Cross Sections for $\gamma p \rightarrow p \eta$ and $\gamma p \rightarrow p \eta\prime$ using data from CLAS at Jefferson Lab.

ORAL

Abstract

Studying $\eta$ and $\eta\prime$ photoproduction presents a good opportunity to search for missing $N^*$ states, since both mesons act as isospin filters. Previous searches for these states in $\gamma p \rightarrow p \eta\prime$ have been hindered by limited statistics in the available experimental data. I will present differential cross sections obtained from the CLAS g11a dataset. Measurements have been made in $\cos{\theta_{CM}^{\eta(\eta\prime)}}$ bins of width 0.1 for $\eta$ photoproduction in 64 $\sqrt{s}$ bins over the energy range $1.68$~GeV $<\sqrt{s}<$ 2.84~GeV and for $\eta\prime$ photoproduction in 40 $\sqrt{s}$ bins over the energy range $1.92$~GeV $<\sqrt{s}<$ 2.84~GeV. The width of the center-of-mass energy bins is from 10~MeV$-$50~MeV, depending on $\sqrt{s}$. In total, 1082 $\eta$ and 682 $\eta\prime$ cross section points are reported. These results represent a tremendous increase in the precision of the world's $\eta\prime$ photoproduction data and extend the energy coverage by $\sim 500$~MeV in $\sqrt{s}$.

Authors

  • Mike Williams

    Carnegie Mellon University