Relativity in the three-nucleon system

H. Kamada; W. Glöckle; H. Witała; J. Golak; R. Skibiński; W. N. Polyzou

doi:10.1007/s00601-008-0311-x

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Relativity in the three-nucleon system

H. Kamada, W. Glöckle, H. Witała, J. Golak, R. Skibiński and W. N. Polyzou

Few-body systems, Vol.44(1-4), pp.291-293

12/01/2008

DOI: 10.1007/s00601-008-0311-x

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Abstract

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.

Article

Atomic

Hadrons

Heavy Ions

Molecular

Nuclear Physics

Optical and Plasma Physics

Particle and Nuclear Physics

Physics

Physics and Astronomy

Details

Title: Subtitle: Relativity in the three-nucleon system
Creators: H. Kamada - Kyushu Institute of Technology
W. Glöckle - Ruhr University Bochum
H. Witała - Jagiellonian University
J. Golak - Jagiellonian University
R. Skibiński - Jagiellonian University
W. N. Polyzou - University of Iowa
Resource Type: Journal article
Publication Details: Few-body systems, Vol.44(1-4), pp.291-293
DOI: 10.1007/s00601-008-0311-x
ISSN: 0177-7963
eISSN: 1432-5411
Publisher: Springer-Verlag
Language: English
Date published: 12/01/2008
Academic Unit: Physics and Astronomy
Record Identifier: 9984428835602771

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