The energy of the gravitational field (as of any other system) is not always the numerical value of the Hamiltonian (for example, not in a Hamilton-Jacobi formulation). We define a classical « Heisenberg representation » which excludes Hamilton-Jacobi-like canonical transformations. Ordinarily, within the Heisenberg representation, there remains only the possibility of time-independent canonical transformation among the dynamical variables. However, the freedom of co-ordinate transformations in general relativity allows many extra « canonical » transformations not found in conventional Lorentz covariant theory. This wider class of canonical formalisms possess all the properties usually associated with the Heisenberg picture in that in each formalism the measurable quantities,gμv(t), are obtained from knowledge of the canonical variables at the same time without any explicit co-ordinate dependence. Further, the Hamiltonian is a constant of motion. Only in Heisenberg frames is the Hamiltonian to be associated with the energy of the system. In spite of the additional freedom of canonical transformations (due to the freedom of co-ordinate change mentioned above), it is shown that the Hamiltonian is numerically the same for a fixed state of the gravitational field in any Heisenberg representation. The energy is then a uniquely definable quantity in the theory. In the process, it is established that two Heisenberg frames can differ by co-ordinate transformations that depend only on the canonical variables and not explicitly on the co-ordinates. These transformations must also preserve the property that at spatial infinity the metric become Lorentz so that the physical boundary conditions be unaltered.
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