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Feedback models in galaxy simulations and probing their impact by cosmological hydrodynamic simulations

Published online by Cambridge University Press:  09 June 2023

Kentaro Nagamine Open the ORCID record for Kentaro Nagamine [Opens in a new window]
Kentaro Nagamine*
Affiliation:
Theoretical Astrophysics Group, Department of Earth and Space Science, Graduate School of Science, Osaka University 1-1 Machikaneyama-cho, Toyonaka, Osaka, 560-0043, Japan Department of Physics & Astronomy, University of Nevada, Las Vegas 4505 S. Maryland Pkwy, Las Vegas, NV 89154-4002, USA Kavli IPMU, The University of Tokyo, 5-1-5 Kashiwanoha, Kashiwa, Chiba, 277-8583, Japan email: kn@astro-osaka.jp
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Abstract

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Feedback effects by supernovae (SNe) and active galactic nuclei (AGNs) are believed to be essential for galaxy evolution and shaping present-day galaxies, but their exact mechanisms on galactic scales and their impact on CGM/IGM are not well understood yet. In galaxy formation simulations, it is still challenging to resolve sub-parsec scales, and we need to implement subgrid models to account for the physics on small scales. In this article, we summarize some of the efforts to build more physically based feedback models, discuss about pushing the resolution to its limits in galaxy simulations, testing galaxy formation codes under the AGORA code comparison project, and how to probe the impact of feedback using cosmological hydrodynamic simulations via Lyα absorption and CGM/IGM tomography technique. We also discuss our future directions of research in this field and how we make progress by comparing our simulations with observations.

Keywords

cosmology: theorygalaxies: formationgalaxies: evolutiongalaxies: ISMgalaxies: high-redshifthydrodynamics
Type
Contributed Paper
Information
Proceedings of the International Astronomical Union , Volume 17 , Symposium S373: Resolving the Rise and Fall of Star Formation in Galaxies (Aug 2022) , August 2021 , pp. 283 - 292
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This is an Open Access article, distributed under the terms of the Creative Commons Attribution licence (https://creativecommons.org/licenses/by/4.0/), which permits unrestricted re-use, distribution, and reproduction in any medium, provided the original work is properly cited.
Copyright
© The Author(s), 2023. Published by Cambridge University Press on behalf of International Astronomical Union

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