Carrollian origin of spacetime subsystem symmetry

Oguzhan Kasikci; Mehmet Ozkan; Yi Pang

doi:10.1103/PhysRevD.108.045020

Carrollian origin of spacetime subsystem symmetry

Oguzhan Kasikci, Mehmet Ozkan^*, Yi Pang^*

^*Corresponding author for this work

Department of Physics Engineering

Research output: Contribution to journal › Article › peer-review

15 Citations (Scopus)

Abstract

We propose that models with spacetime subsystem symmetry are connected to Lorentz invariant models via the Carrollian limit. In this way, a recently proposed model with spacetime subsystem symmetry was readily reproduced together with its conserved charges. We then couple this model to a dynamical Abelian gauge field and Carroll gravity. Our procedure can be applied in arbitrary dimensions and paves the way to construct new models with spacetime subsystem symmetry.

Original language	English
Article number	045020
Journal	Physical Review D
Volume	108
Issue number	4
DOIs	https://doi.org/10.1103/PhysRevD.108.045020
Publication status	Published - 15 Aug 2023

Bibliographical note

Publisher Copyright:
© 2023 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.

Funding

We are grateful to Utku Zorba for feedback and comments on the manuscript. M. O. is supported in part by TUBITAK Grant No. 121F064 and Istanbul Technical University Research Fund under Grant No. TGA-2020-42570. M. O. acknowledges the support by the Distinguished Young Scientist Award BAGEP of the Science Academy. M. O. also acknowledges the support by the Outstanding Young Scientist Award of the Turkish Academy of Sciences (TUBA-GEBIP). The work of Y. P. is supported in part by National Natural Science Foundation of China (NSFC) under Grant No. 12175164. Y. P. also acknowledges support by the National Key Research and Development Program under Grant No. 2022YFE0134300.

Funders	Funder number
Istanbul Technical University Research Fund	TGA-2020-42570
TUBA-GEBIP
National Natural Science Foundation of China	12175164
Türkiye Bilimsel ve Teknolojik Araştırma Kurumu	121F064
Türkiye Bilimler Akademisi
Bilim Akademisi
National Key Research and Development Program of China	2022YFE0134300

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10.1103/PhysRevD.108.045020

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Carrollian origin of spacetime subsystem symmetry

Abstract

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