{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:SMC7KGX4X3GFW3QBQKJ5H6LO42","short_pith_number":"pith:SMC7KGX4","schema_version":"1.0","canonical_sha256":"9305f51afcbecc5b6e018293d3f96ee6b5a459b100a8c3367ccf3933bd8fca4a","source":{"kind":"arxiv","id":"1706.00455","version":3},"attestation_state":"computed","paper":{"title":"Critical point in the phase diagram of primordial quark-gluon matter from black hole physics","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-lat","hep-ph","hep-th","nucl-ex"],"primary_cat":"nucl-th","authors_text":"(2) Rutgers U., 3), (3) Houston U., (4) IIP, Brazil), Claudia Ratti (3), Israel Portillo (3), Jacquelyn Noronha-Hostler (2, Jorge Noronha (1), Renato Critelli (1), Romulo Rougemont (4) ((1) Sao Paulo U.","submitted_at":"2017-06-01T18:52:43Z","abstract_excerpt":"Strongly interacting matter undergoes a crossover phase transition at high temperatures $T\\sim 10^{12}$ K and zero net-baryon density. A fundamental question in the theory of strong interactions, Quantum Chromodynamics (QCD), is whether a hot and dense system of quarks and gluons displays critical phenomena when doped with more quarks than antiquarks, where net-baryon number fluctuations diverge. Recent lattice QCD work indicates that such a critical point can only occur in the baryon dense regime of the theory, which defies a description from first principles calculations. Here we use the hol"},"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":"1706.00455","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"nucl-th","submitted_at":"2017-06-01T18:52:43Z","cross_cats_sorted":["hep-lat","hep-ph","hep-th","nucl-ex"],"title_canon_sha256":"0a236291cb8765a2f99715e61b558d240ea9d210dad2f6541454d700665c0417","abstract_canon_sha256":"ef596622a8601b185bade4ed988f39f155d2268b9b5c883c6ef53f34a40f8f47"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:29:30.426017Z","signature_b64":"HgNmEEXWguN1bycscnnkfh7r7yH8x/nFmei7AvqZqu9OyfqP+XS80j4Pp+JP+KzFDAzj6/bJYe/NLuHO2OD0Dg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"9305f51afcbecc5b6e018293d3f96ee6b5a459b100a8c3367ccf3933bd8fca4a","last_reissued_at":"2026-05-18T00:29:30.425485Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:29:30.425485Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Critical point in the phase diagram of primordial quark-gluon matter from black hole physics","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-lat","hep-ph","hep-th","nucl-ex"],"primary_cat":"nucl-th","authors_text":"(2) Rutgers U., 3), (3) Houston U., (4) IIP, Brazil), Claudia Ratti (3), Israel Portillo (3), Jacquelyn Noronha-Hostler (2, Jorge Noronha (1), Renato Critelli (1), Romulo Rougemont (4) ((1) Sao Paulo U.","submitted_at":"2017-06-01T18:52:43Z","abstract_excerpt":"Strongly interacting matter undergoes a crossover phase transition at high temperatures $T\\sim 10^{12}$ K and zero net-baryon density. A fundamental question in the theory of strong interactions, Quantum Chromodynamics (QCD), is whether a hot and dense system of quarks and gluons displays critical phenomena when doped with more quarks than antiquarks, where net-baryon number fluctuations diverge. Recent lattice QCD work indicates that such a critical point can only occur in the baryon dense regime of the theory, which defies a description from first principles calculations. Here we use the hol"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1706.00455","kind":"arxiv","version":3},"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":"1706.00455","created_at":"2026-05-18T00:29:30.425569+00:00"},{"alias_kind":"arxiv_version","alias_value":"1706.00455v3","created_at":"2026-05-18T00:29:30.425569+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1706.00455","created_at":"2026-05-18T00:29:30.425569+00:00"},{"alias_kind":"pith_short_12","alias_value":"SMC7KGX4X3GF","created_at":"2026-05-18T12:31:43.269735+00:00"},{"alias_kind":"pith_short_16","alias_value":"SMC7KGX4X3GFW3QB","created_at":"2026-05-18T12:31:43.269735+00:00"},{"alias_kind":"pith_short_8","alias_value":"SMC7KGX4","created_at":"2026-05-18T12:31:43.269735+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2604.20196","citing_title":"Chiral first order phase transition at finite baryon density and zero temperature from self-consistent pole masses in the linear sigma model with quarks","ref_index":58,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/SMC7KGX4X3GFW3QBQKJ5H6LO42","json":"https://pith.science/pith/SMC7KGX4X3GFW3QBQKJ5H6LO42.json","graph_json":"https://pith.science/api/pith-number/SMC7KGX4X3GFW3QBQKJ5H6LO42/graph.json","events_json":"https://pith.science/api/pith-number/SMC7KGX4X3GFW3QBQKJ5H6LO42/events.json","paper":"https://pith.science/paper/SMC7KGX4"},"agent_actions":{"view_html":"https://pith.science/pith/SMC7KGX4X3GFW3QBQKJ5H6LO42","download_json":"https://pith.science/pith/SMC7KGX4X3GFW3QBQKJ5H6LO42.json","view_paper":"https://pith.science/paper/SMC7KGX4","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1706.00455&json=true","fetch_graph":"https://pith.science/api/pith-number/SMC7KGX4X3GFW3QBQKJ5H6LO42/graph.json","fetch_events":"https://pith.science/api/pith-number/SMC7KGX4X3GFW3QBQKJ5H6LO42/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/SMC7KGX4X3GFW3QBQKJ5H6LO42/action/timestamp_anchor","attest_storage":"https://pith.science/pith/SMC7KGX4X3GFW3QBQKJ5H6LO42/action/storage_attestation","attest_author":"https://pith.science/pith/SMC7KGX4X3GFW3QBQKJ5H6LO42/action/author_attestation","sign_citation":"https://pith.science/pith/SMC7KGX4X3GFW3QBQKJ5H6LO42/action/citation_signature","submit_replication":"https://pith.science/pith/SMC7KGX4X3GFW3QBQKJ5H6LO42/action/replication_record"}},"created_at":"2026-05-18T00:29:30.425569+00:00","updated_at":"2026-05-18T00:29:30.425569+00:00"}