  We present a summary of future prospects for direct detection of dark matter
within the GeV/c2 to TeV/c2 mass range. This is paired with a new definition of
the neutrino fog in order to better quantify the rate of diminishing returns on
sensitivity due to irreducible neutrino backgrounds. A survey of dark matter
candidates predicted to fall within this mass range demonstrates that fully
testing multiple well-motivated theo-ries will require expanding the
currently-funded generation of experiments down to and past the neutrino fog.
We end with the status and plans for next-generation exper-iments and novel R&D
concepts which will get us there.
