The result (10.5) can be generalized to any monotonically increasing potentials V such that V ′(r)∕r is decreasing, in the form
![]() | (10.7) |
The proof is given in Ref. [98], in a polished form due to A. Martin. Some comments are in order:
i) The inequality is saturated in the harmonic-oscillator case. This explains why, with general potentials, the actual value is not too far from the bound, as seen previously in the linear case.
ii) For a power-law potential V = 1 2Brβ with 1 ≤ β ≤ 2, one can get a simple analytic bound on δ12 for the ground state by using the virial theorem and the variational principle. The sequence is
![]() | (10.8) |
since the exact energy E is smaller than any variational approximation Evar. A trial wave function
of Gaussian shape Ψ(,
) ∝ exp −1
2α(
2 +
2) leads to
![]() | (10.9) |
so finally,
![]() | (10.10) |
iii) If the potential V grows faster than the harmonic oscillator, there are conflicting
contributions from the centrifugal barrier in Eq. (10.4) and from the terms in V ′ whose
expectation becomes larger than m∕8π. There are cases where the latter effect
dominates. For instance, for V = 1
2Br3, the problem consists of comparing the zero-range
correlation with the mean separation. From an accurate hyperspherical calculation, one gets for
m = B = 1
![]() | (10.11) |
Hence the inequality (10.7) is clearly violated.
iv) There are in fact good reasons to believe that the inequality (10.7) is inverted if d∕dr(V ′∕r) > 0 everywhere. For perturbations around the harmonic oscillator, i.e., for V = r2 + λw(r), one already has
![]() | (10.12) |
at first order, whereas the expectation value of 2
ρ contributes only at second order. A numerical
investigation shows that for V = r2.1 or even V = r2.01, one gets, indeed, the inequality
8πδ12 > m
.