{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2025:D4VYTZ5NFLTXWYFSV7XQ53SXGY","short_pith_number":"pith:D4VYTZ5N","schema_version":"1.0","canonical_sha256":"1f2b89e7ad2ae77b60b2afef0eee573632030b90b742b74d3f295fc5eaae3b32","source":{"kind":"arxiv","id":"2512.05315","version":2},"attestation_state":"computed","paper":{"title":"Nuclear parameter inference with semi-agnostic priors","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["nucl-th"],"primary_cat":"astro-ph.HE","authors_text":"Anthea F. Fantina, Francesca Gulminelli, Jocelyn Read, Lami Suleiman","submitted_at":"2025-12-04T23:26:38Z","abstract_excerpt":"Radio pulsar timing, X-ray pulse profile modeling, and gravitational-wave detections of binary mergers involving at least one neutron star probe the properties of dense, neutron-rich matter in thermodynamic regimes inaccessible to nuclear laboratories. Such inference relies on building appropriate equation-of-state priors, such as the recently introduced semi-agnostic constructions that incorporate nuclear theory and experimental information available in low- to intermediate-density regimes, while offering the necessary flexibility at high density. In this paper, we assess how detections of ma"},"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":"2512.05315","kind":"arxiv","version":2},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.HE","submitted_at":"2025-12-04T23:26:38Z","cross_cats_sorted":["nucl-th"],"title_canon_sha256":"6859c51bc1a4d6d7d26bb78b123eff558017c7f73732aa613b59a3f95488d879","abstract_canon_sha256":"5bb18839bc9cea623909ee5d03597a86a1f980a058547f387bf3d9fb2712111a"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-08-12T01:24:15.268577Z","signature_b64":"2bIib5DAf3EE2dp5YzLVgCGjRTlZzzn7aD49mhkkIljDPoQ3kvGgeq7Shdx2mCqh7SLM53asIupYPK8RgACzBQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"1f2b89e7ad2ae77b60b2afef0eee573632030b90b742b74d3f295fc5eaae3b32","last_reissued_at":"2026-08-12T01:24:15.266481Z","signature_status":"signed_v1","first_computed_at":"2026-08-12T01:24:15.266481Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Nuclear parameter inference with semi-agnostic priors","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["nucl-th"],"primary_cat":"astro-ph.HE","authors_text":"Anthea F. Fantina, Francesca Gulminelli, Jocelyn Read, Lami Suleiman","submitted_at":"2025-12-04T23:26:38Z","abstract_excerpt":"Radio pulsar timing, X-ray pulse profile modeling, and gravitational-wave detections of binary mergers involving at least one neutron star probe the properties of dense, neutron-rich matter in thermodynamic regimes inaccessible to nuclear laboratories. Such inference relies on building appropriate equation-of-state priors, such as the recently introduced semi-agnostic constructions that incorporate nuclear theory and experimental information available in low- to intermediate-density regimes, while offering the necessary flexibility at high density. In this paper, we assess how detections of ma"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2512.05315","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/2512.05315/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":"2512.05315","created_at":"2026-08-12T01:24:15.270549+00:00"},{"alias_kind":"arxiv_version","alias_value":"2512.05315v2","created_at":"2026-08-12T01:24:15.270549+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2512.05315","created_at":"2026-08-12T01:24:15.270549+00:00"},{"alias_kind":"pith_short_12","alias_value":"D4VYTZ5NFLTX","created_at":"2026-08-12T01:24:15.270549+00:00"},{"alias_kind":"pith_short_16","alias_value":"D4VYTZ5NFLTXWYFS","created_at":"2026-08-12T01:24:15.270549+00:00"},{"alias_kind":"pith_short_8","alias_value":"D4VYTZ5N","created_at":"2026-08-12T01:24:15.270549+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":2,"internal_anchor_count":2,"sample":[{"citing_arxiv_id":"2607.08412","citing_title":"Relativistic Mean Field Approach with Chiral Symmetry Breaking and Quark Confinement in the light of Astrophysical Observations","ref_index":50,"is_internal_anchor":true},{"citing_arxiv_id":"2604.05428","citing_title":"Reconstruction of fast-rotating neutron star observables with the neural network","ref_index":65,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/D4VYTZ5NFLTXWYFSV7XQ53SXGY","json":"https://pith.science/pith/D4VYTZ5NFLTXWYFSV7XQ53SXGY.json","graph_json":"https://pith.science/api/pith-number/D4VYTZ5NFLTXWYFSV7XQ53SXGY/graph.json","events_json":"https://pith.science/api/pith-number/D4VYTZ5NFLTXWYFSV7XQ53SXGY/events.json","paper":"https://pith.science/paper/D4VYTZ5N"},"agent_actions":{"view_html":"https://pith.science/pith/D4VYTZ5NFLTXWYFSV7XQ53SXGY","download_json":"https://pith.science/pith/D4VYTZ5NFLTXWYFSV7XQ53SXGY.json","view_paper":"https://pith.science/paper/D4VYTZ5N","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2512.05315&json=true","fetch_graph":"https://pith.science/api/pith-number/D4VYTZ5NFLTXWYFSV7XQ53SXGY/graph.json","fetch_events":"https://pith.science/api/pith-number/D4VYTZ5NFLTXWYFSV7XQ53SXGY/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/D4VYTZ5NFLTXWYFSV7XQ53SXGY/action/timestamp_anchor","attest_storage":"https://pith.science/pith/D4VYTZ5NFLTXWYFSV7XQ53SXGY/action/storage_attestation","attest_author":"https://pith.science/pith/D4VYTZ5NFLTXWYFSV7XQ53SXGY/action/author_attestation","sign_citation":"https://pith.science/pith/D4VYTZ5NFLTXWYFSV7XQ53SXGY/action/citation_signature","submit_replication":"https://pith.science/pith/D4VYTZ5NFLTXWYFSV7XQ53SXGY/action/replication_record"}},"created_at":"2026-08-12T01:24:15.270549+00:00","updated_at":"2026-08-12T01:24:15.270549+00:00"}