{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2021:CDYM7EDKJP6QDCXOQLQANUVOFK","short_pith_number":"pith:CDYM7EDK","schema_version":"1.0","canonical_sha256":"10f0cf906a4bfd018aee82e006d2ae2aa816bcbc780c376af66aba77d8769d6e","source":{"kind":"arxiv","id":"2112.04206","version":3},"attestation_state":"computed","paper":{"title":"Inside Anisotropic Black Hole with Vector Hair","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-th"],"primary_cat":"gr-qc","authors_text":"Chenghu Ge, Li Li, Rong-Gen Cai, Run-Qiu Yang","submitted_at":"2021-12-08T10:12:16Z","abstract_excerpt":"We study the internal structure of anisotropic black holes with charged vector hairs. Taking advantage of the scaling symmetries of the system, some radially conserved charges are found via the extension of the Noether theorem. Then, a general proof of no inner horizon of these black holes is presented and the geometry ends at a spacelike singularity. Before reaching the singularity, we find several intermediate regimes both analytically and numerically. In addition to the Einstein-Rosen bridge contracting towards the singularity, the instability triggered by the vector hair results in the osc"},"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":"2112.04206","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2021-12-08T10:12:16Z","cross_cats_sorted":["hep-th"],"title_canon_sha256":"a160325cd897029077204a67b645b14beb760c3c6a74a50e923247db71301c30","abstract_canon_sha256":"bc026c3b20f87e124d6307a150c9b2305654b91ca2aa9c8ef37807b5b8a413bb"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T03:58:59.347698Z","signature_b64":"Iei3EJApkgt4S4eGc+vjYwSpU4YZROu1SAZ81fY+kxsI4B5+q6Q0cpRL1tToeUuhwexSPMMqCwwK3huG0Gp4AA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"10f0cf906a4bfd018aee82e006d2ae2aa816bcbc780c376af66aba77d8769d6e","last_reissued_at":"2026-07-05T03:58:59.347154Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T03:58:59.347154Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Inside Anisotropic Black Hole with Vector Hair","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-th"],"primary_cat":"gr-qc","authors_text":"Chenghu Ge, Li Li, Rong-Gen Cai, Run-Qiu Yang","submitted_at":"2021-12-08T10:12:16Z","abstract_excerpt":"We study the internal structure of anisotropic black holes with charged vector hairs. Taking advantage of the scaling symmetries of the system, some radially conserved charges are found via the extension of the Noether theorem. Then, a general proof of no inner horizon of these black holes is presented and the geometry ends at a spacelike singularity. Before reaching the singularity, we find several intermediate regimes both analytically and numerically. In addition to the Einstein-Rosen bridge contracting towards the singularity, the instability triggered by the vector hair results in the osc"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2112.04206","kind":"arxiv","version":3},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2112.04206/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"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":"2112.04206","created_at":"2026-07-05T03:58:59.347214+00:00"},{"alias_kind":"arxiv_version","alias_value":"2112.04206v3","created_at":"2026-07-05T03:58:59.347214+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2112.04206","created_at":"2026-07-05T03:58:59.347214+00:00"},{"alias_kind":"pith_short_12","alias_value":"CDYM7EDKJP6Q","created_at":"2026-07-05T03:58:59.347214+00:00"},{"alias_kind":"pith_short_16","alias_value":"CDYM7EDKJP6QDCXO","created_at":"2026-07-05T03:58:59.347214+00:00"},{"alias_kind":"pith_short_8","alias_value":"CDYM7EDK","created_at":"2026-07-05T03:58:59.347214+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":3,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2512.19377","citing_title":"Critical phenomenon inside asymptotically flat black holes with spontaneous scalarization","ref_index":10,"is_internal_anchor":false},{"citing_arxiv_id":"2512.24893","citing_title":"Interior structure of black holes with nonlinear terms","ref_index":32,"is_internal_anchor":false},{"citing_arxiv_id":"2604.13104","citing_title":"Nonequilibrium crossover in the supercritical region from quench dynamics","ref_index":59,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/CDYM7EDKJP6QDCXOQLQANUVOFK","json":"https://pith.science/pith/CDYM7EDKJP6QDCXOQLQANUVOFK.json","graph_json":"https://pith.science/api/pith-number/CDYM7EDKJP6QDCXOQLQANUVOFK/graph.json","events_json":"https://pith.science/api/pith-number/CDYM7EDKJP6QDCXOQLQANUVOFK/events.json","paper":"https://pith.science/paper/CDYM7EDK"},"agent_actions":{"view_html":"https://pith.science/pith/CDYM7EDKJP6QDCXOQLQANUVOFK","download_json":"https://pith.science/pith/CDYM7EDKJP6QDCXOQLQANUVOFK.json","view_paper":"https://pith.science/paper/CDYM7EDK","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2112.04206&json=true","fetch_graph":"https://pith.science/api/pith-number/CDYM7EDKJP6QDCXOQLQANUVOFK/graph.json","fetch_events":"https://pith.science/api/pith-number/CDYM7EDKJP6QDCXOQLQANUVOFK/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/CDYM7EDKJP6QDCXOQLQANUVOFK/action/timestamp_anchor","attest_storage":"https://pith.science/pith/CDYM7EDKJP6QDCXOQLQANUVOFK/action/storage_attestation","attest_author":"https://pith.science/pith/CDYM7EDKJP6QDCXOQLQANUVOFK/action/author_attestation","sign_citation":"https://pith.science/pith/CDYM7EDKJP6QDCXOQLQANUVOFK/action/citation_signature","submit_replication":"https://pith.science/pith/CDYM7EDKJP6QDCXOQLQANUVOFK/action/replication_record"}},"created_at":"2026-07-05T03:58:59.347214+00:00","updated_at":"2026-07-05T03:58:59.347214+00:00"}