{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:GQMRV5MZ2N2XP2TEHJ5RFCG4GQ","short_pith_number":"pith:GQMRV5MZ","schema_version":"1.0","canonical_sha256":"34191af599d37577ea643a7b1288dc34279a61893952f5dc07e74f1415e76d3c","source":{"kind":"arxiv","id":"1711.10794","version":2},"attestation_state":"computed","paper":{"title":"Gravitational waves from isolated neutron stars: mass dependence of r-mode instability","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"nucl-th","authors_text":"Debasis Atta, D. N. Basu, Joydev Lahiri, Kouser Imam, Somnath Mukhopadhyay","submitted_at":"2017-11-29T11:45:03Z","abstract_excerpt":"In this work we study the r-mode instability windows and the gravitational wave signatures of neutron stars in the slow rotation approximation using the equation of state obtained from the density dependent M3Y effective interaction. We consider the neutron star matter to be $\\beta$-equilibrated neutron-proton-electron matter at the core with a rigid crust. The fiducial gravitational and viscous timescales, the critical frequencies and the time evolutions of the frequencies and the rates of frequency change are calculated for a range of neutron star masses. We show that the young and hot rotat"},"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":"1711.10794","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"nucl-th","submitted_at":"2017-11-29T11:45:03Z","cross_cats_sorted":[],"title_canon_sha256":"c8eff230e8bc1995dbdc27af80d6feef277109db6f348484f850bb530ffde62a","abstract_canon_sha256":"7546882a34082e34c89f7a40e582061c0957699f9bebb35ef0131f4c550aeb68"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:12:58.623837Z","signature_b64":"w9PH8Jrg7P9zgoPKG9L/e7DTO+xmjN4Gh9OoCb4sPz/n1zt22ZbXjrQYYglXJz/kfHV2HDIPOIyxrTWD4oITCQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"34191af599d37577ea643a7b1288dc34279a61893952f5dc07e74f1415e76d3c","last_reissued_at":"2026-05-18T00:12:58.623154Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:12:58.623154Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Gravitational waves from isolated neutron stars: mass dependence of r-mode instability","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"nucl-th","authors_text":"Debasis Atta, D. N. Basu, Joydev Lahiri, Kouser Imam, Somnath Mukhopadhyay","submitted_at":"2017-11-29T11:45:03Z","abstract_excerpt":"In this work we study the r-mode instability windows and the gravitational wave signatures of neutron stars in the slow rotation approximation using the equation of state obtained from the density dependent M3Y effective interaction. We consider the neutron star matter to be $\\beta$-equilibrated neutron-proton-electron matter at the core with a rigid crust. The fiducial gravitational and viscous timescales, the critical frequencies and the time evolutions of the frequencies and the rates of frequency change are calculated for a range of neutron star masses. We show that the young and hot rotat"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1711.10794","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":""},"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":"1711.10794","created_at":"2026-05-18T00:12:58.623288+00:00"},{"alias_kind":"arxiv_version","alias_value":"1711.10794v2","created_at":"2026-05-18T00:12:58.623288+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1711.10794","created_at":"2026-05-18T00:12:58.623288+00:00"},{"alias_kind":"pith_short_12","alias_value":"GQMRV5MZ2N2X","created_at":"2026-05-18T12:31:18.294218+00:00"},{"alias_kind":"pith_short_16","alias_value":"GQMRV5MZ2N2XP2TE","created_at":"2026-05-18T12:31:18.294218+00:00"},{"alias_kind":"pith_short_8","alias_value":"GQMRV5MZ","created_at":"2026-05-18T12:31:18.294218+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":0,"internal_anchor_count":0,"sample":[]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/GQMRV5MZ2N2XP2TEHJ5RFCG4GQ","json":"https://pith.science/pith/GQMRV5MZ2N2XP2TEHJ5RFCG4GQ.json","graph_json":"https://pith.science/api/pith-number/GQMRV5MZ2N2XP2TEHJ5RFCG4GQ/graph.json","events_json":"https://pith.science/api/pith-number/GQMRV5MZ2N2XP2TEHJ5RFCG4GQ/events.json","paper":"https://pith.science/paper/GQMRV5MZ"},"agent_actions":{"view_html":"https://pith.science/pith/GQMRV5MZ2N2XP2TEHJ5RFCG4GQ","download_json":"https://pith.science/pith/GQMRV5MZ2N2XP2TEHJ5RFCG4GQ.json","view_paper":"https://pith.science/paper/GQMRV5MZ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1711.10794&json=true","fetch_graph":"https://pith.science/api/pith-number/GQMRV5MZ2N2XP2TEHJ5RFCG4GQ/graph.json","fetch_events":"https://pith.science/api/pith-number/GQMRV5MZ2N2XP2TEHJ5RFCG4GQ/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/GQMRV5MZ2N2XP2TEHJ5RFCG4GQ/action/timestamp_anchor","attest_storage":"https://pith.science/pith/GQMRV5MZ2N2XP2TEHJ5RFCG4GQ/action/storage_attestation","attest_author":"https://pith.science/pith/GQMRV5MZ2N2XP2TEHJ5RFCG4GQ/action/author_attestation","sign_citation":"https://pith.science/pith/GQMRV5MZ2N2XP2TEHJ5RFCG4GQ/action/citation_signature","submit_replication":"https://pith.science/pith/GQMRV5MZ2N2XP2TEHJ5RFCG4GQ/action/replication_record"}},"created_at":"2026-05-18T00:12:58.623288+00:00","updated_at":"2026-05-18T00:12:58.623288+00:00"}