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Main Authors: Arenas-Henriquez, Gabriel, Ciambelli, Luca, Diaz, Felipe, Jia, Weizhen, Rivera-Betancour, David
Format: Preprint
Published: 2025
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Online Access:https://arxiv.org/abs/2508.01446
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author Arenas-Henriquez, Gabriel
Ciambelli, Luca
Diaz, Felipe
Jia, Weizhen
Rivera-Betancour, David
author_facet Arenas-Henriquez, Gabriel
Ciambelli, Luca
Diaz, Felipe
Jia, Weizhen
Rivera-Betancour, David
contents We explore asymptotically locally anti-de Sitter spacetimes exhibiting gravitational radiative behavior, employing null gauges that allow for a well-defined flat limit. The radiative content in the bulk is captured by the boundary Cotton and stress tensor, which we collect into a radiative vector. We reinterpret this vector holographically in terms of fluid variables in the dual boundary theory. For algebraically special solutions, we uncover a close connection between bulk radiation and dissipative corrections in the boundary stress tensor, demonstrating a direct link between radiation and entropy production in the boundary fluid. This reveals a rich interplay between radiative dynamics in the bulk and out-of-equilibrium conformal physics at the boundary. We then investigate the flat limit of this correspondence in the context of flat-space holography. In this setting, we construct a Carrollian analogue of the radiative vector and introduce Celestial observables, such as energy detectors, which emerge naturally from the bulk's radiative structure. Our analysis shows that bulk radiation sources the Carrollian viscous stress tensor and heat current, which encodes the Bondi news in this framework. We illustrate our results with explicit examples, including Robinson-Trautman spacetimes and accelerating black holes.
format Preprint
id arxiv_https___arxiv_org_abs_2508_01446
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Radiation in Fluid/Gravity and the Flat Limit
Arenas-Henriquez, Gabriel
Ciambelli, Luca
Diaz, Felipe
Jia, Weizhen
Rivera-Betancour, David
High Energy Physics - Theory
General Relativity and Quantum Cosmology
We explore asymptotically locally anti-de Sitter spacetimes exhibiting gravitational radiative behavior, employing null gauges that allow for a well-defined flat limit. The radiative content in the bulk is captured by the boundary Cotton and stress tensor, which we collect into a radiative vector. We reinterpret this vector holographically in terms of fluid variables in the dual boundary theory. For algebraically special solutions, we uncover a close connection between bulk radiation and dissipative corrections in the boundary stress tensor, demonstrating a direct link between radiation and entropy production in the boundary fluid. This reveals a rich interplay between radiative dynamics in the bulk and out-of-equilibrium conformal physics at the boundary. We then investigate the flat limit of this correspondence in the context of flat-space holography. In this setting, we construct a Carrollian analogue of the radiative vector and introduce Celestial observables, such as energy detectors, which emerge naturally from the bulk's radiative structure. Our analysis shows that bulk radiation sources the Carrollian viscous stress tensor and heat current, which encodes the Bondi news in this framework. We illustrate our results with explicit examples, including Robinson-Trautman spacetimes and accelerating black holes.
title Radiation in Fluid/Gravity and the Flat Limit
topic High Energy Physics - Theory
General Relativity and Quantum Cosmology
url https://arxiv.org/abs/2508.01446