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Title: Update on the OPAL opacity code

Conference ·
DOI:https://doi.org/10.1063/1.39295· OSTI ID:6991070

Persisting discrepancies between theory and observation in a number of astrophysical properties has led to the conjecture that opacity databases may be inaccurate. The OPAL opacity code has been developed to address this question. The physical basis of OPAL removes several of the approximations present in past calculations. For example, it utilizes a much larger and more detailed set of atomic data than was used to construct the Los Alamos Astrophysical Library. This data is generated online, in LS or intermediate coupling, from prefitted analytic effective potentials and is of similar quality as single configuration, relativistic, self-consistent-field calculations. The OPAL code has been used to calculate opacities for the solar core and for Cepheid variable stars. In both cases, significant increases in the opacity compared to the Los Alamos Astrophysical Library were found. 37 refs., 2 figs., 1 tab.

Research Organization:
Lawrence Livermore National Lab. (LLNL), Livermore, CA (United States)
Sponsoring Organization:
DOE/DP
DOE Contract Number:
W-7405-ENG-48
OSTI ID:
6991070
Report Number(s):
UCRL-JC-103348; CONF-891052-2; ON: DE90009946
Resource Relation:
Journal Volume: 206; Conference: Atomic processes in plasmas, Gaithersburg, MD (USA), 2-5 Oct 1989
Country of Publication:
United States
Language:
English