{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2025:AC3UZ46EI5PXLPHRWXP33YIWZD","short_pith_number":"pith:AC3UZ46E","schema_version":"1.0","canonical_sha256":"00b74cf3c4475f75bcf1b5dfbde116c8efabbc402693cfa79c0dd6f9745dc5b5","source":{"kind":"arxiv","id":"2505.13018","version":2},"attestation_state":"computed","paper":{"title":"Holographic Einstein Ring of AdS Reissner Nordstr$\\ddot{o}$m Black Holes with Euler Heisenberg Nonlinear Electrodynamics","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"hep-th","authors_text":"Abhishek Baruah, Prabwal Phukon","submitted_at":"2025-05-19T12:03:26Z","abstract_excerpt":"This study, situated within the framework of the AdS/CFT correspondence, employs wave optics methods to investigate the Einstein ring structure of quantum corrected AdS Reissner Nordstr$\\ddot{o}$m black holes governed by Euler Heisenberg nonlinear electrodynamics. A wave source placed on the AdS boundary yields a response function on the antipodal side, from which a virtual optical system with a convex lens reconstructs the holographic image of the Einstein ring. The analysis systematically explores the impact of physical parameters and observer position on the ring's morphology. As the observ"},"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":"2505.13018","kind":"arxiv","version":2},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"hep-th","submitted_at":"2025-05-19T12:03:26Z","cross_cats_sorted":[],"title_canon_sha256":"0ff8d48efec4c8592dac52973fca990ea50519fddcc79d60b69f9ff199cb7c2e","abstract_canon_sha256":"dbd51ea294bd5eac79907555d79f41b8b3854ec46c27a379eecc8cc1e613618c"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T11:07:24.973794Z","signature_b64":"Ijdv95EQY3Y39zJc7kqI0WJbUlyWKGzgWtJkrFwvh+i254fnOjEFtw9HNu+3VBMM9DsYGywn5cisa+DZjAQ/Cg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"00b74cf3c4475f75bcf1b5dfbde116c8efabbc402693cfa79c0dd6f9745dc5b5","last_reissued_at":"2026-07-05T11:07:24.973321Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T11:07:24.973321Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Holographic Einstein Ring of AdS Reissner Nordstr$\\ddot{o}$m Black Holes with Euler Heisenberg Nonlinear Electrodynamics","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"hep-th","authors_text":"Abhishek Baruah, Prabwal Phukon","submitted_at":"2025-05-19T12:03:26Z","abstract_excerpt":"This study, situated within the framework of the AdS/CFT correspondence, employs wave optics methods to investigate the Einstein ring structure of quantum corrected AdS Reissner Nordstr$\\ddot{o}$m black holes governed by Euler Heisenberg nonlinear electrodynamics. A wave source placed on the AdS boundary yields a response function on the antipodal side, from which a virtual optical system with a convex lens reconstructs the holographic image of the Einstein ring. The analysis systematically explores the impact of physical parameters and observer position on the ring's morphology. As the observ"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2505.13018","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/2505.13018/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":"2505.13018","created_at":"2026-07-05T11:07:24.973373+00:00"},{"alias_kind":"arxiv_version","alias_value":"2505.13018v2","created_at":"2026-07-05T11:07:24.973373+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2505.13018","created_at":"2026-07-05T11:07:24.973373+00:00"},{"alias_kind":"pith_short_12","alias_value":"AC3UZ46EI5PX","created_at":"2026-07-05T11:07:24.973373+00:00"},{"alias_kind":"pith_short_16","alias_value":"AC3UZ46EI5PXLPHR","created_at":"2026-07-05T11:07:24.973373+00:00"},{"alias_kind":"pith_short_8","alias_value":"AC3UZ46E","created_at":"2026-07-05T11:07:24.973373+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2507.23198","citing_title":"High-order QED correction impacts on phase transition of the Euler-Heisenberg dS spacetime","ref_index":50,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/AC3UZ46EI5PXLPHRWXP33YIWZD","json":"https://pith.science/pith/AC3UZ46EI5PXLPHRWXP33YIWZD.json","graph_json":"https://pith.science/api/pith-number/AC3UZ46EI5PXLPHRWXP33YIWZD/graph.json","events_json":"https://pith.science/api/pith-number/AC3UZ46EI5PXLPHRWXP33YIWZD/events.json","paper":"https://pith.science/paper/AC3UZ46E"},"agent_actions":{"view_html":"https://pith.science/pith/AC3UZ46EI5PXLPHRWXP33YIWZD","download_json":"https://pith.science/pith/AC3UZ46EI5PXLPHRWXP33YIWZD.json","view_paper":"https://pith.science/paper/AC3UZ46E","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2505.13018&json=true","fetch_graph":"https://pith.science/api/pith-number/AC3UZ46EI5PXLPHRWXP33YIWZD/graph.json","fetch_events":"https://pith.science/api/pith-number/AC3UZ46EI5PXLPHRWXP33YIWZD/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/AC3UZ46EI5PXLPHRWXP33YIWZD/action/timestamp_anchor","attest_storage":"https://pith.science/pith/AC3UZ46EI5PXLPHRWXP33YIWZD/action/storage_attestation","attest_author":"https://pith.science/pith/AC3UZ46EI5PXLPHRWXP33YIWZD/action/author_attestation","sign_citation":"https://pith.science/pith/AC3UZ46EI5PXLPHRWXP33YIWZD/action/citation_signature","submit_replication":"https://pith.science/pith/AC3UZ46EI5PXLPHRWXP33YIWZD/action/replication_record"}},"created_at":"2026-07-05T11:07:24.973373+00:00","updated_at":"2026-07-05T11:07:24.973373+00:00"}