Author:
Maloomeh F Q,McKeon D.G.C.
Abstract
The Bargmann–Wigner equations for a spin s field are of the form (iγ · ∂ + m)α1α′1 · ψα′1α2...α2s = ··· = (iγ · ∂ + m)α2sα′2s ψα1···α′2s = 0 where ψα1···α2s is totally symmetric in all spinor indices. We consider these wave equations for the case in which ψα1···α2s is totally antisymmetric in all indices, examining in particular the situations in which there are two or three indices.PACS No.: 03.65Pm
Publisher
Canadian Science Publishing
Subject
General Physics and Astronomy
Cited by
1 articles.
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