barbarito, E.o, Barbato, F.kn, Baret, B.p, Baron, S.p, Belias, A.lq, Berbee, E.m, van den Berg, A.M.r, Berkien, A.m, Bertin, V.b, Beurthey, S.b, van Beveren, V.m, Beverini, N.st, Biagi, S.uv, Bianucci, S.t, Billault, M.b,…

KM3NeT; digital optical modulePhysics - Instrumentation and Detectors[PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Physics and Astronomy (miscellaneous)TELESCOPEPhysics::Instrumentation and Detectorsdigital optical moduleFOS: Physical sciencesNeutrino Telescopesneutrino astrophysics; Cherenkov detector; Neutrino TelescopesKM3NeT; Cherenkov; UnderwaterDESIGNCherenkov[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]Instrumentation and Methods for Astrophysics (astro-ph.IM)KM3NeTEngineering (miscellaneous)Astrophysics::Instrumentation and Methods for Astrophysicsneutrino telescopeDATA-ACQUISITIONInstrumentation and Detectors (physics.ins-det)READOUTneutrino astrophysics[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]NEUTRINOSUnderwaterAstrophysics - Instrumentation and Methods for AstrophysicsSYSTEMCherenkov detector
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Cosmic ray composition and energy spectrum from 1–30 PeV using the 40-string configuration of IceTop and IceCube

2012

Astroparticle physics 42, 15 - 32 (2013). doi:10.1016/j.astropartphys.2012.11.003

Knee regionAstrophysicsTracking (particle physics)01 natural sciencesParticle identificationIceCubeTRACKINGWATERCherenkovNeutrino energyNEUTRINO TELESCOPEUltra-high-energy cosmic rayHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsSEADetectorAstrophysics::Instrumentation and Methods for AstrophysicsLIGHTComposition; Cosmic rays; Energy spectrum; IceCube; IceTop; Knee regionddc:540IceTopPARTICLE IDENTIFICATIONAstrophysics - High Energy Astrophysical PhenomenaAstrophysics - Instrumentation and Methods for AstrophysicsIceCube detectorCompositionAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesCosmic rayddc:500.2IceCube Neutrino ObservatorySEARCHESAccelerationcosmic raysdE/dx0103 physical sciences010306 general physicsDETECTORInstrumentation and Methods for Astrophysics (astro-ph.IM)Cherenkov radiationTruncated meanMuon energy010308 nuclear & particles physicsAstronomyAstronomy and Astrophysics540Physics and AstronomycompositionEnergy SpectrumTEVEnergy spectrum
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Low-energy Neutrino Astronomy in LENA

2015

LENA (Low Energy Neutrino Astronomy) is a proposed next-generation neutrino detector based on 50 kilotons of liquid scintillator. The low detection threshold, good energy resolution and excellent background rejection inherent to the liquid-scintillator detectors make LENA a versatile observatory for low-energy neutrinos from astrophysical and terrestrial sources. In the framework of the European LAGUNA-LBNO design study, LENA is also considered as far detector for a very-long baseline neutrino beam from CERN to Pyhasalmi ¨ (Finland). The present contribution gives an overview LENA’s broad research program, highlighting the unique capabilities of liquid scintillator for the detection of low-…

LENAPhysicsParticle physicsta114Physics::Instrumentation and DetectorsSolar neutrinoAstrophysics::High Energy Astrophysical PhenomenaHigh Energy Physics::PhenomenologySolar neutrino problemPhysics and Astronomy(all)astroparticle physics. underground physicsNuclear physicslow-energy neutrino astronomyNeutrino detectorMeasurements of neutrino speedHigh Energy Physics::ExperimentNeutrino astronomyNeutrinoNeutrino oscillationElectron neutrinoPhysics Procedia
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Distillation and stripping pilot plants for the JUNO neutrino detector: Design, operations and reliability

2019

Abstract This paper describes the design, construction principles and operations of the distillation and stripping pilot plants tested at the Daya Bay Neutrino Laboratory, with the perspective to adapt these processes, system cleanliness and leak-tightness standards to the final full scale plants to be used for the purification of the liquid scintillator of the JUNO neutrino detector. The main goal of these plants is to remove radio impurities from the liquid scintillator while increasing its optical attenuation length. Purification of liquid scintillator will be performed with a system combining alumina oxide, distillation, water extraction and steam (or N 2 gas) stripping. Such a combined…

Large-scale experimentNuclear and High Energy PhysicsPhysics - Instrumentation and DetectorsLiquid scintillatorAttenuation length; LAB; Large-scale experiments; Light yield; Liquid scintillator; Nitrogen purging; Radiopurity; Scintillator transparency; Nuclear and High Energy Physics; Instrumentationscintillation counter: liquidMixing (process engineering)Full scaleFOS: Physical sciencesRadiopurityfabricationScintillator01 natural sciences7. Clean energyStripping (fiber)law.inventionNOlaw0103 physical sciencesthorium: admixtureAttenuation length; LAB; Large-scale experiments; Light yield; Liquid scintillator; Nitrogen purging; Radiopurity; Scintillator transparency[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsProcess engineeringDistillationInstrumentationbackground: radioactivityNuclear and High Energy PhysicPhysicsLABJUNOLarge-scale experiments010308 nuclear & particles physicsbusiness.industryuranium: admixtureSettore FIS/01 - Fisica SperimentaleAttenuation lengthInstrumentation and Detectors (physics.ins-det)Attenuation lengthNitrogen purgingNeutrino detectorScintillator transparencyNeutrinobusinessaluminum: oxygenLight yield
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Predictive discrete dark matter model and neutrino oscillations

2012

Dark Matter stability can be achieved through a partial breaking of a flavor symmetry. In this framework we propose a type-II seesaw model where left-handed matter transforms nontrivially under the flavor group Delta(54), providing correlations between neutrino oscillation parameters, consistent with the recent Daya-Bay and RENO reactor angle measurements, as well as lower bounds for neutrinoless double beta decay. The dark matter phenomenology is provided by a Higgs-portal.

