Carrollian Perspective on Celestial Holography
Pith reviewed 2026-05-23 01:22 UTC · model grok-4.3
The pith
A 3d sourced conformal Carrollian field theory holographically describes 4d asymptotically flat gravity.
A machine-rendered reading of the paper's core claim, the machinery that carries it, and where it could break.
Core claim
We show that a 3d sourced conformal Carrollian field theory has the right kinematic properties to holographically describe gravity in 4d asymptotically flat spacetime. The external sources encode the leaks of gravitational radiation at null infinity. The Ward identities of this theory are shown to reproduce those of the 2d celestial CFT after relating Carrollian to celestial operators. This suggests a new set of interplays between gravity in asymptotically flat spacetime, sourced conformal Carrollian field theory and celestial CFT.
What carries the argument
The operator mapping between the 3d Carrollian theory and the 2d celestial CFT that transfers the Ward identities while the external sources track radiation leaks.
If this is right
- External sources in the Carrollian theory directly encode the gravitational radiation escaping at null infinity.
- The Ward identities match those of the celestial CFT once Carrollian operators are related to celestial ones.
- The 3d theory supplies the correct kinematic structure for a holographic description of 4d flat gravity.
- The construction creates a direct bridge among asymptotically flat gravity, sourced Carrollian field theory, and celestial CFT.
Where Pith is reading between the lines
- The same operator relation might be tested on concrete observables such as soft graviton theorems to check consistency.
- Carrollian structures could supply new tools for computing scattering data in flat spacetime that are not available in the celestial CFT alone.
- The framework may extend to other Carrollian limits of known holographic dualities.
Load-bearing premise
The mapping from Carrollian operators to celestial operators transfers the complete set of Ward identities without missing or adding terms or anomalies.
What would settle it
An explicit computation of the Ward identities in a simple case that shows a mismatch after applying the Carrollian-to-celestial operator relation would disprove the reproduction claim.
read the original abstract
We show that a $3d$ sourced conformal Carrollian field theory has the right kinematic properties to holographically describe gravity in $4d$ asymptotically flat spacetime. The external sources encode the leaks of gravitational radiation at null infinity. The Ward identities of this theory are shown to reproduce those of the $2d$ celestial CFT after relating Carrollian to celestial operators. This suggests a new set of interplays between gravity in asymptotically flat spacetime, sourced conformal Carrollian field theory and celestial CFT.
Editorial analysis
A structured set of objections, weighed in public.
Referee Report
Summary. The paper claims that a 3d sourced conformal Carrollian field theory has the kinematic properties to holographically describe 4d asymptotically flat gravity, with external sources encoding gravitational radiation leaks at null infinity. After relating Carrollian operators to celestial operators, the Ward identities of the Carrollian theory reproduce those of the 2d celestial CFT, suggesting new interplays between these frameworks.
Significance. If the operator mapping is shown to preserve the full set of identities, the result would provide a concrete link between sourced Carrollian theories, celestial CFT, and flat-space holography, with sources offering a direct encoding of radiation. This could supply new calculational tools for Ward identities in asymptotically flat settings.
major comments (2)
- [§4] §4: The operator relation is introduced as a direct identification of generators and fields, but the manuscript does not derive that this mapping pulls back the sourced Carrollian Ward identities exactly onto the celestial ones, including all source terms for radiation leaks, without generating extra contact terms or anomalies.
- [§3] §3 and abstract: The claim that the 3d sourced Carrollian theory possesses the 'right kinematic properties' for 4d flat gravity holography is supported only by the reproduction statement; no explicit verification of completeness or anomaly cancellation under the mapping is provided, leaving the central kinematic equivalence unverified at the local level.
minor comments (1)
- The notation distinguishing Carrollian conformal transformations from standard celestial ones could be made more explicit with a side-by-side comparison of generators.
