{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:RVERZMI2ZVBRDFIU7XZDTFZTNL","short_pith_number":"pith:RVERZMI2","schema_version":"1.0","canonical_sha256":"8d491cb11acd43119514fdf23997336afc5762be185546e2dce8d5ffb96e2da7","source":{"kind":"arxiv","id":"1708.04837","version":4},"attestation_state":"computed","paper":{"title":"Neutron stars in the braneworld within the Eddington-inspired Born-Infeld gravity","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc"],"primary_cat":"astro-ph.CO","authors_text":"A. I. Qauli, A. Sulaksono, H. S. Ramadhan, I. Husin, I. Prasetyo","submitted_at":"2017-08-16T10:34:49Z","abstract_excerpt":"We propose the disappearance of \"the hyperon puzzle\" in neutron star (NS) by invoking two new-physics prescriptions: modified gravity theory and braneworld scenario. By assuming that NS lives on a $3$-brane within a $5d$ empty AdS bulk, gravitationally governed by Eddington-inspired Born-Infeld (EiBI) theory, the field equations can be effectively cast into the usual Einstein's with \"apparent\" anisotropic energy-momentum tensor. Solving the corresponding brane-TOV equations numerically, we study its mass-radius relation. It is known that the appearance of finite brane tension $\\lambda$ reduces"},"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":"1708.04837","kind":"arxiv","version":4},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2017-08-16T10:34:49Z","cross_cats_sorted":["gr-qc"],"title_canon_sha256":"21650e0e1d8c256d59d97140820d8d09569e262968563d8f0b395757dce880a7","abstract_canon_sha256":"49733f60a927e224323c166e624f792ba7ca712758b0fc782cfbb9bac823b04c"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:24:51.957422Z","signature_b64":"J+CDSQKK6YK2v3AHIFGaR0DdgM86Bza63EuQmZyBtRYCav3RqWH36DrJOp4uNq0VHgTtrVabAfbk61Kt9LBXBw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"8d491cb11acd43119514fdf23997336afc5762be185546e2dce8d5ffb96e2da7","last_reissued_at":"2026-05-18T00:24:51.956634Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:24:51.956634Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Neutron stars in the braneworld within the Eddington-inspired Born-Infeld gravity","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc"],"primary_cat":"astro-ph.CO","authors_text":"A. I. Qauli, A. Sulaksono, H. S. Ramadhan, I. Husin, I. Prasetyo","submitted_at":"2017-08-16T10:34:49Z","abstract_excerpt":"We propose the disappearance of \"the hyperon puzzle\" in neutron star (NS) by invoking two new-physics prescriptions: modified gravity theory and braneworld scenario. By assuming that NS lives on a $3$-brane within a $5d$ empty AdS bulk, gravitationally governed by Eddington-inspired Born-Infeld (EiBI) theory, the field equations can be effectively cast into the usual Einstein's with \"apparent\" anisotropic energy-momentum tensor. Solving the corresponding brane-TOV equations numerically, we study its mass-radius relation. It is known that the appearance of finite brane tension $\\lambda$ reduces"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1708.04837","kind":"arxiv","version":4},"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":"1708.04837","created_at":"2026-05-18T00:24:51.956757+00:00"},{"alias_kind":"arxiv_version","alias_value":"1708.04837v4","created_at":"2026-05-18T00:24:51.956757+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1708.04837","created_at":"2026-05-18T00:24:51.956757+00:00"},{"alias_kind":"pith_short_12","alias_value":"RVERZMI2ZVBR","created_at":"2026-05-18T12:31:43.269735+00:00"},{"alias_kind":"pith_short_16","alias_value":"RVERZMI2ZVBRDFIU","created_at":"2026-05-18T12:31:43.269735+00:00"},{"alias_kind":"pith_short_8","alias_value":"RVERZMI2","created_at":"2026-05-18T12:31:43.269735+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2605.26124","citing_title":"Astrophysical environment around a black hole in the braneworld and its optical signatures","ref_index":30,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/RVERZMI2ZVBRDFIU7XZDTFZTNL","json":"https://pith.science/pith/RVERZMI2ZVBRDFIU7XZDTFZTNL.json","graph_json":"https://pith.science/api/pith-number/RVERZMI2ZVBRDFIU7XZDTFZTNL/graph.json","events_json":"https://pith.science/api/pith-number/RVERZMI2ZVBRDFIU7XZDTFZTNL/events.json","paper":"https://pith.science/paper/RVERZMI2"},"agent_actions":{"view_html":"https://pith.science/pith/RVERZMI2ZVBRDFIU7XZDTFZTNL","download_json":"https://pith.science/pith/RVERZMI2ZVBRDFIU7XZDTFZTNL.json","view_paper":"https://pith.science/paper/RVERZMI2","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1708.04837&json=true","fetch_graph":"https://pith.science/api/pith-number/RVERZMI2ZVBRDFIU7XZDTFZTNL/graph.json","fetch_events":"https://pith.science/api/pith-number/RVERZMI2ZVBRDFIU7XZDTFZTNL/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/RVERZMI2ZVBRDFIU7XZDTFZTNL/action/timestamp_anchor","attest_storage":"https://pith.science/pith/RVERZMI2ZVBRDFIU7XZDTFZTNL/action/storage_attestation","attest_author":"https://pith.science/pith/RVERZMI2ZVBRDFIU7XZDTFZTNL/action/author_attestation","sign_citation":"https://pith.science/pith/RVERZMI2ZVBRDFIU7XZDTFZTNL/action/citation_signature","submit_replication":"https://pith.science/pith/RVERZMI2ZVBRDFIU7XZDTFZTNL/action/replication_record"}},"created_at":"2026-05-18T00:24:51.956757+00:00","updated_at":"2026-05-18T00:24:51.956757+00:00"}