The gauging procedure and carrollian gravity
arXiv:2206.14178 · doi:10.1007/JHEP09(2022)243
Abstract
We discuss a gauging procedure that allows us to construct lagrangians that dictate the dynamics of an underlying Cartan geometry. In a sense to be made precise in the paper, the starting datum in the gauging procedure is a Klein pair corresponding to a homogeneous space. What the gauging procedure amounts to is the construction of a Cartan geometry modelled on that Klein geometry, with the gauge field defining a Cartan connection. The lagrangian itself consists of all gauge-invariant top-forms constructed from the Cartan connection and its curvature. After demonstrating that this procedure produces four-dimensional General Relativity upon gauging Minkowski spacetime, we proceed to gauge all four-dimensional maximally symmetric carrollian spaces: Carroll, (anti-)de Sitter--Carroll and the lightcone. For the first three of these spaces, our lagrangians generalise earlier first-order lagrangians. The resulting theories of carrollian gravity all take the same form, which seems to be a manifestation of model mutation at the level of the lagrangians. The odd one out, the lightcone, is not reductive and this means that although the equations of motion take the same form as in the other cases, the geometric interpretation is different. For all carrollian theories of gravity we obtain analogues of the Gauss--Bonnet, Pontryagin and Nieh--Yan topological terms, as well as two additional terms that are intrinsically carrollian and seem to have no lorentzian counterpart. Since we gauge the theories from scratch this work also provides a no-go result for the electric carrollian theory in a first-order formulation.
arXiv comment34+1 pages, 2 figures
References in corpus (31)
- Barbero's Hamiltonian derived from a generalized Hilbert-Palatini action
- Conformal Carroll groups and BMS symmetry
- Carrollian Perspective on Celestial Holography
- Flat Holography: Aspects of the dual field theory
- Gauging the Carroll Algebra and Ultra-Relativistic Gravity
- Newtonian Gravity and the Bargmann Algebra
- Carrollian Physics at the Black Hole Horizon
- Flat holography and Carrollian fluids
- Carroll versus Galilei Gravity
- Horava-Lifshitz Gravity From Dynamical Newton-Cartan Geometry
- Fractons, dipole symmetries and curved spacetime
- MacDowell-Mansouri gravity and Cartan geometry
- Carroll Expansion of General Relativity
- BMS Group at Spatial Infinity: the Hamiltonian (ADM) approach
- The BMS4 algebra at spatial infinity
- Carroll symmetry of plane gravitational waves
- Connections and dynamical trajectories in generalised Newton-Cartan gravity II. An ambient perspective
- Carrollian and celestial spaces at infinity
- Topological Interpretation of Barbero-Immirzi Parameter
- 4d Lorentzian Holst action with topological terms
- Limits of JT gravity
- From the Einstein-Cartan to the Ashtekar-Barbero canonical constraints, passing through the Nieh-Yan functional
- Spatially isotropic homogeneous spacetimes
- AdS Carroll Chern-Simons supergravity in 2+1 dimensions and its flat limit
- Limits of three-dimensional gravity and metric kinematical Lie algebras in any dimension
- Asymptotic gravitational charges
- Three-dimensional Spin-3 Theories Based on General Kinematical Algebras
- Geometry and BMS Lie algebras of spatially isotropic homogeneous spacetimes
- Hamiltonian derivation of dual gravitational charges
- The Effective Action of Superrotation Modes
- Tractor geometry of asymptotically flat spacetimes