The Bargmann-Wigner Formalism for Spin 2

Simple item page
dc.creatorDvoeglazov, Valeri V.
dc.date1998-05-18
dc.date.accessioned2026-07-07T04:32:24Z
dc.date.available2026-07-07T04:32:24Z
dc.descriptionWe proceed to derive equations for the symmetric tensor of the second rank on the basis of the Bargmann-Wigner formalism in a straightforward way. The symmetric multispinor of the fourth rank is used. It is constructed out of the Dirac 4-spinors. Due to serious problems with the interpretation of the results obtained on using the standard procedure we generalize it and obtain the spin-2 relativistic equations, which are consistent with the previous one. The importance of the 4-vector field (and its gauge part) is pointed out.
dc.descriptionReVTeX file, 6pp
dc.identifierhttps://arxiv.org/abs/math-ph/9805017
dc.identifierhttp://arxiv.org/abs/math-ph/9805017
dc.identifierAdv. Appl. Clifford Algebras v. 10 , No. 1 (2000) pp. 7-14
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/58175
dc.subjectMathematical Physics
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectHigh Energy Physics - Phenomenology
dc.subjectHigh Energy Physics - Theory
dc.subjectQuantum Physics
dc.titleThe Bargmann-Wigner Formalism for Spin 2
dc.typetext

Files

Collections

arXiv