Abstract
Making use of the correlation function determined on the basis of the Brueckner theory, we calculate total absorption rates, the effects of the short-range NN correlations on the branching ratio W(pnnn)W(pppn), and the distribution of the absorption rate with respect to the opening angle between the emitted nucleons in negative-pion absorption by C12 nuclei. Although Rtheor (pp;180°90°) is about ten times as small as the experimental value, other theoretical results are in excellent agreement with the experimental results.

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