Search results for "Solar data"

showing 4 items of 4 documents

Status of a hybrid three-neutrino interpretation of neutrino data

2001

We reanalyze the non-standard interaction (NSI) solutions to the solar neutrino problem in the light of the latest solar, atmospheric and reactor neutrino data. We show that such solutions, although preferred by the solar data and consistent with the oscillation description of the atmospheric neutrino data, are ruled out by the first results of the KamLAND reactor experiment, at more than 3_sigma.

PhysicsNuclear and High Energy PhysicsParticle physicsOscillationPhysics::Instrumentation and DetectorsSigmaFísicaFOS: Physical sciencesSolar neutrino problemInterpretation (model theory)Physics::GeophysicsHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Astrophysics::Solar and Stellar AstrophysicsHigh Energy Physics::ExperimentReactor neutrinoAstrophysics::Earth and Planetary AstrophysicsNeutrinoAtmospheric neutrinoSolar data
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Solving the solar neutrino puzzle with KamLAND and solar data

2001

We study what will be learnt about the solar neutrino puzzle and solar neutrino oscillations once the data from the KamLAND reactor neutrino experiment (soon to become available) are combined with those from the current solar neutrino experiments. We find that, in agreement with previous estimates, if the solution to the solar neutrino puzzle falls on the LMA region, KamLAND should be able to ``pin-point'' the right solution with unprecedented accuracy after a few years of data taking. Furthermore, the light side ($\theta\pi/4$) at the 95% confidence level (CL) for most of the LMA region allowed by the current data at the 99% CL, while the addition of the KamLAND data need not improve our a…

PhysicsNuclear and High Energy PhysicsParticle physicsOscillationPhysics::Instrumentation and DetectorsSolar neutrinoFOS: Physical sciencesOrder (ring theory)SigmaSolar neutrino problemHigh Energy Physics - ExperimentHigh Energy Physics - PhenomenologyHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)AstronomiaAstrophysics::Solar and Stellar AstrophysicsHigh Energy Physics::ExperimentNeutrino oscillationBorexinoParticle Physics - PhenomenologySolar data
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Constraining nonstandard neutrino-quark interactions with solar, reactor and accelerator data

2009

We present a reanalysis of nonstandard neutrino-down-quark interactions of electron and tau neutrinos using solar, reactor and accelerator data. In addition updating the analysis by including new solar data from SNO phase III and Borexino, as well as new KamLAND data and solar fluxes, a key role is played in our analysis by the combination of these results with the CHARM data. The latter allows us to better constrain the axial and axial-vector electron and tau-neutrino nonstandard interaction parameters characterizing the deviations from the Standard Model predictions.

QuarkHistoryNuclear and High Energy PhysicsParticle physicsPhysics::Instrumentation and DetectorsPhase (waves)FOS: Physical sciencesElectronEducationStandard ModelPhysics::GeophysicsHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)Charm (quantum number)Nuclear Experiment (nucl-ex)Neutrino oscillationNuclear ExperimentSolar and Stellar Astrophysics (astro-ph.SR)BorexinoSolar dataPhysicsNeutral currentHigh Energy Physics::PhenomenologyFísicaComputer Science ApplicationsHigh Energy Physics - PhenomenologyAstrophysics - Solar and Stellar AstrophysicsHigh Energy Physics::ExperimentNeutrino
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A methodology for optimisation of solar dish-Stirling systems size, based on the local frequency distribution of direct normal irradiance

2021

Abstract In geographical areas where direct solar irradiation levels are relatively high, concentrated solar energy systems are one of the most promising green energy technologies. Dish-Stirling systems are those that achieve the highest levels of solar-to-electric conversion efficiency, and yet they are still among the least common commercially available technologies. This paper focuses on a strategy aimed at promoting greater diffusion of dish-Stirling systems, which involves optimizing the size of the collector aperture area based on the hourly frequency distributions of beam irradiance and defining a new incentive scheme with a feed-in tariff that is variable with the installed costs of…

Stirling engineSettore ING-IND/11 - Fisica Tecnica AmbientaleMeteorologyLCOEbusiness.industryNumerical modelsMechanical EngineeringConcentrating Solar PowerEnergy conversion efficiencyIrradianceBuilding and ConstructionManagement Monitoring Policy and LawSolar energylaw.inventionRenewable energyIncentive policiesElectric power systemGeneral EnergylawSolar datasetsDish-StirlingEnvironmental scienceFrequency distributionCost of electricity by sourcebusiness
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