# BESIII Exotics

**Authors:** G. Mezzadri (on behalf of the BESIII collaboration)

arXiv: 1906.08930 · 2019-06-24

## TL;DR

BESIII is actively studying exotic $XYZ$ states in the charmonium sector, with plans to upgrade and explore the nature of the $Y(4660)$ resonance through direct cross section measurements.

## Contribution

This paper discusses the current status and future plans of BESIII in investigating the $XYZ$ states, especially the $Y(4660)$, with an upgraded energy range and new data collection strategies.

## Key findings

- Initial observations of the $Y(4660)$ resonance.
- Plans to measure cross sections around the peak.
- Potential verification of baryonium interpretation.

## Abstract

Since few years, a new family of exotic states has been appearing above the open-heavy meson thresholds: the so-called $XYZ$ states. BESIII at the BEPCII $e^+e^-$ collider plays a unique role in the study of those particles in the charmonium sector. Changing the beam energy, BESIII can collect large data samples by means of scans of the resonant region, accessing directly to all vector states. As part of a larger upgrade program, BESIII has planned to increase the center of mass energy to reach $4.7$ GeV: this will allow BESIII to investigate the nature of the $Y(4660)$, that was at first observed by Belle and BaBar after Initial State Radiation only in $\pi\pi \psi(2s)$ and $\Lambda_c$ $\bar{\Lambda}_c$ final states. The relative branching ratio seems to point toward a baryonium interpretation of the resonance, as expected in Rossi-Veneziano model. BESIII can directly measure the cross sections around the expected peak position and verify this prediction. In this presentation, the status of the $XYZ$ searches at BESIII will be presented, with a focus also on the plans for the newest data taking and for the $Y(4660)$ studies.

## Full text

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## Figures

7 figures with captions in the complete paper: https://tomesphere.com/paper/1906.08930/full.md

## References

26 references — full list in the complete paper: https://tomesphere.com/paper/1906.08930/full.md

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Source: https://tomesphere.com/paper/1906.08930