Angular-momentum dependence of nuclear-level densities at finite tempe
ratures are investigated in the static-path approximation (SPA) to the
partition function using a cranked quadrupole-interaction hamiltonian
in the following three schemes: (i) cranking about the x-axis, (ii) c
ranking about the z-axis and (iii) cranking about the z-axis but corre
cting for the orientation fluctuation of the axis. Performing numerica
l computations for an sd- and a pf-shell nucleus, we find that the x-a
xis-cranking results are satisfactory for reasonably heavy nuclei and
this offers a computationally faster method to include the angular-mom
entum dependence at high temperatures in the SPA approach. It also app
ears that at high spins the inclusion of the orientation-fluctuation c
orrection would be important.