Search results for "Abilities"

showing 10 items of 538 documents

Precise measurement of the neutrino mixing parameter θ23 from muon neutrino disappearance in an off-axis beam

2014

New data from the T2K neutrino oscillation experiment produce the most precise measurement of the neutrino mixing parameter theta_{23}. Using an off-axis neutrino beam with a peak energy of 0.6 GeV and a data set corresponding to 6.57 x 10^{20} protons on target, T2K has fit the energy-dependent nu_mu oscillation probability to determine oscillation parameters. Marginalizing over the values of other oscillation parameters yields sin^2 (theta_{23}) = 0.514 +0.055/-0.056 (0.511 +- 0.055), assuming normal (inverted) mass hierarchy. The best-fit mass-squared splitting for normal hierarchy is Delta m^2_{32} = (2.51 +- 0.10) x 10^{-3} eV^2/c^4 (inverted hierarchy: Delta m^2_{13} = (2.48 +- 0.10) …

Particle physicsGeneral PhysicsPhysics MultidisciplinaryMODELSGeneral Physics and AstronomyFOS: Physical sciencesMASS01 natural sciences09 EngineeringHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)Physics and Astronomy (all)0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]SCATTERINGMuon neutrino010306 general physicsNeutrino oscillationDETECTORMixing (physics)01 Mathematical SciencesPhysicsNeutronsScience & Technology02 Physical Sciences010308 nuclear & particles physicsScatteringOscillationhep-exPhysicsFísicaT2K CollaborationPhysical SciencesSYMMETRIESHigh Energy Physics::ExperimentNeutrinoHigh energy physics Mixing Parameter estimation Parameter extractionConfidence limit Energy dependent Neutrino oscillations Off-axis neutrino beam Oscillation parameters Oscillation probabilities Precise measurements Statistical uncertaintyBeam (structure)Energy (signal processing)
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Symptomatic seizures in preterm newborns: A review on clinical features and prognosis

2018

Abstract Neonatal seizures are the most common neurological event in newborns, showing higher prevalence in preterm than in full-term infants. In the majority of cases they represent acute symptomatic phenomena, the main etiologies being intraventricular haemorrhage, hypoxic-ischemic encephalopathy, central nervous system infections and transient metabolic derangements. Current definition of neonatal seizures requires detection of paroxysmal EEG-changes, and in preterm newborns the incidence of electrographic-only seizures seems to be particularly high, further stressing the crucial role of electroencephalogram monitoring in this population. Imaging work-up includes an integration of serial…

Pediatricsmedicine.medical_specialtyPrognosiDevelopmental DisabilitiesPopulationEncephalopathyInfant Premature DiseasesReviewElectroencephalographyCerebral palsy03 medical and health sciencesEpilepsy0302 clinical medicineRisk FactorsSeizures030225 pediatricsmedicineNewborn; Outcome; Prognosis; Seizures; TreatmentHumanseducationNeurophysiological MonitoringUltrasonographyOutcomeeducation.field_of_studymedicine.diagnostic_testbusiness.industryInfant Newbornlcsh:RJ1-570BrainSymptomatic seizuresElectroencephalographylcsh:PediatricsGeneral MedicineOff-Label Usemedicine.diseaseNewbornPrognosisMagnetic Resonance ImagingNeurophysiological MonitoringSeizureTreatmentEtiologyAnticonvulsantsbusiness030217 neurology & neurosurgeryInfant Premature
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Confined crystallization of a HKUST-1 metal–organic framework within mesostructured silica with enhanced structural resistance towards water

2017

A HKUST-1 metal–organic framework was crystallized in the NH2-modified mesostructured silica FDU-12 in order to improve its structural stability upon water exposure. In-depth structural characterization studies of the designed composite confirmed successful formation of the MOF phase within the ordered spherical mesopores of the silica matrix. In spite of the confinement within the cavities, MOF exhibits full accessibility for the adsorbed gas molecules. In contrast to the bulk HKUST-1, which undergoes slow phase transition in a humid environment, the structural integrity of the HKUST-1 in the humid-protective matrix remains unchanged even after immersion and stirring in water at elevated t…

