{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2025:BOUJSRE5TJENHOKSWE4MED2IOD","short_pith_number":"pith:BOUJSRE5","schema_version":"1.0","canonical_sha256":"0ba899449d9a48d3b952b138c20f4870c6bbd55d21587d824ccd52c4321a7f84","source":{"kind":"arxiv","id":"2503.00678","version":2},"attestation_state":"computed","paper":{"title":"Black holes surrounded by massive vector fields in Kaluza-Klein gravity","license":"http://creativecommons.org/licenses/by-nc-nd/4.0/","headline":"","cross_cats":["astro-ph.HE","hep-th"],"primary_cat":"gr-qc","authors_text":"Ankit Anand, B. Cuadros-Melgar, Kimet Jusufi, Kourosh Nozari, Sara Saghafi","submitted_at":"2025-03-02T01:00:56Z","abstract_excerpt":"We present an exact black hole solution surrounded by massive vector fields predicted by Kaluza-Klein (KK) gravity. KK gravity in four dimensions (4D) is of particular interest, as it predicts a tower of particle states, including gravitons with spin-0 and spin-1 components, in addition to the massless spin-2 gravitons of general relativity. The extra degrees of freedom in the gravitational sector modify the law of gravity, allowing the theory to explain the effects attributed to dark matter in the universe. In this paper, we construct a black hole solution surrounded by massive spin-1 gravito"},"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":"2503.00678","kind":"arxiv","version":2},"metadata":{"license":"http://creativecommons.org/licenses/by-nc-nd/4.0/","primary_cat":"gr-qc","submitted_at":"2025-03-02T01:00:56Z","cross_cats_sorted":["astro-ph.HE","hep-th"],"title_canon_sha256":"e3e782929105e0f1613e9653bee4c5f0440e6ad9bc4b695e99244096c223c69b","abstract_canon_sha256":"a2a28f9597e9cbfa3e9fc5be5d6cb55a56de254903fb0817bc00d19857ffc864"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T11:03:21.839834Z","signature_b64":"Rfz3uEOPx8gzv4uVsnLCp2QhfSjNzOxeQJ0hcQ7fgIxtKdh4gbqASQFWenITe9glwM10hn7qlrvIu9HEhbMaCQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"0ba899449d9a48d3b952b138c20f4870c6bbd55d21587d824ccd52c4321a7f84","last_reissued_at":"2026-07-05T11:03:21.839347Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T11:03:21.839347Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Black holes surrounded by massive vector fields in Kaluza-Klein gravity","license":"http://creativecommons.org/licenses/by-nc-nd/4.0/","headline":"","cross_cats":["astro-ph.HE","hep-th"],"primary_cat":"gr-qc","authors_text":"Ankit Anand, B. Cuadros-Melgar, Kimet Jusufi, Kourosh Nozari, Sara Saghafi","submitted_at":"2025-03-02T01:00:56Z","abstract_excerpt":"We present an exact black hole solution surrounded by massive vector fields predicted by Kaluza-Klein (KK) gravity. KK gravity in four dimensions (4D) is of particular interest, as it predicts a tower of particle states, including gravitons with spin-0 and spin-1 components, in addition to the massless spin-2 gravitons of general relativity. The extra degrees of freedom in the gravitational sector modify the law of gravity, allowing the theory to explain the effects attributed to dark matter in the universe. In this paper, we construct a black hole solution surrounded by massive spin-1 gravito"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2503.00678","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/2503.00678/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":"2503.00678","created_at":"2026-07-05T11:03:21.839415+00:00"},{"alias_kind":"arxiv_version","alias_value":"2503.00678v2","created_at":"2026-07-05T11:03:21.839415+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2503.00678","created_at":"2026-07-05T11:03:21.839415+00:00"},{"alias_kind":"pith_short_12","alias_value":"BOUJSRE5TJEN","created_at":"2026-07-05T11:03:21.839415+00:00"},{"alias_kind":"pith_short_16","alias_value":"BOUJSRE5TJENHOKS","created_at":"2026-07-05T11:03:21.839415+00:00"},{"alias_kind":"pith_short_8","alias_value":"BOUJSRE5","created_at":"2026-07-05T11:03:21.839415+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2411.14176","citing_title":"Dark Universe inspired by the Kaluza-Klein gravity and impact on Primordial Gravitational Waves","ref_index":53,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/BOUJSRE5TJENHOKSWE4MED2IOD","json":"https://pith.science/pith/BOUJSRE5TJENHOKSWE4MED2IOD.json","graph_json":"https://pith.science/api/pith-number/BOUJSRE5TJENHOKSWE4MED2IOD/graph.json","events_json":"https://pith.science/api/pith-number/BOUJSRE5TJENHOKSWE4MED2IOD/events.json","paper":"https://pith.science/paper/BOUJSRE5"},"agent_actions":{"view_html":"https://pith.science/pith/BOUJSRE5TJENHOKSWE4MED2IOD","download_json":"https://pith.science/pith/BOUJSRE5TJENHOKSWE4MED2IOD.json","view_paper":"https://pith.science/paper/BOUJSRE5","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2503.00678&json=true","fetch_graph":"https://pith.science/api/pith-number/BOUJSRE5TJENHOKSWE4MED2IOD/graph.json","fetch_events":"https://pith.science/api/pith-number/BOUJSRE5TJENHOKSWE4MED2IOD/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/BOUJSRE5TJENHOKSWE4MED2IOD/action/timestamp_anchor","attest_storage":"https://pith.science/pith/BOUJSRE5TJENHOKSWE4MED2IOD/action/storage_attestation","attest_author":"https://pith.science/pith/BOUJSRE5TJENHOKSWE4MED2IOD/action/author_attestation","sign_citation":"https://pith.science/pith/BOUJSRE5TJENHOKSWE4MED2IOD/action/citation_signature","submit_replication":"https://pith.science/pith/BOUJSRE5TJENHOKSWE4MED2IOD/action/replication_record"}},"created_at":"2026-07-05T11:03:21.839415+00:00","updated_at":"2026-07-05T11:03:21.839415+00:00"}