Published July 15, 2016 | Version v1

The Phantom SPH code

  • 1. Monash Centre for Astrophysics
  • 2. University of Leicester

Description

I will present the capabilities of the Phantom SPH code for global simulations of dust and gas in protoplanetary discs. I will present our new algorithms for simulating both small and large grains in discs, as well as our progress towards simulating evolving grain populations and coupling with radiation. Finally, I will discuss our recent applications to HL Tau and the physics of dust gap opening.

 

Files

planets2016-PriceD_poster.pdf

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