{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2020:T26OICQQ6ZUIDKL32EVV37SNTI","short_pith_number":"pith:T26OICQQ","schema_version":"1.0","canonical_sha256":"9ebce40a10f66881a97bd12b5dfe4d9a2f23cb5a282e546a2db50b4be46e54eb","source":{"kind":"arxiv","id":"2002.01477","version":1},"attestation_state":"computed","paper":{"title":"High-energy Cosmic Ray production in X-ray Binary Jets","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"A. J. Cooper, D. Gaggero, S. Markoff, S. Zhang","submitted_at":"2020-02-04T19:00:00Z","abstract_excerpt":"As smaller analogs of Active Galactic Nuclei (AGN), X-ray Binaries (XRBs) are also capable of launching jets that accelerate particles to high energies. In this work, we reexamine XRB jets as potential sources of high-energy cosmic rays (CRs) and explore whether they could provide a significant second Galactic component to the CR spectrum. In the most intriguing scenario, XRB-CRs could dominate the observed spectrum above the so-called \"knee\" feature at $\\sim 3 \\times 10^{15}$ eV, offering an explanation for several key issues in this transition zone from Galactic to extragalactic CRs. We disc"},"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":"2002.01477","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2020-02-04T19:00:00Z","cross_cats_sorted":[],"title_canon_sha256":"9730ee751fc37e2892689ed1cc295971a6c46187ecc572ecb3b80afc2e661b03","abstract_canon_sha256":"1bffdb7e69025283a7a2118017d591663daf925c9401151fc386f3463a3953e3"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T00:40:46.572174Z","signature_b64":"TJ5OmbRB/l3msMkXm+0Ebhvjxx1oaovZMzPCzXY1j/o9j30xk3cVIx/0I/rtfrUx0mbAuZ3cbSUjkhr70bNJBA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"9ebce40a10f66881a97bd12b5dfe4d9a2f23cb5a282e546a2db50b4be46e54eb","last_reissued_at":"2026-07-05T00:40:46.571671Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T00:40:46.571671Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"High-energy Cosmic Ray production in X-ray Binary Jets","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"A. J. Cooper, D. Gaggero, S. Markoff, S. Zhang","submitted_at":"2020-02-04T19:00:00Z","abstract_excerpt":"As smaller analogs of Active Galactic Nuclei (AGN), X-ray Binaries (XRBs) are also capable of launching jets that accelerate particles to high energies. In this work, we reexamine XRB jets as potential sources of high-energy cosmic rays (CRs) and explore whether they could provide a significant second Galactic component to the CR spectrum. In the most intriguing scenario, XRB-CRs could dominate the observed spectrum above the so-called \"knee\" feature at $\\sim 3 \\times 10^{15}$ eV, offering an explanation for several key issues in this transition zone from Galactic to extragalactic CRs. We disc"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2002.01477","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/2002.01477/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":"2002.01477","created_at":"2026-07-05T00:40:46.571738+00:00"},{"alias_kind":"arxiv_version","alias_value":"2002.01477v1","created_at":"2026-07-05T00:40:46.571738+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2002.01477","created_at":"2026-07-05T00:40:46.571738+00:00"},{"alias_kind":"pith_short_12","alias_value":"T26OICQQ6ZUI","created_at":"2026-07-05T00:40:46.571738+00:00"},{"alias_kind":"pith_short_16","alias_value":"T26OICQQ6ZUIDKL3","created_at":"2026-07-05T00:40:46.571738+00:00"},{"alias_kind":"pith_short_8","alias_value":"T26OICQQ","created_at":"2026-07-05T00:40:46.571738+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/T26OICQQ6ZUIDKL32EVV37SNTI","json":"https://pith.science/pith/T26OICQQ6ZUIDKL32EVV37SNTI.json","graph_json":"https://pith.science/api/pith-number/T26OICQQ6ZUIDKL32EVV37SNTI/graph.json","events_json":"https://pith.science/api/pith-number/T26OICQQ6ZUIDKL32EVV37SNTI/events.json","paper":"https://pith.science/paper/T26OICQQ"},"agent_actions":{"view_html":"https://pith.science/pith/T26OICQQ6ZUIDKL32EVV37SNTI","download_json":"https://pith.science/pith/T26OICQQ6ZUIDKL32EVV37SNTI.json","view_paper":"https://pith.science/paper/T26OICQQ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2002.01477&json=true","fetch_graph":"https://pith.science/api/pith-number/T26OICQQ6ZUIDKL32EVV37SNTI/graph.json","fetch_events":"https://pith.science/api/pith-number/T26OICQQ6ZUIDKL32EVV37SNTI/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/T26OICQQ6ZUIDKL32EVV37SNTI/action/timestamp_anchor","attest_storage":"https://pith.science/pith/T26OICQQ6ZUIDKL32EVV37SNTI/action/storage_attestation","attest_author":"https://pith.science/pith/T26OICQQ6ZUIDKL32EVV37SNTI/action/author_attestation","sign_citation":"https://pith.science/pith/T26OICQQ6ZUIDKL32EVV37SNTI/action/citation_signature","submit_replication":"https://pith.science/pith/T26OICQQ6ZUIDKL32EVV37SNTI/action/replication_record"}},"created_at":"2026-07-05T00:40:46.571738+00:00","updated_at":"2026-07-05T00:40:46.571738+00:00"}