Review Article

Solar Neutrinos

Figure 21

Expected nuclear recoil spectrum from WIMP scatters in LXe for a spin-independent WIMP-nucleon cross-section of (red solid) and ā€‰ (red dashed) and a WIMP mass of 100 GeV/ , along with the differential energy spectrum for pp (blue) and Be (cyan) neutrinos, and the electron recoil spectrum from the double beta decay of Xe (green). Assumptions are 99.5% discrimination of electronic recoils, 50% acceptance of nuclear recoils, and 80% flat analysis cuts acceptance. Taken from [185].
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