{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2025:FTMEBSJJKHABA4ZIVVORPDRTTI","short_pith_number":"pith:FTMEBSJJ","schema_version":"1.0","canonical_sha256":"2cd840c92951c0107328ad5d178e339a05b53170a072bc7f4466ff198f9e45b7","source":{"kind":"arxiv","id":"2507.07397","version":1},"attestation_state":"computed","paper":{"title":"LIQUIDating the Gallium Anomaly","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"hep-ph","authors_text":"Garv Chauhan, Patrick Huber","submitted_at":"2025-07-10T03:28:01Z","abstract_excerpt":"The gallium anomaly has a global significance of greater than $5\\sigma$. Most viable BSM solutions quickly run into strong tensions with reactor and solar neutrino data. We propose to use indium (${}^{115}\\text{In}$) as a target as it offers a low threshold and reasonably high cross section. The neutrino-indium charged current cross section can be calibrated using the well-constrained solar ${}^{7}\\text{Be}$ neutrino flux that lies very close in energy to the ${}^{51}\\text{Cr}$ neutrino lines. The triple coincidence provided by ${}^{115}\\text{In}$ neutrino capture can be fully exploited by an "},"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":"2507.07397","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"hep-ph","submitted_at":"2025-07-10T03:28:01Z","cross_cats_sorted":[],"title_canon_sha256":"f878bf1dc3b9e8f3f493febbd74f3f9a3ffeb707603eb6870888063dad02a8b8","abstract_canon_sha256":"5e0361f931670e2757935cde43bc127811384c0f9d04ac69e7ecd78f2beb64dc"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T11:34:57.152027Z","signature_b64":"tUHQzxjqmHnmeEtzGzmE7CG/6VvjEbWHeiAF4UbG8CkfTp8UkAD7NekJV6SWd66qRdRwlEiyr416X+6UiJJdCQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"2cd840c92951c0107328ad5d178e339a05b53170a072bc7f4466ff198f9e45b7","last_reissued_at":"2026-07-05T11:34:57.151450Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T11:34:57.151450Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"LIQUIDating the Gallium Anomaly","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"hep-ph","authors_text":"Garv Chauhan, Patrick Huber","submitted_at":"2025-07-10T03:28:01Z","abstract_excerpt":"The gallium anomaly has a global significance of greater than $5\\sigma$. Most viable BSM solutions quickly run into strong tensions with reactor and solar neutrino data. We propose to use indium (${}^{115}\\text{In}$) as a target as it offers a low threshold and reasonably high cross section. The neutrino-indium charged current cross section can be calibrated using the well-constrained solar ${}^{7}\\text{Be}$ neutrino flux that lies very close in energy to the ${}^{51}\\text{Cr}$ neutrino lines. The triple coincidence provided by ${}^{115}\\text{In}$ neutrino capture can be fully exploited by an "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2507.07397","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/2507.07397/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":"2507.07397","created_at":"2026-07-05T11:34:57.151523+00:00"},{"alias_kind":"arxiv_version","alias_value":"2507.07397v1","created_at":"2026-07-05T11:34:57.151523+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2507.07397","created_at":"2026-07-05T11:34:57.151523+00:00"},{"alias_kind":"pith_short_12","alias_value":"FTMEBSJJKHAB","created_at":"2026-07-05T11:34:57.151523+00:00"},{"alias_kind":"pith_short_16","alias_value":"FTMEBSJJKHABA4ZI","created_at":"2026-07-05T11:34:57.151523+00:00"},{"alias_kind":"pith_short_8","alias_value":"FTMEBSJJ","created_at":"2026-07-05T11:34:57.151523+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2606.30758","citing_title":"The effect of nuclear recoil on neutrino oscillations: Toward understanding of short baseline anomalies","ref_index":29,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/FTMEBSJJKHABA4ZIVVORPDRTTI","json":"https://pith.science/pith/FTMEBSJJKHABA4ZIVVORPDRTTI.json","graph_json":"https://pith.science/api/pith-number/FTMEBSJJKHABA4ZIVVORPDRTTI/graph.json","events_json":"https://pith.science/api/pith-number/FTMEBSJJKHABA4ZIVVORPDRTTI/events.json","paper":"https://pith.science/paper/FTMEBSJJ"},"agent_actions":{"view_html":"https://pith.science/pith/FTMEBSJJKHABA4ZIVVORPDRTTI","download_json":"https://pith.science/pith/FTMEBSJJKHABA4ZIVVORPDRTTI.json","view_paper":"https://pith.science/paper/FTMEBSJJ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2507.07397&json=true","fetch_graph":"https://pith.science/api/pith-number/FTMEBSJJKHABA4ZIVVORPDRTTI/graph.json","fetch_events":"https://pith.science/api/pith-number/FTMEBSJJKHABA4ZIVVORPDRTTI/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/FTMEBSJJKHABA4ZIVVORPDRTTI/action/timestamp_anchor","attest_storage":"https://pith.science/pith/FTMEBSJJKHABA4ZIVVORPDRTTI/action/storage_attestation","attest_author":"https://pith.science/pith/FTMEBSJJKHABA4ZIVVORPDRTTI/action/author_attestation","sign_citation":"https://pith.science/pith/FTMEBSJJKHABA4ZIVVORPDRTTI/action/citation_signature","submit_replication":"https://pith.science/pith/FTMEBSJJKHABA4ZIVVORPDRTTI/action/replication_record"}},"created_at":"2026-07-05T11:34:57.151523+00:00","updated_at":"2026-07-05T11:34:57.151523+00:00"}