The standard CDM model fails to describe the power spectrum of fluctuations
since it gives too much power at small scales. Among other possible improv
ements, it has barn suggested that an agreement with observations can be ac
hieved with the addition of a late decaying particle, through the injection
of nonthermal radiation and the consequent increase of the horizon length
at the equivalence time. We analyze the possibility of implementing this id
ea in some extensions of the electroweak standard model, discussing the cos
mological and astrophysical bounds to which these schemes are subject. (C)
2000 Elsevier Science B.V. All rights reserved. PACS: 12.60.Jv: 14.60.St; 9
5.35. + d; 98.65. - r; 98.80.Cq.