Mixed Symmetry Solutions of Generalized Three-Particle Bargmann-Wigner Equations in the Strong-Coupling Limit

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dc.creatorPfister, Winfried
dc.date1995-05-02
dc.date.accessioned2026-07-07T12:03:48Z
dc.date.available2026-07-07T12:03:48Z
dc.descriptionStarting from a nonlinear isospinor-spinor field equation, generalized three-particle Bargmann-Wigner equations are derived. In the strong-coupling limit, a special class of spin 1/2 bound-states are calculated. These solutions which are antisymmetric with respect to all indices, have mixed symmetries in isospin-superspin space and in spin orbit space. As a consequence of this mixed symmetry, we get three solution manifolds. In appendix \ref{b}, table 2, these solution manifolds are interpreted as the three generations of leptons and quarks. This interpretation will be justified in a forthcoming paper.
dc.description17 pages
dc.identifierhttps://arxiv.org/abs/hep-th/9505015
dc.identifierhttp://arxiv.org/abs/hep-th/9505015
dc.identifierNuovoCim.A108:1427-1444,1995
dc.identifierdoi:10.1007/BF02821059
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/207914
dc.subjectHigh Energy Physics - Theory
dc.titleMixed Symmetry Solutions of Generalized Three-Particle Bargmann-Wigner Equations in the Strong-Coupling Limit
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