Carrollian $\mathbb{R}^\times$-bundles II: Sigma Models on Event Horizons

Fuente: arXiv
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Autore principale: Bruce, Andrew James
Natura: Preprint
Pubblicazione: 2025
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_version_ 1866908456620916736
author Bruce, Andrew James
author_facet Bruce, Andrew James
contents Carrollian field theories are usually understood as limits of relativistic theories. In this note, we use Carrollian $\mathbb{R}^\times$-bundles equipped with a principal connection to construct Carrollian sigma models intrinsically. The resulting theories are neither ``electric'' nor ``magnetic'' in the usual sense. As a physically suggestive example, we derive a Carrollian wave equation governing the dynamics of a scalar field on the event horizon of a Schwarzschild black hole.
format Preprint
id arxiv_https___arxiv_org_abs_2507_00544
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Carrollian $\mathbb{R}^\times$-bundles II: Sigma Models on Event Horizons
Bruce, Andrew James
General Relativity and Quantum Cosmology
High Energy Physics - Theory
Mathematical Physics
53Z05, 70S99, 83Cxx
Carrollian field theories are usually understood as limits of relativistic theories. In this note, we use Carrollian $\mathbb{R}^\times$-bundles equipped with a principal connection to construct Carrollian sigma models intrinsically. The resulting theories are neither ``electric'' nor ``magnetic'' in the usual sense. As a physically suggestive example, we derive a Carrollian wave equation governing the dynamics of a scalar field on the event horizon of a Schwarzschild black hole.
title Carrollian $\mathbb{R}^\times$-bundles II: Sigma Models on Event Horizons
topic General Relativity and Quantum Cosmology
High Energy Physics - Theory
Mathematical Physics
53Z05, 70S99, 83Cxx
url https://arxiv.org/abs/2507.00544