Ramses is an open source code written by Romain Teyssier to model astrophysical systems, featuring self-gravitating, magnetised, compressible, radiative fluid flow. Based on the Adaptive Mesh Refinement (AMR) technique, it has been widely used for cosmological simulations of the Universe, isolated as well as cosmological resimulations of individual galaxies, simulations of molecular clouds, star formation, supernovae remnants, accretion disks around black holes and planets.
Ramses is currently used by a constantly growing community of astrophysicists all around the world, with many groups in France, United Kingdom, Danemark, South Korea and the United States.
This website’s goal is to promote the activities of the Ramses community in France and is edited by the SNO Ramses.
We are testing Github Discussions as a new forum. Start asking and answering questions about Ramses on this new tool !
The SPHINX suite of cosmological radiation-hydrodynamical simulations is designed to simultaneously capture large-scale reionization and the escape of ionizing radiation from thousands of resolved galaxies during the first billion years of the Universe. The SPHINX volumes resolve haloes down to the atomic cooling limit and model the interstellar medium of galaxies with ≈ 10 parsec…