Resumen

Despite the absence of a lightcone structure, some solutions of Carroll gravity show black hole-like behaviour. We define Carroll black holes as solutions of Carroll gravity that exhibit Carroll thermal properties and have a Carroll extremal surface, notions introduced in our work. The latter is a Carroll analogue of a Lorentzian extremal surface. As examples, we discuss the Carroll versions of Schwarzschild, Reissner–Nordström, and BTZ black holes and black hole solutions of generic 1+1 dimensional Carroll dilaton gravity, including Carroll JT and Carroll Witten black holes.

Idioma originalInglés
PublicaciónSciPost Physics
Volumen15
N.º6
DOI
EstadoPublicada - 2023

Nota bibliográfica

Publisher Copyright:
Copyright D. Fernández de la Pradilla et al. This work is licensed under the Creative Commons Attribution 4.0 International License.

Áreas temáticas de ASJC Scopus

  • Física y Astronomía General

Huella

Profundice en los temas de investigación de 'Carroll black holes'. En conjunto forman una huella única.

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