{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2020:5YH32C52EM5WZAHEMFUXCUVJ7Z","short_pith_number":"pith:5YH32C52","schema_version":"1.0","canonical_sha256":"ee0fbd0bba233b6c80e461697152a9fe620c20f04bc67e10fdc072f28e30225e","source":{"kind":"arxiv","id":"2012.10184","version":2},"attestation_state":"computed","paper":{"title":"Compact body in a tidal environment: New types of relativistic Love numbers, and a post-Newtonian operational definition for tidally induced multipole moments","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"Eric Poisson","submitted_at":"2020-12-18T12:07:08Z","abstract_excerpt":"We examine the tidal deformation of a nonrotating compact body (material body or black hole) in general relativity. The body's exterior metric is calculated in a simultaneous expansion in powers of the ratio between the distance to the body and three distinct length scales: the radius of curvature of the external spacetime in which the body is inserted, the scale of spatial inhomogeneity of the curvature, and the scale of temporal variation. The metric is valid in the body's immediate neighborhood, which excludes the external matter responsible for the tidal environment. The body's tidal respo"},"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":"2012.10184","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2020-12-18T12:07:08Z","cross_cats_sorted":[],"title_canon_sha256":"10f2f3038b11a01b355a3d03ae5c2631f12926eadbbf69e7a0510d6f8d5a3d93","abstract_canon_sha256":"99681f0b57f5d41ff1983ab9bc9a4c65a99d7a01d2ba94669f4ad62dcdd4ca77"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T02:25:32.312936Z","signature_b64":"Yic5bNG5MWBD+1T4i9BEmCjFNdugA4YoavNmwJ4fIKYQo+b+TVr6PiyYyJuT8TljgFPwUfhOD+hCJTOOtvObDA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"ee0fbd0bba233b6c80e461697152a9fe620c20f04bc67e10fdc072f28e30225e","last_reissued_at":"2026-07-05T02:25:32.312457Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T02:25:32.312457Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Compact body in a tidal environment: New types of relativistic Love numbers, and a post-Newtonian operational definition for tidally induced multipole moments","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"Eric Poisson","submitted_at":"2020-12-18T12:07:08Z","abstract_excerpt":"We examine the tidal deformation of a nonrotating compact body (material body or black hole) in general relativity. The body's exterior metric is calculated in a simultaneous expansion in powers of the ratio between the distance to the body and three distinct length scales: the radius of curvature of the external spacetime in which the body is inserted, the scale of spatial inhomogeneity of the curvature, and the scale of temporal variation. The metric is valid in the body's immediate neighborhood, which excludes the external matter responsible for the tidal environment. The body's tidal respo"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2012.10184","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/2012.10184/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":"2012.10184","created_at":"2026-07-05T02:25:32.312514+00:00"},{"alias_kind":"arxiv_version","alias_value":"2012.10184v2","created_at":"2026-07-05T02:25:32.312514+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2012.10184","created_at":"2026-07-05T02:25:32.312514+00:00"},{"alias_kind":"pith_short_12","alias_value":"5YH32C52EM5W","created_at":"2026-07-05T02:25:32.312514+00:00"},{"alias_kind":"pith_short_16","alias_value":"5YH32C52EM5WZAHE","created_at":"2026-07-05T02:25:32.312514+00:00"},{"alias_kind":"pith_short_8","alias_value":"5YH32C52","created_at":"2026-07-05T02:25:32.312514+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":9,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2606.19446","citing_title":"Dynamical Tidal Response of Neutron Stars: from Effective Field Theory to Gravitational Waveforms","ref_index":56,"is_internal_anchor":false},{"citing_arxiv_id":"2504.07862","citing_title":"Resummation of Universal Tails in Gravitational Waveforms","ref_index":104,"is_internal_anchor":false},{"citing_arxiv_id":"2511.12580","citing_title":"Dynamical Tidal Response of Non-rotating Black Holes: Connecting the MST Formalism and Worldline EFT","ref_index":100,"is_internal_anchor":false},{"citing_arxiv_id":"2511.19626","citing_title":"Universal Relations with Dynamical Tides","ref_index":37,"is_internal_anchor":false},{"citing_arxiv_id":"2601.14979","citing_title":"The relativistic restricted three-body problem: geometry and motion around tidally perturbed black holes","ref_index":53,"is_internal_anchor":false},{"citing_arxiv_id":"2603.22467","citing_title":"High-order effective-one-body tidal interactions and gravitational scattering","ref_index":26,"is_internal_anchor":false},{"citing_arxiv_id":"2604.27046","citing_title":"Tidal Response and Thermodynamics of Black Holes","ref_index":36,"is_internal_anchor":false},{"citing_arxiv_id":"2605.08569","citing_title":"The Good, the Bad, and the Subtle: Relativistic mode sums for neutron-star tidal response","ref_index":31,"is_internal_anchor":false},{"citing_arxiv_id":"2604.08653","citing_title":"Love numbers of black holes and compact objects","ref_index":64,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/5YH32C52EM5WZAHEMFUXCUVJ7Z","json":"https://pith.science/pith/5YH32C52EM5WZAHEMFUXCUVJ7Z.json","graph_json":"https://pith.science/api/pith-number/5YH32C52EM5WZAHEMFUXCUVJ7Z/graph.json","events_json":"https://pith.science/api/pith-number/5YH32C52EM5WZAHEMFUXCUVJ7Z/events.json","paper":"https://pith.science/paper/5YH32C52"},"agent_actions":{"view_html":"https://pith.science/pith/5YH32C52EM5WZAHEMFUXCUVJ7Z","download_json":"https://pith.science/pith/5YH32C52EM5WZAHEMFUXCUVJ7Z.json","view_paper":"https://pith.science/paper/5YH32C52","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2012.10184&json=true","fetch_graph":"https://pith.science/api/pith-number/5YH32C52EM5WZAHEMFUXCUVJ7Z/graph.json","fetch_events":"https://pith.science/api/pith-number/5YH32C52EM5WZAHEMFUXCUVJ7Z/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/5YH32C52EM5WZAHEMFUXCUVJ7Z/action/timestamp_anchor","attest_storage":"https://pith.science/pith/5YH32C52EM5WZAHEMFUXCUVJ7Z/action/storage_attestation","attest_author":"https://pith.science/pith/5YH32C52EM5WZAHEMFUXCUVJ7Z/action/author_attestation","sign_citation":"https://pith.science/pith/5YH32C52EM5WZAHEMFUXCUVJ7Z/action/citation_signature","submit_replication":"https://pith.science/pith/5YH32C52EM5WZAHEMFUXCUVJ7Z/action/replication_record"}},"created_at":"2026-07-05T02:25:32.312514+00:00","updated_at":"2026-07-05T02:25:32.312514+00:00"}