Search Swinburne Research Bank
Please use this identifier to cite or link to this item: http://hdl.handle.net/1959.3/41432
|Download PDF (Published version) (Adobe Acrobat PDF, -1 bytes)|
- 3D SPH simulations of grain growth in protoplanetary disks
- Laibe, Guillaume; Gonzalez, Jean-Francois; Fouchet, Laure; Maddison, Sarah T.
- We present the first results of the treatment of grain growth in our 3D, two-fluid (gas+dust) SPH code describing protoplanetary disks. We implement a scheme able to reproduce the variation of grain sizes caused by a variety of physical processes and test it with the analytical expression of grain growth given by Stepinski & Valageas (1997) in simulations of a typical T Tauri disk around a one solar mass star. The results are in agreement with a turbulent growing process and validate the method. We are now able to simulate the grain growth process in a protoplanetary disk given by a more realistic physical description, currently under development. We discuss the implications of the combined effect of grain growth and dust vertical settling and radial migration on subsequent planetesimal formation.
- Publication type
- Conference paper
- Research centre
- Swinburne University of Technology. Faculty of Information and Communication Technologies. Centre for Astrophysics and Supercomputing
- Exoplanets: detection, formation and dynamics: proceedings of the International Astronomical Union Symposium 249, Suzhou, China, 22-26 October 2007 / Yi-Sui Sun, Sylvio Ferraz Mello and Ji-Lin Zhou (eds.), Vol. 3, no. (2008), pp. 385-388
- Publication year
- Numerical methods; Planetary systems; Protoplanetary disks; SPH
- Cambridge University Press
- 1743-9213 (series ISSN)
- 9780521874717, 0521874718
- Publisher URL
- Copyright © International Astronomical Union 2008. The published version is reproduced in accordance with the copyright policy of the publisher.
- Full text
- Peer reviewed