Three-dimensional Maxwellian Carroll gravity theory and the cosmological constant
Abstract
In this work, we present the three-dimensional Maxwell Carroll gravity by considering the ultra relativistic limit of the Maxwell Chern-Simons gravity theory defined in three spacetime dimensions. We show that an extension of the Maxwellian Carroll symmetry is necessary in order for the invariant tensor of the ultra-relativistic Maxwellian algebra to be non-degenerate. Consequently, we discuss the origin of the aforementioned algebra and theory as a flat limit. We show that the theoretical setup with cosmological constant yielding the extended Maxwellian Carroll Chern-Simons gravity in the vanishing cosmological constant limit is based on a new enlarged extended version of the Carroll symmetry. Indeed, the latter exhibits a non-degenerate invariant tensor allowing the proper construction of a Chern-Simons gravity theory which reproduces the extended Maxwellian Carroll gravity in the flat limit. (C) 2021 The Author(s). Published by Elsevier B.V.
Más información
Título según WOS: | Three-dimensional Maxwellian Carroll gravity theory and the cosmological constant |
Título de la Revista: | PHYSICS LETTERS B |
Volumen: | 823 |
Editorial: | ELSEVIER SCIENCE BV |
Fecha de publicación: | 2021 |
DOI: |
10.1016/j.physletb.2021.136735 |
Notas: | ISI |