Development of SPH: Toward Understanding of Disk-planet Interaction Near the Disk Inner Edge

Yuri FUJII; Kazunari IWASAKI; Yusuke TSUKAMOTO; Shu-ichiro INUTSUKA

Presentation information

Oral

Symbol P (Space and Planetary Sciences) » P-PS Planetary Sciences

[P-PS21_29AM2] Planetary Sciences

Tue. Apr 29, 2014 11:00 AM - 12:45 PM 416 (4F)

Convener:*Satoshi Okuzumi(Graduate School of Science, Tokyo Institute of Technology), Kosuke Kurosawa(Planetary Exploration Research Center, Chiba Institute of Technology), Chair:Peng Hong(Department of Complexity Science and Engineering, Graduate School of Frontier Sciences, The University of Tokyo), Masanori Onishi(Graduate School of Science, Kobe University)

12:30 PM - 12:45 PM

[PPS21-P06_PG] Development of SPH: Toward Understanding of Disk-planet Interaction Near the Disk Inner Edge

3-min talk in an oral session

*Yuri FUJII¹, Kazunari IWASAKI¹, Yusuke TSUKAMOTO¹, Shu-ichiro INUTSUKA¹ (1.Nagoya University)

Keywords:exoplanet, protoplanetary disk, smoothed particle hydrodynamics

Recent observations of exoplanets reveal the existence of close-in planets. These planets are thought to form in outer disks and migrate inward because of the disk-planet interaction. If there are disk inner cavities, planets can stop migrating and stay in close-in orbit. Disk evolution is highly affected by these planets. Thus, the understanding of the interaction between disks and close-in planets is crucial. In this study, we develop a numerical scheme to investigate the interaction between disks and planets. Although the grid-based schemes are widely used in this context, there are difficulties in calculating with a disk inner cavity or eccentric planets. These difficulties can be removed by smoothed particle hydrodynamics (SPH) with high accuracy. In this presentation, we will talk about the development of code and the performance evaluation.