{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2020:SFDFJQLJ7LAGWQABEXVEAD3XF3","short_pith_number":"pith:SFDFJQLJ","schema_version":"1.0","canonical_sha256":"914654c169fac06b400125ea400f772ec56a21b694a834a0912d8f72208c17ba","source":{"kind":"arxiv","id":"2006.14590","version":1},"attestation_state":"computed","paper":{"title":"XENON1T Anomaly: A Light $Z^\\prime$","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE","hep-ex","hep-th"],"primary_cat":"hep-ph","authors_text":"Farinaldo S. Queiroz, Manfred Lindner, Tessio B. de Melo, Yann Mambrini","submitted_at":"2020-06-25T17:35:41Z","abstract_excerpt":"We have witnessed the beginning of an era where dark matter and neutrino detectors can probe similar new physics phenomena. Motivated by the low-energy electron recoil spectrum observed by the dark matter experiment, XENON1T, at Gran Sasso laboratory, we interpret the observed signal not in terms of a dark matter particle, but rather in the context of a new light $Z^\\prime$ gauge boson. We discuss how such a light $Z^\\prime$ rises in a Two Higgs Doublet Model augmented by an abelian gauge symmetry where neutrino masses and the flavor problem are addressed, in agreement with neutrino-electron s"},"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":"2006.14590","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2020-06-25T17:35:41Z","cross_cats_sorted":["astro-ph.HE","hep-ex","hep-th"],"title_canon_sha256":"42882edcfc3ac6d75424b295aae48fa5eea295727712a61d46380bcb965063df","abstract_canon_sha256":"2884c631c61aec3dbeb05f018c633d208ee138dca1ec1a04b46ca42cd464883c"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T01:55:57.302838Z","signature_b64":"xUOOJR/WcxMQ03qqO9hZW2nJaUzlPBCwphEvzG0H5qSn0HvBi9k8Yk8u2CMhMtSI7FYfl5R/l7cXCPZiqHTJCQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"914654c169fac06b400125ea400f772ec56a21b694a834a0912d8f72208c17ba","last_reissued_at":"2026-07-05T01:55:57.302356Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T01:55:57.302356Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"XENON1T Anomaly: A Light $Z^\\prime$","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE","hep-ex","hep-th"],"primary_cat":"hep-ph","authors_text":"Farinaldo S. Queiroz, Manfred Lindner, Tessio B. de Melo, Yann Mambrini","submitted_at":"2020-06-25T17:35:41Z","abstract_excerpt":"We have witnessed the beginning of an era where dark matter and neutrino detectors can probe similar new physics phenomena. Motivated by the low-energy electron recoil spectrum observed by the dark matter experiment, XENON1T, at Gran Sasso laboratory, we interpret the observed signal not in terms of a dark matter particle, but rather in the context of a new light $Z^\\prime$ gauge boson. We discuss how such a light $Z^\\prime$ rises in a Two Higgs Doublet Model augmented by an abelian gauge symmetry where neutrino masses and the flavor problem are addressed, in agreement with neutrino-electron s"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2006.14590","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/2006.14590/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":"2006.14590","created_at":"2026-07-05T01:55:57.302415+00:00"},{"alias_kind":"arxiv_version","alias_value":"2006.14590v1","created_at":"2026-07-05T01:55:57.302415+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2006.14590","created_at":"2026-07-05T01:55:57.302415+00:00"},{"alias_kind":"pith_short_12","alias_value":"SFDFJQLJ7LAG","created_at":"2026-07-05T01:55:57.302415+00:00"},{"alias_kind":"pith_short_16","alias_value":"SFDFJQLJ7LAGWQAB","created_at":"2026-07-05T01:55:57.302415+00:00"},{"alias_kind":"pith_short_8","alias_value":"SFDFJQLJ","created_at":"2026-07-05T01:55:57.302415+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2606.12408","citing_title":"When direct detection constrains reheating temperature: freeze-in with stronger couplings and inflaton-seeded freeze-in","ref_index":17,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/SFDFJQLJ7LAGWQABEXVEAD3XF3","json":"https://pith.science/pith/SFDFJQLJ7LAGWQABEXVEAD3XF3.json","graph_json":"https://pith.science/api/pith-number/SFDFJQLJ7LAGWQABEXVEAD3XF3/graph.json","events_json":"https://pith.science/api/pith-number/SFDFJQLJ7LAGWQABEXVEAD3XF3/events.json","paper":"https://pith.science/paper/SFDFJQLJ"},"agent_actions":{"view_html":"https://pith.science/pith/SFDFJQLJ7LAGWQABEXVEAD3XF3","download_json":"https://pith.science/pith/SFDFJQLJ7LAGWQABEXVEAD3XF3.json","view_paper":"https://pith.science/paper/SFDFJQLJ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2006.14590&json=true","fetch_graph":"https://pith.science/api/pith-number/SFDFJQLJ7LAGWQABEXVEAD3XF3/graph.json","fetch_events":"https://pith.science/api/pith-number/SFDFJQLJ7LAGWQABEXVEAD3XF3/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/SFDFJQLJ7LAGWQABEXVEAD3XF3/action/timestamp_anchor","attest_storage":"https://pith.science/pith/SFDFJQLJ7LAGWQABEXVEAD3XF3/action/storage_attestation","attest_author":"https://pith.science/pith/SFDFJQLJ7LAGWQABEXVEAD3XF3/action/author_attestation","sign_citation":"https://pith.science/pith/SFDFJQLJ7LAGWQABEXVEAD3XF3/action/citation_signature","submit_replication":"https://pith.science/pith/SFDFJQLJ7LAGWQABEXVEAD3XF3/action/replication_record"}},"created_at":"2026-07-05T01:55:57.302415+00:00","updated_at":"2026-07-05T01:55:57.302415+00:00"}