Search results for "LABOR"

showing 10 items of 3876 documents

Astrophysics and spectroscopy with microcalorimeters on an electron beam ion trap

2003

The importance of the combination of electron beam ion trap (EBIT) spectroscopy with X-ray microcalorimeters in the field of astrophysics was discussed. X-ray astronomy involves heavily charged ion instruments , especially EBIT, to obtain improved quality atomic data. In this regard, the research program at the National Institute of Standards and Technology, which uses X-ray spectroscopic methods to study plasma and atomic physics, was also discussed.

PhysicsNuclear and High Energy PhysicsAstrophysics::Instrumentation and Methods for AstrophysicsX-rayHighly charged ionSurfaces Coatings and FilmFizikai tudományokSurfaces and InterfacesPlasmaAstrophysicsHighly charged ionIonX-rayNuclear physicsSettore FIS/05 - Astronomia E AstrofisicaTermészettudományokMicrocalorimeterIonizationCathode rayAtomic physicsLaboratory astrophysicSpectroscopyElectron beam ion trapInstrumentationElectron beam ion trapNuclear Instruments and Methods in Physics Research Section B: Beam Interactions with Materials and Atoms
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Results of the search for neutrinoless double-βdecay inMo100with the NEMO-3 experiment

2015

The NEMO-3 detector, which had been operating in the Modane Underground Laboratory from 2003 to 2010, was designed to search for neutrinoless double $\beta$ ($0\nu\beta\beta$) decay. We report final results of a search for $0\nu\beta\beta$ decays with $6.914$ kg of $^{100}$Mo using the entire NEMO-3 data set with a detector live time of $4.96$ yr, which corresponds to an exposure of 34.3 kg$\cdot$yr. We perform a detailed study of the expected background in the $0\nu\beta\beta$ signal region and find no evidence of $0\nu\beta\beta$ decays in the data. The level of observed background in the $0\nu\beta\beta$ signal region $[2.8-3.2]$ MeV is $0.44 \pm 0.13$ counts/yr/kg, and no events are obs…

PhysicsNuclear and High Energy PhysicsParticle physics010308 nuclear & particles physicsSignal region01 natural sciencesBeta decayLower limitNuclear physicsMAJORANADouble beta decay0103 physical sciencesUnderground laboratoryBeta (velocity)Neutrino010306 general physicsPhysical Review D
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Is it possible to determine the S-factor of the hep process from a laboratory experiment?

2000

We discuss the problem of solar hep neutrinos originating from the reaction p + 3He -> 4He + e+ + nu and obtain a relation between the astrophysical S-factor of the hep process and the cross section of the process e- + 4He -> 3H + n + nu near threshold. The relation is based on the isotopic invariance of strong interactions. The measurement of the latter cross section would allow to obtain experimental information on S(hep), the value of which, at the moment, is known only from theoretical calculations.

PhysicsNuclear and High Energy PhysicsParticle physicsNuclear TheoryS-factorAstrophysics (astro-ph)FOS: Physical sciencesValue (computer science)FísicaAstrophysicsNuclear Theory (nucl-th)Moment (mathematics)Near thresholdCross section (physics)High Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Laboratory experimentNeutrino
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Reactor neutrino background at the proposed LAGUNA sites

2012

Abstract The electron antineutrino background from reactors is estimated in proposed LAGUNA sites using commercial fission reactors operational in 2009. Calculations are made for an input to background studies like e.g. geoneutrino measurement uncertainty estimation.

PhysicsNuclear physicsNuclear and High Energy PhysicsParticle physicsFissionGeoneutrinoUnderground laboratoryMeasurement uncertaintyReactor neutrinoNeutrino oscillationElectron neutrinoAtomic and Molecular Physics and OpticsNuclear Physics B - Proceedings Supplements
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Initial nucleon structure results with chiral quarks at the physical point

2014

We report initial nucleon structure results computed on lattices with 2+1 dynamical M\"obius domain wall fermions at the physical point generated by the RBC and UKQCD collaborations. At this stage, we evaluate only connected quark contributions. In particular, we discuss the nucleon vector and axial-vector form factors, nucleon axial charge and the isovector quark momentum fraction. From currently available statistics, we estimate the stochastic accuracy of the determination of $g_A$ and $_{u-d}$ to be around 10%, and we expect to reduce that to 5% within the next year. To reduce the computational cost of our calculations, we extensively use acceleration techniques such as low-eigenmode def…

PhysicsNuclear physicsPhysical pointHigh Energy Physics - LatticeHigh Energy Physics::LatticeNuclear TheoryHigh Energy Physics - Lattice (hep-lat)FOS: Physical sciencesddc:530National laboratory
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Role of excitons in double Raman resonances in GaAs quantum wells

