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In-flight (K-,N) Reactions for Study of Kaon-nucleus Interaction

机译:飞行中(K-,N)反应用于研究Kaon核相互作用

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We would like to emphasize that the in-flight (K-,N) reactions are particularly useful for the study of the K-nucleus interaction.Since the reaction mechanism is well known,there is little ambiguity to derive the K-nucleus interaction from the measured missing mass spectra.Here we discuss the missing mass spectra of the (K-,N) reactions on the 12C and 16O targets.The spectra show an appreciable amount of strength below the K-nucleus threshold which indicates that the K-nuclear potential is strongly attractive.Comparison of the missing mass spectra with theoretical calculations leads to a potential depth of around-190 MeV for the 12C(K-,n) reaction.A less deep potential of around-160 MeV reproduces well that of the 12C(K-,p) reaction.The difference can be due to isospin dependence of the interaction.Our data show that the K-nucleus potential is very deep to realize kaon condensation in the core of neutron stars.
机译:我们想强调的是,机上(K-,N)反应对于研究K-核相互作用特别有用。由于反应机理众所周知,因此从中得出K-核相互作用几乎没有歧义。在这里我们讨论了在12C和16O靶上(K-,N)反应的缺失质谱图,光谱显示了在K核阈值以下的相当数量的强度,这表明K核电势极具吸引力。将缺失的质谱与理论计算进行比较,得出12C(K-,n)反应的电势深度约为190 MeV.160MeV左右的电势较小的深度可以很好地再现12C的电势(K-,p)反应。差异可能是由于相互作用的同位旋依赖性所致。我们的数据表明,K核势很深,可以在中子星核心中实现钾离子凝聚。

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