{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2022:3VNESVAVMUA4T44L4BNW5LAY2P","short_pith_number":"pith:3VNESVAV","schema_version":"1.0","canonical_sha256":"dd5a4954156501c9f38be05b6eac18d3f7101c2ef26214c308f52db82c16a93a","source":{"kind":"arxiv","id":"2209.05223","version":2},"attestation_state":"computed","paper":{"title":"FCNC $B$ and $K$ Meson Decays with Light Bosonic Dark Matter","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["hep-ex"],"primary_cat":"hep-ph","authors_text":"German Valencia, Xiao-Dong Ma, Xiao-Gang He","submitted_at":"2022-09-12T13:12:50Z","abstract_excerpt":"We consider decays of $B$ and $K$ mesons into a pseudo-scalar or vector meson plus missing energy. Within the SM, these modes originate from flavor changing neutral current (FCNC) processes with two neutrinos in the final state. In this paper we consider the experimental upper bounds on these modes and interpret the difference between these bounds and the SM prediction as a window into new light invisible particles. In particular we consider the case where some new symmetry requires the new particles to be produced in pairs. We first construct the general low energy effective Lagrangian coupli"},"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":"2209.05223","kind":"arxiv","version":2},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"hep-ph","submitted_at":"2022-09-12T13:12:50Z","cross_cats_sorted":["hep-ex"],"title_canon_sha256":"b9424052d56f8ea726a589c02eac12395dbe944ee4070310ff08d3bef7a1189b","abstract_canon_sha256":"505af8e7c6dfa6e5c4862bb10855452369873922fb6f3f15d68ea032067501b6"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T05:52:59.915350Z","signature_b64":"Gm5oDLXYJCC03PEps/eM9SF+Lt+F8ndlNbLNI98jGUXtDLyNgd5XgOu3pdIwk47QTeH520j9sd2CW9GNdYPTAA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"dd5a4954156501c9f38be05b6eac18d3f7101c2ef26214c308f52db82c16a93a","last_reissued_at":"2026-07-05T05:52:59.914897Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T05:52:59.914897Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"FCNC $B$ and $K$ Meson Decays with Light Bosonic Dark Matter","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["hep-ex"],"primary_cat":"hep-ph","authors_text":"German Valencia, Xiao-Dong Ma, Xiao-Gang He","submitted_at":"2022-09-12T13:12:50Z","abstract_excerpt":"We consider decays of $B$ and $K$ mesons into a pseudo-scalar or vector meson plus missing energy. Within the SM, these modes originate from flavor changing neutral current (FCNC) processes with two neutrinos in the final state. In this paper we consider the experimental upper bounds on these modes and interpret the difference between these bounds and the SM prediction as a window into new light invisible particles. In particular we consider the case where some new symmetry requires the new particles to be produced in pairs. We first construct the general low energy effective Lagrangian coupli"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2209.05223","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2209.05223/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":"2209.05223","created_at":"2026-07-05T05:52:59.914956+00:00"},{"alias_kind":"arxiv_version","alias_value":"2209.05223v2","created_at":"2026-07-05T05:52:59.914956+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2209.05223","created_at":"2026-07-05T05:52:59.914956+00:00"},{"alias_kind":"pith_short_12","alias_value":"3VNESVAVMUA4","created_at":"2026-07-05T05:52:59.914956+00:00"},{"alias_kind":"pith_short_16","alias_value":"3VNESVAVMUA4T44L","created_at":"2026-07-05T05:52:59.914956+00:00"},{"alias_kind":"pith_short_8","alias_value":"3VNESVAV","created_at":"2026-07-05T05:52:59.914956+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":2,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2605.09140","citing_title":"Can a Nonstandard Invisible Pair Mimic the Michel Distribution?","ref_index":31,"is_internal_anchor":false},{"citing_arxiv_id":"2605.05947","citing_title":"Kaon Portal to Freeze-in Dark Matter","ref_index":25,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/3VNESVAVMUA4T44L4BNW5LAY2P","json":"https://pith.science/pith/3VNESVAVMUA4T44L4BNW5LAY2P.json","graph_json":"https://pith.science/api/pith-number/3VNESVAVMUA4T44L4BNW5LAY2P/graph.json","events_json":"https://pith.science/api/pith-number/3VNESVAVMUA4T44L4BNW5LAY2P/events.json","paper":"https://pith.science/paper/3VNESVAV"},"agent_actions":{"view_html":"https://pith.science/pith/3VNESVAVMUA4T44L4BNW5LAY2P","download_json":"https://pith.science/pith/3VNESVAVMUA4T44L4BNW5LAY2P.json","view_paper":"https://pith.science/paper/3VNESVAV","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2209.05223&json=true","fetch_graph":"https://pith.science/api/pith-number/3VNESVAVMUA4T44L4BNW5LAY2P/graph.json","fetch_events":"https://pith.science/api/pith-number/3VNESVAVMUA4T44L4BNW5LAY2P/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/3VNESVAVMUA4T44L4BNW5LAY2P/action/timestamp_anchor","attest_storage":"https://pith.science/pith/3VNESVAVMUA4T44L4BNW5LAY2P/action/storage_attestation","attest_author":"https://pith.science/pith/3VNESVAVMUA4T44L4BNW5LAY2P/action/author_attestation","sign_citation":"https://pith.science/pith/3VNESVAVMUA4T44L4BNW5LAY2P/action/citation_signature","submit_replication":"https://pith.science/pith/3VNESVAVMUA4T44L4BNW5LAY2P/action/replication_record"}},"created_at":"2026-07-05T05:52:59.914956+00:00","updated_at":"2026-07-05T05:52:59.914956+00:00"}