1996

Raman scattering by longitudinal-optical phonons has been measured in GaAs-AlAs multiple quantum wells at high magnetic fields. Doubly resonant scattering processes are observed at photon energies corresponding to magneto-excitons with different principal quantum numbers for the incoming and outgoing channels. The existence of these initially forbidden scattering processes, their resonance energies, and their relative intensities are correctly reproduced by our theoretical description. The model takes into account the excitonic nature of the intermediate states, as well as scattering processes involving a nonzero in-plane phonon wave vector, which is required to allow inter-Landau level sca…

PhysicsPhonon scatteringCondensed matter physicsCondensed Matter::OtherScatteringScattering lengthCorrelated Electron Systems / High Field Magnet Laboratory (HFML)02 engineering and technologyCondensed Matter::Mesoscopic Systems and Quantum Hall Effect021001 nanoscience & nanotechnology01 natural sciencesScattering amplitudeCondensed Matter::Materials Sciencesymbols.namesakeX-ray Raman scattering0103 physical sciencesPrincipal quantum numbersymbolsScattering theoryAtomic physics010306 general physics0210 nano-technologyGeneralLiterature_REFERENCE(e.g.dictionariesencyclopediasglossaries)Raman scatteringPhysical Review B
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Soft X-Ray Irradiation of Methanol Ice: Implication for H2CO Formation in Interstellar Regions

2010

We performed 0.3 keV soft X-ray irradiation of a methanol ice at 8 K under ultra-high vacuum conditions. To the best of our knowledge, this is the first time that soft X-rays are used to study photolysis of ice analogs. Despite the low irradiation dose of 10{sup -6} photons molecule{sup -1}, the formation of formaldehyde has been observed. The results of our experiments suggest that X-rays may be a promising candidate to the formation of complex molecules in regions where UV radiation is severely inhibited.

PhysicsPhotodissociationFormaldehydeAstronomy and AstrophysicsRadiationPhotochemistryChemical reactionDecompositionchemistry.chemical_compoundISM: molecules – methods: laboratory – X-rays: ISMSettore FIS/05 - Astronomia E AstrofisicachemistrySpace and Planetary ScienceMoleculeIrradiationMethanolAtomic physics
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Target thickness dependence of the Be(p,xn) neutron energy spectrum

2014

We report on the current status of the analysis of an experiment performed at The Svedberg Laboratory, with the aim of investigating the produced neutron field by Be(p,xn) converters of three different thicknesses with a 30 MeV proton beam. The neutron energy spectra were measured with the Time of Flight technique using a BC-501 liquid scintillator with good n-γ Pulse Shape Discrimination properties, while the detected events were recorded simultaneously by two Data AcQuisition systems. In this paper, we present the experimental setup, the analysis technique and some preliminary results.  AlFONS

PhysicsProtonPhysicsQC1-999neutronsScintillatorThe Svedberg LaboratoryNeutron temperatureSpectral linespectrumNuclear physicsSubatomär fysikData acquisitionnuclear physicsSubatomic PhysicsNeutronBeam (structure)energy
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An investigation of environmental temperature effects on energy exchange by thermal radiation

2013

The radiative heating or cooling of a body placed in an environment, whose temperature is considered constant is described by Stefan's law. In this paper, an analysis is made of how a time-dependent environmental temperature influences the heating/cooling process. We compare experimental results for a resistor first heated by the Joule effect inside a glass vacuum tube and then cooled under two different conditions: in a bath at a constant temperature and in air. We also discuss a model that describes how the time-dependent tube temperature influences the radiative resistor cooling by identifying the properties of the environment that make the resistor cooling rate linear.

PhysicsRadiative coolingSettore FIS/08 - Didattica E Storia Della FisicaJoule effectVacuum tubeGeneral Physics and AstronomyThermodynamicsMechanicslaw.inventionThermal radiationlawRadiative transferLaboratory procedures Thermal radiation Physics educationTube (fluid conveyance)ResistorConstant (mathematics)American Journal of Physics
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A laboratory experiment on inferring Poiseuille's law for undergraduate students

2006

In this paper a laboratory experiment is proposed to infer Poiseuille's law. A simple set-up based on two flasks joined by a detachable tube allows one to measure using tubes of different radii and different lengths. One of the flasks is connected to a vacuum pump to control the pressure differential between the tube extremes. The influence on the flow of different radii, lengths, pressures and viscosities can be studied in a didactic way by measuring the flow rate for each of these variables. The experiment can be performed getting together the students in groups, so that each group concentrates on the effect on the flow of a specific variable, leaving the rest fixed. After putting togethe…

PhysicsRest (physics)Laboratory flaskFlow (mathematics)LawGeneral Physics and AstronomyVacuum pumpTube (container)Hagen–Poiseuille equationMeasure (mathematics)law.inventionVolumetric flow rateEuropean Journal of Physics
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