The fully relativistic multi-configuration Dirac–Hartree–Fock method for atomic structure calculations for multiply charged ions: the example of Ca XV

2021 ◽  
Vol 75 (1) ◽  
Author(s):  
Najah Alwadie ◽  
Abeer Almodlej ◽  
Nabil Ben Nessib ◽  
Milan S. Dimitrijević
Atoms ◽  
2020 ◽  
Vol 8 (4) ◽  
pp. 85
Author(s):  
Charlotte Froese Fischer ◽  
Andrew Senchuk

Variational methods are used extensively in the calculation of transition rates for numerous lines in a spectrum. In the GRASP code, solutions of the multiconfiguration Dirac–Hartree–Fock (MCDHF) equations that optimize the orbitals are represented by numerical values on a grid using finite differences for integration and differentiation. The numerical accuracy and efficiency of existing procedures are evaluated and some modifications proposed with heavy elements in mind.


Atoms ◽  
2018 ◽  
Vol 6 (2) ◽  
pp. 22 ◽  
Author(s):  
Thomas Gomez ◽  
Taisuke Nagayama ◽  
Chris Fontes ◽  
Dave Kilcrease ◽  
Stephanie Hansen ◽  
...  

Author(s):  
Thomas Gomez ◽  
Taisuke Nagayama ◽  
Dave Kilcrease ◽  
Stephanie Hansen ◽  
Mike Montgomery ◽  
...  

Atomic structure of N-electron atoms is often determined using the Hartree-Fock method, which is an integro-differential equation. The exchange term of the Hartree-Fock equations is usually treated as an inhomogeneous term of a differential equation, or with a local density approximation. This work uses matrix methods to solve for the Hartree-Fock equations, rather than the more commonly-used shooting method to integrate an inhomogeneous differential equation. It is well known that a derivative operator can be expressed as a matrix made of finite-difference coefficients; energy eigenvalues and eigenvectors can be obtained by using computer linear-algebra packages. We extend the same technique to integro-differential equations, where a discretized integral can be written as a sum in matrix form. This method is compared against experiment and standard atomic structure calculations. We also can use this method for free-electron wavefunctions. This technique is important for spectral line broadening in two ways: improving the atomic structure calculations, and improving the motion of the plasma electrons that collide with the atom.


2009 ◽  
Vol 87 (12) ◽  
pp. 1275-1282 ◽  
Author(s):  
Émile Biémont ◽  
Mathieu Clar ◽  
Saturnin Yoca Enzonga ◽  
Vanessa Fivet ◽  
Pascal Quinet ◽  
...  

Relativistic Hartree–Fock and multiconfigurational Dirac–Fock calculations of atomic structure and transition rates have been carried out in trebly ionized lanthanum (La3+, Z = 57). The calculations have to cope with configuration interaction effects but also with the very complex situation of the collapse of the 4f wave function. The calculations are compared to experimental data obtained with beam-foil spectroscopy in the extreme ultraviolet, at ion energies that favour the production of the spectrum La IV. Besides lines known from sliding spark discharges, many more lines are observed that have not yet been identified. Time-resolved measurements yield three level lifetimes in La IV that agree roughly with the results of our own calculations.


New observations of the 5p spectra of Cs i and Ba i are reported. The extreme complexity of the structure does not permit precise configuration labels to be attached to all the excited levels. Nevertheless, more than 160 transitions in Ba i have been ordered into 14 series converging on experimentally known levels of the parent ion. An attempt has been made to analyse the limit structure by comparison with the data for Cs I and Hartree-Fock atomic structure calculations. The results obtained are consistent with previous interpretations of the double ionization anomaly in Ba I. Further comments are made on the comparison between experiment and the predictions of the r.p.a.e. theory for 5p excitation in Ba i. It is shown that the 5p 6 6s 2 S 1/2 -> 5p 5 6s 2 2 P 1/2 and 2 P 3/2 transitions of Cs i have been incorrectly identified and new assignments are proposed.


2020 ◽  
Vol 232 ◽  
pp. 04009
Author(s):  
B. P. McCormick ◽  
A. E. Stuchbery ◽  
A. Goasduff ◽  
A. Kusoglu ◽  
G. Georgiev

A promising technique for g-factor measurements on short-lived nuclear states utilises the hyperfine fields of free ions in vacuum. To fully utilise this technique the hyperfine interaction must be modelled based on atomic structure calculations. Atomic structure calculations were performed using the most recent release of the General Relativistic Atomic Structure Package, and Monte-Carlo simulations of atomic-decay cascades in highly charged ions were developed. The simulations were used to fit experimental data on excited 56Fe ions recoiling in vacuum with a view to determining the first-excited state g factor, g(21+), of 56Fe.


Sign in / Sign up

Export Citation Format

Share Document