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The First Star-by-star $N$-body/Hydrodynamics Simulation of Our Galaxy Coupling with a Surrogate Model

Fuente: arXiv
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Bibliographic Details
Main Authors: Hirashima, Keiya, Fujii, Michiko S., Saitoh, Takayuki R., Harada, Naoto, Nomura, Kentaro, Yoshikawa, Kohji, Hirai, Yutaka, Asano, Tetsuro, Moriwaki, Kana, Iwasawa, Masaki, Okamoto, Takashi, Makino, Junichiro
Format: Preprint
Published: 2025
Subjects:
Astrophysics of Galaxies
Distributed, Parallel, and Cluster Computing
Machine Learning
Computational Physics
Online Access:
Acceder al recurso
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