Estimates for a weaker isovector potential than previously adopted are
put forward. It is also strongly mass and, energy dependent. The resu
lting isovector particle-hole interaction is weaker in Lighter nuclei
and the isovector quadrupole resonance should be located at lower ener
gy than previously expected. The uncertainties arising from the separa
tion of the potential asymmetry energy in nuclear matter calculations
are discussed.