{"total":13,"items":[{"citing_arxiv_id":"2606.28239","ref_index":18,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Gravitational Compton scattering at the fourth post-Minkowskian order","primary_cat":"hep-th","submitted_at":"2026-06-26T16:24:12+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"Derives gravitational Compton amplitude at O(G^4) and N-matrix element for scattering phase shift, verified by agreement with black-hole perturbation theory.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.23450","ref_index":20,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"NLO Angular Impulse and Leading Singularities to all orders in spin for Kerr Black Holes","primary_cat":"hep-th","submitted_at":"2026-06-22T15:02:49+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"NLO angular impulse for Kerr black holes computed to all orders in spin via KMOC formalism and leading singularities, with consistency checks and potential extraction.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"Porto,The effective field theorist's approach to gravitational dynamics,Phys. Rept. 633(2016) 1 [1601.04914]. [18] D. Neill and I.Z. Rothstein,Classical Space-Times from the S Matrix,Nucl. Phys. B877 (2013) 177 [1304.7263]. - 80 - [19] N.E.J. Bjerrum-Bohr, J.F. Donoghue and P. Vanhove,On-shell Techniques and Universal Results in Quantum Gravity,JHEP02(2014) 111 [1309.0804]. [20] N.E.J. Bjerrum-Bohr, B.R. Holstein, L. Plant' e and P. Vanhove,Graviton-Photon Scattering,Phys. Rev. D91(2015) 064008 [1410.4148]. [21] N.E.J. Bjerrum-Bohr, J.F. Donoghue, B.R. Holstein, L. Plant' e and P. Vanhove,Bending of Light in Quantum Gravity,Phys. Rev. Lett.114(2015) 061301 [1410.7590]. [22] M. Levi and J. Steinhoff,Complete conservative dynamics for inspiralling compact binaries"},{"citing_arxiv_id":"2606.05978","ref_index":38,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Lecture notes: Introduction to the Off-shell Double Copy Program","primary_cat":"hep-th","submitted_at":"2026-06-04T10:19:23+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":2.0,"formal_verification":"none","one_line_summary":"Lecture notes reviewing gauge and gravitational theories to present the off-shell single and double copy, including T-duality approaches.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.19948","ref_index":2,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Iterative Solution of the Kerr Black Hole Metric","primary_cat":"hep-th","submitted_at":"2026-05-19T15:04:24+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"A double perturbative expansion of the Kerr metric is obtained by recursively solving the Einstein equations in harmonic gauge to arbitrary order in G and a, with re-summation requiring redundant harmonic coordinate terms.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.18544","ref_index":11,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"The Classical Gravitational Impulse at High Energies","primary_cat":"hep-th","submitted_at":"2026-05-18T15:24:32+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"The gravitational impulse for ultrarelativistic massive scalars is resummed to all orders in G_N at fixed G_N s/mb, recovering post-Minkowski results and predicting the leading high-energy behavior to eleventh post-Minkowski order.