The resonant $Ï^+γ\toÏ^+Ï^0$ amplitude from Quantum Chromodynamics
arXiv:1507.06622 · doi:10.1103/PhysRevLett.115.242001
Abstract
We present the first ab initio calculation of a radiative transition of a hadronic resonance within quantum chromodynamics (QCD). We compute the amplitude for $ÏÏ\to Ïγ^\star$, as a function of the energy of the $ÏÏ$ pair and the virtuality of the photon, in the kinematic regime where $ÏÏ$ couples strongly to the unstable $Ï$ resonance. This exploratory calculation is performed using a lattice discretization of QCD with quark masses corresponding to $m_Ï\approx 400$~MeV. We obtain a description of the energy dependence of the transition amplitude, constrained at 48 kinematic points, that we can analytically continue to the $Ï$ pole and identify from its residue the $Ï\to Ïγ^\star$ form factor.
V2, version accepted for publication in PRL. More references added