%0 Generic %1 price2017phantom %A Price, Daniel J. %A Wurster, James %A Nixon, Chris %A Tricco, Terrence S. %A Toupin, Stéven %A Pettitt, Alex %A Chan, Conrad %A Laibe, Guillaume %A Glover, Simon %A Dobbs, Clare %A Nealon, Rebecca %A Liptai, David %A Worpel, Hauke %A Bonnerot, Clément %A Dipierro, Giovanni %A Ragusa, Enrico %A Federrath, Christoph %A Iaconi, Roberto %A Reichardt, Thomas %A Forgan, Duncan %A Hutchison, Mark %A Constantino, Thomas %A Ayliffe, Ben %A Mentiplay, Daniel %A Hirsh, Kieran %A Lodato, Giuseppe %D 2017 %K code phantom sph %T Phantom: A smoothed particle hydrodynamics and magnetohydrodynamics code for astrophysics %U http://arxiv.org/abs/1702.03930 %X 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.

@misc{price2017phantom, 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, 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.}, added-at = {2017-02-15T14:09:57.000+0100}, author = {Price, Daniel J. and Wurster, James and Nixon, Chris and Tricco, Terrence S. and Toupin, Stéven and Pettitt, Alex and Chan, Conrad and Laibe, Guillaume and Glover, Simon and Dobbs, Clare and Nealon, Rebecca and Liptai, David and Worpel, Hauke and Bonnerot, Clément and Dipierro, Giovanni and Ragusa, Enrico and Federrath, Christoph and Iaconi, Roberto and Reichardt, Thomas and Forgan, Duncan and Hutchison, Mark and Constantino, Thomas and Ayliffe, Ben and Mentiplay, Daniel and Hirsh, Kieran and Lodato, Giuseppe}, biburl = {https://www.bibsonomy.org/bibtex/29e86e1d92f9b39fa472e97d0e53e74ea/miki}, description = {[1702.03930] Phantom: A smoothed particle hydrodynamics and magnetohydrodynamics code for astrophysics}, interhash = {64154e9770b10a8fdb08cb7e3eb4ebd7}, intrahash = {9e86e1d92f9b39fa472e97d0e53e74ea}, keywords = {code phantom sph}, note = {cite arxiv:1702.03930Comment: 77 pages, 51 figures, 335 equations, submitted to PASA. Code available from https://phantomsph.bitbucket.io/}, timestamp = {2017-02-15T14:09:57.000+0100}, title = {Phantom: A smoothed particle hydrodynamics and magnetohydrodynamics code for astrophysics}, url = {http://arxiv.org/abs/1702.03930}, year = 2017 }