{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2018:SFI5Z574MZO2H46JZQFQ6R722X","short_pith_number":"pith:SFI5Z574","schema_version":"1.0","canonical_sha256":"9151dcf7fc665da3f3c9cc0b0f47fad5f417f9d8971a2d6ec2c5a37c732c397a","source":{"kind":"arxiv","id":"1803.04686","version":1},"attestation_state":"computed","paper":{"title":"Current status and desired accuracy of the isotopic production cross sections relevant to astrophysics of cosmic rays I. Li, Be, B, C, N","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-ex","hep-th","nucl-ex","nucl-th"],"primary_cat":"astro-ph.HE","authors_text":"David Maurin, Igor V. Moskalenko, Michael Unger, Yoann Genolini","submitted_at":"2018-03-13T08:59:44Z","abstract_excerpt":"The accuracy of the current generation of cosmic-ray (CR) experiments, such as AMS-02, PAMELA, CALET, and ISS-CREAM, is now reaching $\\sim$1--3\\% in a wide range in energy per nucleon from GeV/n to multi-TeV/n. Their correct interpretation could potentially lead to discoveries of new physics and subtle effects that were unthinkable just a decade ago. However, a major obstacle in doing so is the current uncertainty in the isotopic production cross sections that can be as high as 20--50\\% or even larger in some cases. While there is a recently reached consensus in the astrophysics community that"},"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":"1803.04686","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2018-03-13T08:59:44Z","cross_cats_sorted":["hep-ex","hep-th","nucl-ex","nucl-th"],"title_canon_sha256":"f56ef883a75ec61177d12245918f15ede21e1080ebac6de35d816102e97b2ffd","abstract_canon_sha256":"b6817b6bcd5742c689e0cc8c8d650a45aff885015a44eb17cc9fd5a4a442cbe1"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:04:49.529832Z","signature_b64":"CjXOTE/+nw1iGOh2B742jxs4Q8eqmlLUR+MM5UuLi7qBllZQFpIuYUsBV6XJ0+BhOy1MM2nj4gEiZvskyu3KCg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"9151dcf7fc665da3f3c9cc0b0f47fad5f417f9d8971a2d6ec2c5a37c732c397a","last_reissued_at":"2026-05-18T00:04:49.529149Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:04:49.529149Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Current status and desired accuracy of the isotopic production cross sections relevant to astrophysics of cosmic rays I. Li, Be, B, C, N","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-ex","hep-th","nucl-ex","nucl-th"],"primary_cat":"astro-ph.HE","authors_text":"David Maurin, Igor V. Moskalenko, Michael Unger, Yoann Genolini","submitted_at":"2018-03-13T08:59:44Z","abstract_excerpt":"The accuracy of the current generation of cosmic-ray (CR) experiments, such as AMS-02, PAMELA, CALET, and ISS-CREAM, is now reaching $\\sim$1--3\\% in a wide range in energy per nucleon from GeV/n to multi-TeV/n. Their correct interpretation could potentially lead to discoveries of new physics and subtle effects that were unthinkable just a decade ago. However, a major obstacle in doing so is the current uncertainty in the isotopic production cross sections that can be as high as 20--50\\% or even larger in some cases. While there is a recently reached consensus in the astrophysics community that"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1803.04686","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":"1803.04686","created_at":"2026-05-18T00:04:49.529243+00:00"},{"alias_kind":"arxiv_version","alias_value":"1803.04686v1","created_at":"2026-05-18T00:04:49.529243+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1803.04686","created_at":"2026-05-18T00:04:49.529243+00:00"},{"alias_kind":"pith_short_12","alias_value":"SFI5Z574MZO2","created_at":"2026-05-18T12:32:53.628368+00:00"},{"alias_kind":"pith_short_16","alias_value":"SFI5Z574MZO2H46J","created_at":"2026-05-18T12:32:53.628368+00:00"},{"alias_kind":"pith_short_8","alias_value":"SFI5Z574","created_at":"2026-05-18T12:32:53.628368+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/SFI5Z574MZO2H46JZQFQ6R722X","json":"https://pith.science/pith/SFI5Z574MZO2H46JZQFQ6R722X.json","graph_json":"https://pith.science/api/pith-number/SFI5Z574MZO2H46JZQFQ6R722X/graph.json","events_json":"https://pith.science/api/pith-number/SFI5Z574MZO2H46JZQFQ6R722X/events.json","paper":"https://pith.science/paper/SFI5Z574"},"agent_actions":{"view_html":"https://pith.science/pith/SFI5Z574MZO2H46JZQFQ6R722X","download_json":"https://pith.science/pith/SFI5Z574MZO2H46JZQFQ6R722X.json","view_paper":"https://pith.science/paper/SFI5Z574","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1803.04686&json=true","fetch_graph":"https://pith.science/api/pith-number/SFI5Z574MZO2H46JZQFQ6R722X/graph.json","fetch_events":"https://pith.science/api/pith-number/SFI5Z574MZO2H46JZQFQ6R722X/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/SFI5Z574MZO2H46JZQFQ6R722X/action/timestamp_anchor","attest_storage":"https://pith.science/pith/SFI5Z574MZO2H46JZQFQ6R722X/action/storage_attestation","attest_author":"https://pith.science/pith/SFI5Z574MZO2H46JZQFQ6R722X/action/author_attestation","sign_citation":"https://pith.science/pith/SFI5Z574MZO2H46JZQFQ6R722X/action/citation_signature","submit_replication":"https://pith.science/pith/SFI5Z574MZO2H46JZQFQ6R722X/action/replication_record"}},"created_at":"2026-05-18T00:04:49.529243+00:00","updated_at":"2026-05-18T00:04:49.529243+00:00"}