The collective yrast band of the nucleus Cr-48 is Studied using the sp
herical shell model and the Hartree-Fock-Bogoliubov (HFB) method. Both
approaches produce basically the same axially symmetric intrinsic sta
te up to the-accurately reproduced-observed backbending. Agreement bet
ween both calculations extends to most observables. The only significa
nt discrepancy comes from the static moments of inertia and can be att
ributed to the need of a more refined treatment of pairing correlation
s in the HFB calculation.