Analysis of rescattering effects in $$3\pi $$ final states
Dominik Stamen (Helmholtz-Institut für Strahlen- und Kernphysik (Theorie), Bethe Center for Theoretical Physics, Universität Bonn, Bonn, 53115, Germany); Tobias Isken (Helmholtz-Institut für Strahlen- und Kernphysik (Theorie), Bethe Center for Theoretical Physics, Universität Bonn, Bonn, 53115, Germany, Helmholtz Forschungsakademie Hessen für FAIR (HFHF), GSI Helmholtzzentrum für Schwerionenforschung GmbH, Planckstraße 1, Darmstadt, 64291, Germany); Bastian Kubis (Helmholtz-Institut für Strahlen- und Kernphysik (Theorie), Bethe Center for Theoretical Physics, Universität Bonn, Bonn, 53115, Germany); Mikhail Mikhasenko (ORIGINS Excellence Cluster, Ludwig-Maximilians-Universität München, Munich, 80939, Germany); Malwin Niehus (Helmholtz-Institut für Strahlen- und Kernphysik (Theorie), Bethe Center for Theoretical Physics, Universität Bonn, Bonn, 53115, Germany)
Decays into three particles are often described in terms of two-body resonances and a non-interacting spectator particle. To go beyond this simplest isobar model, crossed-channel rescattering effects need to be accounted for. We quantify the importance of these rescattering effects in three-pion systems for different decay masses and angular-momentum quantum numbers. We provide amplitude decompositions for four decay processes with total $$J^{PC} = 0^{--}$$ , $$1^{--}$$ , $$1^{-+}$$ , and $$2^{++}$$ , all of which decay predominantly as $$\rho \pi $$ states. Two-pion rescattering is described in terms of an Omnès function, which incorporates the $$\rho $$ resonance. Inclusion of crossed-channel effects is achieved by solving the Khuri–Treiman integral equations. The unbinned log-likelihood estimator is used to determine the significance of the rescattering effects beyond two-body resonances; we compute the minimum number of events necessary to unambiguously find these in future Dalitz-plot analyses. Kinematic effects that enhance or dilute the rescattering are identified for the selected set of quantum numbers and various masses.