WhiskyMHD: General Relativistic Magnetohydrodynamics

Discussion topics for individual codes
Post Reply
User avatar
Guardian of the Codes
Posts: 1130
Joined: Wed Aug 04, 2004 4:18 pm
Location: Washington, DC

WhiskyMHD: Numerical Code for General Relativistic Magnetohydrodynamics

Post by owlice » Sat Oct 30, 2010 5:48 pm

WhiskyMHD: Numerical Code for General Relativistic Magnetohydrodynamics

Abstract: Whisky is a code to evolve the equations of general relativistic hydrodynamics (GRHD) and magnetohydrodynamics (GRMHD) in 3D Cartesian coordinates on a curved dynamical background. It was originally developed by and for members of the EU Network on Sources of Gravitational Radiation and is based on the Cactus Computational Toolkit. Whisky can also implement adaptive mesh refinement (AMR) if compiled together with Carpet.

Whisky has grown from earlier codes such as GR3D and GRAstro_Hydro, but has been rewritten to take advantage of some of the latest research performed here in the EU. The motivation behind Whisky is to compute gravitational radiation waveforms for systems that involve matter. Examples would include the merger of a binary system containing a neutron star, which are expected to be reasonably common in the universe and expected to produce substantial amounts of radiation. Other possible sources are given in the projects list.

Credit: Baiotti, Luca; Giacomazzo, Bruno; Hawke, Ian; et al.

Site: https://whiskycode.org/

Bibcode: 2010ascl.soft10084B

Preferred citation method: https://ui.adsabs.harvard.edu/abs/2005PhRvD..71b4035B https://ui.adsabs.harvard.edu/abs/2007CQGra..24S.235G https://ui.adsabs.harvard.edu/abs/2005PhRvD..71j4006H

ID: ascl:1010.084
Last edited by Ada Coda on Sun Oct 18, 2020 7:39 pm, edited 1 time in total.
Reason: Updated code entry.
Code-seeking owl at your service

Post Reply