The Canonical Lagrangian Approach To Three-Space General Relativity
Vasudev Shyam, Madhavan Venkatesh

TL;DR
This paper analyzes the canonical Lagrangian structure of three-space General Relativity, revealing the dynamics, gauge transformations, and symplectic reduction within the BF'O action framework.
Contribution
It provides a detailed study of the symplectic and presymplectic structures, deriving the canonical vector field and discussing observables in three-space GR.
Findings
Derived the canonical Lagrangian vector field for the BF'O action
Established the symplectic reduction of the constrained phase space
Clarified the gauge transformations and physical evolution in three-space GR
Abstract
We study the action for the three-space formalism of General Relativity, better known as the BF\'O (Barbour--Foster--\'O Murchadha) action, which is a square-root BSW (Baierlein--Sharp--Wheeler) action. In particular, we explore the (pre)symplectic structure by pulling it back via a Legendre map to the tangent bundle of the configuration space of this action. With it we attain the canonical Lagrangian vector field which generates the gauge transformations (3-diffeomorphisms) and the true physical evolution of the system. This vector field encapsulates all the dynamics of the system. We also discuss briefly the observables and perennials for this theory. We then present a symplectic reduction of the constrained phase space.
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