Abstract

The recent observation and measurement of the decay $Z_c(3900) \to \rho \eta_c$ provides the data on the relative strength of the pion and $\rho$ coupling in the corresponding transitions between exotic resonances and pure heavy quarkonium. It is argued that using these data, the heavy quark limit for the $c$ and $b$ quarks, the heavy quark spin symmetry (HQSS) and the vector dominance for photon emission by the light quarks, one can (approximately) quantitatively estimate the rates of the radiative transitions from $\Upsilon(5S)$ to the expected $G$-odd states of molecular bottomonium $W_{bJ}$. The estimate of the cross section of the processes $e^+e^- \to \gamma W_{bJ}$ at the maximum of the $\Upsilon(5S)$ resonance comes out in the ballpark of 0.1\,pb, which sets a benchmark for a possible search for these processes at BelleII.

Highlights

  • The recent observation and measurement of the decay Zcð3900Þ → ρηc provides the data on the relative strength of the pion and ρ coupling in the corresponding transitions between exotic resonances and pure heavy quarkonium

  • Some early predictions for the decay Zcð3900Þ → ρηc within alternative models of the Zc resonances are in Refs. [8,9,10] and a more general overview of the experimental data and the models for the threshold “XYZ”

  • At energy below the threshold for emission of ρ it is possible to produce the expected G-odd resonances by radiative transitions [17], i.e., by having the emission of a ρ0 substituted by emission of a photon from a state produced directly in eþe− annihilation

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Summary

Published by the American Physical Society

States the expected WbJ resonances are not allowed by the G parity to emerge as a result of a one-pion transition from a JPC 1⁄4 1−− state produced in eþe−. At energy below the threshold for emission of ρ it is possible to produce the expected G-odd resonances by radiative transitions [17], i.e., by having the emission of a ρ0 substituted by emission of a photon from a state produced directly in eþe− annihilation. If the threshold resonance Zcð3900Þ retains this spin structure, this would explain essentially equal strength of its transitions to ortho-charmonium (e.g., J=ψ) and to para-charmonium (e.g., ηc). This behavior of the discussed molecular states was first observed for the Zb resonances.

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