Search results for "nuclear physics"

showing 10 items of 5307 documents

Quadrupole interaction of $^{8}$Li and $^{9}$Li in LiNbO$_{3}$ and the quadrupole moment of $^{9}$Li

1988

The quadrupole interaction of nuclear spin polarized8Li (I=2) and9Li (I=3/2) in LiNbO3 has been studied at room temperature. The polarization was achieved by optical pumping of a fast atomic beam with circularly polarized laser light. The atoms were implanted into a hexagonal LiNbO3 single crystal and the quadrupole splitting ofβ-NMR spectra was measured. A ratio of ¦Q(9Li)/Q(8Li)¦=0.88(4) for the nuclear quadrupole moments was deduced, yielding a new value of ¦Q(9Li)¦=25.3 (9) mb for the quadrupole moment of9Li.

Nuclear and High Energy PhysicsChemistryIsotopes of lithiumNuclear TheoryPhysics::OpticsQuadrupole splittingSpectral lineOptical pumpingQuadrupolePhysics::Accelerator PhysicsNuclear fusionNuclear Physics - ExperimentPhysics::Atomic PhysicsAtomic physicsQuadrupole mass analyzerSingle crystal
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Nuclear moments and laser spectroscopy

1990

Laser spectroscopy measurements have yielded a wealth of new information about the moments and charge radii of unstable isotopes. The procedures of evaluating these moments from the magnetic dipole and electric quadrupole terms of the hyperfine structure arew discussed. Examples are presented, with emphasis on the isotopic chains of odd-proton nuclei, and their essential features are put into the context of current theoretical model descriptions for spherical and deformed nuclei. Finally, new developments of extremely sensitive experimental techniques are discussed with regard to an application to nuclei very far from stability.

Nuclear and High Energy PhysicsChemistryNuclear TheoryCharge (physics)Context (language use)Condensed Matter PhysicsAtomic and Molecular Physics and OpticsQuadrupoleNuclear Physics - ExperimentPhysics::Atomic PhysicsPhysical and Theoretical ChemistryAtomic physicsNuclear ExperimentSpectroscopyMagnetic dipoleHyperfine structureHyperfine Interactions
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How to measure nuclear ground-state properties in simple systems such as 11Li or U91+?

2008

Abstract Atomic spectroscopy yields key information on properties of ground and isomeric states via a determination of the hyperfine structure and isotope shift. In order to deduce precise nuclear moments and charge radii, the electromagnetic fields produced by the electrons at the site of the nucleus must be known with high accuracy. This is presently possible only for simple systems with very few electrons. This contribution describes two scenarios for such experiments: the determination of the charge radius of the neutron-rich isotopes 8,9Li and of the halo nucleus 11Li at the on-line isotope separators at GSI and TRIUMF and the Highly charged Ion TRAP (HITRAP) facility which is under co…

Nuclear and High Energy PhysicsChemistryNuclear TheoryHighly charged ionHalo nucleusElectronAtomic spectroscopyIonNuclear physicsCharge radiusPhysics::Atomic PhysicsAtomic physicsNuclear ExperimentGround stateInstrumentationHyperfine structureNuclear Instruments and Methods in Physics Research Section B: Beam Interactions with Materials and Atoms
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Towards on-line production of N=Z94Ag at IGISOL

2008

Abstract A future study of the ground state and low-lying isomeric states of 94 Ag and 96 Ag at the Ion Guide Isotope Separator On-Line (IGISOL) facility, University of Jyvaskyla, requires the development of a low-energy beam of neutron-deficient silver. In order to attain the highest possible extraction efficiencies the coupling of a hot cavity graphite catcher device to the IGISOL mass-separator is planned. A heavy-ion fusion-evaporation reaction will produce the silver recoils which will be captured in the graphite catcher. Resonant laser ionization techniques will be applied to efficiently and selectively ionize the evaporated silver atoms. A simulation program has been written to study…

Nuclear and High Energy PhysicsChemistrySeparator (oil production)LaserIonlaw.inventionNuclear physicslawIonizationPhysics::Atomic and Molecular ClustersThermal emittancePhysics::Atomic PhysicsGraphiteAtomic physicsNuclear ExperimentGround stateInstrumentationBeam (structure)Nuclear Instruments and Methods in Physics Research Section B: Beam Interactions with Materials and Atoms
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Measurement of the neutrino-oxygen neutral-current interaction cross section by observing nuclear deexcitation gamma rays

