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9 - Three-body nuclei

Published online by Cambridge University Press:  05 March 2012

Ian J. Thompson
Affiliation:
Lawrence Livermore National Laboratory
Filomena M. Nunes
Affiliation:
Michigan State University
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Summary

One never notices what has been done; one can only see what remains to be done.

Marie Curie

The direct reaction of a two-body projectile with a target constitutes a three-body problem, as discussed in the previous chapter. The next most complicated group of processes involve a three-body projectile, which with a target make a four-body reaction problem. This group includes reactions where the projectile is a two nucleon halo nucleus, and in this chapter we present theories for the structure and reactions of such nuclei. First we introduce the topic of halo nuclei, then describe three-body models for bound and scattering states. Finally we discuss four-body reaction models within DWBA, the adiabatic approximation and the eikonal approximation, and conclude by looking at four-body CDCC.

Definitions of halo and deeply bound states

Stable nuclei are characterized by large binding energies and extremely long lifetimes. Figure 9.1 shows the nuclear chart for light nuclei. As we add protons or neutrons to the system, and move away from the valley of stability (black squares in Fig. 9.1), the binding energy of the valence nucleons becomes smaller and smaller until eventually the system can no longer bind. Around the nuclear dripline, we frequently find exotic structures called halo nuclei [1]. The halo phenomenon comes from a significant decoupling of the valence nucleon (or nucleons) from the remaining nucleons, which form a core.

Type
Chapter
Information
Nuclear Reactions for Astrophysics
Principles, Calculation and Applications of Low-Energy Reactions
, pp. 274 - 295
Publisher: Cambridge University Press
Print publication year: 2009

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