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arXiv · 2202.12247

Constraints on dark matter self-interaction from galactic core size

Tirtha Sankar Ray·Sambo Sarkar·Abinash Kumar Shaw
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Abstract

Self-interaction of particulate dark matter may help thermalising the central region of the galactic halo and driving core formation. The core radius is expectedly sensitive to the self-interaction strength of dark matter (DM). In this paper we study the feasibility of constraining dark matter self-interaction from the distribution of the core radius in isolated haloes. We perform systematic DM only $N$-body simulations of spherically symmetric isolated galactic haloes in the mass range of $10^{10} $-$10^{15}M_{\odot}$, incorporating the impact of isotropic DM self-interaction. Comparing the simulated profiles with the observational data, we provide a conservative upper limit on the self-interaction cross-section, $ \sigma/m < $ $ 9.8 $ $\ \rm cm^2 /\rm gm $ at $ 95 \% $ confidence level. We report significant dependence of the derived bounds on the galactic density distribution models assumed for the analysis.

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Tirtha Sankar Ray, Sambo Sarkar, Abinash Kumar Shaw. 2022-02-24. Constraints on dark matter self-interaction from galactic core size. https://doi.org/10.1088/1475-7516%2F2022%2F09%2F011

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