Search results for "neutron"

showing 10 items of 2330 documents

Long-term optical and X-ray variability of the Be/X-ray binary H 1145-619: Discovery of an ongoing retrograde density wave

2017

Multiwavelength monitoring of Be/X-ray binaries is crucial to understand the mechanisms producing their outbursts. H 1145-619 is one of these systems, which has recently displayed X-ray activity. We investigate the correlation between the optical emission and the X-ray activity to predict the occurrence of new X-ray outbursts from the inferred state of the circumstellar disc. We have performed a multiwavelength study of H 1145-619 from 1973 to 2017 and present here a global analysis of its variability over the last 40 years. We have used optical spectra from the SAAO, SMARTS and SALT telescopes and optical photometry from INTEGRAL/OMC and ASAS. We also used X-ray observations from INTEGRAL/…

BrightnessBe starAstrophysics::High Energy Astrophysical Phenomenamedia_common.quotation_subjectX-ray binarystars: emission-lineFOS: Physical sciencesAstrophysics01 natural sciencesSpectral lineDensity wave theoryPhotometry (optics)X-rays: binariesstars: neutrontechniques: photometric0103 physical sciencesAstrophysics::Solar and Stellar Astrophysics010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)Astrophysics::Galaxy Astrophysicsmedia_commonHigh Energy Astrophysical Phenomena (astro-ph.HE)Physics010308 nuclear & particles physicsBeAstronomy and AstrophysicsLight curvestars: emission-line BeAstrophysics - Solar and Stellar Astrophysics13. Climate actionSpace and Planetary ScienceSkyAstrophysics::Earth and Planetary AstrophysicsAstrophysics - High Energy Astrophysical Phenomenatechniques: spectroscopicAstronomy & Astrophysics
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Study of the Spin Wave Linewidth in a 1-D Easy-Plane Ferromagnet Using Neutron Polarization Analysis

1990

An anomalous wavevector dependence in the spin wave linewidth associated with fluctuations out of the easy plane is observed for the first time in the one-dimensional easy-plane ferromagnet CsNiF3 by means of inelastic polarized neutron scattering. The linewidths of the spin waves, one attributed to spin fluctuations out of the easy plane and another in the easy plane, are studied separately throughout the Brillouin zone. The zone boundary narrowing of the linewidth associated with the spin fluctuations in the easy plane is observed for the first time in agreement with the classical spin wave theory. The deviations from the classical result at large qc and high temperature are interpreted a…

Brillouin zonePhysicsLaser linewidthCondensed matter physicsSpin polarizationSpin waveSpin Hall effectGeneral Physics and AstronomyCondensed Matter::Strongly Correlated ElectronsWave vectorNeutron scatteringPolarization (waves)Europhysics Letters (EPL)
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Orientational glass behaviour of K Br0.96(CN)0.04

1981

Ultrasonic measurements on the mixed crystal K Br0.96(CN)0.04 show a minimum of most of the elastic constants at 16 K. In addition we determinedc11(T) at 10 MHz and at 50 MHz observing dispersion effects. These results and previous Brillouin and neutron scattering results of other authors on higher CN-concentrations are interpreted by an orientational glass behaviour. A semiquantitative description is given in terms of the mean random field approximation.

Brillouin zoneRandom fieldMaterials scienceNuclear magnetic resonanceDispersion (optics)Ultrasonic sensorNeutron scatteringCondensed Matter PhysicsSpectroscopyOrientational glassSmall-angle neutron scatteringMolecular physicsElectronic Optical and Magnetic Materials
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Search for Gravitational-wave Signals Associated with Gamma-Ray Bursts during the Second Observing Run of Advanced LIGO and Advanced Virgo

2019

We present the results of targeted searches for gravitational-wave transients associated with gamma-ray bursts during the second observing run of Advanced LIGO and Advanced Virgo, which took place from 2016 November to 2017 August. We have analyzed 98 gamma-ray bursts using an unmodeled search method that searches for generic transient gravitational waves and 42 with a modeled search method that targets compact-binary mergers as progenitors of short gamma-ray bursts. Both methods clearly detect the previously reported binary merger signal GW170817, with p-values of <9.38 10-6 (modeled) and 3.1 10-4 (unmodeled). We do not find any significant evidence for gravitational-wave signals associate…

