{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2013:PYZUSHGYQJ74IAPTGLQEDUBZWU","short_pith_number":"pith:PYZUSHGY","schema_version":"1.0","canonical_sha256":"7e33491cd8827fc401f332e041d039b50ef14b5edf09acbd53ecac2d9d3b540e","source":{"kind":"arxiv","id":"1306.0908","version":3},"attestation_state":"computed","paper":{"title":"Partially massless gravitons do not destroy general relativity black holes","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE","hep-th"],"primary_cat":"gr-qc","authors_text":"Paolo Pani, Richard Brito, Vitor Cardoso","submitted_at":"2013-06-04T20:00:16Z","abstract_excerpt":"Recent nonlinear completions of Fierz-Pauli theory for a massive spin-2 field include nonlinear massive gravity and bimetric theories. The spectrum of black-hole solutions in these theories is rich, and comprises the same vacuum solutions of Einstein's gravity enlarged to include a cosmological constant. It was recently shown that Schwarzschild (de Sitter) black holes in these theories are generically unstable against spherical perturbations. Here we show that a notable exception is partially massless gravity, where the mass of the graviton is fixed in terms of the cosmological constant by \\mu"},"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":"1306.0908","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2013-06-04T20:00:16Z","cross_cats_sorted":["astro-ph.HE","hep-th"],"title_canon_sha256":"15ac3cd36ae7e3ec5ce3fbb3e948cc61e58e03cac81c24f71f8bfc7e49c37965","abstract_canon_sha256":"5cc6c91415a5e194e1d69faf23571b7d6885b63b0172d569ccb31f06e815f1c2"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T03:15:18.044223Z","signature_b64":"U15hI65PObkUjFga2m8b114iPBXLpoGOL/almbR8TtI/860fKox5ulrMq4VG+vcEkJo4/M78SPLAAh5jzDYNCg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"7e33491cd8827fc401f332e041d039b50ef14b5edf09acbd53ecac2d9d3b540e","last_reissued_at":"2026-05-18T03:15:18.043336Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T03:15:18.043336Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Partially massless gravitons do not destroy general relativity black holes","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE","hep-th"],"primary_cat":"gr-qc","authors_text":"Paolo Pani, Richard Brito, Vitor Cardoso","submitted_at":"2013-06-04T20:00:16Z","abstract_excerpt":"Recent nonlinear completions of Fierz-Pauli theory for a massive spin-2 field include nonlinear massive gravity and bimetric theories. The spectrum of black-hole solutions in these theories is rich, and comprises the same vacuum solutions of Einstein's gravity enlarged to include a cosmological constant. It was recently shown that Schwarzschild (de Sitter) black holes in these theories are generically unstable against spherical perturbations. Here we show that a notable exception is partially massless gravity, where the mass of the graviton is fixed in terms of the cosmological constant by \\mu"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1306.0908","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":""},"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":"1306.0908","created_at":"2026-05-18T03:15:18.043489+00:00"},{"alias_kind":"arxiv_version","alias_value":"1306.0908v3","created_at":"2026-05-18T03:15:18.043489+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1306.0908","created_at":"2026-05-18T03:15:18.043489+00:00"},{"alias_kind":"pith_short_12","alias_value":"PYZUSHGYQJ74","created_at":"2026-05-18T12:27:57.521954+00:00"},{"alias_kind":"pith_short_16","alias_value":"PYZUSHGYQJ74IAPT","created_at":"2026-05-18T12:27:57.521954+00:00"},{"alias_kind":"pith_short_8","alias_value":"PYZUSHGY","created_at":"2026-05-18T12:27:57.521954+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"1501.07274","citing_title":"Testing General Relativity with Present and Future Astrophysical Observations","ref_index":111,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/PYZUSHGYQJ74IAPTGLQEDUBZWU","json":"https://pith.science/pith/PYZUSHGYQJ74IAPTGLQEDUBZWU.json","graph_json":"https://pith.science/api/pith-number/PYZUSHGYQJ74IAPTGLQEDUBZWU/graph.json","events_json":"https://pith.science/api/pith-number/PYZUSHGYQJ74IAPTGLQEDUBZWU/events.json","paper":"https://pith.science/paper/PYZUSHGY"},"agent_actions":{"view_html":"https://pith.science/pith/PYZUSHGYQJ74IAPTGLQEDUBZWU","download_json":"https://pith.science/pith/PYZUSHGYQJ74IAPTGLQEDUBZWU.json","view_paper":"https://pith.science/paper/PYZUSHGY","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1306.0908&json=true","fetch_graph":"https://pith.science/api/pith-number/PYZUSHGYQJ74IAPTGLQEDUBZWU/graph.json","fetch_events":"https://pith.science/api/pith-number/PYZUSHGYQJ74IAPTGLQEDUBZWU/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/PYZUSHGYQJ74IAPTGLQEDUBZWU/action/timestamp_anchor","attest_storage":"https://pith.science/pith/PYZUSHGYQJ74IAPTGLQEDUBZWU/action/storage_attestation","attest_author":"https://pith.science/pith/PYZUSHGYQJ74IAPTGLQEDUBZWU/action/author_attestation","sign_citation":"https://pith.science/pith/PYZUSHGYQJ74IAPTGLQEDUBZWU/action/citation_signature","submit_replication":"https://pith.science/pith/PYZUSHGYQJ74IAPTGLQEDUBZWU/action/replication_record"}},"created_at":"2026-05-18T03:15:18.043489+00:00","updated_at":"2026-05-18T03:15:18.043489+00:00"}