{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2014:DS533EYKKDZ3NP4YOGQ5M66HDD","short_pith_number":"pith:DS533EYK","schema_version":"1.0","canonical_sha256":"1cbbbd930a50f3b6bf9871a1d67bc718c52dd68ec3f60310d1ff9d147052c77f","source":{"kind":"arxiv","id":"1405.7427","version":1},"attestation_state":"computed","paper":{"title":"The Reach of Threshold-Corrected Dark QCD","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"hep-ph","authors_text":"Jayden L. Newstead, Russell H. TerBeek","submitted_at":"2014-05-29T00:04:46Z","abstract_excerpt":"We consider a recently-proposed model which posits the existence of composite dark matter, wherein dark \"quarks\" transforming as fundamentals under an $SU(3)_d$ gauge group undergo a confining phase and form dark baryons. The model attempts to explain both the $\\mathcal{O}(1)$ relic density ratio, $\\Omega_{\\mathrm{dark}}/\\Omega_{\\mathrm{baryon}}\\sim 5.4$, as well as the asymmetric production of both dark and baryonic matter via leptogenesis. Though the solution of $\\beta$ functions for $SU(3)_c$ and $SU(3)_d$ constitutes the main drive of the model, no threshold corrections were taken into acc"},"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":"1405.7427","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2014-05-29T00:04:46Z","cross_cats_sorted":["astro-ph.HE"],"title_canon_sha256":"e74df2f70dc3f183253f36e704005219aaf799e2fd8632e7063e016e7ff20b61","abstract_canon_sha256":"0023decf226c92eb592c3b8685b2f485d03580e61509268ec43d4d827e297d15"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:40:55.923715Z","signature_b64":"nNzqmblbTgF+MsRcZPx89b6w1XmBANGtNiTmdGivcxIniuh04fq2dZOk2OMd3FX8pWnkFPtGlp9eQRby60VXCg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"1cbbbd930a50f3b6bf9871a1d67bc718c52dd68ec3f60310d1ff9d147052c77f","last_reissued_at":"2026-05-18T02:40:55.923079Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:40:55.923079Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The Reach of Threshold-Corrected Dark QCD","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"hep-ph","authors_text":"Jayden L. Newstead, Russell H. TerBeek","submitted_at":"2014-05-29T00:04:46Z","abstract_excerpt":"We consider a recently-proposed model which posits the existence of composite dark matter, wherein dark \"quarks\" transforming as fundamentals under an $SU(3)_d$ gauge group undergo a confining phase and form dark baryons. The model attempts to explain both the $\\mathcal{O}(1)$ relic density ratio, $\\Omega_{\\mathrm{dark}}/\\Omega_{\\mathrm{baryon}}\\sim 5.4$, as well as the asymmetric production of both dark and baryonic matter via leptogenesis. Though the solution of $\\beta$ functions for $SU(3)_c$ and $SU(3)_d$ constitutes the main drive of the model, no threshold corrections were taken into acc"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1405.7427","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":"1405.7427","created_at":"2026-05-18T02:40:55.923153+00:00"},{"alias_kind":"arxiv_version","alias_value":"1405.7427v1","created_at":"2026-05-18T02:40:55.923153+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1405.7427","created_at":"2026-05-18T02:40:55.923153+00:00"},{"alias_kind":"pith_short_12","alias_value":"DS533EYKKDZ3","created_at":"2026-05-18T12:28:25.294606+00:00"},{"alias_kind":"pith_short_16","alias_value":"DS533EYKKDZ3NP4Y","created_at":"2026-05-18T12:28:25.294606+00:00"},{"alias_kind":"pith_short_8","alias_value":"DS533EYK","created_at":"2026-05-18T12:28:25.294606+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2604.21168","citing_title":"Neutron Portal and Dark Matter-Baryon Coincidence: from UV Completion to Phenomenology","ref_index":48,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/DS533EYKKDZ3NP4YOGQ5M66HDD","json":"https://pith.science/pith/DS533EYKKDZ3NP4YOGQ5M66HDD.json","graph_json":"https://pith.science/api/pith-number/DS533EYKKDZ3NP4YOGQ5M66HDD/graph.json","events_json":"https://pith.science/api/pith-number/DS533EYKKDZ3NP4YOGQ5M66HDD/events.json","paper":"https://pith.science/paper/DS533EYK"},"agent_actions":{"view_html":"https://pith.science/pith/DS533EYKKDZ3NP4YOGQ5M66HDD","download_json":"https://pith.science/pith/DS533EYKKDZ3NP4YOGQ5M66HDD.json","view_paper":"https://pith.science/paper/DS533EYK","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1405.7427&json=true","fetch_graph":"https://pith.science/api/pith-number/DS533EYKKDZ3NP4YOGQ5M66HDD/graph.json","fetch_events":"https://pith.science/api/pith-number/DS533EYKKDZ3NP4YOGQ5M66HDD/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/DS533EYKKDZ3NP4YOGQ5M66HDD/action/timestamp_anchor","attest_storage":"https://pith.science/pith/DS533EYKKDZ3NP4YOGQ5M66HDD/action/storage_attestation","attest_author":"https://pith.science/pith/DS533EYKKDZ3NP4YOGQ5M66HDD/action/author_attestation","sign_citation":"https://pith.science/pith/DS533EYKKDZ3NP4YOGQ5M66HDD/action/citation_signature","submit_replication":"https://pith.science/pith/DS533EYKKDZ3NP4YOGQ5M66HDD/action/replication_record"}},"created_at":"2026-05-18T02:40:55.923153+00:00","updated_at":"2026-05-18T02:40:55.923153+00:00"}