{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2023:F6L7RBLF7FRDVV4CYWHO4VFIOK","short_pith_number":"pith:F6L7RBLF","schema_version":"1.0","canonical_sha256":"2f97f88565f9623ad782c58eee54a87292907a959c0ced78b323512174ceb36b","source":{"kind":"arxiv","id":"2311.04680","version":1},"attestation_state":"computed","paper":{"title":"Holographic Einstein Rings of Black Holes in Scalar-Tensor-Vector Gravity","license":"http://creativecommons.org/publicdomain/zero/1.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"M. Israr Aslam, Rabia Saleem, Xiao-Xiong Zeng, Xin-Yun Hu","submitted_at":"2023-11-08T13:39:19Z","abstract_excerpt":"With the help of AdS/CFT correspondence, we analyze the holographic Einstein images via the response function of the complex scalar field as a probe wave on the AdS Schwarzschild scalar-tensor-vector gravity (STVG) black hole (BH). We find that the amplitude of the response function $|\\langle O\\rangle|$ decreases with the increasing values of the coupling parameter $\\alpha$, while it increases with the decreasing values of temperature $T$. The frequency $\\omega$ of the wave source also plays a significant role in wave periods, as we increase the values of $\\omega$, we find a decrease in period"},"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":"2311.04680","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/publicdomain/zero/1.0/","primary_cat":"gr-qc","submitted_at":"2023-11-08T13:39:19Z","cross_cats_sorted":[],"title_canon_sha256":"7d4f220e2bce273918ea6a534e22c56bfd4869947e206c84f2155b1cac48624c","abstract_canon_sha256":"b2ae2917fd5b4715ce151bc99e7fea19655443c00864a4f97b9494a9ec34c529"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T07:10:39.855934Z","signature_b64":"Rn/bVPzNFtu7K2NwbpfZOyvzAOIYRNyyPql6ndxmjLh9yBfFQODnKds9D/AZW+MYAFZY2M+VBoMaorBWG6RRBA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"2f97f88565f9623ad782c58eee54a87292907a959c0ced78b323512174ceb36b","last_reissued_at":"2026-07-05T07:10:39.855439Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T07:10:39.855439Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Holographic Einstein Rings of Black Holes in Scalar-Tensor-Vector Gravity","license":"http://creativecommons.org/publicdomain/zero/1.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"M. Israr Aslam, Rabia Saleem, Xiao-Xiong Zeng, Xin-Yun Hu","submitted_at":"2023-11-08T13:39:19Z","abstract_excerpt":"With the help of AdS/CFT correspondence, we analyze the holographic Einstein images via the response function of the complex scalar field as a probe wave on the AdS Schwarzschild scalar-tensor-vector gravity (STVG) black hole (BH). We find that the amplitude of the response function $|\\langle O\\rangle|$ decreases with the increasing values of the coupling parameter $\\alpha$, while it increases with the decreasing values of temperature $T$. The frequency $\\omega$ of the wave source also plays a significant role in wave periods, as we increase the values of $\\omega$, we find a decrease in period"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2311.04680","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/2311.04680/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":"2311.04680","created_at":"2026-07-05T07:10:39.855497+00:00"},{"alias_kind":"arxiv_version","alias_value":"2311.04680v1","created_at":"2026-07-05T07:10:39.855497+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2311.04680","created_at":"2026-07-05T07:10:39.855497+00:00"},{"alias_kind":"pith_short_12","alias_value":"F6L7RBLF7FRD","created_at":"2026-07-05T07:10:39.855497+00:00"},{"alias_kind":"pith_short_16","alias_value":"F6L7RBLF7FRDVV4C","created_at":"2026-07-05T07:10:39.855497+00:00"},{"alias_kind":"pith_short_8","alias_value":"F6L7RBLF","created_at":"2026-07-05T07:10:39.855497+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2501.15139","citing_title":"Holographic Einstein Ring of Quantum Corrected AdS-Reissner-Nordstrom Black Holes in Kiselev Spacetime","ref_index":36,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/F6L7RBLF7FRDVV4CYWHO4VFIOK","json":"https://pith.science/pith/F6L7RBLF7FRDVV4CYWHO4VFIOK.json","graph_json":"https://pith.science/api/pith-number/F6L7RBLF7FRDVV4CYWHO4VFIOK/graph.json","events_json":"https://pith.science/api/pith-number/F6L7RBLF7FRDVV4CYWHO4VFIOK/events.json","paper":"https://pith.science/paper/F6L7RBLF"},"agent_actions":{"view_html":"https://pith.science/pith/F6L7RBLF7FRDVV4CYWHO4VFIOK","download_json":"https://pith.science/pith/F6L7RBLF7FRDVV4CYWHO4VFIOK.json","view_paper":"https://pith.science/paper/F6L7RBLF","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2311.04680&json=true","fetch_graph":"https://pith.science/api/pith-number/F6L7RBLF7FRDVV4CYWHO4VFIOK/graph.json","fetch_events":"https://pith.science/api/pith-number/F6L7RBLF7FRDVV4CYWHO4VFIOK/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/F6L7RBLF7FRDVV4CYWHO4VFIOK/action/timestamp_anchor","attest_storage":"https://pith.science/pith/F6L7RBLF7FRDVV4CYWHO4VFIOK/action/storage_attestation","attest_author":"https://pith.science/pith/F6L7RBLF7FRDVV4CYWHO4VFIOK/action/author_attestation","sign_citation":"https://pith.science/pith/F6L7RBLF7FRDVV4CYWHO4VFIOK/action/citation_signature","submit_replication":"https://pith.science/pith/F6L7RBLF7FRDVV4CYWHO4VFIOK/action/replication_record"}},"created_at":"2026-07-05T07:10:39.855497+00:00","updated_at":"2026-07-05T07:10:39.855497+00:00"}