The complementarity between chiral perturbation theory and the linear sigma
model in the scalar channel is exploited to study pi (0)pi (0) production
in rho and omega radiative decays, where the effects of a low mass scalar r
esonance sigma (500) should manifest. The recently reported data on rho -->
pi (0)pi (0)gamma seem to require the contribution of a low mass and moder
ately narrow sigma (500). The omega --> pi (0)pi (0)gamma can properties of
this controversial state could be fixed by improving the accuracy of these
measurements. Data on omega --> pi (0)pi (0)gamma can also be accommodated
in our framework, but are much less sensitive to the sigma (500) propertie
s. (C) 2001 Published by Elsevier Science B.V.