Halo spin and elongation create a direction-dependent clustering signal that is governed by alignment with the surrounding cosmic web, whereas orientation-averaged secondary bias is governed by tidal anisotropy.
D., Smith , R., & Shinn , J.-H
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Anisotropic Secondary Bias of Dark Matter Haloes in a $\Lambda$CDM Universe
Halo spin and elongation create a direction-dependent clustering signal that is governed by alignment with the surrounding cosmic web, whereas orientation-averaged secondary bias is governed by tidal anisotropy.