Eugene Wigner and Translational Symmetries

dc.creatorKim, Y. S.
dc.date1996-12-05
dc.date.accessioned2026-07-07T03:08:57Z
dc.date.available2026-07-07T03:08:57Z
dc.descriptionAs Einstein's $E = mc^{2}$ unifies the energy-momentum relation for massive and massless particles, Wigner's little group unifies their internal space-time symmetries. It is pointed out that translational symmetries play essential roles both in formulating the problem, and in deriving the conclusions. The input translational symmetry is the space-time translation, and the output translational symmetry is built in the E(2)-like little group for massless particles. The translational degrees of freedom in this little group are gauge degrees of freedom. It should be noted that a number of condensed matter physicists played important supporting and supplementary roles in Wigner's unification of internal space-time symmetries of massive and massless particles.
dc.description11 pages, LaTeX file, no figures; presented at the 4th International School on Theoretical Physics: Symmetry and Structural Properties of Condensed Matter (Zajaczkowo, Poland, August-September, 1996); to be published in the Proceedings
dc.identifierhttps://arxiv.org/abs/cond-mat/9612057
dc.identifierhttp://arxiv.org/abs/cond-mat/9612057
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/27703
dc.subjectCondensed Matter
dc.subjectHigh Energy Physics - Theory
dc.titleEugene Wigner and Translational Symmetries
dc.typetext

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