{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2013:QVSCQBENFVBDZZLTDOHBVSO3G7","short_pith_number":"pith:QVSCQBEN","schema_version":"1.0","canonical_sha256":"856428048d2d423ce5731b8e1ac9db37e49da4f11b0c2e15d97b4216f9eccee4","source":{"kind":"arxiv","id":"1306.2315","version":1},"attestation_state":"computed","paper":{"title":"Xenophobic Dark Matter","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","hep-ex"],"primary_cat":"hep-ph","authors_text":"David Sanford, Jason Kumar, Jonathan L. Feng","submitted_at":"2013-06-10T20:00:04Z","abstract_excerpt":"We consider models of xenophobic dark matter, in which isospin-violating dark matter-nucleon interactions significantly degrade the response of xenon direct detection experiments. For models of near-maximal xenophobia, with neutron-to-proton coupling ratio $f_n / f_p \\approx -0.64$, and dark matter mass near 8 GeV, the regions of interest for CoGeNT and CDMS-Si and the region of interest identified by Collar and Fields in CDMS-Ge data can be brought into agreement. This model may be tested in future direct, indirect, and collider searches. Interestingly, because the natural isotope abundance o"},"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":"1306.2315","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2013-06-10T20:00:04Z","cross_cats_sorted":["astro-ph.CO","hep-ex"],"title_canon_sha256":"d8e92ec075366ea26da67c2cdaad4d9982b8d2342c921ffda42adbb13b497499","abstract_canon_sha256":"0024e2712916270c8e156c0f74964d5c1822c60263180bc77bf82804bab8ea88"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T03:16:19.345049Z","signature_b64":"uuZnDvx5j5TXfoMglXFiDS9+9KyLB0AiDon1alul8KFnMuLsiy1ayoMBiJw8mQN50ypBFg0AQ3AG/W4+trV3Aw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"856428048d2d423ce5731b8e1ac9db37e49da4f11b0c2e15d97b4216f9eccee4","last_reissued_at":"2026-05-18T03:16:19.344563Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T03:16:19.344563Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Xenophobic Dark Matter","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","hep-ex"],"primary_cat":"hep-ph","authors_text":"David Sanford, Jason Kumar, Jonathan L. Feng","submitted_at":"2013-06-10T20:00:04Z","abstract_excerpt":"We consider models of xenophobic dark matter, in which isospin-violating dark matter-nucleon interactions significantly degrade the response of xenon direct detection experiments. For models of near-maximal xenophobia, with neutron-to-proton coupling ratio $f_n / f_p \\approx -0.64$, and dark matter mass near 8 GeV, the regions of interest for CoGeNT and CDMS-Si and the region of interest identified by Collar and Fields in CDMS-Ge data can be brought into agreement. This model may be tested in future direct, indirect, and collider searches. Interestingly, because the natural isotope abundance o"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1306.2315","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":""},"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":"1306.2315","created_at":"2026-05-18T03:16:19.344647+00:00"},{"alias_kind":"arxiv_version","alias_value":"1306.2315v1","created_at":"2026-05-18T03:16:19.344647+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1306.2315","created_at":"2026-05-18T03:16:19.344647+00:00"},{"alias_kind":"pith_short_12","alias_value":"QVSCQBENFVBD","created_at":"2026-05-18T12:27:57.521954+00:00"},{"alias_kind":"pith_short_16","alias_value":"QVSCQBENFVBDZZLT","created_at":"2026-05-18T12:27:57.521954+00:00"},{"alias_kind":"pith_short_8","alias_value":"QVSCQBEN","created_at":"2026-05-18T12:27:57.521954+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2601.06457","citing_title":"Physical implications of a double right-handed gauge symmetry","ref_index":52,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/QVSCQBENFVBDZZLTDOHBVSO3G7","json":"https://pith.science/pith/QVSCQBENFVBDZZLTDOHBVSO3G7.json","graph_json":"https://pith.science/api/pith-number/QVSCQBENFVBDZZLTDOHBVSO3G7/graph.json","events_json":"https://pith.science/api/pith-number/QVSCQBENFVBDZZLTDOHBVSO3G7/events.json","paper":"https://pith.science/paper/QVSCQBEN"},"agent_actions":{"view_html":"https://pith.science/pith/QVSCQBENFVBDZZLTDOHBVSO3G7","download_json":"https://pith.science/pith/QVSCQBENFVBDZZLTDOHBVSO3G7.json","view_paper":"https://pith.science/paper/QVSCQBEN","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1306.2315&json=true","fetch_graph":"https://pith.science/api/pith-number/QVSCQBENFVBDZZLTDOHBVSO3G7/graph.json","fetch_events":"https://pith.science/api/pith-number/QVSCQBENFVBDZZLTDOHBVSO3G7/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/QVSCQBENFVBDZZLTDOHBVSO3G7/action/timestamp_anchor","attest_storage":"https://pith.science/pith/QVSCQBENFVBDZZLTDOHBVSO3G7/action/storage_attestation","attest_author":"https://pith.science/pith/QVSCQBENFVBDZZLTDOHBVSO3G7/action/author_attestation","sign_citation":"https://pith.science/pith/QVSCQBENFVBDZZLTDOHBVSO3G7/action/citation_signature","submit_replication":"https://pith.science/pith/QVSCQBENFVBDZZLTDOHBVSO3G7/action/replication_record"}},"created_at":"2026-05-18T03:16:19.344647+00:00","updated_at":"2026-05-18T03:16:19.344647+00:00"}