  We investigate the comparative studies of cosmological baryon asymmetry in
different neutrino mass models with and without {\theta}_13 by considering the
three diagonal form of Dirac neutrino mass matrices, down-quark (4,2), up-quark
(8,4) and charged lepton (6,2). The predictions of any models with {\theta}_13
are consistent in all the three stages of leptogenesis calculations and the
results are better than the predictions of any models without {\theta}_13 which
are consistent in a piecemeal manner with the observational data. For the best
model, the normal hierarchy Type-IA for charged lepton (6,2) without
{\theta}_13, the predicted inflaton mass required to produce the observed
baryon asymmetry is found to be 3.6x10 to the power 10 GeV corresponding to
reheating temperature TR 4.5x10 to the power 6 GeV, while for the same model
with {\theta}_13, the inflaton mass is 2.24x10 to the power 11 GeV, TR 4.865x10
to the power 6 GeV and weak scale gravitino mass m(2 divided by 3) 100 GeV
without causing the gravitino problem. These values apply to the recent
discovery of Higgs boson of mass 125 GeV. The relic abundance of gravitino is
proportional to the reheating temperature of the thermal bath. One can have the
right order of relic dark matter abundance only if the reheating temperature is
bounded to below 10 to the power 7 GeV.
