{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:3WFG5EWLRD2H3IX3D63QVQPPHD","short_pith_number":"pith:3WFG5EWL","schema_version":"1.0","canonical_sha256":"dd8a6e92cb88f47da2fb1fb70ac1ef38e9ba4b96973c16da7b0b2f256edbce14","source":{"kind":"arxiv","id":"2406.18635","version":2},"attestation_state":"computed","paper":{"title":"Dark Matter from Dark Glueball Dominance","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"hep-ph","authors_text":"David E. Morrissey, David McKeen, Michael Shamma, Riku Mizuta","submitted_at":"2024-06-26T18:00:00Z","abstract_excerpt":"New gauge forces can play an important role in the evolution of the early universe. In this work we investigate the cosmological implications of a pure Yang-Mills dark sector that is dominantly populated after primordial inflation. Such a dark sector takes the form of a bath of dark gluons at high temperatures, but confines at lower temperatures to produce a spectrum of dark glueballs. These glueballs then undergo a freezeout process such that the remnant population is nearly completely dominated by the lightest state. To reproduce the observed cosmology, this lightest glueball species must de"},"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":"2406.18635","kind":"arxiv","version":2},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"hep-ph","submitted_at":"2024-06-26T18:00:00Z","cross_cats_sorted":["astro-ph.CO"],"title_canon_sha256":"434d703da992fd6d222b63268aa31c6bd5bc3f27d4fec5306087af6dd9e53105","abstract_canon_sha256":"5af056b12d821ab5b6c44ecc9973e69d628d048167b136f6afd27de0580b1a5e"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T10:13:01.491468Z","signature_b64":"iJGdONhoW9OyWEqZVBJMNgczlI9o5DPjb0Y8+bws2PzfSYkVFA4bQDY/p0VX32RJ/vUYJtTylrsQG4hWtn2JAA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"dd8a6e92cb88f47da2fb1fb70ac1ef38e9ba4b96973c16da7b0b2f256edbce14","last_reissued_at":"2026-07-05T10:13:01.490981Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T10:13:01.490981Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Dark Matter from Dark Glueball Dominance","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"hep-ph","authors_text":"David E. Morrissey, David McKeen, Michael Shamma, Riku Mizuta","submitted_at":"2024-06-26T18:00:00Z","abstract_excerpt":"New gauge forces can play an important role in the evolution of the early universe. In this work we investigate the cosmological implications of a pure Yang-Mills dark sector that is dominantly populated after primordial inflation. Such a dark sector takes the form of a bath of dark gluons at high temperatures, but confines at lower temperatures to produce a spectrum of dark glueballs. These glueballs then undergo a freezeout process such that the remnant population is nearly completely dominated by the lightest state. To reproduce the observed cosmology, this lightest glueball species must de"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2406.18635","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2406.18635/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"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":"2406.18635","created_at":"2026-07-05T10:13:01.491036+00:00"},{"alias_kind":"arxiv_version","alias_value":"2406.18635v2","created_at":"2026-07-05T10:13:01.491036+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2406.18635","created_at":"2026-07-05T10:13:01.491036+00:00"},{"alias_kind":"pith_short_12","alias_value":"3WFG5EWLRD2H","created_at":"2026-07-05T10:13:01.491036+00:00"},{"alias_kind":"pith_short_16","alias_value":"3WFG5EWLRD2H3IX3","created_at":"2026-07-05T10:13:01.491036+00:00"},{"alias_kind":"pith_short_8","alias_value":"3WFG5EWL","created_at":"2026-07-05T10:13:01.491036+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2606.30760","citing_title":"Rich Phenomenology from Simple Ingredients: A Review of Confining Dark Sectors","ref_index":116,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/3WFG5EWLRD2H3IX3D63QVQPPHD","json":"https://pith.science/pith/3WFG5EWLRD2H3IX3D63QVQPPHD.json","graph_json":"https://pith.science/api/pith-number/3WFG5EWLRD2H3IX3D63QVQPPHD/graph.json","events_json":"https://pith.science/api/pith-number/3WFG5EWLRD2H3IX3D63QVQPPHD/events.json","paper":"https://pith.science/paper/3WFG5EWL"},"agent_actions":{"view_html":"https://pith.science/pith/3WFG5EWLRD2H3IX3D63QVQPPHD","download_json":"https://pith.science/pith/3WFG5EWLRD2H3IX3D63QVQPPHD.json","view_paper":"https://pith.science/paper/3WFG5EWL","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2406.18635&json=true","fetch_graph":"https://pith.science/api/pith-number/3WFG5EWLRD2H3IX3D63QVQPPHD/graph.json","fetch_events":"https://pith.science/api/pith-number/3WFG5EWLRD2H3IX3D63QVQPPHD/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/3WFG5EWLRD2H3IX3D63QVQPPHD/action/timestamp_anchor","attest_storage":"https://pith.science/pith/3WFG5EWLRD2H3IX3D63QVQPPHD/action/storage_attestation","attest_author":"https://pith.science/pith/3WFG5EWLRD2H3IX3D63QVQPPHD/action/author_attestation","sign_citation":"https://pith.science/pith/3WFG5EWLRD2H3IX3D63QVQPPHD/action/citation_signature","submit_replication":"https://pith.science/pith/3WFG5EWLRD2H3IX3D63QVQPPHD/action/replication_record"}},"created_at":"2026-07-05T10:13:01.491036+00:00","updated_at":"2026-07-05T10:13:01.491036+00:00"}