Abstract
We study the geometry of foliated non-Lorentzian spacetimes in terms of the Godbillon-Vey class of the foliation. We relate the intrinsic torsion of a foliated Aristotelian manifold to its Godbillon-Vey class, and interpret it as a measure of the local spin of the spatial leaves in the time direction. With this characterisation, the Godbillon-Vey class is an obstruction to integrability of the G -structure defining the Aristotelian spacetime. We use these notions to formulate a new geometric approach to hydrodynamics of fluid flows by endowing them with Aristotelian structures. We establish conditions under which the Godbillon-Vey class represents an obstruction to steady flow of the fluid and prove new conservation laws.
Original language | English |
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Article number | 455201 |
Journal | Journal of Physics A: Mathematical and Theoretical |
Volume | 56 |
Issue number | 45 |
Early online date | 13 Oct 2023 |
DOIs | |
Publication status | Published - 10 Nov 2023 |
Keywords
- G-structures
- foliations
- fluid dynamics
- non-relativistic structures
- Godbillon-Vey class