Left handedPhysicsNuclear and High Energy PhysicsParticle physics010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyDark matterScalar field dark matterFísica01 natural sciencesSeesaw molecular geometryDouble beta decay0103 physical sciencesHiggs bosonHigh Energy Physics::Experiment010306 general physicsNeutrino oscillationPhenomenology (particle physics)Physical Review D
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Left-handed neutrino disappearance probe of neutrino mass and character

1996

We explore the sensitivity to a non vanishing neutrino mass offered by dynamical observables, i.e., branching ratios and polarizations. The longitudinal polarization in the C.M. frame decreases by a 4% for $D^+ \rightarrow \tau^+ \nu_\tau$ and $m_{\nu_\tau}=24$ MeV. Taking advantage of the fact that the polarization is a Lorentz variant quantity, we study the polarization effects in a boosted frame. By means of a neutrino beam, produced by a high velocity boosted parent able to flip the neutrino helicity, we find that an enhanced left-handed neutrino deficit, induced by a Wigner rotation, appears.

Left handedPhysicsParticle physicsLorentz transformationHigh Energy Physics::PhenomenologyWigner rotationFOS: Physical sciencesFísicaGeneral Physics and AstronomyObservableNeutrino beamPolarization (waves)HelicityNuclear physicssymbols.namesakeHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)symbolsHigh Energy Physics::ExperimentNeutrino
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Supersymmetric SO(10)-inspired GUTs with sliding scales

2013

We construct lists of supersymmetric models with extended gauge groups at intermediate steps, all of which are inspired by SO(10) unification. We consider three different kinds of setups: (i) the model has exactly one additional intermediate scale with a left-right (LR) symmetric group; (ii) SO(10) is broken to the LR group via an intermediate Pati-Salam scale; and (iii) the LR group is broken into SU(3)(c) X SU(2)(L) X U(1)(R) X U(1)(B-L), before breaking to the standard model (SM) group. We use sets of conditions, which we call the "sliding mechanism," which yield unification with the extended gauge group(s) allowed at arbitrary intermediate energy scales. All models thus can have new gau…

Left-right symmetryNeutrino massModelsUnificationHigh Energy Physics::PhenomenologyGrand unified theoryNumberFísicaHiggs-bosonR-ParityBreakingLeptons
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Measurement of the group velocity of light in sea water at the ANTARES site

2012

The group velocity of light has been measured at eight different wavelengths between 385 nm and 532 nm in the Mediterranean Sea at a depth of about 2.2 km with the ANTARES optical beacon systems. A parametrisation of the dependence of the refractive index on wavelength based on the salinity, pressure and temperature of the sea water at the ANTARES site is in good agreement with these measurements.

Light velocityRefractive indexAtmospheric sciencesNeutrino telescope01 natural scienceslaw.inventionHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)Mediterranean sealawOptical beacon systemPhysicsOptical beaconPressure and temperature[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Wavelengthoptical beacon system; neutrino telescope; antares; refractive index; velocity of lightVelocity of lightGroup velocityFísica nuclear[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE][PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]ParametrisationFOS: Physical sciencesddc:500.2010309 opticsOpticsLight--Speed--Measurement0103 physical sciencesOptical systemsSeawater14. Life underwater:Física::Acústica [Àrees temàtiques de la UPC]ANTARES010308 nuclear & particles physicsbusiness.industryAstronomy and AstrophysicsLaser[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]SalinityLlum -- VelocitatFISICA APLICADAVelocity of lightMediterranean seaSeawaterNeutrino telescopesbusiness[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Refractive indexSYSTEM
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The Design and Sensitivity of JUNO's scintillator radiopurity pre-detector OSIRIS

2021

The European physical journal / C 81(11), 973 (2021). doi:10.1140/epjc/s10052-021-09544-4

Liquid scintillatorPhysics - Instrumentation and DetectorsPhysics and Astronomy (miscellaneous)Physics::Instrumentation and Detectorsscintillation counter: liquidmeasurement methodsQC770-798Astrophysics01 natural sciencesthorium: nuclidedesign [detector]neutrinoRadioactive purityPhysicsLow energy neutrinoJUNOliquid [scintillation counter]biologySettore FIS/01 - Fisica SperimentaleDetectorInstrumentation and Detectors (physics.ins-det)3. Good healthQB460-466Physics::Space Physicsnuclide [uranium]FOS: Physical sciencesScintillatornuclide [thorium]530NONuclear physicsPE2_2uranium: nuclideNuclear and particle physics. Atomic energy. Radioactivity0103 physical sciencesddc:530Sensitivity (control systems)[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsJUNO neutrino physics liquid scintillatorEngineering (miscellaneous)background: radioactivitydetector: designMeasurement method010308 nuclear & particles physicsradioactivity [background]biology.organism_classificationsensitivityHigh Energy Physics::ExperimentReactor neutrinoOsiris
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