Compact Halo around the Sun Accreted after Dark Matter Dissipative Self Interaction
Ran Huo

TL;DR
This paper models the formation of a compact dark matter halo around the Sun due to dissipative self-interactions, revealing a density profile that could impact dark matter detection efforts.
Contribution
It develops a Boltzmann equation framework to describe dark matter accretion onto the Sun, providing the first detailed density profile prediction for such a halo.
Findings
Dark matter forms a halo around the Sun with a density profile proportional to r^{-1.6}.
Local dark matter density near the Sun can be significantly higher than the galactic background.
Potential for enhanced dark matter signals in solar gamma-ray observations.
Abstract
If dark matter particle can be decelerated due to its dissipative self scattering, except for sinking at the galaxy scale to speed up structure formation, it can also be accreted onto local celestial bodies such as the Sun, forming a compact halo. With some simplified assumptions we develop the Boltzmann equation set based on the partition function of the elliptical orbits, and numerically solve it for the accretion process. We find that the orbited dark matter particles will form a halo around the Sun, with the density profile well fitted to be proportional to in a wide range of radius. While around the earth such local halo contribution is always several orders below the galactic component, in a very small region centered around the Sun the sunk dark matter particles can lead to a halo density several orders larger than the background galactic component, in particular in…
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Taxonomy
TopicsDark Matter and Cosmic Phenomena · Advanced Thermodynamics and Statistical Mechanics · Solar and Space Plasma Dynamics
