The collective hamiltonian will be constructed from the potential
energy function with the zero-point vibration term and the mass
parameters obtained within the cranking model as well as the generator
coordinate method (GCM+GOA).
First the calculation will be performed for the well known nuclei
in order to fix the parameters of the models. The obtained results for the
atomic masses, the MSR values and their isotopic shifts, as well as on
the Q2 and B(E2) values and positions of the lowest excited states of nuclei
will be compared with the newest experimental data. Then the models will be
applied to nuclei far from -stability line (close to the proton
and neutron drip lines) and from the superheavy region.