### Abstract

We present results for the electron-impact excitation of all Ne-like ions from Na+ to Kr26+ obtained using the intermediate-coupling frame transformation R-matrix approach. For each ion's calculation, the close-coupling expansion is taken to be the 113 LS terms (209 levels) belonging to the configurations [1s(2)]2s(2)2p(6), 2s(2)2p(5){3, 4, 5}l, 2s2p(6){3, 4, 5}l (l is an element of s, p, d, f, and g), and 2s(2)2p(5){6, 7} l' (l' is an element of s, p, and d). An additional configuration interaction effect arising from configurations of 2s(2)2p(4)3l{3, 4, 5}l" (l" is an element of s, p, d, f and g) was included in the target expansion. A detailed comparison of the target structure has been made for six specific ions (Si4+, Ar8+, Ca10+, Fe16+, Ni18+, and Kr26+) spanning the sequence to assess the accuracy for the entire sequence. Effective collision strengths (Gamma s) are presented at temperatures ranging from 2x10(2)(q+1)(2) K to 2x10(6)(q+1)(2) K (where q is the residual charge of ions, i. e. Z-10). Detailed comparisons for the.s are made with the results of previous calculations for several ions, which span the sequence. Furthermore, we examine the iso-electronic trends of effective collision strengths as a function of temperature. The present results are the only R-matrix ones for the majority of the ions and the most extensive and complete data for modelling to-date.

Original language | English |
---|---|

Number of pages | 20 |

Journal | Astronomy and Astrophysics |

Volume | 518 |

Issue number | July/August |

DOIs | |

Publication status | Published - 3 Sep 2010 |

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### Keywords

- atomic data
- atomic processes
- plasmas
- collision strengths
- FE-XVII
- energy-levels
- breit-pauli
- NI-XIX
- laboratory measurements
- rate coefficients
- radiative rates
- emission-lines

### Cite this

*Astronomy and Astrophysics*,

*518*(July/August). https://doi.org/10.1051/0004-6361/201014170

}

*Astronomy and Astrophysics*, vol. 518, no. July/August. https://doi.org/10.1051/0004-6361/201014170

**R-matrix electron-impact excitation data for the Ne-like iso-electronic sequence.** / Liang, G. Y.; Badnell, N. R.

Research output: Contribution to journal › Article

TY - JOUR

T1 - R-matrix electron-impact excitation data for the Ne-like iso-electronic sequence

AU - Liang, G. Y.

AU - Badnell, N. R.

PY - 2010/9/3

Y1 - 2010/9/3

N2 - We present results for the electron-impact excitation of all Ne-like ions from Na+ to Kr26+ obtained using the intermediate-coupling frame transformation R-matrix approach. For each ion's calculation, the close-coupling expansion is taken to be the 113 LS terms (209 levels) belonging to the configurations [1s(2)]2s(2)2p(6), 2s(2)2p(5){3, 4, 5}l, 2s2p(6){3, 4, 5}l (l is an element of s, p, d, f, and g), and 2s(2)2p(5){6, 7} l' (l' is an element of s, p, and d). An additional configuration interaction effect arising from configurations of 2s(2)2p(4)3l{3, 4, 5}l" (l" is an element of s, p, d, f and g) was included in the target expansion. A detailed comparison of the target structure has been made for six specific ions (Si4+, Ar8+, Ca10+, Fe16+, Ni18+, and Kr26+) spanning the sequence to assess the accuracy for the entire sequence. Effective collision strengths (Gamma s) are presented at temperatures ranging from 2x10(2)(q+1)(2) K to 2x10(6)(q+1)(2) K (where q is the residual charge of ions, i. e. Z-10). Detailed comparisons for the.s are made with the results of previous calculations for several ions, which span the sequence. Furthermore, we examine the iso-electronic trends of effective collision strengths as a function of temperature. The present results are the only R-matrix ones for the majority of the ions and the most extensive and complete data for modelling to-date.

AB - We present results for the electron-impact excitation of all Ne-like ions from Na+ to Kr26+ obtained using the intermediate-coupling frame transformation R-matrix approach. For each ion's calculation, the close-coupling expansion is taken to be the 113 LS terms (209 levels) belonging to the configurations [1s(2)]2s(2)2p(6), 2s(2)2p(5){3, 4, 5}l, 2s2p(6){3, 4, 5}l (l is an element of s, p, d, f, and g), and 2s(2)2p(5){6, 7} l' (l' is an element of s, p, and d). An additional configuration interaction effect arising from configurations of 2s(2)2p(4)3l{3, 4, 5}l" (l" is an element of s, p, d, f and g) was included in the target expansion. A detailed comparison of the target structure has been made for six specific ions (Si4+, Ar8+, Ca10+, Fe16+, Ni18+, and Kr26+) spanning the sequence to assess the accuracy for the entire sequence. Effective collision strengths (Gamma s) are presented at temperatures ranging from 2x10(2)(q+1)(2) K to 2x10(6)(q+1)(2) K (where q is the residual charge of ions, i. e. Z-10). Detailed comparisons for the.s are made with the results of previous calculations for several ions, which span the sequence. Furthermore, we examine the iso-electronic trends of effective collision strengths as a function of temperature. The present results are the only R-matrix ones for the majority of the ions and the most extensive and complete data for modelling to-date.

KW - atomic data

KW - atomic processes

KW - plasmas

KW - collision strengths

KW - FE-XVII

KW - energy-levels

KW - breit-pauli

KW - NI-XIX

KW - laboratory measurements

KW - rate coefficients

KW - radiative rates

KW - emission-lines

UR - http://www.scopus.com/inward/record.url?scp=77956308467&partnerID=8YFLogxK

U2 - 10.1051/0004-6361/201014170

DO - 10.1051/0004-6361/201014170

M3 - Article

VL - 518

JO - Astronomy and Astrophysics

JF - Astronomy and Astrophysics

SN - 0004-6361

IS - July/August

ER -