{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2015:OJ2OR3IVOPZHXNNQTU3RMVXUGC","short_pith_number":"pith:OJ2OR3IV","schema_version":"1.0","canonical_sha256":"7274e8ed1573f27bb5b09d371656f43089197dfa4779ea5e4dcbb2edd021e81e","source":{"kind":"arxiv","id":"1507.06349","version":4},"attestation_state":"computed","paper":{"title":"Computer tools in particle physics","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-ex"],"primary_cat":"hep-ph","authors_text":"Avelino Vicente","submitted_at":"2015-07-22T22:24:14Z","abstract_excerpt":"The field of particle physics is living very exciting times with a plethora of experiments looking for new physics in complementary ways. This has made increasingly necessary to obtain precise predictions in new physics models in order to be ready for a discovery that might be just around the corner. However, analyzing new models and studying their phenomenology can be really challenging. Computing mass matrices, interaction vertices and decay rates is already a tremendous task. In addition, obtaining predictions for the dark matter relic density and its detection prospects, computing flavor o"},"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":"1507.06349","kind":"arxiv","version":4},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2015-07-22T22:24:14Z","cross_cats_sorted":["hep-ex"],"title_canon_sha256":"adb498e4453d49bb63e8af09ab3146b48f4e13b7e7b7cf0cb41ccfa4242ac0a6","abstract_canon_sha256":"600dc0c0d1200551d52ad364defd339648e83674914898317394e71799d122b1"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:44:18.117654Z","signature_b64":"ZKLs6BTPwis0Sqyd1ffoPexarOIucmMTfoTAL67uqnsbLbvAg0KCTomDOHvR+5t/mdKwawShpViLZ+kyepPNAQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"7274e8ed1573f27bb5b09d371656f43089197dfa4779ea5e4dcbb2edd021e81e","last_reissued_at":"2026-05-18T00:44:18.117144Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:44:18.117144Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Computer tools in particle physics","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-ex"],"primary_cat":"hep-ph","authors_text":"Avelino Vicente","submitted_at":"2015-07-22T22:24:14Z","abstract_excerpt":"The field of particle physics is living very exciting times with a plethora of experiments looking for new physics in complementary ways. This has made increasingly necessary to obtain precise predictions in new physics models in order to be ready for a discovery that might be just around the corner. However, analyzing new models and studying their phenomenology can be really challenging. Computing mass matrices, interaction vertices and decay rates is already a tremendous task. In addition, obtaining predictions for the dark matter relic density and its detection prospects, computing flavor o"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1507.06349","kind":"arxiv","version":4},"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":"1507.06349","created_at":"2026-05-18T00:44:18.117237+00:00"},{"alias_kind":"arxiv_version","alias_value":"1507.06349v4","created_at":"2026-05-18T00:44:18.117237+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1507.06349","created_at":"2026-05-18T00:44:18.117237+00:00"},{"alias_kind":"pith_short_12","alias_value":"OJ2OR3IVOPZH","created_at":"2026-05-18T12:29:34.919912+00:00"},{"alias_kind":"pith_short_16","alias_value":"OJ2OR3IVOPZHXNNQ","created_at":"2026-05-18T12:29:34.919912+00:00"},{"alias_kind":"pith_short_8","alias_value":"OJ2OR3IV","created_at":"2026-05-18T12:29:34.919912+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":3,"internal_anchor_count":2,"sample":[{"citing_arxiv_id":"2409.16961","citing_title":"Correlative study of flavor anomalies and dark matter in the light of scalar leptoquark","ref_index":66,"is_internal_anchor":true},{"citing_arxiv_id":"2605.05312","citing_title":"Monochromatic neutrinos from scotogenic dark matter","ref_index":20,"is_internal_anchor":true},{"citing_arxiv_id":"2605.05312","citing_title":"Monochromatic neutrinos from scotogenic dark matter","ref_index":20,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/OJ2OR3IVOPZHXNNQTU3RMVXUGC","json":"https://pith.science/pith/OJ2OR3IVOPZHXNNQTU3RMVXUGC.json","graph_json":"https://pith.science/api/pith-number/OJ2OR3IVOPZHXNNQTU3RMVXUGC/graph.json","events_json":"https://pith.science/api/pith-number/OJ2OR3IVOPZHXNNQTU3RMVXUGC/events.json","paper":"https://pith.science/paper/OJ2OR3IV"},"agent_actions":{"view_html":"https://pith.science/pith/OJ2OR3IVOPZHXNNQTU3RMVXUGC","download_json":"https://pith.science/pith/OJ2OR3IVOPZHXNNQTU3RMVXUGC.json","view_paper":"https://pith.science/paper/OJ2OR3IV","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1507.06349&json=true","fetch_graph":"https://pith.science/api/pith-number/OJ2OR3IVOPZHXNNQTU3RMVXUGC/graph.json","fetch_events":"https://pith.science/api/pith-number/OJ2OR3IVOPZHXNNQTU3RMVXUGC/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/OJ2OR3IVOPZHXNNQTU3RMVXUGC/action/timestamp_anchor","attest_storage":"https://pith.science/pith/OJ2OR3IVOPZHXNNQTU3RMVXUGC/action/storage_attestation","attest_author":"https://pith.science/pith/OJ2OR3IVOPZHXNNQTU3RMVXUGC/action/author_attestation","sign_citation":"https://pith.science/pith/OJ2OR3IVOPZHXNNQTU3RMVXUGC/action/citation_signature","submit_replication":"https://pith.science/pith/OJ2OR3IVOPZHXNNQTU3RMVXUGC/action/replication_record"}},"created_at":"2026-05-18T00:44:18.117237+00:00","updated_at":"2026-05-18T00:44:18.117237+00:00"}