Scaling of collision strengths for highly-excited states of ions of the H- and He-like sequences
Fernández-Menchero, L. and Del Zanna, G. and Badnell, N. R. (2016) Scaling of collision strengths for highly-excited states of ions of the H- and He-like sequences. Astronomy and Astrophysics, 592. A135. ISSN 0004-6361 (https://doi.org/10.1051/0004-6361/201628484)
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Abstract
Emission lines from highly-excited states (n ≥ 5) of H- and He-like ions have been detected in astrophysical sources and fusion plasmas. For such excited states, R-matrix or distorted wave calculations for electron-impact excitation are very limited, due to the large size of the atomic basis set needed to describe them. Calculations for n ≥ 6 are also not generally available. We study the behaviour of the electron-impact excitation collision strengths and effective collision strengths for the most important transitions used to model electron collision dominated astrophysical plasmas, solar, for example. We investigate the dependence on the relevant parameters: the principal quantum number n or the nuclear charge Z. We also estimate the importance of coupling to highly-excited states and the continuum by comparing the results of different sized calculations. We provide analytic formulae to calculate the electron-impact excitation collision strengths and effective collision strengths to highly-excited states (n ≥ 8) of H- and He-like ions. These extrapolated effective collision strengths can be used to interpret astrophysical and fusion plasma via collisional-radiative modelling.
ORCID iDs
Fernández-Menchero, L., Del Zanna, G. and Badnell, N. R. ORCID: https://orcid.org/0000-0001-7418-7996;-
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Item type: Article ID code: 58263 Dates: DateEvent31 August 2016Published15 August 2016Published Online6 June 2016AcceptedNotes: Reproduced with permission from Astronomy & Astrophysics, © ESO Subjects: Science > Astronomy
Science > PhysicsDepartment: Faculty of Science > Physics Depositing user: Pure Administrator Date deposited: 26 Oct 2016 09:16 Last modified: 11 Nov 2024 11:32 Related URLs: URI: https://strathprints.strath.ac.uk/id/eprint/58263