Dark matter detection in two easy steps
arXiv:1312.1363 · doi:10.1103/PhysRevD.89.055008
Abstract
Multi-component dark matter particles may have a more intricate direct detection signal than simple elastic scattering on nuclei. In a broad class of well-motivated models the inelastic excitation of dark matter particles is followed by de-excitation via -decay. In experiments with fine energy resolution, such as many decay experiments, this motivates a highly model-independent search for the sidereal daily modulation of an unexpected line. Such a signal arises from two-step WIMP interaction: the WIMP is first excited in the lead shielding and subsequently decays back to the ground state via the emission of a monochromatic within the detector volume. We explore this idea in detail by considering the model of magnetic inelastic WIMPs, and take a sequence of CUORE-type detectors as an example. We find that under reasonable assumptions about detector performance it is possible to efficiently explore mass splittings of up to few hundreds of keV for a WIMP of weak-scale mass and transitional magnetic moments. The modulation can be cheaply and easily enhanced by the presence of additional asymmetric lead shielding. We devise a toy simulation to show that a specially designed asymmetric shielding may result in up to diurnal modulations of the two-step WIMP signal, leading to additional strong gains in sensitivity.
14 pages, 14 figures
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