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Generally, both BPSRs and MSPs are believed to be recycled and spun-up in binary accreting phases, and evolved below the spin-up line setting by the Eddington accretion rate ($\\dot{M}{\\bf \\simeq}10^{18} g/s$). It is noticed that most BPSRs are distributed around the spin-up line with mass accretion rate $\\dot{M}=10^{16} g/s$ and almost all MSP samples lie above the spin-up line with $\\dot{M}\\sim10^{15} g/s$. Thus, we calcul"},"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":"1304.2489","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2013-04-09T08:30:55Z","cross_cats_sorted":[],"title_canon_sha256":"7324344e58ba4209ef792e3bc92001791e49e38b3ce05bdb07307bc0a586a769","abstract_canon_sha256":"681ab9091263b22a3eeec88507c85fe839e59251fcb5b1339437ec3c25eb7df4"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T03:28:31.786441Z","signature_b64":"yVn6g+R5s+Xk54mswsF3EUVBdYMeRqpsY61rPGqGEtX/VI6c6s2toI2/YgjtGKYUOKVvMof5WjMERJsYaopNAg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"7a3be0a64855411dfba81623a5abece0c796417df62d01f3e4e51560151ee730","last_reissued_at":"2026-05-18T03:28:31.785555Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T03:28:31.785555Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Binary Pulsars in Magnetic Field versus Spin Period Diagram","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Pan Yuanyue, Wang Na, Zhang Chengmin","submitted_at":"2013-04-09T08:30:55Z","abstract_excerpt":"We analyzed 186 binary pulsars (BPSRs) in the magnetic field versus spin period (B-P) diagram, where their relations to the millisecond pulsars (MSPs) can be clearly shown. 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