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High Angular Momentum Halo Gas: a Feedback and Code-Independent Prediction of LCDM

Abstract:

We investigate angular momentum acquisition in Milky Way sized galaxies by comparing five high resolution zoom-in simulations, each implementing identical cosmological initial conditions, but utilizing different hydrodynamic codes: Enzo, Art, Ramses, Arepo, and Gizmo-PSPH. Each code implements a distinct set of feedback and star formation prescriptions. We find that while many galaxy and halo properties vary between the different codes (and feedback prescriptions), there is qualitative agreem...

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Stewart, K More by this author
Oñorbe, J More by this author
Bullock, J More by this author
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URN:
uuid:cdf8f28c-ac5c-4bfa-a1b1-9f18187966c6
Source identifiers:
631498
Local pid:
pubs:631498
Keywords:

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