Burst astrophysicAstrofísicaneutron star: binary010504 meteorology & atmospheric sciencesBinary numberAstrophysics01 natural sciencesLIGOQCSUPERNOVArelativistic jetsQBHigh Energy Astrophysical Phenomena (astro-ph.HE)Settore FIS/01counterpartGRBGravitational waves (678)Physical SciencesRELATIVISTIC JETSAstrophysics - High Energy Astrophysical PhenomenaGravitational waveGravitationstarsblack-holeAstrophysics::High Energy Astrophysical PhenomenaGeneral Relativity and Quantum Cosmology (gr-qc)precursor activityGravitational wavesSettore FIS/05 - Astronomia e AstrofisicasupernovaCORE-COLLAPSEGamma-ray burstGravitational wave sourcesScience & TechnologyVirgoRCUKAstronomy and AstrophysicsHigh energy astrophysics (739)RedshiftDewey Decimal Classification::500 | Naturwissenschaften::520 | Astronomie Kartographiedetector: sensitivityVIRGOSpace and Planetary Sciencegravitational radiation: emissionBLACK-HOLEddc:520Gravitational wave astronomyGamma-ray burst[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]STARSGravitacióAstronomySignalGeneral Relativity and Quantum CosmologyBurst astrophysicslocalizationemission010303 astronomy & astrophysicsPhysicsDetectorGamma-ray bursts (629)[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]Gravitational wave sourcePRECURSOR ACTIVITYGamma-ray burstsLIGO (920)High energy astrophysicsdata analysis methodBurst astrophysics (187)FOS: Physical sciencesAstrophysics::Cosmology and Extragalactic Astrophysicsgamma ray: burstAstronomy & AstrophysicsMASSgravitational radiation: direct detectionGravitational wave astronomy Gravitational wave sources LIGO; Gravitational waves Gamma-ray bursts Burst astrophysics High energy astrophysicsGravitational wave astronomy (675)electromagnetic field: production0103 physical sciencesnumerical calculationsGRB; gravitational waves; LIGO; VirgoSTFC0105 earth and related environmental sciencesgravitational wavesneutron starsGravitational waveCOUNTERPARTgravitational radiationLIGOcore-collapsegravitational radiation detectorGravitational wave sources (677)radiationNeutron starPhysics and AstronomymassRADIATIONEMISSIONGravitational wave astronomy; Gravitational wave sources; LIGO; Gravitational waves; Gamma-ray bursts; Burst astrophysics; High energy astrophysics
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Evidence of a sudden increase in the nuclear size of proton-rich silver-96

2021

Understanding the evolution of the nuclear charge radius is one of the long-standing challenges for nuclear theory. Recently, density functional theory calculations utilizing Fayans functionals have successfully reproduced the charge radii of a variety of exotic isotopes. However, difficulties in the isotope production have hindered testing these models in the immediate region of the nuclear chart below the heaviest self-conjugate doubly-magic nucleus 100Sn, where the near-equal number of protons (Z) and neutrons (N) lead to enhanced neutron-proton pairing. Here, we present an optical excursion into this region by crossing the N = 50 magic neutron number in the silver isotopic chain with th…

CHARGE RADIIEFFICIENCYProtonScienceSYMMETRYNuclear TheoryGeneral Physics and AstronomyIONIZATION SPECTROSCOPY[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]01 natural sciencesGeneral Biochemistry Genetics and Molecular BiologyEffective nuclear chargeArticleNuclear physicsCharge radiusMOMENTS0103 physical sciencesexperimental nuclear physicsNeutronNuclear Physics - ExperimentPhysics::Atomic PhysicsBETA-DECAYExperimental nuclear physics010306 general physicsLASER SPECTROSCOPYNuclear ExperimentPhysicsRESONANCE IONIZATIONisotoopitMultidisciplinaryScience & TechnologyIsotope010308 nuclear & particles physicsQGeneral ChemistryRadiusION-SOURCEMultidisciplinary SciencesTheoretical nuclear physicsNeutron numbertheoretical nuclear physicsScience & Technology - Other TopicsISOTOPESDensity functional theoryydinfysiikka
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Proton-neutron pairing correlations in the self-conjugate nucleus 42Sc

2021

Collinear laser spectroscopy of the N=Z=21 self-conjugate nucleus 42Sc has been performed at the JYFL IGISOL IV facility in order to determine the change in nuclear mean-square charge radius between the Iπ=0+ ground state and the Iπ=7+ isomer via the measurement of the 42g,42mSc isomer shift. New multi-configurational Dirac-Fock calculations for the atomic mass shift and field shift factors have enabled a recalibration of the charge radii of the 42−46Sc isotopes which were measured previously. While consistent with the treatment of proton-neutron, proton-proton and neutron-neutron pairing on an equal footing, the reduction in size for the isomer is observed to be of a significantly larger m…

CHARGE RADIINuclear and High Energy PhysicsProtonCollinear laser spectroscopyQC1-999spektroskopiaNuclear TheoryFOS: Physical sciencesAstronomy & Astrophysicsnucl-ex01 natural sciencesPhysics Particles & FieldsCharge radius0103 physical sciencesPhysics::Atomic and Molecular Clustersddc:530NeutronNuclear Physics - ExperimentNuclear Experiment (nucl-ex)010306 general physicsNuclear ExperimentNuclear ExperimentPhysicsisotoopitScience & TechnologyIsotopeMagnetic moment010308 nuclear & particles physicsPhysicsProton-neutron pairingTABLEHyperfine structure and isotope shiftAtomic mass3. Good healthCharge radiusPhysics NuclearPairingPhysical SciencesSHELL-MODELAtomic physicsydinfysiikkaGround stateskandiumPhysics Letters B
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Deformation and mixing of coexisting shapes in neutron-deficient polonium isotopes

