Search results for "IONIZATION"

showing 10 items of 1255 documents

Laser spectroscopy measurement of isotope shifts and nuclear moments of short-lived neon isotopes

2003

Within the scope of a laser spectroscopy study of nuclear structure in the sd shell we are measuring nuclear moments and isotope shifts of neon isotopes. An ultra-sensitive variant of collinear laser spectroscopy [1, 2] is applied to a neutralized fast beam from ISOLDE (CERN). The non-optical detection is based on optical pumping, state selective collisional ionization and β-activity counting. This method gives access in particular to the short-lived isotopes in the extended chain of 17–26,28Ne.

PhysicsIsotopeAnalytical chemistryNuclear structurePhysics::OpticsOptical pumpingIsotopes of neonIonizationPhysics::Atomic PhysicsAtomic physicsNuclear ExperimentSpectroscopyAtomic vapor laser isotope separationBeam (structure)
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Experiments with stored exotic nuclei at relativistic energies

2006

Abstract A review and recent progress are presented from experiments on masses and lifetimes of bare and few-electron exotic nuclei at GSI. Relativistic rare isotopes produced via projectile fragmentation and fission were separated in flight by the fragment separator FRS and injected into the storage ring ESR. This worldwide unique experimental method gives access to all fragments with half-lives down to the microsecond range. The great research potential is demonstrated by the discovery of new isotopes along with simultaneous mass and lifetime measurements. Single particle decay measurements and the continuous recording of both stored mother and daughter nuclei open up a new era for nuclea…

PhysicsIsotopeFissionNuclear TheoryCondensed Matter PhysicsNuclear physicsMicrosecondParticle decayIonizationNuclear spectroscopyPhysical and Theoretical ChemistryAtomic physicsNuclear ExperimentInstrumentationProjectile fragmentationSpectroscopyStorage ringInternational Journal of Mass Spectrometry
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Isotope Shift Measurements for Superdeformed Fission Isomeric States

1998

Optical isotope shift measurements have been performed for the ${}^{240,242}{\mathrm{Am}}^{f}$ fission isomers with low target production rates of $10{\mathrm{s}}^{\ensuremath{-}1}$ employing resonance ionization spectroscopy in a buffer gas cell. Isotope shift ratios ${\mathrm{IS}}^{240f,241}/{\mathrm{IS}}^{243,241}\phantom{\rule{0ex}{0ex}}=\phantom{\rule{0ex}{0ex}}39.2(8)$ and ${\mathrm{IS}}^{242f,241}/{\mathrm{IS}}^{243,241}\phantom{\rule{0ex}{0ex}}=\phantom{\rule{0ex}{0ex}}41.4(8)$ have been measured at the 500.02 nm transition. A difference in the nuclear mean charge radii $\ensuremath{\delta}〈{r}^{2}{〉}_{\mathrm{opt}}^{242f,241}\phantom{\rule{0ex}{0ex}}=\phantom{\rule{0ex}{0ex}}5.34(2…

PhysicsIsotopeFissionResonance ionizationQuadrupoleGeneral Physics and AstronomyCharge (physics)Production (computer science)Atomic physicsPhysical Review Letters
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Isotope shifts and hyperfine structure in the $\mathsf{ 3d ^2D_J \rightarrow 4p ^2P_J}$ transitions in calcium II

1998

The isotope shift and hyperfine structure in the three \(\) - transitions in Ca II have been studied by fast ion beam collinear laser spectroscopy for all stable Ca isotopes. The metastable 3d states were populated within the surface ionization source of a mass separator with a probability of about 0.1%. After resonant excitation to the 4p levels with diode laser light around 850 nm the uv photons from the \(\) transitions to the ground state were used for detection. Hyperfine structure parameters A and B for the odd isotope 43Ca, as evaluated from the splittings observed, agree well with theoretical predictions from relativistic many-body perturbation theory. Field shift constants \(\) and…

PhysicsIsotopeMetastabilityThermal ionizationPhysics::Atomic PhysicsElectronic structureAtomic physicsSpectroscopyGround stateHyperfine structureAtomic and Molecular Physics and OpticsExcitationThe European Physical Journal D - Atomic, Molecular and Optical Physics
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First observation of the β-decay of neutron-rich 215Pb and 218Bi by the pulsed-release technique and resonant laser ionisation

2003

The neutron-rich Tl, Pb and Bi isotopes are of exceptional interest to trace the evolution of single-particle levels away from the doubly magic 208Pb towards the neutron-rich side of the nuclear chart. While 208Pb is well understood in terms of the shell model, experimental data on the heavier isotopes is very scarce and it is far from clear to what extent the shell model is upheld [1]. Furthermore, large branchings ratios for β-delayed neutron emission are expected in this mass region, adding astrophysical interest to the subject [2].

