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Seminars

Implementation and Application of A Multifluid Dust Module in Athena++

by Dr Pinghui Huang (University of Victoria, Canada)

Asia/Shanghai
TDLI

TDLI

Description
Abstract

In recent years, ALMA discovered many protoplanetary disks with sub-structures in dust continuum and gas line observations. These sub-structures are believed in being tightly related to the planet formation and gas-dust interactions in disks. We have implemented a multifluid dust module in the Athena++ MHD code. The module can accommodate an arbitrary number of dust species interacting with the gas via aerodynamic drag, with a number of numerical solvers. In particular, we describe two second-order accurate, fully-implicit solvers that are stable in stiff aerodynamic drags between gas and dust. Moreover, we formulate a consistent treatment of dust concentration diffusion with dust back-reaction, which incorporates momentum diffusion and ensures Galilean invariance. This dust module is implemented to be compatible with most existing features of Athena++ and it will be particularly useful for studies of dust dynamics and planet formation in protoplanetary disks.

Biography

2013-2019,  PhD in Planetary Science, Astronomy, Purple Mountain Observatory, Chinese Academy of Sciences

2019-2022,  Postdoc Researcher, Institute for Advance Study, Tsinghua University

2023-now,   Postdoc Researcher, University of Victoria, Canada

Chair
Dong Lai
Division
Astronomy and Astrophysics
Other information
Venue: N601
Tencent Meetinghttps://net.sjtu.edu.cn/info/1218/3042.htm
Meeting ID940 623 893