{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2019:XWDUF62XLA262GIDDVTGETEPGA","short_pith_number":"pith:XWDUF62X","schema_version":"1.0","canonical_sha256":"bd8742fb575835ed19031d66624c8f3016c97f7b4167aaa9e242818f1f561d82","source":{"kind":"arxiv","id":"1906.11702","version":1},"attestation_state":"computed","paper":{"title":"The force-free dipole magnetosphere in non-linear electrodynamics","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc"],"primary_cat":"astro-ph.HE","authors_text":"Huiquan Li, Jiancheng Wang, Xiaolin Yang","submitted_at":"2019-06-27T14:48:46Z","abstract_excerpt":"Quantum electrodynamics (QED) effects may be included in physical processes of magnetar and pulsar magnetospheres with strong magnetic fields. Involving the quantum corrections, the Maxwell electrodynamics is modified to non-linear electrodynamics. In this work, we study the force-free magnetosphere in non-linear electrodynamics in a general framework. The pulsar equation describing a steady and axisymmetric magnetosphere is derived, which now admits solutions with corrections. We derive the first-order non-linear corrections to the near-zone dipole magnetosphere in some popular non-linear eff"},"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":"1906.11702","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2019-06-27T14:48:46Z","cross_cats_sorted":["gr-qc"],"title_canon_sha256":"ec656553905d138552d34b99e80ae01f9ce1f38dde5306e9b07ec946ba8c99b6","abstract_canon_sha256":"b0f528d7e95dc9b46a17761fda85f8e062496d5a67414df14d963f8746cd187b"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T00:55:02.494561Z","signature_b64":"JMrORkiofl0N8VT8BVzZ0LB/J994/uD/CS41lQZFYtHinsAX0O77CTnTTsml6jFdE1lrsFilaiPcYxHhtftPBw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"bd8742fb575835ed19031d66624c8f3016c97f7b4167aaa9e242818f1f561d82","last_reissued_at":"2026-07-05T00:55:02.494049Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T00:55:02.494049Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The force-free dipole magnetosphere in non-linear electrodynamics","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc"],"primary_cat":"astro-ph.HE","authors_text":"Huiquan Li, Jiancheng Wang, Xiaolin Yang","submitted_at":"2019-06-27T14:48:46Z","abstract_excerpt":"Quantum electrodynamics (QED) effects may be included in physical processes of magnetar and pulsar magnetospheres with strong magnetic fields. Involving the quantum corrections, the Maxwell electrodynamics is modified to non-linear electrodynamics. In this work, we study the force-free magnetosphere in non-linear electrodynamics in a general framework. The pulsar equation describing a steady and axisymmetric magnetosphere is derived, which now admits solutions with corrections. We derive the first-order non-linear corrections to the near-zone dipole magnetosphere in some popular non-linear eff"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1906.11702","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/1906.11702/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"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":"1906.11702","created_at":"2026-07-05T00:55:02.494108+00:00"},{"alias_kind":"arxiv_version","alias_value":"1906.11702v1","created_at":"2026-07-05T00:55:02.494108+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1906.11702","created_at":"2026-07-05T00:55:02.494108+00:00"},{"alias_kind":"pith_short_12","alias_value":"XWDUF62XLA26","created_at":"2026-07-05T00:55:02.494108+00:00"},{"alias_kind":"pith_short_16","alias_value":"XWDUF62XLA262GID","created_at":"2026-07-05T00:55:02.494108+00:00"},{"alias_kind":"pith_short_8","alias_value":"XWDUF62X","created_at":"2026-07-05T00:55:02.494108+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"1908.11104","citing_title":"Black hole magnetospheres in the Born-Infeld theory","ref_index":4,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/XWDUF62XLA262GIDDVTGETEPGA","json":"https://pith.science/pith/XWDUF62XLA262GIDDVTGETEPGA.json","graph_json":"https://pith.science/api/pith-number/XWDUF62XLA262GIDDVTGETEPGA/graph.json","events_json":"https://pith.science/api/pith-number/XWDUF62XLA262GIDDVTGETEPGA/events.json","paper":"https://pith.science/paper/XWDUF62X"},"agent_actions":{"view_html":"https://pith.science/pith/XWDUF62XLA262GIDDVTGETEPGA","download_json":"https://pith.science/pith/XWDUF62XLA262GIDDVTGETEPGA.json","view_paper":"https://pith.science/paper/XWDUF62X","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1906.11702&json=true","fetch_graph":"https://pith.science/api/pith-number/XWDUF62XLA262GIDDVTGETEPGA/graph.json","fetch_events":"https://pith.science/api/pith-number/XWDUF62XLA262GIDDVTGETEPGA/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/XWDUF62XLA262GIDDVTGETEPGA/action/timestamp_anchor","attest_storage":"https://pith.science/pith/XWDUF62XLA262GIDDVTGETEPGA/action/storage_attestation","attest_author":"https://pith.science/pith/XWDUF62XLA262GIDDVTGETEPGA/action/author_attestation","sign_citation":"https://pith.science/pith/XWDUF62XLA262GIDDVTGETEPGA/action/citation_signature","submit_replication":"https://pith.science/pith/XWDUF62XLA262GIDDVTGETEPGA/action/replication_record"}},"created_at":"2026-07-05T00:55:02.494108+00:00","updated_at":"2026-07-05T00:55:02.494108+00:00"}