The energies obtained were
eV (LDA),
eV (VMC
with LDA orbitals),
eV (VMC with natural orbitals),
eV (DMC with LDA orbitals), and
eV (DMC with
natural orbitals). The VMC wave function appears to show a very
slight improvement with natural orbitals compared with LDA
orbitals. However, to within statistical accuracy, the DMC energies
obtained with LDA and natural orbitals are the same. This indicates
that the nodal surfaces given by the LDA and natural orbitals are of
the same quality.
This was investigated by performing DMC calculations in silicon with
an fcc simulation cell containing 16 atoms. The smaller simulation
cell enabled a large number of independent configurations to be
obtained rapidly. Wave functions expanded in a basis of atom-centered
Gaussians were obtained from the HF and DFT code
CRYSTAL95. [130] Special care was taken to ensure that the
LDA and HF calculations were done in equivalent ways to try and
eliminate any bias in the comparison. A basis set of four
uncontracted
functions and one
polarization function per
pseudo-atom was optimized separately for each calculation. The
quality of the basis set is high - to obtain the same energy within a
plane wave calculation would require a basis set cutoff of 12.5 Ry.
The same non-local LDA pseudopotential was used as in the earlier
calculations. The Ewald interaction was used in the many-body
Hamiltonian to avoid any charge-density dependence on the
interaction. Approximately
walker moves obtained DMC
total energies and statistical accuracies of -107.488(3) eV per atom
and -107.464(3) eV per atom for the LDA and HF guiding wave functions
respectively.
The walker energies were approximately normally distributed. Using a
conventional students t-test, [19] the 95%
confidence interval on the difference in energies obtained was
eV per atom, showing that for this system it is very likely
that the DMC energy from a determinant of LDA orbitals is lower than
that from a determinant of HF orbitals. Therefore, for this system, a
determinant of LDA orbitals has a marginally better nodal structure
than a determinant of HF orbitals.