0000000001276801

AUTHOR

J. Farine

showing 4 related works from this author

Direct evidence for neutrino flavor transformation from neutral-current interactions in the Sudbury Neutrino Observatory

2002

Observations of neutral current neutrino interactions on deuterium in the Sudbury Neutrino Observatory are reported. Using the neutral current, elastic scattering, and charged current reactions and assuming the standard 8B shape, the electron-neutrino component of the 8B solar flux is 1.76 +/-0.05(stat.)+/-0.09(syst.) x10^6/(cm^2 s), for a kinetic energy threshold of 5 MeV. The non-electron neutrino component is 3.41+/-0.45(stat.)+0.48,-0.45(syst.) x10^6/(cm^2 s), 5.3 standard deviations greater than zero, providing strong evidence for solar electron neutrino flavor transformation. The total flux measured with the NC reaction is 5.09 +0.44,-0.43(stat.)+0.46,-0.43(syst.)x10^6/(cm^2 s), consi…

Particle physicsPhysics::Instrumentation and DetectorsSolar neutrinoAstrophysics::High Energy Astrophysical PhenomenaGeneral Physics and AstronomyFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciences7. Clean energyHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)Tau neutrino0103 physical sciencesNuclear Experiment (nucl-ex)010306 general physicsNeutrino oscillationNuclear ExperimentNuclear ExperimentPhysicsSudbury Neutrino Observatory010308 nuclear & particles physicsHigh Energy Physics::PhenomenologySolar neutrino problemNeutrino detectorHigh Energy Physics::ExperimentAstrophysics::Earth and Planetary AstrophysicsNeutrinoLepton
researchProduct

Measurement of day and night neutrino energy spectra at SNO and constraints on neutrino mixing parameters

2002

The Sudbury Neutrino Observatory (SNO) has measured day and night solar neutrino energy spectra and rates. For charged current events, assuming an undistorted $^8$B spectrum, the night minus day rate is $14.0% \pm 6.3% ^{+1.5}_{-1.4}%$ of the average rate. If the total flux of active neutrinos is additionally constrained to have no asymmetry, the $\nu_e$ asymmetry is found to be $7.0% \pm 4.9% ^{+1.3}_{-1.2}%$. A global solar neutrino analysis in terms of matter-enhanced oscillations of two active flavors strongly favors the Large Mixing Angle (LMA) solution.

Astrophysics::High Energy Astrophysical PhenomenaSolar neutrinoFOS: Physical sciencesGeneral Physics and AstronomyFluxCosmic rayAstrophysics7. Clean energy01 natural sciencesHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)0103 physical sciencesNuclear astrophysicsNuclear Experiment (nucl-ex)010306 general physicsNeutrino oscillationNuclear ExperimentAstrophysics::Galaxy AstrophysicsCharged currentPhysicsSudbury Neutrino Observatory010308 nuclear & particles physicsAstrophysics (astro-ph)High Energy Physics::Phenomenology13. Climate actionHigh Energy Physics::ExperimentAstrophysics::Earth and Planetary AstrophysicsNeutrino
researchProduct

Measurement of the Spectral Shape of the β -Decay of Xe137 to the Ground State of Cs137 in EXO-200 and Comparison with Theory

2020

We report on a comparison between the theoretically predicted and experimentally measured spectra of the first-forbidden nonunique β-decay transition ^{137}Xe(7/2^{-})→^{137}Cs(7/2^{+}). The experimental data were acquired by the EXO-200 experiment during a deployment of an AmBe neutron source. The ultralow background environment of EXO-200, together with dedicated source deployment and analysis procedures, allowed for collection of a pure sample of the decays, with an estimated signal to background ratio of more than 99 to 1 in the energy range from 1075 to 4175 keV. In addition to providing a rare and accurate measurement of the first-forbidden nonunique β-decay shape, this work constitut…

PhysicsSpectral shape analysisGeneral Physics and AstronomyNuclear dataContext (language use)Electron7. Clean energy01 natural sciencesSpectral line0103 physical sciencesNeutron sourceAtomic physics010306 general physicsGround stateEnergy (signal processing)Physical Review Letters
researchProduct

Measurement of the Spectral Shape of the beta-decay of 137Xe to the Ground State of 137Cs in EXO-200 and Comparison with Theory

2020

We report on a comparison between the theoretically predicted and experimentally measured spectra of the first-forbidden non-unique $\beta$-decay transition $^{137}\textrm{Xe}(7/2^-)\to\,^{137}\textrm{Cs}(7/2^+)$. The experimental data were acquired by the EXO-200 experiment during a deployment of an AmBe neutron source. The ultra-low background environment of EXO-200, together with dedicated source deployment and analysis procedures, allowed for collection of a pure sample of the decays, with an estimated signal-to-background ratio of more than 99-to-1 in the energy range from 1075 to 4175 keV. In addition to providing a rare and accurate measurement of the first-forbidden non-unique $\bet…

Nuclear Theory (nucl-th)Nuclear TheoryFOS: Physical sciencesNuclear Experiment (nucl-ex)Nuclear Experiment
researchProduct