Dense Dark Matter Hairs Spreading Out from Earth, Jupiter and Other Compact Bodies
Gary Prezeau

TL;DR
This paper predicts the existence of dark matter hairs—concentrated filaments extending from celestial bodies—arising from the fine-grained structure of dark matter halos, with significant density enhancements detectable near planetary cores.
Contribution
It introduces the concept of dark matter hairs resulting from the stream structure of halos, supported by analytical models and numerical simulations using the FAIR algorithm.
Findings
Dark matter hairs have density enhancements up to 10^8 for Jupiter.
The roots of hairs are located at specific distances from planetary centers with enhancements up to 10^11.
Hairs can reveal planetary interior density layers.
Abstract
It is shown that compact bodies project out strands of concentrated dark matter filaments henceforth simply called hairs. These hairs are a consequence of the fine-grained stream structure of dark matter halos, and as such constitute a new physical prediction of CDM. Using both an analytical model of planetary density and numerical simulations utilizing the Fast Accurate Integrand Renormalization (FAIR) algorithm (a fast geodesics calculator described below) with realistic planetary density inputs, dark matter streams moving through a compact body are shown to produce hugely magnified dark matter densities along the stream velocity axis going through the center of the body. Typical hair density enhancements are for Earth and for Jupiter. The largest enhancements occur for particles streaming through the core of the body that mostly focus at a single point called…
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