{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2014:SGYOMICJK7S4UAIARELUQRHIVE","short_pith_number":"pith:SGYOMICJ","schema_version":"1.0","canonical_sha256":"91b0e6204957e5ca010089174844e8a91b031864df7ab429df4bdf00a76e62b2","source":{"kind":"arxiv","id":"1411.3727","version":2},"attestation_state":"computed","paper":{"title":"The SIMPlest Miracle","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-ph","authors_text":"Eric Kuflik, Hitoshi Murayama, Jay G. Wacker, Tomer Volansky, Yonit Hochberg","submitted_at":"2014-11-13T21:00:07Z","abstract_excerpt":"It has recently been proposed that dark matter could be a thermal relic of 3-to-2 scatterings in a strongly coupled hidden sector. We present explicit classes of strongly coupled gauge theories that admit this behavior. These are QCD-like theories of dynamical chiral symmetry breaking, where the pions play the role of dark matter. The number-changing 3-to-2 process, which sets the dark matter relic abundance, arises from the Wess-Zumino-Witten term. The theories give an explicit relationship between the 3-to-2 annihilation rate and the 2-to-2 self-scattering rate, which alters predictions for "},"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":"1411.3727","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2014-11-13T21:00:07Z","cross_cats_sorted":[],"title_canon_sha256":"63fe8e7f6cf7ac6f954e93348ef570372aac6740f6c2b437c93091be0df589ef","abstract_canon_sha256":"d9b3fbcd4b910895afdd1c50321cc85036946a9401bd4a1be6639360ab52d822"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:36:20.319040Z","signature_b64":"lJilTi2IWSWzC819MZLOXiDB+8/IjagL7T2SF/c+Wc+jkDnqYyZv+TNLR1N/kKu5KQSNcHsDH0jXNaO0fbggBg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"91b0e6204957e5ca010089174844e8a91b031864df7ab429df4bdf00a76e62b2","last_reissued_at":"2026-05-18T01:36:20.318247Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:36:20.318247Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The SIMPlest Miracle","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-ph","authors_text":"Eric Kuflik, Hitoshi Murayama, Jay G. Wacker, Tomer Volansky, Yonit Hochberg","submitted_at":"2014-11-13T21:00:07Z","abstract_excerpt":"It has recently been proposed that dark matter could be a thermal relic of 3-to-2 scatterings in a strongly coupled hidden sector. We present explicit classes of strongly coupled gauge theories that admit this behavior. These are QCD-like theories of dynamical chiral symmetry breaking, where the pions play the role of dark matter. The number-changing 3-to-2 process, which sets the dark matter relic abundance, arises from the Wess-Zumino-Witten term. The theories give an explicit relationship between the 3-to-2 annihilation rate and the 2-to-2 self-scattering rate, which alters predictions for "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1411.3727","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":"1411.3727","created_at":"2026-05-18T01:36:20.318385+00:00"},{"alias_kind":"arxiv_version","alias_value":"1411.3727v2","created_at":"2026-05-18T01:36:20.318385+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1411.3727","created_at":"2026-05-18T01:36:20.318385+00:00"},{"alias_kind":"pith_short_12","alias_value":"SGYOMICJK7S4","created_at":"2026-05-18T12:28:49.207871+00:00"},{"alias_kind":"pith_short_16","alias_value":"SGYOMICJK7S4UAIA","created_at":"2026-05-18T12:28:49.207871+00:00"},{"alias_kind":"pith_short_8","alias_value":"SGYOMICJ","created_at":"2026-05-18T12:28:49.207871+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":6,"internal_anchor_count":5,"sample":[{"citing_arxiv_id":"1907.04324","citing_title":"Dark Matter Energy Deposition and Production from the Table-Top to the Cosmos","ref_index":50,"is_internal_anchor":true},{"citing_arxiv_id":"2501.14864","citing_title":"Super-Kamiokande Strongly Constrains Leptophilic Dark Matter Capture in the Sun","ref_index":88,"is_internal_anchor":true},{"citing_arxiv_id":"2503.19691","citing_title":"Strongly Interacting Dark Matter admixed Neutron Stars","ref_index":60,"is_internal_anchor":true},{"citing_arxiv_id":"2509.19009","citing_title":"Finite-temperature Yang-Mills theories with the density of states method: towards the continuum limit","ref_index":55,"is_internal_anchor":true},{"citing_arxiv_id":"2602.02678","citing_title":"Axion-Like Electrophilic Portal for Pion Dark Matter","ref_index":3,"is_internal_anchor":true},{"citing_arxiv_id":"2604.06315","citing_title":"Dark Matter on a Slide","ref_index":3,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/SGYOMICJK7S4UAIARELUQRHIVE","json":"https://pith.science/pith/SGYOMICJK7S4UAIARELUQRHIVE.json","graph_json":"https://pith.science/api/pith-number/SGYOMICJK7S4UAIARELUQRHIVE/graph.json","events_json":"https://pith.science/api/pith-number/SGYOMICJK7S4UAIARELUQRHIVE/events.json","paper":"https://pith.science/paper/SGYOMICJ"},"agent_actions":{"view_html":"https://pith.science/pith/SGYOMICJK7S4UAIARELUQRHIVE","download_json":"https://pith.science/pith/SGYOMICJK7S4UAIARELUQRHIVE.json","view_paper":"https://pith.science/paper/SGYOMICJ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1411.3727&json=true","fetch_graph":"https://pith.science/api/pith-number/SGYOMICJK7S4UAIARELUQRHIVE/graph.json","fetch_events":"https://pith.science/api/pith-number/SGYOMICJK7S4UAIARELUQRHIVE/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/SGYOMICJK7S4UAIARELUQRHIVE/action/timestamp_anchor","attest_storage":"https://pith.science/pith/SGYOMICJK7S4UAIARELUQRHIVE/action/storage_attestation","attest_author":"https://pith.science/pith/SGYOMICJK7S4UAIARELUQRHIVE/action/author_attestation","sign_citation":"https://pith.science/pith/SGYOMICJK7S4UAIARELUQRHIVE/action/citation_signature","submit_replication":"https://pith.science/pith/SGYOMICJK7S4UAIARELUQRHIVE/action/replication_record"}},"created_at":"2026-05-18T01:36:20.318385+00:00","updated_at":"2026-05-18T01:36:20.318385+00:00"}