# Radiative decays of the spin-$2$ partner of $X(3872)$

**Authors:** Pan-Pan Shi, Jorgivan M. Dias, Feng-Kun Guo

arXiv: 2302.13017 · 2023-06-08

## TL;DR

This paper investigates the radiative decay properties of the hypothesized spin-2 partner of X(3872), predicting decay ratios and suggesting experimental searches to shed light on its nature and relation to observed structures.

## Contribution

It provides the first detailed estimate of radiative decay widths for the X2 as a D*D* molecular state and proposes experimental strategies for its detection.

## Key findings

- Predicted the decay width ratio of X2 to gamma psi(2S) and gamma J/psi to be less than 1.0.
- Estimated the number of X2 events in two-photon collisions at Belle.
- Suggested experimental search methods in gamma J/psi invariant mass distributions.

## Abstract

It has been generally expected that the $X(3872)$ has a spin-2 partner, $X_2$, with quantum numbers $J^{PC}=2^{++}$. In the hadronic molecular model, its mass was predicted to be below the $D^*\bar D^*$ threshold, and the new structure reported in the $\gamma \psi(2S)$ invariant mass distribution by the Belle Collaboration with mass $M= (4014.3 \pm 4.0 \pm 1.5)$ MeV and decay width $\Gamma= (4 \pm 11 \pm 6)$ MeV, with a global significance of 2.8 $\sigma$, is a nice candidate for it. We consider the radiative decay widths for the $X_{2}\to \gamma\psi$ with $\psi=J/\psi, \psi(2S)$ treating the $X_2$ as a $D^*\bar{D}^*$ shallow bound state, and estimate the events of $X_2$ in two-photon collisions that can be collected in the $\gamma J/\psi\to\gamma\ell^+\ell^-$ ($\ell=e,\mu$) final states at Belle. Based on the upper limit for the ratio of decay widths of $X(3872)\to \gamma \psi(2S)$ and $X(3872)\to \gamma J/\psi$ measured by BESIII, we predict the similar ratio $\Gamma(X_2\to \gamma \psi(2S))/\Gamma(X_2\to \gamma J/\psi)$ to be smaller than $1.0$. We suggest searching for the $X_2$ signal in the $\gamma J/\psi$ invariant mass distribution via two-photon fusions. The results will lead to insights into both the $X(3872)$ and the new structure observed by Belle.

## Full text

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## Figures

11 figures with captions in the complete paper: https://tomesphere.com/paper/2302.13017/full.md

## References

64 references — full list in the complete paper: https://tomesphere.com/paper/2302.13017/full.md

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Source: https://tomesphere.com/paper/2302.13017