{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:6Y6HLBGUSUXXAI4G7RLB7WRC5H","short_pith_number":"pith:6Y6HLBGU","schema_version":"1.0","canonical_sha256":"f63c7584d4952f702386fc561fda22e9ebf6a9c5e85d879a23253d18b7dcdfc3","source":{"kind":"arxiv","id":"2411.18349","version":2},"attestation_state":"computed","paper":{"title":"High density symmetry energy: A key to the solution of the hyperon puzzle","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.HE","hep-ph","nucl-ex"],"primary_cat":"nucl-th","authors_text":"Jun-Ting Ye, Lie-Wen Chen, Rui Wang, Si-Pei Wang","submitted_at":"2024-11-27T13:52:59Z","abstract_excerpt":"The recently developed nuclear effective interaction based on the so-called N3LO Skyrme pseudopotential is extended to include the hyperon-nucleon and hyperon-hyperon interactions by assuming the similar density, momentum, and isospin dependence as for the nucleon-nucleon interaction. The parameters in these interactions are determined from either experimental information if any or chiral effective field theory or lattice QCD calculations of the hyperon potentials in nuclear matter around nuclear saturation density $\\rho_0$. We find that varying the high density behavior of the symmetry energy"},"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":"2411.18349","kind":"arxiv","version":2},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"nucl-th","submitted_at":"2024-11-27T13:52:59Z","cross_cats_sorted":["astro-ph.HE","hep-ph","nucl-ex"],"title_canon_sha256":"1d18162cea9d2779ed087422576a6741ecf1a3dc0318de3973ff7c389867d2ef","abstract_canon_sha256":"c297359df090b1079e275c6f94fdfd3fecc62ad9d18c01d844d5c7a4a4e4bdbb"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T10:52:38.551831Z","signature_b64":"0uhMVayrkLXiOZcvAG5n6qvH+NyoYnWls7WIHby6DQL0XkjXHqJowY7WkvW2pgOED6RP3tfj3+9KAoIPfwrNAw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"f63c7584d4952f702386fc561fda22e9ebf6a9c5e85d879a23253d18b7dcdfc3","last_reissued_at":"2026-07-05T10:52:38.551352Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T10:52:38.551352Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"High density symmetry energy: A key to the solution of the hyperon puzzle","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.HE","hep-ph","nucl-ex"],"primary_cat":"nucl-th","authors_text":"Jun-Ting Ye, Lie-Wen Chen, Rui Wang, Si-Pei Wang","submitted_at":"2024-11-27T13:52:59Z","abstract_excerpt":"The recently developed nuclear effective interaction based on the so-called N3LO Skyrme pseudopotential is extended to include the hyperon-nucleon and hyperon-hyperon interactions by assuming the similar density, momentum, and isospin dependence as for the nucleon-nucleon interaction. The parameters in these interactions are determined from either experimental information if any or chiral effective field theory or lattice QCD calculations of the hyperon potentials in nuclear matter around nuclear saturation density $\\rho_0$. We find that varying the high density behavior of the symmetry energy"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2411.18349","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/2411.18349/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":"2411.18349","created_at":"2026-07-05T10:52:38.551412+00:00"},{"alias_kind":"arxiv_version","alias_value":"2411.18349v2","created_at":"2026-07-05T10:52:38.551412+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2411.18349","created_at":"2026-07-05T10:52:38.551412+00:00"},{"alias_kind":"pith_short_12","alias_value":"6Y6HLBGUSUXX","created_at":"2026-07-05T10:52:38.551412+00:00"},{"alias_kind":"pith_short_16","alias_value":"6Y6HLBGUSUXXAI4G","created_at":"2026-07-05T10:52:38.551412+00:00"},{"alias_kind":"pith_short_8","alias_value":"6Y6HLBGU","created_at":"2026-07-05T10:52:38.551412+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2505.00390","citing_title":"Neutron Star Radii from Laboratory Experiments","ref_index":144,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/6Y6HLBGUSUXXAI4G7RLB7WRC5H","json":"https://pith.science/pith/6Y6HLBGUSUXXAI4G7RLB7WRC5H.json","graph_json":"https://pith.science/api/pith-number/6Y6HLBGUSUXXAI4G7RLB7WRC5H/graph.json","events_json":"https://pith.science/api/pith-number/6Y6HLBGUSUXXAI4G7RLB7WRC5H/events.json","paper":"https://pith.science/paper/6Y6HLBGU"},"agent_actions":{"view_html":"https://pith.science/pith/6Y6HLBGUSUXXAI4G7RLB7WRC5H","download_json":"https://pith.science/pith/6Y6HLBGUSUXXAI4G7RLB7WRC5H.json","view_paper":"https://pith.science/paper/6Y6HLBGU","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2411.18349&json=true","fetch_graph":"https://pith.science/api/pith-number/6Y6HLBGUSUXXAI4G7RLB7WRC5H/graph.json","fetch_events":"https://pith.science/api/pith-number/6Y6HLBGUSUXXAI4G7RLB7WRC5H/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/6Y6HLBGUSUXXAI4G7RLB7WRC5H/action/timestamp_anchor","attest_storage":"https://pith.science/pith/6Y6HLBGUSUXXAI4G7RLB7WRC5H/action/storage_attestation","attest_author":"https://pith.science/pith/6Y6HLBGUSUXXAI4G7RLB7WRC5H/action/author_attestation","sign_citation":"https://pith.science/pith/6Y6HLBGUSUXXAI4G7RLB7WRC5H/action/citation_signature","submit_replication":"https://pith.science/pith/6Y6HLBGUSUXXAI4G7RLB7WRC5H/action/replication_record"}},"created_at":"2026-07-05T10:52:38.551412+00:00","updated_at":"2026-07-05T10:52:38.551412+00:00"}