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Charges, conserved quantities and fluxes in de Sitter spacetime

Charges, conserved quantities and fluxes in de Sitter spacetime
Charges, conserved quantities and fluxes in de Sitter spacetime

We discuss the definition of conserved quantities in asymptotically locally de Sitter spacetimes. One may define an analog of holographic charges at future and past infinity and at other Cauchy surfaces It as integrals over the intersection of timelike surfaces C and the Cauchy surface It. In general, the charges Qt defined on the Cauchy surface It depend on C, but if gravitational flux is absent the charges are independent of C. On the other hand, if there is a net gravitational flux entering or leaving the spacetime region bounded by C1, C2 and two Cauchy surfaces then ΔQt(C1,C2)=Qt(C1)-Qt(C2) changes by the same amount.

2470-0010
Skenderis, Kostas
09f32871-ffb1-4f4a-83bc-df05f4d17a09
Taylor, Marika
5515acab-1bed-4607-855a-9e04252aec22
Poole, Aaron D
d4c61a7b-87f8-4361-b794-449449b88d32
Skenderis, Kostas
09f32871-ffb1-4f4a-83bc-df05f4d17a09
Taylor, Marika
5515acab-1bed-4607-855a-9e04252aec22
Poole, Aaron D
d4c61a7b-87f8-4361-b794-449449b88d32

Skenderis, Kostas, Taylor, Marika and Poole, Aaron D (2022) Charges, conserved quantities and fluxes in de Sitter spacetime. Physical Review D, 106 (6), [L061901]. (doi:10.1103/PhysRevD.106.L061901).

Record type: Article

Abstract

We discuss the definition of conserved quantities in asymptotically locally de Sitter spacetimes. One may define an analog of holographic charges at future and past infinity and at other Cauchy surfaces It as integrals over the intersection of timelike surfaces C and the Cauchy surface It. In general, the charges Qt defined on the Cauchy surface It depend on C, but if gravitational flux is absent the charges are independent of C. On the other hand, if there is a net gravitational flux entering or leaving the spacetime region bounded by C1, C2 and two Cauchy surfaces then ΔQt(C1,C2)=Qt(C1)-Qt(C2) changes by the same amount.

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More information

Accepted/In Press date: 20 August 2022
Published date: 8 September 2022
Additional Information: Funding Information: K. S. and M. T. acknowledge support from the Science and Technology Facilities Council (Consolidated Grant “Exploring the Limits of the Standard Model and Beyond”). A. P. is supported by an EPSRC fellowship. Publisher Copyright: © 2022 authors. Published by the American Physical Society. Published by the American Physical Society under the terms of the "https://creativecommons.org/licenses/by/4.0/"Creative Commons Attribution 4.0 International license. Further distribution of this work must maintain attribution to the author(s) and the published article's title, journal citation, and DOI. Funded by SCOAP3.

Identifiers

Local EPrints ID: 470356
URI: http://eprints.soton.ac.uk/id/eprint/470356
ISSN: 2470-0010
PURE UUID: 402de3e8-af0a-4c00-acd1-7f8850f9e650
ORCID for Kostas Skenderis: ORCID iD orcid.org/0000-0003-4509-5472
ORCID for Marika Taylor: ORCID iD orcid.org/0000-0001-9956-601X
ORCID for Aaron D Poole: ORCID iD orcid.org/0000-0002-4966-4874

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Date deposited: 06 Oct 2022 17:14
Last modified: 17 Mar 2024 03:28

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