Strings near black holes are Carrollian

Fuente: arXiv
Guardado en:
Detalles Bibliográficos
Autores principales: Bagchi, Arjun, Banerjee, Aritra, Hartong, Jelle, Have, Emil, Kolekar, Kedar S., Mandlik, Mangesh
Formato: Preprint
Publicado: 2023
Materias:
Acceso en línea:
Etiquetas: Agregar Etiqueta
Sin Etiquetas, Sea el primero en etiquetar este registro!
_version_ 1866913285761138688
author Bagchi, Arjun
Banerjee, Aritra
Hartong, Jelle
Have, Emil
Kolekar, Kedar S.
Mandlik, Mangesh
author_facet Bagchi, Arjun
Banerjee, Aritra
Hartong, Jelle
Have, Emil
Kolekar, Kedar S.
Mandlik, Mangesh
contents We demonstrate that strings near the horizon of a Schwarzschild black hole, when viewed by a stationary observer at infinity, probe a string Carroll geometry, where the effective lightspeed is given by the distance from the horizon. We expand the Polyakov action in powers of this lightspeed to find a theory of Carrollian strings. We show that the string shrinks to a point to leading order near the horizon, which follows a null geodesic in a two-dimensional Rindler space. At the next-to-leading order the string oscillates in the embedding fields associated with the near-horizon two-sphere.
format Preprint
id arxiv_https___arxiv_org_abs_2312_14240
institution arXiv
publishDate 2023
record_format arxiv
spellingShingle Strings near black holes are Carrollian
Bagchi, Arjun
Banerjee, Aritra
Hartong, Jelle
Have, Emil
Kolekar, Kedar S.
Mandlik, Mangesh
High Energy Physics - Theory
General Relativity and Quantum Cosmology
We demonstrate that strings near the horizon of a Schwarzschild black hole, when viewed by a stationary observer at infinity, probe a string Carroll geometry, where the effective lightspeed is given by the distance from the horizon. We expand the Polyakov action in powers of this lightspeed to find a theory of Carrollian strings. We show that the string shrinks to a point to leading order near the horizon, which follows a null geodesic in a two-dimensional Rindler space. At the next-to-leading order the string oscillates in the embedding fields associated with the near-horizon two-sphere.
title Strings near black holes are Carrollian
topic High Energy Physics - Theory
General Relativity and Quantum Cosmology
url https://arxiv.org/abs/2312.14240