Fig. 4: Present limits and future sensitivities to spin-independent (SI) dark matter-nucleon cross section.
From: Progress and prospects in the underground laboratories' search for dark matter
Solid lines are limits at 90% confidence level (C.L.) from previous or currently running dark matter direct detection experiments28,32,37,49,51,54,120,147,148,149,150,151,152,153,154,155,156. Dashed lines are projected 90% C.L. exclusion sensitivity of future experiments77,78,88,92,122,157,158,159. The shaded gray region is the neutrino fog for a xenon target.
