Simulation code for fluids in three dimensions

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2024-01-29, 2024-01-29

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software
software

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This simulation code is used to conduct simulations of relativistic fluids with non-relativistic bulk velocities in three dimensions under the ultra-relativistic equation of state. The code has been used to conduct the simulations in the paper: Primordial acoustic turbulence: three-dimensional simulations and gravitational wave predictions by Jani Dahl, Mark Hindmarsh, Kari Rummukainen, and David Weir. For further information about the code, see the README.md file.

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