arXiv · 2503.04586
Investigating the nature of $N(1535)$ and $\Lambda(1405)$ in a quenched chiral quark model
Abstract
In this work, we systematically study $N(1440)$, $N(1535)$, and $\Lambda(1405)$ in both the quenched three-quark and five-quark frameworks using the Gaussian Expansion Method (GEM) within the chiral quark model. Our calculations show that $N(1535)$ can be reproduced as a three-quark state ($N(1P)$), while $N(1440)$ and $\Lambda(1405)$ cannot be accommodated as the three-quark candidates, ($N(2S)$ and $\Lambda(1P)$), respectively. In the five-quark framework, we find that the $\Lambda K$ state for $N(1535)$ can not form a bound state, while in the $N\bar{K}$ channel there will $\Lambda(1405)$ form a shallow bound state. Based on the complex-scaling method, we performed complete coupled-channels calculations and obtained six resonance states with energies ranging from 1.8 GeV to 2.2 GeV, in addition with one bound state located around $\Sigma \pi$ channel. However, neither molecular candidates in $\Lambda K$ channel for $N(1535)$ nor $N\bar{K}$ for $\Lambda(1405)$ are included in these states. This is because the strong coupling between $N\bar{K}$ and $\Sigma \pi$ will make the $N\bar{K}$ unbound, while the weak coupling between $\Lambda K$ and $\Sigma K$ can not help form a stable structure around $\Lambda K$ threshold. Thus, under the quenched quark model, our results support $N(1535)$ as a three-quark state, while $N(1440)$ is neither a three-quark nor a five-quark state. In addition, we find that although $\Lambda(1405)$ can be primarily a five-quark state, it requires a mixture of three-quark and five-quark components for stability. In the future, an exploration on the mixing effects between bare baryons with these relevant two-body hadronic channel components will be carried out to further test our conclusions.
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Yue Tan, Zi-Xuan Ma, Xiaoyun Chen, Xiaohuang Hu, Youchang Yang, Qi Huang, Jialun Ping. 2025-03-06. Investigating the nature of $N(1535)$ and $\Lambda(1405)$ in a quenched chiral quark model. https://arxiv.org/abs/2503.04586
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