{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:ZV4SB2VZEQSDD5XCH3EBWWEKU4","short_pith_number":"pith:ZV4SB2VZ","schema_version":"1.0","canonical_sha256":"cd7920eab9242431f6e23ec81b588aa7080a8e955c884a03ff005ed098e6e2bb","source":{"kind":"arxiv","id":"1711.10502","version":2},"attestation_state":"computed","paper":{"title":"Quasinormal modes and Strong Cosmic Censorship","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":"2017-11-28T19:00:06Z","abstract_excerpt":"The fate of Cauchy horizons, such as those found inside charged black holes, is intrinsically connected to the decay of small perturbations exterior to the event horizon. As such, the validity of the strong cosmic censorship (SCC) conjecture is tied to how effectively the exterior damps fluctuations. Here, we study massless scalar fields in the exterior of Reissner--Nordstrom--de Sitter black holes. Their decay rates are governed by quasinormal modes of the black hole. We identify three families of modes in these spacetimes: one directly linked to the photon sphere, well described by standard "},"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":"1711.10502","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2017-11-28T19:00:06Z","cross_cats_sorted":["hep-th","math-ph","math.MP"],"title_canon_sha256":"ea63fd3e1d2d6fbfc3bb3d67053f672c9234b0c29fbe2871808fa232ab7c4484","abstract_canon_sha256":"878c978069a1e2048d44e2a1ffb7e26e01aad687c0feb48a5efcf4ac43ee0f45"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:25:15.915969Z","signature_b64":"U3B4orMJMYfSNhuRr0v9GE/MjLqta+yhb9e3qeiQCR/ATaRESwx7G6krotW6lsBWajmQTeFu64BoKZYh3INsAg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"cd7920eab9242431f6e23ec81b588aa7080a8e955c884a03ff005ed098e6e2bb","last_reissued_at":"2026-05-18T00:25:15.915384Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:25:15.915384Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Quasinormal modes and Strong Cosmic Censorship","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":"2017-11-28T19:00:06Z","abstract_excerpt":"The fate of Cauchy horizons, such as those found inside charged black holes, is intrinsically connected to the decay of small perturbations exterior to the event horizon. As such, the validity of the strong cosmic censorship (SCC) conjecture is tied to how effectively the exterior damps fluctuations. Here, we study massless scalar fields in the exterior of Reissner--Nordstrom--de Sitter black holes. Their decay rates are governed by quasinormal modes of the black hole. We identify three families of modes in these spacetimes: one directly linked to the photon sphere, well described by standard "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1711.10502","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":"1711.10502","created_at":"2026-05-18T00:25:15.915501+00:00"},{"alias_kind":"arxiv_version","alias_value":"1711.10502v2","created_at":"2026-05-18T00:25:15.915501+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1711.10502","created_at":"2026-05-18T00:25:15.915501+00:00"},{"alias_kind":"pith_short_12","alias_value":"ZV4SB2VZEQSD","created_at":"2026-05-18T12:31:59.375834+00:00"},{"alias_kind":"pith_short_16","alias_value":"ZV4SB2VZEQSDD5XC","created_at":"2026-05-18T12:31:59.375834+00:00"},{"alias_kind":"pith_short_8","alias_value":"ZV4SB2VZ","created_at":"2026-05-18T12:31:59.375834+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":4,"internal_anchor_count":2,"sample":[{"citing_arxiv_id":"2605.21533","citing_title":"Long-lived quasinormal modes of Asymptotically de Sitter Black Holes in Generalized Proca Theory","ref_index":23,"is_internal_anchor":true},{"citing_arxiv_id":"2601.18613","citing_title":"Correspondence between quasinormal modes and grey-body factors of Schwarzschild--Tangherlini black holes","ref_index":31,"is_internal_anchor":true},{"citing_arxiv_id":"1904.05363","citing_title":"Testing the nature of dark compact objects: a status report","ref_index":20,"is_internal_anchor":false},{"citing_arxiv_id":"2605.12113","citing_title":"Quasinormal Spectra of Fields of Various Spin in Asymptotically de Sitter Black Holes within Generalized Proca Theory","ref_index":8,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/ZV4SB2VZEQSDD5XCH3EBWWEKU4","json":"https://pith.science/pith/ZV4SB2VZEQSDD5XCH3EBWWEKU4.json","graph_json":"https://pith.science/api/pith-number/ZV4SB2VZEQSDD5XCH3EBWWEKU4/graph.json","events_json":"https://pith.science/api/pith-number/ZV4SB2VZEQSDD5XCH3EBWWEKU4/events.json","paper":"https://pith.science/paper/ZV4SB2VZ"},"agent_actions":{"view_html":"https://pith.science/pith/ZV4SB2VZEQSDD5XCH3EBWWEKU4","download_json":"https://pith.science/pith/ZV4SB2VZEQSDD5XCH3EBWWEKU4.json","view_paper":"https://pith.science/paper/ZV4SB2VZ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1711.10502&json=true","fetch_graph":"https://pith.science/api/pith-number/ZV4SB2VZEQSDD5XCH3EBWWEKU4/graph.json","fetch_events":"https://pith.science/api/pith-number/ZV4SB2VZEQSDD5XCH3EBWWEKU4/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/ZV4SB2VZEQSDD5XCH3EBWWEKU4/action/timestamp_anchor","attest_storage":"https://pith.science/pith/ZV4SB2VZEQSDD5XCH3EBWWEKU4/action/storage_attestation","attest_author":"https://pith.science/pith/ZV4SB2VZEQSDD5XCH3EBWWEKU4/action/author_attestation","sign_citation":"https://pith.science/pith/ZV4SB2VZEQSDD5XCH3EBWWEKU4/action/citation_signature","submit_replication":"https://pith.science/pith/ZV4SB2VZEQSDD5XCH3EBWWEKU4/action/replication_record"}},"created_at":"2026-05-18T00:25:15.915501+00:00","updated_at":"2026-05-18T00:25:15.915501+00:00"}