Semi-Riemannian structures for symmetric Galilean spacetimes
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We introduce semi-Riemannian structures well-adapted to certain fields of observers in a Galilean spacetime. The Levi-Civita connection of such a semi-Riemannian metric will allow us to obtain variational characterizations of the Galilean geodesics as well as global results on the topological and differentiable structure of the spacetime. Moreover, these new semi-Riemannian metrics provide a new way to compare the studied Newton–Cartan models with their relativistic counterparts.
We introduce semi-Riemannian structures well-adapted to certain fields of observers in a Galilean spacetime. The Levi-Civita connection of such a semi-Riemannian metric will allow us to obtain variational characterizations of the Galilean geodesics as well as global results on the topological and differentiable structure of the spacetime. Moreover, these new semi-Riemannian metrics provide a new way to compare the studied Newton–Cartan models with their relativistic counterparts.
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Open Access funding provided thanks to the CRUE-CSIC agreement with Springer Nature.
The authors would like to thank the referees for their valuable comments and suggestions. The second author is partially supported by Spanish MICINN project PID2020-116126GB-I00. The rest of the authors are partially supported by Spanish MICINN project PID2021-126217NB-I00 and Andalusian FEDER 1380930-F.
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