Abstract
Widths and shifts are calculated in the electron impact approximation, using close-coupling theory, for the transitions 2s-2p, 2s-3p, 2p-3s, 2p-3d, 3s-3p and 3p-3d in Be II, B III, C IV, O VI and Ne VIII, and the transitions 2s2 1S-2s2p 1Po, 2s2p 3Po-2p2 3P, 2s2p 1Po-2p2 1D and 1S in C III, O V and Ne VII. Results are compared with those from previous calculations and from experiments. Approximate formulae must be used to estimate linewidths for some 106 transitions which are of importance for the calculation of stellar envelope opacities. Results for the quantum mechanical calculations for 42 transitions are used to obtain provisional best estimates for the parameters in these formulae.
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
More From: Journal of Physics B: Atomic, Molecular and Optical Physics
Disclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.