Non-strange partner of strangeonium-like state Y(2175)

TL;DR

This paper predicts a non-strange partner to the Y(2175) state, called Y(1915), and suggests experimental methods to detect it, providing insights into the structure of strangeonium and related states.

Contribution

The paper introduces the prediction of the Y(1915) state as the non-strange partner of Y(2175), and proposes experimental search strategies at various colliders.

Findings

Y(1915) predicted with mass ~1915 MeV and width 317-354 MeV.

Experimental channels for detecting Y(1915) are proposed.

Comparison of omega and phi families offers insights into strangeonium states.

Abstract

Inspired by the observed Y(2175) state, we predict its non-strange partner Y(1915), which has a resonance structure with mass around 1915 MeV and width about $317\sim 354$ MeV. Experimental search for Y(1915) is proposed by analyzing the $\omega f_0(980)$ or $\omega \pi\pi$ invariant mass spectrum of the $e^+e^-\to \omega f_0(980), \omega \pi\pi$ and $J/\psi\to \eta \omega f_0(980)$ processes, which are accessible at Belle, BaBar, BESIII and forthcoming BelleII. Considering similarity between two families, the comparison of the mass spectra of $\omega$ and $\phi$ families can provide important information on the 1D state of $\phi$ family, $\phi(1910)$, which has a very broad resonance structure with mass around 1910 MeV regarded as the strangeonium partner of $\omega(1650)$. This also answers the question why the 1D state $\phi(1910)$ is still missing in experiment. This is supported by our former study on the properties of Y(2175), which explains Y(2175) as the 2D strangeonium because our theoretical total width is comparable with the Belle data.