{"total":14,"items":[{"citing_arxiv_id":"2606.28239","ref_index":37,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"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":"2606.27544","ref_index":26,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Gravitational wave scattering at $\\mathcal{O}(G^4)$: Murua construction and elliptics","primary_cat":"hep-th","submitted_at":"2026-06-25T20:47:33+00:00","verdict":"UNVERDICTED","verdict_confidence":"UNKNOWN","novelty_score":7.0,"formal_verification":"none","one_line_summary":"O(G^4) gravitational wave scattering amplitude computed in worldline QFT with Murua decomposition, matched to black hole perturbation theory to validate the formalism for Schwarzschild black holes.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.13599","ref_index":5,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Black Hole Thermodynamics Meets On-Shell Amplitudes: Local Detailed Balance and Thermal Spectrum from Spin Universality and Unitarity","primary_cat":"hep-th","submitted_at":"2026-06-11T17:18:18+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"An on-shell framework derives local detailed balance and the black hole thermal spectrum from spin universality and unitarity.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.11423","ref_index":68,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Weak-field waveforms for generic relativistic orbits","primary_cat":"hep-th","submitted_at":"2026-06-09T20:16:49+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Outlines a Schwinger-Keldysh path-integral framework that derives worldline equations of motion and computes weak-field gravitational waveforms independently for unspecified relativistic orbits.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.18544","ref_index":28,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"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":"2605.14958","ref_index":56,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Conservative and dissipative sectors in a nonlinear scalar model for the gravitational self-force problem","primary_cat":"gr-qc","submitted_at":"2026-05-14T15:26:44+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"Multiple Hamiltonian definitions of the conservative second-order self-force are identified in a nonlinear scalar toy model, restricted to unbound scattering trajectories.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.12214","ref_index":59,"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":"[57] S. Mougiakakos, M. M. Riva and F. Vernizzi, Gravitational Bremsstrahlung in the post-Minkowskian effective field theory,Phys. Rev. D104(2021) 024041 [2102.08339]. [58] C. 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."},{"citing_arxiv_id":"2604.25916","ref_index":71,"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":"Heissenberg, Phys. Rev. D111, 126012 (2025), arXiv:2501.02904 [hep-th]. [68] C. Heissenberg and R. Russo, (2025), arXiv:2511.13835 [hep-th]. [69] D. Bini and T. Damour, Phys. Rev. D112, 044002 (2025), arXiv:2504.20204 [hep-th]. [70] Z. 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D73, 104031 (2006), arXiv:gr-"},{"citing_arxiv_id":"2604.25270","ref_index":47,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Integrand Analysis, Leading Singularities and Canonical Bases beyond Polylogarithms","primary_cat":"hep-th","submitted_at":"2026-04-28T06:29:00+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"Feynman integrals selected for unit leading singularities in complex geometries satisfy epsilon-factorized differential equations with new transcendental functions corresponding to periods and differential forms in the Gauss-Manin connection.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"05154]. [44] F. Forner, C. Nega and L. Tancredi,On the photon self-energy to three loops in QED, 2411.19042. [45] C. Duhr, S. Maggio, F. Porkert, C. Semper and S.F. 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Plefka,Calabi-Yau periods for black hole scattering in"},{"citing_arxiv_id":"2604.22009","ref_index":83,"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":"Brandhuber, G. R. Brown, G. Chen, S. De Angelis, J. Gowdy and G. Travaglini, One-loop gravitational bremsstrahlung and waveforms from a heavy-mass effective field theory,JHEP06(2023) 048 [2303.06111]. [82] A. Brandhuber, G. R. Brown, G. Chen, J. Gowdy and G. Travaglini,Resummed spinning waveforms from five-point amplitudes,JHEP02(2024) 026 [2310.04405]. [83] S. De Angelis, P. P. Novichkov and R. Gonzo,Spinning waveforms from the Kosower-Maybee-O'Connell formalism at leading order,Phys. Rev. D110(2024) L041502 [2309.17429]. [84] A. Herderschee, R. Roiban and F. Teng,The sub-leading scattering waveform from amplitudes,JHEP06(2023) 004 [2303.06112]. [85] S. Caron-Huot, M. Giroux, H. S. Hannesdottir and S."},{"citing_arxiv_id":"2604.14134","ref_index":64,"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":"20665 [hep-th]. [62] Gregor K¨ alin and Rafael A. Porto, \"From Bound- ary Data to Bound States,\" JHEP01, 072 (2020), arXiv:1910.03008 [hep-th]. [63] Christoph Dlapa, Gregor K¨ alin, Zhengwen Liu, and Rafael A. Porto, \"Local in Time Conservative Binary Dynamics at Fourth Post-Minkowskian Order,\" Phys. Rev. Lett.132, 221401 (2024), arXiv:2403.04853 [hep- th]. [64] Zvi Bern, Enrico Herrmann, Radu Roiban, Michael S. Ruf, Alexander V. Smirnov, Sid Smith, and Mao Zeng, \"Scattering Amplitudes and Conservative Binary Dynamics atO(G 5) without Self-Force Truncation,\" (2025), arXiv:2512.23654 [hep-th]. [65] Mathias Driesse, Gustav Uhre Jakobsen, Gustav Mogull, Christoph Nega, Jan Plefka, Benjamin Sauer, and Johann Usovitsch, \"Conservative Black Hole Scat-"},{"citing_arxiv_id":"2604.09545","ref_index":39,"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":"order, while preserving locality in time throughout. As a side product, the PB prescription determines the universal value of the Effective One Body (EOB) coefficients ¯d5loc anda 6loc, in a manner that is consistent with the \"Tutti-Frutti\" framework [85], as well as the conjecture that allπ 2 contributions originate exclusively from the potential region to 5PN order [39]. We examine other possible ways of disentangling conservative and dissipative contribu- tions within the effective theory. For instance, we show that performing anoff-shellsplit of the Feynman action leads to an explicit cancellation among the nonlocal terms, thus allow- ing for a formulation that remains entirely local and consistent with a variational principle."},{"citing_arxiv_id":"2602.06947","ref_index":65,"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:2601.16256 [hep-th]. [62] Z. Bern, E. Herrmann, R. Roiban, M. S. Ruf, A. V. Smirnov, S. Smith, and M. Zeng, (2025), arXiv:2512.23654 [hep-th]. [63] A. Brandhuber, G. R. Brown, P. Pichini, G. Travaglini, and P. Vives Matasan, (2025), arXiv:2512.05017 [hep- th]. [64] J.-W. Kim, R. Patil, T. Scheopner, and J. Steinhoff, (2025), arXiv:2511.05649 [hep-th]. [65] A. Brandhuber, G. R. Brown, G. Chen, S. De Angelis, J. Gowdy, and G. Travaglini, JHEP06, 048 (2023), arXiv:2303.06111 [hep-th]. [66] A. Herderschee, R. Roiban, and F. Teng, JHEP06, 004 (2023), arXiv:2303.06112 [hep-th]. [67] A. Elkhidir, D. O'Connell, M. Sergola, and I. A. Vazquez-Holm, JHEP07, 272 (2024), arXiv:2303.06211 [hep-th]. [68] A. Georgoudis, C."},{"citing_arxiv_id":"2601.08252","ref_index":32,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Resumming Scattering Amplitudes for Waveforms","primary_cat":"hep-th","submitted_at":"2026-01-13T06:19:05+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"A new projector-based formalism determines effective potentials from perturbative amplitudes and resums them to compute non-perturbative gravitational waveforms for generic two-body trajectories.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null}],"limit":50,"offset":0}