{"total":22,"items":[{"citing_arxiv_id":"2605.22037","ref_index":19,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Classical Renormalization Group Equations for General Relativity","primary_cat":"gr-qc","submitted_at":"2026-05-21T06:20:50+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"A Legendre transform establishes an exact duality between the classical Polchinski equation and the authors' classical RG equation for the gravitational effective action.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.18544","ref_index":27,"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":"2605.12214","ref_index":47,"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":"de la Cruz,Classical off-shell currents,JHEP03(2023) 068 [2212.09259]. [45] N. E. J. Bjerrum-Bohr, G. Chen, C. J. Eriksen and N. Shah,The gravitational Compton amplitude from flat and curved spacetimes at second post-Minkowskian order,JHEP10(2025) 235 [2506.19705]. [46] V. F. He and J. Parra-Martinez,Generalized Unitarity Method for Worldline Field Theory,2510.00989. [47] L. Bohnenblust, H. Ita, M. Kraus and J. Schlenk, Gravitational Bremsstrahlung in black-hole scattering atO G3\u0001 : linear-in-spin effects,JHEP11(2024) 109 [2312.14859]. [48] L. Bohnenblust, H. Ita, M. Kraus and J. Schlenk, Gravitational bremsstrahlung in black-hole scattering at O G3\u0001 : quadratic-in-spin effects,JHEP12(2025) 100 [2505.15724]. [49] M."},{"citing_arxiv_id":"2604.25916","ref_index":67,"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":"Rev. D110, 064005 (2024), arXiv:2406.04878 [gr-qc]. [65] M. Driesse, G. U. Jakobsen, G. Mogull, J. Plefka, B. Sauer, and J. Usovitsch, Phys. Rev. Lett.132, 241402 (2024), arXiv:2403.07781 [hep-th]. [66] M. Driesse, G. U. Jakobsen, A. Klemm, G. Mogull, C. Nega, J. Plefka, B. Sauer, and J. Usovitsch, Nature 641, 603 (2025), arXiv:2411.11846 [hep-th]. [67] C. 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. Bern, E. Herrmann, R. Roiban, M. S. Ruf, A. V. Smirnov, S. Smith, and M. Zeng, (2025), arXiv:2512.23654 [hep-th]."},{"citing_arxiv_id":"2604.25270","ref_index":49,"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":"Maggio,Three-loop banana integrals with three equal masses,2511.19245. [47] S. Pögel, T. Teschke, X. Wang and S. Weinzierl,The unequal-mass three-loop banana integral,JHEP01(2026) 021 [2507.23594]. [48] Z. Bern, E. Herrmann, R. Roiban, M.S. Ruf, A.V. Smirnov, S. Smith et al.,Scattering Amplitudes and Conservative Binary Dynamics atO(G5)without Self-Force Truncation, 2512.23654. [49] A. Klemm, C. Nega, B. Sauer and J. Plefka,Calabi-Yau periods for black hole scattering in classical general relativity,Phys. Rev. D109(2024) 124046 [2401.07899]. - 46 - [50] M. Driesse, G.U. Jakobsen, A. Klemm, G. Mogull, C. Nega, J. Plefka et al.,High-precision black hole scattering with Calabi-Yau manifolds,2411.11846. [51] M. Driesse, G.U. Jakobsen, G."},{"citing_arxiv_id":"2604.22009","ref_index":87,"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":"background","top_context_polarity":"background","context_text":"amplitudes,JHEP06(2023) 004 [2303.06112]. [85] S. Caron-Huot, M. Giroux, H. S. Hannesdottir and S. Mizera,What can be measured asymptotically?,JHEP01(2024) 139 [2308.02125]. [86] F. Febres Cordero, M. Kraus, G. Lin, M. S. Ruf and M. 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[89] Z."},{"citing_arxiv_id":"2604.14134","ref_index":59,"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":"vitsch, \"Conservative Black Hole Scattering at Fifth Post-Minkowskian and First Self-Force Order,\" Phys. Rev. Lett.132, 241402 (2024), arXiv:2403.07781 [hep- th]. [58] Gregor K¨ alin, Jakob Neef, and Rafael A. Porto, \"Radiation-reaction in the Effective Field Theory ap- proach to Post-Minkowskian dynamics,\" JHEP01, 140 (2023), arXiv:2207.00580 [hep-th]. [59] Mathias Driesse, Gustav Uhre Jakobsen, Albrecht Klemm, Gustav Mogull, Christoph Nega, Jan Plefka, Benjamin Sauer, and Johann Usovitsch, \"Emergence of Calabi-Yau manifolds in high-precision black-hole scat- tering,\" Nature641, 603-607 (2025), arXiv:2411.11846 [hep-th]. [60] Zvi Bern, Enrico Herrmann, Radu Roiban, Michael S. Ruf, Alexander V. Smirnov, Vladimir A."},{"citing_arxiv_id":"2604.09545","ref_index":32,"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":"method","top_context_polarity":"use_method","context_text":"The identification of scattering observables with (gauge-dependent) dynamical quantities is often achieved by working in an isotropic-like coordinate system, in which for instance a Hamiltonian can be arranged to depend only onrandp 2 [44, 45]. This construction admits a natural extension to the dissipative sector, where matching computations to either an energy flux [46] or an effective force [32] provide the appropriate bridge between observables and dynamical variables. In what follows, we build on these ideas to construct isotropic-like representations for the various nonlinear gravitational radiation-reaction effects identified in this work. For reasons that will become clear momentarily we decompose the force in isotropic-like coordinates as follows:"},{"citing_arxiv_id":"2604.09129","ref_index":24,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Picard-Fuchs Equations of Twisted Differential forms associated to Feynman Integrals","primary_cat":"math.AG","submitted_at":"2026-04-10T09:11:16+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"An extension of the Griffiths-Dwork algorithm produces twisted Picard-Fuchs operators for hypergeometric, elliptic, and Calabi-Yau motives from families of Feynman integrals.