  We show that in the CMSSM with the non-holomorphic soft SUSY breaking terms,
the Yukawa coupling unification of the third family fermions at the GUT scale,
called $ t-b-\tau $ Yukawa unification (YU), is possible under the recent
collider and Dark Matter results. The YU parameter can also be found $
R_{tb\tau} \approx 1 $, called perfect unification. We find that the squark
masses exceed 3 TeV while the stau can be considerably lighter. In the case of
YU, the $ \tan\beta $ is in the interval $ [46,55] $. We obtain bino-like dark
matter (DM) of mass in the range of $ 0.6$ TeV $ \lesssim m_{\chi_{1}^{0}}
\lesssim 1.3 $ TeV where the recent Dark Matter direct detection limits are
also satisfied. We also identify A-resonance solutions which reduce the relic
abundance of LSP neutralino down to the ranges compatible with the current
Planck measurements.
