期刊
PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF AUSTRALIA
卷 35, 期 -, 页码 -出版社
CAMBRIDGE UNIV PRESS
DOI: 10.1017/pasa.2018.25
关键词
accretion, accretion disks; hydrodynamics; ISM: general; magnetohydrodynamics (MHD); methods: numerical
资金
- Australian Research Council (ARC) [FT130100034]
- Science and Technology Facilities Council [ST/M005917/1]
- ARC Discovery Projects [DP150104329, DP170100603]
- Deutsche Forschungsgemeinschaft [SFB 881]
- European Research Council via the ERC Advanced Grant 'STARLIGHT' [339177]
- Astronomy Australia Ltd
- Pawsey National Supercomputing Centre
- Swinburne
- Australian Government's Education Investment Fund
- [DP130102078]
- [DP1094585]
- STFC [ST/M005917/1] Funding Source: UKRI
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.
作者
我是这篇论文的作者
点击您的名字以认领此论文并将其添加到您的个人资料中。
推荐
暂无数据