Abstract
Background: Nucleon knockout reactions have been previously used to extract single particle information from nuclei. The analysis of nucleon knockout from a stable projectile in the collision with a proton target and the comparison with the experimental data is a key test for the reaction and structure models used to evaluate the reaction observables.
Purpose: We analyze and knockout from , assuming that only the heavy fragment or core (taken as inert), the knockout particle , and the proton target participate in the collision process with the aim of (i) getting insight to the dominant kinematic conditions of the emitted particles; (ii) clarifying the dynamics of the reaction; (iii) exploring the isospin dependence (here and knockout) of the calculated reaction cross sections.
Method: We solve three-body Faddeev/Alt-Grassberger-Sandhas (Faddeev/AGS) equations for transition operators and calculate kinematically fully exclusive, semi-inclusive, and inclusive cross sections.
Results: We show that (i) the dominant final-state kinematic conditions are consistent with the assumption of quasifree scattering reaction mechanism; (ii) the distortions due to higher order multiple scattering terms depend on the final-state kinematics, and the and final state interaction provide significant effects in the calculated observables; (iii) the twofold energy–polar angle and polar angle–polar angle cross sections exhibit distinct - and -knockout behaviors. Finally we also show that the Faddeev/AGS formalism is able to a certain extent to reproduce the available experimental data for the knockout.
Conclusions: Kinematically fully exclusive measurements of and knockout are needed to rigorously assess the role of the distortion, as it cannot be taken into account as an overall reduction factor. This is a prerequisite for a reliable understanding of the structure of the projectile and the reaction mechanism. In addition, realistic interactions inferred from ab initio structure models are needed for analyzing experimental data.
11 More- Received 20 September 2016
- Revised 31 October 2018
DOI:https://doi.org/10.1103/PhysRevC.99.054622
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