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.12214","ref_index":60,"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":"Dlapa, G. K¨ alin, Z. Liu, J. Neef and R. A. Porto, Radiation Reaction and Gravitational Waves at Fourth Post-Minkowskian Order,Phys. Rev. Lett.130(2023) 101401 [2210.05541]. [59] C. Dlapa, G. K¨ alin, Z. Liu and R. A. Porto, Nonlocal-in-time tail effects in gravitational scattering to fifth Post-Minkowskian and tenth self-force orders, 2604.25916. [60] C. Dlapa, G. K¨ alin, Z. Liu and R. A. Porto, Local-in-Time Conservative Binary Dynamics at Fifth 16 Post-Minkowskian and First Self-Force Orders,Phys. Rev. Lett.135(2025) 251401 [2506.20665]. [61] Z. Bern, E. Herrmann, R. Roiban, M. S. Ruf, A. V. Smirnov, S. Smith et al.,Scattering Amplitudes and Conservative Binary Dynamics atO(G 5)without Self-Force Truncation,2512."},{"citing_arxiv_id":"2605.05067","ref_index":55,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Gravitational multipoles from scattering amplitudes in higher dimensions","primary_cat":"hep-th","submitted_at":"2026-05-06T16:02:24+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"In five dimensions, minimally coupled massive vector and antisymmetric tensor fields produce only mass or stress quadrupoles respectively from scattering amplitudes, failing to match the Myers-Perry black hole and demonstrating breakdown of spin universality.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"Ke,Effective interactions and on-shell recursion relation for massive spin 3/2,JHEP04(2025) 014 [2408.16065]. [53] J.F. Donoghue, B.R. Holstein, B. Garbrecht and T. Konstandin,Quantum corrections to the Reissner-Nordstr¨ om and Kerr-Newman metrics,Phys. Lett. B529(2002) 132 [hep-th/0112237]. [54] B.R. Holstein and J.F. Donoghue,Classical physics and quantum loops,Phys. Rev. Lett.93 (2004) 201602 [hep-th/0405239]. [55] N.E.J. Bjerrum-Bohr, P.H. Damgaard, G. Festuccia, L. Plant' e and P. Vanhove,General Relativity from Scattering Amplitudes,Phys. Rev. Lett.121(2018) 171601 [1806.04920]. [56] S. Mougiakakos and P. Vanhove,Schwarzschild-Tangherlini metric from scattering amplitudes in various dimensions,Phys. Rev. D103(2021) 026001 [2010.08882]. [57] S. D'Onofrio, F."},{"citing_arxiv_id":"2604.25916","ref_index":32,"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":"5PM order can be separated into local- and nonlocal-in- time contributions as follows [62] ˆH ell 5PM = ˆE0 + i=5X i=1 ˆci(loc) ˆri + i=5X i=1 ˆci(nloc) ˆri − i=5X i=4 G \u0012 ˆH dEsrc dt \u0013 (i−1)PM log \u0012 ˆr e2γE \u0013 , (10) with ˆH≡ H M ν ,ˆr= r GM , and ˆE0 ≡ 1 M ν P a p p2 +m 2a is the normalized kinetic term. The ˆc 1|2|3(loc) are the PM- exact coefficients throughO(G 3) computed in [32, 34, 39, 40], withγ= (E 1E2 +p 2)/m1m2. The coefficient ˆc4(loc) was obtained in [61] to all SF orders, while the 5PM coefficient ˆc 5(loc) was derived in [62] at the 1SF level. The factor multiplying log ˆr e2γE \u0001 in (10) can be shown to depend on lower order ˆci's com- bined with the source (\"1rad\"-only) energy flux. The relation follows from the general structure in (1), in-"},{"citing_arxiv_id":"2604.22009","ref_index":51,"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":"Mogull, J. Plefka, B. Sauer and Y. Xu,Conservative Scattering of Spinning Black Holes at Fourth Post-Minkowskian Order,Phys. Rev. Lett.131 (2023) 151401 [2306.01714]. [50] G. U. Jakobsen, G. Mogull, J. Plefka and B. Sauer,Dissipative Scattering of Spinning Black Holes at Fourth Post-Minkowskian Order,Phys. Rev. Lett.131 (2023) 241402 [2308.11514]. [51] G. U. Jakobsen, G. Mogull, J. Plefka and B. Sauer,Tidal effects and renormalization at fourth post-Minkowskian order,Phys. Rev. D109(2024) L041504 [2312.00719]. [52] D. Neill and I. Z. Rothstein,Classical Space-Times from the S Matrix,Nucl. Phys. B877(2013) 177 [1304.7263]. [53] A. Luna, I. Nicholson, D. O'Connell and C. D. White,Inelastic Black Hole"},{"citing_arxiv_id":"2604.14134","ref_index":47,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"All-order structure of static gravitational interactions and the seventh post-Newtonian potential","primary_cat":"hep-th","submitted_at":"2026-04-15T17:55:46+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"A closed formula computes static post-Newtonian corrections at arbitrary odd orders in gravity, yielding the explicit seventh post-Newtonian potential that matches an independent diagrammatic method.