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"Weinzierl, \"Feynman integrals, geometries and differential equa- tions,\" PoSRADCOR2023(2024), 007 [arXiv:2309.07531 [hep-th]]. TWISTED PICARD-FUCHS EQUATIONS 19 [23] A. Klemm, C. Nega, B. Sauer and J. Plefka, \"Calabi-Yau periods for black hole scattering in classical general relativity,\" Phys. Rev. D109(2024) no.12, 124046 [arXiv:2401.07899 [hep-th]]. [24] M. Driesse, G. U. Jakobsen, A. Klemm, G. Mogull, C. Nega, J. Plefka, B. Sauer and J. Uso- vitsch, \"Emergence of Calabi-Yau manifolds in high-precision black-hole scattering,\" Nature 641(2025) no.8063, 603-607 [arXiv:2411.11846 [hep-th]]. [25] H. Frellesvig, R. Morales, S. P¨ ogel, S. Weinzierl and M. Wilhelm, \"Calabi-Yau Feynman integrals in gravity:ε-factorized form for apparent singularities,\" JHEP02(2025), 209"},{"citing_arxiv_id":"2602.06947","ref_index":52,"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":"Here, observables are naturally expressed in a partial-wave expansion that encodes strong-field dynam- ics and finite size effects. Establishing a direct connection between plane-wave amplitudes from post-Minkowskian perturbation theory and partial-wave amplitudes from black hole perturbation theory is therefore essential for extracting and classifying the finite-size effects [52, 97, 100, 102, 115-117] and modeling them within the ef- fective actions to enable first-principles predictions of gravitational-wave observables. A direct comparison be- tween these two representations-requiring a projection integral from plane-wave to partial-wave amplitudes- has not been achieved beyond tree level [89, 118]. A key obstacle is increasingly complex singular integrals"},{"citing_arxiv_id":"2601.22697","ref_index":11,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"A complex-linear reformulation of Hamilton-Jacobi theory and emergent quantum structure","primary_cat":"quant-ph","submitted_at":"2026-01-30T08:14:55+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Embedding classical Hamilton-Jacobi amplitude and phase into a complex field yields a linear equation from which quantum mechanics emerges structurally when the real part of a scaling parameter is nonzero.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2601.08252","ref_index":28,"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},{"citing_arxiv_id":"2512.13794","ref_index":67,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"The spectrum of Feynman-integral geometries at two loops","primary_cat":"hep-th","submitted_at":"2025-12-15T19:00:02+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":8.0,"formal_verification":"none","one_line_summary":"Two-loop Feynman integrals involve Riemann spheres, elliptic curves, hyperelliptic curves of genus 2 and 3, K3 surfaces, and a rationalizable Del Pezzo surface of degree 2.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"Dlapa, J.M. Henn and F.J. Wagner,An algorithmic approach to finding canonical differential equations for elliptic Feynman integrals,JHEP08(2023) 120 [2211.16357]. [66] G.U. Jakobsen, G. 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]. [67] M. Driesse, G.U. Jakobsen, G. Mogull, J. Plefka, B. Sauer and J. Usovitsch, Conservative Black Hole Scattering at Fifth Post-Minkowskian and First Self-Force Order,Phys. Rev. Lett.132(2024) 241402 [2403.07781]. [68] M. Driesse, G.U. Jakobsen, A. Klemm, G. Mogull, C. Nega, J. Plefka, B. Sauer and J. Usovitsch,Emergence of Calabi-Yau manifolds in high-precision black-hole"},{"citing_arxiv_id":"2512.10518","ref_index":16,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Fano and Reflexive Polytopes from Feynman Integrals","primary_cat":"hep-th","submitted_at":"2025-12-11T10:41:45+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"Quasi-finite Feynman integrals produce sparse Fano and reflexive polytopes that encode degenerate Calabi-Yau varieties and link to del Pezzo surfaces, K3 surfaces, and Calabi-Yau threefolds.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2512.02274","ref_index":38,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Gravitational radiation from hyperbolic orbits: comparison between self-force, post-Minkowskian, post-Newtonian, and numerical relativity results","primary_cat":"gr-qc","submitted_at":"2025-12-01T23:40:30+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Self-force calculations of radiated gravitational wave energy from hyperbolic orbits around Schwarzschild black holes agree with post-Minkowskian results for large impact parameters and velocities up to 0.7c, with further comparisons to post-Newtonian and numerical relativity.