Coulomb interaction term of the Hubbard model (or more general
Anderson lattice model) is written in a site-centered, localized
atomic-like orbitals basis set which is not explicitly defined.
Wannier functions (WF) are regarded as a best possible choice for
these orbitals. We propose a method where Wannier functions are
calculated in explicit form and ab-initio full-orbital Hamiltonian
is projected on the Wannier function subspace defined for partially
filled bands of interest. The calculated in this way few (Wannier)
orbitals Hamiltonian together with Coulomb interaction term between
Wannier orbitals (with interaction strength parameters computed in
constrain calculations) is used as ab-initio set up of correlation
problem that can be solved then by one of the methods developed in
many-body community, for example by dynamical mean-field theory
(DMFT). The self-energy operator obtained in such calculations is
defined in Wannier functions basis and can be converted back into
full-orbital Hilbert space, that in its turn can be used for
calculation of the full-orbital interacting Green function . Using
this Green function one can calculate the charge density changed by
correlations together with a new set of Wannier functions and so to
define a fully self-consistent scheme. The Green function can be
also used to calculate spectral, magnetic and electronic properties
of the system under investigation. The results obtained by this
method for SrVO3 and V2O3 are
reported and compared with the previous results by more simple
computation method and new bulk sensitive experimental spectroscopic
data.
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