{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2025:NV7G4QK2ECWHGGAQTFFXIQDPYU","short_pith_number":"pith:NV7G4QK2","schema_version":"1.0","canonical_sha256":"6d7e6e415a20ac731810994b74406fc52a59aa00f11c95182d52bf50aac6ca3d","source":{"kind":"arxiv","id":"2501.17185","version":1},"attestation_state":"computed","paper":{"title":"Relativistic chiral nuclear forces: status and prospects","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-lat","hep-ph","nucl-ex"],"primary_cat":"nucl-th","authors_text":"Jun-Xu Lu, Li-Sheng Geng, Yang Xiao, Zhi-Wei Liu","submitted_at":"2025-01-26T08:42:50Z","abstract_excerpt":"Understanding nuclear structure, reactions, and the properties of neutron stars from \\textit{ab initio} calculations from the nucleon degrees of freedom has always been a primary goal of nuclear physics, in which the microscopic nuclear force serves as the fundamental input. So far, the Weinberg chiral nuclear force, first proposed by the Nobel laureate Weinberg, has become the \\textit{de facto} standard input for nuclear \\textit{ab initio} studies. However, compared to their non-relativistic counterparts, relativistic \\textit{ab initio} calculations, which describe better nuclear observables,"},"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":"2501.17185","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"nucl-th","submitted_at":"2025-01-26T08:42:50Z","cross_cats_sorted":["hep-lat","hep-ph","nucl-ex"],"title_canon_sha256":"4012b48227482c304bbf3f294438445ab7493f9ceae6c8c42de186d988effa80","abstract_canon_sha256":"caffce04ac032e738934e25c6849e2bd87fd3c56a5560bba1605c6c5089ced20"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T10:06:48.757546Z","signature_b64":"U6W7K4IAcfIJ/o6ynO1QBWyiLXseP7OGLZMqaFt3Z3CkOTFjG6lf+dfqm70YYBBuYd1s40jad1QKb77jGl9zBw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"6d7e6e415a20ac731810994b74406fc52a59aa00f11c95182d52bf50aac6ca3d","last_reissued_at":"2026-07-05T10:06:48.757051Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T10:06:48.757051Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Relativistic chiral nuclear forces: status and prospects","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-lat","hep-ph","nucl-ex"],"primary_cat":"nucl-th","authors_text":"Jun-Xu Lu, Li-Sheng Geng, Yang Xiao, Zhi-Wei Liu","submitted_at":"2025-01-26T08:42:50Z","abstract_excerpt":"Understanding nuclear structure, reactions, and the properties of neutron stars from \\textit{ab initio} calculations from the nucleon degrees of freedom has always been a primary goal of nuclear physics, in which the microscopic nuclear force serves as the fundamental input. So far, the Weinberg chiral nuclear force, first proposed by the Nobel laureate Weinberg, has become the \\textit{de facto} standard input for nuclear \\textit{ab initio} studies. However, compared to their non-relativistic counterparts, relativistic \\textit{ab initio} calculations, which describe better nuclear observables,"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2501.17185","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/2501.17185/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":"2501.17185","created_at":"2026-07-05T10:06:48.757118+00:00"},{"alias_kind":"arxiv_version","alias_value":"2501.17185v1","created_at":"2026-07-05T10:06:48.757118+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2501.17185","created_at":"2026-07-05T10:06:48.757118+00:00"},{"alias_kind":"pith_short_12","alias_value":"NV7G4QK2ECWH","created_at":"2026-07-05T10:06:48.757118+00:00"},{"alias_kind":"pith_short_16","alias_value":"NV7G4QK2ECWHGGAQ","created_at":"2026-07-05T10:06:48.757118+00:00"},{"alias_kind":"pith_short_8","alias_value":"NV7G4QK2","created_at":"2026-07-05T10:06:48.757118+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2506.00864","citing_title":"Perspectives for hyperon and hypernuclei physics","ref_index":80,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/NV7G4QK2ECWHGGAQTFFXIQDPYU","json":"https://pith.science/pith/NV7G4QK2ECWHGGAQTFFXIQDPYU.json","graph_json":"https://pith.science/api/pith-number/NV7G4QK2ECWHGGAQTFFXIQDPYU/graph.json","events_json":"https://pith.science/api/pith-number/NV7G4QK2ECWHGGAQTFFXIQDPYU/events.json","paper":"https://pith.science/paper/NV7G4QK2"},"agent_actions":{"view_html":"https://pith.science/pith/NV7G4QK2ECWHGGAQTFFXIQDPYU","download_json":"https://pith.science/pith/NV7G4QK2ECWHGGAQTFFXIQDPYU.json","view_paper":"https://pith.science/paper/NV7G4QK2","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2501.17185&json=true","fetch_graph":"https://pith.science/api/pith-number/NV7G4QK2ECWHGGAQTFFXIQDPYU/graph.json","fetch_events":"https://pith.science/api/pith-number/NV7G4QK2ECWHGGAQTFFXIQDPYU/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/NV7G4QK2ECWHGGAQTFFXIQDPYU/action/timestamp_anchor","attest_storage":"https://pith.science/pith/NV7G4QK2ECWHGGAQTFFXIQDPYU/action/storage_attestation","attest_author":"https://pith.science/pith/NV7G4QK2ECWHGGAQTFFXIQDPYU/action/author_attestation","sign_citation":"https://pith.science/pith/NV7G4QK2ECWHGGAQTFFXIQDPYU/action/citation_signature","submit_replication":"https://pith.science/pith/NV7G4QK2ECWHGGAQTFFXIQDPYU/action/replication_record"}},"created_at":"2026-07-05T10:06:48.757118+00:00","updated_at":"2026-07-05T10:06:48.757118+00:00"}