Dark matter halo mass functions and density profiles from mass and energy cascade
Zhijie (Jay) Xu

TL;DR
This paper presents an analytical framework for dark matter halo mass functions and density profiles based on mass and energy cascade theory, predicting a cuspy inner slope of -4/3 and matching simulation results.
Contribution
It introduces a novel analytical model deriving halo mass functions and density profiles without collapse assumptions, incorporating energy cascade concepts.
Findings
Predicts a halo inner density slope of -4/3
Derives a halo mass function with power-law and exponential behavior
Matches results with Illustris simulation data
Abstract
Without relying on a spherical or ellipsoidal collapse model, we analytically derive the halo mass function and cuspy halo density (inner slope of -4/3) based on the mass and energy cascade theory in dark matter flow. The hierarchical halo structure formation leads to halo or particle random walk with a position-dependent waiting time . The inverse mass cascade from small to large scales leads to the halo random walk in mass space with , where is the halo mass and is a halo geometry parameter with predicted value of 2/3. The corresponding Fokker-Planck solution for halo random walk in mass space gives rise to the halo mass function with a power-law behavior on small scale and exponential decay on large scale. This can be further improved by considering two different for haloes below and above a critical mass scale ,…
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Taxonomy
TopicsDark Matter and Cosmic Phenomena · Galaxies: Formation, Evolution, Phenomena · Cosmology and Gravitation Theories
