Our main concern in this work is to show how higher shell admixtures affect
the spectrum of Q.Q interaction. We first review how, in the valence space
, the Familiar SU(3) result for the energy spectrum can be obtained using a
coordinate space Q.Q interaction rather than the Elliott one which is symm
etric in r and p. We then reemphasize that the Elliott spectrum goes as L(L
+1) where L. is the orbital angular momentum. While in many cases this is c
ompatible with the rotational formula which involves I(I+1), where I is the
total angular momentum, there are cases, e.g., odd-odd nuclei, where there
is disagreement. Finally, we consider higher shell admixtures and devise a
scheme so as to obtain results, with the Q.Q interaction, which converge a
s the model spaces are increased. We consider not only ground stale rotatio
nal bands but also those that involve intruder stales. (C) 1999 Academic Pr
ess.