{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2015:HDODAA6YIBPVQ5YCRMQDPQBFPM","short_pith_number":"pith:HDODAA6Y","schema_version":"1.0","canonical_sha256":"38dc3003d8405f5877028b2037c0257b0b4a42541f7df70a286f38481c245971","source":{"kind":"arxiv","id":"1502.02929","version":3},"attestation_state":"computed","paper":{"title":"Neutron stars in Einstein-$\\Lambda$ gravity: the cosmological constant effects","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"B. Eslam Panah, G. H. Bordbar, S. H. Hendi","submitted_at":"2015-02-10T15:00:39Z","abstract_excerpt":"Regarding a $d-$dimensional spherically symmetric line element in the context of Einstein-$\\Lambda$ gravity, the hydrostatic equilibrium equation of stars is obtained. Then, by using the lowest order constrained variational (LOCV) method with the AV$18$ potential and employing microscopic many body calculations in the modern equation of state, the structure properties of neutron stars are investigated. Regardless of cosmological point of view and considering arbitrary positive and negative values of the cosmological constant, the maximum mass of the neutron stars and their corresponding radius"},"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":"1502.02929","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2015-02-10T15:00:39Z","cross_cats_sorted":[],"title_canon_sha256":"7ce85dd739127096327b1b25b685e66348bd7f6d78cd474ca4ed005e89c0604c","abstract_canon_sha256":"3f90b90b309aee44b669d5be90a42eff16434f13b1542ea2266bde022573861b"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:52:02.375769Z","signature_b64":"1zxUCOka/1N1scl7/Hd10YjnBt2T6KapshFwV3jbCVmHIFMNQxEuMKOeLfQOI0MdHi4/yHWJ8bZfSbcSNWFcAA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"38dc3003d8405f5877028b2037c0257b0b4a42541f7df70a286f38481c245971","last_reissued_at":"2026-05-18T00:52:02.375213Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:52:02.375213Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Neutron stars in Einstein-$\\Lambda$ gravity: the cosmological constant effects","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"B. Eslam Panah, G. H. Bordbar, S. H. Hendi","submitted_at":"2015-02-10T15:00:39Z","abstract_excerpt":"Regarding a $d-$dimensional spherically symmetric line element in the context of Einstein-$\\Lambda$ gravity, the hydrostatic equilibrium equation of stars is obtained. Then, by using the lowest order constrained variational (LOCV) method with the AV$18$ potential and employing microscopic many body calculations in the modern equation of state, the structure properties of neutron stars are investigated. Regardless of cosmological point of view and considering arbitrary positive and negative values of the cosmological constant, the maximum mass of the neutron stars and their corresponding radius"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1502.02929","kind":"arxiv","version":3},"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":"1502.02929","created_at":"2026-05-18T00:52:02.375292+00:00"},{"alias_kind":"arxiv_version","alias_value":"1502.02929v3","created_at":"2026-05-18T00:52:02.375292+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1502.02929","created_at":"2026-05-18T00:52:02.375292+00:00"},{"alias_kind":"pith_short_12","alias_value":"HDODAA6YIBPV","created_at":"2026-05-18T12:29:25.134429+00:00"},{"alias_kind":"pith_short_16","alias_value":"HDODAA6YIBPVQ5YC","created_at":"2026-05-18T12:29:25.134429+00:00"},{"alias_kind":"pith_short_8","alias_value":"HDODAA6Y","created_at":"2026-05-18T12:29:25.134429+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/HDODAA6YIBPVQ5YCRMQDPQBFPM","json":"https://pith.science/pith/HDODAA6YIBPVQ5YCRMQDPQBFPM.json","graph_json":"https://pith.science/api/pith-number/HDODAA6YIBPVQ5YCRMQDPQBFPM/graph.json","events_json":"https://pith.science/api/pith-number/HDODAA6YIBPVQ5YCRMQDPQBFPM/events.json","paper":"https://pith.science/paper/HDODAA6Y"},"agent_actions":{"view_html":"https://pith.science/pith/HDODAA6YIBPVQ5YCRMQDPQBFPM","download_json":"https://pith.science/pith/HDODAA6YIBPVQ5YCRMQDPQBFPM.json","view_paper":"https://pith.science/paper/HDODAA6Y","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1502.02929&json=true","fetch_graph":"https://pith.science/api/pith-number/HDODAA6YIBPVQ5YCRMQDPQBFPM/graph.json","fetch_events":"https://pith.science/api/pith-number/HDODAA6YIBPVQ5YCRMQDPQBFPM/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/HDODAA6YIBPVQ5YCRMQDPQBFPM/action/timestamp_anchor","attest_storage":"https://pith.science/pith/HDODAA6YIBPVQ5YCRMQDPQBFPM/action/storage_attestation","attest_author":"https://pith.science/pith/HDODAA6YIBPVQ5YCRMQDPQBFPM/action/author_attestation","sign_citation":"https://pith.science/pith/HDODAA6YIBPVQ5YCRMQDPQBFPM/action/citation_signature","submit_replication":"https://pith.science/pith/HDODAA6YIBPVQ5YCRMQDPQBFPM/action/replication_record"}},"created_at":"2026-05-18T00:52:02.375292+00:00","updated_at":"2026-05-18T00:52:02.375292+00:00"}