Production of X_b via radiative transition of Υ(10753)

We studied the radiative transitions between the Υ(10753), the S-D mixed state of the Υ(4S) and Υ_1(3 ^3D_1), and the X_b, the heavy quark flavor symmetry counterpart of the X(3782) in the bottomonium sector. The radiative transition was assumed to occur through the intermediate bottom mesons, including P-wave B_1^(') mesons as well as the S-wave B^(*) ones. The consideration of the B_1^(') mesons leads to the couplings to be in S-wave, and hence enhances the contributions of the intermediate meson loops. The radiative decay width for the Υ(10753)→γ X_b is predicted to be order of 10 keV, corresponding to a branching fraction of 10^-4. Based on the theoretical results, we strongly suggest to search for the X_b in the e^+e^-→γ X_b with X_b→ππχ_b1 near √(s)=10.754 GeV, and it is hoped that the calculations here could be tested by the future Belle II experiments.