A New Generation of Los Alamos Opacity Tables
arXiv:1601.01005 · doi:10.3847/0004-637X/817/2/116
Abstract
We present a new, publicly available, set of Los Alamos OPLIB opacity tables for the elements hydrogen through zinc. Our tables are computed using the Los Alamos ATOMIC opacity and plasma modeling code, and make use of atomic structure calculations that use fine-structure detail for all the elements considered. Our equation-of-state (EOS) model, known as ChemEOS, is based on the minimization of free energy in a chemical picture and appears to be a reasonable and robust approach to determining atomic state populations over a wide range of temperatures and densities. In this paper we discuss in detail the calculations that we have performed for the 30 elements considered, and present some comparisons of our monochromatic opacities with measurements and other opacity codes. We also use our new opacity tables in solar modeling calculations and compare and contrast such modeling with previous work.
References in corpus (4)
- Modules for Experiments in Stellar Astrophysics (MESA): Binaries, Pulsations, and Explosions
- Control and diagnosis of temperature, density, and uniformity in x-ray heated iron/magnesium samples for opacity measurements
- First solar models with OPAS opacity tables
- The Cep/SPB star 12 Lacertae: extended mode identification and complex seismic modelling
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