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Gravitational observables, intrinsic coordinates, and canonical maps. (English) Zbl 1170.83392

Summary: It is well known that in a generally covariant gravitational theory the choice of spacetime scalars as coordinates yields phase-space observables (or “invariants”). However, their relation to the symmetry group of diffeomorphism transformations has remained obscure. In a symmetry-inspired approach we construct invariants out of canonically induced active gauge transformations. These invariants may be interpreted as the full set of dynamical variables evaluated in the intrinsic coordinate system.
The functional invariants can explicitly be written as a Taylor expansion in the coordinates of any observer, and the coefficients have a physical and geometrical interpretation. Surprisingly, all invariants can be obtained as limits of a family of canonical transformations. This permits a short (again geometric) proof that all invariants, including the lapse and shift, satisfy Poisson brackets that are equal to the invariants of their corresponding Dirac brackets.

MSC:

83C47 Methods of quantum field theory in general relativity and gravitational theory
70H45 Constrained dynamics, Dirac’s theory of constraints
70H33 Symmetries and conservation laws, reverse symmetries, invariant manifolds and their bifurcations, reduction for problems in Hamiltonian and Lagrangian mechanics

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