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Title: Low-energy fine-structure resonances in photoionization of O ii

Journal Article · · Physical Review. A
;  [1];  [2];  [3]
  1. Department of Astronomy, Ohio State University, Columbus, Ohio 43210 (United States)
  2. Facultad de Educaci, Pontificia Universidad Catholica de Chile, Avda Vicua Mackenna 4860, Macul, Santiago (Chile)
  3. Institut fuer Theoretische Physik, Teilinstitut 1, D-70550 Stuttgart (Germany)

Resonant features in low-energy photoionization cross sections are reported in coupled-channel calculations for O ii including relativistic fine structure. The calculations reveal extensive near-threshold resonant structures in the small energy region between the fine structure levels of the ground state 2p{sup 2}({sup 3}P{sub 0,1,2}) of the residual ion O iii. Although the resonances have not yet been observed, they are similar to other experimentally observed features. They are expected to significantly enhance the very-low-temperature dielectronic recombination rates, potentially leading to the resolution of an outstanding nebular abundances anomaly. Higher energy partial and total photoionization cross sections of the ground configuration levels 2p{sup 3}({sup 4}S{sub 3/2}{sup o},{sup 2}D{sub 3/2,5/2}{sup o},{sup 2}P{sub 1/2,3/2}{sup o}) are found to be in agreement with experimental measurements on synchrotron-based photon sources [1-3], thereby identifying the excited O iii levels present in the ion beams. These are also the first results from a recently developed version of Breit-Pauli R-matrix (BPRM) codes, with inclusion of two-body magnetic interaction terms. The improved relativistic treatment could be important for other astrophysical applications and for more precise benchmarking of experimental measurements.

OSTI ID:
21529009
Journal Information:
Physical Review. A, Vol. 82, Issue 6; Other Information: DOI: 10.1103/PhysRevA.82.065401; (c) 2010 American Institute of Physics; ISSN 1050-2947
Country of Publication:
United States
Language:
English