%0 Journal Article
%T Production of the X(3872) in charmonia radiative decays
%A Feng-Kun Guo
%A Christoph Hanhart
%A Ulf-G. MeiŁżner
%A Qian Wang
%A Qiang Zhao
%J Physics
%D 2013
%I arXiv
%R 10.1016/j.physletb.2013.06.053
%X We discuss the possibilities of producing the X(3872), which is assumed to be a D \bar D^* bound state, in radiative decays of charmonia. We argue that the ideal energy regions to observe the X(3872) associated with a photon in e^+e^- annihilations are around the Y(4260) mass and around 4.45 GeV, due to the presence of the S-wave D \bar D_1(2420) and D^* \bar D_1(2420) threshold, respectively. Especially, if the Y(4260) is dominantly a D \bar D_1 molecule and the X(3872) a D \bar D^* molecule, the radiative transition strength will be quite large.
%U http://arxiv.org/abs/1306.3096v2