Geometry of Carrollian Stretched Horizons

TL;DR

This paper develops a comprehensive geometric and dynamical framework for Carrollian stretched horizons, unifying various causal surfaces and linking gravity with Carrollian fluid dynamics, with implications for black hole physics.

Contribution

It introduces a universal sCarrollian structure on any surface, generalizing null surface structures, and connects Einstein equations with Carrollian geometry and symmetries.

Findings

Unified sCarrollian framework for causal surfaces

Derived Einstein equations in sCarrollian variables

Linked gravity on horizons to Carrollian fluid dynamics

Abstract

In this paper, we present a comprehensive toolbox for studying Carrollian stretched horizons, encompassing their geometry, dynamics, symplectic geometry, symmetries, and corresponding Noether charges. We introduce a precise definition of ruled stretched Carrollian structures (sCarrollian structures) on any surface, generalizing the conventional Carrollian structures of null surfaces, along with the notions of sCarrollian connection and sCarrollian stress tensor. Our approach unifies the sCarrollian (intrinsic) and stretched horizon (embedding) perspectives, providing a universal framework for any causal surface, whether timelike or null. We express the Einstein equations in sCarrollian variables and discuss the phase space symplectic structure of the sCarrollian geometry. Through Noether's theorem, we derive the Einstein equation and canonical charge and compute the evolution of the canonical charge along the transverse (radial) direction. The latter can be interpreted as a spin-2 symmetry charge. Our framework establishes a novel link between gravity on stretched horizons and Carrollian fluid dynamics and unifies various causal surfaces studied in the literature, including non-expanding and isolated horizons. We expect this work to provide insights into the hydrodynamical description of black holes and the quantization of null surfaces.