Effective collision strengths for forbidden transitions among the 3s(2)3p(3) fine-structure levels of ClIII

Citation
Ca. Ramsbottom et al., Effective collision strengths for forbidden transitions among the 3s(2)3p(3) fine-structure levels of ClIII, M NOT R AST, 307(3), 1999, pp. 669-676
Citations number
22
Categorie Soggetti
Space Sciences
Journal title
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
ISSN journal
00358711 → ACNP
Volume
307
Issue
3
Year of publication
1999
Pages
669 - 676
Database
ISI
SICI code
0035-8711(19990811)307:3<669:ECSFFT>2.0.ZU;2-M
Abstract
Effective collision strengths for the 10 astrophysically important fine-str ucture forbidden transitions among the S-4 degrees, D-2 degrees and P-2 deg rees levels in the 3s(2)3p(3) configuration of Cl III are presented. The ca lculation employs the multichannel R-matrix method to compute the electron- impact excitation collision strengths in a close-coupling expansion, which incorporates the lowest 23 LS target eigenstates of Cl III. These states ar e formed from the 3s(2)3p(3), 3s3p(4), 3s(2)3p(2)3d and 3s(2)3p(2)4s config urations. The Maxwellian-averaged effective collision strengths an presente d graphically for all 10 fine-structure transitions over a wide range of el ectron temperatures appropriate for astrophysical applications [log T(K) = 3.3 - log T(K) = 5.9]. Comparisons are made with the earlier seven-state cl ose-coupling calculation of Butler & Zeippen, and in general excellent agre ement is found in the low-temperature region where a comparison is possible [log T(K) = 3.3 - log T(K) = 4.7], However, discrepancies of up to 30 per cent are found to occur for the forbidden transitions which involve the S-4 degrees ground state level, particularly for the lowest temperatures consi dered. At the higher temperatures, the present data are the only reliable r esults currently available.