The spin-orbit nearest-neighbor sp(3)s* model is widely believed able to re
produce accurately the valence bands of most m-V and group-IV semiconductor
s, essential for modeling the in-plane dispersion of valence- and inter-ban
d quantum heterostructures. To check this belief, we study valence-band war
ping in the spin-orbit sp(3)s* model including interactions up to second-ne
arest-neighbor, providing exact, analytic formulas for the [110] and [111]
light- and heavy-hole masses; Surprisingly, we find that the second-nearest
-neighbor model offers significantly more flexibility in fitting these mass
es independently of those along [001] than does the nearest-neighbor model.
[S0163-1829(99)10007-9].