The quadratic pion scalar radius, la r^2ra^pi_s, plays an important role for present precise determinations of pipi scattering. Recently, Yndurain, using an Omn`es representation of the null isospin(I) non-strange pion scalar form factor, obtains la
r^2ra^pi_s=0.75pm 0.07 fm^2. This value is larger than the one calculated by solving the corresponding Muskhelishvili-Omn`es equations, la r^2ra^pi_s=0.61pm 0.04 fm^2. A large discrepancy between both values, given the precision, then results. We reanalyze Yndurains method and show that by imposing continuity of the resulting pion scalar form factor under tiny changes in the input pipi phase shifts, a zero in the form factor for some S-wave I=0 T-matrices is then required. Once this is accounted for, the resulting value is la r^2ra_s^pi=0.65pm 0.05 fm^2. The main source of error in our determination is present experimental uncertainties in low energy S-wave I=0 pipi phase shifts. Another important contribution to our error is the not yet settled asymptotic behaviour of the phase of the scalar form factor from QCD.
We perform a dispersive theoretical study of the reaction gammagammato pi^0pi^0 emphasizing the low energy region. The large source of theoretical uncertainty to calculate the gammagammatopi^0pi^0 total cross section for sqrt{s}gtrsim 0.5 GeV within
the dispersive approach is removed. This is accomplished by taking one more subtraction in the dispersion relations, where the extra subtraction constant is fixed by considering new low energy constraints, one of them further refined by taking into consideration the f_0(980) region. This allows us to make sharper predictions for the cross section for sqrt{s}lesssim 0.8 GeV, below the onset of D-wave contributions. In this way, were new more precise data on gammagammatopi^0pi^0 available one might then distinguish between different parameterizations of the pipi isoscalar S-wave. We also elaborate on the width of the sigma resonance to gammagamma and provide new values.
