Development of 1-D non-ideal MHD simulation code towards understanding Long-term Evolution of Protoplanetary Disk
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arXiv
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| Autori principali: | , , , |
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| Natura: | Preprint |
| Pubblicazione: |
2025
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| _version_ | 1866911098330939392 |
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| author | Kobayashi, Yudai Takaishi, Daisuke Tsukamoto, Yusuke Basu, Shantanu |
| author_facet | Kobayashi, Yudai Takaishi, Daisuke Tsukamoto, Yusuke Basu, Shantanu |
| contents | We developed a one-dimensional magnetohydrodynamic (MHD) simulation code to investigate the long-term evolution of protoplanetary disks with low computational cost. In this simulation code, the physical processes necessary for protostellar formation and protoplanetary disk evolution, such as magnetic braking, non-ideal MHD effects, and angular momentum transport due to viscosity, are implemented. Using this simulation code, we performed the simulations of the long-term evolution of protoplanetary disks starting from the molecular cloud. Our simulation results suggest that the disk size and mass are a few tens of au and $\sim 0.01 M_\odot$ at $10^5$ years after protostellar formation. These values were relatively consistent with observations. The disk evolves through magnetic braking, and its radial profiles are consistent with the analytical solutions of previous studies. Our simulation code will be an important tool for studying the long-term evolution of protoplanetary disks. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2508_06089 |
| institution | arXiv |
| publishDate | 2025 |
| record_format | arxiv |
| spellingShingle | Development of 1-D non-ideal MHD simulation code towards understanding Long-term Evolution of Protoplanetary Disk Kobayashi, Yudai Takaishi, Daisuke Tsukamoto, Yusuke Basu, Shantanu Earth and Planetary Astrophysics Instrumentation and Methods for Astrophysics We developed a one-dimensional magnetohydrodynamic (MHD) simulation code to investigate the long-term evolution of protoplanetary disks with low computational cost. In this simulation code, the physical processes necessary for protostellar formation and protoplanetary disk evolution, such as magnetic braking, non-ideal MHD effects, and angular momentum transport due to viscosity, are implemented. Using this simulation code, we performed the simulations of the long-term evolution of protoplanetary disks starting from the molecular cloud. Our simulation results suggest that the disk size and mass are a few tens of au and $\sim 0.01 M_\odot$ at $10^5$ years after protostellar formation. These values were relatively consistent with observations. The disk evolves through magnetic braking, and its radial profiles are consistent with the analytical solutions of previous studies. Our simulation code will be an important tool for studying the long-term evolution of protoplanetary disks. |
| title | Development of 1-D non-ideal MHD simulation code towards understanding Long-term Evolution of Protoplanetary Disk |
| topic | Earth and Planetary Astrophysics Instrumentation and Methods for Astrophysics |
| url | https://arxiv.org/abs/2508.06089 |