{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:LKTDNWGEX7LV3MDRGQJQ2XIIL4","short_pith_number":"pith:LKTDNWGE","schema_version":"1.0","canonical_sha256":"5aa636d8c4bfd75db07134130d5d085f099f54859d2f440c4cf441caf2ab1488","source":{"kind":"arxiv","id":"1712.04378","version":1},"attestation_state":"computed","paper":{"title":"PArthENoPE reloaded","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-ph"],"primary_cat":"astro-ph.CO","authors_text":"G. Mangano, G. Miele, O. Pisanti, P.F. de Salas, R. Consiglio, S. Pastor","submitted_at":"2017-12-12T16:31:00Z","abstract_excerpt":"We describe the main features of a new and updated version of the program PArthENoPE, which computes the abundances of light elements produced during Big Bang Nucleosynthesis. As the previous first release in 2008, the new one, PArthENoPE 2.0, will be soon publicly available and distributed from the code site, http://parthenope.na.infn.it. Apart from minor changes, which will be also detailed, the main improvements are as follows. The powerful, but not freely accessible, NAG routines have been substituted by ODEPACK libraries, without any significant loss in precision. Moreover, we have develo"},"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":"1712.04378","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2017-12-12T16:31:00Z","cross_cats_sorted":["hep-ph"],"title_canon_sha256":"cdbe896677cd9ab3c79c3264fa9fc567f6590631d572f4772416355a1b2ad528","abstract_canon_sha256":"18f1c1708f64ba78e515edf42f78e5c9be21b5c30753856daddbafb722de4c9e"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:07:18.121940Z","signature_b64":"JBnlAu5DOhfLFV0dCwZQNIybOEAy/1Zn2DIGfCYp41V60I3UoROAyM8ET6qqKfokwceGii8eCnBX+Mrb4CPlBg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"5aa636d8c4bfd75db07134130d5d085f099f54859d2f440c4cf441caf2ab1488","last_reissued_at":"2026-05-18T00:07:18.121190Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:07:18.121190Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"PArthENoPE reloaded","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-ph"],"primary_cat":"astro-ph.CO","authors_text":"G. Mangano, G. Miele, O. Pisanti, P.F. de Salas, R. Consiglio, S. Pastor","submitted_at":"2017-12-12T16:31:00Z","abstract_excerpt":"We describe the main features of a new and updated version of the program PArthENoPE, which computes the abundances of light elements produced during Big Bang Nucleosynthesis. As the previous first release in 2008, the new one, PArthENoPE 2.0, will be soon publicly available and distributed from the code site, http://parthenope.na.infn.it. Apart from minor changes, which will be also detailed, the main improvements are as follows. The powerful, but not freely accessible, NAG routines have been substituted by ODEPACK libraries, without any significant loss in precision. Moreover, we have develo"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1712.04378","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":"1712.04378","created_at":"2026-05-18T00:07:18.121300+00:00"},{"alias_kind":"arxiv_version","alias_value":"1712.04378v1","created_at":"2026-05-18T00:07:18.121300+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1712.04378","created_at":"2026-05-18T00:07:18.121300+00:00"},{"alias_kind":"pith_short_12","alias_value":"LKTDNWGEX7LV","created_at":"2026-05-18T12:31:28.150371+00:00"},{"alias_kind":"pith_short_16","alias_value":"LKTDNWGEX7LV3MDR","created_at":"2026-05-18T12:31:28.150371+00:00"},{"alias_kind":"pith_short_8","alias_value":"LKTDNWGE","created_at":"2026-05-18T12:31:28.150371+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":2,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2507.23354","citing_title":"Consistent $N_{\\rm eff}$ fitting in big bang nucleosynthesis analysis","ref_index":42,"is_internal_anchor":true},{"citing_arxiv_id":"2604.13535","citing_title":"Double the axions, half the tension: multi-field early dark energy eases the Hubble tension","ref_index":194,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/LKTDNWGEX7LV3MDRGQJQ2XIIL4","json":"https://pith.science/pith/LKTDNWGEX7LV3MDRGQJQ2XIIL4.json","graph_json":"https://pith.science/api/pith-number/LKTDNWGEX7LV3MDRGQJQ2XIIL4/graph.json","events_json":"https://pith.science/api/pith-number/LKTDNWGEX7LV3MDRGQJQ2XIIL4/events.json","paper":"https://pith.science/paper/LKTDNWGE"},"agent_actions":{"view_html":"https://pith.science/pith/LKTDNWGEX7LV3MDRGQJQ2XIIL4","download_json":"https://pith.science/pith/LKTDNWGEX7LV3MDRGQJQ2XIIL4.json","view_paper":"https://pith.science/paper/LKTDNWGE","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1712.04378&json=true","fetch_graph":"https://pith.science/api/pith-number/LKTDNWGEX7LV3MDRGQJQ2XIIL4/graph.json","fetch_events":"https://pith.science/api/pith-number/LKTDNWGEX7LV3MDRGQJQ2XIIL4/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/LKTDNWGEX7LV3MDRGQJQ2XIIL4/action/timestamp_anchor","attest_storage":"https://pith.science/pith/LKTDNWGEX7LV3MDRGQJQ2XIIL4/action/storage_attestation","attest_author":"https://pith.science/pith/LKTDNWGEX7LV3MDRGQJQ2XIIL4/action/author_attestation","sign_citation":"https://pith.science/pith/LKTDNWGEX7LV3MDRGQJQ2XIIL4/action/citation_signature","submit_replication":"https://pith.science/pith/LKTDNWGEX7LV3MDRGQJQ2XIIL4/action/replication_record"}},"created_at":"2026-05-18T00:07:18.121300+00:00","updated_at":"2026-05-18T00:07:18.121300+00:00"}