English

Optab: Public code for generating gas opacity tables for radiation hydrodynamics simulations

Instrumentation and Methods for Astrophysics 2022-03-14 v1 Earth and Planetary Astrophysics High Energy Astrophysical Phenomena Solar and Stellar Astrophysics

Abstract

We have developed a public code, Optab, that outputs Rosseland, Planck, and two-temperature Planck mean gas opacity tables for radiation hydrodynamics simulations in astrophysics. The code is developed for modern high-performance computing, being written in Fortran 90 and using Message Passing Interface and Hierarchical Data Format, Version 5. The purpose of this work is to provide a platform on which users can generate opacity tables for their own research purposes. Therefore, the code has been designed so that a user can easily modify, change, or add opacity sources in addition to those already implemented, which include bremsstrahlung, photoionization, Rayleigh scattering, line absorption, and collision-induced absorption. In this paper, we provide details of the opacity calculations in our code and present validation tests to evaluate the performance of our code.

Keywords

Cite

@article{arxiv.2112.05689,
  title  = {Optab: Public code for generating gas opacity tables for radiation hydrodynamics simulations},
  author = {Shigenobu Hirose and Peter Hauschildt and Takashi Minoshima and Kengo Tomida and Takayoshi Sano},
  journal= {arXiv preprint arXiv:2112.05689},
  year   = {2022}
}

Comments

Astronomy and Astrophysics, in press

R2 v1 2026-06-24T08:12:38.593Z