Hamiltonian approach to GR – Part 1: covariant theory of classical gravity

Abstract

Abstract A challenging issue in General Relativity concerns the determination of the manifestly covariant continuum Hamiltonian structure underlying the Einstein field equations and the related formulation of the corresponding covariant Hamilton–Jacobi theory. The task is achieved by adopting a synchronous variational principle requiring distinction between the prescribed deterministic metric tensor $$\widehat{g}(r)\equiv \{ \widehat{g}_{\mu \nu }(r)\} $$ g ^ ( r ) ≡ { g ^ μ ν ( r ) } solution of the Einstein field equations which determines the geometry of the background space-time and suitable variational fields $$x\equiv \{ g,\pi \} $$ x ≡ { g , π } obeying an appropriate set of continuum Hamilton equations, referred to here as GR-Hamilton equations. It is shown that a prerequisite for reaching such a goal is that of casting the same equations in evolutionary form by means of a Lagrangian parametrization for a suitably reduced canonical state. As a result, the corresponding Hamilton–Jacobi theory is established in manifestly covariant form. Physical implications of the theory are discussed. These include the investigation of the structural stability of the GR-Hamilton equations with respect to vacuum solutions of the Einstein equations, assuming that wave-like perturbations are governed by the canonical evolution equations.

Keywords

• Canonical Transformation
• Jacobi Equation
• Hamiltonian Structure
• Potential Density
• Gauge Function