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Efficient and Accurate Force Replay in Cosmological-baryonic Simulations

We construct time-evolving gravitational potential models for a Milky Way–mass galaxy from the FIRE-2 suite of cosmological-baryonic simulations using basis function expansions. These models capture the angular variation with spherical harmonics for the halo and azimuthal harmonics for the disk, and...

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Autori principali: Arpit Arora, Robyn Sanderson, Christopher Regan, Nicolás Garavito-Camargo, Emily Bregou, Nondh Panithanpaisal, Andrew Wetzel, Emily C. Cunningham, Sarah R. Loebman, Adriana Dropulic, Nora Shipp
Natura: Artigo
Lingua:Inglês
Pubblicazione: IOP Publishing 2024-01-01
Serie:The Astrophysical Journal
Soggetti:
Dark matter
Milky Way evolution
Galaxy dynamics
Accesso online:https://doi.org/10.3847/1538-4357/ad88f0
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