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Adiabatic hyperspherical expansion and three-body halos

  • A. S. Jensen
  • A. Cobis
  • D. V. Fedorov
  • E. Garrido
  • E. Nielsen
Part of the Few-Body Systems book series (FEWBODY, volume 10)

Abstract

The three-body problem is formulated by use of hyperspherical coordinates and an adiabatic expansion of the Faddeev equations. For large distances and short-range potentials the equations simplify substantially and allow high accuracy solutions. The method can be formulated in two dimensions where the three-body systems have different properties. Applications for halo nuclei, Borromean systems, Efimov states, the hypertriton and helium plasma in astrophysical surroundings are briefly discussed.

Keywords

Halo Nucleus Final State Interaction Faddeev Equation Helium Plasma Faddeev Component 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

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Copyright information

© Springer-Verlag/Wien 1999

Authors and Affiliations

  • A. S. Jensen
    • 1
  • A. Cobis
    • 1
  • D. V. Fedorov
    • 1
  • E. Garrido
    • 2
  • E. Nielsen
    • 1
  1. 1.Inst. of Physics and AstronomyAarhus UniversityAarhus CDenmark
  2. 2.Inst. de Estructura de la MateriaCSICMadridSpain

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