RASCAS: Resonant line transfer in AMR simulations

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Ada Coda
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RASCAS: Resonant line transfer in AMR simulations

Post by Ada Coda » Wed Feb 26, 2020 3:17 am

RASCAS: Resonant line transfer in AMR simulations

Abstract: The massively parallel code RASCAS (RAdiative SCattering in Astrophysical Simulations) performs radiative transfer on an adaptive mesh with an octree structure using the Monte Carlo technique. The code features full MPI parallelization, domain decomposition, adaptive load-balancing, and a standard peeling algorithm to construct mock observations. The radiative transport of resonant line photons through different mixes of species (e.g. HI, SiII, MgII, FeII), including their interaction with dust, is implemented in a modular fashion to allow new transitions to be easily added to the code. RASCAS may also be used to propagate photons at any wavelength (e.g. stellar continuum or fluorescent lines), and has been designed to be easily customizable and to process simulations of arbitrarily large sizes on large supercomputers.

Credit: Michel-Dansac, Leo; Blaizot, Jeremy; Garel, Thibault; Verhamme, Anne; Kimm, Taysun; Trebitsch, Maxime

Site: https://git-cral.univ-lyon1.fr/rascas/rascas
https://ui.adsabs.harvard.edu/abs/2020arXiv200111252M

Bibcode: 2020ascl.soft02002M

Preferred citation method: https://ui.adsabs.harvard.edu/abs/2020arXiv200111252M

ID: ascl:2002.002

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