{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:AWNFIQCKTQQ7HADAHPYQKY7XJ6","short_pith_number":"pith:AWNFIQCK","schema_version":"1.0","canonical_sha256":"059a54404a9c21f380603bf10563f74f8ad8dc05090eb06d48a9bcdd6309c7aa","source":{"kind":"arxiv","id":"2405.02482","version":2},"attestation_state":"computed","paper":{"title":"Solar Neutrinos in Cryogenic Detectors","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"hep-ph","authors_text":"A. Bento, A. Bertolini, A. Garai, A. Langenk\\\"amper, B. Mauri, D. Fuchs, D. Hauff, F. Dominsky, F. Petricca, F. Pr\\\"obst, F. Pucci, L. Canonica, L. Stodolsky, M. Mancuso, N. Ferreiro Iachellini, S. Di Lorenzo","submitted_at":"2024-05-03T21:13:11Z","abstract_excerpt":"Coherent elastic neutrino-nucleus scattering (CE$\\nu$NS) poses an irreducible background in the search for dark matter-nucleus elastic scatterings, which is commonly known as the neutrino floor. As direct dark matter search experiments keep improving their sensitivity into so far unexplored regions, they face the challenge of approaching this neutrino floor. A precise description of the CE$\\nu$NS signal is therefore crucial for the description of backgrounds for future DM searches. In this work we discuss the scenario of detecting neutrinos in low-threshold, high-exposure cryogenic solid state"},"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":"2405.02482","kind":"arxiv","version":2},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"hep-ph","submitted_at":"2024-05-03T21:13:11Z","cross_cats_sorted":["astro-ph.CO"],"title_canon_sha256":"dea04d281c4b5d666fe3511ce1bd3bf1f868cd38d2e21d5f3e881800b44ffb46","abstract_canon_sha256":"c29bf3711b17476b1414e091c24fad1a4f0efeeee5edc6ad13bfb6494cb3d163"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T09:23:33.161557Z","signature_b64":"8x2kbwJPWEa7Q0yfRG7DXhG+vERE2JLcK1Eoz75YktLuEfFtPsvBOq1fgkRZ1k9Jf08WnlWnnxD2y9w6YbBPCg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"059a54404a9c21f380603bf10563f74f8ad8dc05090eb06d48a9bcdd6309c7aa","last_reissued_at":"2026-07-05T09:23:33.161100Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T09:23:33.161100Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Solar Neutrinos in Cryogenic Detectors","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"hep-ph","authors_text":"A. Bento, A. Bertolini, A. Garai, A. Langenk\\\"amper, B. Mauri, D. Fuchs, D. Hauff, F. Dominsky, F. Petricca, F. Pr\\\"obst, F. Pucci, L. Canonica, L. Stodolsky, M. Mancuso, N. Ferreiro Iachellini, S. Di Lorenzo","submitted_at":"2024-05-03T21:13:11Z","abstract_excerpt":"Coherent elastic neutrino-nucleus scattering (CE$\\nu$NS) poses an irreducible background in the search for dark matter-nucleus elastic scatterings, which is commonly known as the neutrino floor. As direct dark matter search experiments keep improving their sensitivity into so far unexplored regions, they face the challenge of approaching this neutrino floor. A precise description of the CE$\\nu$NS signal is therefore crucial for the description of backgrounds for future DM searches. In this work we discuss the scenario of detecting neutrinos in low-threshold, high-exposure cryogenic solid state"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2405.02482","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/2405.02482/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":"2405.02482","created_at":"2026-07-05T09:23:33.161157+00:00"},{"alias_kind":"arxiv_version","alias_value":"2405.02482v2","created_at":"2026-07-05T09:23:33.161157+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2405.02482","created_at":"2026-07-05T09:23:33.161157+00:00"},{"alias_kind":"pith_short_12","alias_value":"AWNFIQCKTQQ7","created_at":"2026-07-05T09:23:33.161157+00:00"},{"alias_kind":"pith_short_16","alias_value":"AWNFIQCKTQQ7HADA","created_at":"2026-07-05T09:23:33.161157+00:00"},{"alias_kind":"pith_short_8","alias_value":"AWNFIQCK","created_at":"2026-07-05T09:23:33.161157+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2505.01183","citing_title":"The CRESST experiment: towards the next-generation of sub-GeV direct dark matter detection","ref_index":68,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/AWNFIQCKTQQ7HADAHPYQKY7XJ6","json":"https://pith.science/pith/AWNFIQCKTQQ7HADAHPYQKY7XJ6.json","graph_json":"https://pith.science/api/pith-number/AWNFIQCKTQQ7HADAHPYQKY7XJ6/graph.json","events_json":"https://pith.science/api/pith-number/AWNFIQCKTQQ7HADAHPYQKY7XJ6/events.json","paper":"https://pith.science/paper/AWNFIQCK"},"agent_actions":{"view_html":"https://pith.science/pith/AWNFIQCKTQQ7HADAHPYQKY7XJ6","download_json":"https://pith.science/pith/AWNFIQCKTQQ7HADAHPYQKY7XJ6.json","view_paper":"https://pith.science/paper/AWNFIQCK","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2405.02482&json=true","fetch_graph":"https://pith.science/api/pith-number/AWNFIQCKTQQ7HADAHPYQKY7XJ6/graph.json","fetch_events":"https://pith.science/api/pith-number/AWNFIQCKTQQ7HADAHPYQKY7XJ6/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/AWNFIQCKTQQ7HADAHPYQKY7XJ6/action/timestamp_anchor","attest_storage":"https://pith.science/pith/AWNFIQCKTQQ7HADAHPYQKY7XJ6/action/storage_attestation","attest_author":"https://pith.science/pith/AWNFIQCKTQQ7HADAHPYQKY7XJ6/action/author_attestation","sign_citation":"https://pith.science/pith/AWNFIQCKTQQ7HADAHPYQKY7XJ6/action/citation_signature","submit_replication":"https://pith.science/pith/AWNFIQCKTQQ7HADAHPYQKY7XJ6/action/replication_record"}},"created_at":"2026-07-05T09:23:33.161157+00:00","updated_at":"2026-07-05T09:23:33.161157+00:00"}