Phase transitionMaterials scienceRenewable Energy Sustainability and the EnvironmentComposite numberEngineering controlled terms: Crystalline materialsOrganometallicsStability Compendex keywords Confined crystallizationElevated temperatureMesostructured silicaMetal organic frameworkSpherical mesoporesStructural characterizationStructural resistanceStructural stabilities Engineering main heading: SilicaNanotechnology02 engineering and technologyGeneral Chemistry010402 general chemistry021001 nanoscience & nanotechnology01 natural sciences0104 chemical scienceslaw.inventionAdsorptionChemical engineeringlawPhase (matter)MoleculeGeneral Materials ScienceMetal-organic frameworkCrystallization0210 nano-technologyMesoporous material
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Ab initiosimulations of accretion disc instability

2003

We show that accretion disks, both in the subcritical and supercritical accretion rate regime, may exhibit significant amplitude luminosity oscillations. The luminosity time behavior has been obtained by performing a set of time-dependent 2D SPH simulations of accretion disks with different values of alpha and accretion rate. In this study, to avoid any influence of the initial disk configuration, we produced the disks injecting matter from an outer edge far from the central object. The period of oscillations is 2 - 50 s respectively for the two cases, and the variation amplitude of the disc luminosity is 10^38 - 10^39 erg/s. An explanation of this luminosity behavior is proposed in terms o…

PhysicsAstrophysics::High Energy Astrophysical PhenomenaAstrophysics (astro-ph)black hole physicsAb initioFOS: Physical sciencesAstronomy and AstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsRadiationAstrophysicsaccretion discsInstabilityLuminosityViscosityAmplitudeaccretionRadiation pressureinstabilitiesSpace and Planetary ScienceLimit cyclehydrodynamicsAstrophysics::Earth and Planetary AstrophysicsAstrophysics::Galaxy AstrophysicsMonthly Notices of the Royal Astronomical Society
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Nonlinear stability of relativistic sheared planar jets

2005

The linear and non-linear stability of sheared, relativistic planar jets is studied by means of linear stability analysis and numerical hydrodynamical simulations. Our results extend the previous Kelvin-Hemlholtz stability studies for relativistic, planar jets in the vortex sheet approximation performed by Perucho et al. (2004a,b) by including a shear layer between the jet and the external medium and more general perturbations. The models considered span a wide range of Lorentz factors ($2.5-20$) and internal energies ($0.08 c^2-60 c^2$) and are classified into three classes according to the main characteristics of their long-term, non-linear evolution. We observe a clear separation of thes…

PhysicsInternal energyLorentz transformationAstrophysics (astro-ph)FOS: Physical sciencesAstronomy and AstrophysicsMechanicsAstrophysicsGalaxies: jets ; Hydrodynamics ; InstabilitiesUNESCO::ASTRONOMÍA Y ASTROFÍSICAAstrophysicsKinetic energyWavelengthsymbols.namesakeLorentz factorAstrophysical jetMach numberSpace and Planetary ScienceInstabilitiesVortex sheetsymbolsHydrodynamicsjets [Galaxies]:ASTRONOMÍA Y ASTROFÍSICA [UNESCO]
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Coherent effects in the multimode dynamics of inhomogeneously broadened ring lasers

2004

We investigate under which conditions coherent effects manifest in the multimode dynamics of inhomogeneously broadened ring lasers. In particular, we demonstrate that for long enough cavities standard rate equations for class-B lasers fail in describing the multimode dynamics.

PhysicsLaser instabilities; Inhomogeneously broadened laser; Coherent effectsMulti-mode optical fiberCoherent effectsbusiness.industryDynamics (mechanics)Physics::OpticsRate equationLaserRing (chemistry)Atomic and Molecular Physics and OpticsElectronic Optical and Magnetic Materialslaw.inventionLaser instabilitiesOpticslawInhomogeneously broadened laserFiber laserElectrical and Electronic EngineeringPhysical and Theoretical Chemistrybusiness
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Structure analysis of the virtual Compton scattering amplitude at low energies

1998

We analyze virtual Compton scattering off the nucleon at low energies in a covariant, model-independent formalism. We define a set of invariant functions which, once the irregular nucleon pole terms have been subtracted in a gauge-invariant fashion, is free of poles and kinematical zeros. The covariant treatment naturally allows one to implement the constraints due to Lorentz and gauge invariance, crossing symmetry, and the discrete symmetries. In particular, when applied to the $ep\to e'p'\gamma$ reaction, charge-conjugation symmetry in combination with nucleon crossing generates four relations among the ten originally proposed generalized polarizabilities of the nucleon.

