Japan Geoscience Union Meeting 2022

Presentation information

[J] Oral

M (Multidisciplinary and Interdisciplinary) » M-GI General Geosciences, Information Geosciences & Simulations

[M-GI33] Computational sciences on the universe, galaxies, stars, planets, and their environments

Mon. May 23, 2022 10:45 AM - 12:15 PM Exhibition Hall Special Setting (1) (Exhibition Hall 8, Makuhari Messe)

convener:Yoshi-Yuki Hayashi(Department of Planetology/CPS, Graduate School of Science, Kobe University), convener:Junichiro Makino(Kobe University), Kanya Kusano(Institute for Space-Earth Environmental Research, Nagoya University), convener:Eiichiro Kokubo(Division of Science, National Astronomical Observatory of Japan), Chairperson:Junichiro Makino(Kobe University)

11:15 AM - 11:30 AM

[MGI33-08] Development of simulation code for planetary system formation (GPLUM) : Prospect by high-resolution N-body simulation

*Yota Ishigaki1,2, Eiichiro Kokubo3, Masaki Fujimoto2, Junichiro Makino4,5 (1.University of Tokyo, 2.Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency, 3.National Astronomical Observatory of Japan, 4.Kobe University, 5.RIKEN Center for computational Science)

Keywords:planet formation, N-body simulation

It is generally accepted that planetary systems are formed from protoplanetary disks surrounding a central star. In the standard model, planets are formed by the accretion of planetesimals in the disk. The accretion process of planetesimals is mainly investigated using N-body simulations of planetesimal systems.

In this study, we have developed a new N-body simulation code, GPLUM, using the particle-particle particle-tree scheme (P3T scheme). We have implemented a more efficient algorithm than the conventional P3T code in GPLUM, which enables us to perform global, high-resolution N-body simulations. With GPLUM we can conduct new experiments such as parameter surveys using N-body simulations.

We present results of large-scale N-body simulations of the formation process of planetary systems by GPLUM using the supercomputer Fugaku. We investigate the resolution dependence of N-body simulations of the planet formation process by the high-resolution simulation. By comparing the results of N-body simulations with N=104, 105, and 106, we discuss how the accretion process of planetesimals and protoplanets is affected by the resolution of N-body simulations.

We also investigate the planetesimal accretion with a new collision model, which is derived from the SPH collision experiments. We discuss the dependence of the planetesimal growth on the collision model. We also present the future prospects of planet formation simulations using high-resolution N-body simulations with GPLUM on Fugaku.