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"Ruf, Alexander V. Smirnov, Vladimir A. Smirnov, and Mao Zeng, \"Amplitudes, supersymmetric black hole scattering atO G5\u0001 , and loop integration,\" JHEP10, 023 (2024), arXiv:2406.01554 [hep-th]. [46] David A. Kosower, Ben Maybee, and Donal O'Connell, \"Amplitudes, Observables, and Classical Scattering,\" JHEP02, 137 (2019), arXiv:1811.10950 [hep-th]. [47] N. E. J. Bjerrum-Bohr, Poul H. Damgaard, Guido Fes- tuccia, Ludovic Plant' e, and Pierre Vanhove, \"Gen- eral Relativity from Scattering Amplitudes,\" Phys. Rev. Lett.121, 171601 (2018), arXiv:1806.04920 [hep-th]. [48] Andrea Cristofoli, N. E. J. Bjerrum-Bohr, Poul H. Damgaard, and Pierre Vanhove, \"Post-Minkowskian Hamiltonians in general relativity,\" Phys."},{"citing_arxiv_id":"2604.09545","ref_index":13,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Black Hole Dynamics at Fifth Post-Newtonian Order","primary_cat":"gr-qc","submitted_at":"2026-04-10T17:58:53+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"Derives 5PN scattering observables and a conservative Hamiltonian contribution for black holes that determines EOB parameters d5loc and a6loc.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"Blanchet,Gravitational Radiation from Post-Newtonian Sources and Inspiralling Compact Binaries,Living Rev. Rel.17(2014) 2 [1310.1528]. [11] I. Z. Rothstein,Progress in effective field theory approach to the binary inspiral problem,Gen. Rel. Grav.46(2014) 1726. [12] G. Sch¨ afer and P. Jaranowski,Hamiltonian formulation of general relativity and post-Newtonian dynamics of compact binaries,Living Rev. Rel.21(2018) 7 [1805.07240]. [13] R. A. Porto,The effective field theorist's approach to gravitational dynamics,Phys. Rept.633 (2016) 1 [1601.04914]. [14] W. D. Goldberger,Effective field theories of gravity and compact binary dynamics: A Snowmass 2021 whitepaper, inSnowmass 2021, 6, 2022,2206.14249. [15] D. Neill and I. Z. Rothstein,Classical Space-Times from the S Matrix,Nucl. Phys."},{"citing_arxiv_id":"2602.06947","ref_index":8,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"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":"method","top_context_polarity":"use_method","context_text":"J. Bjerrum-Bohr, P. H. Damgaard, G. Festuc- cia, L. Plante, and P. Vanhove, Phys. Rev. Lett.121, 171601 (2018), arXiv:1806.04920 [hep-th]. [6] C. Cheung, I. Z. Rothstein, and M. P. Solon, Phys. Rev. Lett.121, 251101 (2018), arXiv:1808.02489 [hep-th]. [7] D. A. Kosower, B. Maybee, and D. O'Connell, JHEP 02, 137 (2019), arXiv:1811.10950 [hep-th]. 7 [8] G. Kälin and R. A. Porto, (2020), arXiv:2006.01184 [hep-th]. [9] G. Mogull, J. Plefka, and J. Steinhoff, JHEP02, 048 (2021), arXiv:2010.02865 [hep-th]. [10] A. Cristofoli, N. E. J. Bjerrum-Bohr, P. H. Damgaard, and P. Vanhove, Phys. Rev. D100, 084040 (2019), arXiv:1906.01579 [hep-th]. [11] Z.Bern, C.Cheung, R.Roiban, C.-H.Shen, M.P.Solon, and M. Zeng, Phys."},{"citing_arxiv_id":"2510.07390","ref_index":83,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"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":"2, 024012 [2210.07165]. [81] T. Damour and P. Rettegno,Strong-field scattering of two black holes: Numerical relativity meets post-Minkowskian gravity, Phys. Rev. D107(2023), no. 6, 064051 [2211.01399]. [82] D. Bini and T. 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