{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2025:SMNPA7YDVMPE2DLLI5EH7C4ZEZ","short_pith_number":"pith:SMNPA7YD","schema_version":"1.0","canonical_sha256":"931af07f03ab1e4d0d6b47487f8b99264588caa86f9f99e213dabb0a7c6b36c6","source":{"kind":"arxiv","id":"2506.17581","version":1},"attestation_state":"computed","paper":{"title":"Binary Neutron Star Mergers as Potential Sources for Ultra-High-Energy Cosmic Rays and High-Energy Neutrinos","license":"http://creativecommons.org/publicdomain/zero/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Gang Guo, Meng-Ru Wu, Yong-Zhong Qian","submitted_at":"2025-06-21T04:25:17Z","abstract_excerpt":"Recent studies suggest that the most energetic cosmic rays, exceeding 100 EeV, may primarily consist of $r$-process nuclei. This highlights binary neutron star mergers and collapsars as promising sources of ultra-high-energy cosmic rays (UHECRs). Building on these insights, we examine the conditions that facilitate the efficient production of UHE $r$-process nuclei during the prompt radiation (PR), extended emission (EE), and plateau emission phases of short gamma-ray bursts (sGRBs) following neutron star mergers. Our study reveals that jets associated with the PR phase, characterized by typic"},"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":"2506.17581","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/publicdomain/zero/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2025-06-21T04:25:17Z","cross_cats_sorted":[],"title_canon_sha256":"51ff1646364c3fca857fff4ca7bf51f1f39253954d8ff853212ef1162b565ce1","abstract_canon_sha256":"05ad77aa069a7860b13b40e39afad30509b49c379982f9ea9e1b7225b3f12bff"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T11:25:19.879405Z","signature_b64":"AgpNuPGkM33db+/N6XL+dXheMZnetI6tWk5yE9aHujAhJGaWTUfoxlauE8tYPXE9jyJf0xdEOVG1nLJEhI6bDA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"931af07f03ab1e4d0d6b47487f8b99264588caa86f9f99e213dabb0a7c6b36c6","last_reissued_at":"2026-07-05T11:25:19.878915Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T11:25:19.878915Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Binary Neutron Star Mergers as Potential Sources for Ultra-High-Energy Cosmic Rays and High-Energy Neutrinos","license":"http://creativecommons.org/publicdomain/zero/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Gang Guo, Meng-Ru Wu, Yong-Zhong Qian","submitted_at":"2025-06-21T04:25:17Z","abstract_excerpt":"Recent studies suggest that the most energetic cosmic rays, exceeding 100 EeV, may primarily consist of $r$-process nuclei. This highlights binary neutron star mergers and collapsars as promising sources of ultra-high-energy cosmic rays (UHECRs). Building on these insights, we examine the conditions that facilitate the efficient production of UHE $r$-process nuclei during the prompt radiation (PR), extended emission (EE), and plateau emission phases of short gamma-ray bursts (sGRBs) following neutron star mergers. Our study reveals that jets associated with the PR phase, characterized by typic"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2506.17581","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/2506.17581/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":"2506.17581","created_at":"2026-07-05T11:25:19.878980+00:00"},{"alias_kind":"arxiv_version","alias_value":"2506.17581v1","created_at":"2026-07-05T11:25:19.878980+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2506.17581","created_at":"2026-07-05T11:25:19.878980+00:00"},{"alias_kind":"pith_short_12","alias_value":"SMNPA7YDVMPE","created_at":"2026-07-05T11:25:19.878980+00:00"},{"alias_kind":"pith_short_16","alias_value":"SMNPA7YDVMPE2DLL","created_at":"2026-07-05T11:25:19.878980+00:00"},{"alias_kind":"pith_short_8","alias_value":"SMNPA7YD","created_at":"2026-07-05T11:25:19.878980+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/SMNPA7YDVMPE2DLLI5EH7C4ZEZ","json":"https://pith.science/pith/SMNPA7YDVMPE2DLLI5EH7C4ZEZ.json","graph_json":"https://pith.science/api/pith-number/SMNPA7YDVMPE2DLLI5EH7C4ZEZ/graph.json","events_json":"https://pith.science/api/pith-number/SMNPA7YDVMPE2DLLI5EH7C4ZEZ/events.json","paper":"https://pith.science/paper/SMNPA7YD"},"agent_actions":{"view_html":"https://pith.science/pith/SMNPA7YDVMPE2DLLI5EH7C4ZEZ","download_json":"https://pith.science/pith/SMNPA7YDVMPE2DLLI5EH7C4ZEZ.json","view_paper":"https://pith.science/paper/SMNPA7YD","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2506.17581&json=true","fetch_graph":"https://pith.science/api/pith-number/SMNPA7YDVMPE2DLLI5EH7C4ZEZ/graph.json","fetch_events":"https://pith.science/api/pith-number/SMNPA7YDVMPE2DLLI5EH7C4ZEZ/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/SMNPA7YDVMPE2DLLI5EH7C4ZEZ/action/timestamp_anchor","attest_storage":"https://pith.science/pith/SMNPA7YDVMPE2DLLI5EH7C4ZEZ/action/storage_attestation","attest_author":"https://pith.science/pith/SMNPA7YDVMPE2DLLI5EH7C4ZEZ/action/author_attestation","sign_citation":"https://pith.science/pith/SMNPA7YDVMPE2DLLI5EH7C4ZEZ/action/citation_signature","submit_replication":"https://pith.science/pith/SMNPA7YDVMPE2DLLI5EH7C4ZEZ/action/replication_record"}},"created_at":"2026-07-05T11:25:19.878980+00:00","updated_at":"2026-07-05T11:25:19.878980+00:00"}