{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2015:4NHSCED7YFUIYS3H7RON6LOU7E","short_pith_number":"pith:4NHSCED7","schema_version":"1.0","canonical_sha256":"e34f21107fc1688c4b67fc5cdf2dd4f910eb14a8ac183c01bd85db0d7ba8d120","source":{"kind":"arxiv","id":"1510.03969","version":1},"attestation_state":"computed","paper":{"title":"Shedding Light on the EOS-Gravity Degeneracy and Constraining the Nuclear Symmetry Energy from the Gravitational Binding Energy of Neutron Stars","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.SR","gr-qc","nucl-ex"],"primary_cat":"nucl-th","authors_text":"Bao-An Li, F. J. Fattoyev, W. G. Newton, Xiao-Tao He","submitted_at":"2015-10-14T05:38:41Z","abstract_excerpt":"A thorough understanding of properties of neutron stars requires both a reliable knowledge of the equation of state (EOS) of super-dense nuclear matter and the strong-field gravity theories simultaneously. To provide information that may help break this EOS-gravity degeneracy, we investigate effects of nuclear symmetry energy on the gravitational binding energy of neutron stars within GR and the scalar-tensor subset of alternative gravity models. We focus on effects of the slope $L$ of nuclear symmetry energy at saturation density and the high-density behavior of nuclear symmetry energy. We fi"},"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":"1510.03969","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"nucl-th","submitted_at":"2015-10-14T05:38:41Z","cross_cats_sorted":["astro-ph.SR","gr-qc","nucl-ex"],"title_canon_sha256":"3c928564e9a24d3a049646c73e5202d02e9295f886802d66c1f8bb62d2751a4f","abstract_canon_sha256":"bab8342a2cbf64162d7ad93ead4908588892c9c2246d1e857cf3f0e447e50153"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:16:34.913278Z","signature_b64":"at+xPKVdZibtS6K8sudMyK2yLLA4vUBGXedPcWJCeGcKZU2Jwt8W18NaT6PUGQPKivsc1KppMVhr4W2mnsJvCQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"e34f21107fc1688c4b67fc5cdf2dd4f910eb14a8ac183c01bd85db0d7ba8d120","last_reissued_at":"2026-05-18T01:16:34.912618Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:16:34.912618Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Shedding Light on the EOS-Gravity Degeneracy and Constraining the Nuclear Symmetry Energy from the Gravitational Binding Energy of Neutron Stars","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.SR","gr-qc","nucl-ex"],"primary_cat":"nucl-th","authors_text":"Bao-An Li, F. J. Fattoyev, W. G. Newton, Xiao-Tao He","submitted_at":"2015-10-14T05:38:41Z","abstract_excerpt":"A thorough understanding of properties of neutron stars requires both a reliable knowledge of the equation of state (EOS) of super-dense nuclear matter and the strong-field gravity theories simultaneously. To provide information that may help break this EOS-gravity degeneracy, we investigate effects of nuclear symmetry energy on the gravitational binding energy of neutron stars within GR and the scalar-tensor subset of alternative gravity models. We focus on effects of the slope $L$ of nuclear symmetry energy at saturation density and the high-density behavior of nuclear symmetry energy. We fi"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1510.03969","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":""},"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":"1510.03969","created_at":"2026-05-18T01:16:34.912728+00:00"},{"alias_kind":"arxiv_version","alias_value":"1510.03969v1","created_at":"2026-05-18T01:16:34.912728+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1510.03969","created_at":"2026-05-18T01:16:34.912728+00:00"},{"alias_kind":"pith_short_12","alias_value":"4NHSCED7YFUI","created_at":"2026-05-18T12:29:05.191682+00:00"},{"alias_kind":"pith_short_16","alias_value":"4NHSCED7YFUIYS3H","created_at":"2026-05-18T12:29:05.191682+00:00"},{"alias_kind":"pith_short_8","alias_value":"4NHSCED7","created_at":"2026-05-18T12:29:05.191682+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/4NHSCED7YFUIYS3H7RON6LOU7E","json":"https://pith.science/pith/4NHSCED7YFUIYS3H7RON6LOU7E.json","graph_json":"https://pith.science/api/pith-number/4NHSCED7YFUIYS3H7RON6LOU7E/graph.json","events_json":"https://pith.science/api/pith-number/4NHSCED7YFUIYS3H7RON6LOU7E/events.json","paper":"https://pith.science/paper/4NHSCED7"},"agent_actions":{"view_html":"https://pith.science/pith/4NHSCED7YFUIYS3H7RON6LOU7E","download_json":"https://pith.science/pith/4NHSCED7YFUIYS3H7RON6LOU7E.json","view_paper":"https://pith.science/paper/4NHSCED7","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1510.03969&json=true","fetch_graph":"https://pith.science/api/pith-number/4NHSCED7YFUIYS3H7RON6LOU7E/graph.json","fetch_events":"https://pith.science/api/pith-number/4NHSCED7YFUIYS3H7RON6LOU7E/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/4NHSCED7YFUIYS3H7RON6LOU7E/action/timestamp_anchor","attest_storage":"https://pith.science/pith/4NHSCED7YFUIYS3H7RON6LOU7E/action/storage_attestation","attest_author":"https://pith.science/pith/4NHSCED7YFUIYS3H7RON6LOU7E/action/author_attestation","sign_citation":"https://pith.science/pith/4NHSCED7YFUIYS3H7RON6LOU7E/action/citation_signature","submit_replication":"https://pith.science/pith/4NHSCED7YFUIYS3H7RON6LOU7E/action/replication_record"}},"created_at":"2026-05-18T01:16:34.912728+00:00","updated_at":"2026-05-18T01:16:34.912728+00:00"}