$\Xi$-nucleus potential for $\Xi^-$ quasifree production in the $^9$Be($K^-$, $K^+$) reaction

TL;DR

This study phenomenologically analyzes the $ ext{Xi}^-$ production spectrum in the $^9$Be($K^-$, $K^+$) reaction at 1.8 GeV/c, revealing a weak attractive $ ext{Xi}$-nucleus potential consistent with experimental data.

Contribution

It provides a new phenomenological determination of the $ ext{Xi}$-nucleus potential strength and emphasizes the importance of energy dependence in the reaction amplitude.

Findings

Weak attraction in the $ ext{Xi}$-nucleus potential with $V_0^ ext{Xi} = -17 ext{ MeV}$

Sufficient explanation of the data with a Woods-Saxon potential model

Confirmation of the significance of energy dependence in the reaction amplitude

Abstract

We study phenomenologically a $\Xi^-$ production spectrum of the $^9$Be($K^-$, $K^+$) reaction at 1.8 GeV/$c$ within the distorted-wave impulse approximation using the optimal Fermi-averaged $K^- p \to K^+ \Xi^-$ amplitude. We attempt to clarify properties of a $\Xi$-nucleus potential for $\Xi^-$-$^8$Li, comparing the calculated spectrum with the data of the BNL-E906 experiment. The results show a weak attraction in the $\Xi$-nucleus potential for $\Xi^-$-$^8$Li, which can sufficiently explain the data in the $\Xi^-$ quasifree region. The strength of $V_0^\Xi =$ $-17 \pm 6$ MeV is favored within the Woods-Saxon potential, accompanied by the reasonable absorption of $W_0^\Xi =$ $-5$ MeV for $\Xi^-p \to \Xi^0n$, $\Lambda\Lambda$ transitions in nuclear medium. It is difficult to determine the value of $W_0^\Xi$ from the data due to the insufficient resolution of 14.7 MeV FWHM. The energy dependence of the Fermi-averaged $K^- p \to K^+ \Xi^-$ amplitude is also confirmed by this analysis, and its importance in the nuclear ($K^-$, $K^+$) reaction is emphasized.