Halo Profile Evolution and Velocity Bias
Kwan Chuen Chan

TL;DR
This paper introduces a model that incorporates finite halo profiles into velocity bias calculations, revealing significant $k^2$ corrections that persist over time and emphasizing the importance of profile evolution in halo modeling.
Contribution
The paper generalizes the fluid equation approximation for halos to include finite profiles, deriving $k^2$ correction terms in velocity bias and validating the model with numerical profile evolution.
Findings
Profile correction leads to significant $k^2$ terms in velocity bias.
Spherical collapse model reasonably describes halo profile evolution.
Profile evolution impacts halo velocity bias calculations.
Abstract
We propose a simple model that elucidates the generation of halo velocity bias. The fluid equation approximation is often adopted in modelling the evolution of the halo density field. In this approach, halos are often taken to be point particles even though in reality they are finite-sized objects. In this paper, we generalize the fluid equation approximation to halos to include the finite extent of halos by taking into account the halo profile. We compute the perturbation of the halo density and velocity field to second order and find that the profile correction gives rise to correction terms in Fourier space. These corrections are more important for velocity than for density. In particular, the profile correction generates correction term in the velocity bias and the correction terms do not decay away in the long term limit, but it is not constant. We model the halo…
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