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        <title>How a Scalar Field Halo Forms Around a Binary Black Hole</title>
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        <description>An animated explainer showing how ultralight scalar fields — a candidate for dark matter — can form a dense halo around a binary black hole system. Based on research from Roy et al. (2025), arXiv:2510.17967. The scalar halo extracts orbital energy from the binary, producing a unique gravitational-wave signature that LIGO could detect. This animation shows a cross-section of the halo reaching ~480 km radius at densities around 10⁹ g/cm³, with spiral density waves transporting energy out of the binary orbit. Part of the companion piece 'Dear Gravity, What The Fuck Was That?' at magnus919.com</description>
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