{"total":22,"items":[{"citing_arxiv_id":"2606.27421","ref_index":3,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Observing Massive Scattering from Null Infinity","primary_cat":"hep-th","submitted_at":"2026-06-25T18:00:00+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Late-time Bondi mass aspect at future null infinity acts as a detector for massive radiation, with its in-in correlations relating to weighted sums of scattering cross sections.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.26163","ref_index":108,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Large-$N$ Carrollian Thermodynamics from AdS Black-Hole Phase-Space Contractions","primary_cat":"hep-th","submitted_at":"2026-06-24T06:24:41+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"Finite Carrollian black-hole thermodynamics arises as a double-scaled low-temperature large-N ensemble in AdS/CFT, with the boundary Brown-York stress tensor reproducing the contracted bulk Hamiltonian and first law.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.05303","ref_index":35,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Krylov Complexity: Flat bands and Carroll breaking deformations","primary_cat":"hep-th","submitted_at":"2026-06-03T18:00:19+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Krylov complexity growth distinguishes phase-dependent resilience of Carrollian sectors in all-bands-flat fermionic ladders against delocalizing perturbations and exhibits UV sensitivity in a continuum Carroll scalar field with gradient deformation.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.03955","ref_index":12,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Flat from AdS: in any dimension and for any spin","primary_cat":"hep-th","submitted_at":"2026-06-02T17:43:00+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"Recovers Minkowski massless integer-spin solution space as smooth limit of AdS solution space for even dimensions via cosmological-constant expansion of source and vev.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.02722","ref_index":36,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Asymptotically-FLRW$_3$ spacetimes","primary_cat":"gr-qc","submitted_at":"2026-06-01T18:00:07+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"Introduces asymptotically-FLRW3 spacetimes whose asymptotic symmetry group is the one-parameter family BMS3^k, fully characterizes the scalar-field solution space, identifies covariant mass/angular-momentum aspects and news via vacuum orbits, and exhibits exactly conserved non-linear Newman-Penrose ","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.15269","ref_index":14,"ref_count":2,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Kerroll black holes","primary_cat":"hep-th","submitted_at":"2026-05-14T18:00:01+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"Rotating black holes are constructed in magnetic Carroll gravity, including an intrinsically Carrollian dressed solution and a Kerroll black hole from an odd-power c-expansion of GR, with conserved charges computed.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.09947","ref_index":63,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"The Free Particle--Oscillator--Inverted Oscillator Triangle: Conformal Bridges, Metaplectic Rotations and $\\mathfrak{osp}(1|2)$ Structure","primary_cat":"hep-th","submitted_at":"2026-05-11T03:51:09+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"The free particle, harmonic oscillator, and inverted oscillator are unified as parabolic, elliptic, and hyperbolic realizations of the same conformal module, with explicit mappings between their states, coherent states, and scattering data via metaplectic rotations and Mellin transforms.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"Quant. Grav.31(2014) 205009; [arXiv:1405.2264 [hep-th]]. [61] L. Marsot,\"Planar Carrollean dynamics, and the Carroll quantum Hall effect,\"Annals Phys.447(2022) 168582; [arXiv:2110.08489 [hep-th]]. [62] J. Figueroa-O'Farrill, A. Pérez and S. Prohazka,\"Carroll/fracton particles and their correspondence,\"JHEP06(2023) 207; [arXiv:2305.06730 [hep-th]]. 