{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2010:6ZIEZ4PN2CWCHHT5CAOJGZYPCF","short_pith_number":"pith:6ZIEZ4PN","schema_version":"1.0","canonical_sha256":"f6504cf1edd0ac239e7d101c93670f115b2a501b17c1435216ad7fa2295eed23","source":{"kind":"arxiv","id":"1010.2585","version":2},"attestation_state":"computed","paper":{"title":"Internal structure of charged black holes","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-th"],"primary_cat":"gr-qc","authors_text":"Dong-han Yeom, Dong-il Hwang","submitted_at":"2010-10-13T07:23:32Z","abstract_excerpt":"We investigate the internal structure of charged black holes with a spherically symmetric model in the double-null coordinate system. Hawking radiation is considered using the S-wave approximation of semiclassical back-reaction and discharge is simulated by supplying an oppositely charged matter to the black hole. In the stage of formation, the internal structure is determined by the mass and charge of collapsing matter. When the charge-mass ratio is small, a wormhole-like internal structure is observed. The structure becomes analogous to the static limit as the ratio reaches unity. After the "},"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":"1010.2585","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2010-10-13T07:23:32Z","cross_cats_sorted":["hep-th"],"title_canon_sha256":"e0b5ec6c22d7e1ad69b8ff57493c1c8d6403943566a497405af0ef8fe2ac76b5","abstract_canon_sha256":"0fab58ed167af52a668e2ae13104d385586dbc0f6851c98453c2ccc5f4a18b79"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T04:10:57.046458Z","signature_b64":"ShOnn3Q8R1vrpRIV/BCBXlpEe4KL6Ae5nn5Hpc3AnlCrYJtkeWDuAg/E/5oatWtumf7lydzB8jkpKWDXV7fQAw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"f6504cf1edd0ac239e7d101c93670f115b2a501b17c1435216ad7fa2295eed23","last_reissued_at":"2026-05-18T04:10:57.045946Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T04:10:57.045946Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Internal structure of charged black holes","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-th"],"primary_cat":"gr-qc","authors_text":"Dong-han Yeom, Dong-il Hwang","submitted_at":"2010-10-13T07:23:32Z","abstract_excerpt":"We investigate the internal structure of charged black holes with a spherically symmetric model in the double-null coordinate system. Hawking radiation is considered using the S-wave approximation of semiclassical back-reaction and discharge is simulated by supplying an oppositely charged matter to the black hole. In the stage of formation, the internal structure is determined by the mass and charge of collapsing matter. When the charge-mass ratio is small, a wormhole-like internal structure is observed. The structure becomes analogous to the static limit as the ratio reaches unity. After the "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1010.2585","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":"1010.2585","created_at":"2026-05-18T04:10:57.046019+00:00"},{"alias_kind":"arxiv_version","alias_value":"1010.2585v2","created_at":"2026-05-18T04:10:57.046019+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1010.2585","created_at":"2026-05-18T04:10:57.046019+00:00"},{"alias_kind":"pith_short_12","alias_value":"6ZIEZ4PN2CWC","created_at":"2026-05-18T12:26:04.259169+00:00"},{"alias_kind":"pith_short_16","alias_value":"6ZIEZ4PN2CWCHHT5","created_at":"2026-05-18T12:26:04.259169+00:00"},{"alias_kind":"pith_short_8","alias_value":"6ZIEZ4PN","created_at":"2026-05-18T12:26:04.259169+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":2,"internal_anchor_count":2,"sample":[{"citing_arxiv_id":"2605.15576","citing_title":"Regular black hole with sub-Planckian curvature and suppressed exponential mass inflation","ref_index":36,"is_internal_anchor":true},{"citing_arxiv_id":"2508.09988","citing_title":"General Boosted Black Holes: A First Approximation","ref_index":29,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/6ZIEZ4PN2CWCHHT5CAOJGZYPCF","json":"https://pith.science/pith/6ZIEZ4PN2CWCHHT5CAOJGZYPCF.json","graph_json":"https://pith.science/api/pith-number/6ZIEZ4PN2CWCHHT5CAOJGZYPCF/graph.json","events_json":"https://pith.science/api/pith-number/6ZIEZ4PN2CWCHHT5CAOJGZYPCF/events.json","paper":"https://pith.science/paper/6ZIEZ4PN"},"agent_actions":{"view_html":"https://pith.science/pith/6ZIEZ4PN2CWCHHT5CAOJGZYPCF","download_json":"https://pith.science/pith/6ZIEZ4PN2CWCHHT5CAOJGZYPCF.json","view_paper":"https://pith.science/paper/6ZIEZ4PN","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1010.2585&json=true","fetch_graph":"https://pith.science/api/pith-number/6ZIEZ4PN2CWCHHT5CAOJGZYPCF/graph.json","fetch_events":"https://pith.science/api/pith-number/6ZIEZ4PN2CWCHHT5CAOJGZYPCF/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/6ZIEZ4PN2CWCHHT5CAOJGZYPCF/action/timestamp_anchor","attest_storage":"https://pith.science/pith/6ZIEZ4PN2CWCHHT5CAOJGZYPCF/action/storage_attestation","attest_author":"https://pith.science/pith/6ZIEZ4PN2CWCHHT5CAOJGZYPCF/action/author_attestation","sign_citation":"https://pith.science/pith/6ZIEZ4PN2CWCHHT5CAOJGZYPCF/action/citation_signature","submit_replication":"https://pith.science/pith/6ZIEZ4PN2CWCHHT5CAOJGZYPCF/action/replication_record"}},"created_at":"2026-05-18T04:10:57.046019+00:00","updated_at":"2026-05-18T04:10:57.046019+00:00"}