From the Weyl-Schr\"{o}dinger connection to the accelerating Universe -- extending Einstein's gravity via a length preserving nonmetricity

TL;DR

This paper explores a modified gravitational theory based on Schr"odinger's length-preserving nonmetricity, extending Einstein's gravity and providing a geometric explanation for dark energy, with implications for cosmology and the accelerating universe.

Contribution

It introduces a novel gravitational model using Schr"odinger's nonmetricity, analyzes its cosmological effects, and compares predictions with observational data, extending previous geometric approaches.

Findings

The metric variation yields extra nonmetricity terms acting as dark energy.

The theory's cosmological models fit observational Hubble data.

Comparison with DM shows promising agreement.

Abstract

One of the important extensions of Riemann geometry is Weyl geometry, which is essentially based on the ideas of conformal invariance and nonmetricity. A similar non-Riemannian geometry was proposed by Erwin Schr\"{o}dinger in the late 1940s, in a geometry which is simpler, and (probably) more elegant than the Weyl geometry. Even it contains nonmetricity, the Schr\"{o}dinger connection preserves the length of vectors under parallel transport, and thus seems to be more physical than the Weyl connection. Interestingly enough, Schr\"{o}dinger's approach did not attract much interest in the field of gravitational physics. It is the goal of the present paper to reconsider the Schr\"{o}dinger geometry as a potential candidate for a gravitational theory extending standard general relativity. We consider a gravitational action constructed from a length preserving non-metricity, in the absence of torsion, and investigate its variation in both Palatini and metric formalisms. While the Palatini variation leads to standard general relativity, the metric version of the theory adds some non-metricity dependent extra terms in the gravitational Einstein equations, which can be interpreted as representing a geometric type dark energy. After obtaining the generalized Friedmann equations, we analyze in detail the cosmological implications of the theory, by considering two distinct models, corresponding to a dark energy satisfying a linear equation of state, and to conserved matter energy, respectively. In both cases we compare the predictions of the Weyl-Schr\"{o}dinger cosmology with a set of observational data for the Hubble function, and with the results of the $\Lambda$CDM standard paradigm.