E(A+M)PEC - An OpenCL Atomic & Molecular Plasma Emission Code For Interstellar Medium Simulations
Astrophysics of Galaxies
2019-08-19 v1 High Energy Astrophysical Phenomena
Abstract
E(A+M)PEC traces the ionization structure, cooling and emission spectra of plasmas. It is written in OpenCL, runs in NVIDIA Graphics Processor Units and can be coupled to any HD or MHD code to follow the dynamical and thermal evolution of any plasma in, e.g., the interstellar medium (ISM).
Cite
@article{arxiv.1109.5362,
title = {E(A+M)PEC - An OpenCL Atomic & Molecular Plasma Emission Code For Interstellar Medium Simulations},
author = {Miguel A. de Avillez and Emanuele Spitoni and Dieter Breitschwerdt},
journal= {arXiv preprint arXiv:1109.5362},
year = {2019}
}
Comments
To be published in "Advances in Computational Astrophysics: Methods, Tools and Outcomes", R. Dolcetta, M. Limongi, A. Tornambe (Editors), ASP Conf. Series