### Abstract

Methods. We have carried out intermediate coupling frame transformation R-matrix calculations which include a total of 238 fine-structure levels in both the configuration interaction target and close-coupling collision expansions. These arise from the configurations 1s2 2 {s, p} nl with n = 3−7, and l = 0−4 for n ≤ 5 and l = 0−2 for n = 6,7.

Results. We obtain ordinary collision strengths and Maxwell-averaged effective collision strengths for the electron-impact excitation of all the ions of the Be-like sequence, from B+ to Zn26+. We compare with previous R-matrix calculations and interpolated values for some benchmark ions. We find good agreement for transitions n = 2−2 with previous R-matrix calculations but some disagreements with interpolated values. We also find good agreement for the most intense transitions n = 2−3 which contribute via cascade to the (n = 2) diagnostic radiating levels.

Original language | English |
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Article number | A104 |

Number of pages | 11 |

Journal | Astronomy and Astrophysics |

Volume | 566 |

Early online date | 23 Jun 2014 |

DOIs | |

Publication status | Published - 2014 |

### Fingerprint

### Keywords

- atomic data
- astrophysical plasma
- fusion plasma
- collision strengths

### Cite this

*Astronomy and Astrophysics*,

*566*, [A104]. https://doi.org/10.1051/0004-6361/201423864

}

*Astronomy and Astrophysics*, vol. 566, A104. https://doi.org/10.1051/0004-6361/201423864

**R-matrix electron-impact excitation data for the Be-like iso-electronic sequence.** / Fernández-Menchero, L.; Del Zanna, G.; Badnell, N.R.

Research output: Contribution to journal › Article

TY - JOUR

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

AU - Fernández-Menchero, L.

AU - Del Zanna, G.

AU - Badnell, N.R.

PY - 2014

Y1 - 2014

N2 - Aims. Emission lines from ions in the Be-like isoelectronic sequence can be used for reliable diagnostics of temperature and density of astrophysical and fusion plasmas over a wide range of temperatures. Surprisingly, interpolated data is all that is available for a number of astrophysically important ions.Methods. We have carried out intermediate coupling frame transformation R-matrix calculations which include a total of 238 fine-structure levels in both the configuration interaction target and close-coupling collision expansions. These arise from the configurations 1s2 2 {s, p} nl with n = 3−7, and l = 0−4 for n ≤ 5 and l = 0−2 for n = 6,7.Results. We obtain ordinary collision strengths and Maxwell-averaged effective collision strengths for the electron-impact excitation of all the ions of the Be-like sequence, from B+ to Zn26+. We compare with previous R-matrix calculations and interpolated values for some benchmark ions. We find good agreement for transitions n = 2−2 with previous R-matrix calculations but some disagreements with interpolated values. We also find good agreement for the most intense transitions n = 2−3 which contribute via cascade to the (n = 2) diagnostic radiating levels.

AB - Aims. Emission lines from ions in the Be-like isoelectronic sequence can be used for reliable diagnostics of temperature and density of astrophysical and fusion plasmas over a wide range of temperatures. Surprisingly, interpolated data is all that is available for a number of astrophysically important ions.Methods. We have carried out intermediate coupling frame transformation R-matrix calculations which include a total of 238 fine-structure levels in both the configuration interaction target and close-coupling collision expansions. These arise from the configurations 1s2 2 {s, p} nl with n = 3−7, and l = 0−4 for n ≤ 5 and l = 0−2 for n = 6,7.Results. We obtain ordinary collision strengths and Maxwell-averaged effective collision strengths for the electron-impact excitation of all the ions of the Be-like sequence, from B+ to Zn26+. We compare with previous R-matrix calculations and interpolated values for some benchmark ions. We find good agreement for transitions n = 2−2 with previous R-matrix calculations but some disagreements with interpolated values. We also find good agreement for the most intense transitions n = 2−3 which contribute via cascade to the (n = 2) diagnostic radiating levels.

KW - atomic data

KW - astrophysical plasma

KW - fusion plasma

KW - collision strengths

U2 - 10.1051/0004-6361/201423864

DO - 10.1051/0004-6361/201423864

M3 - Article

VL - 566

JO - Astronomy and Astrophysics

JF - Astronomy and Astrophysics

SN - 0004-6361

M1 - A104

ER -