47 [63] R. Ruzziconi,\"Carrollian physics and holography,\"Phys. Rept.1182(2026) 1-87; [arXiv:2602.02644 [hep-th]]. [64] M. Castagnino, R. Diener, L. Lara, G. Puccini,\"Rigged Hilbert spaces and time-asymmetry: the case of the upside-down simple harmonic oscillator,\"Int. J. Theor. Phys.36(1997) 2349; [arXiv:quant-ph/0006011]. [65] A. Prouff,\"Egorov's theorem in the Weyl-Hörmander calculus,\"[arXiv:2412."},{"citing_arxiv_id":"2605.05334","ref_index":36,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Carroll fermions from null reduction: A case of good and bad fermions","primary_cat":"hep-th","submitted_at":"2026-05-06T18:06:01+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"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.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"Gomis,A non-lorentzian primer,SciPost Phys. Lect. Notes69(2023) 1, [2206.12177]. [33] A. Bagchi, A. Banerjee, P. Dhivakar, S. Mondal and A. Shukla,The Carrollian kaleidoscope, Eur. Phys. J. C86(2026) 429, [2506.16164]. [34] L. Ciambelli and P. Jai-akson,Foundations of Carrollian Geometry, [2510.21651]. [35] K. Nguyen,Lectures on Carrollian Holography, [2511.10162]. [36] R. Ruzziconi,Carrollian physics and holography,Phys. Rept.1182(2026) 1-87, [2602.02644]. [37] E. Ekiz, E. O. Kahya and U. Zorba,Quantization of Carrollian fermions,Phys. Rev. D111 (2025) 105019, [2502.05645]. [38] K. Banerjee, R. Basu, B. Krishnan, S. Maulik, A. Mehra and A. Ray,One-loop quantum effects in Carroll scalars,Phys. Rev. D108(2023) 085022, [2307."},{"citing_arxiv_id":"2605.03155","ref_index":23,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Flat Space Physics from AdS Actions","primary_cat":"hep-th","submitted_at":"2026-05-04T20:53:41+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"Reducing 4D massless and massive scalar actions in flat and Klein space to 3D theories on hyperbolic slices produces continuous spectra linked by boundary terms, with boundary modes matching light-cone or null-infinity limits.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"Additionally, we study how the reduced field variables behave under the extrapolate dictio- nary. For massless fields, the extrapolate limits of the reduced 3D field are equivalent to taking a limit where the 4D field approaches the lightcone or null infinity, matching the natural holo- graphic dictionary that has been studied for massless particles in Minkowski space [23]. For massive scalars, however, only one of the possible extrapolate limits encodes the value of the field on the lightcone. The other limit seemingly has no nice geometric interpretation. Under- standing what the 3D extrapolate limit of the reduced field computes will hopefully lead to a deeper understanding of the role of massive particles in flat space holography."},{"citing_arxiv_id":"2604.27815","ref_index":14,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Couch-Torrence conformal inversion, supersymmetry and conserved charges for D3-branes","primary_cat":"hep-th","submitted_at":"2026-04-30T12:57:58+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"Couch-Torrence inversion matches Newman-Penrose charges at null infinity to Aretakis charges near horizons for D3-branes in D=10 and bound states in D=4,5, with supersymmetry mapping scalar charges to spinorial dilatino charges.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"On the other hand, thanks to the geometric duality between null infinity 1 and extremal non-expanding (non-) rotating horizons put forward in [11] it is tantalizing to speculate on a possible 'holographic' interpretation of the conserved NP charges as KK modes of the 'dilaton' and its superpartners also at null infinity. This observation may give more than a hint to Carrollian 'flat-space holography' [14,15], possibly in connection with 'celestial holography' [16] and BMSVB (Bondi-Metzner-Sachs and Van de Burg) super-translations and super-rotations [17-20]. One should however, be careful as to the classical nature of this correspondence. After all, Weyl anomalies could require corrections to the map between the two sets of asymptotic charges. This treatment goes beyond the scope of our current analysis."