Scaling Relations of Halo Cores for Self-Interacting Dark Matter
Henry W. Lin, Abraham Loeb

TL;DR
This paper presents an analytic model predicting that dark matter self-interactions lead to universal scaling relations for halo cores, consistent with recent empirical findings and applicable across different halo masses.
Contribution
It introduces a simple formalism showing that dark matter self-interactions produce universal core scaling relations largely independent of particle physics details.
Findings
Predicted core density and radius relation $ ho_c r_c \,\approx\ 41\,\text{M}_\odot \text{pc}^{-2}$
Scaling relations for core mass, radius, and velocity dispersion match observational data
Predicted scatter in relations agrees with numerical simulations and observations
Abstract
Using a simple analytic formalism, we demonstrate that significant dark matter self-interactions produce halo cores that obey scaling relations nearly independent of the underlying particle physics parameters such as the annihilation cross section and the mass of the dark matter particle. For dwarf galaxies, we predict that the core density and the core radius should obey with a weak mass dependence . Remarkably, such a scaling relation has recently been empirically inferred. Scaling relations involving core mass, core radius, and core velocity dispersion are predicted and agree well with observational data. By calibrating against numerical simulations, we predict the scatter in these relations and find them to be in excellent agreement with existing data. Future observations can test our predictions…
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