Generic Theory of Geometrodynamics from Noether's theorem for the Diff(M) symmetry group
J\"urgen Struckmeier, David Vasak, Johannes Kirsch

TL;DR
This paper derives a comprehensive geometrodynamics framework from Noether's theorem applied to diffeomorphism invariance, generalizing Einstein's equations to include spin and mass effects on gravity and torsion.
Contribution
It introduces a generic Einstein-type equation derived from symmetry principles, extending general relativity to include massive spin particles and torsion effects.
Findings
Massive spin particles influence gravitational source terms.
Massive vector fields induce spacetime torsion.
The framework generalizes Einstein's equations to broader matter fields.
Abstract
We work out the most general theory for the interaction of spacetime geometry and matter fields -- commonly referred to as geometrodynamics -- for spin- and spin- particles. The minimum set of postulates to be introduced is that (i) the action principle should apply and that(ii) the total action should by form-invariant under the (local) diffeomorphism group. The second postulate thus implements the Principle of General Relativity. According to Noether's theorem, this physical symmetry gives rise to a conserved Noether current, from which the complete set of theories compatible with both postulates can be deduced. This finally results in a new generic Einstein-type equation, which can be interpreted as an energy-momentum balance equation emerging from the Lagrangian for the source-free dynamics of gravitation and the energy-momentum tensor of the source system .…
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