0000000000330764

AUTHOR

Michael Meyer

showing 6 related works from this author

Short distance neutrino oscillations with Borexino

2014

International audience; The Borexino detector has convincingly shown its outstanding performances in the low energy, sub-MeV regime through its unprecedented accomplishments in the solar and geo-neutrinos detection. These performances make it the ideal tool to accomplish a state-of-the-art experiment able to test unambiguously the long-standing issue of the existence of a sterile neutrino, as suggested by the several anomalous results accumulated over the past two decades, i.e. the outputs of the LSND and Miniboone experiments, the results of the source calibration of the two Gallium solar neutrino experiments, and the recently hinted reactor anomaly. The SOX project will exploit two source…

Particle physicsSterile neutrinoneutrino: solarPhysics::Instrumentation and DetectorsQC1-999Solar neutrinoscintillation counter: liquidanomalyneutrino: beam7. Clean energy01 natural sciencesNuclear physicsMiniBooNEPhysics and Astronomy (all)0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]010306 general physicsNeutrino oscillationBorexinoenergy: lowPhysicsgallium010308 nuclear & particles physicsantineutrino: beamPhysicsDetectorHigh Energy Physics::Phenomenologytalk: Noto 2014/09/30neutrino: sterilecalibrationneutrino: nuclear reactorceriumLSNDradioactivityHigh Energy Physics::ExperimentBorexinoneutrino: familychromiumneutrino: oscillationNeutrinoAnomaly (physics)performanceexperimental results
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A test of electric charge conservation with Borexino

2015

Borexino is a liquid scintillation detector located deep underground at the Laboratori Nazionali del Gran Sasso (LNGS, Italy). Thanks to the unmatched radio-purity of the scintillator, and to the well understood detector response at low energy, a new limit on the stability of the electron for decay into a neutrino and a single mono-energetic photon was obtained. This new bound, tau > 6.6 10**28 yr at 90 % C.L., is two orders of magnitude better than the previous limit.

Particle physicsPhysics - Instrumentation and DetectorsOrders of magnitude (temperature)Physics::Instrumentation and DetectorsGeneral Physics and AstronomyFOS: Physical sciencesElectronScintillatorElectric chargeHigh Energy Physics - ExperimentNuclear physicsPhysics and Astronomy (all)High Energy Physics - Experiment (hep-ex)ddc:550Nuclear ExperimentBorexinoComputingMilieux_MISCELLANEOUSPhysics[PHYS]Physics [physics]Liquid scintillation countingDetectorAstrophysics::Instrumentation and Methods for AstrophysicsInstrumentation and Detectors (physics.ins-det)High Energy Physics::ExperimentNeutrino[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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Exposure to Gastric Acid Inhibitors Increases the Risk of Infection in Preterm Very Low Birth Weight Infants but Concomitant Administration of Lactof…

2018

Objective: To investigate whether exposure to inhibitors of gastric acidity, such as H2 blockers or proton pump inhibitors, can independently increase the risk of infections in very low birth weight (VLBW) preterm infants in the neonatal intensive care unit. Study design: This is a secondary analysis of prospectively collected data from a multicenter, randomized controlled trial of bovine lactoferrin (BLF) supplementation (with or without the probiotic Lactobacillus rhamnosus GG) vs placebo in prevention of late-onset sepsis (LOS) and necrotizing enterocolitis (NEC) in preterm infants. Inhibitors of gastric acidity were used at the recommended dosages/schedules based on the clinical judgmen…

ColonizationProton Pump InhibitorNeonatal intensive care unitAdministration OralHistamine H2 AntagonistProbioticGastroenterologyPediatricsH2 blocker0302 clinical medicineRisk FactorsInfant Very Low Birth Weight030212 general & internal medicineCandidaVLBW neonateLacticaseibacillus rhamnosusGestational agePerinatology and Child HealthHistamine H2 AntagonistsItalyNecrotizing enterocolitismedicine.symptomInfectionInfant PrematureHumanmedicine.medical_specialtyBirth weightGastric AcidSepsis03 medical and health sciencesEnterocolitis NecrotizingIntensive Care Units NeonatalSepsis030225 pediatricsInternal medicinemedicineH2 blockersHumansDietary Supplementbusiness.industryRisk FactorProbioticsInfant NewbornProton Pump Inhibitorsmedicine.diseaseLow birth weightLactoferrinConcomitantDietary SupplementsPediatrics Perinatology and Child HealthVLBW neonatesCandida; Colonization; H2 blockers; Infection; Lactoferrin; VLBW neonates; Pediatrics Perinatology and Child HealthGastric acidLactobacillus rhamnosubusinessNew Zealand
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Recent results from Borexino

