{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2016:JPL7LEN4PJOFAQZYTNIVZ5W5Z5","short_pith_number":"pith:JPL7LEN4","schema_version":"1.0","canonical_sha256":"4bd7f591bc7a5c5043389b515cf6ddcf535135765fc9a4e8db99cb056f5453c2","source":{"kind":"arxiv","id":"1606.02934","version":2},"attestation_state":"computed","paper":{"title":"Internal X-ray plateau in short GRBs: Signature of supramassive fast-rotating quark stars?","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.SR","nucl-th"],"primary_cat":"astro-ph.HE","authors_text":"Ang Li, Bing Zhang, Bin Qi, He Gao, Nai Bo Zhang, Tong Liu","submitted_at":"2016-06-09T12:36:43Z","abstract_excerpt":"A supramassive, strongly-magnetized millisecond neutron star (NS) has been proposed to be the candidate central engine of at least some short gamma-ray bursts (SGRBs), based on the \"internal plateau\" commonly observed in the early X-ray afterglow. While a previous analysis shows a qualitative consistency between this suggestion and the Swift SGRB data, the distribution of observed break time $t_b$ is much narrower than the distribution of the collapse time of supramassive NSs for the several NS equations-of-state (EoSs) investigated. In this paper, we study four recently-constructed \"unified\" "},"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":"1606.02934","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2016-06-09T12:36:43Z","cross_cats_sorted":["astro-ph.SR","nucl-th"],"title_canon_sha256":"73fa9201afb55803882f07d8ad176b3a60893aece6a4799775e540afc7cf7a6c","abstract_canon_sha256":"721d1ae9304babfe11318524a8477e56a313c178d1d904b855f4e433a6eb6cb1"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:00:45.498310Z","signature_b64":"ayYUXuSee5HlmpQkuAVwzJH7u+ot4Hl92869fVMCRqYWr77N0akhMQTrXNjW1CehuT5YeUmKWQLm6ti/ZcvyDw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"4bd7f591bc7a5c5043389b515cf6ddcf535135765fc9a4e8db99cb056f5453c2","last_reissued_at":"2026-05-18T01:00:45.497902Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:00:45.497902Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Internal X-ray plateau in short GRBs: Signature of supramassive fast-rotating quark stars?","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.SR","nucl-th"],"primary_cat":"astro-ph.HE","authors_text":"Ang Li, Bing Zhang, Bin Qi, He Gao, Nai Bo Zhang, Tong Liu","submitted_at":"2016-06-09T12:36:43Z","abstract_excerpt":"A supramassive, strongly-magnetized millisecond neutron star (NS) has been proposed to be the candidate central engine of at least some short gamma-ray bursts (SGRBs), based on the \"internal plateau\" commonly observed in the early X-ray afterglow. While a previous analysis shows a qualitative consistency between this suggestion and the Swift SGRB data, the distribution of observed break time $t_b$ is much narrower than the distribution of the collapse time of supramassive NSs for the several NS equations-of-state (EoSs) investigated. In this paper, we study four recently-constructed \"unified\" "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1606.02934","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":"1606.02934","created_at":"2026-05-18T01:00:45.497962+00:00"},{"alias_kind":"arxiv_version","alias_value":"1606.02934v2","created_at":"2026-05-18T01:00:45.497962+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1606.02934","created_at":"2026-05-18T01:00:45.497962+00:00"},{"alias_kind":"pith_short_12","alias_value":"JPL7LEN4PJOF","created_at":"2026-05-18T12:30:25.849896+00:00"},{"alias_kind":"pith_short_16","alias_value":"JPL7LEN4PJOFAQZY","created_at":"2026-05-18T12:30:25.849896+00:00"},{"alias_kind":"pith_short_8","alias_value":"JPL7LEN4","created_at":"2026-05-18T12:30:25.849896+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/JPL7LEN4PJOFAQZYTNIVZ5W5Z5","json":"https://pith.science/pith/JPL7LEN4PJOFAQZYTNIVZ5W5Z5.json","graph_json":"https://pith.science/api/pith-number/JPL7LEN4PJOFAQZYTNIVZ5W5Z5/graph.json","events_json":"https://pith.science/api/pith-number/JPL7LEN4PJOFAQZYTNIVZ5W5Z5/events.json","paper":"https://pith.science/paper/JPL7LEN4"},"agent_actions":{"view_html":"https://pith.science/pith/JPL7LEN4PJOFAQZYTNIVZ5W5Z5","download_json":"https://pith.science/pith/JPL7LEN4PJOFAQZYTNIVZ5W5Z5.json","view_paper":"https://pith.science/paper/JPL7LEN4","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1606.02934&json=true","fetch_graph":"https://pith.science/api/pith-number/JPL7LEN4PJOFAQZYTNIVZ5W5Z5/graph.json","fetch_events":"https://pith.science/api/pith-number/JPL7LEN4PJOFAQZYTNIVZ5W5Z5/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/JPL7LEN4PJOFAQZYTNIVZ5W5Z5/action/timestamp_anchor","attest_storage":"https://pith.science/pith/JPL7LEN4PJOFAQZYTNIVZ5W5Z5/action/storage_attestation","attest_author":"https://pith.science/pith/JPL7LEN4PJOFAQZYTNIVZ5W5Z5/action/author_attestation","sign_citation":"https://pith.science/pith/JPL7LEN4PJOFAQZYTNIVZ5W5Z5/action/citation_signature","submit_replication":"https://pith.science/pith/JPL7LEN4PJOFAQZYTNIVZ5W5Z5/action/replication_record"}},"created_at":"2026-05-18T01:00:45.497962+00:00","updated_at":"2026-05-18T01:00:45.497962+00:00"}