{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2018:L7MLTVNF4KLG2B32H5QP4OPV7F","short_pith_number":"pith:L7MLTVNF","schema_version":"1.0","canonical_sha256":"5fd8b9d5a5e2966d077a3f60fe39f5f9576ef427487b1ce7b83650c1a61fd572","source":{"kind":"arxiv","id":"1808.03631","version":2},"attestation_state":"computed","paper":{"title":"Strong cosmic censorship in charged black-hole spacetimes: still subtle","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-th","math-ph","math.MP"],"primary_cat":"gr-qc","authors_text":"Aron Jansen, Joao L. Costa, Kyriakos Destounis, Peter Hintz, Vitor Cardoso","submitted_at":"2018-08-10T17:31:32Z","abstract_excerpt":"It was recently shown that Strong Cosmic Censorship may be violated in highly charged black-hole spacetimes living in a universe with a positive cosmological constant. Several follow-up works have since suggested that such result, while conceptually interesting, cannot be upheld in practice. We focus here on the claim that the presence of charged massive scalars suffices to save Strong Cosmic Censorship. To the contrary, we show that there still exists a finite region in parameter space where Strong Cosmic Censorship is expected to be violated."},"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":"1808.03631","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2018-08-10T17:31:32Z","cross_cats_sorted":["hep-th","math-ph","math.MP"],"title_canon_sha256":"acc988ad4386ef33d2404ad8e69d17e5cef39e14a4e0fbb58257d9a7014ba278","abstract_canon_sha256":"30698c2818e2af9e74476f84258e095875e5df424954cb4d4061bc587084590b"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:00:51.133009Z","signature_b64":"XaItWMzHX3iZ+QLQ+YY0zwHXZeNI8izx1+DgSBrH40UwBqbDc61jj2M+LxkwSfUHdyilEUuyyjMF91Ym6KkJCA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"5fd8b9d5a5e2966d077a3f60fe39f5f9576ef427487b1ce7b83650c1a61fd572","last_reissued_at":"2026-05-18T00:00:51.132614Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:00:51.132614Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Strong cosmic censorship in charged black-hole spacetimes: still subtle","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-th","math-ph","math.MP"],"primary_cat":"gr-qc","authors_text":"Aron Jansen, Joao L. Costa, Kyriakos Destounis, Peter Hintz, Vitor Cardoso","submitted_at":"2018-08-10T17:31:32Z","abstract_excerpt":"It was recently shown that Strong Cosmic Censorship may be violated in highly charged black-hole spacetimes living in a universe with a positive cosmological constant. Several follow-up works have since suggested that such result, while conceptually interesting, cannot be upheld in practice. We focus here on the claim that the presence of charged massive scalars suffices to save Strong Cosmic Censorship. To the contrary, we show that there still exists a finite region in parameter space where Strong Cosmic Censorship is expected to be violated."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1808.03631","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":"1808.03631","created_at":"2026-05-18T00:00:51.132671+00:00"},{"alias_kind":"arxiv_version","alias_value":"1808.03631v2","created_at":"2026-05-18T00:00:51.132671+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1808.03631","created_at":"2026-05-18T00:00:51.132671+00:00"},{"alias_kind":"pith_short_12","alias_value":"L7MLTVNF4KLG","created_at":"2026-05-18T12:32:33.847187+00:00"},{"alias_kind":"pith_short_16","alias_value":"L7MLTVNF4KLG2B32","created_at":"2026-05-18T12:32:33.847187+00:00"},{"alias_kind":"pith_short_8","alias_value":"L7MLTVNF","created_at":"2026-05-18T12:32:33.847187+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2605.20349","citing_title":"The fate of Reissner--Nordstr\\\"om--de Sitter black holes: nonequilibrium discharge and evaporation","ref_index":54,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/L7MLTVNF4KLG2B32H5QP4OPV7F","json":"https://pith.science/pith/L7MLTVNF4KLG2B32H5QP4OPV7F.json","graph_json":"https://pith.science/api/pith-number/L7MLTVNF4KLG2B32H5QP4OPV7F/graph.json","events_json":"https://pith.science/api/pith-number/L7MLTVNF4KLG2B32H5QP4OPV7F/events.json","paper":"https://pith.science/paper/L7MLTVNF"},"agent_actions":{"view_html":"https://pith.science/pith/L7MLTVNF4KLG2B32H5QP4OPV7F","download_json":"https://pith.science/pith/L7MLTVNF4KLG2B32H5QP4OPV7F.json","view_paper":"https://pith.science/paper/L7MLTVNF","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1808.03631&json=true","fetch_graph":"https://pith.science/api/pith-number/L7MLTVNF4KLG2B32H5QP4OPV7F/graph.json","fetch_events":"https://pith.science/api/pith-number/L7MLTVNF4KLG2B32H5QP4OPV7F/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/L7MLTVNF4KLG2B32H5QP4OPV7F/action/timestamp_anchor","attest_storage":"https://pith.science/pith/L7MLTVNF4KLG2B32H5QP4OPV7F/action/storage_attestation","attest_author":"https://pith.science/pith/L7MLTVNF4KLG2B32H5QP4OPV7F/action/author_attestation","sign_citation":"https://pith.science/pith/L7MLTVNF4KLG2B32H5QP4OPV7F/action/citation_signature","submit_replication":"https://pith.science/pith/L7MLTVNF4KLG2B32H5QP4OPV7F/action/replication_record"}},"created_at":"2026-05-18T00:00:51.132671+00:00","updated_at":"2026-05-18T00:00:51.132671+00:00"}