Canonical ADM Tetrad Gravity: from Metrological Inertial Gauge Variables to Dynamical Tidal Dirac observables
Luca Lusanna (INFN, Firenze)

TL;DR
This paper develops a Hamiltonian formulation of ADM tetrad gravity, identifying physical and gauge degrees of freedom, and explores how inertial effects in non-Euclidean 3-spaces could mimic dark matter phenomena.
Contribution
It introduces a canonical basis in ADM tetrad gravity that separates inertial and tidal variables and links relativistic metrology with gravitational degrees of freedom.
Findings
Inertial gauge variable ${}^3K$ can mimic dark matter effects.
The theory reproduces gravitational wave results in specific gauges.
Dark matter signatures may be interpreted as relativistic inertial effects.
Abstract
Dirac constraint theory allows to identify the York canonical basis (diagonalizing the York-Lichnerowicz approach) in ADM tetrad gravity for asymptotically Minkowskian space-times without super-translations. This allows to identify the inertial (gauge) and tidal (physical) degrees of freedom of the gravitational field and to interpret Ashtekar variables in these space-times. The use of radar 4-coordinates centered on a time-like observer allows to connect the 3+1 splittings of space-time with the relativistic metrology used in atomic physics and astronomy. The asymptotic ADM Poincar\'e group replaces the Poincar\'e group of particle physics. The general relativistic remnant of the gauge freedom in clock synchronization is described by the inertial gauge variable , the trace of the extrinsic curvature of the non-Euclidean 3-spaces. The theory can be linearized in a…
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