The radiative decay of $Ï(3770)$ into the predicted scalar state X(3700)
arXiv:0805.0499 · doi:10.1140/epja/i2009-10767-8
Abstract
We calculate the radiative decay width of the $Ï(3770)$ into the dynamically generated scalar resonance X(3700) which is predicted in a previous paper. The results show that it is possible that the upgraded BEPC-II facility will generate enough statistics in order to observe this decay and thus confirm the existence of the X(3700).
5 pages, 1 figure