Simulated Author's Rebuttal
We thank the referee for their careful reading of the manuscript and for the constructive comments. We respond to each major comment below and will revise the manuscript to incorporate additional details where appropriate.
read point-by-point responses
-
Referee: [§4] The operator relation is introduced as a direct identification of generators and fields, but the manuscript does not derive that this mapping pulls back the sourced Carrollian Ward identities exactly onto the celestial ones, including all source terms for radiation leaks, without generating extra contact terms or anomalies.
Authors: The mapping is introduced via direct identification of the Carrollian and celestial generators together with the corresponding field operators, which is justified by the shared symmetry structure. The manuscript then demonstrates that the Ward identities reproduce under this relation, including the source terms. We agree, however, that an explicit step-by-step derivation confirming the absence of extraneous contact terms or anomalies would strengthen the argument. We will add this derivation to §4 in the revised manuscript. revision: yes
-
Referee: [§3] The claim that the 3d sourced Carrollian theory possesses the 'right kinematic properties' for 4d flat gravity holography is supported only by the reproduction statement; no explicit verification of completeness or anomaly cancellation under the mapping is provided, leaving the central kinematic equivalence unverified at the local level.
Authors: The kinematic properties are established through the matching of the asymptotic symmetry algebras and the explicit reproduction of the Ward identities (which encode the relevant kinematic constraints of 4d flat gravity). We acknowledge that a more detailed local-level verification of completeness and anomaly cancellation would be valuable. We will expand the discussion in §3 and the abstract to include such explicit checks in the revised version. revision: yes
Circularity Check
No significant circularity; derivation chain is self-contained
full rationale
The provided abstract and context describe a mapping between Carrollian and celestial operators that is used to reproduce Ward identities, but no equations or sections are quoted that reduce this reproduction to a self-definition, fitted input, or self-citation chain. The operator relation is presented as an independent step whose validity is external to the target result. No load-bearing self-citations or ansatze smuggled via prior work appear in the text. This is the normal case of an honest non-finding.
Axiom & Free-Parameter Ledger
axioms (2)
- domain assumption A conformal Carrollian field theory in 3d exists with sources that encode null-infinity radiation leaks.
- domain assumption Relating Carrollian operators to celestial operators preserves the full set of Ward identities without extra terms.
Forward citations
Cited by 24 Pith papers
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Kinetic Theory of Carroll Hydrodynamics
A microscopic derivation of Carrollian fluid equations from a statistical mechanics of interacting instantonic branes, plus initial elements of Carrollian thermodynamics.
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Kinetic Theory of Carroll Hydrodynamics
A kinetic theory of interacting instantonic branes yields a first-principles derivation of Carrollian fluid equations and initial elements of Carrollian thermodynamics.
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Carrollian quantum states and flat space holography
Carrollian QFTs from scalar limits admit regular invariant vacua and KMS states only in the massive electric sector; a factorizing quasifree state is constructed for flat-space holography isolating nonseparable zero modes.
-
A Twisted Origin for Magnetic Carroll Supersymmetry
Magnetic Carroll supersymmetry descends from a twisted relativistic parent rather than naive contraction, realized in 3D N=2 with vector multiplet action whose conformal extension matches global super-BMS4.
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On $\sqrt{T\overline{T}}$ deformed pathways: CFT to CCFT
The marginal √(T T-bar) deformation of 2D massless scalars provides a dynamical map from relativistic CFT to Carrollian CCFT symmetries, recovering the electric Carroll theory and a novel magnetic counterpart in the e...
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Kerroll black holes
Rotating black holes are constructed in Carroll gravity via connection freedom and an odd-power GR expansion, yielding an intrinsically Carrollian rotating solution and the Kerroll black hole analog.
-
Carroll fermions from null reduction: A case of good and bad fermions
Carrollian fermionic actions for electric and magnetic sectors are derived from a single Bargmann Dirac action by null reduction, with good and bad fermions as dynamical and constrained modes valid in any dimension.
