{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2016:H5OKIFS3ITL5U6SAZJBHN6QPTX","short_pith_number":"pith:H5OKIFS3","schema_version":"1.0","canonical_sha256":"3f5ca4165b44d7da7a40ca4276fa0f9de9d2b57588cc3a641a97b013556dd6dc","source":{"kind":"arxiv","id":"1603.04373","version":2},"attestation_state":"computed","paper":{"title":"Critical collapse of rotating radiation fluids","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"Carsten Gundlach, Thomas W. Baumgarte","submitted_at":"2016-03-14T18:07:33Z","abstract_excerpt":"We present results from the first fully relativistic simulations of the critical collapse of rotating radiation fluids. We observe critical scaling both in subcritical evolutions, in which case the fluid disperses to infinity and leaves behind flat space, and in supercritical evolutions that lead to the formation of black holes. We measure the mass and angular momentum of these black holes, and find that both show critical scaling with critical exponents that are consistent with perturbative results. The critical exponents are universal; they are not affected by angular momentum, and are indep"},"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":"1603.04373","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2016-03-14T18:07:33Z","cross_cats_sorted":[],"title_canon_sha256":"d068912dcef14aa258afa9f41799e442a3b2eb932c63ddd09c2bea409d1fae1c","abstract_canon_sha256":"a0dac160a71e4b473b0333d067a81602201e0b80a2cbe6ae598fc3f60bbaefdd"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:12:34.387499Z","signature_b64":"zfHQmlRClu88tw4w/QfWsW2mZrXCageV1gSZ/neceu/jrng5mgW7Km69We2uF+I0PMGqxU6MTJfNS3KlOhf0AQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"3f5ca4165b44d7da7a40ca4276fa0f9de9d2b57588cc3a641a97b013556dd6dc","last_reissued_at":"2026-05-18T01:12:34.386970Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:12:34.386970Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Critical collapse of rotating radiation fluids","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"Carsten Gundlach, Thomas W. Baumgarte","submitted_at":"2016-03-14T18:07:33Z","abstract_excerpt":"We present results from the first fully relativistic simulations of the critical collapse of rotating radiation fluids. We observe critical scaling both in subcritical evolutions, in which case the fluid disperses to infinity and leaves behind flat space, and in supercritical evolutions that lead to the formation of black holes. We measure the mass and angular momentum of these black holes, and find that both show critical scaling with critical exponents that are consistent with perturbative results. The critical exponents are universal; they are not affected by angular momentum, and are indep"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1603.04373","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":"1603.04373","created_at":"2026-05-18T01:12:34.387055+00:00"},{"alias_kind":"arxiv_version","alias_value":"1603.04373v2","created_at":"2026-05-18T01:12:34.387055+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1603.04373","created_at":"2026-05-18T01:12:34.387055+00:00"},{"alias_kind":"pith_short_12","alias_value":"H5OKIFS3ITL5","created_at":"2026-05-18T12:30:19.053100+00:00"},{"alias_kind":"pith_short_16","alias_value":"H5OKIFS3ITL5U6SA","created_at":"2026-05-18T12:30:19.053100+00:00"},{"alias_kind":"pith_short_8","alias_value":"H5OKIFS3","created_at":"2026-05-18T12:30:19.053100+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2505.09202","citing_title":"Angular momentum of vacuum bubbles in a first-order phase transition","ref_index":14,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/H5OKIFS3ITL5U6SAZJBHN6QPTX","json":"https://pith.science/pith/H5OKIFS3ITL5U6SAZJBHN6QPTX.json","graph_json":"https://pith.science/api/pith-number/H5OKIFS3ITL5U6SAZJBHN6QPTX/graph.json","events_json":"https://pith.science/api/pith-number/H5OKIFS3ITL5U6SAZJBHN6QPTX/events.json","paper":"https://pith.science/paper/H5OKIFS3"},"agent_actions":{"view_html":"https://pith.science/pith/H5OKIFS3ITL5U6SAZJBHN6QPTX","download_json":"https://pith.science/pith/H5OKIFS3ITL5U6SAZJBHN6QPTX.json","view_paper":"https://pith.science/paper/H5OKIFS3","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1603.04373&json=true","fetch_graph":"https://pith.science/api/pith-number/H5OKIFS3ITL5U6SAZJBHN6QPTX/graph.json","fetch_events":"https://pith.science/api/pith-number/H5OKIFS3ITL5U6SAZJBHN6QPTX/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/H5OKIFS3ITL5U6SAZJBHN6QPTX/action/timestamp_anchor","attest_storage":"https://pith.science/pith/H5OKIFS3ITL5U6SAZJBHN6QPTX/action/storage_attestation","attest_author":"https://pith.science/pith/H5OKIFS3ITL5U6SAZJBHN6QPTX/action/author_attestation","sign_citation":"https://pith.science/pith/H5OKIFS3ITL5U6SAZJBHN6QPTX/action/citation_signature","submit_replication":"https://pith.science/pith/H5OKIFS3ITL5U6SAZJBHN6QPTX/action/replication_record"}},"created_at":"2026-05-18T01:12:34.387055+00:00","updated_at":"2026-05-18T01:12:34.387055+00:00"}