The Chrono-geometrical Structure of Special and General Relativity: a Re-Visitation of Canonical Geometrodynamics
Luca Lusanna (INFN, Firenze)

TL;DR
This paper revisits the foundational structure of relativity theories, emphasizing the role of non-inertial frames and gauge variables in defining space-time and gravitational effects, leading to a unified view of interactions.
Contribution
It introduces a gauge-theoretic reformulation of relativistic and gravitational theories, clarifying the role of clock synchronization and inertial effects in a canonical framework.
Findings
The gauge variables represent relativistic inertial effects.
The entire chrono-geometrical structure is dynamically determined.
A new perspective on the Hole Argument links gravity and space-time.
Abstract
A modern re-visitation of the consequences of the lack of an intrinsic notion of instantaneous 3-space in relativistic theories leads to a reformulation of their kinematical basis emphasizing the role of non-inertial frames centered on an arbitrary accelerated observer. In special relativity the exigence of predictability implies the adoption of the 3+1 point of view, which leads to a well posed initial value problem for field equations in a framework where the change of the convention of synchronization of distant clocks is realized by means of a gauge transformation. This point of view is also at the heart of the canonical approach to metric and tetrad gravity in globally hyperbolic asymptotically flat space-times, where the use of Shanmugadhasan canonical transformations allows the separation of the physical degrees of freedom of the gravitational field (the tidal effects) from the…
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