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"the mass ratio at 3PM [32] and 4PM [33, 34] order, and the 5PM results are at known leading-order in the mass ratio [28]. The radiation absorbed by the black holes during the scattering event is known at leading order [35, 36]. There is also a range of results made using a double PM-PN expansion [31, 37] and results that also include a third SF expansion [38, 39]. Approaches that map these analytic for scattered binaries results to the bound case include the 'boundary-to-bound' (B2B) map [40-43] and calibration of EOB models [44, 45]. There have been a variety of studies of scattered bina- ries in NR, often with a focus on comparing the scatter- ing angle with PM results [46-51]. This includes testing"},{"citing_arxiv_id":"2511.15240","ref_index":12,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"A construction of single-valued elliptic polylogarithms","primary_cat":"hep-th","submitted_at":"2025-11-19T08:49:12+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"A construction of single-valued elliptic polylogarithms on the punctured elliptic curve is given that reduces to Brown's genus-zero condition upon torus degeneration.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2511.11457","ref_index":33,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Analytic structure of the high-energy gravitational amplitude: multi-H diagrams and classical 5PM logarithms","primary_cat":"hep-th","submitted_at":"2025-11-14T16:28:10+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"Computes the leading double logarithm at 5PM in the high-energy gravitational amplitude via multi-H diagrams and dispersion relations, extracting the single-log imaginary part of the eikonal phase.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2510.07390","ref_index":131,"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":"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 field theory, JHEP02(2021) 048 [2010.02865]. [131] G. U. Jakobsen, G. Mogull, J. Plefka and J. Steinhoff,Gravitational Bremsstrahlung and Hidden Supersymmetry of Spinning Bodies, Phys. Rev. Lett.128(2022), no. 1, 011101 [2106.10256]. [132] G. U. Jakobsen, G. Mogull, J. Plefka, B. Sauer and Y. Xu,Conservative Scattering of Spinning Black Holes at Fourth Post-Minkowskian Order, Phys. Rev. Lett.131(2023), no."},{"citing_arxiv_id":"2509.04425","ref_index":43,"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":33,"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":"in post-Minkowskian gravity, to all orders in spin, and effective-one-body mappings,\" Class. Quant. Grav. 35, 084002 (2018), arXiv:1709.06016 [gr-qc]. [32] Justin Vines, Jan Steinhoff, and Alessandra Buonanno, \"Spinning-black-hole scattering and the test-black-hole limit at second post-Minkowskian order,\" Phys. Rev. D 99, 064054 (2019), arXiv:1812.00956 [gr-qc]. [33] Alfredo Guevara, \"Holomorphic Classical Limit for Spin Effects in Gravitational and Electromagnetic Scatter- ing,\" JHEP 04, 033 (2019), arXiv:1706.02314 [hep-th]. [34] Alfredo Guevara, Alexander Ochirov, and Justin Vines, \"Scattering of Spinning Black Holes from Ex- ponentiated Soft Factors,\" JHEP 09, 056 (2019), arXiv:1812.06895 [hep-th]. [35] Ming-Zhi Chung, Yu-Tin Huang, Jung-Wook Kim, and"},{"citing_arxiv_id":"2508.02800","ref_index":97,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Towards Motivic Coactions at Genus One from Zeta Generators","primary_cat":"hep-th","submitted_at":"2025-08-04T18:11:26+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"Proposes motivic coaction formulae for genus-one iterated integrals over holomorphic Eisenstein series using zeta generators, verifies expected coaction properties, and deduces f-alphabet decompositions of multiple modular values.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"12 124046, [ 2401.07899]. [95] H. Frellesvig, R. Morales, and M. Wilhelm, Classifying post-Minkowskian geometries for gravitational waves via loop-by-loop Baikov , JHEP 08 (2024) 243, [ 2405.17255]. [96] C. Duhr, F. Gasparotto, C. Nega, L. 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Tancredi, On the photon self-energy to three loops in QED , JHEP 03 (2025) 148, [ 2411.19042]."},{"citing_arxiv_id":"2503.12263","ref_index":236,"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":"dynamics in GR was only possible after the interplay between near- and far-zone fields was clarified [217-220], allowing for a systematic resolution of the IR/UV divergences which (separately) plagued the potential and radiation regions [221]. Furthermore, recent devel- opments in the study of scattering processes using techniques inspired by collider physics, e.g. [222-236], have also opened new venues towards simultaneously tackling near- and far- zone dynamics, while at the same time incorporating an infinite tower of velocity corrections at each order in Newton's constant. To quote an example, the study of hereditary and radiation-reaction terms [227-230, 237-239] were instrumental in the determination of the imprint of nonlinear gravitational effects in the dynamics at 5PN order [240], as well as in"}],"limit":50,"offset":0}