Carrollian manifolds can be described as principal R^x-bundles with a degenerate metric, and a chosen connection yields a canonical non-degenerate metric and geodesic dynamics.
Carrollian $\mathbb{R}^\times$-bundles III: The Hodge Star and Hodge--de Rham Laplacians
1 Pith paper cite this work. Polarity classification is still indexing.
abstract
Carrollian $\mathbb{R}^\times$-bundles ($\mathbb{R}^\times := \mathbb{R}\setminus \{0\}$) offer a novel perspective on intrinsic Carrollian geometry using the powerful tools of principal bundles. Given a choice of principal connection, a canonical Lorentzian metric exists on the total space. This metric enables the development of Hodge theory on a Carrollian $\mathbb{R}^\times$-bundle; specifically, the Hodge star operator and Hodge--de Rham Laplacian are constructed. These constructions are obstructed on a Carrollian manifold due to the degenerate metric. The framework of Carrollian $\mathbb{R}^\times$-bundles bridges the gap between Carrollian geometry and (pseudo)-Riemannian geometry. As an example, the question of the Hodge--de Rham Laplacian on the event horizon of a Schwarzschild black hole is addressed. A Carrollian version of electromagnetism is also proposed.
citation-role summary
citation-polarity summary
fields
math.DG 1years
2025 1verdicts
CONDITIONAL 1roles
background 1polarities
support 1representative citing papers
citing papers explorer
-
Carrollian $\mathbb{R}^\times$-bundles: Connections and Beyond
Carrollian manifolds can be described as principal R^x-bundles with a degenerate metric, and a chosen connection yields a canonical non-degenerate metric and geodesic dynamics.