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Related papers: K-vacancy levels in Ne, Mg, Si, S, Ar, and Ca

200 papers

Radiative and Auger decay data have been calculated for modelling the K lines in ions of the nickel isonuclear sequence, from Ni$^+$ up to Ni$^{27+}$. Level energies, transition wavelengths, radiative transition probabilities, and radiative…

Astrophysics · Physics 2009-11-13 P. Palmeri , P. Quinet , C. Mendoza , M. A. Bautista , J. Garcia , M. C. Witthoeft , T. R. Kallman

As part of a project to compute improved atomic data for the spectral modeling of iron K lines, we report extensive calculations and comparisons of atomic data for K-vacancy states in Fe XXIV. The data sets include: (i) energy levels, line…

Astrophysics · Physics 2009-11-07 M. A. Bautista , C. Mendoza , T. R. Kallman , P. Palmeri

We report extensive calculations of the decay properties of fine-structure K-vacancy levels in Fe X-Fe XVII. A large set of level energies, wavelengths, radiative and Auger rates, and fluorescence yields has been computed using three…

Astrophysics · Physics 2009-11-07 C. Mendoza , M. A. Bautista , T. R. Kallman , P. Palmeri

We list vacuum wavelengths, energy levels, statistical weights, transition probabilities and oscillator strengths for permitted resonance spectral lines of all ions of 18 astrophysically important elements (H through Si, S, Ar, Ca, Fe).…

atom-ph · Physics 2009-10-28 D. A. Verner , E. M. Verner , G. J. Ferland

We report calculations of energy levels and radiative rates ($A$-values) for transitions in Cr-like Co IV and Ni V. The quasi-relativistic Hartree-Fock (QRHF) code is adopted for calculating the data although GRASP (general-purpose…

Atomic Physics · Physics 2016-01-20 K. M. Aggarwal , P. Bogdanovich , R. Karpuškienė , F. P. Keenan , R. Kisielius , V. Stancalie

We present a complete set of analytic fits to the non-relativistic photoionization cross sections for the ground states of atoms and ions of elements from H through Si, and S, Ar, Ca, and Fe. Near the ionization thresholds, the fits are…

Astrophysics · Physics 2008-11-26 D. A. Verner , G. J. Ferland , K. T. Korista , D. G. Yakovlev

This is the final report of a three-paper series on the K-shell photoabsorption and photoionization of trace elements, namely F, Na, P, Cl, K, Sc, Ti, V, Cr, Mn, Co, Cu and Zn. K lines and edges from such elements are observed in the X-ray…

Atomic Physics · Physics 2018-08-22 C. Mendoza , M. A. Bautista , P. Palmeri , P. Quinet , M. C. Witthoeft , T. R. Kallman

A detailed analysis of the radiative and Auger de-excitation channels of K-shell vacancy states in Fe II-Fe IX has been carried out. Level energies, wavelengths, A-values, Auger rates and fluorescence yields have been calculated for the…

Astrophysics · Physics 2009-11-07 P. Palmeri , C. Mendoza , T. R. Kallman , M. A. Bautista , M. Melendez

Energy levels, radiative rates and lifetimes are reported for four S-like ions, namely Sc~VI, V VIII, Cr IX, and Mn~X. Two independent atomic structure codes, namely the general-purpose relativistic atomic structure package ({\sc grasp})…

Atomic Physics · Physics 2020-01-08 Kanti Aggarwal

Calculations for energy levels, radiative rates and lifetimes have been performed for three Ne-like ions, namely Hf~LXIII, Ta LXIV and Re LXVI, for which the general-purpose relativistic atomic structure package (GRASP) has been adopted.…

Atomic Physics · Physics 2018-04-11 K M Aggarwal

Reliable atomic data have been computed for the spectral modeling of the nitrogen K lines, which may lead to useful astrophysical diagnostics. Data sets comprise valence and K-vacancy level energies, wavelengths, Einstein $A$-coefficients,…

High Energy Astrophysical Phenomena · Physics 2014-11-20 J. Garcia , T. R. Kallman , M. Witthoeft , E. Behar , C. Mendoza , P. Palmeri , P. Quinet , M. A. Bautista , M. Klapisch

Energy levels and radiative rates (A-values) for transitions in Cr-like Cu~VI and Zn~VII are reported. These data are determined in the quasi-relativistic approach (QR), by employing a very large {\em configuration interaction} (CI)…

Atomic Physics · Physics 2016-07-20 K. M. Aggarwal , P. Bogdanovich , F. P. Keenan , R. Kisielius

We present precise radiative data of line strengths, transition probabilities and oscillator strengths for the allowed transitions among the $nS_{1/2}$, $nP_{1/2,3/2}$, $n'D_{3/2,5/2}$ and $n'F_{5/2,7/2}$ states with $n=4$ to $6$ and…

Atomic Physics · Physics 2022-02-09 Jyoti , Harpreet Kaur , Bindiya Arora , B. K. Sahoo

Extensive calculations of the atomic data required for the spectral modelling of the K-shell photoabsorption of oxygen ions have been carried out in a multi-code approach. The present level energies and wavelengths for the highly ionized…

Astrophysics · Physics 2009-11-10 J. Garcia , C. Mendoza , M. A. Bautista , T. W. Gorczyca , T. R. Kallman , P. Palmeri

Energy levels, radiative rates and lifetimes are reported for the lowest 139 levels of three Ne-like ions, namely Cu~XX, Zn~XXI and Ga~XXII. These levels mostly belong to the 2s$^2$2p$^6$, 2s$^2$2p$^5$3$\ell$, 2s2p$^6$3$\ell$,…

Atomic Physics · Physics 2018-03-13 K M Aggarwal

We calculate the ionization cross sections for H, He or Ne atoms using $\nu_e$ and $\bar \nu_e$ scattering at keV energies. Such cross sections are useful for e.g. $\bar \nu_e$-oscillation experiments using a tritium source. Using realistic…

High Energy Physics - Phenomenology · Physics 2009-11-07 G. J. Gounaris , E. A. Paschos , P. I. Porfyriadis

Widths of $KL_{2,3}$ atomic levels for Ca, Fe, Zn has been calculated in a fully-relativistic way using the extensive multiconfiguration Dirac-Fock and modified Dirac-Hartree-Slater calculations. The study of de-excitation of the…

Atomic Physics · Physics 2015-06-19 Karol Kozioł

Energy levels and radiative rates (A-values) for four types of transitions (E1, E2, M1, and M2) are reported for an astrophysically important Mg-like ion Si~III, whose emission lines have been observed in a variety of plasmas. For the…

Atomic Physics · Physics 2016-11-16 K M Aggarwal

Combined relativistic configuration interaction and many-body perturbation calculations are performed for the 359 fine-structure levels of the $2s^2 2p^3$, $2s 2p^4$, $2p^5$, $2s^2 2p^2 3l$, $2s 2p^3 3l$, $2p^4 3l$, and $2s^2 2p^2 4l$…

Atomic Physics · Physics 2016-03-23 K. Wang , R. Si , W. Dang , P. Jönsson , X. L. Guo , S. Li , Z. B. Chen , H. Zhang , F. Y. Long , H. T. Liu , D. F. Li , R. Hutton , C. Y. Chen , J. Yan

Results for energy levels, radiative rates and electron impact excitation (effective) collision strengths for transitions in Be-like Cl XIV, K XVI and Ge XXIX are reported. For the calculations of energy levels and radiative rates the…

Solar and Stellar Astrophysics · Physics 2015-06-22 K. M. Aggarwal , F. P. Keenan
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