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|a Snowmass2021 Cosmic Frontier White Paper
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|b Dark Matter Physics from Halo Measurements.
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|a Washington, D.C. :
|b United States. Department of Energy. Office of High Energy Physics ;
|a Oak Ridge, Tenn. :
|b Distributed by the Office of Scientific and Technical Information, U.S. Department of Energy,
|c 2022.
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|a "Other: oai:inspirehep.net:2051347."
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|a Bechtol, Keith; et al.;
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|a The non-linear process of cosmic structure formation produces gravitationally bound overdensities of dark matter known as halos. The abundances, density profiles, ellipticities, and spins of these halos can be tied to the underlying fundamental particle physics that governs dark matter at microscopic scales. Thus, macroscopic measurements of dark matter halos offer a unique opportunity to determine the underlying properties of dark matter across the vast landscape of dark matter theories. This white paper summarizes the ongoing rapid development of theoretical and experimental methods, as well as new opportunities, to use dark matter halo measurements as a pillar of dark matter physics.
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|a United States. Department of Energy. Office of High Energy Physics.
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