{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2022:EN5GLP3BTJY6GTAAYNYKTCSFOT","short_pith_number":"pith:EN5GLP3B","schema_version":"1.0","canonical_sha256":"237a65bf619a71e34c00c370a98a4574d12fd2bfe7e28bcfeac294cbfdc31098","source":{"kind":"arxiv","id":"2210.14094","version":2},"attestation_state":"computed","paper":{"title":"Gravitational Waves and Primordial Black Hole Productions from Gluodynamics by Holography","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","gr-qc","hep-th"],"primary_cat":"hep-ph","authors_text":"Li Li, Shao-Jiang Wang, Song He, Zhibin Li","submitted_at":"2022-10-25T15:23:32Z","abstract_excerpt":"Understanding the nature of quantum chromodynamics (QCD) matter is important but challenging due to the presence of non-perturbative dynamics under extreme conditions. We construct a holographic model describing the gluon sector of QCD at finite temperatures in the non-perturbative regime. The equation of state as a function of temperature is in good accordance with the lattice QCD data. Moreover, the Polyakov loop and the gluon condensation, which are proper order parameters to capture the deconfinement phase transition, also agree quantitatively well with the lattice QCD data. We obtain a st"},"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":"2210.14094","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2022-10-25T15:23:32Z","cross_cats_sorted":["astro-ph.CO","gr-qc","hep-th"],"title_canon_sha256":"3fa0ead2ec89849392fc357467520666fc4bcdefd164a65c0ca5cbe5ec5bb2fa","abstract_canon_sha256":"eef2dbf8c2027eba6f3ca4c6ff7f454715d00ad3e8741193c5117cf7ea9cc35f"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T07:47:54.381474Z","signature_b64":"bfPGZw2NLNtNedt10bgjGMOgH7SR1rjnkozFX/VsyY0lZYuUDiapqEpH/G4/puRQCVKcE7yLcfAhyCXpqyTCCg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"237a65bf619a71e34c00c370a98a4574d12fd2bfe7e28bcfeac294cbfdc31098","last_reissued_at":"2026-07-05T07:47:54.380969Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T07:47:54.380969Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Gravitational Waves and Primordial Black Hole Productions from Gluodynamics by Holography","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","gr-qc","hep-th"],"primary_cat":"hep-ph","authors_text":"Li Li, Shao-Jiang Wang, Song He, Zhibin Li","submitted_at":"2022-10-25T15:23:32Z","abstract_excerpt":"Understanding the nature of quantum chromodynamics (QCD) matter is important but challenging due to the presence of non-perturbative dynamics under extreme conditions. We construct a holographic model describing the gluon sector of QCD at finite temperatures in the non-perturbative regime. The equation of state as a function of temperature is in good accordance with the lattice QCD data. Moreover, the Polyakov loop and the gluon condensation, which are proper order parameters to capture the deconfinement phase transition, also agree quantitatively well with the lattice QCD data. We obtain a st"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2210.14094","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/2210.14094/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":"2210.14094","created_at":"2026-07-05T07:47:54.381037+00:00"},{"alias_kind":"arxiv_version","alias_value":"2210.14094v2","created_at":"2026-07-05T07:47:54.381037+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2210.14094","created_at":"2026-07-05T07:47:54.381037+00:00"},{"alias_kind":"pith_short_12","alias_value":"EN5GLP3BTJY6","created_at":"2026-07-05T07:47:54.381037+00:00"},{"alias_kind":"pith_short_16","alias_value":"EN5GLP3BTJY6GTAA","created_at":"2026-07-05T07:47:54.381037+00:00"},{"alias_kind":"pith_short_8","alias_value":"EN5GLP3B","created_at":"2026-07-05T07:47:54.381037+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":5,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2606.01580","citing_title":"Primordial black holes spin from cosmological first-order phase transitions","ref_index":41,"is_internal_anchor":false},{"citing_arxiv_id":"2606.30740","citing_title":"Dynamical evolution of the pressure on the bubble wall","ref_index":100,"is_internal_anchor":false},{"citing_arxiv_id":"2606.01580","citing_title":"Primordial black holes spin from cosmological first-order phase transitions","ref_index":35,"is_internal_anchor":false},{"citing_arxiv_id":"2605.11332","citing_title":"Reviving primordial black hole formation in slow first-order phase transitions","ref_index":11,"is_internal_anchor":false},{"citing_arxiv_id":"2605.11332","citing_title":"Reviving primordial black hole formation in slow first-order phase transitions","ref_index":11,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/EN5GLP3BTJY6GTAAYNYKTCSFOT","json":"https://pith.science/pith/EN5GLP3BTJY6GTAAYNYKTCSFOT.json","graph_json":"https://pith.science/api/pith-number/EN5GLP3BTJY6GTAAYNYKTCSFOT/graph.json","events_json":"https://pith.science/api/pith-number/EN5GLP3BTJY6GTAAYNYKTCSFOT/events.json","paper":"https://pith.science/paper/EN5GLP3B"},"agent_actions":{"view_html":"https://pith.science/pith/EN5GLP3BTJY6GTAAYNYKTCSFOT","download_json":"https://pith.science/pith/EN5GLP3BTJY6GTAAYNYKTCSFOT.json","view_paper":"https://pith.science/paper/EN5GLP3B","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2210.14094&json=true","fetch_graph":"https://pith.science/api/pith-number/EN5GLP3BTJY6GTAAYNYKTCSFOT/graph.json","fetch_events":"https://pith.science/api/pith-number/EN5GLP3BTJY6GTAAYNYKTCSFOT/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/EN5GLP3BTJY6GTAAYNYKTCSFOT/action/timestamp_anchor","attest_storage":"https://pith.science/pith/EN5GLP3BTJY6GTAAYNYKTCSFOT/action/storage_attestation","attest_author":"https://pith.science/pith/EN5GLP3BTJY6GTAAYNYKTCSFOT/action/author_attestation","sign_citation":"https://pith.science/pith/EN5GLP3BTJY6GTAAYNYKTCSFOT/action/citation_signature","submit_replication":"https://pith.science/pith/EN5GLP3BTJY6GTAAYNYKTCSFOT/action/replication_record"}},"created_at":"2026-07-05T07:47:54.381037+00:00","updated_at":"2026-07-05T07:47:54.381037+00:00"}