The S = -2 hypernuclear states formed through (K-, K+) reactions have been studied by using the 1.66 GeV/c K- beam provided by KEK Proton Synchrotron. Investigation has been done on the stars due to the capture of the Ξ- hyperons at rest in nuclear emulsion, which hyperons were produced in (K-, K+) reactions. We observed a clear case of an absorption of Ξ- hyperon at rest by a nucleus followed by a back-to-back emission of two single-Λ hypernuclei.
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Aoki et al. (1993) studied this question.
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