Spectral geometry of black holes in 4d gauged supergravity

P. Bargueño; E. Contreras; J. M. Peña

doi:10.3390/universe7040078

Spectral geometry of black holes in 4d gauged supergravity

P. Bargueño, E. Contreras, J. M. Peña

Física

Producción científica: Contribución a una revista › Artículo › revisión exhaustiva

Resumen

In this work we show that the area of the event horizon of the Chong–Cvetic–Lu–Pope black hole can be reconstructed in terms of the spectra of the Laplacian on the event horizon. This result, which extends previous works regarding the de Sitter–Kerr–Newman case, points towards a possible description of the black hole degrees of freedom in terms of the spectra of canonical operators defined on the event horizon.

Idioma original	Inglés
Número de artículo	78
Publicación	Universe
Volumen	7
N.º	4
DOI	https://doi.org/10.3390/universe7040078
Estado	Publicada - abr. 2021

Acceder al documento

10.3390/universe7040078

Otros archivos y enlaces

Enlace a la publicación en Scopus

Citar esto

@article{59147b07bdf54ecf97ff76e5008c5f69,

title = "Spectral geometry of black holes in 4d gauged supergravity",

abstract = "In this work we show that the area of the event horizon of the Chong–Cvetic–Lu–Pope black hole can be reconstructed in terms of the spectra of the Laplacian on the event horizon. This result, which extends previous works regarding the de Sitter–Kerr–Newman case, points towards a possible description of the black hole degrees of freedom in terms of the spectra of canonical operators defined on the event horizon.",

keywords = "Black holes, Spectral geometry, Supergravity",

author = "P. Bargue{\~n}o and E. Contreras and Pe{\~n}a, {J. M.}",

note = "Publisher Copyright: {\textcopyright} 2021 by the authors. Licensee MDPI, Basel, Switzerland.",

year = "2021",

month = apr,

doi = "10.3390/universe7040078",

language = "Ingl{\'e}s",

volume = "7",

journal = "Universe",

issn = "2218-1997",

number = "4",

}

TY - JOUR

T1 - Spectral geometry of black holes in 4d gauged supergravity

AU - Bargueño, P.

AU - Contreras, E.

AU - Peña, J. M.

PY - 2021/4

Y1 - 2021/4

N2 - In this work we show that the area of the event horizon of the Chong–Cvetic–Lu–Pope black hole can be reconstructed in terms of the spectra of the Laplacian on the event horizon. This result, which extends previous works regarding the de Sitter–Kerr–Newman case, points towards a possible description of the black hole degrees of freedom in terms of the spectra of canonical operators defined on the event horizon.

AB - In this work we show that the area of the event horizon of the Chong–Cvetic–Lu–Pope black hole can be reconstructed in terms of the spectra of the Laplacian on the event horizon. This result, which extends previous works regarding the de Sitter–Kerr–Newman case, points towards a possible description of the black hole degrees of freedom in terms of the spectra of canonical operators defined on the event horizon.

KW - Black holes

KW - Spectral geometry

KW - Supergravity

UR - http://www.scopus.com/inward/record.url?scp=85106895755&partnerID=8YFLogxK

U2 - 10.3390/universe7040078

DO - 10.3390/universe7040078

M3 - Artículo

AN - SCOPUS:85106895755

SN - 2218-1997

VL - 7

JO - Universe

JF - Universe

IS - 4

M1 - 78

ER -

Spectral geometry of black holes in 4d gauged supergravity

Resumen

Acceder al documento

Otros archivos y enlaces

Huella

Citar esto