arXiv · hep-ph/9412237
Direct detection of dark matter in SU(5)xU(1) supergravity
Abstract
We compute the scattering rates for the lightest neutralino $χ^0_1$ in the forthcoming germanium $(^{73}{\rm Ge}+^{76}{\rm Ge})$ detector and a proposed lead detector $(^{207}{\rm Pb})$, within the framework of $SU(5)\times U(1)$ supergravity. We find that in only a small portion ($\lsim10\%$) of the parameter spaces of this class of models, are the rates in the germanium detector above the expected initial experimental sensitivity of 0.1 events/kg/day. However, a much larger portion ($\lsim40\%$) of the parameter spaces could be probed with an improved background rejection capability (0.01 events/kg/day) and/or a more sensitive detector $(^{207}{\rm Pb})$.
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X. Wang, J. Lopez, D. Nanopoulos. 1994-12-05. Direct detection of dark matter in SU(5)xU(1) supergravity. https://doi.org/10.1016/0370-2693(95)00096-4
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