The Hamilton-Jacobi analysis for gravity without dynamics is performed. We report a detailed analysis where the complete set of Hamilton-Jacobi constraints, the characteristic equations and the gauge transformations of the theory are found. We compare our results with those reported in the literature where alternative approaches are used. In addition, we complete our work by performing the canonical covariant analysis by constructing a gauge invariant symplectic structure, and we find a full consistency between the results obtained from both approaches. PACS numbers: 98.80.-k,98.80.Cq
I. INTRODUCTIONIt is well known that three dimensional gravity [3dg] described by Palatini's first order formulation can be expressed as a full connection theory, this is, under a correct election of a connection in a Chern-Simons [CS] theory, 3dg can be obtained. In fact, it has been showed that these theories are equivalent at Lagrangian level up to a total derivative [1,2]. Furthermore, that CS theory turns out to be an extension of three dimensional gravity, since the later requires an invertible triad, whereas in the former this is not a necessary ingredient [3]. Hence, the study of CS theories has been a topic of great interest for the theoretical physics community, because these theories could help us to understand the classical and quantum connection between real gravity and gauge theories [1][2][3][4]. In this respect, the analysis of toy models such as CS theories are great laboratories for testing ideas that could be applicable in real gravity in either classical and quantum regime. Furthermore, the relation between CS and 3dg theories can be extended in order to obtain models with more general structure than Palatini's theory, for instance the Bonzom Livine model [BL] [5,6] and the models reported by V. Hussain, in which there is not generator of the dynamics [7,8]. The BL model describes a set of actions sharing the equations of motion with Palatini's theory; however, the symplectic structure in the BL model depends on a Barbero-Immirizi-like parameter, which may represent a difference at dynamical level [5,6]. In contrast to real gravity theory, on the other hand, in the Hussain theories have not a Hamiltonian constraint, but the vector and the Gauss constraints are present and this fact facilitates the study of quantum aspects of gravity being it a difficult task to perform, thus, the study of toy models brings us insights for study the symmetries of gravity. In this respect, * Electronic address: aescalan@ifuap.buap.mx † Electronic address: ivallejo@ifuap.buap.mx