  We study the implications of the Dark-LMA solution to the solar neutrino
problem for neutrino-less double beta decay ($0\nu\beta\beta$ ). We show that
while the predictions for the effective mass governing $0\nu\beta\beta$ remains
unchanged for the inverted mass scheme, that for normal ordering becomes higher
for the Dark-LMA parameter space and moves into the "desert region" between the
two. This sets a new goal for sensitvity reach for the next generation
experiments if no signal is found for the inverted ordering by the future
search programmes.
