# Interpretation of the newly observed $\Omega_c^0$ resonances

**Authors:** Wei Wang, Rui-Lin Zhu

arXiv: 1704.00179 · 2017-08-02

## TL;DR

This paper models the mass spectra and decay behaviors of doubly strange baryons, interpreting newly observed $	ext{Ω}_c^0$ resonances as P-wave excited states, and explains their narrow widths through heavy quark symmetry.

## Contribution

It provides a theoretical interpretation of newly observed $	ext{Ω}_c^0$ states as P-wave excitations within a heavy-quark-light-diquark framework, incorporating decay analysis via heavy quark effective theory.

## Key findings

- The $	ext{Ω}_c^0(2695)$ and $	ext{Ω}_c^0(2770)$ fit well as S-wave states.
- The five new $	ext{Ω}_c^0$ states are interpreted as P-wave orbitally excited states.
- Decay suppression explains the narrow widths of the new $	ext{Ω}_c^0$ states.

## Abstract

We study the charmed and bottomed doubly strange baryons within the heavy-quark-light-diquark framework. The two strange quarks are assumed to lie in $S$ wave and thus their total spin is 1. We calculate the mass spectra of the $S$ and $P$ wave orbitally excited states and find the $\Omega_c^0 (2695)$ and $\Omega_c^0 (2770)$ fit well as the $S$ wave states of charmed doubly strange baryons. The five newly $\Omega_c^0(X)$ resonances observed by the LHCb Collaboration, i.e. $\Omega_c^0(3000)$, $\Omega_c^0(3050)$, $\Omega_c^0(3066)$, $\Omega_c^0(3090)$, and $\Omega_c^0(3119)$, can be interpreted as the $P$ wave orbitally excited states. In heavy quark effective theory, we analyze their decays into the $\Xi^+_c K^-$ and $\Xi_c'^+ K^-$, and point out that decays of the five P-wave $\Omega_c^0$ states into the $\Xi_c^+ K^-$ and $\Xi_c'^+K^-$ are suppressed by either heavy quark symmetry or phase space. The narrowness of the five newly observed $\Omega_c^0(X)$ states can then be naturally interpreted with heavy quark symmetry.

## Full text

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## References

47 references — full list in the complete paper: https://tomesphere.com/paper/1704.00179/full.md

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Source: https://tomesphere.com/paper/1704.00179