Abstract
Background: Core-excitation effects in the scattering of two-body halo nuclei have been investigated in previous works. In particular, these effects have been found to affect in a significant way the breakup cross sections of neutron-halo nuclei with a deformed core. To account for these effects, appropriate extensions of the continuum-discretized coupled-channels (CDCC) method have been recently proposed.
Purpose: We aim to extend these studies to the case of breakup reactions measured under complete kinematics or semi-inclusive reactions in which only the angular or energy distribution of one of the outgoing fragments is measured.
Method: We use the standard CDCC method as well as its extended version with core excitations, assuming a pseudostate basis for describing the projectile states. Two- and three-body observables are computed by projecting the discrete two-body breakup amplitudes, obtained within these reaction frameworks, onto two-body scattering states with definite relative momentum of the outgoing fragments and a definite state of the core nucleus.
Results: Our working example is the one-neutron halo . Breakup reactions on protons and targets are studied at 63.7 MeV/nucleon and 28.7 MeV, respectively. These energies, for which experimental data exist, and the targets provide two different scenarios where the angular and energy distributions of the fragments are computed. The importance of core dynamical effects is also compared for both cases.
Conclusions: The presented method provides a tool to compute double and triple differential cross sections for outgoing fragments following the breakup of a two-body projectile and might be useful to analyze breakup reactions with other deformed weakly bound nuclei, for which core excitations are expected to play a role. We have found that, while dynamical core excitations are important for the proton target at intermediate energies, they are very small for the Zn target at energies around the Coulomb barrier.
1 More- Received 30 January 2017
DOI:https://doi.org/10.1103/PhysRevC.95.044611
©2017 American Physical Society