# Oscillator strengths and transition probabilities from the Breit–Pauli R-matrix method: Ne IV

## Abstract

The atomic parameters–oscillator strengths, line strengths, radiative decay rates (A), and lifetimes–for fine structure transitions of electric dipole (E1) type for the astrophysically abundant ion Ne IV are presented. The results include 868 fine structure levels with n≤ 10, l≤ 9, and 1/2≤J≤ 19/2 of even and odd parities, and the corresponding 83,767 E1 transitions. The calculations were carried out using the relativistic Breit–Pauli R-matrix method in the close coupling approximation. The transitions have been identified spectroscopically using an algorithm based on quantum defect analysis and other criteria. The calculated energies agree with the 103 observed and identified energies to within 3% or better for most of the levels. Some larger differences are also noted. The A-values show good to fair agreement with the very limited number of available transitions in the table compiled by NIST, but show very good agreement with the latest published multi-configuration Hartree–Fock calculations. The present transitions should be useful for diagnostics as well as for precise and complete spectral modeling in the soft X-ray to infra-red regions of astrophysical and laboratory plasmas. -- Highlights: •The first application of BPRM method for accurate E1 transitions in Ne IV is reported. •Amount of atomic data (n going upmore »

- Authors:

- Publication Date:

- OSTI Identifier:
- 22439761

- Resource Type:
- Journal Article

- Journal Name:
- Atomic Data and Nuclear Data Tables

- Additional Journal Information:
- Journal Volume: 100; Journal Issue: 5; Other Information: Copyright (c) 2014 Elsevier Science B.V., Amsterdam, The Netherlands, All rights reserved.; Country of input: International Atomic Energy Agency (IAEA); Journal ID: ISSN 0092-640X

- Country of Publication:
- United States

- Language:
- English

- Subject:
- 73 NUCLEAR PHYSICS AND RADIATION PHYSICS; ALGORITHMS; ASTROPHYSICS; BREIT-WIGNER FORMULA; E1-TRANSITIONS; ELECTRIC DIPOLES; FINE STRUCTURE; HARTREE-FOCK METHOD; LIFETIME; NEON IONS; OSCILLATOR STRENGTHS; PROBABILITY; R MATRIX; RADIATIVE DECAY; RELATIVISTIC RANGE; SOFT X RADIATION

### Citation Formats

```
Nahar, Sultana N., E-mail: nahar@astronomy.ohio-state.edu.
```*Oscillator strengths and transition probabilities from the Breit–Pauli R-matrix method: Ne IV*. United States: N. p., 2014.
Web. doi:10.1016/J.ADT.2014.02.001.

```
Nahar, Sultana N., E-mail: nahar@astronomy.ohio-state.edu.
```*Oscillator strengths and transition probabilities from the Breit–Pauli R-matrix method: Ne IV*. United States. doi:10.1016/J.ADT.2014.02.001.

```
Nahar, Sultana N., E-mail: nahar@astronomy.ohio-state.edu. Mon .
"Oscillator strengths and transition probabilities from the Breit–Pauli R-matrix method: Ne IV". United States. doi:10.1016/J.ADT.2014.02.001.
```

```
@article{osti_22439761,
```

title = {Oscillator strengths and transition probabilities from the Breit–Pauli R-matrix method: Ne IV},

author = {Nahar, Sultana N., E-mail: nahar@astronomy.ohio-state.edu},

abstractNote = {The atomic parameters–oscillator strengths, line strengths, radiative decay rates (A), and lifetimes–for fine structure transitions of electric dipole (E1) type for the astrophysically abundant ion Ne IV are presented. The results include 868 fine structure levels with n≤ 10, l≤ 9, and 1/2≤J≤ 19/2 of even and odd parities, and the corresponding 83,767 E1 transitions. The calculations were carried out using the relativistic Breit–Pauli R-matrix method in the close coupling approximation. The transitions have been identified spectroscopically using an algorithm based on quantum defect analysis and other criteria. The calculated energies agree with the 103 observed and identified energies to within 3% or better for most of the levels. Some larger differences are also noted. The A-values show good to fair agreement with the very limited number of available transitions in the table compiled by NIST, but show very good agreement with the latest published multi-configuration Hartree–Fock calculations. The present transitions should be useful for diagnostics as well as for precise and complete spectral modeling in the soft X-ray to infra-red regions of astrophysical and laboratory plasmas. -- Highlights: •The first application of BPRM method for accurate E1 transitions in Ne IV is reported. •Amount of atomic data (n going up to 10) is complete for most practical applications. •The calculated energies are in very good agreement with most observed levels. •Very good agreement of A-values and lifetimes with other relativistic calculations. •The results should provide precise nebular abundances, chemical evolution etc.},

doi = {10.1016/J.ADT.2014.02.001},

journal = {Atomic Data and Nuclear Data Tables},

issn = {0092-640X},

number = 5,

volume = 100,

place = {United States},

year = {2014},

month = {9}

}