{"total":11,"items":[{"citing_arxiv_id":"2605.12214","ref_index":51,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"A Runway to Dissipation of Angular Momentum via Worldline Quantum Field Theory","primary_cat":"hep-th","submitted_at":"2026-05-12T14:51:06+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"The authors introduce static correlators in worldline QFT to compute angular momentum dissipation in black hole scattering, reproducing the known O(G^3) flux and extending the approach to electromagnetism at O(α^3).","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"C. Nega, J. Plefka et al.,Emergence of Calabi-Yau manifolds in high-precision black-hole scattering, Nature641(2025) 603 [2411.11846]. [50] M. Driesse, G. U. Jakobsen, G. Mogull, J. Plefka, B. Sauer and J. 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Lett.131(2023) 151401 [2306."},{"citing_arxiv_id":"2604.25916","ref_index":85,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Nonlocal-in-time tail effects in gravitational scattering to fifth Post-Minkowskian and tenth self-force orders","primary_cat":"hep-th","submitted_at":"2026-04-28T17:59:10+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":8.0,"formal_verification":"none","one_line_summary":"Nonlocal-in-time conservative tail contributions to gravitational scattering are derived at 5PM and 10SF orders, expressed via polylogarithms up to weight three and agreeing with prior results through 6PN.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"A. Porto and M. M. Riva, (2026), arXiv:2604.09545 [gr-qc]. [83] G. Brunello, M. K. Mandal, P. Mastrolia, R. Patil, M. Pe- gorin, J. Ronca, S. Smith, J. Steinhoff, and W. J. Tor- res Bobadilla, (2025), arXiv:2512.19498 [hep-th]. [84] G. U. 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Ser.523, 012059 (2014),"},{"citing_arxiv_id":"2604.22009","ref_index":44,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Black Hole Response Theory and its Exact Shockwave Limit","primary_cat":"hep-th","submitted_at":"2026-04-23T18:55:30+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"Black hole response theory in WQFT exactly reproduces the Aichelburg-Sexl shockwave metric, geodesics, and the transfer matrix for gravitational-wave scattering off it via post-Minkowskian resummation.","context_count":1,"top_context_role":"method","top_context_polarity":"use_method","context_text":"spinning two-body dynamics,Phys. Rev. D107(2023) 044033 [2210.06451]. [42] G. U. Jakobsen, G. Mogull, J. Plefka and B. Sauer,All things retarded: radiation-reaction in worldline quantum field theory,JHEP10(2022) 128 [2207.00569]. [43] C. Shi and J. Plefka,Classical double copy of worldline quantum field theory,Phys. Rev. D105(2022) 026007 [2109.10345]. [44] F. Bastianelli, F. Comberiati and L. de la Cruz,Light bending from eikonal in worldline quantum field theory,JHEP02(2022) 209 [2112.05013]. 59 [45] F. Comberiati and C. Shi,Classical Double Copy of Spinning Worldline Quantum Field Theory,JHEP04(2023) 008 [2212.13855]. [46] T. Wang,Binary dynamics from worldline QFT for scalar QED,Phys. Rev. D107"},{"citing_arxiv_id":"2602.18790","ref_index":99,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Generalized Carter & R\\\"udiger Constants of $\\sqrt{\\text{Kerr}}$","primary_cat":"gr-qc","submitted_at":"2026-02-21T10:50:16+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"Generalized Carter and Rüdiger constants for spinning charged probes in √Kerr backgrounds exist only for Wilson coefficients matching spin-exponentiated effective Compton amplitudes up to second order in spin.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"Di Vecchia,Radiation reaction for spinning black-hole scattering,Phys. Lett. B832(2022) 137258 [2203.13272]. [97] N.E.J. Bjerrum-Bohr, G. Chen and M. Skowronek,Classical spin gravitational Compton scattering,JHEP06(2023) 170 [2302.00498]. [98] P.H. Damgaard, J. Hoogeveen, A. Luna and J. 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Xu,Conservative scattering of spinning black holes at fourth post-Minkowskian order,2306."},{"citing_arxiv_id":"2602.06947","ref_index":62,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"The gravitational Compton amplitude at third post-Minkowskian order","primary_cat":"hep-th","submitted_at":"2026-02-06T18:44:09+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"Gravitational Compton amplitude computed to third post-Minkowskian order via worldline EFT with infrared and forward divergences regulated to connect to black hole perturbation theory.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"arXiv:1911.09130 [hep-th]. 8 [59] G. U. Jakobsen, G. Mogull, J. Plefka, and B. Sauer, Phys. Rev. Lett.131, 241402 (2023), arXiv:2308.11514 [hep-th]. [60] G. Kälin and R. A. Porto, JHEP01, 072 (2020), arXiv:1910.03008 [hep-th]. [61] M. 