Understand
To improve the accuracy of the e+e- -> pi+pi-gamma Radiative Return method, one has to control the theoretical uncertainty of the final-state photon emission.
- It is of particular importance at DAPHNE for the analysis, where cuts are relaxed to cover the threshold region.
- By means of Monte Carlo generator PHOKHARA we compare several final-state radiation models and present results, relevant for a meson factory running at sqrt{s}=1 GeV.
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