},{"citing_arxiv_id":"2604.27449","ref_index":11,"ref_count":3,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Phase-Space Contractions of Carrollian Black-Hole Thermodynamics","primary_cat":"hep-th","submitted_at":"2026-04-30T05:44:38+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Double-scaling contractions of extended AdS black-hole thermodynamics produce finite Carrollian phase-space first laws with pressure-volume contributions under the condition α + γ = 1.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2604.27068","ref_index":23,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Holographic realization of higher-spin Carrollian free fields","primary_cat":"hep-th","submitted_at":"2026-04-29T18:02:46+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"A bulk construction in asymptotically flat higher-spin gravity realizes Carrollian free fields and Miura transformations via generalized boundary conditions and screening charges.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"mal algebra [22]. Taken together, this result, along with the insights gained from the AdS case, provided a conceptual foundation for flat space holography, suggesting that gravity in asymptotically flat spacetimes could admit a dual description in terms of a codimension-one Carrollian conformal field theory (CCFT) living at null infinity (see, e.g., [23] for a review). This framework was subsequently extended to higher-spin theories [24, 25] in generalized Bondi gauges. In particular, spin-three gravity in flat space was shown to exhibit an asymp- totic symmetry algebra given by a Carrollian analogue of theW3 algebra. More generally, flat space higher-spin gravity theories, constructed from the corresponding flat higher-spin"},{"citing_arxiv_id":"2604.23677","ref_index":9,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Stationary solutions in the small-$c$ expansion of GR","primary_cat":"gr-qc","submitted_at":"2026-04-26T12:30:50+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"Exact Lense-Thirring-type, C-metric-type, and Hartle-Thorne-type stationary vacuum solutions are constructed in the NLO and NNLO small-c expansion of GR, revealing a richer sector than magnetic Carroll gravity.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"de Boer, J. Hartong, N. A. Obers, W. Sybesma and S. Vandoren,Carroll Symmetry, Dark Energy and Inflation,Front. in Phys.10(2022) 810405, [2110.02319]. [7] J. de Boer, J. Hartong, N. A. Obers, W. Sybesma and S. Vandoren,Carroll stories,JHEP09 (2023) 148, [2307.06827]. [8] L. Ciambelli and P. Jai-akson,Foundations of Carrollian Geometry,2510.21651. [9] R. Ruzziconi,Carrollian physics and holography,Phys. Rept.1182(2026) 1-87, [2602.02644]. [10] A. Bagchi, A. Banerjee, R. Chatterjee and P. Pandit,The Tensionless Lives of Null Strings, 2601.20959. [11] A. Bagchi, A. Bhattacharya, S. Rajesh Iyer and K. Narayan,Black hole Near Horizons through the Looking Glass,2602.20267. [12] K. Nguyen,Lectures on Carrollian Holography,2511."},{"citing_arxiv_id":"2604.22745","ref_index":21,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Carrollian quantum states and flat space holography","primary_cat":"hep-th","submitted_at":"2026-04-24T17:43:52+00:00","verdict":null,"verdict_confidence":null,"novelty_score":null,"formal_verification":null,"one_line_summary":null,"context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"Figueroa-O'Farrill, A. Pérez, and S. Prohazka, \"Carroll/fracton particles and their correspondence,\"JHEP06(5, 2023) 207,arXiv:2305.06730 [hep-th]. [19] A. Bagchi, A. Banerjee, P. Dhivakar, S. Mondal, and A. Shukla, \"The Carrollian Kaleidoscope,\"arXiv:2506.16164 [hep-th]. [20] K. Nguyen, \"Lectures on Carrollian Holography,\"arXiv:2511.10162 [hep-th]. [21] R. Ruzziconi, \"Carrollian physics and holography,\"Phys. Rept.1182(2026) 1-87, arXiv:2602.02644 [hep-th]. [22] X. Bekaert, Y. Herfray, L. Mele, and N. Parrini, \"A geometrical invitation to BMS group theory,\"arXiv:2602.12965 [hep-th]. [23] R. Haag,Local Quantum Physics. Theoretical and Mathematical Physics. Springer, Berlin, 1996. [24] H. Araki,Mathematical theory of quantum fields."