{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:WZQ3SEM2GMEHRCVXVVQHJEVJPY","short_pith_number":"pith:WZQ3SEM2","schema_version":"1.0","canonical_sha256":"b661b9119a3308788ab7ad607492a97e28db9157f55365f8767053d6798c56d1","source":{"kind":"arxiv","id":"2402.18454","version":1},"attestation_state":"computed","paper":{"title":"Prospects for measuring time variation of astrophysical neutrino sources at dark matter detectors","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"hep-ph","authors_text":"Lei Jin, Louis E. Strigari, Samiran Sinha, Yi Zhuang","submitted_at":"2024-02-28T16:27:38Z","abstract_excerpt":"We study the prospects for measuring the time variation of solar and atmospheric neutrino fluxes at future large-scale Xenon and Argon dark matter detectors. For solar neutrinos, a yearly time variation arises from the eccentricity of the Earth's orbit, and, for charged current interactions, from a smaller energy-dependent day-night variation to due flavor regeneration as neutrinos travel through the Earth. For a 100-ton Xenon detector running for 10 years with a Xenon-136 fraction of $\\lesssim 0.1\\%$, in the electron recoil channel a time-variation amplitude of about 0.8\\% is detectable with "},"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":"2402.18454","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2024-02-28T16:27:38Z","cross_cats_sorted":["astro-ph.HE"],"title_canon_sha256":"d656c11fc9296abc35080453dec87be4955ad9536181d2d3b3f6d77d7bb87001","abstract_canon_sha256":"18e6407351771d045740e8369e1b239ffd12e37a64b7cd2d065e285d2e2b4d30"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T07:50:16.346025Z","signature_b64":"DP8ElssrY23wOafRTiIF87514LCCOavKrBtSdo1F+dvjeTRQ/ee1ftDTEDNrFGXyWJw3ju+MFIXKEtdJAm9xBQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"b661b9119a3308788ab7ad607492a97e28db9157f55365f8767053d6798c56d1","last_reissued_at":"2026-07-05T07:50:16.345543Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T07:50:16.345543Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Prospects for measuring time variation of astrophysical neutrino sources at dark matter detectors","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"hep-ph","authors_text":"Lei Jin, Louis E. Strigari, Samiran Sinha, Yi Zhuang","submitted_at":"2024-02-28T16:27:38Z","abstract_excerpt":"We study the prospects for measuring the time variation of solar and atmospheric neutrino fluxes at future large-scale Xenon and Argon dark matter detectors. For solar neutrinos, a yearly time variation arises from the eccentricity of the Earth's orbit, and, for charged current interactions, from a smaller energy-dependent day-night variation to due flavor regeneration as neutrinos travel through the Earth. For a 100-ton Xenon detector running for 10 years with a Xenon-136 fraction of $\\lesssim 0.1\\%$, in the electron recoil channel a time-variation amplitude of about 0.8\\% is detectable with "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2402.18454","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/2402.18454/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":"2402.18454","created_at":"2026-07-05T07:50:16.345599+00:00"},{"alias_kind":"arxiv_version","alias_value":"2402.18454v1","created_at":"2026-07-05T07:50:16.345599+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2402.18454","created_at":"2026-07-05T07:50:16.345599+00:00"},{"alias_kind":"pith_short_12","alias_value":"WZQ3SEM2GMEH","created_at":"2026-07-05T07:50:16.345599+00:00"},{"alias_kind":"pith_short_16","alias_value":"WZQ3SEM2GMEHRCVX","created_at":"2026-07-05T07:50:16.345599+00:00"},{"alias_kind":"pith_short_8","alias_value":"WZQ3SEM2","created_at":"2026-07-05T07:50:16.345599+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":2,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2607.07406","citing_title":"Dark Neutrons as Dark Matter: Collisions in Halos and Direct Detection from Dark CP Violation","ref_index":97,"is_internal_anchor":true},{"citing_arxiv_id":"2606.13469","citing_title":"Simulations of 3-Dimensional Recoil Response to Coherent Elastic Neutrino-Nucleus Scattering Events in Directional Direct Dark Matter Detectors","ref_index":43,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/WZQ3SEM2GMEHRCVXVVQHJEVJPY","json":"https://pith.science/pith/WZQ3SEM2GMEHRCVXVVQHJEVJPY.json","graph_json":"https://pith.science/api/pith-number/WZQ3SEM2GMEHRCVXVVQHJEVJPY/graph.json","events_json":"https://pith.science/api/pith-number/WZQ3SEM2GMEHRCVXVVQHJEVJPY/events.json","paper":"https://pith.science/paper/WZQ3SEM2"},"agent_actions":{"view_html":"https://pith.science/pith/WZQ3SEM2GMEHRCVXVVQHJEVJPY","download_json":"https://pith.science/pith/WZQ3SEM2GMEHRCVXVVQHJEVJPY.json","view_paper":"https://pith.science/paper/WZQ3SEM2","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2402.18454&json=true","fetch_graph":"https://pith.science/api/pith-number/WZQ3SEM2GMEHRCVXVVQHJEVJPY/graph.json","fetch_events":"https://pith.science/api/pith-number/WZQ3SEM2GMEHRCVXVVQHJEVJPY/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/WZQ3SEM2GMEHRCVXVVQHJEVJPY/action/timestamp_anchor","attest_storage":"https://pith.science/pith/WZQ3SEM2GMEHRCVXVVQHJEVJPY/action/storage_attestation","attest_author":"https://pith.science/pith/WZQ3SEM2GMEHRCVXVVQHJEVJPY/action/author_attestation","sign_citation":"https://pith.science/pith/WZQ3SEM2GMEHRCVXVVQHJEVJPY/action/citation_signature","submit_replication":"https://pith.science/pith/WZQ3SEM2GMEHRCVXVVQHJEVJPY/action/replication_record"}},"created_at":"2026-07-05T07:50:16.345599+00:00","updated_at":"2026-07-05T07:50:16.345599+00:00"}