{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2011:RGKI5EQIDUXOQZYZX77NCPVDSR","short_pith_number":"pith:RGKI5EQI","schema_version":"1.0","canonical_sha256":"89948e92081d2ee86719bffed13ea3946f2255480201ef4d93c10fa157843cf7","source":{"kind":"arxiv","id":"1101.5596","version":3},"attestation_state":"computed","paper":{"title":"Constraints from the first LHC data on hadronic event generators for ultra-high energy cosmic-ray physics","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-ex","hep-ph"],"primary_cat":"astro-ph.HE","authors_text":"David d'Enterria, Klaus Werner, Ralph Engel, Sergey Ostapchenko, Tanguy Pierog","submitted_at":"2011-01-28T18:10:59Z","abstract_excerpt":"The determination of the primary energy and mass of ultra-high-energy cosmic-rays (UHECR) generating extensive air-showers in the Earth's atmosphere, relies on the detailed modeling of hadronic multiparticle production at center-of-mass (c.m.) collision energies up to two orders of magnitude higher than those studied at particle colliders. The first Large Hadron Collider (LHC) data have extended by more than a factor of three the c.m. energies in which we have direct proton-proton measurements available to compare to hadronic models. In this work we compare LHC results on inclusive particle pr"},"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":"1101.5596","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2011-01-28T18:10:59Z","cross_cats_sorted":["hep-ex","hep-ph"],"title_canon_sha256":"c628f6a30a803747d22cb7d6e0aa25278368b8584331806f4d97df2b43d2a560","abstract_canon_sha256":"41636748dbccaa4c9ad106d59c7cae821a8b331662358d91a4bfc966c51ac772"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:03:20.734585Z","signature_b64":"4maIHrI/yZ1UkmQXwp5vEC1213ByvlUTJvwK/tRRsZrZCC1LVqiyX58Bt33VAp+jkPIf0uEnBENn8ytdRGEPDA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"89948e92081d2ee86719bffed13ea3946f2255480201ef4d93c10fa157843cf7","last_reissued_at":"2026-05-18T02:03:20.734099Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:03:20.734099Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Constraints from the first LHC data on hadronic event generators for ultra-high energy cosmic-ray physics","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-ex","hep-ph"],"primary_cat":"astro-ph.HE","authors_text":"David d'Enterria, Klaus Werner, Ralph Engel, Sergey Ostapchenko, Tanguy Pierog","submitted_at":"2011-01-28T18:10:59Z","abstract_excerpt":"The determination of the primary energy and mass of ultra-high-energy cosmic-rays (UHECR) generating extensive air-showers in the Earth's atmosphere, relies on the detailed modeling of hadronic multiparticle production at center-of-mass (c.m.) collision energies up to two orders of magnitude higher than those studied at particle colliders. The first Large Hadron Collider (LHC) data have extended by more than a factor of three the c.m. energies in which we have direct proton-proton measurements available to compare to hadronic models. In this work we compare LHC results on inclusive particle pr"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1101.5596","kind":"arxiv","version":3},"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":"1101.5596","created_at":"2026-05-18T02:03:20.734163+00:00"},{"alias_kind":"arxiv_version","alias_value":"1101.5596v3","created_at":"2026-05-18T02:03:20.734163+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1101.5596","created_at":"2026-05-18T02:03:20.734163+00:00"},{"alias_kind":"pith_short_12","alias_value":"RGKI5EQIDUXO","created_at":"2026-05-18T12:26:41.206345+00:00"},{"alias_kind":"pith_short_16","alias_value":"RGKI5EQIDUXOQZYZ","created_at":"2026-05-18T12:26:41.206345+00:00"},{"alias_kind":"pith_short_8","alias_value":"RGKI5EQI","created_at":"2026-05-18T12:26:41.206345+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2604.05512","citing_title":"Measurement of charged-particle production in $\\sqrt{s_\\text{NN}}=9.62$ TeV proton-oxygen collisions as a probe of cosmic-ray air showers with the ATLAS detector","ref_index":33,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/RGKI5EQIDUXOQZYZX77NCPVDSR","json":"https://pith.science/pith/RGKI5EQIDUXOQZYZX77NCPVDSR.json","graph_json":"https://pith.science/api/pith-number/RGKI5EQIDUXOQZYZX77NCPVDSR/graph.json","events_json":"https://pith.science/api/pith-number/RGKI5EQIDUXOQZYZX77NCPVDSR/events.json","paper":"https://pith.science/paper/RGKI5EQI"},"agent_actions":{"view_html":"https://pith.science/pith/RGKI5EQIDUXOQZYZX77NCPVDSR","download_json":"https://pith.science/pith/RGKI5EQIDUXOQZYZX77NCPVDSR.json","view_paper":"https://pith.science/paper/RGKI5EQI","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1101.5596&json=true","fetch_graph":"https://pith.science/api/pith-number/RGKI5EQIDUXOQZYZX77NCPVDSR/graph.json","fetch_events":"https://pith.science/api/pith-number/RGKI5EQIDUXOQZYZX77NCPVDSR/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/RGKI5EQIDUXOQZYZX77NCPVDSR/action/timestamp_anchor","attest_storage":"https://pith.science/pith/RGKI5EQIDUXOQZYZX77NCPVDSR/action/storage_attestation","attest_author":"https://pith.science/pith/RGKI5EQIDUXOQZYZX77NCPVDSR/action/author_attestation","sign_citation":"https://pith.science/pith/RGKI5EQIDUXOQZYZX77NCPVDSR/action/citation_signature","submit_replication":"https://pith.science/pith/RGKI5EQIDUXOQZYZX77NCPVDSR/action/replication_record"}},"created_at":"2026-05-18T02:03:20.734163+00:00","updated_at":"2026-05-18T02:03:20.734163+00:00"}