TY - JOUR
T1 - Phantom
T2 - A smoothed particle hydrodynamics and magnetohydrodynamics code for astrophysics
AU - Price, Daniel J.
AU - Wurster, James
AU - Tricco, Terrence S.
AU - Nixon, Chris
AU - Toupin, Stéven
AU - Pettitt, Alex
AU - Chan, Conrad
AU - Mentiplay, Daniel
AU - Laibe, Guillaume
AU - Glover, Simon
AU - Dobbs, Clare
AU - Nealon, Rebecca
AU - Liptai, David
AU - Worpel, Hauke
AU - Bonnerot, Clément
AU - Dipierro, Giovanni
AU - Ballabio, Giulia
AU - Ragusa, Enrico
AU - Federrath, Christoph
AU - Iaconi, Roberto
AU - Reichardt, Thomas
AU - Forgan, Duncan
AU - Hutchison, Mark
AU - Constantino, Thomas
AU - Ayliffe, Ben
AU - Hirsh, Kieran
AU - Lodato, Giuseppe
N1 - 88 pages, 60 figures, accepted to PASA. Code available from https://phantomsph.bitbucket.io/
PY - 2018/9/25
Y1 - 2018/9/25
N2 - We present Phantom, a fast, parallel, modular and low-memory smoothed particle hydrodynamics and magnetohydrodynamics code developed over the last decade for astrophysical applications in three dimensions. The code has been developed with a focus on stellar, galactic, planetary and high energy astrophysics and has already been used widely for studies of accretion discs and turbulence, from the birth of planets to how black holes accrete. Here we describe and test the core algorithms as well as modules for magnetohydrodynamics, self-gravity, sink particles, H_2 chemistry, dust-gas mixtures, physical viscosity, external forces including numerous galactic potentials as well as implementations of Lense-Thirring precession, Poynting-Robertson drag and stochastic turbulent driving. Phantom is hereby made publicly available.
AB - We present Phantom, a fast, parallel, modular and low-memory smoothed particle hydrodynamics and magnetohydrodynamics code developed over the last decade for astrophysical applications in three dimensions. The code has been developed with a focus on stellar, galactic, planetary and high energy astrophysics and has already been used widely for studies of accretion discs and turbulence, from the birth of planets to how black holes accrete. Here we describe and test the core algorithms as well as modules for magnetohydrodynamics, self-gravity, sink particles, H_2 chemistry, dust-gas mixtures, physical viscosity, external forces including numerous galactic potentials as well as implementations of Lense-Thirring precession, Poynting-Robertson drag and stochastic turbulent driving. Phantom is hereby made publicly available.
KW - astro-ph.IM
KW - astro-ph.EP
KW - astro-ph.GA
KW - astro-ph.HE
KW - astro-ph.SR
UR - https://www.scopus.com/pages/publications/85055290100
U2 - 10.1017/pasa.2018.25
DO - 10.1017/pasa.2018.25
M3 - Article
SN - 1323-3580
VL - 35
JO - Publications of the Astronomical Society of Australia
JF - Publications of the Astronomical Society of Australia
M1 - e031
ER -