Proposes muscovite mica paleodetector framework for heavy composite dark matter using Sedov-Taylor melt modeling validated by SRIM/TRIM, X-ray fluorescence readout, projected sensitivities, and critique of prior etched mica exclusions.
Loosely bound composite dark matter,
3 Pith papers cite this work. Polarity classification is still indexing.
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The nuclear star cluster around Sgr A* is the dominant source of gravitationally boosted dark matter in the Milky Way, with particles up to ~25,000 km/s that enhance sub-GeV detection prospects independently of the DM model.
Review of confining dark sectors summarizing dark matter candidates, abundance mechanisms, discovery channels, and applications to the abundance similarity puzzle.
citing papers explorer
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New Windows on Heavy Dark Matter: Mineral Melt Modelling and X-Ray Readout for Muscovite Mica
Proposes muscovite mica paleodetector framework for heavy composite dark matter using Sedov-Taylor melt modeling validated by SRIM/TRIM, X-ray fluorescence readout, projected sensitivities, and critique of prior etched mica exclusions.
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Boosted Dark Matter from Sagittarius A$^\star$
The nuclear star cluster around Sgr A* is the dominant source of gravitationally boosted dark matter in the Milky Way, with particles up to ~25,000 km/s that enhance sub-GeV detection prospects independently of the DM model.
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Rich Phenomenology from Simple Ingredients: A Review of Confining Dark Sectors
Review of confining dark sectors summarizing dark matter candidates, abundance mechanisms, discovery channels, and applications to the abundance similarity puzzle.