On Hamiltonian formulation of the Einstein-Hilbert action in two dimensions
arXiv:hep-th/0510260 · doi:10.1142/S0217732306020202
Abstract
It is shown that the well-known triviality of the Einstein field equations in two dimensions is not a sufficient condition for the Einstein-Hilbert action to be a total divergence, if the general covariance is to be preserved, that is, a coordinate system is not fixed. Consequently, a Hamiltonian formulation is possible without any modification of the two dimensional Einstein-Hilbert action. We find the resulting constraints and the corresponding gauge transfromations of the metric tensor.
9 pages
References in corpus (5)
- The Dynamics of General Relativity
- A Canonical Approach to the Einstein-Hilbert Action in Two Spacetime Dimensions
- Energy-Momentum Tensor Improvements in Two Dimensions
- Dirac and Lagrangian reductions in the canonical approach to the first order form of the Einstein-Hilbert action
- Peculiarities of the Canonical Analysis of the First Order Form of the Einstein-Hilbert Action in Two Dimensions in Terms of the Metric Tensor or the Metric Density
Cited by in corpus (12)
- Evolution of Spacetime arises due to the departure from Holographic Equipartition in all Lanczos-Lovelock Theories of Gravity
- Structure of Lanczos-Lovelock Lagrangians in Critical Dimensions
- A Canonical Analysis of the Einstein-Hilbert Action in First Order Form
- Perturbative Calculations with the First Order Form of Gauge Theories
- The Canonical Structure of the First Order Einstein-Hilbert Action
- Two-dimensional metric and tetrad gravities as constrained second order systems
- Analysis of Hamiltonian formulations of linearized General Relativity
- General Relativity in two dimensions: a Hamilton-Jacobi constraint analysis
- On the breakdown of space-time in general relativity
- Canonical Formulation of A Bosonic Matter Field in 1+1 Dimensional Curved Space
- Covariant Gauge Fixing and Canonical Quantization
- Algebraic analysis of a model of two-dimensional gravity