{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2014:B7SUYNFJZX7H6RKJMJGNVCEURX","short_pith_number":"pith:B7SUYNFJ","schema_version":"1.0","canonical_sha256":"0fe54c34a9cdfe7f4549624cda88948dea3deed7614fb49dceef23cdf79e4ddd","source":{"kind":"arxiv","id":"1410.7735","version":1},"attestation_state":"computed","paper":{"title":"Relativistic anisotropic star and its maximum mass in higher dimensions","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.SR"],"primary_cat":"gr-qc","authors_text":"Bikash Chandra Paul, Pradip Kumar Chattopadhyay, Shibshankar Kamakar","submitted_at":"2014-10-27T07:31:26Z","abstract_excerpt":"We present a class of relativistic solutions of cold compact anisotropic stars in hydrostatic equilibrium in the framework of higher dimensions using spheroidal geometry. The solutions obtained with Vaidya-Tikekar metric are used to construct stellar models of compact objects and studied their physical features. The effects of anisotropy and extra dimensions on the global properties namely, compactness, mass, radius, equation of state are determined in higher dimensions in terms of the spheroidicity parameter ($\\lambda$). It is noted that for a given configuration, compactness of a star is fou"},"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":"1410.7735","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2014-10-27T07:31:26Z","cross_cats_sorted":["astro-ph.SR"],"title_canon_sha256":"f9f0ca67b4c69c2996c33c2ce4d541bb30dca5f0c953e12c41dc3b38f645c821","abstract_canon_sha256":"26514ced5fddc1bb8817a9856eda02babe599c4b66715124a37988e368e0c95e"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:41:39.149515Z","signature_b64":"F/pCOcYdEt5Zy6F6Zmcqq8zip+f4zicxPTFOuASTaGI3tV8dzOCgfsiSCK1QMJl39l5VOBH55yb6/rr8k8IFCg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"0fe54c34a9cdfe7f4549624cda88948dea3deed7614fb49dceef23cdf79e4ddd","last_reissued_at":"2026-05-18T01:41:39.148902Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:41:39.148902Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Relativistic anisotropic star and its maximum mass in higher dimensions","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.SR"],"primary_cat":"gr-qc","authors_text":"Bikash Chandra Paul, Pradip Kumar Chattopadhyay, Shibshankar Kamakar","submitted_at":"2014-10-27T07:31:26Z","abstract_excerpt":"We present a class of relativistic solutions of cold compact anisotropic stars in hydrostatic equilibrium in the framework of higher dimensions using spheroidal geometry. The solutions obtained with Vaidya-Tikekar metric are used to construct stellar models of compact objects and studied their physical features. The effects of anisotropy and extra dimensions on the global properties namely, compactness, mass, radius, equation of state are determined in higher dimensions in terms of the spheroidicity parameter ($\\lambda$). It is noted that for a given configuration, compactness of a star is fou"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1410.7735","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":"1410.7735","created_at":"2026-05-18T01:41:39.148974+00:00"},{"alias_kind":"arxiv_version","alias_value":"1410.7735v1","created_at":"2026-05-18T01:41:39.148974+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1410.7735","created_at":"2026-05-18T01:41:39.148974+00:00"},{"alias_kind":"pith_short_12","alias_value":"B7SUYNFJZX7H","created_at":"2026-05-18T12:28:22.404517+00:00"},{"alias_kind":"pith_short_16","alias_value":"B7SUYNFJZX7H6RKJ","created_at":"2026-05-18T12:28:22.404517+00:00"},{"alias_kind":"pith_short_8","alias_value":"B7SUYNFJ","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/B7SUYNFJZX7H6RKJMJGNVCEURX","json":"https://pith.science/pith/B7SUYNFJZX7H6RKJMJGNVCEURX.json","graph_json":"https://pith.science/api/pith-number/B7SUYNFJZX7H6RKJMJGNVCEURX/graph.json","events_json":"https://pith.science/api/pith-number/B7SUYNFJZX7H6RKJMJGNVCEURX/events.json","paper":"https://pith.science/paper/B7SUYNFJ"},"agent_actions":{"view_html":"https://pith.science/pith/B7SUYNFJZX7H6RKJMJGNVCEURX","download_json":"https://pith.science/pith/B7SUYNFJZX7H6RKJMJGNVCEURX.json","view_paper":"https://pith.science/paper/B7SUYNFJ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1410.7735&json=true","fetch_graph":"https://pith.science/api/pith-number/B7SUYNFJZX7H6RKJMJGNVCEURX/graph.json","fetch_events":"https://pith.science/api/pith-number/B7SUYNFJZX7H6RKJMJGNVCEURX/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/B7SUYNFJZX7H6RKJMJGNVCEURX/action/timestamp_anchor","attest_storage":"https://pith.science/pith/B7SUYNFJZX7H6RKJMJGNVCEURX/action/storage_attestation","attest_author":"https://pith.science/pith/B7SUYNFJZX7H6RKJMJGNVCEURX/action/author_attestation","sign_citation":"https://pith.science/pith/B7SUYNFJZX7H6RKJMJGNVCEURX/action/citation_signature","submit_replication":"https://pith.science/pith/B7SUYNFJZX7H6RKJMJGNVCEURX/action/replication_record"}},"created_at":"2026-05-18T01:41:39.148974+00:00","updated_at":"2026-05-18T01:41:39.148974+00:00"}