  If a light Higgs boson with mass 125 GeV is fermiophobic, or partially
fermiophobic, then the MSSM is excluded. The minimal supersymmetric
fermiophobic Higgs scenario can naturally be formulated in the context of the
NMSSM that admits Z_3 discrete symmetries. In the fermiophobic NMSSM, the SUSY
naturalness criteria are relaxed by a factor N_c y_t^4/g^4 \sim 25, removing
the little hierarchy problem and allowing sparticle masses to be naturally of
order 2--3 TeV. This scale motivates wino or higgsino dark matter. The SUSY
flavour and CP problems as well as the constraints on sparticle and Higgs boson
masses from b \to s\gamma, B_s \to \mu\mu\ and direct LHC searches are relaxed
in fermiophobic NMSSM. The price to pay is that a new, yet unknown, mechanism
must be introduced to generate fermion masses. We show that in the fermiophobic
NMSSM the radiative Higgs boson branchings to \gamma\gamma, \gamma Z can be
modified compared to the fermiophobic and ordinary standard model predictions,
and fit present collider data better. Suppression of dark matter scattering off
nuclei explains the absence of signal in XENON100.