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Rev. D82, 084010 (2010), arXiv:1006.4907 [gr-qc]. [93] R. A. Isaacson, Gravitational Radiation in the Limit of High Frequency. II. Nonlinear Terms and the Effective Stress Tensor, Phys. Rev.166, 1272 (1968). [94] S. E. Field, J. S. Hesthaven, and S. R. Lau, Discontinu- ous Galerkin method for computing gravitational wave- forms from extreme mass ratio binaries, Class. Quant. Grav.26, 165010 (2009), arXiv:0902.1287 [gr-qc]. [95] L. J. G. Da Silva, R. Panosso Macedo, J. E. Thompson, J. A. V. Kroon, L. Durkan, and O. Long, Hyperboloidal discontinuous time-symmetric numerical algorithm with"},{"citing_arxiv_id":"2510.07390","ref_index":128,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Heterotic Footprints in Classical Gravity: PM dynamics from On-Shell soft amplitudes at one loop","primary_cat":"hep-th","submitted_at":"2025-10-08T18:00:06+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"Derives conservative potential and scattering angle for charged black holes in EMD theory via one-loop soft amplitudes, showing IR finiteness after Lippmann-Schwinger treatment and smooth reduction to GR.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"K¨ alin, Z. Liu and R. A. Porto,Conservative Tidal Effects in Compact Binary Systems to Next-to-Leading Post-Minkowskian Order, Phys. Rev. D102(2020) 124025 [2008.06047]. [127] C. Dlapa, G. K¨ alin, Z. Liu and R. A. Porto,Local in Time Conservative Binary Dynamics at Fourth Post-Minkowskian Order, Phys. Rev. Lett.132(2024), no. 22, 221401 [2403.04853]. [128] C. Dlapa, G. K¨ alin, Z. Liu and R. A. Porto,Bootstrapping the relativistic two-body problem, JHEP08(2023) 109 [2304.01275]. [129] C. Dlapa, G. K¨ alin, Z. Liu and R. A. Porto,Local-in-Time Conservative Binary Dynamics at Fifth Post-Minkowskian and First Self-Force Orders,2506.20665. [130] G. Mogull, J. Plefka and J. Steinhoff,Classical black hole scattering from a worldline quantum"},{"citing_arxiv_id":"2509.04425","ref_index":76,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Hidden simplicity in the scattering for neutron stars and black holes","primary_cat":"hep-th","submitted_at":"2025-09-04T17:46:45+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"Authors define Kerr generating functions for all-loop scattering on Kerr black holes and apply them to compute leading non-linear tidal effects of neutron stars up to four loops in gravity.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2508.10761","ref_index":78,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Unexpected Symmetries of Kerr Black Hole Scattering","primary_cat":"hep-th","submitted_at":"2025-08-14T15:46:29+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"The work establishes conservation of several quantities in Kerr black hole scattering and presents evidence that a spinning probe satisfies asymptotic integrability to quartic spin order at all post-Minkowskian orders.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"turbation theory meets CFT2: Kerr-Compton ampli- tudes from Nekrasov-Shatashvili functions,\" Phys. Rev. D 109, 084071 (2024), arXiv:2312.05965 [hep-th]. [77] Lucile Cangemi, Marco Chiodaroli, Henrik Johans- son, Alexander Ochirov, Paolo Pichini, and Evgeny Skvortsov, \"From higher-spin gauge interactions to Compton amplitudes for root-Kerr,\" JHEP 09, 196 (2024), arXiv:2311.14668 [hep-th]. [78] Andreas Brandhuber, Graham R. Brown, Paolo Pichini, Gabriele Travaglini, and Pablo Vives Matasan, \"Spin- ning binary dynamics in cubic effective field theories of gravity,\" JHEP 08, 188 (2024), arXiv:2405.13826 [hep- th]. [79] Gang Chen and Tianheng Wang, \"Dynamics of spinning binary at 2PM,\" JHEP 12, 213 (2025), arXiv:2406.09086 [hep-th]. [80] Arpan Bhattacharyya, Debodirna Ghosh, Saptaswa"},{"citing_arxiv_id":"2503.12263","ref_index":233,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"The Science of the Einstein Telescope","primary_cat":"gr-qc","submitted_at":"2025-03-15T21:04:14+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":3.0,"formal_verification":"none","one_line_summary":"The paper provides state-of-the-art predictions for the Einstein Telescope's impact on fundamental physics, cosmology, compact-object astrophysics, and multi-messenger astronomy across its proposed configurations.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"Fortunately, many of these issues are naturally handled by importing ideas from particle physics-such as the effective field theory approach [213, 214, 241-244]-which provide a systematic framework to tackle the two-body problem in gravity [220, 240, 245-248]. Moving onto the case of scattering events, the state-of-the-art results in the PM ex- pansion [215, 230, 233], endowed with a resummation scheme [249, 250], have proven to be very successful in matching numerical simulations with exquisite level of precision [251-253], see figure 1.6. For the case of bound states, on the other hand, fundamental challenges arise connecting between observables for unbound/bound motion. The relevance of scatter- - 16 - 4.5 5."},{"citing_arxiv_id":"2411.11846","ref_index":43,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Emergence of Calabi-Yau manifolds in high-precision black hole scattering","primary_cat":"hep-th","submitted_at":"2024-11-18T18:59:58+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":8.0,"formal_verification":"none","one_line_summary":"At 5PM-1SF order, Calabi-Yau three-fold periods emerge in radiation-reacted observables for classical black hole scattering computed with worldline QFT and advanced IBP/DE methods.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null}],"limit":50,"offset":0}