{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2001:XC2DDYBGEASHIE6DQWO2EKYD2V","short_pith_number":"pith:XC2DDYBG","schema_version":"1.0","canonical_sha256":"b8b431e02620247413c3859da22b03d57b85372805d760cb461a2f7e5ceddc89","source":{"kind":"arxiv","id":"hep-th/0110298","version":2},"attestation_state":"computed","paper":{"title":"Quest for Localized 4-D Black Holes in Brane Worlds","license":"","headline":"","cross_cats":["astro-ph","gr-qc","hep-ph"],"primary_cat":"hep-th","authors_text":"Kyriakos Tamvakis (Univ. of Ioannina), Panagiota Kanti (CERN)","submitted_at":"2001-10-31T16:21:00Z","abstract_excerpt":"We investigate the possibility of obtaining localized black hole solutions in brane worlds by introducing a dependence of the four-dimensional line--element on the extra dimension. An analysis, performed for the cases of an empty bulk and of a bulk containing either a scalar or a gauge field, reveals that no conventional type of matter can support such a dependence. Considering a particular ansatz for the five-dimensional line--element that corresponds to a black hole solution with a ``decaying'' horizon, we determine the bulk energy--momentum tensor capable of sustaining such a behaviour. It "},"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":"hep-th/0110298","kind":"arxiv","version":2},"metadata":{"license":"","primary_cat":"hep-th","submitted_at":"2001-10-31T16:21:00Z","cross_cats_sorted":["astro-ph","gr-qc","hep-ph"],"title_canon_sha256":"471d77a3b1fd7adc48ad9e232a9cc3dbf51439380c229d5aa9ac92c200ee5d52","abstract_canon_sha256":"a347002ba98a83c0f0c6af74b56ae0fc0a47ed145ea0692f5575df5cf883893c"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T15:18:28.179229Z","signature_b64":"aQ+PMlQvChgNv2cLHX9CACgxsrh5mz3uve9uBvZgSHv2nl2+pn5jC3sk64xGorJoUcb9+R4PETsbCjcL2AhmDw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"b8b431e02620247413c3859da22b03d57b85372805d760cb461a2f7e5ceddc89","last_reissued_at":"2026-07-04T15:18:28.178818Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T15:18:28.178818Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Quest for Localized 4-D Black Holes in Brane Worlds","license":"","headline":"","cross_cats":["astro-ph","gr-qc","hep-ph"],"primary_cat":"hep-th","authors_text":"Kyriakos Tamvakis (Univ. of Ioannina), Panagiota Kanti (CERN)","submitted_at":"2001-10-31T16:21:00Z","abstract_excerpt":"We investigate the possibility of obtaining localized black hole solutions in brane worlds by introducing a dependence of the four-dimensional line--element on the extra dimension. An analysis, performed for the cases of an empty bulk and of a bulk containing either a scalar or a gauge field, reveals that no conventional type of matter can support such a dependence. Considering a particular ansatz for the five-dimensional line--element that corresponds to a black hole solution with a ``decaying'' horizon, we determine the bulk energy--momentum tensor capable of sustaining such a behaviour. It "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"hep-th/0110298","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/hep-th/0110298/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":"hep-th/0110298","created_at":"2026-07-04T15:18:28.178868+00:00"},{"alias_kind":"arxiv_version","alias_value":"hep-th/0110298v2","created_at":"2026-07-04T15:18:28.178868+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.hep-th/0110298","created_at":"2026-07-04T15:18:28.178868+00:00"},{"alias_kind":"pith_short_12","alias_value":"XC2DDYBGEASH","created_at":"2026-07-04T15:18:28.178868+00:00"},{"alias_kind":"pith_short_16","alias_value":"XC2DDYBGEASHIE6D","created_at":"2026-07-04T15:18:28.178868+00:00"},{"alias_kind":"pith_short_8","alias_value":"XC2DDYBG","created_at":"2026-07-04T15:18:28.178868+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":2,"internal_anchor_count":2,"sample":[{"citing_arxiv_id":"2606.31330","citing_title":"Two-scalar-field $f(R)$ Thick Branes, Gravitational Resonances and Quasinormal Modes","ref_index":31,"is_internal_anchor":true},{"citing_arxiv_id":"2603.23556","citing_title":"On regular black string spacetimes in nonlinear electrodynamics","ref_index":19,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/XC2DDYBGEASHIE6DQWO2EKYD2V","json":"https://pith.science/pith/XC2DDYBGEASHIE6DQWO2EKYD2V.json","graph_json":"https://pith.science/api/pith-number/XC2DDYBGEASHIE6DQWO2EKYD2V/graph.json","events_json":"https://pith.science/api/pith-number/XC2DDYBGEASHIE6DQWO2EKYD2V/events.json","paper":"https://pith.science/paper/XC2DDYBG"},"agent_actions":{"view_html":"https://pith.science/pith/XC2DDYBGEASHIE6DQWO2EKYD2V","download_json":"https://pith.science/pith/XC2DDYBGEASHIE6DQWO2EKYD2V.json","view_paper":"https://pith.science/paper/XC2DDYBG","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=hep-th/0110298&json=true","fetch_graph":"https://pith.science/api/pith-number/XC2DDYBGEASHIE6DQWO2EKYD2V/graph.json","fetch_events":"https://pith.science/api/pith-number/XC2DDYBGEASHIE6DQWO2EKYD2V/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/XC2DDYBGEASHIE6DQWO2EKYD2V/action/timestamp_anchor","attest_storage":"https://pith.science/pith/XC2DDYBGEASHIE6DQWO2EKYD2V/action/storage_attestation","attest_author":"https://pith.science/pith/XC2DDYBGEASHIE6DQWO2EKYD2V/action/author_attestation","sign_citation":"https://pith.science/pith/XC2DDYBGEASHIE6DQWO2EKYD2V/action/citation_signature","submit_replication":"https://pith.science/pith/XC2DDYBGEASHIE6DQWO2EKYD2V/action/replication_record"}},"created_at":"2026-07-04T15:18:28.178868+00:00","updated_at":"2026-07-04T15:18:28.178868+00:00"}