Tetrad Gravity; 2, Dirac's Observables

After a study of the Hamiltonian group of gauge transformations, whose infinitesimal generators are the 14 first class constraints, of a new formulation of canonical tetrad gravity on globally hyperbolic, asymptotically flat at spatial infinity, spacetimes with simultaneity spacelike hypersurfaces with the constraints generating space rotations and space diffeomorphisms on the cotriads are given. Their solutions give the dependence of the cotriads on transformations. The choice of 3-coordinates on $\Sigma_{\tau}$, namely the gauge fixing to the space diffeomorphisms constraints, is equivalent to the choice of how to parametrize the dependence of the cotriad on the last three degrees of freedom: namely to the choice of a parametrization of the superspace of 3-geometries. The Shanmugadhasan canonical transformation, corresponding to the choice of 3-orthogonal coordinates on $\Sigma_{\tau}$ and adapted to 13 of the 14 first class constraints, is found and the superhamiltonian constraint is rewritten in this canonical basis. Some interpretational problems connected with Dirac's observables are discussed: in particular the gauge interpretation of tetrad gravity based on constraint theory implies that a ``gravitational field" is an equivalence class of pseudo-Riemannian spacetimes including different 4-geometries, associated with a well defined equivalence class of conformally related 3-geomotries