Search results for " shell"

showing 10 items of 307 documents

Configuration-interaction calculations of jellium clusters by the nuclear shell model

1994

Configuration-interaction (CI) calculations are performed on Na clusters of up to 20 atoms within the spherical jellium model, with particular attention paid to the magic clusters with N=2, 8, and 20. The interacting valence electrons are assumed to move in the Coulomb field of the jellium core. The numerical work is carried out by the nuclear-structure code oxbash modified to handle LS coupling. The many-particle bases are constructed of harmonic-oscillator single-particle states extending over 11 major shells and, alternatively, of single-particle states generated by the local-spin-density approximation (LSDA). The calculated quantities include ground- and excited state energies, ionizati…

PhysicsField (physics)Excited stateIonizationJelliumPhysics::Atomic and Molecular ClustersQuasiparticleNuclear shell modelConfiguration interactionAtomic physicsValence electronPhysical Review B
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Magicity of theN68iSemidouble-Closed-Shell Nucleus Probed by Gamow-Teller Decay of the Odd-ANeighbors

1999

The particle-hole excitations through the $N\phantom{\rule{0ex}{0ex}}=\phantom{\rule{0ex}{0ex}}40$ subshell around ${}^{68}\mathrm{Ni}$ have been studied by the $\ensuremath{\beta}$ decay of ${}^{69}\mathrm{Co}$ and ${}^{69}\mathrm{Ni}$. The half-life of ${}^{69}\mathrm{Co}$ was measured to be 0.22(2) s, and a new $\ensuremath{\beta}$-decaying isomer with a half-life of 3.5(5) s was identified in ${}^{69}\mathrm{Ni}$. From the decay of the ${}^{69}\mathrm{Ni}$ isomer a 9(4)% mixing of the $\ensuremath{\pi}{p}_{3/2}^{+1}\ensuremath{\nu}{p}_{1/2}^{\ensuremath{-}2}\ensuremath{\nu}{g}_{9/2}^{+2}$ configuration into the ground state of ${}^{69}\mathrm{Cu}$ can be deduced. Significant polarizatio…

PhysicsGeneral Physics and AstronomyAtomic physicsNucleonGround stateOpen shellPhysical Review Letters
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Spin-restricted open-shell coupled-cluster theory

1997

Spin-restricted CC theory is suggested as a new approach for the treatment of high-spin open-shell systems in CC theory. Spin constraints are imposed on the wave function in the sense that the projected spin eigenvalue equations are fulfilled within the (truncated) excitation space. These constraints allow a reduction in the number of independent amplitudes, thus decreasing the computational cost when implemented efficiently. The approach ensures that the spin expectation value always corresponds to the exact value, though the wave function is (for truncated CC treatments) not rigorously spin-adapted. For the specific case of high-spin doublets, detailed equations are derived for amplitudes…

PhysicsGeneral Physics and AstronomyFunction (mathematics)Expectation valueSpace (mathematics)Coupled clusterQuantum mechanicsCondensed Matter::Strongly Correlated ElectronsStatistical physicsPhysical and Theoretical ChemistryWave functionOpen shellEigenvalues and eigenvectorsSpin-½The Journal of Chemical Physics
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On Relativistic Disk Spectroscopy in Compact Objects with X-ray CCD Cameras

2010

X-ray charge-coupled devices (CCDs) are the workhorse detectors of modern X-ray astronomy. Typically covering the 0.3-10.0 keV energy range, CCDs are able to detect photoelectric absorption edges and K shell lines from most abundant metals. New CCDs also offer resolutions of 30-50 (E/dE), which is sufficient to detect lines in hot plasmas and to resolve many lines shaped by dynamical processes in accretion flows. The spectral capabilities of X-ray CCDs have been particularly important in detecting relativistic emission lines from the inner disks around accreting neutron stars and black holes. One drawback of X-ray CCDs is that spectra can be distorted by photon "pile-up", wherein two or mor…

PhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)PhotonSpectrometerAstrophysics::High Energy Astrophysical PhenomenaElectron shellFOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsGeneral Relativity and Quantum Cosmology (gr-qc)General Relativity and Quantum CosmologyRelativistic diskSpectral lineaccretion accretion disks black hole physics instrumentation spectrographs methods analytical X-rays binariesNeutron starSettore FIS/05 - Astronomia E AstrofisicaSpace and Planetary ScienceEmission spectrumAstrophysics::Earth and Planetary AstrophysicsAstrophysics - High Energy Astrophysical PhenomenaSpectroscopyAstrophysics::Galaxy Astrophysics
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Symmetry and Electronic Structure of Noble Metal Nanoparticles and the Role of Relativity

2004

High resolution photoelectron spectra of cold mass selected Cu_n-, Ag_n- and Au_n- with n =53-58 have been measured at a photon energy of 6.42 eV. The observed electron density of states is not the expected simple electron shell structure, but seems to be strongly influenced by electron-lattice interactions. Only Cu55- and Ag55- exhibit highly degenerate states. This is a direct consequence of their icosahedral symmetry, as is confirmed by density functional theory calculations. Neighboring sizes exhibit perturbed electronic structures, as they are formed by removal or addition of atoms to the icosahedron and therefore have lower symmetries. Gold clusters in the same size range show complet…