2016

Journal of Physics Conference Series. - 798, International Conference on Particle Physics and Astrophysics : 10-14 October 2016, Moscow, Russian Federation / proceedings editors: 1. issue: cosmic rays: Arkady Galper (MEPhI, Moscow, Russia) [und 7 andere] 2nd International Conference on Particle Physics and Astrophysics, ICPPA 2016, Moscow, Russia, 11 Oct 2016 - 14 Oct 2016; Bristol : IOP Publ., Journal of Physics Conference Series, 798, 012114 pp. (2017). doi:10.1088/1742-6596/798/1/012114

HistoryParticle physicsneutrino: solarPhysics::Instrumentation and DetectorsSolar neutrinoContext (language use)53001 natural sciencesneutrino: fluxEducationPhysics::GeophysicsNuclear physicsPhysics and Astronomy (all)Low energyenergy: solar0103 physical sciencesEnergy spectrumddc:530010306 general physicsBorexinoscintillation counterPhysicsCharge conservationMultidisciplinary010308 nuclear & particles physicsstabilityComputer Science ApplicationsGran Sassoenergy: productionPhysics::Space PhysicsHigh Energy Physics::ExperimentBorexinoneutrino: geophysics[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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SOX : short distance neutrino oscillations with Borexino

2014

Abstract The Borexino detector has convincingly shown its outstanding performance in the in the sub-MeV regime through its unprecedented accomplishments in the solar and geo-neutrinos detection, which make it the ideal tool to unambiguously test the long-standing issue of the existence of a sterile neutrino, as suggested by several anomalies: the outputs of the LSND and Miniboone experiments, the results of the source calibration of the two Gallium solar ν experiments, and the recently hinted reactor anomaly. The SOX project will exploit two sources, based on chromium and cerium, which deployed under the experiment will emit two intense beams of ν e (Cr) and ν e ‾ (Ce). Interacting in the a…

Sterile neutrinoPhysics::Instrumentation and Detectorsscintillation counter: liquidtalk: Valencia 2014/07/027. Clean energy01 natural sciences[SPI]Engineering Sciences [physics][PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]BorexinoSterile neutrinogalliumPhysicsOscillationneutrino: sterilesolarceriumBorexinochromiumchromium-51neutrino: geophysicsNeutrinoperformanceNuclear and High Energy PhysicsParticle physicsAnomalous oscillations; Borexino; Cerium-144; Chromium-51; SOX; Sterile neutrinosanomalyneutrino/e: beamScintillatorcerium-144Anomalous oscillations; Borexino; Cerium-144; Chromium-51; SOX; Sterile neutrinos; Nuclear and High Energy PhysicsMiniBooNEsterile neutrinos0103 physical sciences010306 general physicsNeutrino oscillation010308 nuclear & particles physicschromium-51cerium-144calibrationGran SassoLSNDAnomalous oscillationSOXneutrino: familyHigh Energy Physics::Experimentnuclear reactorneutrino: oscillationAnomaly (physics)anomalous oscillationsexperimental resultsneutrino/e: oscillation
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The Evolution of Disk Winds from a Combined Study of Optical and Infrared Forbidden Lines

2020

We analyze high-resolution (dv=<10km/s) optical and infrared spectra covering the [OI] 6300 angstrom and [NeII] 12.81 micron lines from a sample of 31 disks in different evolutionary stages. Following work at optical wavelengths, we use Gaussian profiles to fit the [NeII] lines and classify them into HVC (LVC) if the line centroid is more (less) blueshifted than 30 km/s with respect to the stellar radial velocity. Unlike for the [OI] where a HVC is often accompanied by a LVC, all 17 sources with a [NeII] detection have either a HVC or a LVC. [NeII] HVCs are preferentially detected toward high accretors (Macc > 10$^{-8}$ Msun/yr) while LVCs are found in sources with low Macc, low [OI] …

Protoplanetary disks1300010504 meteorology & atmospheric sciencesInfraredFOS: Physical sciencesAstrophysics01 natural sciencesLuminosityStellar accretion disksStellar jets0103 physical sciences1607010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)0105 earth and related environmental sciencesLine (formation)Earth and Planetary Astrophysics (astro-ph.EP)PhysicsSpectral index1579Astronomy and AstrophysicsAstrophysics - Astrophysics of GalaxiesRadial velocityFull width at half maximumWavelengthAstrophysics - Solar and Stellar Astrophysics13. Climate actionSpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)MagnetohydrodynamicsAstrophysics - Earth and Planetary Astrophysics
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