{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2011:JD2HGPHSJNGINIEXBPWKATIILE","short_pith_number":"pith:JD2HGPHS","schema_version":"1.0","canonical_sha256":"48f4733cf24b4c86a0970beca04d085912924d5fe338c1e4cfebbde0620bda94","source":{"kind":"arxiv","id":"1106.5438","version":2},"attestation_state":"computed","paper":{"title":"Equilibrium configurations from gravitational collapse","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE","hep-th"],"primary_cat":"gr-qc","authors_text":"Daniele Malafarina, Pankaj S. Joshi, Ramesh Narayan","submitted_at":"2011-06-27T16:44:50Z","abstract_excerpt":"We develop here a new procedure within Einstein's theory of gravity to generate equilibrium configurations that result as the final state of gravitational collapse from regular initial conditions. As a simplification, we assume that the collapsing fluid is supported only by tangential pressure. We show that the equilibrium geometries generated by this method form a subset of static solutions to the Einstein equations, and that they can either be regular or develop a naked singularity at the center. When a singularity is present, there are key differences in the properties of stable circular or"},"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":"1106.5438","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2011-06-27T16:44:50Z","cross_cats_sorted":["astro-ph.HE","hep-th"],"title_canon_sha256":"c6cd9c3aabdb19c0ea48c5c99768b68325aced55b3cabc10033e613b24965905","abstract_canon_sha256":"fccfcc9a6b458bd30aee00082d49d23c6c13fab493ae564dc5bc096631a24142"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:01:30.346723Z","signature_b64":"5+LAcA0+dg9U3oqqxKunynsWOtpq13G5ssReWS6XLob2W/h4pzFP1pyTLUDGN697KcURygUQK5uQIL2W4FZlBQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"48f4733cf24b4c86a0970beca04d085912924d5fe338c1e4cfebbde0620bda94","last_reissued_at":"2026-05-18T02:01:30.346261Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:01:30.346261Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Equilibrium configurations from gravitational collapse","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE","hep-th"],"primary_cat":"gr-qc","authors_text":"Daniele Malafarina, Pankaj S. Joshi, Ramesh Narayan","submitted_at":"2011-06-27T16:44:50Z","abstract_excerpt":"We develop here a new procedure within Einstein's theory of gravity to generate equilibrium configurations that result as the final state of gravitational collapse from regular initial conditions. As a simplification, we assume that the collapsing fluid is supported only by tangential pressure. We show that the equilibrium geometries generated by this method form a subset of static solutions to the Einstein equations, and that they can either be regular or develop a naked singularity at the center. When a singularity is present, there are key differences in the properties of stable circular or"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1106.5438","kind":"arxiv","version":2},"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":"1106.5438","created_at":"2026-05-18T02:01:30.346328+00:00"},{"alias_kind":"arxiv_version","alias_value":"1106.5438v2","created_at":"2026-05-18T02:01:30.346328+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1106.5438","created_at":"2026-05-18T02:01:30.346328+00:00"},{"alias_kind":"pith_short_12","alias_value":"JD2HGPHSJNGI","created_at":"2026-05-18T12:26:32.869790+00:00"},{"alias_kind":"pith_short_16","alias_value":"JD2HGPHSJNGINIEX","created_at":"2026-05-18T12:26:32.869790+00:00"},{"alias_kind":"pith_short_8","alias_value":"JD2HGPHS","created_at":"2026-05-18T12:26:32.869790+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2604.16545","citing_title":"Energy conditions in static, spherically symmetric spacetimes and effective geometries","ref_index":75,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/JD2HGPHSJNGINIEXBPWKATIILE","json":"https://pith.science/pith/JD2HGPHSJNGINIEXBPWKATIILE.json","graph_json":"https://pith.science/api/pith-number/JD2HGPHSJNGINIEXBPWKATIILE/graph.json","events_json":"https://pith.science/api/pith-number/JD2HGPHSJNGINIEXBPWKATIILE/events.json","paper":"https://pith.science/paper/JD2HGPHS"},"agent_actions":{"view_html":"https://pith.science/pith/JD2HGPHSJNGINIEXBPWKATIILE","download_json":"https://pith.science/pith/JD2HGPHSJNGINIEXBPWKATIILE.json","view_paper":"https://pith.science/paper/JD2HGPHS","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1106.5438&json=true","fetch_graph":"https://pith.science/api/pith-number/JD2HGPHSJNGINIEXBPWKATIILE/graph.json","fetch_events":"https://pith.science/api/pith-number/JD2HGPHSJNGINIEXBPWKATIILE/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/JD2HGPHSJNGINIEXBPWKATIILE/action/timestamp_anchor","attest_storage":"https://pith.science/pith/JD2HGPHSJNGINIEXBPWKATIILE/action/storage_attestation","attest_author":"https://pith.science/pith/JD2HGPHSJNGINIEXBPWKATIILE/action/author_attestation","sign_citation":"https://pith.science/pith/JD2HGPHSJNGINIEXBPWKATIILE/action/citation_signature","submit_replication":"https://pith.science/pith/JD2HGPHSJNGINIEXBPWKATIILE/action/replication_record"}},"created_at":"2026-05-18T02:01:30.346328+00:00","updated_at":"2026-05-18T02:01:30.346328+00:00"}