Please use this identifier to cite or link to this item: http://hdl.handle.net/2381/43628
Title: PHANTOM: A Smoothed Particle Hydrodynamics and Magnetohydrodynamics Code for Astrophysics
Authors: Price, DJ
Wurster, J
Tricco, TS
Nixon, C
Toupin, S
Pettitt, A
Chan, C
Mentiplay, D
Laibe, G
Glover, S
Dobbs, C
Nealon, R
Liptai, D
Worpel, H
Bonnerot, C
Dipierro, G
Ballabio, G
Ragusa, E
Federrath, C
Iaconi, R
Reichardt, T
Forgan, D
Hutchison, M
Constantino, T
Ayliffe, B
Hirsh, K
Lodato, G
First Published: 25-Sep-2018
Publisher: Cambridge University Press (CUP) for Astronomical Society of Australia
Citation: Publications of the Astronomical Society of Australia, 2018, 35, e031, 82 pages
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, H2 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.
DOI Link: 10.1017/pasa.2018.25
ISSN: 1323-3580
eISSN: 1448-6083
Links: https://www.cambridge.org/core/journals/publications-of-the-astronomical-society-of-australia/article/phantom-a-smoothed-particle-hydrodynamics-and-magnetohydrodynamics-code-for-astrophysics/182F569916933E20686B8032111A6182
http://hdl.handle.net/2381/43628
Version: Post-print
Status: Peer-reviewed
Type: Journal Article
Rights: Copyright © 2018, Cambridge University Press (CUP) for Astronomical Society of Australia. Deposited with reference to the publisher’s open access archiving policy. (http://www.rioxx.net/licenses/all-rights-reserved)
Description: The file associated with this record is under embargo until 6 months after publication, in accordance with the publisher's self-archiving policy. The full text may be available through the publisher links provided above.
Appears in Collections:Published Articles, Dept. of Physics and Astronomy

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