Simulation code for fluids in three dimensions

dc.contributor.affiliationUniversity of Helsinki - Dahl, Jani
dc.contributor.authorDahl, Jani
dc.contributor.roleRummukainen, Kari Supervisor
dc.contributor.roleHindmarsh, Mark Supervisor
dc.contributor.roleWeir, David Supervisor
dc.date.accessioned2025-03-24T15:11:13Z
dc.date.issued2024-01-29
dc.date.issued2024-01-29
dc.descriptionThis 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.
dc.identifierhttps://doi.org/10.5281/zenodo.10580342
dc.identifier.urihttps://hydatakatalogi-test-24.it.helsinki.fi/handle/123456789/9027
dc.rightsOpen
dc.rights.licensecc-by-4.0
dc.titleSimulation code for fluids in three dimensions
dc.typesoftware
dc.typesoftware
Zenodo


: