{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2015:SDKES5EWN5IF7HHJZWT4ZX43FI","short_pith_number":"pith:SDKES5EW","schema_version":"1.0","canonical_sha256":"90d44974966f505f9ce9cda7ccdf9b2a392219fb9f3433bd54da8af3795154fd","source":{"kind":"arxiv","id":"1505.07841","version":3},"attestation_state":"computed","paper":{"title":"Applying the effective-source approach to frequency-domain self-force calculations: Lorenz-gauge gravitational perturbations","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"gr-qc","authors_text":"Barry Wardell, Niels Warburton","submitted_at":"2015-05-28T20:02:14Z","abstract_excerpt":"With a view to developing a formalism that will be applicable at second perturbative order, we devise a new practical scheme for computing the gravitational self-force experienced by a point mass moving in a curved background spacetime. Our method works in the frequency domain and employs the effective-source approach, in which a distributional source for the retarded metric perturbation is replaced with an effective source for a certain regularized self-field. A key ingredient of the calculation is the analytic determination of an appropriate puncture field from which the effective source and"},"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":"1505.07841","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2015-05-28T20:02:14Z","cross_cats_sorted":["astro-ph.HE"],"title_canon_sha256":"1c64a0c4de90446f33c9b8fbb6727d48909eb7539563a751cd37e86117a06040","abstract_canon_sha256":"4ae2e3b6bec896ecd98002e8cee30ba8632ac90bccd8c99821ec119356b6bc3c"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T02:48:15.476183Z","signature_b64":"5RGhBtSqfMuKUHglQZSTdmDw74F1oJTH45r7W1bKoLJqSZn07Bwt2sJ5E3zBv+tcIXUngLbbf2HrfHp8tIucBg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"90d44974966f505f9ce9cda7ccdf9b2a392219fb9f3433bd54da8af3795154fd","last_reissued_at":"2026-07-05T02:48:15.475707Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T02:48:15.475707Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Applying the effective-source approach to frequency-domain self-force calculations: Lorenz-gauge gravitational perturbations","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"gr-qc","authors_text":"Barry Wardell, Niels Warburton","submitted_at":"2015-05-28T20:02:14Z","abstract_excerpt":"With a view to developing a formalism that will be applicable at second perturbative order, we devise a new practical scheme for computing the gravitational self-force experienced by a point mass moving in a curved background spacetime. Our method works in the frequency domain and employs the effective-source approach, in which a distributional source for the retarded metric perturbation is replaced with an effective source for a certain regularized self-field. A key ingredient of the calculation is the analytic determination of an appropriate puncture field from which the effective source and"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1505.07841","kind":"arxiv","version":3},"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/1505.07841/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":"1505.07841","created_at":"2026-07-05T02:48:15.475768+00:00"},{"alias_kind":"arxiv_version","alias_value":"1505.07841v3","created_at":"2026-07-05T02:48:15.475768+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1505.07841","created_at":"2026-07-05T02:48:15.475768+00:00"},{"alias_kind":"pith_short_12","alias_value":"SDKES5EWN5IF","created_at":"2026-07-05T02:48:15.475768+00:00"},{"alias_kind":"pith_short_16","alias_value":"SDKES5EWN5IF7HHJ","created_at":"2026-07-05T02:48:15.475768+00:00"},{"alias_kind":"pith_short_8","alias_value":"SDKES5EW","created_at":"2026-07-05T02:48:15.475768+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2510.16113","citing_title":"Post-adiabatic self-force waveforms: slowly spinning primary and precessing secondary","ref_index":125,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/SDKES5EWN5IF7HHJZWT4ZX43FI","json":"https://pith.science/pith/SDKES5EWN5IF7HHJZWT4ZX43FI.json","graph_json":"https://pith.science/api/pith-number/SDKES5EWN5IF7HHJZWT4ZX43FI/graph.json","events_json":"https://pith.science/api/pith-number/SDKES5EWN5IF7HHJZWT4ZX43FI/events.json","paper":"https://pith.science/paper/SDKES5EW"},"agent_actions":{"view_html":"https://pith.science/pith/SDKES5EWN5IF7HHJZWT4ZX43FI","download_json":"https://pith.science/pith/SDKES5EWN5IF7HHJZWT4ZX43FI.json","view_paper":"https://pith.science/paper/SDKES5EW","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1505.07841&json=true","fetch_graph":"https://pith.science/api/pith-number/SDKES5EWN5IF7HHJZWT4ZX43FI/graph.json","fetch_events":"https://pith.science/api/pith-number/SDKES5EWN5IF7HHJZWT4ZX43FI/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/SDKES5EWN5IF7HHJZWT4ZX43FI/action/timestamp_anchor","attest_storage":"https://pith.science/pith/SDKES5EWN5IF7HHJZWT4ZX43FI/action/storage_attestation","attest_author":"https://pith.science/pith/SDKES5EWN5IF7HHJZWT4ZX43FI/action/author_attestation","sign_citation":"https://pith.science/pith/SDKES5EWN5IF7HHJZWT4ZX43FI/action/citation_signature","submit_replication":"https://pith.science/pith/SDKES5EWN5IF7HHJZWT4ZX43FI/action/replication_record"}},"created_at":"2026-07-05T02:48:15.475768+00:00","updated_at":"2026-07-05T02:48:15.475768+00:00"}