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AbstractAbstract
[en] Signals for both direct and indirect dark matter detection depend on the phase-space distribution of dark matter. The possibility of structures with high physical density, known as caustics, has provided an opportunity to increase the discovery potential of the Axion Dark Matter eXperiment (ADMX). I discuss the formation of dark matter caustics and consequences of the caustic ring model for ADMX.
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1 Jan 2010; 7 p; Axions 2010; Gainesville, FL (United States); 15 Jan 2010; LA-UR--10-1454; AC52-06NA25396; Available from http://permalink.lanl.gov/object/tr?what=info:lanl-repo/lareport/LA-UR-10-01454; PURL: https://www.osti.gov/servlets/purl/992163-Ixhowb/
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