{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2023:K5ZTJJADXB3VPDYL4XXYYOF4RW","short_pith_number":"pith:K5ZTJJAD","schema_version":"1.0","canonical_sha256":"577334a403b877578f0be5ef8c38bc8d865f5c955429ef3f94ba39eb952204bb","source":{"kind":"arxiv","id":"2308.10412","version":2},"attestation_state":"computed","paper":{"title":"Quasinormal modes of the bumblebee black holes with a global monopole","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"Zainab Malik","submitted_at":"2023-08-21T01:38:06Z","abstract_excerpt":"We compute quasinormal modes of test fields around spherically symmetric black holes with a global monopole in bumblebee gravity. The frequency of oscillation and the damping rate exhibit significant decreasing as the global monopole parameter is increased. An intriguing observation arises in the extreme limit, where the quasinormal modes manifest a form of universal behavior: the actual oscillation frequency remains unaltered despite variations in the Lorentz symmetry breaking (LSB) parameter. Our calculations are conducted through two distinct methods, both of which yield results that align "},"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":"2308.10412","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2023-08-21T01:38:06Z","cross_cats_sorted":[],"title_canon_sha256":"57408b966888acbe812962a0c7074ac646d6fc95668713db7f4f4f61dbe77c9f","abstract_canon_sha256":"f91184b7a8c1448ac7e4354b781a692d6d06a3c4c4638ee55242d18e3606b11e"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T08:56:13.816974Z","signature_b64":"3SG9BPTgOvR0u9iRHEOCbk9pzlZJnBCXRHQmjwzKfwjoWP+olMCvShnMoNThdwUB82vB5jGYPmxNBnWTpgQdCg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"577334a403b877578f0be5ef8c38bc8d865f5c955429ef3f94ba39eb952204bb","last_reissued_at":"2026-07-05T08:56:13.816418Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T08:56:13.816418Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Quasinormal modes of the bumblebee black holes with a global monopole","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"Zainab Malik","submitted_at":"2023-08-21T01:38:06Z","abstract_excerpt":"We compute quasinormal modes of test fields around spherically symmetric black holes with a global monopole in bumblebee gravity. The frequency of oscillation and the damping rate exhibit significant decreasing as the global monopole parameter is increased. An intriguing observation arises in the extreme limit, where the quasinormal modes manifest a form of universal behavior: the actual oscillation frequency remains unaltered despite variations in the Lorentz symmetry breaking (LSB) parameter. Our calculations are conducted through two distinct methods, both of which yield results that align "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2308.10412","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2308.10412/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"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":"2308.10412","created_at":"2026-07-05T08:56:13.816498+00:00"},{"alias_kind":"arxiv_version","alias_value":"2308.10412v2","created_at":"2026-07-05T08:56:13.816498+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2308.10412","created_at":"2026-07-05T08:56:13.816498+00:00"},{"alias_kind":"pith_short_12","alias_value":"K5ZTJJADXB3V","created_at":"2026-07-05T08:56:13.816498+00:00"},{"alias_kind":"pith_short_16","alias_value":"K5ZTJJADXB3VPDYL","created_at":"2026-07-05T08:56:13.816498+00:00"},{"alias_kind":"pith_short_8","alias_value":"K5ZTJJAD","created_at":"2026-07-05T08:56:13.816498+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":13,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2605.21533","citing_title":"Long-lived quasinormal modes of Asymptotically de Sitter Black Holes in Generalized