  We revisit MSSM scenarios with light neutralino as a dark matter candidate in
view of the latest LHC and dark matter direct and indirect detection
experiments. We show that scenarios with a very light neutralino (~ 10 GeV) and
a scalar bottom quark close in mass, can satisfy all the available constraints
from LEP, Tevatron, LHC, flavour and low energy experiments and provide
solutions in agreement with the bulk of dark matter direct detection
experiments, and in particular with the recent CDMS results.
