{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2022:EUUL54X2IIU3EJNJH5VBUYCCIN","short_pith_number":"pith:EUUL54X2","schema_version":"1.0","canonical_sha256":"2528bef2fa4229b225a93f6a1a6042435afcbc09c25b5bdc7374ca576afbe7c8","source":{"kind":"arxiv","id":"2210.07165","version":2},"attestation_state":"computed","paper":{"title":"Radiated momentum and radiation-reaction in gravitational two-body scattering including time-asymmetric effects","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"Andrea Geralico, Donato Bini, Thibault Damour","submitted_at":"2022-10-13T16:42:27Z","abstract_excerpt":"We compute to high post-Newtonian accuracy the 4-momentum (linear momentum, and energy), radiated as gravitational waves in a two-body system undergoing gravitational scattering. We include, for the first time, all the relevant {\\it time-asymmetric} effects that arise when consistently going three post Newtonian orders beyond the leading post Newtonian order. We find that the inclusion of time-asymmetric radiative effects (both in tails and in the radiation-reacted hyperbolic motion) is crucial to ensure the mass-polynomiality of the post-Minkowskian expansion ($G$ expansion) of the radiated 4"},"verification_status":{"content_addressed":true,"pith_receipt":true,"author_attested":false,"weak_author_claims":0,"strong_author_claims":0,"externally_anchored":false,"storage_verified":false,"citation_signatures":0,"replication_records":0,"graph_snapshot":true,"references_resolved":false,"formal_links_present":false},"canonical_record":{"source":{"id":"2210.07165","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2022-10-13T16:42:27Z","cross_cats_sorted":[],"title_canon_sha256":"66a102c4a5ce239372a312f3e759d71b6544ac5e66bf1f1276a2b20b229d132a","abstract_canon_sha256":"735df013a416e1f7ece5bebb087960d8ffead871ed5535c53870ecdcb68e8a08"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T05:35:25.531807Z","signature_b64":"AFJKA4vR6qPM5T5pT1hqzCMfVMdsxcmgVWBvK/Ef82GYjt2fzDZmDDEYPOs0auybdlARkRaU1pzlPO7XqerUBA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"2528bef2fa4229b225a93f6a1a6042435afcbc09c25b5bdc7374ca576afbe7c8","last_reissued_at":"2026-07-05T05:35:25.531259Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T05:35:25.531259Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Radiated momentum and radiation-reaction in gravitational two-body scattering including time-asymmetric effects","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"Andrea Geralico, Donato Bini, Thibault Damour","submitted_at":"2022-10-13T16:42:27Z","abstract_excerpt":"We compute to high post-Newtonian accuracy the 4-momentum (linear momentum, and energy), radiated as gravitational waves in a two-body system undergoing gravitational scattering. We include, for the first time, all the relevant {\\it time-asymmetric} effects that arise when consistently going three post Newtonian orders beyond the leading post Newtonian order. We find that the inclusion of time-asymmetric radiative effects (both in tails and in the radiation-reacted hyperbolic motion) is crucial to ensure the mass-polynomiality of the post-Minkowskian expansion ($G$ expansion) of the radiated 4"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2210.07165","kind":"arxiv","version":2},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2210.07165/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"references":{"count":0,"sample":[],"resolved_work":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","internal_anchors":0},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"},"aliases":[{"alias_kind":"arxiv","alias_value":"2210.07165","created_at":"2026-07-05T05:35:25.531327+00:00"},{"alias_kind":"arxiv_version","alias_value":"2210.07165v2","created_at":"2026-07-05T05:35:25.531327+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2210.07165","created_at":"2026-07-05T05:35:25.531327+00:00"},{"alias_kind":"pith_short_12","alias_value":"EUUL54X2IIU3","created_at":"2026-07-05T05:35:25.531327+00:00"},{"alias_kind":"pith_short_16","alias_value":"EUUL54X2IIU3EJNJ","created_at":"2026-07-05T05:35:25.531327+00:00"},{"alias_kind":"pith_short_8","alias_value":"EUUL54X2","created_at":"2026-07-05T05:35:25.531327+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":9,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2606.23450","citing_title":"NLO Angular Impulse and Leading Singularities to all orders in spin for Kerr Black Holes","ref_index":164,"is_internal_anchor":false},{"citing_arxiv_id":"2411.11846","citing_title":"Emergence of Calabi-Yau manifolds in high-precision black hole scattering","ref_index":110,"is_internal_anchor":false},{"citing_arxiv_id":"2511.11457","citing_title":"Analytic structure of the high-energy gravitational amplitude: multi-H diagrams and classical 5PM logarithms","ref_index":80,"is_internal_anchor":false},{"citing_arxiv_id":"2510.07390","citing_title":"Heterotic Footprints in Classical Gravity: PM dynamics from On-Shell soft amplitudes at one loop","ref_index":75,"is_internal_anchor":false},{"citing_arxiv_id":"2605.12214","citing_title":"A Runway to Dissipation of Angular Momentum via Worldline Quantum Field Theory","ref_index":15,"is_internal_anchor":false},{"citing_arxiv_id":"2605.08798","citing_title":"Gravitational waveform from radial infall at the third-and-half Post-Newtonian order","ref_index":29,"is_internal_anchor":false},{"citing_arxiv_id":"2604.25916","citing_title":"Nonlocal-in-time tail effects in gravitational scattering to fifth Post-Minkowskian and tenth self-force orders","ref_index":54,"is_internal_anchor":false},{"citing_arxiv_id":"2604.09545","citing_title":"Black Hole Dynamics at Fifth Post-Newtonian Order","ref_index":86,"is_internal_anchor":false},{"citing_arxiv_id":"2503.12263","citing_title":"The Science of the Einstein Telescope","ref_index":239,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/EUUL54X2IIU3EJNJH5VBUYCCIN","json":"https://pith.science/pith/EUUL54X2IIU3EJNJH5VBUYCCIN.json","graph_json":"https://pith.science/api/pith-number/EUUL54X2IIU3EJNJH5VBUYCCIN/graph.json","events_json":"https://pith.science/api/pith-number/EUUL54X2IIU3EJNJH5VBUYCCIN/events.json","paper":"https://pith.science/paper/EUUL54X2"},"agent_actions":{"view_html":"https://pith.science/pith/EUUL54X2IIU3EJNJH5VBUYCCIN","download_json":"https://pith.science/pith/EUUL54X2IIU3EJNJH5VBUYCCIN.json","view_paper":"https://pith.science/paper/EUUL54X2","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2210.07165&json=true","fetch_graph":"https://pith.science/api/pith-number/EUUL54X2IIU3EJNJH5VBUYCCIN/graph.json","fetch_events":"https://pith.science/api/pith-number/EUUL54X2IIU3EJNJH5VBUYCCIN/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/EUUL54X2IIU3EJNJH5VBUYCCIN/action/timestamp_anchor","attest_storage":"https://pith.science/pith/EUUL54X2IIU3EJNJH5VBUYCCIN/action/storage_attestation","attest_author":"https://pith.science/pith/EUUL54X2IIU3EJNJH5VBUYCCIN/action/author_attestation","sign_citation":"https://pith.science/pith/EUUL54X2IIU3EJNJH5VBUYCCIN/action/citation_signature","submit_replication":"https://pith.science/pith/EUUL54X2IIU3EJNJH5VBUYCCIN/action/replication_record"}},"created_at":"2026-07-05T05:35:25.531327+00:00","updated_at":"2026-07-05T05:35:25.531327+00:00"}