{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2022:RVOAROD4ZAYTKMQ6KOFHVNQZAN","short_pith_number":"pith:RVOAROD4","schema_version":"1.0","canonical_sha256":"8d5c08b87cc83135321e538a7ab619034d6b3eeeac1295fa74151f773af0790c","source":{"kind":"arxiv","id":"2203.00023","version":1},"attestation_state":"computed","paper":{"title":"Global Kinetic Modeling of the Intrabinary Shock in Spider Pulsars","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Jorge Cort\\'es, Lorenzo Sironi","submitted_at":"2022-02-28T19:00:05Z","abstract_excerpt":"Spider pulsars are compact binary systems composed of a millisecond pulsar and a low-mass companion. The relativistic magnetically-dominated pulsar wind impacts onto the companion, ablating it and slowly consuming its atmosphere. The interaction forms an intrabinary shock, a proposed site of particle acceleration. We perform global fully-kinetic particle-in-cell simulations of the intrabinary shock, assuming that the pulsar wind consists of plane-parallel stripes of alternating polarity and that the shock wraps around the companion. We find that particles are efficiently accelerated via shock-"},"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":"2203.00023","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2022-02-28T19:00:05Z","cross_cats_sorted":[],"title_canon_sha256":"8ae9a466d3927a55a4602ea224f2a7f170f930f54d4c6e8183620af8b1d64cbb","abstract_canon_sha256":"ded224ac570a9a287f8ba8ad434b7aa0ce1bf1bf6e3524b15d60e4bb144cd982"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T04:41:33.202996Z","signature_b64":"HqBk/5m7xLGondsA446O2oGhs7Oh+6+XuXLVGK/a3r65FfaAdX0sM9yQrsWpZcbFZGz5Ir9oRyqM2UaqpbrhCQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"8d5c08b87cc83135321e538a7ab619034d6b3eeeac1295fa74151f773af0790c","last_reissued_at":"2026-07-05T04:41:33.202596Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T04:41:33.202596Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Global Kinetic Modeling of the Intrabinary Shock in Spider Pulsars","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Jorge Cort\\'es, Lorenzo Sironi","submitted_at":"2022-02-28T19:00:05Z","abstract_excerpt":"Spider pulsars are compact binary systems composed of a millisecond pulsar and a low-mass companion. The relativistic magnetically-dominated pulsar wind impacts onto the companion, ablating it and slowly consuming its atmosphere. The interaction forms an intrabinary shock, a proposed site of particle acceleration. We perform global fully-kinetic particle-in-cell simulations of the intrabinary shock, assuming that the pulsar wind consists of plane-parallel stripes of alternating polarity and that the shock wraps around the companion. We find that particles are efficiently accelerated via shock-"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2203.00023","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/2203.00023/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":"2203.00023","created_at":"2026-07-05T04:41:33.202648+00:00"},{"alias_kind":"arxiv_version","alias_value":"2203.00023v1","created_at":"2026-07-05T04:41:33.202648+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2203.00023","created_at":"2026-07-05T04:41:33.202648+00:00"},{"alias_kind":"pith_short_12","alias_value":"RVOAROD4ZAYT","created_at":"2026-07-05T04:41:33.202648+00:00"},{"alias_kind":"pith_short_16","alias_value":"RVOAROD4ZAYTKMQ6","created_at":"2026-07-05T04:41:33.202648+00:00"},{"alias_kind":"pith_short_8","alias_value":"RVOAROD4","created_at":"2026-07-05T04:41:33.202648+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2603.28528","citing_title":"Search for TeV emission from spider millisecond pulsars with HAWC","ref_index":27,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/RVOAROD4ZAYTKMQ6KOFHVNQZAN","json":"https://pith.science/pith/RVOAROD4ZAYTKMQ6KOFHVNQZAN.json","graph_json":"https://pith.science/api/pith-number/RVOAROD4ZAYTKMQ6KOFHVNQZAN/graph.json","events_json":"https://pith.science/api/pith-number/RVOAROD4ZAYTKMQ6KOFHVNQZAN/events.json","paper":"https://pith.science/paper/RVOAROD4"},"agent_actions":{"view_html":"https://pith.science/pith/RVOAROD4ZAYTKMQ6KOFHVNQZAN","download_json":"https://pith.science/pith/RVOAROD4ZAYTKMQ6KOFHVNQZAN.json","view_paper":"https://pith.science/paper/RVOAROD4","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2203.00023&json=true","fetch_graph":"https://pith.science/api/pith-number/RVOAROD4ZAYTKMQ6KOFHVNQZAN/graph.json","fetch_events":"https://pith.science/api/pith-number/RVOAROD4ZAYTKMQ6KOFHVNQZAN/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/RVOAROD4ZAYTKMQ6KOFHVNQZAN/action/timestamp_anchor","attest_storage":"https://pith.science/pith/RVOAROD4ZAYTKMQ6KOFHVNQZAN/action/storage_attestation","attest_author":"https://pith.science/pith/RVOAROD4ZAYTKMQ6KOFHVNQZAN/action/author_attestation","sign_citation":"https://pith.science/pith/RVOAROD4ZAYTKMQ6KOFHVNQZAN/action/citation_signature","submit_replication":"https://pith.science/pith/RVOAROD4ZAYTKMQ6KOFHVNQZAN/action/replication_record"}},"created_at":"2026-07-05T04:41:33.202648+00:00","updated_at":"2026-07-05T04:41:33.202648+00:00"}