{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2016:OUDV4BVY3BLBSD5NU3LXVNUX3M","short_pith_number":"pith:OUDV4BVY","schema_version":"1.0","canonical_sha256":"75075e06b8d856190fada6d77ab697db0350c018611cf6e2c9544eca6f01fae7","source":{"kind":"arxiv","id":"1603.07694","version":1},"attestation_state":"computed","paper":{"title":"Relativistic Solutions of Anisotropic Compact Objects","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"Bikash Chandra Paul, Rumi Deb","submitted_at":"2016-03-24T18:19:32Z","abstract_excerpt":"We present a class of new relativistic solutions with anisotropic fluid for compact stars in hydrostatic equilibrium. The interior space-time geometry considered here for compact objects are described by parameters namely, $\\lambda$, $k$, $A$, $R$ and $n$. The values of the geometrical parameters are determined here for obtaining a class of physically viable stellar models. The energy-density, radial pressure and tangential pressure are finite and positive inside the anisotropic stars. Considering some stars of known mass we present stellar models which describe compact astrophysical objects w"},"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":"1603.07694","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2016-03-24T18:19:32Z","cross_cats_sorted":[],"title_canon_sha256":"16d4d784e07554ccad03fda0499990cfab3750b9c6f3efbed7b1792dc323a033","abstract_canon_sha256":"ca75ed7640ae32a4aea724c6dca540f225aa267c32cb9bc0441dbf88ccf5e982"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:18:20.135302Z","signature_b64":"59Mtu88mdiZRO1Y1Li49qgj/WQKemJz+O9CW5OfCH9LehKbjETLR6H6hgRejlzWLlE+nYq4wLO+sDOQfneCPBg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"75075e06b8d856190fada6d77ab697db0350c018611cf6e2c9544eca6f01fae7","last_reissued_at":"2026-05-18T01:18:20.134838Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:18:20.134838Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Relativistic Solutions of Anisotropic Compact Objects","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"Bikash Chandra Paul, Rumi Deb","submitted_at":"2016-03-24T18:19:32Z","abstract_excerpt":"We present a class of new relativistic solutions with anisotropic fluid for compact stars in hydrostatic equilibrium. The interior space-time geometry considered here for compact objects are described by parameters namely, $\\lambda$, $k$, $A$, $R$ and $n$. The values of the geometrical parameters are determined here for obtaining a class of physically viable stellar models. The energy-density, radial pressure and tangential pressure are finite and positive inside the anisotropic stars. Considering some stars of known mass we present stellar models which describe compact astrophysical objects w"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1603.07694","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":"1603.07694","created_at":"2026-05-18T01:18:20.134915+00:00"},{"alias_kind":"arxiv_version","alias_value":"1603.07694v1","created_at":"2026-05-18T01:18:20.134915+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1603.07694","created_at":"2026-05-18T01:18:20.134915+00:00"},{"alias_kind":"pith_short_12","alias_value":"OUDV4BVY3BLB","created_at":"2026-05-18T12:30:36.002864+00:00"},{"alias_kind":"pith_short_16","alias_value":"OUDV4BVY3BLBSD5N","created_at":"2026-05-18T12:30:36.002864+00:00"},{"alias_kind":"pith_short_8","alias_value":"OUDV4BVY","created_at":"2026-05-18T12:30:36.002864+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/OUDV4BVY3BLBSD5NU3LXVNUX3M","json":"https://pith.science/pith/OUDV4BVY3BLBSD5NU3LXVNUX3M.json","graph_json":"https://pith.science/api/pith-number/OUDV4BVY3BLBSD5NU3LXVNUX3M/graph.json","events_json":"https://pith.science/api/pith-number/OUDV4BVY3BLBSD5NU3LXVNUX3M/events.json","paper":"https://pith.science/paper/OUDV4BVY"},"agent_actions":{"view_html":"https://pith.science/pith/OUDV4BVY3BLBSD5NU3LXVNUX3M","download_json":"https://pith.science/pith/OUDV4BVY3BLBSD5NU3LXVNUX3M.json","view_paper":"https://pith.science/paper/OUDV4BVY","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1603.07694&json=true","fetch_graph":"https://pith.science/api/pith-number/OUDV4BVY3BLBSD5NU3LXVNUX3M/graph.json","fetch_events":"https://pith.science/api/pith-number/OUDV4BVY3BLBSD5NU3LXVNUX3M/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/OUDV4BVY3BLBSD5NU3LXVNUX3M/action/timestamp_anchor","attest_storage":"https://pith.science/pith/OUDV4BVY3BLBSD5NU3LXVNUX3M/action/storage_attestation","attest_author":"https://pith.science/pith/OUDV4BVY3BLBSD5NU3LXVNUX3M/action/author_attestation","sign_citation":"https://pith.science/pith/OUDV4BVY3BLBSD5NU3LXVNUX3M/action/citation_signature","submit_replication":"https://pith.science/pith/OUDV4BVY3BLBSD5NU3LXVNUX3M/action/replication_record"}},"created_at":"2026-05-18T01:18:20.134915+00:00","updated_at":"2026-05-18T01:18:20.134915+00:00"}