Abstract
The decay width of $N(1535)\rightarrow N\eta$ is as large as that of $N(1535)\rightarrow N\pi$. This is in evident conflict with simple expectations based on flavor symmetry and phase space. Similarly, the decay width of $\Lambda(1670) \rightarrow \Lambda(1116) \eta $ is larger than predicted by flavor symmetry. In this work, we propose that the axial $U(1)_{A}$ anomaly is responsible for an enhanced coupling of (some) excited baryons to the $\eta$ meson. We test this idea by including a new, chirally symmetric but $U(1)_{A}$ anomalous, term in an effective hadronic model decribing baryons and their chiral partners in the mirror assignment. This term enhances the decay of the chiral partners into baryons and an $\eta$ meson, such as $N(1535)\rightarrow N\eta$. Moreover, a strong coupling of $N(1535)$ to $N \eta^\prime $ emerges (this is important for studies of $\eta^\prime$ production processes). Our approach shows that $N(1535)$ is predominantly the chiral partner of $N(939)$, and $\Lambda(1670)$ the chiral partner of $\Lambda(1116)$. Finally, our formalism can be used to couple the pseudoscalar glueball $\tilde{G}$ to baryons. We expect a large cross section for the reaction $\bar{p}p \rightarrow \tilde{G} \rightarrow \bar{p}p(1535)$, which can be experimentally tested in the future PANDA experiment.
Highlights
The experimental decay width of Nð1535Þ → Nη is surprisingly large, ΓNð1535Þ→Nη ≃ ð65 Æ 25Þ MeV [1]
Where the factor 3 takes into account the pion triplet and θP ≃ −44.6° [2] is the pseudoscalar mixing angle defined by jηi 1⁄4 cos θPjηN ≡ ðuu þ ddÞ=pffi2ffii þ sin θPjηS ≡ ssi: This evident violation of flavor symmetry is hard to understand. [Note that phase space would even further reduce the ratio in Eq (1).] One can extend these
Flavor-symmetry considerations to the whole baryon octet fNð1535Þ; Λð1670Þ; Σð1620Þ; Ξð?Þg, which decays into the ground-state baryons fNð939Þ; Λð1116Þ; Σð1193Þ; Ξð1338Þg and one pseudoscalar meson
Summary
The experimental decay width of Nð1535Þ → Nη is surprisingly large, ΓNð1535Þ→Nη ≃ ð65 Æ 25Þ MeV [1]. Investigations of nucleon-meson interactions within twoflavor chiral effective models [13] (based on chiral symmetry and the mirror assignment for Nð1535Þ as the chiral partner of the nucleon) showed that the decay width of Nð1535Þ → Nη cannot be correctly described. The large decay width of Nð1535Þ to Nη is intuitively explained as follows: quantum fluctuations related to the anomaly couple Nð1535Þ to N via emission of two gluons in the isoscalar-pseudoscalar channel I 1⁄4 0, JPC 1⁄4 0−þ Since this di-gluon couples with the same intensity to the quark-antiquark pairs uu, dd, and ss, it couples almost exclusively to η and η0 and is responsible for a decay width which is enhanced compared to simple flavor-symmetry arguments. Axial anomaly, can help to understand the role of hyperons in neutron stars [26,32]
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