Abstract

We extract the e+e−→π+π− cross section in the energy range between 600 and 900 MeV, exploiting the method of initial state radiation. A data set with an integrated luminosity of 2.93 fb−1 taken at a center-of-mass energy of 3.773 GeV with the BESIII detector at the BEPCII collider is used. The cross section is measured with a systematic uncertainty of 0.9%. We extract the pion form factor |Fπ|2 as well as the contribution of the measured cross section to the leading-order hadronic vacuum polarization contribution to (g−2)μ. We find this value to be aμππ,LO(600–900MeV)=(368.2±2.5stat±3.3sys)⋅10−10, which is between the corresponding values using the BaBar or KLOE data.

Highlights

  • IntroductionThe two most precise measurements have been performed by the KLOE Collaboration in Frascati [8] and the BaBar Collaboration at SLAC [9,10]

  • The cross section σππ = σ (e+e− → π +π −) has been measured in the past with ever increasing precision at accelerators in Novosibirsk [1,2,3], Orsay [4], Frascati [5,6,7,8], and SLAC [9,10]

  • The accuracy of the Standard Model (SM) prediction of (g − 2)μ is entirely limited by the knowledge of the hadronic vacuum polarization contribution, which is obtained in a dispersive framework by using experimental data on σ (e+e− → hadrons) [11,12,13]

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Summary

Introduction

The two most precise measurements have been performed by the KLOE Collaboration in Frascati [8] and the BaBar Collaboration at SLAC [9,10]. Both experiments claim a precision of better than 1% in the energy range below 1 GeV, in which the ρ(770) resonance with its decay into pions dominates the total hadronic cross section. In the ISR method events are used in which one of the beam particles radiates a high-energy photon In such a way, the available energy to produce a hadronic (or leptonic) final state is reduced, and the hadronic (or leptonic) mass range below the center-of-mass (cms) energy of the e+e− collider becomes available.

The BESIII experiment
Data sample and MC simulations
Event selection
Efficiency corrections
Background subtraction
Luminosity measurement using Bhabha events
Methods
Unfolding
FSR correction
Radiator function and vacuum polarization correction
Summary of systematic uncertainties
Results
Findings
Conclusion
Full Text
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