},{"citing_arxiv_id":"2604.22582","ref_index":12,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Carrollian ABJM: Fermions and Supersymmetry","primary_cat":"hep-th","submitted_at":"2026-04-24T14:14:39+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"The c to zero limit of ABJM theory produces a Carrollian superconformal theory with extended BMS4 symmetry using Carrollian Dirac matrices.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"BMS/GCA Redux: Towards Flatspace Holography from Non-Relativistic Symmetries, JHEP 10(2012) 092 [1203.5795]. [9] A. Bagchi, R. Basu, A. Kakkar and A. Mehra, Flat Holography: Aspects of the dual field theory, JHEP12(2016) 147 [1609.06203]. [10] A. Bagchi, A. Banerjee, P. Dhivakar, S. Mondal and A. Shukla, The Carrollian Kaleidoscope, 2506.16164. [11] K. Nguyen, Lectures on Carrollian Holography,2511.10162. [12] R. Ruzziconi, Carrollian Physics and Holography,2602.02644. [13] A. Bagchi, P. Dhivakar and S. Dutta, AdS Witten diagrams to Carrollian correlators, JHEP 04(2023) 135 [2303.07388]. [14] A. Bagchi, P. Dhivakar and S. Dutta, Holography in Flat Spacetimes: the case for Carroll, 2311.11246. [15] L.F. Alday, M. Nocchi, R. Ruzziconi and A. Yelleshpur Srikant,"},{"citing_arxiv_id":"2604.13362","ref_index":79,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Quasi-Local Celestial Charges and Multipoles","primary_cat":"hep-th","submitted_at":"2026-04-14T23:59:01+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"Explicit quasi-local formulae for celestial higher-spin charges and multipoles are given on finite 2-surfaces using higher-valence twistor solutions, with a phase-space derivation from self-dual gravity.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"to define a clear notion of radiation, captured inQ−2, which obstructs the null-time conserva- tion of the charges. Identifying radiation at finite distance is usually not an easy task (see, e.g., [74-78] for recent discussions on timelike hypersurfaces), and the fact that the hypersurface is null considerably simplifies this analysis. Null hypersurfaces are known to carry a Carrollian geometry; see e.g. [79] for a review. In this work, celestial symmetries have been identified on arbitrary bulk null hypersurfaces. It would be interesting to further clarify the spacetime geometry associated with these symme- tries, and to understand how the universal Carrollian structure should be extended to properly accommodate them. We also refer to [80-84] for similar identifications of the celestial sym-"},{"citing_arxiv_id":"2604.11602","ref_index":17,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Celestial 1-form symmetries","primary_cat":"hep-th","submitted_at":"2026-04-13T15:11:07+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"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.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"charges as corner charges [14, 15] that survive the imposition of the gauge constraint in the bulk of the slice. Such charges associated with a given codimension-2 surface are therefore implicitly dependent on which codimension-1 slice they are connected to. The language of 1-form symmetries also provides a unifying link between the celestial [16] and Carrollian [17] approaches to flat space holography. Working in 4D flat space, the celestial approach reinterprets asymptotic symmetries as modes of conserved currents of a 2D CFT living on the celestial sphere. These modes are given by integrals over Bondi timeuand contour integrals on the celestial sphere, see e.g.[7, 18, 19] and references therein. On the other hand, the Carrollian approach"},{"citing_arxiv_id":"2604.09771","ref_index":11,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Towards a Carrollian Description of Yang-Mills","primary_cat":"hep-th","submitted_at":"2026-04-10T18:00:17+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"A Carrollian theory on null infinity reproduces all MHV and NMHV Yang-Mills tree amplitudes, with a new explicit NMHV expression.