{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2019:AXDYYKYIDWE4D7MVXKMJSUPIND","short_pith_number":"pith:AXDYYKYI","schema_version":"1.0","canonical_sha256":"05c78c2b081d89c1fd95ba989951e868e9be3a6d7062cdebe1974db9730ff605","source":{"kind":"arxiv","id":"1910.08553","version":2},"attestation_state":"computed","paper":{"title":"Breaking a dark degeneracy: The gamma-ray signature of early matter domination","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE","hep-ph"],"primary_cat":"astro-ph.CO","authors_text":"Adrienne L. Erickcek, M. Sten Delos, Tim Linden","submitted_at":"2019-10-18T18:00:00Z","abstract_excerpt":"The Universe's early thermal history is poorly constrained, and it is possible that it underwent a period of early matter domination driven by a heavy particle or an oscillating scalar field that decayed into radiation before the onset of Big Bang nucleosynthesis. The entropy sourced by this particle's decay reduces the cross section required for thermal-relic dark matter to achieve the observed abundance. This degeneracy between dark matter properties and the thermal history vastly widens the field of viable dark matter candidates, undermining efforts to constrain dark matter's identity. Fort"},"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":"1910.08553","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2019-10-18T18:00:00Z","cross_cats_sorted":["astro-ph.HE","hep-ph"],"title_canon_sha256":"4c164f2156d94bc13dd0efe4534d81b12677f1d1a59c2d0a7de0972d5d165840","abstract_canon_sha256":"4138e79bf3541e7fa155e641279c4dad99bba4183a818bb5b451d1edef6656e9"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T00:29:29.410756Z","signature_b64":"Ge6wQyWNUxytx0EvOI/dsoIncspo/X7wXRRp6uxyNZKhM9AC002K7js/1jPSYeZOPhgxfKWbcXvNUatQHoukBQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"05c78c2b081d89c1fd95ba989951e868e9be3a6d7062cdebe1974db9730ff605","last_reissued_at":"2026-07-05T00:29:29.410375Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T00:29:29.410375Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Breaking a dark degeneracy: The gamma-ray signature of early matter domination","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE","hep-ph"],"primary_cat":"astro-ph.CO","authors_text":"Adrienne L. Erickcek, M. Sten Delos, Tim Linden","submitted_at":"2019-10-18T18:00:00Z","abstract_excerpt":"The Universe's early thermal history is poorly constrained, and it is possible that it underwent a period of early matter domination driven by a heavy particle or an oscillating scalar field that decayed into radiation before the onset of Big Bang nucleosynthesis. The entropy sourced by this particle's decay reduces the cross section required for thermal-relic dark matter to achieve the observed abundance. This degeneracy between dark matter properties and the thermal history vastly widens the field of viable dark matter candidates, undermining efforts to constrain dark matter's identity. Fort"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1910.08553","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/1910.08553/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":"1910.08553","created_at":"2026-07-05T00:29:29.410432+00:00"},{"alias_kind":"arxiv_version","alias_value":"1910.08553v2","created_at":"2026-07-05T00:29:29.410432+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1910.08553","created_at":"2026-07-05T00:29:29.410432+00:00"},{"alias_kind":"pith_short_12","alias_value":"AXDYYKYIDWE4","created_at":"2026-07-05T00:29:29.410432+00:00"},{"alias_kind":"pith_short_16","alias_value":"AXDYYKYIDWE4D7MV","created_at":"2026-07-05T00:29:29.410432+00:00"},{"alias_kind":"pith_short_8","alias_value":"AXDYYKYI","created_at":"2026-07-05T00:29:29.410432+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2412.14322","citing_title":"Free streaming of warm wave dark matter in modified expansion histories","ref_index":74,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/AXDYYKYIDWE4D7MVXKMJSUPIND","json":"https://pith.science/pith/AXDYYKYIDWE4D7MVXKMJSUPIND.json","graph_json":"https://pith.science/api/pith-number/AXDYYKYIDWE4D7MVXKMJSUPIND/graph.json","events_json":"https://pith.science/api/pith-number/AXDYYKYIDWE4D7MVXKMJSUPIND/events.json","paper":"https://pith.science/paper/AXDYYKYI"},"agent_actions":{"view_html":"https://pith.science/pith/AXDYYKYIDWE4D7MVXKMJSUPIND","download_json":"https://pith.science/pith/AXDYYKYIDWE4D7MVXKMJSUPIND.json","view_paper":"https://pith.science/paper/AXDYYKYI","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1910.08553&json=true","fetch_graph":"https://pith.science/api/pith-number/AXDYYKYIDWE4D7MVXKMJSUPIND/graph.json","fetch_events":"https://pith.science/api/pith-number/AXDYYKYIDWE4D7MVXKMJSUPIND/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/AXDYYKYIDWE4D7MVXKMJSUPIND/action/timestamp_anchor","attest_storage":"https://pith.science/pith/AXDYYKYIDWE4D7MVXKMJSUPIND/action/storage_attestation","attest_author":"https://pith.science/pith/AXDYYKYIDWE4D7MVXKMJSUPIND/action/author_attestation","sign_citation":"https://pith.science/pith/AXDYYKYIDWE4D7MVXKMJSUPIND/action/citation_signature","submit_replication":"https://pith.science/pith/AXDYYKYIDWE4D7MVXKMJSUPIND/action/replication_record"}},"created_at":"2026-07-05T00:29:29.410432+00:00","updated_at":"2026-07-05T00:29:29.410432+00:00"}