{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2022:IR7BBCCH2F4VCH6Z525Z53KYLO","short_pith_number":"pith:IR7BBCCH","schema_version":"1.0","canonical_sha256":"447e108847d179511fd9eebb9eed585bb232291628731e4c76db57136469a496","source":{"kind":"arxiv","id":"2208.03170","version":2},"attestation_state":"computed","paper":{"title":"Scattering of gravitational waves off spinning compact objects with an effective worldline theory","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-th"],"primary_cat":"gr-qc","authors_text":"Justin Vines, M. V. S. Saketh","submitted_at":"2022-08-05T13:56:28Z","abstract_excerpt":"We study the process, within classical general relativity, in which an incident gravitational plane wave, of weak amplitude and long wavelength, scatters off a massive spinning compact object, such as a black hole or neutron star. The amplitude of the asymptotic scattered wave, considered here at linear order in Newton's constant $G$ while at higher orders in the object's multipole expansion, is a valuable characterization of the response of the object to external gravitational fields. This amplitude coincides with a classical ($\\hbar\\to0$) limit of a quantum 4-point (object and graviton in, o"},"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":"2208.03170","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2022-08-05T13:56:28Z","cross_cats_sorted":["hep-th"],"title_canon_sha256":"f803c7ad80fe15546deb971d578dc832d3f8e5f5d8902419721188cbc5763bb7","abstract_canon_sha256":"5febb51c87d272e777f7dbd9065982995df96ed88c75b9423c3976dec9acb80b"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T05:30:10.956532Z","signature_b64":"xkSUjDE4hM0Kn16Uf1ssBZha42e3XouFMhmvY2muuABy+TtvyVVt+x1Yqml9HcOQLTmG8sQDB1izoAL1Yr20DA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"447e108847d179511fd9eebb9eed585bb232291628731e4c76db57136469a496","last_reissued_at":"2026-07-05T05:30:10.956088Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T05:30:10.956088Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Scattering of gravitational waves off spinning compact objects with an effective worldline theory","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-th"],"primary_cat":"gr-qc","authors_text":"Justin Vines, M. V. S. Saketh","submitted_at":"2022-08-05T13:56:28Z","abstract_excerpt":"We study the process, within classical general relativity, in which an incident gravitational plane wave, of weak amplitude and long wavelength, scatters off a massive spinning compact object, such as a black hole or neutron star. The amplitude of the asymptotic scattered wave, considered here at linear order in Newton's constant $G$ while at higher orders in the object's multipole expansion, is a valuable characterization of the response of the object to external gravitational fields. This amplitude coincides with a classical ($\\hbar\\to0$) limit of a quantum 4-point (object and graviton in, o"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2208.03170","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/2208.03170/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":"2208.03170","created_at":"2026-07-05T05:30:10.956146+00:00"},{"alias_kind":"arxiv_version","alias_value":"2208.03170v2","created_at":"2026-07-05T05:30:10.956146+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2208.03170","created_at":"2026-07-05T05:30:10.956146+00:00"},{"alias_kind":"pith_short_12","alias_value":"IR7BBCCH2F4V","created_at":"2026-07-05T05:30:10.956146+00:00"},{"alias_kind":"pith_short_16","alias_value":"IR7BBCCH2F4VCH6Z","created_at":"2026-07-05T05:30:10.956146+00:00"},{"alias_kind":"pith_short_8","alias_value":"IR7BBCCH","created_at":"2026-07-05T05:30:10.956146+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2507.18605","citing_title":"Graviton scattering on self-dual black holes","ref_index":34,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/IR7BBCCH2F4VCH6Z525Z53KYLO","json":"https://pith.science/pith/IR7BBCCH2F4VCH6Z525Z53KYLO.json","graph_json":"https://pith.science/api/pith-number/IR7BBCCH2F4VCH6Z525Z53KYLO/graph.json","events_json":"https://pith.science/api/pith-number/IR7BBCCH2F4VCH6Z525Z53KYLO/events.json","paper":"https://pith.science/paper/IR7BBCCH"},"agent_actions":{"view_html":"https://pith.science/pith/IR7BBCCH2F4VCH6Z525Z53KYLO","download_json":"https://pith.science/pith/IR7BBCCH2F4VCH6Z525Z53KYLO.json","view_paper":"https://pith.science/paper/IR7BBCCH","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2208.03170&json=true","fetch_graph":"https://pith.science/api/pith-number/IR7BBCCH2F4VCH6Z525Z53KYLO/graph.json","fetch_events":"https://pith.science/api/pith-number/IR7BBCCH2F4VCH6Z525Z53KYLO/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/IR7BBCCH2F4VCH6Z525Z53KYLO/action/timestamp_anchor","attest_storage":"https://pith.science/pith/IR7BBCCH2F4VCH6Z525Z53KYLO/action/storage_attestation","attest_author":"https://pith.science/pith/IR7BBCCH2F4VCH6Z525Z53KYLO/action/author_attestation","sign_citation":"https://pith.science/pith/IR7BBCCH2F4VCH6Z525Z53KYLO/action/citation_signature","submit_replication":"https://pith.science/pith/IR7BBCCH2F4VCH6Z525Z53KYLO/action/replication_record"}},"created_at":"2026-07-05T05:30:10.956146+00:00","updated_at":"2026-07-05T05:30:10.956146+00:00"}