Schr\"odinger Connections: From Mathematical Foundations Towards Yano-Schr\"odinger Cosmology
Abstract
Schr\"odinger connections are a special class of affine connections, which despite being metric incompatible, preserve length of vectors under autoparallel transport. In the present paper, we introduce a novel coordinate-free formulation of Schr\"odinger connections. After recasting their basic properties in the language of differential geometry, we show that Schr\"odinger connections can be realized through torsion, non-metricity, or both. We then calculate the curvature tensors of Yano-Schr\"odinger geometry and present the first explicit example of a non-static Einstein manifold with torsion. We generalize the Raychaudhuri and Sachs equations to the Schr\"odinger geometry. The length-preserving property of these connections enables us to construct a Lagrangian formulation of the Sachs equation. We also obtain an equation for cosmological distances. After this geometric analysis, we build gravitational theories based on Yano-Schr\"odinger geometry, using both a metric and a metric-affine approach. For the latter, we introduce a novel cosmological hyperfluid that will source the Schr\"odinger geometry. Finally, we construct simple cosmological models within these theories and compare our results with observational data as well as the model.
Turn this paper into a lesson
ArcXiv compiles a structured reading guide from this paper's metadata: plain-English importance, contributions, prerequisite concepts, which sections to read first, flashcards, and a quiz. Grounded in the abstract, never invented.