PhysicsNuclear and High Energy PhysicsPhotonNuclear TheoryLorentz transformationCrossingNuclear TheoryCompton scatteringFOS: Physical sciencesPROTONNuclear Theory (nucl-th)symbols.namesakeHigh Energy Physics - PhenomenologyAmplitudeHigh Energy Physics - Phenomenology (hep-ph)Quantum mechanicsPIONsymbolsCovariant transformationGauge theoryNucleonNUCLEONNuclear Experiment3RD-ORDER SPIN POLARIZABILITIES
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Predictions of covariant chiral perturbation theory for nucleon polarisabilities and polarised Compton scattering

2015

We update the predictions of the SU(2) baryon chiral perturbation theory for the dipole polarisabilities of the proton, $\{\alpha_{E1},\,\beta_{M1}\}_p=\{11.2(0.7),\,3.9(0.7)\}\times10^{-4}$fm$^3$, and obtain the corresponding predictions for the quadrupole, dispersive, and spin polarisabilities: $\{\alpha_{E2},\,\beta_{M2}\}_p=\{17.3(3.9),\,-15.5(3.5)\}\times10^{-4}$fm$^5$, $\{\alpha_{E1\nu},\,\beta_{M1\nu}\}_p=\{-1.3(1.0),\,7.1(2.5)\}\times10^{-4}$fm$^5$, and $\{\gamma_{E1E1},\,\gamma_{M1M1},\,\gamma_{E1M2},\,\gamma_{M1E2}\}_p=\{-3.3(0.8),\,2.9(1.5),\,0.2(0.2),\,1.1(0.3)\}\times10^{-4}$fm$^4$. The results for the scalar polarisabilities are in significant disagreement with semi-empirical …

PhysicsParticle physicsChiral perturbation theoryNuclear TheoryPhysics and Astronomy (miscellaneous)ProtonFOS: Physical sciencesCompton scattering Protons and neutron polarisabilitiesNuclear Theory (nucl-th)BaryonHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)PionProduction (computer science)Sensitivity (control systems)Sum rule in quantum mechanicsNucleonEngineering (miscellaneous)The European Physical Journal C
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Measurements of Double-Polarized Compton Scattering Asymmetries and Extraction of the Proton Spin Polarizabilities

2015

The spin polarizabilities of the nucleon describe how the spin of the nucleon responds to an incident polarized photon. The most model-independent way to measure the nucleon spin polarizabilities is through polarized Compton scattering. Double-polarized Compton scattering asymmetries on the proton were measured in the $\Delta(1232)$ region using circularly polarized incident photons and a transversely polarized proton target at the Mainz Microtron. Fits to asymmetry data were performed using a dispersion model calculation and a baryon chiral perturbation theory calculation, and a separation of all four proton spin polarizabilities in the multipole basis was achieved. The analysis based on a…

PhysicsPhotonProtonNuclear TheoryCompton scatteringGeneral Physics and AstronomyFOS: Physical sciences7. Clean energy3. Good healthBaryonNuclear physicsProton spin crisisspin polarizabilities; nucleon; photon; ∆(1232) region; MAMINuclear Experiment (nucl-ex)NucleonNuclear ExperimentMicrotronNuclear ExperimentSpin-½
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Semi-global simulations of the magneto-rotational instability in core collapse supernovae

2009

Possible effects of magnetic fields in core collapse supernovae rely on an efficient amplification of the weak pre-collapse fields. It has been suggested that the magneto-rotational instability (MRI) leads to rapid field growth. Although MRI studies exist for accretion discs, the application of their results to core collapse supernovae is inhibited as the physics of supernova cores is substantially different from that of accretion discs. We address the problem of growth and saturation of the MRI by means of semi-global simulations, which combine elements of global and local simulations by taking the presence of global background gradients into account and using a local computational grid. W…

PhysicsResistive touchscreenMagnetohydrodynamics (MHD):ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia::Otras [UNESCO]Astrophysics (astro-ph)supernovae : general [Stars]magnetic fields [Stars]FOS: Physical sciencesAstronomy and AstrophysicsAngular velocityMechanicsAstrophysicsMagnetohydrodynamics (MHD); Instabilities; Stars : supernovae : general; Stars : magnetic fieldsAstrophysicsInstabilityMagnetic fieldSupernovaAmplitudeSpace and Planetary ScienceDispersion relationInstabilitiesUNESCO::ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia::OtrasUNESCO::ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia::EstrellasSaturation (chemistry):ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia::Estrellas [UNESCO]
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