Phantom : A Smoothed Particle Hydrodynamics and Magnetohydrodynamics Code for Astrophysics

Giuseppe Lodato, Christoph Federrath, Daniel J. Price, James Wurster, Terrence S. Tricco, Chris Nixon, Stéven Toupin, Alex Pettitt, Conrad Chan, Daniel Mentiplay, Guillaume Laibe, Simon Glover, Clare Dobbs, Rebecca Nealon, David Liptai, Hauke Worpel, Clément Bonnerot, Giovanni Dipierro, Giulia Ballabio, Enrico Ragusa, Roberto Iaconi, Thomas Reichardt, Duncan Forgan, Mark Hutchison, Thomas Constantino, Ben Ayliffe, Kieran Hirsh
2018-01-01

SCID:  54.1/zrwx84rg
Abstract 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, dust–gas mixtures, H 2 chemistry, physical viscosity, external forces including numerous galactic potentials, Lense–Thirring precession, Poynting–Robertson drag, and stochastic turbulent driving. Phantom is hereby made publicly available.
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2018-01-01
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Authors
Giuseppe Lodato
Christoph Federrath
Daniel J. Price
James Wurster
Terrence S. Tricco
Chris Nixon
Stéven Toupin
Alex Pettitt
Conrad Chan
Daniel Mentiplay
Guillaume Laibe
Simon Glover
Clare Dobbs
Rebecca Nealon
David Liptai
Hauke Worpel
Clément Bonnerot
Giovanni Dipierro
Giulia Ballabio
Enrico Ragusa
Roberto Iaconi
Thomas Reichardt
Duncan Forgan
Mark Hutchison
Thomas Constantino
Ben Ayliffe
Kieran Hirsh
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