Search results for "nuclear physics"

showing 10 items of 5307 documents

Evidence for anI=1 isomeric state in96Rb

1981

Aβ-RADOP (β-Radiation Detected Optical Pumping) experiment on the short lived (T1/2=203 ms)96Rb isotope has been performed at the on line mass separator for fission produced alkali isotopes at the TRIGA reactor in Mainz. Irradiation of r.f. onto the polarized sample to induce Zeeman transitions resulted in two signals for nuclear spinsI=2 andI=1. The previously undetermined component withI=1 is interpreted as evidence for an isomeric state in96Rb.

Nuclear and High Energy PhysicsZeeman effectIsotopeFissionChemistryRadiochemistryAlkali metalTRIGANuclear physicsOptical pumpingsymbols.namesakesymbolsNuclear fusionIrradiationZeitschrift f�r Physik A: Atoms and Nuclei
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Evaluation of the magnetic moments of radium isotopes

1990

Using the relativistic linked cluster many-body perturbation procedure we have obtained the hyperfine field at the nucleus of the Ra+ ion in the2S1/2 ground state. There is good agreement between the calculated magnetic moment of213Ra and the results of a recent Zeeman measurement by the collinear laser beam technique. Detailed comparison is carried out between our result and earlier ones.

Nuclear and High Energy PhysicsZeeman effectNeutron magnetic momentIsotopeMagnetic momentChemistryCondensed Matter PhysicsElectron magnetic dipole momentAtomic and Molecular Physics and OpticsIonNuclear physicssymbols.namesakesymbolsPhysics::Atomic PhysicsPhysical and Theoretical ChemistryAtomic physicsGround stateHyperfine structureHyperfine Interactions
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Journal of High Energy Physics

2014

The Double Chooz experiment presents improved measurements of the neutrino mixing angle $\theta_{13}$ using the data collected in 467.90 live days from a detector positioned at an average distance of 1050 m from two reactor cores at the Chooz nuclear power plant. Several novel techniques have been developed to achieve significant reductions of the backgrounds and systematic uncertainties with respect to previous publications, whereas the efficiency of the $\bar\nu_{e}$ signal has increased. The value of $\theta_{13}$ is measured to be $\sin^{2}2\theta_{13} = 0.090 ^{+0.032}_{-0.029}$ from a fit to the observed energy spectrum. Deviations from the reactor $\bar\nu_{e}$ prediction observed ab…

Nuclear and High Energy Physics[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Physics - Instrumentation and DetectorsNeutrino Detectors and TelescopeFOS: Physical sciencesCHOOZ7. Clean energy01 natural sciencesHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)ExperimentDistortion0103 physical sciencesEnergy spectrum[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]High Energy Physics[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsMixing (physics)PhysicsNeutrino Detectors and Telescopes010308 nuclear & particles physicsOscillationPhysics[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]DetectorFunction (mathematics)Instrumentation and Detectors (physics.ins-det)OscillationNeutrinoInstrumentation and Detectors
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Measurements of forward proton production with incident protons and charged pions on nuclear targets at the CERN Proton Synchroton

2010

Measurements of the double-differential proton production cross-section d(2 sigma)/dpd Omega in the range of momentum 0.5 GeV/c <= p < 8.0 GeV/c and angle 0.05 rad <= theta < 0.25 rad in collisions of charged pions and protons on beryllium, carbon, aluminium, copper, tin, tantalum, and lead are presented. The data were taken with the large acceptance HARP detector in the T9 beam line of the CERN Proton Synchrotron. Incident particles were identified by an elaborate system of beam detectors and impinged on a target of 5% of a nuclear interaction length. The tracking and identification of the produced particles was performed using the forward spectrometer of the HARP experiment. Results are o…

Nuclear and High Energy Physics[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Physics::Instrumentation and Detectorsproton; nuclear targets; charged pionsFOS: Physical sciencesddc:500.201 natural sciencesHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)Basic research0103 physical sciencesCERN[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]010306 general physicsNuclear ExperimentInelastic proton scatteringPhysicsLarge Hadron Collider010308 nuclear & particles physicsOther reactions above meson production thresholds[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]FísicaPion-induced reactionsnuclear targetsResearch councilcharged pionsnuclear targetPhysics::Accelerator PhysicsHARP ExperimentHigh Energy Physics::ExperimentHumanitiesHARP Experiment; CERNParticle Physics - Experimentproton
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Measurement of the energy spectrum of cosmic rays above 10^18 eV using the Pierre Auger Observatory

