A dark matter hail: Detecting macroscopic dark matter with asteroids, planetary rings, and craters

Fuente: arXiv
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Autore principale: Picker, Zachary S. C.
Natura: Preprint
Pubblicazione: 2025
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author Picker, Zachary S. C.
author_facet Picker, Zachary S. C.
contents Dark matter could be composed of macroscopic objects with large masses and geometric cross-sections spanning many decades. We investigate the potential interaction of such `stuff-sized' dark matter by considering its interactions with asteroids, planetary rings, and terrestrial bodies. This hail of dark matter could catastrophically destroy these Solar System objects, evaporate them from their orbits, or cause substantial cratering. We estimate these effects and use them to place competitive bounds on a wide, previously-unconstrained swathe of the dark matter parameter space.
format Preprint
id arxiv_https___arxiv_org_abs_2504_07232
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle A dark matter hail: Detecting macroscopic dark matter with asteroids, planetary rings, and craters
Picker, Zachary S. C.
Cosmology and Nongalactic Astrophysics
Earth and Planetary Astrophysics
High Energy Physics - Phenomenology
Dark matter could be composed of macroscopic objects with large masses and geometric cross-sections spanning many decades. We investigate the potential interaction of such `stuff-sized' dark matter by considering its interactions with asteroids, planetary rings, and terrestrial bodies. This hail of dark matter could catastrophically destroy these Solar System objects, evaporate them from their orbits, or cause substantial cratering. We estimate these effects and use them to place competitive bounds on a wide, previously-unconstrained swathe of the dark matter parameter space.
title A dark matter hail: Detecting macroscopic dark matter with asteroids, planetary rings, and craters
topic Cosmology and Nongalactic Astrophysics
Earth and Planetary Astrophysics
High Energy Physics - Phenomenology
url https://arxiv.org/abs/2504.07232