{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2002:4N2P6WFIOPQOL3CDU5IX23UVE6","short_pith_number":"pith:4N2P6WFI","schema_version":"1.0","canonical_sha256":"e374ff58a873e0e5ec43a7517d6e9527871c647a8635126283354e7d056f6d1b","source":{"kind":"arxiv","id":"astro-ph/0211563","version":1},"attestation_state":"computed","paper":{"title":"Bare strange quark stars: formation and emission","license":"","headline":"","cross_cats":["hep-ph"],"primary_cat":"astro-ph","authors_text":"R.X. Xu (PKU)","submitted_at":"2002-11-26T10:57:12Z","abstract_excerpt":"Recent achievements of bare strange stars are briefly reviewed. A nascent protostrange star should be bare because of strong mass ejection and high temperature after the supernova detonation flame, and a crust can also hardly form except for a super-Eddington accretion. The magnetosphere of a bare strange star is composed mainly of electron-positron pair plasma, where both inner and outer vacuum gaps work for radio as well as high energy nonthermal emission. A featureless thermal spectrum is expected since no ion is above the quark surface, whilst electron cyclotron lines could appear in some "},"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":"astro-ph/0211563","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"astro-ph","submitted_at":"2002-11-26T10:57:12Z","cross_cats_sorted":["hep-ph"],"title_canon_sha256":"3ea2d5ed5bc3d5671f741d6c4e9ddef07597996bfb266a1e5dc7fb8634aa9035","abstract_canon_sha256":"147c00e959e0af28e2447f4100201e0e8988028f370f77073fabacb6759db32d"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:21:50.344487Z","signature_b64":"PtxRpX6Y42MPsQTG0W0VwhtG5uob5YmI/3Uj2F9GE/qKKVMc39yPOBEVcsYjApDJPOLqdZV5loxuDs5J0RotBQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"e374ff58a873e0e5ec43a7517d6e9527871c647a8635126283354e7d056f6d1b","last_reissued_at":"2026-05-18T01:21:50.343789Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:21:50.343789Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Bare strange quark stars: formation and emission","license":"","headline":"","cross_cats":["hep-ph"],"primary_cat":"astro-ph","authors_text":"R.X. Xu (PKU)","submitted_at":"2002-11-26T10:57:12Z","abstract_excerpt":"Recent achievements of bare strange stars are briefly reviewed. A nascent protostrange star should be bare because of strong mass ejection and high temperature after the supernova detonation flame, and a crust can also hardly form except for a super-Eddington accretion. The magnetosphere of a bare strange star is composed mainly of electron-positron pair plasma, where both inner and outer vacuum gaps work for radio as well as high energy nonthermal emission. A featureless thermal spectrum is expected since no ion is above the quark surface, whilst electron cyclotron lines could appear in some "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/0211563","kind":"arxiv","version":1},"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":"astro-ph/0211563","created_at":"2026-05-18T01:21:50.343897+00:00"},{"alias_kind":"arxiv_version","alias_value":"astro-ph/0211563v1","created_at":"2026-05-18T01:21:50.343897+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.astro-ph/0211563","created_at":"2026-05-18T01:21:50.343897+00:00"},{"alias_kind":"pith_short_12","alias_value":"4N2P6WFIOPQO","created_at":"2026-05-18T12:25:50.845339+00:00"},{"alias_kind":"pith_short_16","alias_value":"4N2P6WFIOPQOL3CD","created_at":"2026-05-18T12:25:50.845339+00:00"},{"alias_kind":"pith_short_8","alias_value":"4N2P6WFI","created_at":"2026-05-18T12:25:50.845339+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/4N2P6WFIOPQOL3CDU5IX23UVE6","json":"https://pith.science/pith/4N2P6WFIOPQOL3CDU5IX23UVE6.json","graph_json":"https://pith.science/api/pith-number/4N2P6WFIOPQOL3CDU5IX23UVE6/graph.json","events_json":"https://pith.science/api/pith-number/4N2P6WFIOPQOL3CDU5IX23UVE6/events.json","paper":"https://pith.science/paper/4N2P6WFI"},"agent_actions":{"view_html":"https://pith.science/pith/4N2P6WFIOPQOL3CDU5IX23UVE6","download_json":"https://pith.science/pith/4N2P6WFIOPQOL3CDU5IX23UVE6.json","view_paper":"https://pith.science/paper/4N2P6WFI","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=astro-ph/0211563&json=true","fetch_graph":"https://pith.science/api/pith-number/4N2P6WFIOPQOL3CDU5IX23UVE6/graph.json","fetch_events":"https://pith.science/api/pith-number/4N2P6WFIOPQOL3CDU5IX23UVE6/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/4N2P6WFIOPQOL3CDU5IX23UVE6/action/timestamp_anchor","attest_storage":"https://pith.science/pith/4N2P6WFIOPQOL3CDU5IX23UVE6/action/storage_attestation","attest_author":"https://pith.science/pith/4N2P6WFIOPQOL3CDU5IX23UVE6/action/author_attestation","sign_citation":"https://pith.science/pith/4N2P6WFIOPQOL3CDU5IX23UVE6/action/citation_signature","submit_replication":"https://pith.science/pith/4N2P6WFIOPQOL3CDU5IX23UVE6/action/replication_record"}},"created_at":"2026-05-18T01:21:50.343897+00:00","updated_at":"2026-05-18T01:21:50.343897+00:00"}