{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2010:2W5XI2OIKNDF63S3YG4YUJZTBY","short_pith_number":"pith:2W5XI2OI","schema_version":"1.0","canonical_sha256":"d5bb7469c853465f6e5bc1b98a27330e1a57ce6a90a09827959e35b92407be9d","source":{"kind":"arxiv","id":"1006.0972","version":2},"attestation_state":"computed","paper":{"title":"XENON10/100 dark matter constraints in comparison with CoGeNT and DAMA: examining the Leff dependence","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-ex","hep-ph"],"primary_cat":"astro-ph.CO","authors_text":"Christopher Savage, Graciela Gelmini, Katherine Freese, Paolo Gondolo","submitted_at":"2010-06-04T19:54:23Z","abstract_excerpt":"We consider the compatibility of DAMA/LIBRA, CoGeNT, XENON10 and XENON100 results for spin-independent (SI) dark matter Weakly Interacting Massive Particles (WIMPs), particularly at low masses (~ 10 GeV), assuming a standard dark matter halo. The XENON bounds depend on the scintillation efficiency factor Leff for which there is considerable uncertainty. Thus we consider various extrapolations for Leff at low energy. With the Leff measurements we consider, XENON100 results are found to be insensitive to the low energy extrapolation. We find the strongest bounds are from XENON10, rather than XEN"},"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":"1006.0972","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2010-06-04T19:54:23Z","cross_cats_sorted":["hep-ex","hep-ph"],"title_canon_sha256":"c1f4c0a849bab78ce23a2548e92ff6acddf2ddf92b0202c163932e3ea1d19d8a","abstract_canon_sha256":"9ac47f1899dfe18957bdf01c9f2900452f5e2e4460753730a7e7843159b048fc"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T04:26:33.215679Z","signature_b64":"mNZsE1/0Bnz+JsT+ajl1fl9vmCSDVTFHpq6NrrWH/1/sJvMr8XeKmJNKtR5iOY8E0z4moB2GrK/gWkjaSZBpCA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"d5bb7469c853465f6e5bc1b98a27330e1a57ce6a90a09827959e35b92407be9d","last_reissued_at":"2026-05-18T04:26:33.215143Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T04:26:33.215143Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"XENON10/100 dark matter constraints in comparison with CoGeNT and DAMA: examining the Leff dependence","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-ex","hep-ph"],"primary_cat":"astro-ph.CO","authors_text":"Christopher Savage, Graciela Gelmini, Katherine Freese, Paolo Gondolo","submitted_at":"2010-06-04T19:54:23Z","abstract_excerpt":"We consider the compatibility of DAMA/LIBRA, CoGeNT, XENON10 and XENON100 results for spin-independent (SI) dark matter Weakly Interacting Massive Particles (WIMPs), particularly at low masses (~ 10 GeV), assuming a standard dark matter halo. The XENON bounds depend on the scintillation efficiency factor Leff for which there is considerable uncertainty. Thus we consider various extrapolations for Leff at low energy. With the Leff measurements we consider, XENON100 results are found to be insensitive to the low energy extrapolation. We find the strongest bounds are from XENON10, rather than XEN"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1006.0972","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":""},"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":"1006.0972","created_at":"2026-05-18T04:26:33.215219+00:00"},{"alias_kind":"arxiv_version","alias_value":"1006.0972v2","created_at":"2026-05-18T04:26:33.215219+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1006.0972","created_at":"2026-05-18T04:26:33.215219+00:00"},{"alias_kind":"pith_short_12","alias_value":"2W5XI2OIKNDF","created_at":"2026-05-18T12:26:03.138858+00:00"},{"alias_kind":"pith_short_16","alias_value":"2W5XI2OIKNDF63S3","created_at":"2026-05-18T12:26:03.138858+00:00"},{"alias_kind":"pith_short_8","alias_value":"2W5XI2OI","created_at":"2026-05-18T12:26:03.138858+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":0,"internal_anchor_count":0,"sample":[]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/2W5XI2OIKNDF63S3YG4YUJZTBY","json":"https://pith.science/pith/2W5XI2OIKNDF63S3YG4YUJZTBY.json","graph_json":"https://pith.science/api/pith-number/2W5XI2OIKNDF63S3YG4YUJZTBY/graph.json","events_json":"https://pith.science/api/pith-number/2W5XI2OIKNDF63S3YG4YUJZTBY/events.json","paper":"https://pith.science/paper/2W5XI2OI"},"agent_actions":{"view_html":"https://pith.science/pith/2W5XI2OIKNDF63S3YG4YUJZTBY","download_json":"https://pith.science/pith/2W5XI2OIKNDF63S3YG4YUJZTBY.json","view_paper":"https://pith.science/paper/2W5XI2OI","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1006.0972&json=true","fetch_graph":"https://pith.science/api/pith-number/2W5XI2OIKNDF63S3YG4YUJZTBY/graph.json","fetch_events":"https://pith.science/api/pith-number/2W5XI2OIKNDF63S3YG4YUJZTBY/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/2W5XI2OIKNDF63S3YG4YUJZTBY/action/timestamp_anchor","attest_storage":"https://pith.science/pith/2W5XI2OIKNDF63S3YG4YUJZTBY/action/storage_attestation","attest_author":"https://pith.science/pith/2W5XI2OIKNDF63S3YG4YUJZTBY/action/author_attestation","sign_citation":"https://pith.science/pith/2W5XI2OIKNDF63S3YG4YUJZTBY/action/citation_signature","submit_replication":"https://pith.science/pith/2W5XI2OIKNDF63S3YG4YUJZTBY/action/replication_record"}},"created_at":"2026-05-18T04:26:33.215219+00:00","updated_at":"2026-05-18T04:26:33.215219+00:00"}