{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2022:D4GZDUUJMDD2W3XELK74TPGS7D","short_pith_number":"pith:D4GZDUUJ","schema_version":"1.0","canonical_sha256":"1f0d91d28960c7ab6ee45abfc9bcd2f8e0e4f50f1ef22ee7bea2ef55719bbea7","source":{"kind":"arxiv","id":"2202.03887","version":1},"attestation_state":"computed","paper":{"title":"Dark matter, supernova neutrinos and other backgrounds in direct dark matter searches. The ANDES laboratory prospects","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"hep-ph","authors_text":"K.J. Fushimi, M.E. Mosquera, M.M. Saez, O. Civitarese","submitted_at":"2022-02-08T14:22:23Z","abstract_excerpt":"Dark Matter particles can be detected directly via their elastic scattering with nuclei. Next generation experiments can eventually find physical evidences about dark matter candidates. With this motivation in mind, we have calculated the expected signals of dark matter particles in xenon detectors. The calculations were performed by considering different masses and parameters within the minimal supersymmetric standard model. Since the detectors can also detect neutrinos, we have analyzed the supernova neutrino signal including a sterile neutrino in the formalism. Using this 3+1 scheme, we mak"},"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":"2202.03887","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2022-02-08T14:22:23Z","cross_cats_sorted":["astro-ph.HE"],"title_canon_sha256":"430d6de41810f86164ec7e97aef28afbaf87dc0f2250ffb975d5b84d7aa5dc3e","abstract_canon_sha256":"bf61c0889ef041c32648181ba79b907384c9565ff32b8eb18496c9fbb3fe2599"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T03:55:21.064595Z","signature_b64":"XBF0ptIAz0IzDP8RfTop2DDwnsLJM7//gx7wUx7uRVmbhRmyMVb8tfNMFIX4IdcDxgF43FYFVgcmvEiTrUKOBw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"1f0d91d28960c7ab6ee45abfc9bcd2f8e0e4f50f1ef22ee7bea2ef55719bbea7","last_reissued_at":"2026-07-05T03:55:21.064083Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T03:55:21.064083Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Dark matter, supernova neutrinos and other backgrounds in direct dark matter searches. The ANDES laboratory prospects","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"hep-ph","authors_text":"K.J. Fushimi, M.E. Mosquera, M.M. Saez, O. Civitarese","submitted_at":"2022-02-08T14:22:23Z","abstract_excerpt":"Dark Matter particles can be detected directly via their elastic scattering with nuclei. Next generation experiments can eventually find physical evidences about dark matter candidates. With this motivation in mind, we have calculated the expected signals of dark matter particles in xenon detectors. The calculations were performed by considering different masses and parameters within the minimal supersymmetric standard model. Since the detectors can also detect neutrinos, we have analyzed the supernova neutrino signal including a sterile neutrino in the formalism. Using this 3+1 scheme, we mak"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2202.03887","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/2202.03887/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":"2202.03887","created_at":"2026-07-05T03:55:21.064148+00:00"},{"alias_kind":"arxiv_version","alias_value":"2202.03887v1","created_at":"2026-07-05T03:55:21.064148+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2202.03887","created_at":"2026-07-05T03:55:21.064148+00:00"},{"alias_kind":"pith_short_12","alias_value":"D4GZDUUJMDD2","created_at":"2026-07-05T03:55:21.064148+00:00"},{"alias_kind":"pith_short_16","alias_value":"D4GZDUUJMDD2W3XE","created_at":"2026-07-05T03:55:21.064148+00:00"},{"alias_kind":"pith_short_8","alias_value":"D4GZDUUJ","created_at":"2026-07-05T03:55:21.064148+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2412.05213","citing_title":"Probing neutrino mass ordering with supernova neutrinos at NO$\\nu$A including the effect of sterile neutrinos","ref_index":17,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/D4GZDUUJMDD2W3XELK74TPGS7D","json":"https://pith.science/pith/D4GZDUUJMDD2W3XELK74TPGS7D.json","graph_json":"https://pith.science/api/pith-number/D4GZDUUJMDD2W3XELK74TPGS7D/graph.json","events_json":"https://pith.science/api/pith-number/D4GZDUUJMDD2W3XELK74TPGS7D/events.json","paper":"https://pith.science/paper/D4GZDUUJ"},"agent_actions":{"view_html":"https://pith.science/pith/D4GZDUUJMDD2W3XELK74TPGS7D","download_json":"https://pith.science/pith/D4GZDUUJMDD2W3XELK74TPGS7D.json","view_paper":"https://pith.science/paper/D4GZDUUJ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2202.03887&json=true","fetch_graph":"https://pith.science/api/pith-number/D4GZDUUJMDD2W3XELK74TPGS7D/graph.json","fetch_events":"https://pith.science/api/pith-number/D4GZDUUJMDD2W3XELK74TPGS7D/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/D4GZDUUJMDD2W3XELK74TPGS7D/action/timestamp_anchor","attest_storage":"https://pith.science/pith/D4GZDUUJMDD2W3XELK74TPGS7D/action/storage_attestation","attest_author":"https://pith.science/pith/D4GZDUUJMDD2W3XELK74TPGS7D/action/author_attestation","sign_citation":"https://pith.science/pith/D4GZDUUJMDD2W3XELK74TPGS7D/action/citation_signature","submit_replication":"https://pith.science/pith/D4GZDUUJMDD2W3XELK74TPGS7D/action/replication_record"}},"created_at":"2026-07-05T03:55:21.064148+00:00","updated_at":"2026-07-05T03:55:21.064148+00:00"}