General relativity treats space and time on the same footing, that is not what is done in Hamiltonian formulations. Therefore, in order to discuss general relativity in a Hamiltonian fashion, one needs to break that equal footing. This requires a space-time splitting, since only time derivatives are transformed to momenta but not space derivatives.. Chapter1. Introduction 3 BianchiIX-Maxwellsystem. InSection6.3,westudyafree&masslessclassicalscalar field coupled to the Bianchi IX-Maxwell system in the Hamiltonian formalism and

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for any Hamiltonian formulation of General Relativity (GR); (ii) the canonical treatment unavoidably breaks the symmetry between space and time in GR and the resulting algebra of constraints is not the algebra of four-dimensional diffeomorphism; (iii) according to some authors this algebra allows one to derive only spa-. Hamiltonian formalisms provide powerful tools for the computation of approximate analytic solutions of the Einstein field equations. The post-Newtonian computations of the explicit analytic dynamics and motion of compact binaries are discussed within the most often applied Arnowitt-Deser-Misner formalism. The obtention of autonomous Hamiltonians is achieved by the transition to Routhians.