1992
DOI: 10.1142/s0217751x9200226x
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Faddeev-Jackiw Quantization and Constraints

Abstract: In a recent Letter, Faddeev and Jackiw have shown that the reduction of constrained systems into its canonical, first-order form, can bring some new insight into the research of this field. For sympletic manifolds the geometrical structure, called Dirac or generalized bracket, is obtained directly from the inverse of the nonsingular sympletic two-form matrix. In the cases of nonsympletic manifolds, this two-form is degenerated and cannot be inverted to provide the generalized brackets. This singular behavior o… Show more

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Cited by 140 publications
(166 citation statements)
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“…In agreement with the prescription of the symplectic formalism [24][25][26]33], the zero modes correspond to the generators of the gauge symmetry of the original theory (1) (see Appendix B), i.e.…”
Section: Gauge Symmetrysupporting
confidence: 57%
“…In agreement with the prescription of the symplectic formalism [24][25][26]33], the zero modes correspond to the generators of the gauge symmetry of the original theory (1) (see Appendix B), i.e.…”
Section: Gauge Symmetrysupporting
confidence: 57%
“…Most papers about these models are focused on the consistent canonical quantization and their quantum spectrum. This family of models were considered in several approaches including: the symplectic embedding [8,9,10,11], the BFT formalism [9,12,13,17,14,15,16], Stuckelberg field shifting [19,18] or mixed approaches based on first principles of the making gauge systems [9,18,20,21,22].…”
Section: Introductionmentioning
confidence: 99%
“…This approach, the so-called Faddeev-Jackiw (F-J) symplectic formalism (for a detailed account see [37][38][39][40][41][42][43][44]), is useful to obtain in an elegant way several essential elements of a particular physical theory, such as the physical constraints, the local gauge symmetry, 1 In the presence of a cosmological constant, Minkowski space-time is no longer a vacuum solution and the new maximally symmetric solutions are de Sitter (dS) space-time for positive ( dS has SO(3, 1) isometry) and anti-de Sitter (AdS) space-time for negative (AdS has SO(2, 2) isomety). In this respect, the SO(2, 2) group can be seen as a -deformed Poincaré group [56], if → 0 the AdS algebra contracts to the usual Poincaré algebra.…”
Section: Introductionmentioning
confidence: 99%