{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2026:H3XNOZY5UF3F24XZALBD73GEH4","short_pith_number":"pith:H3XNOZY5","schema_version":"1.0","canonical_sha256":"3eeed7671da1765d72f902c23fecc43f1256f7baaa6bb352ef7f5c6262f63329","source":{"kind":"arxiv","id":"2607.07715","version":1},"attestation_state":"computed","paper":{"title":"Gravitational perturbations of a regular T-duality inspired black hole: Quasinormal modes, excitation factors, and time-domain evolution","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-th"],"primary_cat":"gr-qc","authors_text":"Bekir Can L\\\"utf\\\"uo\\u{g}lu, Javlon Rayimbaev, Mardon Abdullaev, Shavkat Karshiboev, Shokhzod Jumaniyozov","submitted_at":"2026-07-03T18:43:45Z","abstract_excerpt":"We study axial gravitational perturbations of the neutral regular black hole generated by a non-local, T-duality-inspired zero-point length and the associated gravitational self-energy. In this geometry, the usual point source is replaced by a regular core, and the zero-point length controls the departure from the Schwarzschild limit. We compute the fundamental quasinormal modes and several overtones using high-order WKB--Pad\\'e methods, and we verify the dominant mode via direct time-domain evolution. When the zero-point length is turned on, the real parts of the ADM-scaled frequencies increa"},"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":"2607.07715","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2026-07-03T18:43:45Z","cross_cats_sorted":["hep-th"],"title_canon_sha256":"226121b3f97410378fc2a9209d5418bea5cac7c2667d265e075a222b74157ee3","abstract_canon_sha256":"1fe63542ca62ee6c5f1552a60736553a1b5977bfd2bbaf44a08d7fe26a5c890a"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-10T00:18:47.082159Z","signature_b64":"LUGLTgrE5ERe0p8rFa6fskmSVLohL/4zkpkNlkYuJUJRR2l94lyZLLmVlyw2vy2WL25JC67evvHE1xbwPc21BA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"3eeed7671da1765d72f902c23fecc43f1256f7baaa6bb352ef7f5c6262f63329","last_reissued_at":"2026-07-10T00:18:47.081677Z","signature_status":"signed_v1","first_computed_at":"2026-07-10T00:18:47.081677Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Gravitational perturbations of a regular T-duality inspired black hole: Quasinormal modes, excitation factors, and time-domain evolution","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-th"],"primary_cat":"gr-qc","authors_text":"Bekir Can L\\\"utf\\\"uo\\u{g}lu, Javlon Rayimbaev, Mardon Abdullaev, Shavkat Karshiboev, Shokhzod Jumaniyozov","submitted_at":"2026-07-03T18:43:45Z","abstract_excerpt":"We study axial gravitational perturbations of the neutral regular black hole generated by a non-local, T-duality-inspired zero-point length and the associated gravitational self-energy. In this geometry, the usual point source is replaced by a regular core, and the zero-point length controls the departure from the Schwarzschild limit. We compute the fundamental quasinormal modes and several overtones using high-order WKB--Pad\\'e methods, and we verify the dominant mode via direct time-domain evolution. When the zero-point length is turned on, the real parts of the ADM-scaled frequencies increa"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2607.07715","kind":"arxiv","version":1},"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/2607.07715/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":"2607.07715","created_at":"2026-07-10T00:18:47.081743+00:00"},{"alias_kind":"arxiv_version","alias_value":"2607.07715v1","created_at":"2026-07-10T00:18:47.081743+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2607.07715","created_at":"2026-07-10T00:18:47.081743+00:00"},{"alias_kind":"pith_short_12","alias_value":"H3XNOZY5UF3F","created_at":"2026-07-10T00:18:47.081743+00:00"},{"alias_kind":"pith_short_16","alias_value":"H3XNOZY5UF3F24XZ","created_at":"2026-07-10T00:18:47.081743+00:00"},{"alias_kind":"pith_short_8","alias_value":"H3XNOZY5","created_at":"2026-07-10T00:18:47.081743+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":0,"internal_anchor_count":0,"sample":[]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/H3XNOZY5UF3F24XZALBD73GEH4","json":"https://pith.science/pith/H3XNOZY5UF3F24XZALBD73GEH4.json","graph_json":"https://pith.science/api/pith-number/H3XNOZY5UF3F24XZALBD73GEH4/graph.json","events_json":"https://pith.science/api/pith-number/H3XNOZY5UF3F24XZALBD73GEH4/events.json","paper":"https://pith.science/paper/H3XNOZY5"},"agent_actions":{"view_html":"https://pith.science/pith/H3XNOZY5UF3F24XZALBD73GEH4","download_json":"https://pith.science/pith/H3XNOZY5UF3F24XZALBD73GEH4.json","view_paper":"https://pith.science/paper/H3XNOZY5","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2607.07715&json=true","fetch_graph":"https://pith.science/api/pith-number/H3XNOZY5UF3F24XZALBD73GEH4/graph.json","fetch_events":"https://pith.science/api/pith-number/H3XNOZY5UF3F24XZALBD73GEH4/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/H3XNOZY5UF3F24XZALBD73GEH4/action/timestamp_anchor","attest_storage":"https://pith.science/pith/H3XNOZY5UF3F24XZALBD73GEH4/action/storage_attestation","attest_author":"https://pith.science/pith/H3XNOZY5UF3F24XZALBD73GEH4/action/author_attestation","sign_citation":"https://pith.science/pith/H3XNOZY5UF3F24XZALBD73GEH4/action/citation_signature","submit_replication":"https://pith.science/pith/H3XNOZY5UF3F24XZALBD73GEH4/action/replication_record"}},"created_at":"2026-07-10T00:18:47.081743+00:00","updated_at":"2026-07-10T00:18:47.081743+00:00"}