2014

We report the first measurement of the neutrino-oxygen neutral-current quasielastic (NCQE) cross section. It is obtained by observing nuclear deexcitation $\gamma$-rays which follow neutrino-oxygen interactions at the Super-Kamiokande water Cherenkov detector. We use T2K data corresponding to $3.01 \times 10^{20}$ protons on target. By selecting only events during the T2K beam window and with well-reconstructed vertices in the fiducial volume, the large background rate from natural radioactivity is dramatically reduced. We observe 43 events in the $4-30$ MeV reconstructed energy window, compared with an expectation of 51.0, which includes an estimated 16.2 background events. The background …

Nuclear and High Energy PhysicsCherenkov detectorPhysics::Instrumentation and DetectorsC-12FOS: Physical sciencesAstronomy & Astrophysicslaw.inventionHigh Energy Physics - ExperimentPhysics Particles & FieldsNuclear physicsSUPER-KAMIOKANDE DETECTORCross section (physics)High Energy Physics - Experiment (hep-ex)lawEXCITATIONABSORPTION[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]SCATTERINGO-16Nuclear ExperimentPhysicsCALIBRATIONScience & TechnologyNeutral currenthep-exPhysicsGamma rayT2K experimentFísica3. Good healthPhysical SciencesNeutrinoWEAKFiducial markerBeam (structure)
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The experience of building and operating COMPASS RICH-1

2010

COMPASS RICH-1 is a large size gaseous Imaging Cherenkov Detector providing hadron identification in the range from 3 to 55 GeV/c, in the wide acceptance spectrometer of the COMPASS Experiment at CERN SPS. It uses a 3 m long C(4)F(10) radiator, a 21 m(2) large VUV mirror surface and two kinds of photon detectors: MAPMTs and MWPCs with CsI photocathodes, covering a total of 5.5 m(2). It is in operation since 2002 and its performance has increased in time thanks to progressive optimization and mostly to a major upgrade which was implemented in 2006. The main characteristics of COMPASS RICH-1 components are described and some specific aspects related to the radiator gas system, the mirror alig…

Nuclear and High Energy PhysicsCherenkov detectorPhysics::Instrumentation and Detectors[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]COMPASS01 natural sciencesParticle identificationParticle identificationlaw.inventionNuclear physicsCOMPASS; CsI; MAPMT; Photon detection; PID; RICH; Instrumentation; Nuclear and High Energy PhysicsOpticslawCompass0103 physical sciencesCOMPASS experimentCsI photoconverter010306 general physicsRICHInstrumentationEvent reconstructionPhysicsLarge Hadron ColliderSpectrometer010308 nuclear & particles physicsbusiness.industryPIDUpgradePhoton detectionMAPMTCsIParticle identification; COMPASS; RICH; MAPMT; CsI photoconverterHigh Energy Physics::Experimentbusiness
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Higher order forward spin polarizability

2010

As a guideline for future experiments to extract the four (leading) spin polarizabilities of the nucleon, we have constructed the forward amplitude for polarized Compton scattering by dispersion integrals. These integrals have been saturated by recently measured helicity-dependent photoabsorption cross sections as well as predictions for pion photoproduction multipoles from several phenomenological descriptions and chiral perturbation theory. The comparison of these results corroborates the strategy to extract the spin polarizabilities by fitting them to polarized Compton data and fixing all higher order spin effects by dispersion relations based on pion photoproduction multipoles.

