[ascl:1709.002]
PHANTOM: Smoothed particle hydrodynamics and magnetohydrodynamics code
Price, Daniel J.;
Wurster, James;
Nixon, Chris;
Tricco, Terrence S.;
Toupin, Stéven;
Pettitt, Alex;
Chan, Conrad;
Laibe, Guillaume;
Glover, Simon;
Dobbs, Clare;
Nealon, Rebecca;
Liptai, David;
Worpel, Hauke;
Bonnerot, Clément;
Dipierro, Giovanni;
Ragusa, Enrico;
Federrath, Christoph;
Iaconi, Roberto;
Reichardt, Thomas;
Forgan, Duncan;
Hutchison, Mark;
Constantino, Thomas;
Ayliffe, Ben;
Mentiplay, Daniel;
Hirsh, Kieran;
Lodato, Giuseppe
Phantom is a smoothed particle hydrodynamics and magnetohydrodynamics code focused on stellar, galactic, planetary, and high energy astrophysics. It is modular, and handles sink particles, self-gravity, two fluid and one fluid dust, ISM chemistry and cooling, physical viscosity, non-ideal MHD, and more. Its modular structure makes it easy to add new physics to the code.
- Code site:
-
https://phantomsph.github.io/
https://github.com/danieljprice/phantom
- Used in:
-
https://ui.adsabs.harvard.edu/abs/2015A%26A...583A.133P
https://ui.adsabs.harvard.edu/abs/2010MNRAS.406.1659P
- Described in:
-
https://ui.adsabs.harvard.edu/abs/2018PASA...35...31P
- Bibcode:
- 2017ascl.soft09002P