PHANTOM: A Smoothed Particle Hydrodynamics and Magnetohydrodynamics Code for Astrophysics

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

Publikováno v: Publ.Astron.Soc.Austral.
Publ.Astron.Soc.Austral., 2018, 35, pp.31. ⟨10.1017/pasa.2018.25⟩
Publications of the Astronomical Society of Australia
Publications of the Astronomical Society of Australia, 35, e031

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

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::68761a1d0871639ceffb191dbc2505a8
https://hal.archives-ouvertes.fr/hal-01983030

On the accumulation of planetesimals near disc gaps created by protoplanets

Autor: Ben A. Ayliffe, Daniel J. Price, Guillaume Laibe, Matthew R. Bate

Publikováno v: Monthly Notices of the Royal Astronomical Society. 423:1450-1462

We have performed three-dimensional two-fluid (gas–dust) hydrodynamical models of circumstellar discs with embedded protoplanets (3–333 M⊕) and small solid bodies (radii 10 cm to 10 m). We find that high-mass planets (≳ Saturn mass) open suff

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_________::38d7b6ac8bca9b5b641e89e08e54232e
https://doi.org/10.1111/j.1365-2966.2012.20967.x

Planet migration: self-gravitating radiation hydrodynamical models of protoplanets with surfaces

Autor: Ben A. Ayliffe, Matthew R. Bate

Publikováno v: Monthly Notices of the Royal Astronomical Society. 408:876-896

We calculate radial migration rates of protoplanets in laminar minimum mass solar nebula discs using three-dimensional self-gravitating radiation hydrodynamical (RHD) models. The protoplanets are free to migrate, whereupon their migration rates are m

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_________::bee35a478abcb1dc5dcc40de2feb55c8
https://doi.org/10.1111/j.1365-2966.2010.17221.x

Gas accretion by planetary cores

Autor: Ben A. Ayliffe, Matthew R. Bate, Tomonori Usuda, Motohide Tamura, Miki Ishii

We present accretion rates obtained from three-dimensional self-gravitating radiation hydrodynamical models of giant planet growth. We investigate the dependence of accretion rates upon grain opacity and core/protoplanet mass. The accretion rates fou

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::eb4f6bd0efb8aa98c462bb0749d2971f

On the relative motions of dense cores and envelopes in star-forming molecular clouds

Autor: Ben A. Ayliffe, James C. Langdon, Howard S. Cohl, Matthew R. Bate

Hydrodynamical simulations of star formation indicate that the motions of protostars through their natal molecular clouds may be crucial in determining the properties of stars through competitive accretion and dynamical interactions. Walsh, Myers & B

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::18b3bd805a25348e52d7882194bfd364
http://arxiv.org/abs/astro-ph/0611421