# Hadronic decay properties of newly observed $\Omega_c$ baryons

**Authors:** Ze Zhao, Dan-Dan Ye, Ailin Zhang

arXiv: 1704.02688 · 2017-07-05

## TL;DR

This paper calculates the hadronic decay widths of newly observed $\\Omega_c$ baryons using a $^3P_0$ model, providing possible quantum state assignments consistent with experimental decay widths.

## Contribution

It offers the first detailed decay width calculations for these states, suggesting specific quantum number assignments based on decay features and experimental data.

## Key findings

- $\\Omega_c(3066)^0$ and $\Omega_c(3090)^0$ are likely $1P$-wave states.
- $\\Omega_c(3000)^0$, $\\Omega_c(3050)^0$, and $\\Omega_c(3119)^0$ favor $1D$-wave state assignments.
- Predicted decay widths align with experimental measurements for these assignments.

## Abstract

Hadronic decay widths of the newly observed charmed strange baryons, $\Omega_c(3000)^0$, $\Omega_c(3050)^0$, $\Omega_c(3066)^0$, $\Omega_c(3090)^0$ and $\Omega_c(3119)^0$ have been calculated in a $^3P_0$ model. Our results indicate that $\Omega_c(3066)^0$ and $\Omega_c(3090)^0$ can be interpreted as the $1P-$wave $\Omega_{c2}(\frac{3}{2}^-)$ or $\Omega_{c2}(\frac{5}{2}^-)$. Though the measured masses of $\Omega_c(3000)^0$, $\Omega_c(3050)^0$ and $\Omega_c(3119)^0$ are lower than existed theoretical predictions of $1D-$wave $\Omega_c$, the hadronic decay features of these $\Omega_c$ favor assignments of the $1D-$wave states. $\Omega_c(3000)^0$ is possibly $\Omega_{c1}(\frac{1}{2}^+)$ or $\Omega_{c1}(\frac{3}{2}^+)$, $\Omega_c(3050)^0$ is possibly $\hat\Omega_{c3}(\frac{5}{2}^+)$ or $\hat\Omega_{c3}(\frac{7}{2}^+)$, and $\Omega_c(3119)^0$ is possibly $\hat\Omega_{c3}(\frac{5}{2}^+)$, $\hat\Omega_{c3}(\frac{7}{2}^+)$, $\Omega_{c3}(\frac{5}{2}^+)$ or $\Omega_{c3}(\frac{7}{2}^+)$. The predicted total decay widths in these assignments are consistent with experiment.

## Full text

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## Figures

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## References

31 references — full list in the complete paper: https://tomesphere.com/paper/1704.02688/full.md

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Source: https://tomesphere.com/paper/1704.02688