Abstract

For low-energy nuclear reactions well above the resonance region, but still below the pion threshold, statistical pre-equilibrium models (e.g., the exciton and the hybrid ones) are a frequent tool for analysis of energy spectra and the cross sections of cluster emission. For α ’s, two essentially distinct approaches are popular, namely the preformed one and the different versions of coalescence approaches, whereas only the latter group of models can be used for other types of cluster ejectiles. The original Iwamoto-Harada model of pre-equilibrium cluster emission was formulated using the overlap of the cluster and its constituent nucleons in momentum space. Transforming it into level or state densities is not a straigthforward task; however, physically the same model was presented at a conference on reaction models five years earlier. At that time, only the densities without spin were used. The introduction of spin variables into the exciton model enabled detailed calculation of the γ emission and its competition with nucleon channels, and – at the same time – it stimulated further developments of the model. However – to the best of our knowledge – no spin formulation has been presented for cluster emission till recently, when the first attempts have been reported, but restricted to the first emission only. We have updated this effort now and we are able to handle (using the same simplifications as in our previous work) pre-equilibrium cluster emission with spin including all nuclei in the reaction chain.

Highlights

  • As already sketched in [11], we have extended some ideas behind those of the original pure IHB model: It is natural to generalize the idea to arbitrary combination of excited and unexcited nucleons, and to all types of clusters

  • The difference between calculations with and without angular momentum is shown to be rather small for nucleon emission, but it is larger for clusters, because i) cluster emission is usually enhanced at higher angular momenta, which means an increased role of the nuclear surface and consequent effective lowering of the Coulomb barrier, especially in the case of deformed nuclei; ii) many of the quantities entering pre-equilibrium reactions are both spin- and energy-dependent and their simple contraction to one variable necessarily affects the results

  • We have developed a simple model to include spin variables into the Iwamoto-Harada-Bisplinghoff model of pre-equilibrium cluster emission

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Summary

Introduction

EPJ Web of Conferences to experimental data. The Milan group [3] suggested the existence of preformed αparticles in nuclei. This approach is practically impossible to generalize to other types of ejectiles, whereas the approach of Ribanský and Obložinský is of general nature. The preformed α-particle model yielded better agreement to data than the other one, but the consequent development of the clusterization model minimized this gap. Having in mind general applicability for wide range of ejectiles, we consider the Iwamoto-Harada (Iwamoto-Harada-Bisplinghoff) model (IHB model) [5, 6] to be a suitable starting point for interpretation of complex particle spectra and other quantities

Coalescence cluster emission
Density Approach to the Iwamoto-Harada Model
Knockout Admixtures in the α Emission
Angular Momentum
Calculations
Conclusions
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