Study of the $\eta$N scattering amplitude through the associated photoproduction of $\varphi$- and $\eta$-mesons in the region of the N*(1535) resonance

Abstract

The $\gamma p\to \varphi \eta p$ reaction is studied in the kinematic region where the $\eta p$ final state originates dominantly from the decay of the N*(1535) resonance. The threshold laboratory photon energy for this reaction (at the peak of the S11 resonance) is $E_{\gamma }^{Lab}=$3 GeV. We will discuss it somewhat above threshold, at $E_{\gamma }^{Lab}\simeq 4-5$ GeV, in order to reach lower (absolute) values of the squared 4-momentum transfer from the initial photon to the final $\varphi$-meson. In these conditions, we expect the t-channel ${\pi }^0$- and $\eta$-meson exchanges to drive the dynamics underlying the $\gamma p\to \varphi \eta p$ process. The initial photon dissociates into the final $\varphi$-meson and a virtual pseudoscalar meson (${\pi }^0$ or $\eta$). The virtual pseudoscalar meson scatters from the proton target to produce the final $\eta p$ state. The ${\pi }^{0}p\to \eta p$ and $\eta p\to \eta p$ amplitudes are derived in the framework of a coupled-channel effective field theory of meson-baryon scattering. We found the $\eta$-meson exchange to be largely dominant. The $\eta$-${\pi }^0$ interference is of the order of $20-30$. The sign of this term is not known and has a significant influence on the results. The $\pi N\to \eta N$ amplitude being largely determined by data on the ${\pi }^{-}p\to \eta n$ reaction, we found that the $\gamma p\to \varphi \eta p$ reaction cross section is rather directly related to the $\eta$-nucleon scattering amplitude in the N*(1535) resonance region. Accurate data on the $\gamma p\to \varphi \eta p$ process would therefore put additional constraints on this still poorly known amplitude.

Comments: 13 pages, 8 figures