Abstract
The Faddeev equation was derived for slving the three body problem. The wave function Ψ is written as the sum of three amplitudes. Each one \({\psi_{ij}}({r_{ij}},{r_k};\alpha )\) is described in one of the three available Jacobi coordinate systems: \({r_{ij}}={x_i}-{x_j},{r_k}= sqrt3({x_k}-X),X=\frac{1}{3}({x_1}+{x_2}+{x_3})\) in terms of the coordinates \({x_i},(i=1,2,3),\) of equal mass particles. The other degrees of freedom a can be spin, isospin etc… Each amplitude is the solution of one Faddeev equation
for pairwise potentials \(V({r_{ij}})\). Then each equation is projected on bipolar harmonics generating coupled two variables integrodifferential equations in coordinate space.
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References
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© 1999 Springer-Verlag/Wien
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Fabre de la Ripelle, M. (1999). Extension of the Faddeev equation to Nuclei. 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_7
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DOI: https://doi.org/10.1007/978-3-7091-6798-4_7
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