{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2020:LRJPIVBOY23N6QXAELHAWSBGSE","short_pith_number":"pith:LRJPIVBO","schema_version":"1.0","canonical_sha256":"5c52f4542ec6b6df42e022ce0b4826912785cbe7a3eb2d06dbfcb04ff1e0cbe9","source":{"kind":"arxiv","id":"2008.05978","version":1},"attestation_state":"computed","paper":{"title":"Renormalization Group Studies of Dense Relativistic Systems","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["nucl-th"],"primary_cat":"hep-ph","authors_text":"Benedikt Schallmo, Jens Braun, Sebastian T\\\"opfel, Timon D\\\"ornfeld","submitted_at":"2020-08-13T15:53:05Z","abstract_excerpt":"Dense relativistic matter has attracted a lot of attention over many decades now, with a focus on an understanding of the phase structure and thermodynamics of dense strong-interaction matter. The analysis of dense strong-interaction matter is complicated by the fact that the system is expected to undergo a transition from a regime governed by spontaneous chiral symmetry breaking at low densities to a regime governed by the presence of a Cooper instability at intermediate and high densities. Renormalization group (RG) approaches have played and still play a prominent role in studies of dense m"},"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":"2008.05978","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2020-08-13T15:53:05Z","cross_cats_sorted":["nucl-th"],"title_canon_sha256":"eff31016fd237708a9e7267973ae762998477d33d1d0d1788d7d0e97b57c3a59","abstract_canon_sha256":"4d4ff99070f7f0db79dfa1c94fcf9819107105162a4005a8443f5bd246749816"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T03:31:53.402749Z","signature_b64":"8gi4CXGxeIK3mulF7x5mnoBcn8l/Z/Yqg+zoCoSQzZRevLLZvbOtOH+5G03lsD6lYWQAxkVe1qEW4TA6xWAHAg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"5c52f4542ec6b6df42e022ce0b4826912785cbe7a3eb2d06dbfcb04ff1e0cbe9","last_reissued_at":"2026-07-05T03:31:53.402264Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T03:31:53.402264Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Renormalization Group Studies of Dense Relativistic Systems","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["nucl-th"],"primary_cat":"hep-ph","authors_text":"Benedikt Schallmo, Jens Braun, Sebastian T\\\"opfel, Timon D\\\"ornfeld","submitted_at":"2020-08-13T15:53:05Z","abstract_excerpt":"Dense relativistic matter has attracted a lot of attention over many decades now, with a focus on an understanding of the phase structure and thermodynamics of dense strong-interaction matter. The analysis of dense strong-interaction matter is complicated by the fact that the system is expected to undergo a transition from a regime governed by spontaneous chiral symmetry breaking at low densities to a regime governed by the presence of a Cooper instability at intermediate and high densities. Renormalization group (RG) approaches have played and still play a prominent role in studies of dense m"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2008.05978","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2008.05978/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":"2008.05978","created_at":"2026-07-05T03:31:53.402322+00:00"},{"alias_kind":"arxiv_version","alias_value":"2008.05978v1","created_at":"2026-07-05T03:31:53.402322+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2008.05978","created_at":"2026-07-05T03:31:53.402322+00:00"},{"alias_kind":"pith_short_12","alias_value":"LRJPIVBOY23N","created_at":"2026-07-05T03:31:53.402322+00:00"},{"alias_kind":"pith_short_16","alias_value":"LRJPIVBOY23N6QXA","created_at":"2026-07-05T03:31:53.402322+00:00"},{"alias_kind":"pith_short_8","alias_value":"LRJPIVBO","created_at":"2026-07-05T03:31:53.402322+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":2,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2605.13934","citing_title":"Diquark Correlators and Phase Structure in the Quark-Meson-Diquark Model beyond Mean Field","ref_index":85,"is_internal_anchor":false},{"citing_arxiv_id":"2605.13934","citing_title":"Diquark Correlators and Phase Structure in the Quark-Meson-Diquark Model beyond Mean Field","ref_index":85,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/LRJPIVBOY23N6QXAELHAWSBGSE","json":"https://pith.science/pith/LRJPIVBOY23N6QXAELHAWSBGSE.json","graph_json":"https://pith.science/api/pith-number/LRJPIVBOY23N6QXAELHAWSBGSE/graph.json","events_json":"https://pith.science/api/pith-number/LRJPIVBOY23N6QXAELHAWSBGSE/events.json","paper":"https://pith.science/paper/LRJPIVBO"},"agent_actions":{"view_html":"https://pith.science/pith/LRJPIVBOY23N6QXAELHAWSBGSE","download_json":"https://pith.science/pith/LRJPIVBOY23N6QXAELHAWSBGSE.json","view_paper":"https://pith.science/paper/LRJPIVBO","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2008.05978&json=true","fetch_graph":"https://pith.science/api/pith-number/LRJPIVBOY23N6QXAELHAWSBGSE/graph.json","fetch_events":"https://pith.science/api/pith-number/LRJPIVBOY23N6QXAELHAWSBGSE/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/LRJPIVBOY23N6QXAELHAWSBGSE/action/timestamp_anchor","attest_storage":"https://pith.science/pith/LRJPIVBOY23N6QXAELHAWSBGSE/action/storage_attestation","attest_author":"https://pith.science/pith/LRJPIVBOY23N6QXAELHAWSBGSE/action/author_attestation","sign_citation":"https://pith.science/pith/LRJPIVBOY23N6QXAELHAWSBGSE/action/citation_signature","submit_replication":"https://pith.science/pith/LRJPIVBOY23N6QXAELHAWSBGSE/action/replication_record"}},"created_at":"2026-07-05T03:31:53.402322+00:00","updated_at":"2026-07-05T03:31:53.402322+00:00"}