  Leptogenesis is an attractive scenario in which neutrino masses and baryon
asymmetry of the Universe are explained together under a minimal set of
assumptions.
  After formulating the problem of initial conditions and introducing the
strong thermal leptogenesis conditions as solution, we show that, within the
framework provided by the \soten~model of leptogenesis, the latter lead to a
set of testable predictions on the same neutrino parameters currently under
experimental investigations.
  The emerging scenario selects the normal ordering of the neutrino mass
pattern, a large value for the reactor mixing angle, $2\deg \lesssim
\theta_{13} \lesssim 20\deg$, as well as a non maximal atmospheric mixing
angle, $16\deg \lesssim \theta_{23} \lesssim 41\deg$, and favours negative
values for the Dirac phase \delta. The signature of the proposed strong thermal
\soten~solutions is in the relation obtained between the effective Majorana
mass and the lightest neutrino mass: $m_{ee} \approx 0.8 \, m_1 \approx 15 $
meV.
