Transition probabilities for forbidden lines in the 3p3 configuration

Details Transition probabilities for forbidden lines in the 3p3 configuration Transition probabilities for forbidden lines in the 3p3 configuration

Jan 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982mnras.198..127m&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 198, Jan. 1982, p. 127-139.

Astronomy and Astrophysics

Astrophysics

142

Astronomical Spectroscopy, Atomic Structure, Forbidden Bands, Isoelectronic Sequence, Transition Probabilities, Computer Programs, Magnetic Dipoles, Nebulae, Wave Functions

Scientific paper

Radiative transition probabilities are calculated, using the atomic structure computer program SUPERSTRUCTURE, for the forbidden lines in the ground configuration 1s2 2s2 2p6 3s2 3p3 of all the members of the P I isoelectronic sequence up to Ni XIV. Improvements are achieved over previous work in this area by the use of such procedures as: (1) configuration interaction, (2) relativistic corrections to the magnetic dipole operator, (3) special radial wave functions, and (4) semi-empirical term energy corrections. The importance of the changes described is discussed in the context of astrophysical problems.

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