The Cangemi-Jackiw manifold in high dimensions and symplectic structure
arXiv:hep-th/0201147 · doi:10.1006/aphy.2002.6252
Abstract
The notion of Poincare gauge manifold (), proposed in the context of an (1+1) gravitational theory by Cangemi and Jackiw (D. Cangemi and R. Jackiw, Ann. Phys. (N.Y.) 225 (1993) 229), is explored from a geometrical point of view. First is defined for arbitrary dimensions, and in the sequence a symplectic structure is attached to . Treating the case of five dimensions, a (4,1)-de Sitter space, aplications are presented studing representations of the Poincare group in association with kinetic theory and the Weyl operators in phase space. The central extension in the Aghassi-Roman-Santilli group (J. J. Aghassi, P. Roman and R. M. Santilli, Phys. Rev. D 1(1970) 2573) is derived as a subgroup of linear transformations in with six dimensions.
arXiv comment19 pages
References in corpus (9)
- A WZW model based on a non-semi-simple group
- Gauge Invariant Formulations of Lineal Gravity
- Galilean-Invariant (2+1)-Dimensional Models with a Chern-Simons-Like Term and D=2 N oncommutative Geometry
- A Class of String Backgrounds as a Semiclassical Limit of WZW Models
- Gauging a Non-Semi-Simple WZW Model
- Nonlinear Realization of a Dynamical Poincare Symmetry by a Field-dependent Diffeomorphism
- Poincaré Gauge Theory for Gravitational Forces in (1+1) Dimensions
- Geometric Gravitational Forces on Particles Moving in a Line
- Galilei covariance and (4,1) de Sitter space