arXiv · hep-ph/9409275
A New Technique for Detecting Supersymmetric Dark Matter
Abstract
We estimate the event rate for excitation of atomic transition by photino-like dark matter. For excitations of several eV, this event rate can exceed naive cross-section by many orders of magnitude. Although the event rate for these atomic excitation is smaller than that of nuclear recoil off of non-zero spin nuclei, the photons emitted by the deexcitation are easier to detect than low-energy nuclear recoils. For many elements, there are several low-lying states with comparable excitation rates, thus, spectral ratios could be used to distinguish signal from background.
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Glenn D. Starkman, David N. Spergel. 1994-09-13. A New Technique for Detecting Supersymmetric Dark Matter. https://doi.org/10.1103/physrevlett.74.2623
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