{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2019:K5FYEUSHJBTF4SWEUT7BBAGKRC","short_pith_number":"pith:K5FYEUSH","schema_version":"1.0","canonical_sha256":"574b82524748665e4ac4a4fe1080ca88b3460b96c0f1dde222636286ff998b38","source":{"kind":"arxiv","id":"1905.00012","version":3},"attestation_state":"computed","paper":{"title":"The phenomenology of dynamical neutron star tides","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"gr-qc","authors_text":"N. Andersson, P. Pnigouras","submitted_at":"2019-04-30T17:40:37Z","abstract_excerpt":"We introduce a phenomenological, physically motivated, model for the effective tidal deformability of a neutron star, adding the frequency dependence (associated with the star's fundamental mode of oscillation) that comes into play during the late stages of the binary inspiral. Testing the model against alternative descriptions, we demonstrate that it provides an accurate representation of the dynamical tide up to close to merger. The simplicity of the prescription makes it an attractive alternative for a gravitational-wave data analysis implementation, facilitating an inexpensive construction"},"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":"1905.00012","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2019-04-30T17:40:37Z","cross_cats_sorted":["astro-ph.HE"],"title_canon_sha256":"0386180bebbf49c0c4d52a9152a3959e099f62da103f6549758f538924261b2a","abstract_canon_sha256":"b1fce88809c9a85ecbe033b34deab28b77af0cd69d3a4285a37f379ce86a9534"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T02:13:10.473822Z","signature_b64":"qTLzd9bXll/AAxxdS2aXywJOc6xRq0eKPdXfnNv7dfFaV2MmtmYWPDZYCzA0vVHiNjVrduBgjpR9qujAFI2YBw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"574b82524748665e4ac4a4fe1080ca88b3460b96c0f1dde222636286ff998b38","last_reissued_at":"2026-07-05T02:13:10.473392Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T02:13:10.473392Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The phenomenology of dynamical neutron star tides","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"gr-qc","authors_text":"N. Andersson, P. Pnigouras","submitted_at":"2019-04-30T17:40:37Z","abstract_excerpt":"We introduce a phenomenological, physically motivated, model for the effective tidal deformability of a neutron star, adding the frequency dependence (associated with the star's fundamental mode of oscillation) that comes into play during the late stages of the binary inspiral. Testing the model against alternative descriptions, we demonstrate that it provides an accurate representation of the dynamical tide up to close to merger. The simplicity of the prescription makes it an attractive alternative for a gravitational-wave data analysis implementation, facilitating an inexpensive construction"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1905.00012","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/1905.00012/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":"1905.00012","created_at":"2026-07-05T02:13:10.473453+00:00"},{"alias_kind":"arxiv_version","alias_value":"1905.00012v3","created_at":"2026-07-05T02:13:10.473453+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1905.00012","created_at":"2026-07-05T02:13:10.473453+00:00"},{"alias_kind":"pith_short_12","alias_value":"K5FYEUSHJBTF","created_at":"2026-07-05T02:13:10.473453+00:00"},{"alias_kind":"pith_short_16","alias_value":"K5FYEUSHJBTF4SWE","created_at":"2026-07-05T02:13:10.473453+00:00"},{"alias_kind":"pith_short_8","alias_value":"K5FYEUSH","created_at":"2026-07-05T02:13:10.473453+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":3,"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":22,"is_internal_anchor":false},{"citing_arxiv_id":"2606.02690","citing_title":"Speed and accuracy for long signals: Frequency-domain effective-one-body waveforms for compact binary coalescences","ref_index":45,"is_internal_anchor":false},{"citing_arxiv_id":"2604.08653","citing_title":"Love numbers of black holes and compact objects","ref_index":84,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/K5FYEUSHJBTF4SWEUT7BBAGKRC","json":"https://pith.science/pith/K5FYEUSHJBTF4SWEUT7BBAGKRC.json","graph_json":"https://pith.science/api/pith-number/K5FYEUSHJBTF4SWEUT7BBAGKRC/graph.json","events_json":"https://pith.science/api/pith-number/K5FYEUSHJBTF4SWEUT7BBAGKRC/events.json","paper":"https://pith.science/paper/K5FYEUSH"},"agent_actions":{"view_html":"https://pith.science/pith/K5FYEUSHJBTF4SWEUT7BBAGKRC","download_json":"https://pith.science/pith/K5FYEUSHJBTF4SWEUT7BBAGKRC.json","view_paper":"https://pith.science/paper/K5FYEUSH","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1905.00012&json=true","fetch_graph":"https://pith.science/api/pith-number/K5FYEUSHJBTF4SWEUT7BBAGKRC/graph.json","fetch_events":"https://pith.science/api/pith-number/K5FYEUSHJBTF4SWEUT7BBAGKRC/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/K5FYEUSHJBTF4SWEUT7BBAGKRC/action/timestamp_anchor","attest_storage":"https://pith.science/pith/K5FYEUSHJBTF4SWEUT7BBAGKRC/action/storage_attestation","attest_author":"https://pith.science/pith/K5FYEUSHJBTF4SWEUT7BBAGKRC/action/author_attestation","sign_citation":"https://pith.science/pith/K5FYEUSHJBTF4SWEUT7BBAGKRC/action/citation_signature","submit_replication":"https://pith.science/pith/K5FYEUSHJBTF4SWEUT7BBAGKRC/action/replication_record"}},"created_at":"2026-07-05T02:13:10.473453+00:00","updated_at":"2026-07-05T02:13:10.473453+00:00"}