3 documentos corresponden a la consulta.
Palabras contadas: heavy: 30, elements: 86
Alonso, M.S. - López-García, Z. - Malaroda, S. - Leone, F.
Astron. Astrophys. 2003;402(1):331-334
2003
Temas: Stars: abundances - Stars: chemically peculiar - Stars: individual: HD 19400 - Stars: individual: HD 34797 - Stars: individual: HD 35456 - Galaxies - Helium - Hydrogen - Magnetic fields - Photometers
Descripción: An analysis of the abundances of the helium-weak CP stars HD 19400, HD 34797 and HD 35456, is presented using ATLAS9 model atmospheres and observational material taken with a REOSC echelle spectrograph attached to the Jorge Sahade 2.15 m telescope at CASLEO. The light elements are deficient except silicon which is overabundant in HD 19400 and HD 34797. The iron peak elements are all overabundant by factors between 5 and 60. The heavy elements show an overabundance in the three stars studied.
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Melo, J.I. - De Azúa, M.C.R. - Peralta, J.E. - Scuseria, G.E.
J Chem Phys 2005;123(20)
2005
Temas: Density functional theory - Douglas-Kroll-Hess approximation - Heavy elements - Quasirelativistic approach - Approximation theory - Hamiltonians - Perturbation techniques - Probability density function - Nuclear magnetic resonance
Descripción: We have employed the Douglas-Kroll-Hess approximation to derive the perturbative Hamiltonians involved in the calculation of NMR spin-spin couplings in molecules containing heavy elements. We have applied this two-component quasirelativistic approach using finite perturbation theory in combination with a generalized Kohn-Sham code that includes the spin-orbit interaction self-consistently and works with Hartree-Fock and both pure and hybrid density functionals. We present numerical results for one-bond spin-spin couplings in the series of tetrahydrides C H4, Si H4, Ge H4, and Sn H4. Our two-component Hartree-Fock results are in good agreement with four-component Dirac-Hartree-Fock calculations, although a density-functional treatment better reproduces the available experimental data. © 2005 American Institute of Physics.
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Badnell, N.R. - O'Mullane, M.G. - Summers, H.P. - Altun, Z. - Bautista, M.A. - Colgan, J. - Gorczyca, T.W. - Mitnik, D.M. - Pindzola, M.S. - Zatsarinny, O.
Astron. Astrophys. 2003;406(3):1151-1165
2003
Temas: Atomic data - Atomic processes - Plasmas - Astrophysics - Database systems - Electrons - Ground state - Plasmas - Dielectronic recombination data - Dynamic finite-density plasmas
Descripción: A programme is outlined for the assembly of a comprehensive dielectronic recombination database within the generalized collisional-radiative (GCR) framework. It is valid for modelling ions of elements in dynamic finite-density plasmas such as occur in transient astrophysical plasmas such as solar flares and in the divertors and high transport regions of magnetic fusion devices. The resolution and precision of the data are tuned to spectral analysis and so are sufficient for prediction of the dielectronic recombination contributions to individual spectral line emissivities. The fundamental data are structured according to the format prescriptions of the Atomic Data and Analysis Structure (ADAS) and the production of relevant GCR derived data for application is described and implemented following ADAS. The requirements on the dielectronic recombination database are reviewed and the new data are placed in context and evaluated with respect to older and more approximate treatments. Illustrative results validate the new high-resolution zero-density dielectronic recombination data in comparison with measurements made in heavy-ion storage rings utilizing an electron cooler. We also exemplify the role of the dielectronic data on GCR coefficient behaviour for some representative light and medium weight elements.
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