Abstract
The relativistic CI method is used to determine transition probabilities for electric quadrupole transitions between the 1s 2 2s 2 2p 2 (3 P 0,3 P 2,1 D 2) and 1s 2 2p 4 3 P 2 even levels of OIII. The variation of the results with the number of configurations used is discussed, both for the Coulomb and the Babushkin (length) gauge.
Similar content being viewed by others
References
Marketos, P., Lambropoulos, P.: Z. Phys. D15, 185 (1990)
Marketos, P., Zambetaki, I., Kleidis, M.: Z. Phys. D27, 17 (1993)
Marketos, P., Zambetaki, I.: J. Phys. B26, L249 (1993)
Dyall, K.G., Grant, I.P., Johnson, C.T., Parpia, F.A., Plummer, E.P.: Comp. Phys. Com.55, 425 (1989)
Baluja, K.L., Doyle, J.G.: J. Phys. B14, L11 (1981)
Bhatia, A.K., Doschek, G.A., Feldman, U.: Astron. Astrophys.76, 359 (1979)
Garstang, R.H.: Planetary Nebulae, IAU Symposium No. 34, pp. 143. Osterbrock, D.E., O'Dell, C.R. (eds.). Dordrecht: Reidel 1968
Nussbaumer, H., Rusca, C.: Astron. Astrophys.72, 129 (1979)
Cheng, K.T., Kim, Y.-K., Desclaux, J.P.: At. Data Nucl. Data Tables24, 111 (1979)
Nussbaumer, H.: Astrophys. J.166, 411 (1971)
Froese Fischer, C., Saha, H.P.: Phys. Scr.32, 181 (1985)
Grant, I.P.: J. Phys. B7, 1458 (1974)
Wiese, W.L., Smith, M.W., Glenon, B.M.: Atomic Transition Probabilities, vol. I, NSRDS-NBS-4, 1966