{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2015:2G6WR4OK4BPVMV74LBEG67EW5H","short_pith_number":"pith:2G6WR4OK","schema_version":"1.0","canonical_sha256":"d1bd68f1cae05f5657fc58486f7c96e9f907cfc67fb9fdc83d9aa9cd2a5ce415","source":{"kind":"arxiv","id":"1510.04713","version":2},"attestation_state":"computed","paper":{"title":"Maxwell perturbations on asymptotically anti-de Sitter spacetimes: Generic boundary conditions and a new branch of quasinormal modes","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-th"],"primary_cat":"gr-qc","authors_text":"Carlos Herdeiro, Marco O. P. Sampaio, Mengjie Wang","submitted_at":"2015-10-15T20:38:20Z","abstract_excerpt":"Perturbations of asymptotically Anti-de-Sitter (AdS) spacetimes are often considered by imposing field vanishing boundary conditions (BCs) at the AdS boundary. Such BCs, of Dirichlet-type, imply a vanishing energy flux at the boundary, but the converse is, generically, not true. Regarding AdS as a gravitational box, we consider vanishing energy flux (VEF) BCs as a more fundamental physical requirement and we show that these BCs can lead to a new branch of modes. As a concrete example, we consider Maxwell perturbations on Kerr-AdS black holes in the Teukolsky formalism, but our formulation appl"},"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":"1510.04713","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2015-10-15T20:38:20Z","cross_cats_sorted":["hep-th"],"title_canon_sha256":"7454d34131748dfdd0db178760811e2bc7fd5f7b0830441c4ccf29afa9fee90f","abstract_canon_sha256":"5c443f7f38122f8c813d999726f4add67aaf00bf993d2c74c9dd8559bdd2be78"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:25:24.245135Z","signature_b64":"492wQ/lcy8OWSwn0WsvUxBoZqDOlURjQ6Bj3/vFuiwZR7MjpJCOgd3zeXUVJxE8jjvG0WHPOJGNyzBpB5EOKAg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"d1bd68f1cae05f5657fc58486f7c96e9f907cfc67fb9fdc83d9aa9cd2a5ce415","last_reissued_at":"2026-05-18T01:25:24.244507Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:25:24.244507Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Maxwell perturbations on asymptotically anti-de Sitter spacetimes: Generic boundary conditions and a new branch of quasinormal modes","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-th"],"primary_cat":"gr-qc","authors_text":"Carlos Herdeiro, Marco O. P. Sampaio, Mengjie Wang","submitted_at":"2015-10-15T20:38:20Z","abstract_excerpt":"Perturbations of asymptotically Anti-de-Sitter (AdS) spacetimes are often considered by imposing field vanishing boundary conditions (BCs) at the AdS boundary. Such BCs, of Dirichlet-type, imply a vanishing energy flux at the boundary, but the converse is, generically, not true. Regarding AdS as a gravitational box, we consider vanishing energy flux (VEF) BCs as a more fundamental physical requirement and we show that these BCs can lead to a new branch of modes. As a concrete example, we consider Maxwell perturbations on Kerr-AdS black holes in the Teukolsky formalism, but our formulation appl"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1510.04713","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":"1510.04713","created_at":"2026-05-18T01:25:24.244602+00:00"},{"alias_kind":"arxiv_version","alias_value":"1510.04713v2","created_at":"2026-05-18T01:25:24.244602+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1510.04713","created_at":"2026-05-18T01:25:24.244602+00:00"},{"alias_kind":"pith_short_12","alias_value":"2G6WR4OK4BPV","created_at":"2026-05-18T12:28:59.999130+00:00"},{"alias_kind":"pith_short_16","alias_value":"2G6WR4OK4BPVMV74","created_at":"2026-05-18T12:28:59.999130+00:00"},{"alias_kind":"pith_short_8","alias_value":"2G6WR4OK","created_at":"2026-05-18T12:28:59.999130+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2605.18947","citing_title":"Quasinormal modes of Proca and Maxwell fields in $d$-dimensional Schwarzschild-AdS black holes","ref_index":60,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/2G6WR4OK4BPVMV74LBEG67EW5H","json":"https://pith.science/pith/2G6WR4OK4BPVMV74LBEG67EW5H.json","graph_json":"https://pith.science/api/pith-number/2G6WR4OK4BPVMV74LBEG67EW5H/graph.json","events_json":"https://pith.science/api/pith-number/2G6WR4OK4BPVMV74LBEG67EW5H/events.json","paper":"https://pith.science/paper/2G6WR4OK"},"agent_actions":{"view_html":"https://pith.science/pith/2G6WR4OK4BPVMV74LBEG67EW5H","download_json":"https://pith.science/pith/2G6WR4OK4BPVMV74LBEG67EW5H.json","view_paper":"https://pith.science/paper/2G6WR4OK","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1510.04713&json=true","fetch_graph":"https://pith.science/api/pith-number/2G6WR4OK4BPVMV74LBEG67EW5H/graph.json","fetch_events":"https://pith.science/api/pith-number/2G6WR4OK4BPVMV74LBEG67EW5H/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/2G6WR4OK4BPVMV74LBEG67EW5H/action/timestamp_anchor","attest_storage":"https://pith.science/pith/2G6WR4OK4BPVMV74LBEG67EW5H/action/storage_attestation","attest_author":"https://pith.science/pith/2G6WR4OK4BPVMV74LBEG67EW5H/action/author_attestation","sign_citation":"https://pith.science/pith/2G6WR4OK4BPVMV74LBEG67EW5H/action/citation_signature","submit_replication":"https://pith.science/pith/2G6WR4OK4BPVMV74LBEG67EW5H/action/replication_record"}},"created_at":"2026-05-18T01:25:24.244602+00:00","updated_at":"2026-05-18T01:25:24.244602+00:00"}