{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2018:6RBD4UR5QLKUBBNSQNO7QCJPHB","short_pith_number":"pith:6RBD4UR5","schema_version":"1.0","canonical_sha256":"f4423e523d82d54085b2835df8092f38418c15945bc39aec1c49e58966c564df","source":{"kind":"arxiv","id":"1802.05432","version":1},"attestation_state":"computed","paper":{"title":"On the timing behavior of PSR B1259-63 under the propeller torque from a transient accretion disc","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"K-S Cheng, Shu-Xu Yi","submitted_at":"2018-02-15T08:16:16Z","abstract_excerpt":"The $\\gamma$-ray pulsar binary system PSR B1259-63 flares in GeV after each periastron. The origin of those flares is still under debate. Recently, [2017ApJ...844..114Y] proposed a mechanism that might explain the GeV flares. In that model, a transient accretion disc is expected to be formed from the matter which was gravity-captured by the neutron star from the main sequence companion's circumstellar disc. The transient accretion disc exerts a spin down torque on the neutron star (propeller effect), which might be traceable via pulsar timing observation of PSR B1259-63. In this paper, we phen"},"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":"1802.05432","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2018-02-15T08:16:16Z","cross_cats_sorted":[],"title_canon_sha256":"73e35ae365f3e9474ccec02eeec7be76b2c1192c299b5b7f803bbd0317c6f35c","abstract_canon_sha256":"4e2c1d589d7a5ac67eb3499f64fd9eb8d51723bd31d5a3c8329979a39f7c724e"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:21:19.687128Z","signature_b64":"3f/DknqPKFTX99AHYc+WIbTEvXz80lFjUHmeBGNU4s2VTESjgaFjegfqknEreWSp6Yf1Y6oJaYslrE9PDIZLDQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"f4423e523d82d54085b2835df8092f38418c15945bc39aec1c49e58966c564df","last_reissued_at":"2026-05-18T00:21:19.685934Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:21:19.685934Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"On the timing behavior of PSR B1259-63 under the propeller torque from a transient accretion disc","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"K-S Cheng, Shu-Xu Yi","submitted_at":"2018-02-15T08:16:16Z","abstract_excerpt":"The $\\gamma$-ray pulsar binary system PSR B1259-63 flares in GeV after each periastron. The origin of those flares is still under debate. Recently, [2017ApJ...844..114Y] proposed a mechanism that might explain the GeV flares. In that model, a transient accretion disc is expected to be formed from the matter which was gravity-captured by the neutron star from the main sequence companion's circumstellar disc. The transient accretion disc exerts a spin down torque on the neutron star (propeller effect), which might be traceable via pulsar timing observation of PSR B1259-63. In this paper, we phen"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1802.05432","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":"1802.05432","created_at":"2026-05-18T00:21:19.686421+00:00"},{"alias_kind":"arxiv_version","alias_value":"1802.05432v1","created_at":"2026-05-18T00:21:19.686421+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1802.05432","created_at":"2026-05-18T00:21:19.686421+00:00"},{"alias_kind":"pith_short_12","alias_value":"6RBD4UR5QLKU","created_at":"2026-05-18T12:32:11.075285+00:00"},{"alias_kind":"pith_short_16","alias_value":"6RBD4UR5QLKUBBNS","created_at":"2026-05-18T12:32:11.075285+00:00"},{"alias_kind":"pith_short_8","alias_value":"6RBD4UR5","created_at":"2026-05-18T12:32:11.075285+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/6RBD4UR5QLKUBBNSQNO7QCJPHB","json":"https://pith.science/pith/6RBD4UR5QLKUBBNSQNO7QCJPHB.json","graph_json":"https://pith.science/api/pith-number/6RBD4UR5QLKUBBNSQNO7QCJPHB/graph.json","events_json":"https://pith.science/api/pith-number/6RBD4UR5QLKUBBNSQNO7QCJPHB/events.json","paper":"https://pith.science/paper/6RBD4UR5"},"agent_actions":{"view_html":"https://pith.science/pith/6RBD4UR5QLKUBBNSQNO7QCJPHB","download_json":"https://pith.science/pith/6RBD4UR5QLKUBBNSQNO7QCJPHB.json","view_paper":"https://pith.science/paper/6RBD4UR5","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1802.05432&json=true","fetch_graph":"https://pith.science/api/pith-number/6RBD4UR5QLKUBBNSQNO7QCJPHB/graph.json","fetch_events":"https://pith.science/api/pith-number/6RBD4UR5QLKUBBNSQNO7QCJPHB/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/6RBD4UR5QLKUBBNSQNO7QCJPHB/action/timestamp_anchor","attest_storage":"https://pith.science/pith/6RBD4UR5QLKUBBNSQNO7QCJPHB/action/storage_attestation","attest_author":"https://pith.science/pith/6RBD4UR5QLKUBBNSQNO7QCJPHB/action/author_attestation","sign_citation":"https://pith.science/pith/6RBD4UR5QLKUBBNSQNO7QCJPHB/action/citation_signature","submit_replication":"https://pith.science/pith/6RBD4UR5QLKUBBNSQNO7QCJPHB/action/replication_record"}},"created_at":"2026-05-18T00:21:19.686421+00:00","updated_at":"2026-05-18T00:21:19.686421+00:00"}