教育背景
- 2022- 2025, 东京科学大学 , 博士
- 2020- 2022, 东京工业大学 , 硕士
- 2016- 2020, 庆应义塾大学 , 学士
工作经历
- 2025-至今, 欧宝app官方网站下载李政道研究所, 博士后
研究方向
- 原始行星盘
- 行星形成理论
代表性论文专著
- T. Okamoto, T. Guillot, R. Marschall, M. Kunitomo, N.F.W. Ligterink, and S. Ida. “Noble gas enrichment in Jovian atmosphere via disk photoevaporation”Accepted by Astronomy and Astrophysics
- T. Okamoto and S. Ida. (2024)“Effects from different grades of stickiness between icy and silicate particles on carbon depletion in protoplanetary disks”Astronomy and Astrophysics, 692, A11, doi: 10.1051/0004-6361/202451908
- A. Morbidelli, Y. Marrocchi, A. Ali Ahmad, A. Bhandare, S. Charnoz, B. Commerçon, C. P. Dullemond, T. Guillot, P. Hennebelle, Y.-N.Lee, F. Lovascio, R. Marschall, B. Marty, A. Maury, and T. Okamoto. (2024)“Formation and evolution of a protoplanetary disk: Combining observations, simulations, and cosmochemical constraints”Astronomy and Astrophysics, 691, A147, doi: 10.1051/0004-6361/202451388.
- S. Arakawa, D. Yamamoto, L. Ishizaki, T. Okamoto, and N. Kawasaki. (2024)“Oxygen Isotope Exchange between Dust Aggregates and Ambient Nebular Gas”The Astrophysical Journal, 974.2, p. 199, doi: 10.3847/1538-4357/ad7795.
- L. Ishizaki, S. Tachibana, T. Okamoto, D. Yamamoto, and S. Ida. (2023)“Effective Reaction Temperatures of Irreversible Dust Chemical Reactions in a Protoplanetary Disk”The Astrophysical Journal, 957.1, p. 47, doi: 10.3847/1538-4357/acf310
- T. Okamoto and S. Ida. (2022)“Monte Carlo Simulation of Dust Particles in a Protoplanetary Disk: Crystalline to Amorphous Silicate Ratio in Comets”The Astrophysical Journal, 928.2, p. 171, doi: 10.3847/1538-4357/ac4bc1.