The $\Xi N$ interaction constrained by recent ${\Xi }^{-}$ hypernuclei experiments

Abstract

The $\Xi N$ interaction is investigated in the quark mean-field (QMF) model based on recent observables of the ${\Xi }^{-}{+}^{14}\mathrm{N}$ (${}_{{\Xi }^{-}}^{15}\mathrm{C}$) system. The experimental data about the binding energy of $1p$-state ${\Xi }^{-}$ hyperon in ${}_{{\Xi }^{-}}^{15}\mathrm{C}$ hypernuclei at KISO, IBUKI, E07-T011, E176-14-03-35 events are conflated as $B_{{\Xi }^{-}}(1p)=1.14\pm 0.11$ MeV. With this constraint, the coupling strengths between the vector meson and $\Xi$ hyperon are fixed in three QMF parameter sets. Meanwhile, the ${\Xi }^{-}$ binding energy of $1s$ state in ${}_{{\Xi }^{-}}^{15}\mathrm{C}$ is predicted as $B_{{\Xi }^{-}}(1s)=5.66\pm 0.38$ MeV with the same interactions, which are completely consistent with the data from the KINKA and IRRAWADDY events. Finally, the single $\Xi N$ potential is calculated in the symmetric nuclear matter in the framework of QMF models. It is $U_{\Xi N}=-11.96\pm 0.85$ MeV at nuclear saturation density, which will contribute to the study on the strangeness degree of freedom in compact star.

12pages, 4 figures, 2 tables

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Cited by in corpus (6)

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• $\Xi$ hypernuclei ${}_{\Xi }^{15}$C, ${}_{\Xi }^{12}$Be and $\Xi N$ two-body interaction
• Density-dependent relativistic mean-field model for ${\Xi }^{-}$ hypernuclei
• Impact of $\Xi$-Hypernuclear Constraints on Relativistic Equation of State and Properties of Hyperon Stars
• Effects of Phi and ${\sigma }^{\ast }$-meson on properties of hyperon stars including $\Delta$ resonance