2015

Coulomb-excitation experiments are performed with postaccelerated beams of neutron-deficient Po196,198,200,202 isotopes at the REX-ISOLDE facility. A set of matrix elements, coupling the low-lying states in these isotopes, is extracted. In the two heaviest isotopes, Po200,202, the transitional and diagonal matrix elements of the 2+1 state are determined. In Po196,198 multistep Coulomb excitation is observed, populating the 4+1,0+2, and 2+2 states. The experimental results are compared to the results from the measurement of mean-square charge radii in polonium isotopes, confirming the onset of deformation from Po196 onwards. Three model descriptions are used to compare to the data. Calculati…

CHARGE RADIINuclear and High Energy PhysicsTRANSITION-PROBABILITYchemistry.chemical_elementCoulomb excitation[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]7. Clean energy01 natural sciences114 Physical sciencessymbols.namesakeMatrix (mathematics)NUCLEAR-DATA SHEETSCOULOMB-EXCITATION0103 physical sciencesSTATE PROPERTIESNuclear Physics - ExperimentNeutronfysiikka010306 general physicsEVEN-EVEN NUCLIDESMixing (physics)isotopesPoloniumINTRUDER STATESGAMMA-RAY SPECTROSCOPYPhysicsSPIN STATESisotoopitPO ISOTOPESIsotopeta114010308 nuclear & particles physicsBohr modelchemistryPhysics and AstronomysymbolsAtomic physicsInteracting boson modelphysicspolonium25.70.De 23.20.Js 25.60.−t 27.80.+w
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Nucleon localization function in rotating nuclei

2020

Background: An electron localization function was originally introduced to visualize bond structures in molecules. It became a useful tool to describe electron configurations in atoms, molecules and solids. In nuclear physics, a nucleon localization function (NLF) has been used to characterize clusters in light nuclei, fragment formation in fission and pasta phases in the inner crust of neutron stars. Purpose: We use the NLF to study the nuclear response to fast rotation. Methods: We generalize the NLF to the case of nuclear rotation. The extended expressions involve both time-even and time-odd local densities. Since current density and density gradient contribute to the NLF primarily at th…

CURRENTSAngular momentumNuclear TheoryMEAN-FIELDNuclear TheoryFOS: Physical sciences114 Physical sciences01 natural sciencesNuclear Theory (nucl-th)Total angular momentum quantum number0103 physical sciencesSUPERDEFORMED BANDSDISTRIBUTIONScollective levelsNeutron010306 general physicsSpin (physics)EQUATIONSPhysicsCRANKED HARMONIC-OSCILLATOR010308 nuclear & particles physicsYrastnucleon distributionnuclear structure and decaysSTATEElectron localization functionComputational physicsELECTRON LOCALIZATIONMean field theorySYMMETRIESydinfysiikkaNucleonPhysical Review C
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Cadmium mass measurements between the neutron shell closures at N=50 and 82

2010

International audience; The mass values of the neutron-deficient cadmium isotopes 99−109Cd and of the neutronrich isotopes 114,120,122−124,126,128Cd have been measured using ISOLTRAP. The behavior of the separation energies of the cadmium isotopes from N = 50 to 82 is discussed.

CadmiumIsotopehigh-precision mass measurementsChemistryStable isotope ratioPenning trapRadiochemistrychemistry.chemical_element020206 networking & telecommunications02 engineering and technology[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]ISOLTRAP7. Clean energyISOLTRAPcadmium massesIsotope separationlaw.inventionlawIsotopes of cadmium0202 electrical engineering electronic engineering information engineering020201 artificial intelligence & image processingNeutron21.10.Dr 21.30.Fe 27.60.+j 32.10.BiNucleon
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Isotope shifts in natural cerium

2003

High resolution crossed beam resonance fluorescence laser spectroscopy has been performed on an atomic beam of naturally occurring cerium, and isotope shifts have been measured in several transitions. Changes in mean square charge radius, δ〈r 2〉, have been extracted using the King plot technique and show the characteristic increase at the N = 82 neutron shell closure. The measurements form the basis for further investigations of radioactive isotopes and isomers on both sides of the shell closure.

CeriumMaterials scienceResonance fluorescencechemistryIsotopeCharge radiusPhysics::Atomic and Molecular ClustersShell (structure)chemistry.chemical_elementNeutronAtomic physicsSpectroscopyBeam (structure)
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