{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2015:Y6RDB7C6HAKAHHF3QMFEAGXNFD","short_pith_number":"pith:Y6RDB7C6","schema_version":"1.0","canonical_sha256":"c7a230fc5e3814039cbb830a401aed28c5a5e7ca4975499fd8a0aa37a31f9d8a","source":{"kind":"arxiv","id":"1503.05859","version":1},"attestation_state":"computed","paper":{"title":"Evolutionary tracks of millisecond pulsars with low-mass companions","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Filip Ficek, Mieszko Rutkowski, W{\\l}odek Klu\\'zniak","submitted_at":"2015-03-19T17:59:13Z","abstract_excerpt":"We consider the evolution of millisecond radio pulsars in binary systems with a main-sequence or evolved stellar companion. Evolution of non-accreting binary systems with \"eclipsing\" milisecond pulsars was described by Klu\\'zniak, Czerny & Ray (1992) who predicted that systems like the one containing the Terzan 5 PSR 1744-24A will in the future become accreting low mass X-ray binaries (LMXBs), while PSR 1957+20 may evaporate its companion. The model presented in the current paper gives similar results for these two objects and allows to obtain diverse evolutionary tracks of millisecond pulsars"},"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":"1503.05859","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2015-03-19T17:59:13Z","cross_cats_sorted":[],"title_canon_sha256":"837a885eb1fe2d3226f574627cee408f48862229006da9d5afaa1e2070d41b60","abstract_canon_sha256":"51644aa5fa0431fff054eb0e973c8ca6cc9a0558ad9f3fe4ddeb70bb394258c6"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:20:50.982103Z","signature_b64":"AC8M+eaQJjF/m2j9sSPH0HIZvhPKkdiiiQOTzGhp7AxnoAm9NW/fgbpl8YE1cG0Ahox/dppUr9EW43WvCirSCA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"c7a230fc5e3814039cbb830a401aed28c5a5e7ca4975499fd8a0aa37a31f9d8a","last_reissued_at":"2026-05-18T02:20:50.981391Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:20:50.981391Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Evolutionary tracks of millisecond pulsars with low-mass companions","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Filip Ficek, Mieszko Rutkowski, W{\\l}odek Klu\\'zniak","submitted_at":"2015-03-19T17:59:13Z","abstract_excerpt":"We consider the evolution of millisecond radio pulsars in binary systems with a main-sequence or evolved stellar companion. Evolution of non-accreting binary systems with \"eclipsing\" milisecond pulsars was described by Klu\\'zniak, Czerny & Ray (1992) who predicted that systems like the one containing the Terzan 5 PSR 1744-24A will in the future become accreting low mass X-ray binaries (LMXBs), while PSR 1957+20 may evaporate its companion. The model presented in the current paper gives similar results for these two objects and allows to obtain diverse evolutionary tracks of millisecond pulsars"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1503.05859","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":"1503.05859","created_at":"2026-05-18T02:20:50.981507+00:00"},{"alias_kind":"arxiv_version","alias_value":"1503.05859v1","created_at":"2026-05-18T02:20:50.981507+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1503.05859","created_at":"2026-05-18T02:20:50.981507+00:00"},{"alias_kind":"pith_short_12","alias_value":"Y6RDB7C6HAKA","created_at":"2026-05-18T12:29:50.041715+00:00"},{"alias_kind":"pith_short_16","alias_value":"Y6RDB7C6HAKAHHF3","created_at":"2026-05-18T12:29:50.041715+00:00"},{"alias_kind":"pith_short_8","alias_value":"Y6RDB7C6","created_at":"2026-05-18T12:29:50.041715+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/Y6RDB7C6HAKAHHF3QMFEAGXNFD","json":"https://pith.science/pith/Y6RDB7C6HAKAHHF3QMFEAGXNFD.json","graph_json":"https://pith.science/api/pith-number/Y6RDB7C6HAKAHHF3QMFEAGXNFD/graph.json","events_json":"https://pith.science/api/pith-number/Y6RDB7C6HAKAHHF3QMFEAGXNFD/events.json","paper":"https://pith.science/paper/Y6RDB7C6"},"agent_actions":{"view_html":"https://pith.science/pith/Y6RDB7C6HAKAHHF3QMFEAGXNFD","download_json":"https://pith.science/pith/Y6RDB7C6HAKAHHF3QMFEAGXNFD.json","view_paper":"https://pith.science/paper/Y6RDB7C6","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1503.05859&json=true","fetch_graph":"https://pith.science/api/pith-number/Y6RDB7C6HAKAHHF3QMFEAGXNFD/graph.json","fetch_events":"https://pith.science/api/pith-number/Y6RDB7C6HAKAHHF3QMFEAGXNFD/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/Y6RDB7C6HAKAHHF3QMFEAGXNFD/action/timestamp_anchor","attest_storage":"https://pith.science/pith/Y6RDB7C6HAKAHHF3QMFEAGXNFD/action/storage_attestation","attest_author":"https://pith.science/pith/Y6RDB7C6HAKAHHF3QMFEAGXNFD/action/author_attestation","sign_citation":"https://pith.science/pith/Y6RDB7C6HAKAHHF3QMFEAGXNFD/action/citation_signature","submit_replication":"https://pith.science/pith/Y6RDB7C6HAKAHHF3QMFEAGXNFD/action/replication_record"}},"created_at":"2026-05-18T02:20:50.981507+00:00","updated_at":"2026-05-18T02:20:50.981507+00:00"}