Relativity in the three-nucleon system

A Poincaré-invariant formulation of the three-body system is used. The two-body force embedded in the three-particle Hilbert space is generated out of the high-precision NN forces by solving a nonlinear equation. The solution of the relativistic 3 N Faddeev equation for 3 H reveals less binding ener...

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Bibliographic Details
Published in:Few-body systems 2008-12, Vol.44 (1-4), p.291-293
Main Authors: Kamada, H., Glöckle, W., Witała, H., Golak, J., Skibiński, R., Polyzou, W. N.
Format: Article
Language:English
Subjects:
Atomic
Geometry
Hadrons
Heavy Ions
Molecular
Nonlinear equations
Nuclear Physics
Optical and Plasma Physics
Particle and Nuclear Physics
Particle physics
Physics
Physics and Astronomy
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Summary:A Poincaré-invariant formulation of the three-body system is used. The two-body force embedded in the three-particle Hilbert space is generated out of the high-precision NN forces by solving a nonlinear equation. The solution of the relativistic 3 N Faddeev equation for 3 H reveals less binding energy than for the nonrelativistic one. The effect of the Wigner spin rotation on the binding energy is very small.
ISSN:0177-7963
1432-5411
DOI:10.1007/s00601-008-0311-x