Proca Theory","ref_index":101,"is_internal_anchor":false},{"citing_arxiv_id":"2601.17906","citing_title":"Telling tails and quasi-resonances in the vicinity of Dymnikova regular black hole","ref_index":150,"is_internal_anchor":false},{"citing_arxiv_id":"2604.24349","citing_title":"Scalar, electromagnetic, and Dirac perturbations of regular black holes constituting primordial dark matter","ref_index":57,"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":73,"is_internal_anchor":false},{"citing_arxiv_id":"2605.11364","citing_title":"Bardeen spacetime as quantum corrected black hole: Grey-body factors and quasinormal modes of gravitational perturbations","ref_index":114,"is_internal_anchor":false},{"citing_arxiv_id":"2605.11013","citing_title":"Massive Scalar Quasinormal Modes, Greybody Factors, and Absorption Cross Section of a Parity-Symmetric Beyond-Horndeski Black Hole","ref_index":142,"is_internal_anchor":false},{"citing_arxiv_id":"2604.14999","citing_title":"A First-Order Eikonal Framework for Quasinormal Modes, Shadows, Strong Lensing, and Grey-Body Factors in a Scalarized Black-Hole Metric","ref_index":20,"is_internal_anchor":false},{"citing_arxiv_id":"2605.03659","citing_title":"Long-lived massive scalar modes, grey-body factors, and absorption cross sections of the Reissner--Nordstr\\\"om-like brane-world black hole","ref_index":89,"is_internal_anchor":false},{"citing_arxiv_id":"2604.25471","citing_title":"Massive scalar quasinormal modes of an asymptotically flat regular black hole supported by a phantom Dirac--Born--Infeld field","ref_index":151,"is_internal_anchor":false},{"citing_arxiv_id":"2604.24349","citing_title":"Scalar, electromagnetic, and Dirac perturbations of regular black holes constituting primordial dark matter","ref_index":57,"is_internal_anchor":false},{"citing_arxiv_id":"2604.11845","citing_title":"Quasi-resonances in the vicinity of Einstein-Maxwell-dilaton black hole","ref_index":64,"is_internal_anchor":false},{"citing_arxiv_id":"2604.13613","citing_title":"From Ringdown to Lensing: Analytic Eikonal Modes of Quasi-Topological Regular Black Holes","ref_index":16,"is_internal_anchor":false},{"citing_arxiv_id":"2604.14999","citing_title":"A First-Order Eikonal Framework for Quasinormal Modes, Shadows, Strong Lensing, and Grey-Body Factors in a Scalarized Black-Hole Metric","ref_index":20,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/K5ZTJJADXB3VPDYL4XXYYOF4RW","json":"https://pith.science/pith/K5ZTJJADXB3VPDYL4XXYYOF4RW.json","graph_json":"https://pith.science/api/pith-number/K5ZTJJADXB3VPDYL4XXYYOF4RW/graph.json","events_json":"https://pith.science/api/pith-number/K5ZTJJADXB3VPDYL4XXYYOF4RW/events.json","paper":"https://pith.science/paper/K5ZTJJAD"},"agent_actions":{"view_html":"https://pith.science/pith/K5ZTJJADXB3VPDYL4XXYYOF4RW","download_json":"https://pith.science/pith/K5ZTJJADXB3VPDYL4XXYYOF4RW.json","view_paper":"https://pith.science/paper/K5ZTJJAD","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2308.10412&json=true","fetch_graph":"https://pith.science/api/pith-number/K5ZTJJADXB3VPDYL4XXYYOF4RW/graph.json","fetch_events":"https://pith.science/api/pith-number/K5ZTJJADXB3VPDYL4XXYYOF4RW/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/K5ZTJJADXB3VPDYL4XXYYOF4RW/action/timestamp_anchor","attest_storage":"https://pith.science/pith/K5ZTJJADXB3VPDYL4XXYYOF4RW/action/storage_attestation","attest_author":"https://pith.science/pith/K5ZTJJADXB3VPDYL4XXYYOF4RW/action/author_attestation","sign_citation":"https://pith.science/pith/K5ZTJJADXB3VPDYL4XXYYOF4RW/action/citation_signature","submit_replication":"https://pith.science/pith/K5ZTJJADXB3VPDYL4XXYYOF4RW/action/replication_record"}},"created_at":"2026-07-05T08:56:13.816498+00:00","updated_at":"2026-07-05T08:56:13.816498+00:00"}