-
Carrollian ABJM: Fermions and Supersymmetry
The c to zero limit of ABJM theory produces a Carrollian superconformal theory with extended BMS4 symmetry using Carrollian Dirac matrices.
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Carroll fermions, expansions and the lightcone
Carrollian fermion actions are obtained from relativistic Dirac theory via c-expansion and connected to light-cone dynamics through co-dimension one Carroll subalgebras in the Poincaré algebra.
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Celestial 1-form symmetries
In self-dual Yang-Mills the S-algebra becomes an algebra of 1-form symmetries whose 2-form currents link integrability to the equality of Carrollian corner charges and celestial chiral algebra modes.
-
Towards a Carrollian Description of Yang-Mills
A Carrollian theory on null infinity reproduces all MHV and NMHV Yang-Mills tree amplitudes, with a new explicit NMHV expression.
-
On Carrollian Loop Amplitudes for Gauge Theory and Gravity
Loop-level Carrollian amplitudes in N=4 SYM and N=8 supergravity are differential operators on tree-level versions, with logarithmic eikonal behavior and IR-safe factorization via natural splitting.
-
The gravitational S-matrix from the path integral: asymptotic symmetries and soft theorems
A path integral with asymptotic boundary conditions produces the gravitational S-matrix and derives soft graviton theorems from extended BMS symmetry Ward identities.
-
Soft Algebras in AdS$_4$ from Light Ray Operators in CFT$_3$
A conformal map identifies the flat-space soft gluon S-algebra with light-ray operators built from CFT3 currents and their descendants in AdS4.
-
From Asymptotically Flat Gravity to Finite Causal Diamonds
The soft sector phase space of asymptotically flat gravity equals the phase space of radial size fluctuations of a finite causal diamond in flat spacetime.
-
Conformal Blocks in 2d Carrollian/Galilean CFTs and Excited State Entanglement Entropy
Derives heavy-light conformal blocks in 2d C/G CFTs and computes excited-state entanglement entropy via replica trick, finding thermal form that reproduces holographic EE and establishes dictionary between boundary we...
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Strings near BTZ black holes: A Carrollian Chronicle
The paper classifies families of closed bosonic string solutions in the near-horizon non-extremal BTZ spacetime and identifies novel features via string-Carroll expansion.
-
Radiation in Fluid/Gravity and the Flat Limit
Establishes a holographic link between bulk gravitational radiation and dissipative corrections plus entropy production in boundary fluids, then constructs Carrollian analogues and celestial observables in the flat limit.
-
QFT in Klein space
Authors construct canonical and path-integral quantizations for QFT in Klein space using extra modes, deriving correlation functions that match Minkowski space via analytical continuation.
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Operator Product Expansion in Carrollian CFT
Constructs Carrollian OPEs that govern short-distance behavior, extends representation theory for composites, and classifies 2-, 3-, and 4-point correlators/amplitudes under Carrollian symmetry.
-
On Carrollian Loop Amplitudes for Gauge Theory and Gravity
Loop-level Carrollian amplitudes in gauge theory and gravity preserve tree-level structures, show logarithmic dependence in the eikonal regime, and factorize to yield an IR-safe definition.
-
More on Bulk Local State Reconstruction in Flat/Carr CFT
Bulk local states are built in flat holography via induced representations, with a dual basis resolving 3D bra-ket scaling issues and a tilde basis enabling explicit constructions in higher dimensions that recover the...
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Lectures on the Bondi--Metzner--Sachs group and related topics in infrared physics
Lecture notes that build the BMS group from prerequisites to applications in soft theorems, memory effects, and new material on asymptotic conformal Killing horizons.
-
The Carrollian Kaleidoscope
A review summarizing Carrollian symmetries, CCFT constructions, and applications in AFS holography, Carroll hydrodynamics, and condensed matter phenomena such as fractons and flat bands.
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