{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2012:HRC2BTRSLGADKCQS5ACUXCZNRU","short_pith_number":"pith:HRC2BTRS","schema_version":"1.0","canonical_sha256":"3c45a0ce325980350a12e8054b8b2d8d289bb784bf5964499e58c48b9f8c61bd","source":{"kind":"arxiv","id":"1203.0158","version":1},"attestation_state":"computed","paper":{"title":"Hybrid protoneutron stars with the Dyson-Schwinger quark model","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-ph"],"primary_cat":"nucl-th","authors_text":"G. F. Burgio, H. Chen, H.-J. Schulze, M. Baldo","submitted_at":"2012-03-01T11:40:51Z","abstract_excerpt":"We study the hadron-quark phase transition at finite temperature in the interior of protoneutron stars, combining the Dyson-Schwinger model for quark matter with the Brueckner-Hartree-Fock approach for hadronic matter. We discuss the dependence of the results on different nuclear three-body forces and on details of the quark model. %Compared to the bag model, the transition from the hadron phase %(without hyperons) to the quark phase appears at large density. A maximum mass exceeding two solar masses can be obtained with a strong three-body force and suitable parameter values in the Dyson-Schw"},"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":"1203.0158","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"nucl-th","submitted_at":"2012-03-01T11:40:51Z","cross_cats_sorted":["hep-ph"],"title_canon_sha256":"8feb699c8776e281ca1801f287d215a1c4a51b8e258251d98bff7f6a1710be05","abstract_canon_sha256":"26a5a896f8c70664fd0d2bbf8fc19c2eb309229ec9287b902220f62ac733d098"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:58:17.872333Z","signature_b64":"0uHzjfWCSMq18XoPLWyYau8cNr3qgXz0qtdWmuEizmcs8acRbMPhpXGYYeZ/+GHlC22xuYmSF3tEZqTn1CNhDQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"3c45a0ce325980350a12e8054b8b2d8d289bb784bf5964499e58c48b9f8c61bd","last_reissued_at":"2026-05-18T01:58:17.871893Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:58:17.871893Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Hybrid protoneutron stars with the Dyson-Schwinger quark model","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-ph"],"primary_cat":"nucl-th","authors_text":"G. F. Burgio, H. Chen, H.-J. Schulze, M. Baldo","submitted_at":"2012-03-01T11:40:51Z","abstract_excerpt":"We study the hadron-quark phase transition at finite temperature in the interior of protoneutron stars, combining the Dyson-Schwinger model for quark matter with the Brueckner-Hartree-Fock approach for hadronic matter. We discuss the dependence of the results on different nuclear three-body forces and on details of the quark model. %Compared to the bag model, the transition from the hadron phase %(without hyperons) to the quark phase appears at large density. A maximum mass exceeding two solar masses can be obtained with a strong three-body force and suitable parameter values in the Dyson-Schw"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1203.0158","kind":"arxiv","version":1},"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":"1203.0158","created_at":"2026-05-18T01:58:17.871952+00:00"},{"alias_kind":"arxiv_version","alias_value":"1203.0158v1","created_at":"2026-05-18T01:58:17.871952+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1203.0158","created_at":"2026-05-18T01:58:17.871952+00:00"},{"alias_kind":"pith_short_12","alias_value":"HRC2BTRSLGAD","created_at":"2026-05-18T12:27:09.501522+00:00"},{"alias_kind":"pith_short_16","alias_value":"HRC2BTRSLGADKCQS","created_at":"2026-05-18T12:27:09.501522+00:00"},{"alias_kind":"pith_short_8","alias_value":"HRC2BTRS","created_at":"2026-05-18T12:27:09.501522+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":0,"internal_anchor_count":0,"sample":[]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/HRC2BTRSLGADKCQS5ACUXCZNRU","json":"https://pith.science/pith/HRC2BTRSLGADKCQS5ACUXCZNRU.json","graph_json":"https://pith.science/api/pith-number/HRC2BTRSLGADKCQS5ACUXCZNRU/graph.json","events_json":"https://pith.science/api/pith-number/HRC2BTRSLGADKCQS5ACUXCZNRU/events.json","paper":"https://pith.science/paper/HRC2BTRS"},"agent_actions":{"view_html":"https://pith.science/pith/HRC2BTRSLGADKCQS5ACUXCZNRU","download_json":"https://pith.science/pith/HRC2BTRSLGADKCQS5ACUXCZNRU.json","view_paper":"https://pith.science/paper/HRC2BTRS","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1203.0158&json=true","fetch_graph":"https://pith.science/api/pith-number/HRC2BTRSLGADKCQS5ACUXCZNRU/graph.json","fetch_events":"https://pith.science/api/pith-number/HRC2BTRSLGADKCQS5ACUXCZNRU/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/HRC2BTRSLGADKCQS5ACUXCZNRU/action/timestamp_anchor","attest_storage":"https://pith.science/pith/HRC2BTRSLGADKCQS5ACUXCZNRU/action/storage_attestation","attest_author":"https://pith.science/pith/HRC2BTRSLGADKCQS5ACUXCZNRU/action/author_attestation","sign_citation":"https://pith.science/pith/HRC2BTRSLGADKCQS5ACUXCZNRU/action/citation_signature","submit_replication":"https://pith.science/pith/HRC2BTRSLGADKCQS5ACUXCZNRU/action/replication_record"}},"created_at":"2026-05-18T01:58:17.871952+00:00","updated_at":"2026-05-18T01:58:17.871952+00:00"}