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Magnetic Carrollian gravity from the Carroll algebra

Indexado

WoS	WOS:000854842400002
Scopus	SCOPUS_ID:85138182612

DOI

10.1007/JHEP09(2022)127

Año

2022

Tipo

artículo de investigación

Citas Totales

Autores Afiliación Chile

Instituciones Chile

% Participación
Internacional

Autores
Afiliación Extranjera

Instituciones
Extranjeras

Abstract

We explicitly establish the equivalence between the magnetic Carrollian limit of Einstein gravity defined through the Hamiltonian formalism and the Carrollian theory of gravity defined through a gauging of the Carroll algebra along the lines of standard Poincaré (or (A)dS) gaugings.

Revista

Revista	ISSN
Journal Of High Energy Physics	1029-8479

Métricas Externas

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Disciplinas de Investigación

WOS
Physics, Particles & Fields

Scopus
Sin Disciplinas

SciELO
Sin Disciplinas

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Publicaciones WoS (Ediciones: ISSHP, ISTP, AHCI, SSCI, SCI), Scopus, SciELO Chile.

Colaboración Institucional

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Autores - Afiliación

Ord.	Autor	Género	Institución - País
1	Campoleoni, A.	Mujer	Université de Mons - Bélgica Univ Mons UMONS - Bélgica
2	Henneaux, M	Hombre	Université libre de Bruxelles - Bélgica Collège de France - Francia Univ Libre Bruxelles - Bélgica Coll France - Francia
3	Pekar, Simon	Hombre	Université de Mons - Bélgica Univ Mons UMONS - Bélgica
4	PEREZ-DONOSO, ALFREDO HECTOR	Hombre	Centro de Estudios Científicos - Chile Universidad San Sebastián - Chile
5	Salgado-Rebolledo, Patricio	Hombre	Wroclaw University of Science and Technology - Polonia Wroclaw Univ Sci & Technol - Polonia Politechnika Wroclawska - Polonia

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Financiamiento

Fuente
FONDECYT
ERC Advanced Grant "High-Spin-Grav"
FNRS-Belgium
Solvay Family
Fonds de la Recherche Scientifique FNRS-Belgium FNRS
Norwegian Financial Mechanism 2014-2021 via the National Science Centre (NCN) POLS grant

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Agradecimientos

Agradecimiento
We wish to thank Arnaud Delfante, Joaquim Gomis and Stefan Prohazka for useful discussions. The work of A.C. and S.P. was supported by the Fonds de la Recherche Scientifique FNRS-Belgium FNRS under Grants No. FC.36447, F.4503.20 (HighSpinSymm) and T.0022.19 (Fundamental issues in extended gravitational theories). The work of M.H. was partially supported by the ERC Advanced Grant "High-Spin-Grav", by FNRS-Belgium (conventions FRFC PDRT.1025.14 and IISN 4.4503.15), as well as by funds from the Solvay Family. The research of A.P. is partially supported by Fondecyt grants No. 1211226 and 1220910. P.S-R. has received funding from the Norwegian Financial Mechanism 2014-2021 via the National Science Centre (NCN) POLS grant 2020/37/K/ST3/03390.

Agradecimiento

We wish to thank Arnaud Delfante, Joaquim Gomis and Stefan Prohazka for useful discussions. The work of A.C. and S.P. was supported by the Fonds de la Recherche Scientifique FNRS-Belgium FNRS under Grants No. FC.36447, F.4503.20 (HighSpinSymm) and T.0022.19 (Fundamental issues in extended gravitational theories). The work of M.H. was partially supported by the ERC Advanced Grant "High-Spin-Grav", by FNRS-Belgium (conventions FRFC PDRT.1025.14 and IISN 4.4503.15), as well as by funds from the Solvay Family. The research of A.P. is partially supported by Fondecyt grants No. 1211226 and 1220910. P.S-R. has received funding from the Norwegian Financial Mechanism 2014-2021 via the National Science Centre (NCN) POLS grant 2020/37/K/ST3/03390.