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"07388]. - 22 - [8] A. Bagchi, P. Dhivakar and S. Dutta,Holography in flat spacetimes: the case for Carroll, JHEP08(2024) 144 [2311.11246]. [9] L. F. Alday, M. Nocchi, R. Ruzziconi and A. Yelleshpur Srikant,Carrollian amplitudes from holographic correlators,JHEP03(2025) 158 [2406.19343]. [10] K. Nguyen,Lectures on Carrollian Holography,2511.10162. [11] R. Ruzziconi,Carrollian Physics and Holography,2602.02644. [12] G. Barnich and C. Troessaert,Supertranslations call for superrotations,PoSCNCFG2010 (2010) 010 [1102.4632]. [13] K. Nguyen,Carrollian conformal correlators and massless scattering amplitudes,JHEP01 (2024) 076 [2311.09869]. [14] L. Donnay, A. Puhm and A. Strominger,Conformally Soft Photons and Gravitons,JHEP01"},{"citing_arxiv_id":"2604.09275","ref_index":10,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Aspects of Non-Relativistic Supersymmetric Theories","primary_cat":"hep-th","submitted_at":"2026-04-10T12:43:12+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":2.0,"formal_verification":"none","one_line_summary":"Discusses features of non-relativistic supersymmetric field theories from Galilean and Carrollian points of view to aid construction of electric and magnetic variants.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2604.08498","ref_index":14,"ref_count":4,"confidence":0.9,"is_internal_anchor":false,"paper_title":"On Carrollian Loop Amplitudes for Gauge Theory and Gravity","primary_cat":"hep-th","submitted_at":"2026-04-09T17:42:28+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"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.","context_count":2,"top_context_role":"background","top_context_polarity":"background","context_text":"7 071602, [arXiv:2202.04702]. [11] L. Donnay, A. Fiorucci, Y. Herfray, and R. Ruzziconi,Bridging Carrollian and celestial holography,Phys. Rev. D107(2023), no. 12 126027, [arXiv:2212.12553]. [12] A. Bagchi, A. Banerjee, P. Dhivakar, S. Mondal, and A. Shukla,The Carrollian Kaleidoscope,arXiv:2506.16164. [13] K. Nguyen,Lectures on Carrollian Holography,arXiv:2511.10162. [14] R. Ruzziconi,Carrollian Physics and Holography,arXiv:2602.02644. [15] L. Mason, R. Ruzziconi, and A. Yelleshpur Srikant,Carrollian amplitudes and celestial symmetries,JHEP05(2024) 012, [arXiv:2312.10138]. [16] J. de Boer, J. Hartong, N. A. Obers, W. Sybesma, and S. Vandoren,Carroll stories,JHEP 09(2023) 148, [arXiv:2307.06827]. [17] J. de Boer, J."},{"citing_arxiv_id":"2603.28269","ref_index":30,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"A Twisted Origin for Magnetic Carroll Supersymmetry","primary_cat":"hep-th","submitted_at":"2026-03-30T10:53:00+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"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.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"12, (2023) 126027,arXiv:2212.12553 [hep-th]. [27] A. Saha, \"Carrollian approach to 1 + 3D flat holography,\"JHEP06(2023) 051,arXiv:2304.02696 [hep-th]. [28] K. Nguyen and P. West, \"Carrollian Conformal Fields and Flat Holography,\"Universe9no. 9, (2023) 385, arXiv:2305.02884 [hep-th]. [29] R. Ruzziconi, \"Carrollian Physics and Holography,\" arXiv:2602.02644 [hep-th]. [30] H. Bondi, M. G. J. van der Burg, and A. W. K. Metzner, \"Gravitational waves in general relativity. 7. Waves from axisymmetric isolated systems,\"Proc. Roy. Soc. Lond. A269(1962) 21-52. [31] R. Sachs, \"Asymptotic symmetries in gravitational theory,\"Phys. Rev.128(1962) 2851-2864. [32] P. J. McCarthy, \"Structure of the bondi-metzner-sachs group,\"Journal of Mathematical Physics13no."},{"citing_arxiv_id":"2603.17045","ref_index":38,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"The gravitational S-matrix from the path integral: asymptotic symmetries and soft theorems","primary_cat":"hep-th","submitted_at":"2026-03-17T18:28:46+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"A path integral with asymptotic boundary conditions produces the gravitational S-matrix and derives soft graviton theorems from extended BMS symmetry Ward identities.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null}],"limit":50,"offset":0}