{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2014:AC36KANBKYWIYUYFTZ5WPNZ3FZ","short_pith_number":"pith:AC36KANB","schema_version":"1.0","canonical_sha256":"00b7e501a1562c8c53059e7b67b73b2e48217ee1553d3a899a012646da6b9db1","source":{"kind":"arxiv","id":"1410.2236","version":5},"attestation_state":"computed","paper":{"title":"Macro Dark Matter","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA","hep-ph"],"primary_cat":"astro-ph.CO","authors_text":"Bryan W. Lynn, David M. Jacobs, Glenn D. Starkman","submitted_at":"2014-10-08T19:57:44Z","abstract_excerpt":"Dark matter is a vital component of the current best model of our universe, $\\Lambda$CDM. There are leading candidates for what the dark matter could be (e.g. weakly-interacting massive particles, or axions), but no compelling observational or experimental evidence exists to support these particular candidates, nor any beyond-the-Standard-Model physics that might produce such candidates. This suggests that other dark matter candidates, including ones that might arise in the Standard Model, should receive increased attention. Here we consider a general class of dark matter candidates with chara"},"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":"1410.2236","kind":"arxiv","version":5},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2014-10-08T19:57:44Z","cross_cats_sorted":["astro-ph.GA","hep-ph"],"title_canon_sha256":"4c65386398abe602386103cf892a48f7f5e990b8b5489d4811bc4795e797d62b","abstract_canon_sha256":"ede8a2dfdd8791b477e2395f2dfd3b21b6a702edbd8b7df6317121d9a1166960"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:37:23.364310Z","signature_b64":"Hkw3jjtrDz9lc9nf4C01ZAifpEtiY0zFNC/6vSWrpzgb1EKVK6RfRMjwhRKsDL93osbWPMc9zWW5oaHXeAstBw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"00b7e501a1562c8c53059e7b67b73b2e48217ee1553d3a899a012646da6b9db1","last_reissued_at":"2026-05-18T01:37:23.363594Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:37:23.363594Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Macro Dark Matter","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA","hep-ph"],"primary_cat":"astro-ph.CO","authors_text":"Bryan W. Lynn, David M. Jacobs, Glenn D. Starkman","submitted_at":"2014-10-08T19:57:44Z","abstract_excerpt":"Dark matter is a vital component of the current best model of our universe, $\\Lambda$CDM. There are leading candidates for what the dark matter could be (e.g. weakly-interacting massive particles, or axions), but no compelling observational or experimental evidence exists to support these particular candidates, nor any beyond-the-Standard-Model physics that might produce such candidates. This suggests that other dark matter candidates, including ones that might arise in the Standard Model, should receive increased attention. Here we consider a general class of dark matter candidates with chara"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1410.2236","kind":"arxiv","version":5},"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":"1410.2236","created_at":"2026-05-18T01:37:23.363704+00:00"},{"alias_kind":"arxiv_version","alias_value":"1410.2236v5","created_at":"2026-05-18T01:37:23.363704+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1410.2236","created_at":"2026-05-18T01:37:23.363704+00:00"},{"alias_kind":"pith_short_12","alias_value":"AC36KANBKYWI","created_at":"2026-05-18T12:28:19.803747+00:00"},{"alias_kind":"pith_short_16","alias_value":"AC36KANBKYWIYUYF","created_at":"2026-05-18T12:28:19.803747+00:00"},{"alias_kind":"pith_short_8","alias_value":"AC36KANB","created_at":"2026-05-18T12:28:19.803747+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":2,"internal_anchor_count":2,"sample":[{"citing_arxiv_id":"2603.15585","citing_title":"QCD-driven dark matter: AQNs formation and observational tests","ref_index":35,"is_internal_anchor":true},{"citing_arxiv_id":"2605.13958","citing_title":"Baryoid Dark Matter from $\\mathbb{Z}_N$ Domain Walls: The $(N-1):1$ origin of the dark matter-baryon coincidence","ref_index":36,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/AC36KANBKYWIYUYFTZ5WPNZ3FZ","json":"https://pith.science/pith/AC36KANBKYWIYUYFTZ5WPNZ3FZ.json","graph_json":"https://pith.science/api/pith-number/AC36KANBKYWIYUYFTZ5WPNZ3FZ/graph.json","events_json":"https://pith.science/api/pith-number/AC36KANBKYWIYUYFTZ5WPNZ3FZ/events.json","paper":"https://pith.science/paper/AC36KANB"},"agent_actions":{"view_html":"https://pith.science/pith/AC36KANBKYWIYUYFTZ5WPNZ3FZ","download_json":"https://pith.science/pith/AC36KANBKYWIYUYFTZ5WPNZ3FZ.json","view_paper":"https://pith.science/paper/AC36KANB","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1410.2236&json=true","fetch_graph":"https://pith.science/api/pith-number/AC36KANBKYWIYUYFTZ5WPNZ3FZ/graph.json","fetch_events":"https://pith.science/api/pith-number/AC36KANBKYWIYUYFTZ5WPNZ3FZ/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/AC36KANBKYWIYUYFTZ5WPNZ3FZ/action/timestamp_anchor","attest_storage":"https://pith.science/pith/AC36KANBKYWIYUYFTZ5WPNZ3FZ/action/storage_attestation","attest_author":"https://pith.science/pith/AC36KANBKYWIYUYFTZ5WPNZ3FZ/action/author_attestation","sign_citation":"https://pith.science/pith/AC36KANBKYWIYUYFTZ5WPNZ3FZ/action/citation_signature","submit_replication":"https://pith.science/pith/AC36KANBKYWIYUYFTZ5WPNZ3FZ/action/replication_record"}},"created_at":"2026-05-18T01:37:23.363704+00:00","updated_at":"2026-05-18T01:37:23.363704+00:00"}