{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2016:QYT3GW4DZ5XTPOL6MNETLLRXES","short_pith_number":"pith:QYT3GW4D","schema_version":"1.0","canonical_sha256":"8627b35b83cf6f37b97e634935ae372489ecd3cd562d4d7990187206cf5f515e","source":{"kind":"arxiv","id":"1608.08207","version":1},"attestation_state":"computed","paper":{"title":"Uniformly rotating neutron stars","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.SR","gr-qc"],"primary_cat":"astro-ph.HE","authors_text":"Kuantay Boshkayev","submitted_at":"2016-08-29T02:44:16Z","abstract_excerpt":"In this chapter we review the recent results on the equilibrium configurations of static and uniformly rotating neutron stars within the Hartle formalism. We start from the Einstein-Maxwell-Thomas-Fermi equations formulated and extended by Belvedere et al. (2012, 2014). We demonstrate how to conduct numerical integration of these equations for different central densities ${\\it \\rho}_c$ and angular velocities $\\Omega$ and compute the static $M^{stat}$ and rotating $M^{rot}$ masses, polar $R_p$ and equatorial $R_{\\rm eq}$ radii, eccentricity $\\epsilon$, moment of inertia $I$, angular momentum $J"},"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":"1608.08207","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2016-08-29T02:44:16Z","cross_cats_sorted":["astro-ph.SR","gr-qc"],"title_canon_sha256":"6611dfc91ea4365bbe7b7e2655dfc959138143f9aa38d710e8f100a13bc82c72","abstract_canon_sha256":"447c1829482038b81eefd7a8ee52a967b2a9e5afa5859f1ac662affaa3ecce43"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:06:25.082741Z","signature_b64":"y9GeKo01LbpfmVOaoZfJmyncNQT6DBAQcyAkWSn9o2kyu0nnmXURr+tjQUjGJ+Imn0cYWFO4cYYk4sVYkopDAQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"8627b35b83cf6f37b97e634935ae372489ecd3cd562d4d7990187206cf5f515e","last_reissued_at":"2026-05-18T01:06:25.082369Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:06:25.082369Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Uniformly rotating neutron stars","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.SR","gr-qc"],"primary_cat":"astro-ph.HE","authors_text":"Kuantay Boshkayev","submitted_at":"2016-08-29T02:44:16Z","abstract_excerpt":"In this chapter we review the recent results on the equilibrium configurations of static and uniformly rotating neutron stars within the Hartle formalism. We start from the Einstein-Maxwell-Thomas-Fermi equations formulated and extended by Belvedere et al. (2012, 2014). We demonstrate how to conduct numerical integration of these equations for different central densities ${\\it \\rho}_c$ and angular velocities $\\Omega$ and compute the static $M^{stat}$ and rotating $M^{rot}$ masses, polar $R_p$ and equatorial $R_{\\rm eq}$ radii, eccentricity $\\epsilon$, moment of inertia $I$, angular momentum $J"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1608.08207","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":"1608.08207","created_at":"2026-05-18T01:06:25.082430+00:00"},{"alias_kind":"arxiv_version","alias_value":"1608.08207v1","created_at":"2026-05-18T01:06:25.082430+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1608.08207","created_at":"2026-05-18T01:06:25.082430+00:00"},{"alias_kind":"pith_short_12","alias_value":"QYT3GW4DZ5XT","created_at":"2026-05-18T12:30:41.710351+00:00"},{"alias_kind":"pith_short_16","alias_value":"QYT3GW4DZ5XTPOL6","created_at":"2026-05-18T12:30:41.710351+00:00"},{"alias_kind":"pith_short_8","alias_value":"QYT3GW4D","created_at":"2026-05-18T12:30:41.710351+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/QYT3GW4DZ5XTPOL6MNETLLRXES","json":"https://pith.science/pith/QYT3GW4DZ5XTPOL6MNETLLRXES.json","graph_json":"https://pith.science/api/pith-number/QYT3GW4DZ5XTPOL6MNETLLRXES/graph.json","events_json":"https://pith.science/api/pith-number/QYT3GW4DZ5XTPOL6MNETLLRXES/events.json","paper":"https://pith.science/paper/QYT3GW4D"},"agent_actions":{"view_html":"https://pith.science/pith/QYT3GW4DZ5XTPOL6MNETLLRXES","download_json":"https://pith.science/pith/QYT3GW4DZ5XTPOL6MNETLLRXES.json","view_paper":"https://pith.science/paper/QYT3GW4D","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1608.08207&json=true","fetch_graph":"https://pith.science/api/pith-number/QYT3GW4DZ5XTPOL6MNETLLRXES/graph.json","fetch_events":"https://pith.science/api/pith-number/QYT3GW4DZ5XTPOL6MNETLLRXES/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/QYT3GW4DZ5XTPOL6MNETLLRXES/action/timestamp_anchor","attest_storage":"https://pith.science/pith/QYT3GW4DZ5XTPOL6MNETLLRXES/action/storage_attestation","attest_author":"https://pith.science/pith/QYT3GW4DZ5XTPOL6MNETLLRXES/action/author_attestation","sign_citation":"https://pith.science/pith/QYT3GW4DZ5XTPOL6MNETLLRXES/action/citation_signature","submit_replication":"https://pith.science/pith/QYT3GW4DZ5XTPOL6MNETLLRXES/action/replication_record"}},"created_at":"2026-05-18T01:06:25.082430+00:00","updated_at":"2026-05-18T01:06:25.082430+00:00"}