E(A+M)PEC - An OpenCL Atomic & Molecular Plasma Emission Code For Interstellar Medium Simulations
Miguel A. de Avillez (U. Evora, Portugal), Emanuele Spitoni (U., Evora), and Dieter Breitschwerdt (Tech. Univ. Berlin, Germany)

TL;DR
E(A+M)PEC is an open-source, GPU-accelerated plasma emission code designed for simulating ionization, cooling, and spectra in interstellar medium environments, compatible with various hydrodynamic codes.
Contribution
It introduces a GPU-accelerated, flexible plasma emission code that can be integrated with existing hydrodynamic simulations for ISM studies.
Findings
Efficiently traces ionization and cooling in plasma simulations.
Compatible with NVIDIA GPUs and various hydrodynamic codes.
Enables detailed spectral modeling of the interstellar medium.
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).
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Taxonomy
TopicsPlasma Diagnostics and Applications · Advanced Chemical Physics Studies · Astrophysics and Star Formation Studies
