Constraints on the ωπ form factor from analyticity and unitarity

Abstract

Form factors are important low-energy quantities and an accurate knowledge of these sheds light on the strong interactions. A variety of methods based on general principles have been developed to use information known in different energy regimes to constrain them in regions where experimental information needs to be tested precisely. Here we review our recent work on the electromagnetic [Formula: see text] form factor in a model-independent framework known as the method of unitarity bounds, partly motivated by the discrepancies noted recently between the theoretical calculations of the form factor based on dispersion relations and certain experimental data measured from the decay [Formula: see text]. We have applied a modified dispersive formalism, which uses as input the discontinuity of the [Formula: see text] form factor calculated by unitarity below the [Formula: see text] threshold and an integral constraint on the square of its modulus above this threshold. The latter constraint was obtained by exploiting unitarity and the positivity of the spectral function of a QCD correlator, computed on the spacelike axis by operator product expansion and perturbative QCD. An alternative constraint is obtained by using data available at higher energies for evaluating an integral of the modulus squared with a suitable weight function. From these conditions we derived upper and lower bounds on the modulus of the [Formula: see text] form factor in the region below the [Formula: see text] threshold. The results confirm the existence of a disagreement between dispersion theory and experimental data on the [Formula: see text] form factor around 0.6 GeV, including those from NA60 published in 2016.