PhysicsIsotopeNeutron emissionlawAstrophysics::High Energy Astrophysical PhenomenaIonizationNuclear TheorySHELL modelNeutronAtomic physicsNuclear ExperimentLaserlaw.invention
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Isotope shifts and hyperfine structure in calcium 4snp and 4snf F Rydberg states

2000

Isotope shifts and hyperfine structure have been measured in 4snp 1 P1 and Rydberg states for all stable calcium isotopes and the radioisotope 41Ca using high-resolution laser spectroscopy. Triple-resonance excitation via Rydberg state was followed by photoionization with a CO2 laser and mass selective ion detection. Isotope shifts for the even-mass isotopes have been analyzed to derive specific mass shift and field shift factors. The apparent isotope shifts for 41Ca and 43Ca exhibit anomalous values that are n-dependent. This is interpreted in terms of hyperfine-induced fine-structure mixing, which becomes very pronounced when singlet-triplet fine-structure splitting is comparable to the h…

PhysicsIsotopePhotoionizationAtomic and Molecular Physics and OpticsIsotopes of calciumsymbols.namesakeIsotopic shiftKinetic isotope effectRydberg formulasymbolsPhysics::Atomic PhysicsRydberg stateAtomic physicsHyperfine structureThe European Physical Journal D
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Decay of Neutron-Rich Mn Nuclides and Deformation of Heavy Fe Isotopes

1998

The use of chemically selective laser ionization combined with beta-delayed neutron counting at CERN/ISOLDE has permitted identification and half-life measurements for 623-ms Mn-61 up through 14-ms Mn-69. The measured half-lives are found to be significantly longer near N=40 than the values calculated with a QRPA shell model using ground-state deformations from the FRDM and ETFSI models. Gamma-ray singles and coincidence spectroscopy has been performed for Mn-64 and Mn-66 decays to levels of Fe-64 and Fe-66, revealing a significant drop in the energy of the first 2+ state in these nuclides that suggests an unanticipated increase in collectivity near N=40.

PhysicsIsotopeSHELL modelFOS: Physical sciencesGeneral Physics and AstronomyIonizationQuasiparticleNuclear Physics - ExperimentNeutronNuclideNuclear Experiment (nucl-ex)Atomic physicsSpectroscopyNuclear ExperimentPhysical Review Letters
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Calculation of atomic properties of superheavy elements Z=110–112 and their ions

2020

We calculate the spectra, electric dipole transition rates, and isotope shifts of the superheavy elements Ds ($Z=110$), Rg ($Z=111$), and Cn ($Z=112$) and their ions. These calculations were performed using a recently developed, efficient version of the ab intio configuration-interaction combined with perturbation theory to treat distant effects. The successive ionization potentials of the three elements are also calculated and compared to lighter analogous elements.

PhysicsIsotopeSuperheavy Elements7. Clean energy01 natural sciencesSpectral line010305 fluids & plasmasIonAtomic propertiesIonization0103 physical sciencesAtomic physicsElectric dipole transitionPerturbation theory010306 general physicsPhysical Review A
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Jet propagation through inhomogeneous media and shock ionization

2021

In this contribution we present the first numerical simulations of a relativistic outflow propagating through the inner hundreds of parsecs of its host galaxy, including atomic and ionised hydrogen, and the cooling effects of ionisation. Our results are preliminary, but we observe efficient shock ionization of atomic hydrogen in interstellar clouds. The mean density of the interstellar medium in these initial simulations is lower than that expected in typical galaxies, which makes cooling times longer and thus no recombination is observed inside the shocked region. The velocities achieved by the shocked gas in the simulations are in agreement with observational results, although with a wide…

PhysicsJet (fluid)HydrogenAstrophysics::High Energy Astrophysical PhenomenaInterstellar cloudchemistry.chemical_elementAstronomy and AstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsGalaxyShock (mechanics)Computational physicsInterstellar mediumchemistrySpace and Planetary ScienceIonizationOutflowPhysics::Atomic PhysicsAstrophysics - High Energy Astrophysical PhenomenaAstrophysics::Galaxy Astrophysics
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The diagnostic potential of Fe lines applied to protostellar jets

2013

We investigate the diagnostic capabilities of the iron lines for tracing the physical conditions of the shock-excited gas in jets driven by pre-main sequence stars. We have analyzed the 300-2500 nm X-shooter spectra of two jets driven by the pre-main sequence stars ESO-Halpha 574 and Par-Lup 3-4. Both spectra are very rich in [FeII] lines over the whole spectral range; in addition, lines from [FeIII] are detected in the ESO-H\alpha 574 spectrum. NLTE codes along with codes for the ionization equilibrium are used to derive the gas excitation conditions of electron temperature and density, and fractional ionization. The iron gas-phase abundance is provided by comparing the iron lines emissivi…

PhysicsJet (fluid)Range (particle radiation)ISM: individual objects: ESO-Hα 574 Par-Lup 3-4 ISM: jets and outflows ISM: lines and bands stars: pre-main sequenceFOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsAstrophysics - Astrophysics of GalaxiesSpectral lineStarsindividual objects: ESO-Hα 574 Par-Lup 3-4 ISM: jets and outflows ISM: lines and bands stars: pre-main sequence [ISM]Astrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceIonizationAstrophysics of Galaxies (astro-ph.GA)EmissivityElectron temperatureAtomic physicsExcitationSolar and Stellar Astrophysics (astro-ph.SR)
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