Search results for "Antineutrinos"

showing 5 items of 5 documents

Search for low-energy neutrinos from astrophysical sources with Borexino

2019

We report on searches for neutrinos and antineutrinos from astrophysical sources performed with the Borexino detector at the Laboratori Nazionali del Gran Sasso in Italy. Electron antineutrinos ($\bar{\nu}_e$) are detected in an organic liquid scintillator through the inverse $\beta$-decay reaction. In the present work we set model-independent upper limits in the energy range 1.8-16.8 MeV on neutrino fluxes from unknown sources that improve our previous results, on average, by a factor 2.5. Using the same data set, we first obtain experimental constraints on the diffuse supernova $\bar{\nu}_e$ fluxes in the previously unexplored region below 8 MeV. A search for $\bar{\nu}_e$ in the solar ne…

antineutrinosPhysics - Instrumentation and Detectorssolar flaresmagnetic field: highneutrino: solarPhysics::Instrumentation and DetectorsSolar neutrinoscintillation counter: liquidelastic scatteringantineutrino/e: particle identification01 natural sciences7. Clean energyneutrino: fluxlaw.inventionHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)law[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]neutrino: supernova26.65.+t010303 astronomy & astrophysicsBorexinoElastic scatteringPhysicsSolar flareSupernova Relic Neutrinosneutrino: energy spectrumS067EB8neutrinosInstrumentation and Detectors (physics.ins-det)neutrino: magnetic momentDiffuse Supernova Neutrino Background3. Good healthSupernovaHomestakeddc:540neutrino: flavorAntineutrinoBorexinoNeutrino97.60.BwHomestake experimentFlareantineutrino/e: fluxAntineutrinos13.15.+G; 26.65.+T; 29.40.Mc; 97.60.Bw; Antineutrinos; Diffuse supernova neutrino background; Neutrinos; Solar flares; Supernova relic neutrinosAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesSupernova relic neutrinosupernova relic neutrinosNONuclear physics13.15.+gPE2_2Antineutrinos; Neutrinos; Diffuse supernova neutrino background; Supernova relic neutrinos; Solar flares0103 physical sciencesNeutrino[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]Neutrinosdiffuse supernova neutrino background010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyAstronomy and Astrophysicsneutrino: particle source29.40.McGran SassoSolar flareSolar Flares13. Climate actionspectralHigh Energy Physics::Experimentexperimental results
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TAGS measurements for neutrino physics and applications

2017

En la actualidad un gran número de temas de interés en Física Nuclear continúan planteando interrogantes fundamentales. Una de las fuentes de información más esclarecedoras es el proceso de la desintegración beta. Gracias al estudio experimental de este fenómeno en núcleos alejados de la estabilidad, es posible extraer valiosa información sobre estructura nuclear. En esa línea, esta tesis se centra en la determinación de las intensidades beta que pueblan los estados excitados del núcleo hijo en la desintegración beta de núcleos exóticos de gran interés. Para ello se ha utilizado la técnica de Espectroscopía gamma de Absorción Total (TAGS, por sus siglas en inglés), basada en el uso de grand…

espectroscopía de absorción totalespectro de antineutrinos de un reactorsimulaciones MC:FÍSICA::Física atómica y nuclear ::Estructura nuclear [UNESCO]datos nuclearesdesintegración betaUNESCO::FÍSICA::Nucleónica::Detectores de partículas:FÍSICA::Nucleónica::Detectores de partículas [UNESCO]:FÍSICA::Física atómica y nuclear ::Desintegración nuclear [UNESCO]estructura nuclearemisión retardada de neutronesUNESCO::FÍSICA::Física atómica y nuclear ::Desintegración nucleardesintegración doble betadetectores de centellenoUNESCO::FÍSICA::Física atómica y nuclear ::Estructura nuclearcalor residual de un reactor
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A search for neutrino–antineutrino mass inequality by means of sterile neutrino oscillometry

2015

The investigation of the oscillation pattern induced by the sterile neutrinos might determine the oscillation parameters, and at the same time, allow to probe CPT symmetry in the leptonic sector through neutrino-antineutrino mass inequality. We propose to use a large scintillation detector like JUNO or LENA to detect electron neutrinos and electron antineutrinos from MCi electron capture or beta decay sources. Our calculations indicate that such an experiment is realistic and could be performed in parallel to the current research plans for JUNO and RENO. Requiring at least 5$\sigma$ confidence level and assuming the values of the oscillation parameters indicated by the current global fit, w…

Nuclear and High Energy PhysicsSterile neutrinoParticle physicsPhysics - Instrumentation and DetectorsElectron captureCPT symmetryFOS: Physical sciencesElectronHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)sterile neutrinoslcsh:Nuclear and particle physics. Atomic energy. RadioactivityNeutrino oscillationPhysicsta114OscillationHigh Energy Physics::PhenomenologyInstrumentation and Detectors (physics.ins-det)oscillation patternHigh Energy Physics - Phenomenologyelectron antineutrinoslcsh:QC770-798High Energy Physics::ExperimentNeutrinoGALLEXelectron neutrinos
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Borexino’s search for low-energy neutrino and antineutrino signals correlated with gamma-ray bursts

2017

International audience; A search for neutrino and antineutrino events correlated with 2350 gamma-ray bursts (GRBs) is performed with Borexino data collected between December 2007 and November 2015. No statistically significant excess over background is observed. We look for electron antineutrinos ( ν¯e ) that inverse beta decay on protons with energies from 1.8  MeV to 15  MeV and set the best limit on the neutrino fluence from GRBs below 8  MeV. The signals from neutrinos and antineutrinos from GRBs that scatter on electrons are also searched for, a detection channel made possible by the particularly radio-pure scintillator of Borexino. We obtain currently the best limits on the neutrino f…

antineutrinoselectronAntineutrinosneutrino: solarPhysics::Instrumentation and Detectorsdata acquisitionSolar neutrino[ PHYS.ASTR ] Physics [physics]/Astrophysics [astro-ph]Astrophysics::High Energy Astrophysical Phenomenalow energy/MeV neutrinosElectrongamma ray: burst01 natural sciencesNuclear physicsLow energy/MeV neutrino0103 physical sciencesNeutrinoLow energy/MeV neutrinosNeutrinosNuclear Experiment010303 astronomy & astrophysicsGamma-ray burstBorexinoscintillation counterPhysicsflavor010308 nuclear & particles physicsbackgroundgamma-ray burstsneutrinosAntineutrinos; Gamma-ray bursts; Low energy/MeV neutrinos; Neutrinos; Astronomy and AstrophysicsAstronomy and Astrophysicssemileptonic decayantineutrinocorrelation: timeNeutrino detectorInverse beta decayddc:540Scintillation counterreadoutHigh Energy Physics::ExperimentBorexinoGamma-ray burstsNeutrinoGamma-ray burst[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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Total Absorption Spectroscopy of Fission Fragments Relevant for Reactor Antineutrino Spectra Determination

2015

8 pags., 3 figs., 1 tab. ; Presented at the XXXIV Mazurian Lakes Conference on Physics, Piaski, Poland, September 6–13, 2015.

Physicsantineutrinosfission fragmentTotal absorption spectroscopyta114010308 nuclear & particles physicsFissionGeneral Physics and Astronomy[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]Total Absorption Spectroscopy01 natural sciences7. Clean energyBeta decaySpectral lineIonizing radiationNuclear physicsIGISOL facility0103 physical sciences010306 general physicsNuclear Experiment
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