{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2019:AFZMOIFI4ALDUUXMN32YYW5OVT","short_pith_number":"pith:AFZMOIFI","schema_version":"1.0","canonical_sha256":"0172c720a8e0163a52ec6ef58c5baeacc9b19b6112e805883db929642b64b7a9","source":{"kind":"arxiv","id":"1902.05941","version":2},"attestation_state":"computed","paper":{"title":"Five-dimensional scale-dependent black holes with constant curvature and Solv horizons","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-th"],"primary_cat":"gr-qc","authors_text":"\\'A. Rinc\\'on, E. Contreras, P. Bargue\\~no","submitted_at":"2019-02-15T18:49:00Z","abstract_excerpt":"In this work, we investigate five-dimensional scale-dependent black hole solutions by modelling their event horizon with some of the eight Thurston three-dimensional geometries. Specifically, we construct constant curvature scale-dependent black holes and also the more exotic scale-dependent Solv black hole. These new solutions are obtained by promoting both the gravitational and the cosmological couplings to $r$-dependent functions, in light of a particular description of the effective action inspired by the high energy philosophy. Interestingly, the so-called running parameter, together with"},"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":"1902.05941","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2019-02-15T18:49:00Z","cross_cats_sorted":["hep-th"],"title_canon_sha256":"3a0918f924c0196df4e1b8ad3e6a2ee5a7746527439600ff3059337fde527f75","abstract_canon_sha256":"b04b1e2c2d402a1ce96a940a0cdb946386d90fa28d46fd9505c8bd47564fb53e"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T01:03:58.018164Z","signature_b64":"RWKBQJ+Kmy6qbkAUvllsBHn9W5dJT4t5vyIiFqxZbiL0va+0rOvrmjSaoFCSpdUBTxEf52v8xn95Cu8oSRw4DA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"0172c720a8e0163a52ec6ef58c5baeacc9b19b6112e805883db929642b64b7a9","last_reissued_at":"2026-07-05T01:03:58.017742Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T01:03:58.017742Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Five-dimensional scale-dependent black holes with constant curvature and Solv horizons","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-th"],"primary_cat":"gr-qc","authors_text":"\\'A. Rinc\\'on, E. Contreras, P. Bargue\\~no","submitted_at":"2019-02-15T18:49:00Z","abstract_excerpt":"In this work, we investigate five-dimensional scale-dependent black hole solutions by modelling their event horizon with some of the eight Thurston three-dimensional geometries. Specifically, we construct constant curvature scale-dependent black holes and also the more exotic scale-dependent Solv black hole. These new solutions are obtained by promoting both the gravitational and the cosmological couplings to $r$-dependent functions, in light of a particular description of the effective action inspired by the high energy philosophy. Interestingly, the so-called running parameter, together with"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1902.05941","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/1902.05941/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":"1902.05941","created_at":"2026-07-05T01:03:58.017801+00:00"},{"alias_kind":"arxiv_version","alias_value":"1902.05941v2","created_at":"2026-07-05T01:03:58.017801+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1902.05941","created_at":"2026-07-05T01:03:58.017801+00:00"},{"alias_kind":"pith_short_12","alias_value":"AFZMOIFI4ALD","created_at":"2026-07-05T01:03:58.017801+00:00"},{"alias_kind":"pith_short_16","alias_value":"AFZMOIFI4ALDUUXM","created_at":"2026-07-05T01:03:58.017801+00:00"},{"alias_kind":"pith_short_8","alias_value":"AFZMOIFI","created_at":"2026-07-05T01:03:58.017801+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"1907.03545","citing_title":"Relativistic strange quark stars in Lovelock gravity","ref_index":91,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/AFZMOIFI4ALDUUXMN32YYW5OVT","json":"https://pith.science/pith/AFZMOIFI4ALDUUXMN32YYW5OVT.json","graph_json":"https://pith.science/api/pith-number/AFZMOIFI4ALDUUXMN32YYW5OVT/graph.json","events_json":"https://pith.science/api/pith-number/AFZMOIFI4ALDUUXMN32YYW5OVT/events.json","paper":"https://pith.science/paper/AFZMOIFI"},"agent_actions":{"view_html":"https://pith.science/pith/AFZMOIFI4ALDUUXMN32YYW5OVT","download_json":"https://pith.science/pith/AFZMOIFI4ALDUUXMN32YYW5OVT.json","view_paper":"https://pith.science/paper/AFZMOIFI","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1902.05941&json=true","fetch_graph":"https://pith.science/api/pith-number/AFZMOIFI4ALDUUXMN32YYW5OVT/graph.json","fetch_events":"https://pith.science/api/pith-number/AFZMOIFI4ALDUUXMN32YYW5OVT/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/AFZMOIFI4ALDUUXMN32YYW5OVT/action/timestamp_anchor","attest_storage":"https://pith.science/pith/AFZMOIFI4ALDUUXMN32YYW5OVT/action/storage_attestation","attest_author":"https://pith.science/pith/AFZMOIFI4ALDUUXMN32YYW5OVT/action/author_attestation","sign_citation":"https://pith.science/pith/AFZMOIFI4ALDUUXMN32YYW5OVT/action/citation_signature","submit_replication":"https://pith.science/pith/AFZMOIFI4ALDUUXMN32YYW5OVT/action/replication_record"}},"created_at":"2026-07-05T01:03:58.017801+00:00","updated_at":"2026-07-05T01:03:58.017801+00:00"}