Carrollian Approach to D Flat Holography
arXiv:2304.02696 · doi:10.1007/JHEP06(2023)051
Abstract
The isomorphism between the (extended) BMS algebra and the D Carrollian conformal algebra hints towards a co-dimension one formalism of flat holography with the field theory residing on the null-boundary of the asymptotically flat space-time enjoying a D Carrollian conformal symmetry. Motivated by this fact, we study the general symmetry properties of a source-less D Carrollian CFT, adopting a purely field-theoretic approach. After deriving the position-space Ward identities, we show how the D bulk super-translation and the super-rotation memory effects emerge from them, manifested by the presence of a temporal step-function factor in the same. Temporal-Fourier transforming these memory effect equations, we directly reach the bulk null-momentum-space leading and sub-leading soft graviton theorems. Along the way, we construct six Carrollian fields , , and corresponding to these soft graviton fields and the Celestial stress-tensors, purely in terms of the Carrollian stress-tensor components. The 2D Celestial shadow-relations and the null-state conditions arise as two natural byproducts of these constructions. We then show that those six fields consist of the modes that implement the super-rotations and a subset of the super-translations on the quantum fields. The temporal step-function allows us to relate the operator product expansions (OPEs) with the operator commutation relations via a complex contour integral prescription. We deduce that not all of those six fields can be taken together to form consistent OPEs. So choosing , and as the local fields, we form their mutual OPEs using only the OPE-commutativity property, under two general assumptions. The symmetry algebra manifest in these holomorphic-sector OPEs is then shown to be with an abelian ideal.
arXiv commentSection 3.3 is revised and contains a new result. Added references
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- Super-Carrollian and Super-Galilean Field Theories
- Symmetry group at future null infinity II: Vector theory
- Carrollian Supersymmetry and SYK-like models
- Carroll Hawking effect
- Quantization of Carrollian conformal scalar theories
- Extended Kinematical 3D Gravity Theories
- Irrelevant and marginal deformed BMS field theories
- Radiation in Fluid/Gravity and the Flat Limit
- Bulk Reconstruction of Scalar Excitations in Flat/CCFT and the Flat Limit from (A)dS/CFT
- Asymptotic Limit of Null Hypersurfaces
- Quantization of Carrollian fermions
- Carroll spinors
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- Hydrodynamics in the Carrollian regime
- Carroll-Schrödinger Equation
- Celestial Eikonal Amplitudes in the Near-Horizon Region
- Loop corrections versus marginal deformation in celestial holography
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- CFT reconstruction of local bulk operators in half-Minkowski space