{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2013:FCZ3LVZMYDQXEBASZ6GIIHOY3U","short_pith_number":"pith:FCZ3LVZM","schema_version":"1.0","canonical_sha256":"28b3b5d72cc0e1720412cf8c841dd8dd09689d3963fabaa6c96a701cfc6e550b","source":{"kind":"arxiv","id":"1310.7945","version":1},"attestation_state":"computed","paper":{"title":"Direct Detection Portals for Self-interacting Dark Matter","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-ph","authors_text":"Hai-Bo Yu, Manoj Kaplinghat, Sean Tulin","submitted_at":"2013-10-29T20:00:46Z","abstract_excerpt":"Dark matter self-interactions can affect the small scale structure of the Universe, reducing the central densities of dwarfs and low surface brightness galaxies in accord with observations. From a particle physics point of view, this points toward the existence of a 1-100 MeV particle in the dark sector that mediates self-interactions. Since mediator particles will generically couple to the Standard Model, direct detection experiments provide sensitive probes of self-interacting dark matter. We consider three minimal mechanisms for coupling the dark and visible sectors: photon kinetic mixing, "},"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":"1310.7945","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2013-10-29T20:00:46Z","cross_cats_sorted":[],"title_canon_sha256":"9fc0baf6115636cc019731c44d849b772daf42a3cfeb97e98cf7f38d35ded327","abstract_canon_sha256":"5ff917bc9a45f2b19eeb62470f9b52ca911f98a49c367ea60d31bcec86012450"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:46:47.646204Z","signature_b64":"qMvvEHZHPKtCof1P95MPAuVY/6ldJEh8rQNSzyqL7/Jo/nvPDlJWeLwY/sNMh/imKNKudnR+e1SYqp3Q+fsXCg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"28b3b5d72cc0e1720412cf8c841dd8dd09689d3963fabaa6c96a701cfc6e550b","last_reissued_at":"2026-05-18T01:46:47.645359Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:46:47.645359Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Direct Detection Portals for Self-interacting Dark Matter","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-ph","authors_text":"Hai-Bo Yu, Manoj Kaplinghat, Sean Tulin","submitted_at":"2013-10-29T20:00:46Z","abstract_excerpt":"Dark matter self-interactions can affect the small scale structure of the Universe, reducing the central densities of dwarfs and low surface brightness galaxies in accord with observations. From a particle physics point of view, this points toward the existence of a 1-100 MeV particle in the dark sector that mediates self-interactions. Since mediator particles will generically couple to the Standard Model, direct detection experiments provide sensitive probes of self-interacting dark matter. We consider three minimal mechanisms for coupling the dark and visible sectors: photon kinetic mixing, "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1310.7945","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":"1310.7945","created_at":"2026-05-18T01:46:47.645524+00:00"},{"alias_kind":"arxiv_version","alias_value":"1310.7945v1","created_at":"2026-05-18T01:46:47.645524+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1310.7945","created_at":"2026-05-18T01:46:47.645524+00:00"},{"alias_kind":"pith_short_12","alias_value":"FCZ3LVZMYDQX","created_at":"2026-05-18T12:27:45.050594+00:00"},{"alias_kind":"pith_short_16","alias_value":"FCZ3LVZMYDQXEBAS","created_at":"2026-05-18T12:27:45.050594+00:00"},{"alias_kind":"pith_short_8","alias_value":"FCZ3LVZM","created_at":"2026-05-18T12:27:45.050594+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2604.15006","citing_title":"Cosmology of Inelastic Self-Interacting Dark Matter: Linear Evolution and Observational Constraints","ref_index":32,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/FCZ3LVZMYDQXEBASZ6GIIHOY3U","json":"https://pith.science/pith/FCZ3LVZMYDQXEBASZ6GIIHOY3U.json","graph_json":"https://pith.science/api/pith-number/FCZ3LVZMYDQXEBASZ6GIIHOY3U/graph.json","events_json":"https://pith.science/api/pith-number/FCZ3LVZMYDQXEBASZ6GIIHOY3U/events.json","paper":"https://pith.science/paper/FCZ3LVZM"},"agent_actions":{"view_html":"https://pith.science/pith/FCZ3LVZMYDQXEBASZ6GIIHOY3U","download_json":"https://pith.science/pith/FCZ3LVZMYDQXEBASZ6GIIHOY3U.json","view_paper":"https://pith.science/paper/FCZ3LVZM","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1310.7945&json=true","fetch_graph":"https://pith.science/api/pith-number/FCZ3LVZMYDQXEBASZ6GIIHOY3U/graph.json","fetch_events":"https://pith.science/api/pith-number/FCZ3LVZMYDQXEBASZ6GIIHOY3U/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/FCZ3LVZMYDQXEBASZ6GIIHOY3U/action/timestamp_anchor","attest_storage":"https://pith.science/pith/FCZ3LVZMYDQXEBASZ6GIIHOY3U/action/storage_attestation","attest_author":"https://pith.science/pith/FCZ3LVZMYDQXEBASZ6GIIHOY3U/action/author_attestation","sign_citation":"https://pith.science/pith/FCZ3LVZMYDQXEBASZ6GIIHOY3U/action/citation_signature","submit_replication":"https://pith.science/pith/FCZ3LVZMYDQXEBASZ6GIIHOY3U/action/replication_record"}},"created_at":"2026-05-18T01:46:47.645524+00:00","updated_at":"2026-05-18T01:46:47.645524+00:00"}