SU(N) supersymmetry on S 3 × R spacetime

Details SU(N) supersymmetry on S 3 × R spacetime SU(N) supersymmetry on S 3 × R spacetime

Jun 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002fophl..15..277d&link_type=abstract

Foundations of Physics Letters, Volume 15, Issue 3, pp.277-286

Physics

Scientific paper

As the whole physical community is celebrating 30 years of supersymmetry, the aim of the present paper is to analyse an 50(3,1) × SU(N)— gauge invariant supersymmetric model on the Einstein’s universe. Thus, by exploiting the maximal S 3 symmetry, which allows the use of group theoretical techniques, we deal with a (1/2, 1, 3/2)—spin particle system on the S 3 × R manifold. After we derive the Dirac-Rarita-Schwinger-Yang-Mills-type field equations, we focus on the additional terms that come into theory as a result of the compactness of space and spin coupling to gravity.

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