{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2026:MCHI2NEU74KOMOVCL6HCWDTCNK","short_pith_number":"pith:MCHI2NEU","schema_version":"1.0","canonical_sha256":"608e8d3494ff14e63aa25f8e2b0e626a9e5900fdccd3dcc031c1676f3bf3e99c","source":{"kind":"arxiv","id":"2603.28415","version":2},"attestation_state":"computed","paper":{"title":"Long-lived quasinormal frequencies for regular black hole supported by the Einasto profile in the presence of the magnetic field","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"Milena Skvortsova","submitted_at":"2026-03-30T13:27:04Z","abstract_excerpt":"We investigate quasinormal modes, grey-body factors, and absorption cross-sections of a massive scalar field in regular black-hole spacetimes supported by the Einasto density profile. The analysis is performed for $\\tilde n=1/2$, $1$, and $5$, where the scalar mass $\\mu$ is treated as an effective parameter induced by an external environment. Quasinormal frequencies are computed with high-order WKB expansions and Pad\\'e resummation, and are cross-checked by time-domain evolution. We show that increasing the effective mass and varying the Einasto parameters can strongly suppress the damping rat"},"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":"2603.28415","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2026-03-30T13:27:04Z","cross_cats_sorted":[],"title_canon_sha256":"6c12bfa98dede94bf7d69951212c70755f37a86abd59fa04d50c44c22066e071","abstract_canon_sha256":"299f12ddac04c43f7f7476814cf1be26265d38653f426951e6a8ea98c31e091e"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-08-04T02:09:36.643690Z","signature_b64":"u6lSsbuBx/xcIx1hOw7O9cnL1qejKOkcNAVQ7kMEoZuZnXzBqr5EscAE3rtf8CX52sB3qiwC96VHoE89mzoGAQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"608e8d3494ff14e63aa25f8e2b0e626a9e5900fdccd3dcc031c1676f3bf3e99c","last_reissued_at":"2026-08-04T02:09:36.641972Z","signature_status":"signed_v1","first_computed_at":"2026-08-04T02:09:36.641972Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Long-lived quasinormal frequencies for regular black hole supported by the Einasto profile in the presence of the magnetic field","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"Milena Skvortsova","submitted_at":"2026-03-30T13:27:04Z","abstract_excerpt":"We investigate quasinormal modes, grey-body factors, and absorption cross-sections of a massive scalar field in regular black-hole spacetimes supported by the Einasto density profile. The analysis is performed for $\\tilde n=1/2$, $1$, and $5$, where the scalar mass $\\mu$ is treated as an effective parameter induced by an external environment. Quasinormal frequencies are computed with high-order WKB expansions and Pad\\'e resummation, and are cross-checked by time-domain evolution. We show that increasing the effective mass and varying the Einasto parameters can strongly suppress the damping rat"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2603.28415","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/2603.28415/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":"2603.28415","created_at":"2026-08-04T02:09:36.643523+00:00"},{"alias_kind":"arxiv_version","alias_value":"2603.28415v2","created_at":"2026-08-04T02:09:36.643523+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2603.28415","created_at":"2026-08-04T02:09:36.643523+00:00"},{"alias_kind":"pith_short_12","alias_value":"MCHI2NEU74KO","created_at":"2026-08-04T02:09:36.643523+00:00"},{"alias_kind":"pith_short_16","alias_value":"MCHI2NEU74KOMOVC","created_at":"2026-08-04T02:09:36.643523+00:00"},{"alias_kind":"pith_short_8","alias_value":"MCHI2NEU","created_at":"2026-08-04T02:09:36.643523+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":14,"internal_anchor_count":14,"sample":[{"citing_arxiv_id":"2607.07955","citing_title":"Wave and particle probes of a regular T-duality-inspired black hole with gravitational self-energy","ref_index":58,"is_internal_anchor":true},{"citing_arxiv_id":"2606.08631","citing_title":"Hawking Radiation from the Dymnikova Regular Black Hole","ref_index":33,"is_internal_anchor":true},{"citing_arxiv_id":"2606.08351","citing_title":"Hawking Emission from Black Holes Evaporating toward Wormholes and the Accuracy of the WKB Approximation","ref_index":48,"is_internal_anchor":true},{"citing_arxiv_id":"2605.21533","citing_title":"Long-lived quasinormal modes of Asymptotically de Sitter Black Holes in Generalized Proca Theory","ref_index":34,"is_internal_anchor":true},{"citing_arxiv_id":"2604.24349","citing_title":"Scalar, electromagnetic, and Dirac perturbations of regular black holes constituting primordial dark matter","ref_index":52,"is_internal_anchor":true},{"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":35,"is_internal_anchor":true},{"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":73,"is_internal_anchor":true},{"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":28,"is_internal_anchor":true},{"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":108,"is_internal_anchor":true},{"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":78,"is_internal_anchor":true},{"citing_arxiv_id":"2604.25961","citing_title":"Strong-field signatures of a regular black hole in an Einasto dark matter halo","ref_index":38,"is_internal_anchor":true},{"citing_arxiv_id":"2604.24659","citing_title":"Hawking Temperature, Sparsity and Energy Emission Rate of Dark Matter Halo Regular Black Holes","ref_index":36,"is_internal_anchor":true},{"citing_arxiv_id":"2604.24349","citing_title":"Scalar, electromagnetic, and Dirac perturbations of regular black holes constituting primordial dark matter","ref_index":52,"is_internal_anchor":true},{"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":108,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/MCHI2NEU74KOMOVCL6HCWDTCNK","json":"https://pith.science/pith/MCHI2NEU74KOMOVCL6HCWDTCNK.json","graph_json":"https://pith.science/api/pith-number/MCHI2NEU74KOMOVCL6HCWDTCNK/graph.json","events_json":"https://pith.science/api/pith-number/MCHI2NEU74KOMOVCL6HCWDTCNK/events.json","paper":"https://pith.science/paper/MCHI2NEU"},"agent_actions":{"view_html":"https://pith.science/pith/MCHI2NEU74KOMOVCL6HCWDTCNK","download_json":"https://pith.science/pith/MCHI2NEU74KOMOVCL6HCWDTCNK.json","view_paper":"https://pith.science/paper/MCHI2NEU","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2603.28415&json=true","fetch_graph":"https://pith.science/api/pith-number/MCHI2NEU74KOMOVCL6HCWDTCNK/graph.json","fetch_events":"https://pith.science/api/pith-number/MCHI2NEU74KOMOVCL6HCWDTCNK/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/MCHI2NEU74KOMOVCL6HCWDTCNK/action/timestamp_anchor","attest_storage":"https://pith.science/pith/MCHI2NEU74KOMOVCL6HCWDTCNK/action/storage_attestation","attest_author":"https://pith.science/pith/MCHI2NEU74KOMOVCL6HCWDTCNK/action/author_attestation","sign_citation":"https://pith.science/pith/MCHI2NEU74KOMOVCL6HCWDTCNK/action/citation_signature","submit_replication":"https://pith.science/pith/MCHI2NEU74KOMOVCL6HCWDTCNK/action/replication_record"}},"created_at":"2026-08-04T02:09:36.643523+00:00","updated_at":"2026-08-04T02:09:36.643523+00:00"}