{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2019:CXL2ZGTM5IWHTY6N2TSK5E5FKS","short_pith_number":"pith:CXL2ZGTM","schema_version":"1.0","canonical_sha256":"15d7ac9a6cea2c79e3cdd4e4ae93a554b1c3abbe604f92058aa514e4a8d51bf3","source":{"kind":"arxiv","id":"1910.14336","version":2},"attestation_state":"computed","paper":{"title":"Magnetar birth: rotation rates and gravitational-wave emission","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc"],"primary_cat":"astro-ph.HE","authors_text":"D. I. Jones, S. K. Lander","submitted_at":"2019-10-31T09:53:48Z","abstract_excerpt":"Understanding the evolution of the angle $\\chi$ between a magnetar's rotation and magnetic axes sheds light on the star's birth properties. This evolution is coupled with that of the stellar rotation $\\Omega$, and depends on the competing effects of internal viscous dissipation and external torques. We study this coupled evolution for a model magnetar with a strong internal toroidal field, extending previous work by modelling -- for the first time in this context -- the strong proto-magnetar wind acting shortly after birth. We also account for the effect of buoyancy forces on viscous dissipati"},"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":"1910.14336","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2019-10-31T09:53:48Z","cross_cats_sorted":["gr-qc"],"title_canon_sha256":"2abbe16136749008e97fd2af45f5cfccbfc188c8db548673d0e20707daf07323","abstract_canon_sha256":"cae968a1a99ce5cc126928bd2e399adfd37821b1bdae6971fb4176714fa16ea3"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T00:54:46.429912Z","signature_b64":"dyke+7c63oGe1tr5CUHp4M3ts42elvEsQalFKATtHfsSqFWH3mkz0rHYv+//tv/e61tLjfSIV3l7O/19ynnfAg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"15d7ac9a6cea2c79e3cdd4e4ae93a554b1c3abbe604f92058aa514e4a8d51bf3","last_reissued_at":"2026-07-05T00:54:46.429498Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T00:54:46.429498Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Magnetar birth: rotation rates and gravitational-wave emission","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc"],"primary_cat":"astro-ph.HE","authors_text":"D. I. Jones, S. K. Lander","submitted_at":"2019-10-31T09:53:48Z","abstract_excerpt":"Understanding the evolution of the angle $\\chi$ between a magnetar's rotation and magnetic axes sheds light on the star's birth properties. This evolution is coupled with that of the stellar rotation $\\Omega$, and depends on the competing effects of internal viscous dissipation and external torques. We study this coupled evolution for a model magnetar with a strong internal toroidal field, extending previous work by modelling -- for the first time in this context -- the strong proto-magnetar wind acting shortly after birth. We also account for the effect of buoyancy forces on viscous dissipati"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1910.14336","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/1910.14336/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":"1910.14336","created_at":"2026-07-05T00:54:46.429554+00:00"},{"alias_kind":"arxiv_version","alias_value":"1910.14336v2","created_at":"2026-07-05T00:54:46.429554+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1910.14336","created_at":"2026-07-05T00:54:46.429554+00:00"},{"alias_kind":"pith_short_12","alias_value":"CXL2ZGTM5IWH","created_at":"2026-07-05T00:54:46.429554+00:00"},{"alias_kind":"pith_short_16","alias_value":"CXL2ZGTM5IWHTY6N","created_at":"2026-07-05T00:54:46.429554+00:00"},{"alias_kind":"pith_short_8","alias_value":"CXL2ZGTM","created_at":"2026-07-05T00:54:46.429554+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2512.09878","citing_title":"GFH-v2 Pipeline for Searches of Long-Transient Gravitational Waves from Newborn Magnetars","ref_index":23,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/CXL2ZGTM5IWHTY6N2TSK5E5FKS","json":"https://pith.science/pith/CXL2ZGTM5IWHTY6N2TSK5E5FKS.json","graph_json":"https://pith.science/api/pith-number/CXL2ZGTM5IWHTY6N2TSK5E5FKS/graph.json","events_json":"https://pith.science/api/pith-number/CXL2ZGTM5IWHTY6N2TSK5E5FKS/events.json","paper":"https://pith.science/paper/CXL2ZGTM"},"agent_actions":{"view_html":"https://pith.science/pith/CXL2ZGTM5IWHTY6N2TSK5E5FKS","download_json":"https://pith.science/pith/CXL2ZGTM5IWHTY6N2TSK5E5FKS.json","view_paper":"https://pith.science/paper/CXL2ZGTM","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1910.14336&json=true","fetch_graph":"https://pith.science/api/pith-number/CXL2ZGTM5IWHTY6N2TSK5E5FKS/graph.json","fetch_events":"https://pith.science/api/pith-number/CXL2ZGTM5IWHTY6N2TSK5E5FKS/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/CXL2ZGTM5IWHTY6N2TSK5E5FKS/action/timestamp_anchor","attest_storage":"https://pith.science/pith/CXL2ZGTM5IWHTY6N2TSK5E5FKS/action/storage_attestation","attest_author":"https://pith.science/pith/CXL2ZGTM5IWHTY6N2TSK5E5FKS/action/author_attestation","sign_citation":"https://pith.science/pith/CXL2ZGTM5IWHTY6N2TSK5E5FKS/action/citation_signature","submit_replication":"https://pith.science/pith/CXL2ZGTM5IWHTY6N2TSK5E5FKS/action/replication_record"}},"created_at":"2026-07-05T00:54:46.429554+00:00","updated_at":"2026-07-05T00:54:46.429554+00:00"}