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.
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Jensen, A.S., Cobis, A., Fedorov, D.V., Garrido, E., Nielsen, E. (1999). Adiabatic hyperspherical expansion and three-body halos. In: Desplanques, B., Protasov, K., Silvestre-Brac, B., Carbonell, J. (eds) Few-Body Problems in Physics ’98. Few-Body Systems, vol 10. Springer, Vienna. https://doi.org/10.1007/978-3-7091-6798-4_3
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DOI: https://doi.org/10.1007/978-3-7091-6798-4_3
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