For a given nonlocal density , the auxiliary functions or , which define its quasi-local approximation, can be calculated as their best possible approximations in terms of local densities. However, the usefulness of the expansion relies on the assumption that generic forms of these functions can be estimated and then applied to all many-body systems of a given kind.
The standard
Slater approximation [24,25], which is routinely used to evaluate the
Coulomb exchange energy (cf. Refs. [26,27]), corresponds to
The NV functions , , and are plotted
in Fig. 1 with solid, dashed, and dotted lines,
respectively. One can see that for large , functions
and have zeros close to one another and the same signs.
Indeed, asymptotically both behave like
. Therefore,
the gauge-invariance condition (19) can be satisfied almost everywhere.
On the other hand, functions and
, have asymptotically opposite signs, and the
corresponding gauge-invariance condition (27) can be almost
nowhere satisfied. Nevertheless, as discussed in Sec. 2.2,
what really matters are the moments of interaction (23) and
(29), where functions and are probed
only within the range of the interaction, that is, up to
1-2. Therefore, for the NV expansion, one can safely
use approximations:
By the same token, we can replace in Eqs. (31)-(33)
the Bessel functions by Gaussians having the same leading-order
dependence on , namely,
|