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...

وصف كامل

التفاصيل البيبلوغرافية
الحاوية / القاعدة:	The Astrophysical Journal
المؤلفون الرئيسيون:	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
التنسيق:	مقال
اللغة:	الإنجليزية
منشور في:	IOP Publishing 2024-01-01
الموضوعات:	Dark matter Milky Way evolution Galaxy dynamics
الوصول للمادة أونلاين:	https://doi.org/10.3847/1538-4357/ad88f0

مواد مشابهة

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