Cosmic vorticity and the origin of halo spins
Noam I Libeskind, Yehuda Hoffman, Matthias Steinmetz, Stefan, Gottloeber, Alexander Knebe, Steffen Hess

TL;DR
This study uses cosmological simulations to show that halo spins are strongly aligned with vorticity in the nonlinear phase of structure formation, indicating a two-phase angular momentum growth process.
Contribution
It demonstrates the transition from shear-driven to vorticity-driven angular momentum acquisition in halos, highlighting the role of vorticity near virialization.
Findings
Halo spin aligns with ambient vorticity.
Vorticity is perpendicular to the fastest collapsing axis.
Results are consistent across halo masses and environments.
Abstract
In the standard model of cosmology, structure emerges out of non-rotational flow and the angular momentum of collapsing halos is induced by tidal torques. The growth of halo angular momentum in the linear and quasi-linear phases is associated with a shear, curl-free, flow and it is well described within the linear framework of tidal torque theory (TTT). However, TTT is rendered irrelevant as haloes approach turn around and virialization. At that stage the flow field around halos has non-zero vorticity. Using a cosmological simulation, we have examined the importance of the curl of the velocity field (vorticity) in determining halo spin, finding a strong alignment between the two. We have also examined the alignment of vorticity with the principle axes of the shear tensor, finding that it tends to be perpendicular to the axis along which material is collapsing fastest (e1). This behavior…
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