PhysicsIcosahedral symmetryDegenerate energy levelsElectron shellGeneral Physics and AstronomyFOS: Physical sciencesElectronic structureSpectral lineCondensed Matter - Other Condensed MatterAb initio quantum chemistry methodsDensity of statesDensity functional theoryAtomic physicsOther Condensed Matter (cond-mat.other)
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Spontaneous fission instability of the neutron-deficient No and Rf isotopes: The new isotope No249

2021

In the heaviest elements, the instability of atomic nuclei against spontaneous fission leads to ever shorter nuclear half-lives. Upon falling below a timescale of ${10}^{\ensuremath{-}14}$ s, the border of existence of isotopes is crossed because this is the timescale on which the formation of atomic shells occurs. Analysis of the experimental data on the spontaneous fission half-lives of Rf isotopes in relation with their expected single-particle orbitals hint at a potentially abrupt decrease in half-lives of unknown neutron-deficient Rf isotopes with neutron numbers $l149$, which suggests that the isotopic border is already almost reached. However, this conjecture, which cannot be explain…

PhysicsIsotopeAtomic orbitalFissionAtomic nucleusElectron shellNeutronAtomic physicsNuclear ExperimentSpontaneous fissionLine (formation)Physical Review C
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Many-body origin of the plasmon resonance in small metal clusters

1994

The origin of the plasmon excitation in small metal clusters is studied within the jellium model through ab initio electronic-structure calculations based on the nuclear shell model. In the limit of infinite size, the plasmon classically represents pure harmonic motion of the center of mass of the valence electrons. It is shown that this limit is already well approximated by clusters of only eight electrons.

PhysicsJelliumPhysics::Atomic and Molecular ClustersNuclear shell modelAb initioCenter of massElectronSurface plasmon resonanceAtomic physicsValence electronAtomic and Molecular Physics and OpticsPlasmonZeitschrift f�r Physik D Atoms, Molecules and Clusters
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Translationally invariant coupled cluster method in coordinate space for nuclei

2002

We study a formulation of the translationally invariant coupled cluster method in coordinate space for finite nuclei. The new formulation remedies convergence problems that plagued previous calculations in configuration space. The method is applied to light nuclei using semi-realistic central interactions.

PhysicsLight nucleusNuclear and High Energy Physics/dk/atira/pure/subjectarea/asjc/3100/3106Nuclear structureInvariant (physics)Physics and Astronomy(all)Coupled clusterClassical mechanics/dk/atira/pure/subjectarea/asjc/3100Quantum electrodynamicsNuclear binding energyConfiguration spaceCLOSED-SHELL NUCLEI; MODEL-CALCULATIONS; CBF THEORY; DEPENDENT CORRELATIONS; PAIR CORRELATIONS; FINITE SYSTEMS; GROUND-STATE; JASTROW; O-16; Nuclear binding energy; Nuclear model; Nuclear structure; Nucleon-nucleon potential (formulation of translationally invariant coupled cluster method in coordinate space for closed shell nuclei within 0p-shell with use of semi-realistic central nucleon-nucleon interactions)Coordinate spaceGround state
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Sub-Barrier Coulomb Excitation ofSn110and Its Implications for theSn100Shell Closure

2007

The first excited 2(+) state of the unstable isotope Sn-110 has been studied in safe Coulomb excitation at 2.82 MeV/u using the MINIBALL array at the REX-ISOLDE post accelerator at CERN. This is the first measurement of the reduced transition probability of this state using this method for a neutron deficient Sn isotope. The strength of the approach lies in the excellent peak-to-background ratio that is achieved. The extracted reduced transition probability, B(E2 : 0(+) -> 2(+)) 0.220 +/- 0.022e(2) b(2), strengthens the observation of the evolution of the B(E2) values of neutron deficient Sn isotopes that was observed recently in intermediate-energy Coulomb excitation of Sn-108. It implies …

PhysicsMass numberIsotope010308 nuclear & particles physicsShell (structure)Nuclear shell modelGeneral Physics and AstronomyCoulomb excitation7. Clean energy01 natural sciencesClosure (computer programming)Excited state0103 physical sciencesNeutronAtomic physicsNuclear Experiment010306 general physicsPhysical Review Letters
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Communication: Spin densities within a unitary group based spin-adapted open-shell coupled-cluster theory: Analytic evaluation of isotropic hyperfine…

2015

We report analytical calculations of isotropic hyperfine-coupling constants in radicals using a spin-adapted open-shell coupled-cluster theory, namely, the unitary group based combinatoric open-shell coupled-cluster (COSCC) approach within the singles and doubles approximation. A scheme for the evaluation of the one-particle spin-density matrix required in these calculations is outlined within the spin-free formulation of the COSCC approach. In this scheme, the one-particle spin-density matrix for an open-shell state with spin S and MS = + S is expressed in terms of the one- and two-particle spin-free (charge) density matrices obtained from the Lagrangian formulation that is used for calcul…

PhysicsMatrix (mathematics)Coupled clusterUnitary groupQuantum mechanicsIsotropyGeneral Physics and AstronomyOrder (group theory)Charge (physics)Physical and Theoretical ChemistryOpen shellSpin-½The Journal of Chemical Physics
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