{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:RLKCCOK3BWR42OVHGHHCCD53AG","short_pith_number":"pith:RLKCCOK3","schema_version":"1.0","canonical_sha256":"8ad421395b0da3cd3aa731ce210fbb01957c3cdf8086b26191c9235ac78dbfa6","source":{"kind":"arxiv","id":"2410.10493","version":1},"attestation_state":"computed","paper":{"title":"Global fit to the 2HDM with generic sources of flavour violation using \\textsf{GAMBIT}","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"hep-ph","authors_text":"Andreas Crivellin, Cristian Sierra, Peter Athron, Syuhei Iguro, Tom\\'as E. Gonzalo","submitted_at":"2024-10-14T13:37:46Z","abstract_excerpt":"We perform a global statistical analysis of the two-Higgs-doublet model with generic sources of flavour violation using \\textsf{GAMBIT}. This is particularly interesting in light of deviations from the Standard Model predictions observed in $b\\to c\\tau\\bar \\nu$ and $b\\to s\\ell^+\\ell^-$ transitions as well as the indications for a charged Higgs with a mass of 130\\,GeV in top quark decays. Including all relevant constraints from precision, flavour and collider observables, we find that it is possible to simultaneously explain both the charged and neutral current $B$ anomalies. We study the impac"},"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":"2410.10493","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"hep-ph","submitted_at":"2024-10-14T13:37:46Z","cross_cats_sorted":[],"title_canon_sha256":"a24c1f373300ee1f4ddbf91d55f0c241301ba1fe2f3829166c8bd19951d49a2f","abstract_canon_sha256":"9bef4ad3d057089359e176ae64af4a32c1e7e0d1751d788c16f820b22b45f3c4"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T09:40:20.117328Z","signature_b64":"R2sFeLqSLrPK6tcmP3fZWMD/LQBrmKHm5+t+0u/nIiBM+F+pY75jFbKldw+Zh1g3wJsPdOSj9E0E/frhSpspAw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"8ad421395b0da3cd3aa731ce210fbb01957c3cdf8086b26191c9235ac78dbfa6","last_reissued_at":"2026-07-05T09:40:20.116807Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T09:40:20.116807Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Global fit to the 2HDM with generic sources of flavour violation using \\textsf{GAMBIT}","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"hep-ph","authors_text":"Andreas Crivellin, Cristian Sierra, Peter Athron, Syuhei Iguro, Tom\\'as E. Gonzalo","submitted_at":"2024-10-14T13:37:46Z","abstract_excerpt":"We perform a global statistical analysis of the two-Higgs-doublet model with generic sources of flavour violation using \\textsf{GAMBIT}. This is particularly interesting in light of deviations from the Standard Model predictions observed in $b\\to c\\tau\\bar \\nu$ and $b\\to s\\ell^+\\ell^-$ transitions as well as the indications for a charged Higgs with a mass of 130\\,GeV in top quark decays. Including all relevant constraints from precision, flavour and collider observables, we find that it is possible to simultaneously explain both the charged and neutral current $B$ anomalies. We study the impac"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2410.10493","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2410.10493/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"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":"2410.10493","created_at":"2026-07-05T09:40:20.116863+00:00"},{"alias_kind":"arxiv_version","alias_value":"2410.10493v1","created_at":"2026-07-05T09:40:20.116863+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2410.10493","created_at":"2026-07-05T09:40:20.116863+00:00"},{"alias_kind":"pith_short_12","alias_value":"RLKCCOK3BWR4","created_at":"2026-07-05T09:40:20.116863+00:00"},{"alias_kind":"pith_short_16","alias_value":"RLKCCOK3BWR42OVH","created_at":"2026-07-05T09:40:20.116863+00:00"},{"alias_kind":"pith_short_8","alias_value":"RLKCCOK3","created_at":"2026-07-05T09:40:20.116863+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":2,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2607.02276","citing_title":"A Comprehensive Analysis of $B_s \\to D_s^{**}\\ell\\nu_\\ell$ Decays Within and Beyond the Standard Model","ref_index":42,"is_internal_anchor":false},{"citing_arxiv_id":"2509.08043","citing_title":"Testing Viability of Benchmark Dark Matter Models for the Galactic Center Excess","ref_index":96,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/RLKCCOK3BWR42OVHGHHCCD53AG","json":"https://pith.science/pith/RLKCCOK3BWR42OVHGHHCCD53AG.json","graph_json":"https://pith.science/api/pith-number/RLKCCOK3BWR42OVHGHHCCD53AG/graph.json","events_json":"https://pith.science/api/pith-number/RLKCCOK3BWR42OVHGHHCCD53AG/events.json","paper":"https://pith.science/paper/RLKCCOK3"},"agent_actions":{"view_html":"https://pith.science/pith/RLKCCOK3BWR42OVHGHHCCD53AG","download_json":"https://pith.science/pith/RLKCCOK3BWR42OVHGHHCCD53AG.json","view_paper":"https://pith.science/paper/RLKCCOK3","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2410.10493&json=true","fetch_graph":"https://pith.science/api/pith-number/RLKCCOK3BWR42OVHGHHCCD53AG/graph.json","fetch_events":"https://pith.science/api/pith-number/RLKCCOK3BWR42OVHGHHCCD53AG/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/RLKCCOK3BWR42OVHGHHCCD53AG/action/timestamp_anchor","attest_storage":"https://pith.science/pith/RLKCCOK3BWR42OVHGHHCCD53AG/action/storage_attestation","attest_author":"https://pith.science/pith/RLKCCOK3BWR42OVHGHHCCD53AG/action/author_attestation","sign_citation":"https://pith.science/pith/RLKCCOK3BWR42OVHGHHCCD53AG/action/citation_signature","submit_replication":"https://pith.science/pith/RLKCCOK3BWR42OVHGHHCCD53AG/action/replication_record"}},"created_at":"2026-07-05T09:40:20.116863+00:00","updated_at":"2026-07-05T09:40:20.116863+00:00"}