0000000000461862

AUTHOR

E. A. Garcés

showing 4 related works from this author

The liquid-argon scintillation pulseshape in DEAP-3600

2020

AbstractDEAP-3600 is a liquid-argon scintillation detector looking for dark matter. Scintillation events in the liquid argon (LAr) are registered by 255 photomultiplier tubes (PMTs), and pulseshape discrimination (PSD) is used to suppress electromagnetic background events. The excellent PSD performance of LAr makes it a viable target for dark matter searches, and the LAr scintillation pulseshape discussed here is the basis of PSD. The observed pulseshape is a combination of LAr scintillation physics with detector effects. We present a model for the pulseshape of electromagnetic background events in the energy region of interest for dark matter searches. The model is composed of (a) LAr scin…

PhotomultiplierPhysics - Instrumentation and DetectorsPhysics and Astronomy (miscellaneous)Physics::Instrumentation and DetectorsDark matterFOS: Physical scienceslcsh:AstrophysicsScintillatorWavelength shifter01 natural sciencesParticle detectorDEAPOptics0103 physical scienceslcsh:QB460-466lcsh:Nuclear and particle physics. Atomic energy. Radioactivity010306 general physicsEngineering (miscellaneous)PhysicsScintillation010308 nuclear & particles physicsbusiness.industryInstrumentation and Detectors (physics.ins-det)Scintillation counterlcsh:QC770-798businessEuropean Physical Journal C: Particles and Fields
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The weak mixing angle from low energy neutrino measurements: A global update

2016

Taking into account recent theoretical and experimental inputs on reactor fluxes we reconsider the determination of the weak mixing angle from low energy experiments. We perform a global analysis to all available neutrino-electron scattering data from reactor antineutrino experiments, obtaining sin^2(theta_W) = 0.252 \pm 0.030. We discuss the impact of the new theoretical prediction for the neutrino spectrum, the new measurement of the reactor antineutrino spectrum by the Daya Bay collaboration, as well as the effect of radiative corrections. We also reanalyze the measurements of the nu_e-e cross section at accelerator experiments including radiative corrections. By combining reactor and ac…

ImaginationNuclear and High Energy Physicsmedia_common.quotation_subjectFOS: Physical sciences01 natural sciencesHigh Energy Physics - ExperimentPhysics::GeophysicsNuclear physicsHigh Energy Physics - Experiment (hep-ex)Cross section (physics)High Energy Physics - Phenomenology (hep-ph)Low energy0103 physical sciencesRadiative transfer010306 general physicsMixing (physics)media_commonPhysics010308 nuclear & particles physicsScatteringWeinberg anglelcsh:QC1-999High Energy Physics - PhenomenologyHigh Energy Physics::ExperimentNeutrinolcsh:PhysicsPhysics Letters B
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Testing the Standard Model and beyond with the LENA proposal

2014

We discuss the possibility of a precision measurement of the electroweak mixing angle and a probe for new physics in the leptonic process of neutrino electron scattering. In the new physics schemes we explore the case of non standard neutrino interactions (NSI). The LENA proposal, currently under discussion, considers a large detector and the use of an articial, 51 Cr, radioactive neutrino source with of 5 MCi intensity. We also discuss the possible use of the solar neutrino

PhysicsHistorySterile neutrinoParticle physicsPhysics::Instrumentation and DetectorsSolar neutrinoPhysics beyond the Standard ModelHigh Energy Physics::PhenomenologySolar neutrino problemComputer Science ApplicationsEducationNuclear physicsNeutrino detectorMeasurements of neutrino speedHigh Energy Physics::ExperimentNeutrinoNeutrino oscillationJournal of Physics: Conference Series
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Low-energy neutrino-electron scattering as a Standard Model probe: the potential of LENA as case study

2011

Several proposals for studying neutrinos with large detectors are currently under discussion. We suggest that they could provide a precise measurement of the electroweak mixing angle as well as a probe for new physics, such as non-standard neutrino interactions (NSI), and the electroweak gauge structure. We illustrate this explicitly for the case of the LENA proposal, either with an artificial radioactive source or by using the solar neutrino flux.

Nuclear and High Energy PhysicsParticle physicsPhysics::Instrumentation and DetectorsPhysics beyond the Standard ModelSolar neutrinoAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciences7. Clean energy01 natural sciencesStandard ModelHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)0103 physical sciences010306 general physicsNeutrino oscillationPhysics010308 nuclear & particles physicsElectroweak interactionHigh Energy Physics::PhenomenologyFísicaSolar neutrino problemHigh Energy Physics - PhenomenologyHigh Energy Physics::ExperimentNeutrinoElectron scattering
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