{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2012:6RSENOPNSBJNIXY33GFI66KCDP","short_pith_number":"pith:6RSENOPN","schema_version":"1.0","canonical_sha256":"f46446b9ed9052d45f1bd98a8f79421bf1b86c793e179c7f6f6bc1d9a69b6aa8","source":{"kind":"arxiv","id":"1208.3697","version":2},"attestation_state":"computed","paper":{"title":"Antiquark nuggets as dark matter: New constraints and detection prospects","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Peter. W. Gorham","submitted_at":"2012-08-17T21:44:40Z","abstract_excerpt":"Current evidence for dark matter in the universe does not exclude heavy composite nuclear-density objects consisting of bound quarks or antiquarks over a significant range of masses. Here we analyze one such proposed scenario, which hypothesizes antiquark nuggets with a range of log10(B) = 24-30 with specific predictions for spectral emissivity via interactions with normal matter. We find that, if these objects make up the majority of the dark matter density in the solar neighborhood, their radiation efficiency in solids is marginally constrained, due to limits from the total geothermal energy"},"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":"1208.3697","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2012-08-17T21:44:40Z","cross_cats_sorted":[],"title_canon_sha256":"c6ed57c8814dedb4604066aeac6efe01ef3e5ff5d1025e7133ae48aaf38d5b3f","abstract_canon_sha256":"7c00802143c509083bacc1a54a528cca7a72dda3f5f195f45272028af202c050"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T03:22:29.253648Z","signature_b64":"/B6JqdYvaR3VPCmGrduEmDADEPJHPtvw+40oXGHEVp2e4r9T6oZIdW2NJvqa2HhXGI2/99Q6dX/nvreCq7Z7DQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"f46446b9ed9052d45f1bd98a8f79421bf1b86c793e179c7f6f6bc1d9a69b6aa8","last_reissued_at":"2026-05-18T03:22:29.252889Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T03:22:29.252889Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Antiquark nuggets as dark matter: New constraints and detection prospects","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Peter. W. Gorham","submitted_at":"2012-08-17T21:44:40Z","abstract_excerpt":"Current evidence for dark matter in the universe does not exclude heavy composite nuclear-density objects consisting of bound quarks or antiquarks over a significant range of masses. Here we analyze one such proposed scenario, which hypothesizes antiquark nuggets with a range of log10(B) = 24-30 with specific predictions for spectral emissivity via interactions with normal matter. We find that, if these objects make up the majority of the dark matter density in the solar neighborhood, their radiation efficiency in solids is marginally constrained, due to limits from the total geothermal energy"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1208.3697","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":"1208.3697","created_at":"2026-05-18T03:22:29.252993+00:00"},{"alias_kind":"arxiv_version","alias_value":"1208.3697v2","created_at":"2026-05-18T03:22:29.252993+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1208.3697","created_at":"2026-05-18T03:22:29.252993+00:00"},{"alias_kind":"pith_short_12","alias_value":"6RSENOPNSBJN","created_at":"2026-05-18T12:26:56.085431+00:00"},{"alias_kind":"pith_short_16","alias_value":"6RSENOPNSBJNIXY3","created_at":"2026-05-18T12:26:56.085431+00:00"},{"alias_kind":"pith_short_8","alias_value":"6RSENOPN","created_at":"2026-05-18T12:26:56.085431+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2603.15585","citing_title":"QCD-driven dark matter: AQNs formation and observational tests","ref_index":63,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/6RSENOPNSBJNIXY33GFI66KCDP","json":"https://pith.science/pith/6RSENOPNSBJNIXY33GFI66KCDP.json","graph_json":"https://pith.science/api/pith-number/6RSENOPNSBJNIXY33GFI66KCDP/graph.json","events_json":"https://pith.science/api/pith-number/6RSENOPNSBJNIXY33GFI66KCDP/events.json","paper":"https://pith.science/paper/6RSENOPN"},"agent_actions":{"view_html":"https://pith.science/pith/6RSENOPNSBJNIXY33GFI66KCDP","download_json":"https://pith.science/pith/6RSENOPNSBJNIXY33GFI66KCDP.json","view_paper":"https://pith.science/paper/6RSENOPN","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1208.3697&json=true","fetch_graph":"https://pith.science/api/pith-number/6RSENOPNSBJNIXY33GFI66KCDP/graph.json","fetch_events":"https://pith.science/api/pith-number/6RSENOPNSBJNIXY33GFI66KCDP/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/6RSENOPNSBJNIXY33GFI66KCDP/action/timestamp_anchor","attest_storage":"https://pith.science/pith/6RSENOPNSBJNIXY33GFI66KCDP/action/storage_attestation","attest_author":"https://pith.science/pith/6RSENOPNSBJNIXY33GFI66KCDP/action/author_attestation","sign_citation":"https://pith.science/pith/6RSENOPNSBJNIXY33GFI66KCDP/action/citation_signature","submit_replication":"https://pith.science/pith/6RSENOPNSBJNIXY33GFI66KCDP/action/replication_record"}},"created_at":"2026-05-18T03:22:29.252993+00:00","updated_at":"2026-05-18T03:22:29.252993+00:00"}