In the light of the recent Boomerang and Maxima observations of the CMB whi
ch show an anomalously low second acoustic peak, we reexamine the predictio
n by Adams et al (1997) that this would be the consequence of a 'step' in t
he primordial spectrum induced by a spontaneous symmetry breaking phase tra
nsition during primordial inflation. We demonstrate that a deviation from s
cale-invariance around k similar to 0.1 h Mpc(-1) can simultaneously explai
n both the feature identified earlier in the APM galaxy power spectrum as w
ell the recent CMB anisotropy data, with a baryon density consistent with t
he BBN value. Such a break also allows a good fit to the data on cluster ab
undances even for a critical density matter-dominated universe with sere co
smological constant.