{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2014:BUBBNKLSKCGFFNOR5JCFAXZ2YL","short_pith_number":"pith:BUBBNKLS","schema_version":"1.0","canonical_sha256":"0d0216a972508c52b5d1ea44505f3ac2dd8ea586245c832b3a97dadef1ee5093","source":{"kind":"arxiv","id":"1409.7385","version":2},"attestation_state":"computed","paper":{"title":"Newtonian View of General Relativistic Stars","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"gr-qc","authors_text":"A. M. Oliveira, H. E. S. Velten, I. G. Salako, J. C. Fabris","submitted_at":"2014-09-25T13:09:12Z","abstract_excerpt":"Although general relativistic cosmological solutions, even in the presence of pressure, can be mimicked by using neo-Newtonian hydrodynamics, it is not clear whether there exists the same Newtonian correspondence for spherical static configurations. General relativity solutions for stars are known as the Tolman-Oppenheimer-Volkoff (TOV) equations. On the other hand, the Newtonian description does not take into account the total pressure effects and therefore can not be used in strong field regimes. We discuss how to incorporate pressure in the stellar equilibrium equations within the neo-Newto"},"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":"1409.7385","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2014-09-25T13:09:12Z","cross_cats_sorted":["astro-ph.CO"],"title_canon_sha256":"ad9b95bf6f321ff31d46a761d03e9ba07de2c75339acf47fa85f2e9bbaa97abb","abstract_canon_sha256":"fa790823e3edc431441e29d404c7bd6fa909da56018f4cc08d219d5417e1b24c"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:41:56.804941Z","signature_b64":"x1lkIC0y/yOEWW1JCUFWcmj5e+ljZOoK8jv42ajG4vhBGiM00RnUuYtYUR/jJsTUoL7+Ehk8QWHBI2G6pVRxAw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"0d0216a972508c52b5d1ea44505f3ac2dd8ea586245c832b3a97dadef1ee5093","last_reissued_at":"2026-05-18T01:41:56.804376Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:41:56.804376Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Newtonian View of General Relativistic Stars","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"gr-qc","authors_text":"A. M. Oliveira, H. E. S. Velten, I. G. Salako, J. C. Fabris","submitted_at":"2014-09-25T13:09:12Z","abstract_excerpt":"Although general relativistic cosmological solutions, even in the presence of pressure, can be mimicked by using neo-Newtonian hydrodynamics, it is not clear whether there exists the same Newtonian correspondence for spherical static configurations. General relativity solutions for stars are known as the Tolman-Oppenheimer-Volkoff (TOV) equations. On the other hand, the Newtonian description does not take into account the total pressure effects and therefore can not be used in strong field regimes. We discuss how to incorporate pressure in the stellar equilibrium equations within the neo-Newto"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1409.7385","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":""},"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":"1409.7385","created_at":"2026-05-18T01:41:56.804472+00:00"},{"alias_kind":"arxiv_version","alias_value":"1409.7385v2","created_at":"2026-05-18T01:41:56.804472+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1409.7385","created_at":"2026-05-18T01:41:56.804472+00:00"},{"alias_kind":"pith_short_12","alias_value":"BUBBNKLSKCGF","created_at":"2026-05-18T12:28:22.404517+00:00"},{"alias_kind":"pith_short_16","alias_value":"BUBBNKLSKCGFFNOR","created_at":"2026-05-18T12:28:22.404517+00:00"},{"alias_kind":"pith_short_8","alias_value":"BUBBNKLS","created_at":"2026-05-18T12:28:22.404517+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":0,"internal_anchor_count":0,"sample":[]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/BUBBNKLSKCGFFNOR5JCFAXZ2YL","json":"https://pith.science/pith/BUBBNKLSKCGFFNOR5JCFAXZ2YL.json","graph_json":"https://pith.science/api/pith-number/BUBBNKLSKCGFFNOR5JCFAXZ2YL/graph.json","events_json":"https://pith.science/api/pith-number/BUBBNKLSKCGFFNOR5JCFAXZ2YL/events.json","paper":"https://pith.science/paper/BUBBNKLS"},"agent_actions":{"view_html":"https://pith.science/pith/BUBBNKLSKCGFFNOR5JCFAXZ2YL","download_json":"https://pith.science/pith/BUBBNKLSKCGFFNOR5JCFAXZ2YL.json","view_paper":"https://pith.science/paper/BUBBNKLS","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1409.7385&json=true","fetch_graph":"https://pith.science/api/pith-number/BUBBNKLSKCGFFNOR5JCFAXZ2YL/graph.json","fetch_events":"https://pith.science/api/pith-number/BUBBNKLSKCGFFNOR5JCFAXZ2YL/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/BUBBNKLSKCGFFNOR5JCFAXZ2YL/action/timestamp_anchor","attest_storage":"https://pith.science/pith/BUBBNKLSKCGFFNOR5JCFAXZ2YL/action/storage_attestation","attest_author":"https://pith.science/pith/BUBBNKLSKCGFFNOR5JCFAXZ2YL/action/author_attestation","sign_citation":"https://pith.science/pith/BUBBNKLSKCGFFNOR5JCFAXZ2YL/action/citation_signature","submit_replication":"https://pith.science/pith/BUBBNKLSKCGFFNOR5JCFAXZ2YL/action/replication_record"}},"created_at":"2026-05-18T01:41:56.804472+00:00","updated_at":"2026-05-18T01:41:56.804472+00:00"}