2010

We report a measurement of the flux of cosmic rays with unprecedented precision and Statistics using the Pierre Auger Observatory Based on fluorescence observations in coincidence with at least one Surface detector we derive a spectrum for energies above 10(18) eV We also update the previously published energy spectrum obtained with the surface detector array The two spectra are combined addressing the systematic uncertainties and, in particular. the influence of the energy resolution on the spectral shape The spectrum can be described by a broken power law E-gamma with index gamma = 3 3 below the ankle which is measured at log(10)(E-ankle/eV) = 18 6 Above the ankle the spectrum is describe…

Nuclear and High Energy Physics[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Radiación CósmicaAstronomyAstrophysics::High Energy Astrophysical Phenomenaenergy spectrumFluxFOS: Physical sciencesCosmic rayAstrophysicsElectronSURFACE DETECTORUPPER LIMITENERGIAPHOTON FRACTION01 natural sciencesSpectral lineAugerNuclear physicscosmic raysObservatorySHOWERS0103 physical sciencesHigh-Energy Cosmic Ray010306 general physicsCosmic raysCiencias ExactasPhysicsPierre Auger ObservatoryHigh Energy Astrophysical Phenomena (astro-ph.HE)010308 nuclear & particles physicsPhysics[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Spectral densityFísicaPierre Auger ObservatoryCosmic rayELECTRONS3. Good healthPierre Auger Observatory; Cosmic rays; Energy spectrumSIMULATIONExperimental High Energy PhysicsComputingMethodologies_DOCUMENTANDTEXTPROCESSINGFluorescenciaARRAYFísica nuclearEnergy spectrumAstrophysics - High Energy Astrophysical PhenomenaSYSTEM
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Response of the XENON100 dark matter detector to nuclear recoils

2013

Results from the nuclear recoil calibration of the XENON100 dark matter detector installed underground at the Laboratori Nazionali del Gran Sasso (LNGS), Italy are presented. Data from measurements with an external 241AmBe neutron source are compared with a detailed Monte Carlo simulation which is used to extract the energy dependent charge-yield Qy and relative scintillation efficiency Leff. A very good level of absolute spectral matching is achieved in both observable signal channels - scintillation S1 and ionization S2 - along with agreement in the 2-dimensional particle discrimination space. The results confirm the validity of the derived signal acceptance in earlier reported dark matte…

Nuclear and High Energy Physics[PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Cosmology and Nongalactic Astrophysics (astro-ph.CO)[SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]Physics::Instrumentation and DetectorsMonte Carlo methodDark matterFOS: Physical sciences01 natural sciencesdark matterParticle detectorNuclear physics[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]RecoilIonization0103 physical sciences010306 general physicsNuclear ExperimentInstrumentation and Methods for Astrophysics (astro-ph.IM)PhysicsScintillation010308 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]Neutron sourceAstrophysics - Instrumentation and Methods for AstrophysicsAstrophysics - Cosmology and Nongalactic Astrophysics
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Measurement of the b hadron lifetime with the dipole method

1993

A measurement of the average lifetime of b hadrons has been performed with the dipole method on a sample of 260000 hadronic Z decays recorded with the ALEPH detector during 1991. The dipole is the distance between the vertices built in the opposite hemispheres. The mean dipole is extracted from all the events without attempting b enrichment. Comparing the average of the data dipole distribution with a Monte Carlo calibration curve obtained with different b lifetimes, an average b hadron lifetime of 1.51 +/- 0.08 ps is extracted. RI ANTONELLI, ANTONELLA/C-6238-2011; Buttar, Craig/D-3706-2011; Stahl, Achim/E-8846-2011; Passalacqua, Luca/F-5127-2011; Murtas, Fabrizio/B-5729-2012; St.Denis, Ric…

