The Newtonian limit of orthonormal frames in metric theories of gravity
arXiv:2410.01800 · doi:10.1007/s10714-025-03490-2
Abstract
We extend well-known results on the Newtonian limit of Lorentzian metrics to orthonormal frames. Concretely, we prove that, given a one-parameter family of Lorentzian metrics that in the Newtonian limit converges to a Galilei structure, any family of orthonormal frames for these metrics converges pointwise to a Galilei frame, assuming that the two obvious necessary conditions are satisfied: the spatial frame must not rotate indefinitely as the limit is approached, and the frame's boost velocity with respect to some fixed reference observer needs to converge.
12.5+3+1.5 pages (main text + references + appendix), to appear in General Relativity and Gravitation. v2: reference updated. v3: extended results, added references. v4: extended results. v5: corrected lemma
References in corpus (10)
- Carroll versus Newton and Galilei: two dual non-Einsteinian concepts of time
- Newtonian Gravity and the Bargmann Algebra
- Spacetime Symmetries of the Quantum Hall Effect
- Dynamics of Carroll Particles
- Lifshitz Space-Times for Schroedinger Holography
- Non-Relativistic Gravity and its Coupling to Matter
- Teleparallel Newton--Cartan gravity
- The Non-Relativistic Geometric Trinity of Gravity
- Generalized Newton-Cartan Geometries for Particles and Strings
- The classification of general affine connections in Newton--Cartan geometry: Towards metric-affine Newton--Cartan gravity