Abstract

Using the Nambu--Jona-Lasinio model with the $U(2)\times U(2)$ chiral symmetric effective four-quark interactions, we derive the amplitude of the radiative decay $f_1(1285) \to\pi^+\pi^-\gamma$, find the decay width $\Gamma (f_1\to\pi^+\pi^-\gamma)=346\,\mbox{keV}$ and obtain the spectral di-pion effective mass distribution. It is shown that in contrast to the majority of theoretical estimates (which consider the $a_1(1260)$ meson exchange as the dominant one), the most relevant contribution to this process comes out from the $\rho^0$-resonance exchange related with the triangle $f_1\rho^0\gamma$ anomaly. The spectral function is obtained to be confronted with the future empirical data.

Highlights

  • The anomalous radiative decay f1 → ρ0γ of the axialvector IGðJPCÞ 1⁄4 0þð1þþÞf1ð1285Þ meson has been described recently [1], with dynamics determined by the effective meson Lagrangian

  • The model reproduces the nontrivial structure of the f1ργ vertex, and fixes fully the values of the coupling constants involved

  • The decay width that has been obtained, Γf1→ργ 1⁄4 311 keV, is compatible with the recently published value Γf1→ρ0γ 1⁄4 453 Æ 177 keV [10] measured for the first time in photo-production from a proton target using the CLAS detector at Jefferson Laboratory

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Summary

INTRODUCTION

The anomalous radiative decay f1 → ρ0γ of the axialvector IGðJPCÞ 1⁄4 0þð1þþÞf1ð1285Þ meson has been described recently [1], with dynamics determined by the effective meson Lagrangian. It would be interesting to analyze as well the role of these anomalies in the f1ð1285Þ → πþπ−γ decay. This transition has not been measured yet, a clear signal of f1ð1285Þ has been seen in the effective mass spectrum of the πþπ−γ system in the reaction π−N → π−πþπ−γN at a pion beam with the momentum pπ− 1⁄4 37 GeV=c studied at the VES spectrometer of IHEP [12]. An earlier attempt of the theoretical description of the f1ð1285Þ → πþπ−γ decay width can be found in [14] It is made in the framework of the Uð2ÞL × Uð2ÞR chiral theory of mesons.

Published by the American Physical Society
Collecting above formulas we come to the following result
CONCLUSIONS
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