{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2016:LSO67RBHZYQCCN7PWEIAUEOEXY","short_pith_number":"pith:LSO67RBH","schema_version":"1.0","canonical_sha256":"5c9defc427ce202137efb1100a11c4be2913dc66a31def7ad21b0eb3f3347c73","source":{"kind":"arxiv","id":"1601.05749","version":5},"attestation_state":"computed","paper":{"title":"Gravitational lensing of charged Ayon-Beato-Garcia black holes and non-linear effects of Maxwell fields","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"physics.gen-ph","authors_text":"H. Ghaffarnejad, H. Niad, M. A. Mojahedi","submitted_at":"2016-01-17T22:08:13Z","abstract_excerpt":"Non-singular Ayon-Beato-Garcia (ABG) spherically symmetric static black hole (BH) with charge to mass ratio $q$ is metric solution of Born-Infeld nonlinear Maxwell-Einstein theory. Central region of the BH behaves as (anti-) de Sitter for $(|q|>1)~|q|<1 .$ In case of $|q|=1$ the BH central region behaves as Minkowski flat metric. Nonlinear Electromagnetic (NEM) fields counterpart causes to deviate light geodesics and so light rays will forced to move on effective metric. In this paper we study weak and strong gravitational lensing of light rays by seeking affects of NEM fields counterpart on i"},"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":"1601.05749","kind":"arxiv","version":5},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"physics.gen-ph","submitted_at":"2016-01-17T22:08:13Z","cross_cats_sorted":[],"title_canon_sha256":"b03f67aa9c7a94862b2f39ecacaecf9452b71c88ca69790dd4f15e6476fd3969","abstract_canon_sha256":"fb1e07a4ad2b5b3b9c9db0a9dbc492c7a165813de5ec643f1aa9556eef55fe86"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:21:29.314905Z","signature_b64":"X6GRyDlJ8/vNTjNjdLhMJHjVfnTV8JZhoF6oHyegdchQcdDQ8VfUJX11+cwjH+x58BLTbv/1MHHZP43znezmCQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"5c9defc427ce202137efb1100a11c4be2913dc66a31def7ad21b0eb3f3347c73","last_reissued_at":"2026-05-18T00:21:29.314351Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:21:29.314351Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Gravitational lensing of charged Ayon-Beato-Garcia black holes and non-linear effects of Maxwell fields","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"physics.gen-ph","authors_text":"H. Ghaffarnejad, H. Niad, M. A. Mojahedi","submitted_at":"2016-01-17T22:08:13Z","abstract_excerpt":"Non-singular Ayon-Beato-Garcia (ABG) spherically symmetric static black hole (BH) with charge to mass ratio $q$ is metric solution of Born-Infeld nonlinear Maxwell-Einstein theory. Central region of the BH behaves as (anti-) de Sitter for $(|q|>1)~|q|<1 .$ In case of $|q|=1$ the BH central region behaves as Minkowski flat metric. Nonlinear Electromagnetic (NEM) fields counterpart causes to deviate light geodesics and so light rays will forced to move on effective metric. In this paper we study weak and strong gravitational lensing of light rays by seeking affects of NEM fields counterpart on i"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1601.05749","kind":"arxiv","version":5},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"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":"1601.05749","created_at":"2026-05-18T00:21:29.314452+00:00"},{"alias_kind":"arxiv_version","alias_value":"1601.05749v5","created_at":"2026-05-18T00:21:29.314452+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1601.05749","created_at":"2026-05-18T00:21:29.314452+00:00"},{"alias_kind":"pith_short_12","alias_value":"LSO67RBHZYQC","created_at":"2026-05-18T12:30:29.479603+00:00"},{"alias_kind":"pith_short_16","alias_value":"LSO67RBHZYQCCN7P","created_at":"2026-05-18T12:30:29.479603+00:00"},{"alias_kind":"pith_short_8","alias_value":"LSO67RBH","created_at":"2026-05-18T12:30:29.479603+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2608.10071","citing_title":"Probing nonlinear electrodynamics-sourced black holes via light and orbital mechanics","ref_index":46,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/LSO67RBHZYQCCN7PWEIAUEOEXY","json":"https://pith.science/pith/LSO67RBHZYQCCN7PWEIAUEOEXY.json","graph_json":"https://pith.science/api/pith-number/LSO67RBHZYQCCN7PWEIAUEOEXY/graph.json","events_json":"https://pith.science/api/pith-number/LSO67RBHZYQCCN7PWEIAUEOEXY/events.json","paper":"https://pith.science/paper/LSO67RBH"},"agent_actions":{"view_html":"https://pith.science/pith/LSO67RBHZYQCCN7PWEIAUEOEXY","download_json":"https://pith.science/pith/LSO67RBHZYQCCN7PWEIAUEOEXY.json","view_paper":"https://pith.science/paper/LSO67RBH","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1601.05749&json=true","fetch_graph":"https://pith.science/api/pith-number/LSO67RBHZYQCCN7PWEIAUEOEXY/graph.json","fetch_events":"https://pith.science/api/pith-number/LSO67RBHZYQCCN7PWEIAUEOEXY/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/LSO67RBHZYQCCN7PWEIAUEOEXY/action/timestamp_anchor","attest_storage":"https://pith.science/pith/LSO67RBHZYQCCN7PWEIAUEOEXY/action/storage_attestation","attest_author":"https://pith.science/pith/LSO67RBHZYQCCN7PWEIAUEOEXY/action/author_attestation","sign_citation":"https://pith.science/pith/LSO67RBHZYQCCN7PWEIAUEOEXY/action/citation_signature","submit_replication":"https://pith.science/pith/LSO67RBHZYQCCN7PWEIAUEOEXY/action/replication_record"}},"created_at":"2026-05-18T00:21:29.314452+00:00","updated_at":"2026-05-18T00:21:29.314452+00:00"}