{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2023:347YTV4YZTJ42RAXECMRZ7NFKF","short_pith_number":"pith:347YTV4Y","schema_version":"1.0","canonical_sha256":"df3f89d798ccd3cd441720991cfda5514a8b779a6c8b6fa53a480bf197d9aeab","source":{"kind":"arxiv","id":"2307.08734","version":2},"attestation_state":"computed","paper":{"title":"Equation of State of Cold Quark Matter to $O(\\alpha_s^3 \\ln \\alpha_s)$","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE","nucl-th"],"primary_cat":"hep-ph","authors_text":"Kaapo Sepp\\\"anen, Risto Paatelainen, Saga S\\\"appi, Tyler Gorda","submitted_at":"2023-07-17T18:00:01Z","abstract_excerpt":"Accurately understanding the equation of state (EOS) of high-density, zero-temperature quark matter plays an essential role in constraining the behavior of dense strongly interacting matter inside the cores of neutron stars. In this Letter, we study the weak-coupling expansion of the EOS of cold quark matter and derive the complete, gauge-invariant contributions from the long-wavelength, dynamically screened gluonic sector at next-to-next-to-next-to-leading order (N3LO) in the strong coupling constant $\\alpha_s$. This elevates the EOS result to the $O(\\alpha_s^3 \\ln \\alpha_s)$ level, leaving o"},"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":"2307.08734","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2023-07-17T18:00:01Z","cross_cats_sorted":["astro-ph.HE","nucl-th"],"title_canon_sha256":"6c5ca53702f4c4e8ae5e38b5554087d8781ef871f71ecc2f176d63cd7c297db8","abstract_canon_sha256":"353cfa3c3d9ac320d28e668951d801812f64a78f31390d44167fa8b5185e3ddd"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T07:11:57.917448Z","signature_b64":"CIiyDq39TPFDPs1nO5V2qb6VYQ5Myd7904+/QuKfBvEt+AVuIzBzzkSSX9AgqknWwKaPKDe/9+4+ATb4N1HDCA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"df3f89d798ccd3cd441720991cfda5514a8b779a6c8b6fa53a480bf197d9aeab","last_reissued_at":"2026-07-05T07:11:57.916944Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T07:11:57.916944Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Equation of State of Cold Quark Matter to $O(\\alpha_s^3 \\ln \\alpha_s)$","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE","nucl-th"],"primary_cat":"hep-ph","authors_text":"Kaapo Sepp\\\"anen, Risto Paatelainen, Saga S\\\"appi, Tyler Gorda","submitted_at":"2023-07-17T18:00:01Z","abstract_excerpt":"Accurately understanding the equation of state (EOS) of high-density, zero-temperature quark matter plays an essential role in constraining the behavior of dense strongly interacting matter inside the cores of neutron stars. In this Letter, we study the weak-coupling expansion of the EOS of cold quark matter and derive the complete, gauge-invariant contributions from the long-wavelength, dynamically screened gluonic sector at next-to-next-to-next-to-leading order (N3LO) in the strong coupling constant $\\alpha_s$. This elevates the EOS result to the $O(\\alpha_s^3 \\ln \\alpha_s)$ level, leaving o"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2307.08734","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/2307.08734/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":"2307.08734","created_at":"2026-07-05T07:11:57.917003+00:00"},{"alias_kind":"arxiv_version","alias_value":"2307.08734v2","created_at":"2026-07-05T07:11:57.917003+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2307.08734","created_at":"2026-07-05T07:11:57.917003+00:00"},{"alias_kind":"pith_short_12","alias_value":"347YTV4YZTJ4","created_at":"2026-07-05T07:11:57.917003+00:00"},{"alias_kind":"pith_short_16","alias_value":"347YTV4YZTJ42RAX","created_at":"2026-07-05T07:11:57.917003+00:00"},{"alias_kind":"pith_short_8","alias_value":"347YTV4Y","created_at":"2026-07-05T07:11:57.917003+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":3,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2605.08584","citing_title":"The Non-parametric Equation of State Realizes a Generalized Quark-Hadron Crossover","ref_index":71,"is_internal_anchor":false},{"citing_arxiv_id":"2606.29576","citing_title":"Quark and hybrid stars with renormalization group improvement of NNLO perturbative QCD","ref_index":30,"is_internal_anchor":false},{"citing_arxiv_id":"2605.08584","citing_title":"The Non-parametric Equation of State Realizes a Generalized Quark-Hadron Crossover","ref_index":48,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/347YTV4YZTJ42RAXECMRZ7NFKF","json":"https://pith.science/pith/347YTV4YZTJ42RAXECMRZ7NFKF.json","graph_json":"https://pith.science/api/pith-number/347YTV4YZTJ42RAXECMRZ7NFKF/graph.json","events_json":"https://pith.science/api/pith-number/347YTV4YZTJ42RAXECMRZ7NFKF/events.json","paper":"https://pith.science/paper/347YTV4Y"},"agent_actions":{"view_html":"https://pith.science/pith/347YTV4YZTJ42RAXECMRZ7NFKF","download_json":"https://pith.science/pith/347YTV4YZTJ42RAXECMRZ7NFKF.json","view_paper":"https://pith.science/paper/347YTV4Y","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2307.08734&json=true","fetch_graph":"https://pith.science/api/pith-number/347YTV4YZTJ42RAXECMRZ7NFKF/graph.json","fetch_events":"https://pith.science/api/pith-number/347YTV4YZTJ42RAXECMRZ7NFKF/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/347YTV4YZTJ42RAXECMRZ7NFKF/action/timestamp_anchor","attest_storage":"https://pith.science/pith/347YTV4YZTJ42RAXECMRZ7NFKF/action/storage_attestation","attest_author":"https://pith.science/pith/347YTV4YZTJ42RAXECMRZ7NFKF/action/author_attestation","sign_citation":"https://pith.science/pith/347YTV4YZTJ42RAXECMRZ7NFKF/action/citation_signature","submit_replication":"https://pith.science/pith/347YTV4YZTJ42RAXECMRZ7NFKF/action/replication_record"}},"created_at":"2026-07-05T07:11:57.917003+00:00","updated_at":"2026-07-05T07:11:57.917003+00:00"}