Nuclear and High Energy PhysicsChiral perturbation theoryNuclear Theorynucl-thNuclear TheoryFOS: Physical sciencesNucleon spin structurenucl-ex01 natural sciencesHigh Energy Physics - ExperimentNuclear physicsNuclear Theory (nucl-th)High Energy Physics - Experiment (hep-ex)PionHigh Energy Physics - Phenomenology (hep-ph)PolarizabilityDispersion relation0103 physical sciencesNuclear Experiment (nucl-ex)010306 general physicsNuclear ExperimentNuclear ExperimentSpin-½Physics010308 nuclear & particles physicshep-exCompton scatteringhep-phHigh Energy Physics - PhenomenologyQuantum electrodynamicsNucleon
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Measurement of the radiative K-e3 branching ratio

2005

We present a measurement of the relative branching ratio of the decay KL -> pi e nu gamma (Ke3gamma) with respect to KL-> pi e nu (gamma) (Ke3+Ke3gamma) decay. The result is based on observation of 19 000 Ke3gamma and 5.6 x 10^6 Ke3 decays. The value of the branching ratio is Br(Ke3gamma, Egamma^*>30 MeV,theta(e,gamma)^*>20^o)/Br(Ke3)= (0.964+-0.008+0.011-0.009)%. This result agrees with theoretical predictions but is at variance with a recently published result.

Nuclear and High Energy PhysicsChiral perturbation theoryPhotonHadronFOS: Physical scienceskaon decay; NEUTRAL KAON; branching ratio7. Clean energy01 natural sciencesNEUTRAL KAONHigh Energy Physics - ExperimentNuclear physicsmesoni KHigh Energy Physics - Experiment (hep-ex)0103 physical sciencesRadiative transfer[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]radiative kaon decays010306 general physicsmesoni K; decadimenti radiativiPhysics010308 nuclear & particles physicsBranching fractionK13 DECAYSBremsstrahlungkaon decayAmplitudedecadimenti radiativibranching ratioAtomic physicsParticle Physics - Experiment
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Proton-air cross section measurement with the ARGO-YBJ cosmic ray experiment

2009

The proton-air cross section in the energy range 1-100 TeV has been measured by the ARGO-YBJ cosmic ray experiment. The analysis is based on the flux attenuation for different atmospheric depths (i.e. zenith angles) and exploits the detector capabilities of selecting the shower development stage by means of hit multiplicity, density and lateral profile measurements at ground. The effects of shower fluctuations, the contribution of heavier primaries and the uncertainties of the hadronic interaction models, have been taken into account. The results have been used to estimate the total proton-proton cross section at center of mass energies between 70 and 500 GeV, where no accelerator data are …

Nuclear and High Energy PhysicsCosmic rays Proton-air cross section gamma astronomyProtonAstrophysics::High Energy Astrophysical PhenomenaHadronCosmic rayCross Section01 natural sciencesCosmic RayHigh Energy Physics - ExperimentNuclear physics0103 physical sciencesMultiplicity (chemistry)010306 general physicsNuclear ExperimentZenithArgoPhysics010308 nuclear & particles physicsAttenuationDetectorSettore FIS/01 - Fisica SperimentaleAstrophysics::Instrumentation and Methods for Astrophysics3. Good healthHadronic InteractionHigh Energy Physics::ExperimentExtensive Air Showers
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Study of the electromagnetic background in the XENON100 experiment

2011

The XENON100 experiment, located at the Laboratori Nazionali del Gran Sasso (LNGS), aims to directly detect dark matter in the form of Weakly Interacting Massive Particles (WIMPs) via their elastic scattering off xenon nuclei. We present a comprehensive study of the predicted electronic recoil background coming from radioactive decays inside the detector and shield materials, and intrinsic contamination. Based on GEANT4 Monte Carlo simulations using a detailed geometry together with the measured radioactivity of all detector components, we predict an electronic recoil background in the WIMP-search energy range (0-100 keV) in the 30 kg fiducial mass of less than 10e-2 events/(kg-day-keV), co…

Nuclear and High Energy PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)[PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Physics::Instrumentation and DetectorsMonte Carlo methodDark matterchemistry.chemical_elementFOS: Physical sciences01 natural sciences7. Clean energyParticle detectorNuclear physicsXenonRecoil0103 physical sciences010306 general physicsNuclear ExperimentInstrumentation and Methods for Astrophysics (astro-ph.IM)PhysicsElastic scattering010308 nuclear & particles physicsDetectorAstrophysics::Instrumentation and Methods for Astrophysics[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]chemistryHigh Energy Physics::ExperimentAstrophysics - Instrumentation and Methods for AstrophysicsRadioactive decayAstrophysics - Cosmology and Nongalactic Astrophysics
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