Search results for "GALLEX"

showing 9 items of 9 documents

Small Residues Inhibit Homo-Dimerization of the Human Carbonic Anhydrase XII Transmembrane Domain

2021

Amino acids with small side chains and motifs of small residues in a distance of four are rather abundant in human single-span transmembrane helices. While interaction of such helices appears to be common, the role of the small residues in mediating and/or stabilizing transmembrane helix oligomers remains mostly elusive. Yet, the mere existence of (small)xxx(small) motifs in transmembrane helices is frequently used to model dimeric TM helix structures. The single transmembrane helix of the human carbonic anhydrases XII contains a large number of amino acids with small side chains, and critical involvement of these small amino acids in dimerization of the transmembrane domain has been sugges…

540 Chemistry and allied sciencesGALLEXGxxxGChemical technologycarbonic anhydrase XIITP1-1185transmembrane domainArticle570 Life sciencessmall amino acidsChemical engineering540 ChemieTP155-156interaction propensity570 Biowissenschaftenhelix–helix interactioninteraction motifMembranes
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Global three-neutrino oscillation analysis of neutrino data

2001

A global analysis of the solar, atmospheric and reactor neutrino data is presented in terms of three-neutrino oscillations. We include the most recent solar neutrino rates of Homestake, SAGE, GALLEX and GNO, as well as the recent 1117 day Super-Kamiokande data sample, including the recoil electron energy spectrum both for day and night periods and we treat in a unified way the full parameter space for oscillations, correctly accounting for the transition from the matter enhanced (MSW) to the vacuum oscillations regime. Likewise, we include in our description conversions with $\theta_{12} > \pi/4$. For the atmospheric data we perform our analysis of the contained events and the upward-going …

Nuclear and High Energy PhysicsParticle physicsAstrofísica nuclearOscillationsSolar neutrinoFOS: Physical sciencesParameter spacePartícules (Física nuclear)High Energy Physics - Phenomenology (hep-ph)Phenomenological theory (Physics)BibliographyOscil·lacionsNeutrinsNeutrinosNeutrino oscillationParticles (Nuclear physics)PhysicsCosmologiaMuonOscillationHigh Energy Physics - PhenomenologyFenomenologia (Física)High Energy Physics::ExperimentNuclear astrophysicsAstrophysics::Earth and Planetary AstrophysicsNeutrinoGALLEX
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Light sterile neutrino sensitivity at the nuSTORM facility

2014

A facility that can deliver beams of electron and muon neutrinos from the decay of a stored muon beam has the potential to unambiguously resolve the issue of the evidence for light sterile neutrinos that arises in short-baseline neutrino oscillation experiments and from estimates of the effective number of neutrino flavors from fits to cosmological data. In this paper, we show that the nuSTORM facility, with stored muons of 3.8 GeV/c $\pm$ 10%, will be able to carry out a conclusive muon neutrino appearance search for sterile neutrinos and test the LSND and MiniBooNE experimental signals with 10$\sigma$ sensitivity, even assuming conservative estimates for the systematic uncertainties. This…

Nuclear and High Energy PhysicsParticle physicsPhysics::Instrumentation and DetectorsSolar neutrinoAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstronomy & AstrophysicsComputer Science::Digital LibrariesPartícules (Física nuclear)High Energy Physics - ExperimentMiniBooNENuclear physicsHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)0201 Astronomical and Space SciencesTOOLKITNeutrino oscillationDETECTOR0206 Quantum PhysicsPhysicsGALLEXScience & Technologyhep-exPhysicsPHYSICS PARTICLES & FIELDSHigh Energy Physics::Phenomenologyhep-phSolar neutrino problemNuclear & Particles PhysicsCosmic neutrino backgroundHigh Energy Physics - PhenomenologyNeutrino detectorPhysical Sciences0202 Atomic Molecular Nuclear Particle and Plasma PhysicsComputer Science::Mathematical SoftwareMeasurements of neutrino speedPhysics::Accelerator PhysicsHigh Energy Physics::ExperimentNeutrinoParticle Physics - Experiment
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Four-neutrino oscillation solutions of the solar neutrino problem

2000

We present an analysis of the neutrino oscillation solutions of the solar neutrino problem in the framework of four-neutrino mixing where a sterile neutrino is added to the three standard ones. We perform a fit to the full data set corresponding to the 825-day Super-Kamiokande data sample as well as to Chlorine, GALLEX and SAGE and Kamiokande experiments. In our analysis we use all measured total event rates as well as all Super-Kamiokande data on the zenith angle dependence and the recoil electron energy spectrum. We consider both transitions via the Mikheyev-Smirnov-Wolfenstein (MSW) mechanism as well as oscillations in vacuum (just-so) and find the allowed solutions for different values …

