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dc.contributor.authorDudko, I. G.-
dc.contributor.authorRed'kov, V. M.-
dc.contributor.authorSemenyuk, O. A.-
dc.contributor.authorKisel, V. V.-
dc.date.accessioned2023-09-18T06:38:01Z-
dc.date.available2023-09-18T06:38:01Z-
dc.date.issued2022-
dc.identifier.citationNonlinear Phenomena in Complex Systems. - 2022. - Vol. 25. - № 3. - P. 286-296ru
dc.identifier.issn1561-4085-
dc.identifier.urihttps://elib.bsu.by/handle/123456789/301879-
dc.description.abstractThe most of studies in the theory of spin 2 feld were performed with the use of the 2-nd order equations. The spin 2 particle theory proposed by F.I. Fedorov is based on the first order equations requires a 30-component set of tensors. Besides, by him and coauthors was elaborated a more general theory, which is based on 50-component set of tensors. In the present paper, we consider this more general theory in presence of arbitrary electromagnetic felds and Riemannian space-time backgrounds. First we study the 50-component theory for a massive particle. In this case, there arises the non-minimal interaction with the curved space-time background through the Ricci and Riemann tensors. It is important that the theory under consideration allows for a new massless limit for the spin 2 feld. This fact is of special interest, because the conventional Pauli - Fierz theory for the massless feld does not possess gauge symmetry in the curved space-time, in particular, in models with the vanishing Ricci tensor. We show that the generalized theory possesses such a gauge symmetry in all space-time models for which the Ricci tensor vanishes.ru
dc.language.isoenru
dc.publisherMinsk : Education and Upbringingru
dc.rightsinfo:eu-repo/semantics/openAccessru
dc.subjectЭБ БГУ::ЕСТЕСТВЕННЫЕ И ТОЧНЫЕ НАУКИ::Физикаru
dc.titleSpin 2 Particle with Anomalous Magnetic Moment in Riemann Space-Time : A Massless Case with the Gauge Symmetryru
dc.typearticleru
dc.rights.licenseCC BY 4.0ru
dc.identifier.DOI10.33581/1561-4085-2022-25-3-286-296-
Располагается в коллекциях:2022. Volume 25. Number 3

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