{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:RFUSIHTDCSSXCHZBOS2EEIKVHP","short_pith_number":"pith:RFUSIHTD","schema_version":"1.0","canonical_sha256":"8969241e6314a5711f2174b44221553bfcdc3fc57292b7940fa93e07685ea562","source":{"kind":"arxiv","id":"1704.01804","version":2},"attestation_state":"computed","paper":{"title":"Glueball dark matter in non-standard cosmologies","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-th"],"primary_cat":"hep-ph","authors_text":"Bobby Samir Acharya, Edward Hardy, Malcolm Fairbairn","submitted_at":"2017-04-06T12:25:48Z","abstract_excerpt":"Hidden sector glueball dark matter is well motivated by string theory, compactifications of which often have extra gauge groups uncoupled to the visible sector. We study the dynamics of glueballs in theories with a period of late time primordial matter domination followed by a low final reheating temperature due to a gravitationally coupled modulus. Compared to scenarios with a high reheating temperature, the required relic abundance is possible with higher hidden sector confinement scales, and less extreme differences in the entropy densities of the hidden and visible sectors. Both of these c"},"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":"1704.01804","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2017-04-06T12:25:48Z","cross_cats_sorted":["hep-th"],"title_canon_sha256":"e734c0d366ca5c046a5d3b4d9c74ea037ac91ecfdf3782b7d5188050f3a081c9","abstract_canon_sha256":"8629fd665d6d48667431de66c4d9123ec0e6336486146ecac06ec024d4f1401e"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:38:03.088821Z","signature_b64":"3lZ4xoRbcM67ZPDLdvA272uEvUIaOYi4hlEJ9NjiWe08vTSez3SpT5ZXKgafC/6kFVnatN/qsN/uSUdQclGdDw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"8969241e6314a5711f2174b44221553bfcdc3fc57292b7940fa93e07685ea562","last_reissued_at":"2026-05-18T00:38:03.088395Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:38:03.088395Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Glueball dark matter in non-standard cosmologies","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-th"],"primary_cat":"hep-ph","authors_text":"Bobby Samir Acharya, Edward Hardy, Malcolm Fairbairn","submitted_at":"2017-04-06T12:25:48Z","abstract_excerpt":"Hidden sector glueball dark matter is well motivated by string theory, compactifications of which often have extra gauge groups uncoupled to the visible sector. We study the dynamics of glueballs in theories with a period of late time primordial matter domination followed by a low final reheating temperature due to a gravitationally coupled modulus. Compared to scenarios with a high reheating temperature, the required relic abundance is possible with higher hidden sector confinement scales, and less extreme differences in the entropy densities of the hidden and visible sectors. Both of these c"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1704.01804","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":"1704.01804","created_at":"2026-05-18T00:38:03.088452+00:00"},{"alias_kind":"arxiv_version","alias_value":"1704.01804v2","created_at":"2026-05-18T00:38:03.088452+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1704.01804","created_at":"2026-05-18T00:38:03.088452+00:00"},{"alias_kind":"pith_short_12","alias_value":"RFUSIHTDCSSX","created_at":"2026-05-18T12:31:39.905425+00:00"},{"alias_kind":"pith_short_16","alias_value":"RFUSIHTDCSSXCHZB","created_at":"2026-05-18T12:31:39.905425+00:00"},{"alias_kind":"pith_short_8","alias_value":"RFUSIHTD","created_at":"2026-05-18T12:31:39.905425+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"1907.01944","citing_title":"Dark Horse, Dark Matter: Revisiting the SO(16)x SO(16)' Nonsupersymmetric Model in the LHC and Dark Energy Era","ref_index":78,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/RFUSIHTDCSSXCHZBOS2EEIKVHP","json":"https://pith.science/pith/RFUSIHTDCSSXCHZBOS2EEIKVHP.json","graph_json":"https://pith.science/api/pith-number/RFUSIHTDCSSXCHZBOS2EEIKVHP/graph.json","events_json":"https://pith.science/api/pith-number/RFUSIHTDCSSXCHZBOS2EEIKVHP/events.json","paper":"https://pith.science/paper/RFUSIHTD"},"agent_actions":{"view_html":"https://pith.science/pith/RFUSIHTDCSSXCHZBOS2EEIKVHP","download_json":"https://pith.science/pith/RFUSIHTDCSSXCHZBOS2EEIKVHP.json","view_paper":"https://pith.science/paper/RFUSIHTD","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1704.01804&json=true","fetch_graph":"https://pith.science/api/pith-number/RFUSIHTDCSSXCHZBOS2EEIKVHP/graph.json","fetch_events":"https://pith.science/api/pith-number/RFUSIHTDCSSXCHZBOS2EEIKVHP/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/RFUSIHTDCSSXCHZBOS2EEIKVHP/action/timestamp_anchor","attest_storage":"https://pith.science/pith/RFUSIHTDCSSXCHZBOS2EEIKVHP/action/storage_attestation","attest_author":"https://pith.science/pith/RFUSIHTDCSSXCHZBOS2EEIKVHP/action/author_attestation","sign_citation":"https://pith.science/pith/RFUSIHTDCSSXCHZBOS2EEIKVHP/action/citation_signature","submit_replication":"https://pith.science/pith/RFUSIHTDCSSXCHZBOS2EEIKVHP/action/replication_record"}},"created_at":"2026-05-18T00:38:03.088452+00:00","updated_at":"2026-05-18T00:38:03.088452+00:00"}