Nuclear and High Energy PhysicsSterile neutrinoParticle physicsAstrofísica nuclearSolar neutrinoSolar neutrinosFOS: Physical sciencesAstrophysicsHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)Neutrins solarsCollisions (Nuclear physics)BibliographyNeutrino oscillationMixing (physics)Particles (Nuclear physics)PhysicsAstrophysics (astro-ph)High Energy Physics::PhenomenologyFísicaSolar neutrino problemHigh Energy Physics - PhenomenologyDistribution (mathematics)Col·lisions (Física nuclear)Nuclear astrophysicsHigh Energy Physics::ExperimentGALLEX
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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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Omnibus experiment: CPT and CP violation with sterile neutrinos

2016

We propose to probe both the CPT and CP violation together with the search for sterile neutrinos in one do-it-all experiment. This omnibus experiment would utilize neutrino oscillometry with large scintillator detectors like LENA, JUNO or RENO-50 and manmade radioactive sources similar to the ones used by the GALLEX experiment. Our calculations indicate that such an experiment is realistic and could be performed in parallel to the main research plan for JUNO, LENA, or RENO-50. Assuming as the starting point the values of the oscillation parameters indicated by the current global fit (in 3 active + 1 sterile scenario) and requiring at least 5 sigma confidence level, we estimate that with the…

PhysicsHistorySterile neutrinoParticle physicsSigmaComputer Science ApplicationsEducationNuclear physicsResearch planScintillation counterCP violationNeutrinoGALLEXNeutrino oscillationJournal of Physics: Conference Series
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Status of the MSW solutions of the solar neutrino problem

2000

We present an updated global analysis of two-flavor MSW solutions to the solar neutrino problem in terms of conversions of nu_e into active or sterile neutrinos. We perform a fit to the full data set corresponding to the 825-day Super-Kamiokande data sample as well as to Chlorine, GALLEX and SAGE experiments. We use all measured total event rates as well as Super-Kamiokande data on the zenith angle dependence, energy spectrum and seasonal variation of the events. For conversions into active neutrinos we find that, although the data on the total event rates favours the Small Mixing Angle (SMA) solution, once the full data set is included both SMA and Large Mixing Angle (LMA) solutions give a…

PhysicsNuclear and High Energy PhysicsParticle physicsSterile neutrinoStandard solar modelSolar neutrinoAstrophysics (astro-ph)FOS: Physical sciencesFísicaSolar neutrino problemAstrophysicsHigh Energy Physics - ExperimentMassless particleHigh Energy Physics - PhenomenologyHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)GALLEXNeutrinoNeutrino oscillationNuclear Physics B
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Status of the MSW Solutions to the Solar Neutrino Problem

2000

In this talk we present the results of an updated global analysis of two-flavor MSW solutions to the solar neutrino problem in terms of conversions of $\nu_e$ into active or sterile neutrinos including the the full data set corresponding to the 825-day Super-Kamiokande data sample as well as to Chlorine, GALLEX and SAGE experiments.

PhysicsNuclear and High Energy PhysicsSterile neutrinoParticle physicsSolar neutrinoSAGEHigh Energy Physics::PhenomenologyFOS: Physical sciencesSolar neutrino problemAtomic and Molecular Physics and OpticsHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Full dataHigh Energy Physics::ExperimentGALLEXNeutrino oscillation
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The gallium anomaly revisited

2019

The gallium anomaly, i.e. the missing electron-neutrino flux from $^{37}$Ar and $^{51}$Cr electron-capture decays as measured by the GALLEX and SAGE solar-neutrino detectors, has been among us already for about two decades. We present here a new estimate of the significance of this anomaly based on cross-section calculations using nuclear shell-model wave functions obtained by exploiting recently developed two-nucleon interactions. The gallium anomaly of the GALLEX and SAGE experiments is found to be smaller than that obtained in previous evaluations, decreasing the significance from 3.0σ to 2.3σ. This result is compatible with the recent indication in favor of short-baseline ν¯e disappeara…

gallium anomalyNuclear and High Energy PhysicsNuclear Theorychemistry.chemical_elementFluxFOS: Physical sciencesneutrino-nucleus interactions01 natural sciencesNuclear physicsNuclear Theory (nucl-th)High Energy Physics - Phenomenology (hep-ph)0103 physical sciencesGallium010306 general physicsWave functionMixing (physics)Physics010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyNuclear shell modelcharged-current cross-sectionslcsh:QC1-999High Energy Physics - Phenomenologynuclear shell modelchemistryHigh Energy Physics::ExperimentAnomaly (physics)NeutrinoGALLEXydinfysiikkalcsh:PhysicsPhysics Letters B
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