Nuclear and High Energy Physics[PHYS.HEXP] Physics [physics]/High Energy Physics - Experiment [hep-ex]Calibration curveElectron–positron annihilationMonte Carlo methodHadronElementary particleDiscrete dipole approximation01 natural sciencesinformationNuclear physicsALEPH Experiment0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]mutualisation.010306 general physicsALEPH experimentPhysics010308 nuclear & particles physicsPhysicsmediologyterritoryDipoleHigh Energy Physics::Experimentterritorial intelligenceParticle Physics - Experiment
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High-resolution laser spectroscopy with the Collinear Resonance Ionisation Spectroscopy (CRIS) experiment at CERN-ISOLDE

2016

The Collinear Resonance Ionisation Spectroscopy (CRIS) experiment at CERN has achieved high-resolution resonance ionisation laser spectroscopy with a full width at half maximum linewidth of 20(1) MHz for 219;221Fr, and has measured isotopes as short lived as 5 ms with 214Fr. This development allows for greater precision in the study of hyperfine structures and isotope shifts, as well as a higher selectivity of singleisotope, even single-isomer, beams. These achievements are linked with the development of a new laser laboratory and new data-acquisition systems. publisher: Elsevier articletitle: High-resolution laser spectroscopy with the Collinear Resonance Ionisation Spectroscopy (CRIS) exp…

Nuclear and High Energy Physics[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]7. Clean energy01 natural scienceslaw.inventionLaser linewidthlawIonization0103 physical sciencesNuclear Physics - ExperimentLaser spectroscopy010306 general physicsSpectroscopyInstrumentationHyperfine structureLarge Hadron Collider010308 nuclear & particles physicsChemistryData acquisitionResonanceLaserIon beam purificationIsotope shiftFull width at half maximumHyperfine structureAtomic physicsNuclear Instruments and Methods in Physics Research Section B: Beam Interactions with Materials and Atoms
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Collectivity in the light radon nuclei measured directly via Coulomb excitation

2015

Background: Shape coexistence in heavy nuclei poses a strong challenge to state-of-the-art nuclear models, where several competing shape minima are found close to the ground state. A classic region for investigating this phenomenon is in the region around Z=82 and the neutron midshell at N=104. Purpose: Evidence for shape coexistence has been inferred from α-decay measurements, laser spectroscopy, and in-beam measurements. While the latter allow the pattern of excited states and rotational band structures to be mapped out, a detailed understanding of shape coexistence can only come from measurements of electromagnetic matrix elements. Method: Secondary, radioactive ion beams of Rn202 and Rn…

Nuclear and High Energy Physics[PHYS.NUCL]Physics [physics]/Nuclear Theory [nucl-th]PopulationFOS: Physical sciencesCoulomb excitationshape coexistence01 natural sciences0103 physical sciencesNuclear Physics - ExperimentNeutroncollectivityNuclear Experiment (nucl-ex)010306 general physicseducationSpectroscopyNuclear ExperimentPhysicseducation.field_of_studyta114010308 nuclear & particles physicsGamma rayradonPhysique atomique et nucléaire3. Good healthRadonExcited stateQuadrupoleAtomic physicsGround state
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Properties of nuclei in the nobelium region studied within the covariant, Skyrme, and Gogny energy density functionals

2015

We calculate properties of the ground and excited states of nuclei in the nobelium region for proton and neutron numbers of 92 &lt;= Z &lt;= 104 and 144 &lt;= N &lt;= 156, respectively. We use three different energy-density-functional (EDF) approaches, based on covariant, Skyrme, and Gogny functionals, each within two different parameter sets. A comparative analysis of the results obtained for odd-even mass staggerings, quasiparticle spectra, and moments of inertia allows us to identify single-particle and shell effects that are characteristic to these different models and to illustrate possible systematic uncertainties related to using the EDF modelling

Nuclear and High Energy Physics[PHYS.NUCL]Physics [physics]/Nuclear Theory [nucl-th]ProtonNuclear TheoryNuclear Theorychemistry.chemical_elementFOS: Physical sciences7. Clean energySpectral lineMoments of inertiaNuclear physicsNuclear Theory (nucl-th)NeutronCovariant transformationHeavy and superheavy nucleiPhysicsta114Odd–even mass staggeringMoment of inertiachemistryExcited stateQuasiparticleNobeliumQuasiparticle excitationsNuclear energy density functionalsNuclear masses
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