{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2011:NT66MZ56PJS2DVXZAU37EO6B6K","short_pith_number":"pith:NT66MZ56","schema_version":"1.0","canonical_sha256":"6cfde667be7a65a1d6f90537f23bc1f2afbc611d5b917e26cc1ecc43df7b245c","source":{"kind":"arxiv","id":"1102.0691","version":2},"attestation_state":"computed","paper":{"title":"Calculation of High Energy Neutrino-Nucleon Cross Sections and Uncertainties Using the MSTW Parton Distribution Functions and Implications for Future Experiments","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.IM"],"primary_cat":"hep-ph","authors_text":"Amy Connolly, David Waters, Robert S. Thorne","submitted_at":"2011-02-03T14:16:48Z","abstract_excerpt":"We present a new calculation of the cross sections for charged current (CC) and neutral current (NC) $\\nu N$ and $\\bar{\\nu} N$ interactions in the neutrino energy range $10^{4}<E_{\\nu}<10^{12}$ GeV using the most recent MSTW parton distribution functions (PDFs), MSTW 2008. We also present the associated uncertainties propagated from the PDFs, as well as parametrizations of the cross section central values, their uncertainty bounds, and the inelasticity distributions for ease of use in Monte Carlo simulations. For the latter we only provide parametrizations for energies above $10^7$ GeV. Finall"},"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":"1102.0691","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2011-02-03T14:16:48Z","cross_cats_sorted":["astro-ph.IM"],"title_canon_sha256":"853cd1e98a8a562b5b8e625b291f7cd2d9b10348a7118f567d7298aec501ec41","abstract_canon_sha256":"61943428aa1d239dccbdda4ab2733679618e6f93b2928e499af01f5d5c095c2b"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T04:15:28.295827Z","signature_b64":"FBQZwcIO2BxH13zm2Z9GyV+uJfmYfUnPTRsWMCh40SamWDRcLuKP2QpM3x+wyzCDoWb5NZmV8vvw1n7I8PViAQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"6cfde667be7a65a1d6f90537f23bc1f2afbc611d5b917e26cc1ecc43df7b245c","last_reissued_at":"2026-05-18T04:15:28.295354Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T04:15:28.295354Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Calculation of High Energy Neutrino-Nucleon Cross Sections and Uncertainties Using the MSTW Parton Distribution Functions and Implications for Future Experiments","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.IM"],"primary_cat":"hep-ph","authors_text":"Amy Connolly, David Waters, Robert S. Thorne","submitted_at":"2011-02-03T14:16:48Z","abstract_excerpt":"We present a new calculation of the cross sections for charged current (CC) and neutral current (NC) $\\nu N$ and $\\bar{\\nu} N$ interactions in the neutrino energy range $10^{4}<E_{\\nu}<10^{12}$ GeV using the most recent MSTW parton distribution functions (PDFs), MSTW 2008. We also present the associated uncertainties propagated from the PDFs, as well as parametrizations of the cross section central values, their uncertainty bounds, and the inelasticity distributions for ease of use in Monte Carlo simulations. For the latter we only provide parametrizations for energies above $10^7$ GeV. Finall"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1102.0691","kind":"arxiv","version":2},"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":"1102.0691","created_at":"2026-05-18T04:15:28.295441+00:00"},{"alias_kind":"arxiv_version","alias_value":"1102.0691v2","created_at":"2026-05-18T04:15:28.295441+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1102.0691","created_at":"2026-05-18T04:15:28.295441+00:00"},{"alias_kind":"pith_short_12","alias_value":"NT66MZ56PJS2","created_at":"2026-05-18T12:26:37.096874+00:00"},{"alias_kind":"pith_short_16","alias_value":"NT66MZ56PJS2DVXZ","created_at":"2026-05-18T12:26:37.096874+00:00"},{"alias_kind":"pith_short_8","alias_value":"NT66MZ56","created_at":"2026-05-18T12:26:37.096874+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":2,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2601.11203","citing_title":"Little Red Dots as Hidden Neutrino Sources","ref_index":94,"is_internal_anchor":true},{"citing_arxiv_id":"2605.04268","citing_title":"Sensitivity of the As-Built Askaryan Radio Array to Ultra-High Energy Neutrinos","ref_index":31,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/NT66MZ56PJS2DVXZAU37EO6B6K","json":"https://pith.science/pith/NT66MZ56PJS2DVXZAU37EO6B6K.json","graph_json":"https://pith.science/api/pith-number/NT66MZ56PJS2DVXZAU37EO6B6K/graph.json","events_json":"https://pith.science/api/pith-number/NT66MZ56PJS2DVXZAU37EO6B6K/events.json","paper":"https://pith.science/paper/NT66MZ56"},"agent_actions":{"view_html":"https://pith.science/pith/NT66MZ56PJS2DVXZAU37EO6B6K","download_json":"https://pith.science/pith/NT66MZ56PJS2DVXZAU37EO6B6K.json","view_paper":"https://pith.science/paper/NT66MZ56","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1102.0691&json=true","fetch_graph":"https://pith.science/api/pith-number/NT66MZ56PJS2DVXZAU37EO6B6K/graph.json","fetch_events":"https://pith.science/api/pith-number/NT66MZ56PJS2DVXZAU37EO6B6K/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/NT66MZ56PJS2DVXZAU37EO6B6K/action/timestamp_anchor","attest_storage":"https://pith.science/pith/NT66MZ56PJS2DVXZAU37EO6B6K/action/storage_attestation","attest_author":"https://pith.science/pith/NT66MZ56PJS2DVXZAU37EO6B6K/action/author_attestation","sign_citation":"https://pith.science/pith/NT66MZ56PJS2DVXZAU37EO6B6K/action/citation_signature","submit_replication":"https://pith.science/pith/NT66MZ56PJS2DVXZAU37EO6B6K/action/replication_record"}},"created_at":"2026-05-18T04:15:28.295441+00:00","updated_at":"2026-05-18T04:15:28.295441+00:00"}