# Hybrid connections on Hessian manifolds

**Authors:** Arnaud Ch\'eritat, Guillaume Tahar

arXiv: 2302.12543 · 2026-04-14

## TL;DR

This paper introduces hybrid connections on Hessian manifolds, exploring their properties, and constructs a new natural connection on the unit ball that bridges hyperbolic models.

## Contribution

It defines hybrid connections with specific geometric properties, characterizes their differences from the Levi-Civita connection, and identifies a canonical model in pseudo-Euclidean spaces.

## Key findings

- The difference between hybrid and Levi-Civita connections is given by the logarithmic differential of a Hessian potential.
- A new natural connection on the open unit ball is constructed, bridging Cayley-Klein and Poincaré models.
- A unique pseudo-Riemannian metric makes unparameterized geodesics have constant speed with respect to the isochrone metric.

## Abstract

A Hessian manifold $(M,D,g)$ is a manifold $M$ with a flat connection $D$ and a Riemannian or pseudo-Riemannian metric $g$ that is locally of the form $D^2 f$ for some function $f$. On a Hessian manifold $(M,D,g)$, we define a hybrid connection as an incompressible affine connection $\nabla$ that is projectively flat relative to $D$ (its unparametrized geodesics are aligned with the affine structure of $D$) and whose first-order infinitesimal holonomy at each point of $M$ is an infinitesimal isometry of the pseudo-Riemannian metric $g$. In this paper, we investigate the properties of hybrid connections, proving in particular that for a hybrid connection $\nabla$, the difference $\nabla-D$ is determined by the logarithmic differential of a function that serves as a Hessian potential for $g$. In the special case of pseudo-Euclidean manifolds, we identify canonical models and obtain in particular a new natural connection on the open unit ball that provides a compromise between properties of Cayley-Klein and Poincar\'e hyperbolic models. We also find a unique (up to a scaling) pseudo-Riemannian metric $h$ such that unparameterized geodesics of $\nabla$ have a constant speed with respect to the so-called isochrone metric $h$.

## Full text

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## Figures

8 figures with captions in the complete paper: https://tomesphere.com/paper/2302.12543/full.md

## References

14 references — full list in the complete paper: https://tomesphere.com/paper/2302.12543/full.md

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Source: https://tomesphere.com/paper/2302.12543