{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2012:U5ULROD6ERNGZBCWQ2XKCQVAAJ","short_pith_number":"pith:U5ULROD6","schema_version":"1.0","canonical_sha256":"a768b8b87e245a6c845686aea142a00256bf0cadbf33ecd5a1e1c569bd00d6b8","source":{"kind":"arxiv","id":"1207.2833","version":1},"attestation_state":"computed","paper":{"title":"Formation of Millisecond Pulsars from Intermediate- and Low-Mass X-ray Binaries","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Xiang-Dong Li (NJU), Yong Shao","submitted_at":"2012-07-12T03:09:07Z","abstract_excerpt":"We present a systematic study of the evolution of intermediate- and low-mass X-ray binaries consisting of an accreting neutron star of mass $1.0-1.8 M_{\\odot}$ and a donor star of mass $1.0-6.0 M_{\\odot}$. In our calculations we take into account physical processes such as unstable disk accretion, radio ejection, bump-induced detachment, and outflow from the $L_{2}$ point. Comparing the calculated results with the observations of binary radio pulsars, we report the following results. (1) The allowed parameter space for forming binary pulsars in the initial orbital period - donor mass plane inc"},"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":"1207.2833","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2012-07-12T03:09:07Z","cross_cats_sorted":[],"title_canon_sha256":"58308c0fc1543edc2961c7aff8b28258ae910aec7a8c1454523af10f6a38c6e9","abstract_canon_sha256":"2b07c88030ff7e6896daf3559024a5a776c7d6df1e8a812ef1fd1730802fb3ab"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:56:24.660399Z","signature_b64":"CDCSsSUPcyrW9k2WdoACCT9sgRkzhD1kEhwsXKDMNvd7q5raQLvbvVxGWyIOJqG+NBjL0j7GKHDwR6QmAxH3DQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"a768b8b87e245a6c845686aea142a00256bf0cadbf33ecd5a1e1c569bd00d6b8","last_reissued_at":"2026-05-18T01:56:24.659640Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:56:24.659640Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Formation of Millisecond Pulsars from Intermediate- and Low-Mass X-ray Binaries","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Xiang-Dong Li (NJU), Yong Shao","submitted_at":"2012-07-12T03:09:07Z","abstract_excerpt":"We present a systematic study of the evolution of intermediate- and low-mass X-ray binaries consisting of an accreting neutron star of mass $1.0-1.8 M_{\\odot}$ and a donor star of mass $1.0-6.0 M_{\\odot}$. In our calculations we take into account physical processes such as unstable disk accretion, radio ejection, bump-induced detachment, and outflow from the $L_{2}$ point. Comparing the calculated results with the observations of binary radio pulsars, we report the following results. (1) The allowed parameter space for forming binary pulsars in the initial orbital period - donor mass plane inc"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1207.2833","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":"1207.2833","created_at":"2026-05-18T01:56:24.659764+00:00"},{"alias_kind":"arxiv_version","alias_value":"1207.2833v1","created_at":"2026-05-18T01:56:24.659764+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1207.2833","created_at":"2026-05-18T01:56:24.659764+00:00"},{"alias_kind":"pith_short_12","alias_value":"U5ULROD6ERNG","created_at":"2026-05-18T12:27:23.164592+00:00"},{"alias_kind":"pith_short_16","alias_value":"U5ULROD6ERNGZBCW","created_at":"2026-05-18T12:27:23.164592+00:00"},{"alias_kind":"pith_short_8","alias_value":"U5ULROD6","created_at":"2026-05-18T12:27:23.164592+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/U5ULROD6ERNGZBCWQ2XKCQVAAJ","json":"https://pith.science/pith/U5ULROD6ERNGZBCWQ2XKCQVAAJ.json","graph_json":"https://pith.science/api/pith-number/U5ULROD6ERNGZBCWQ2XKCQVAAJ/graph.json","events_json":"https://pith.science/api/pith-number/U5ULROD6ERNGZBCWQ2XKCQVAAJ/events.json","paper":"https://pith.science/paper/U5ULROD6"},"agent_actions":{"view_html":"https://pith.science/pith/U5ULROD6ERNGZBCWQ2XKCQVAAJ","download_json":"https://pith.science/pith/U5ULROD6ERNGZBCWQ2XKCQVAAJ.json","view_paper":"https://pith.science/paper/U5ULROD6","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1207.2833&json=true","fetch_graph":"https://pith.science/api/pith-number/U5ULROD6ERNGZBCWQ2XKCQVAAJ/graph.json","fetch_events":"https://pith.science/api/pith-number/U5ULROD6ERNGZBCWQ2XKCQVAAJ/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/U5ULROD6ERNGZBCWQ2XKCQVAAJ/action/timestamp_anchor","attest_storage":"https://pith.science/pith/U5ULROD6ERNGZBCWQ2XKCQVAAJ/action/storage_attestation","attest_author":"https://pith.science/pith/U5ULROD6ERNGZBCWQ2XKCQVAAJ/action/author_attestation","sign_citation":"https://pith.science/pith/U5ULROD6ERNGZBCWQ2XKCQVAAJ/action/citation_signature","submit_replication":"https://pith.science/pith/U5ULROD6ERNGZBCWQ2XKCQVAAJ/action/replication_record"}},"created_at":"2026-05-18T01:56:24.659764+00:00","updated_at":"2026-05-18T01:56:24.659764+00:00"}