{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:N5DPPFQ5BNZTNFPUFFRBYPSHY5","short_pith_number":"pith:N5DPPFQ5","schema_version":"1.0","canonical_sha256":"6f46f7961d0b733695f429621c3e47c74c31eb35b7ba44df700997b0cde823fe","source":{"kind":"arxiv","id":"1702.04636","version":2},"attestation_state":"computed","paper":{"title":"Hawking Radiation and Deflection of Light from Rindler Modified Schwarzschild Black Hole","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"physics.gen-ph","authors_text":"A. Ovgun, I. Sakalli","submitted_at":"2017-02-14T01:41:06Z","abstract_excerpt":"We investigate the Hawking radiation of massive spin-1 vector particles, which are coupled to vacuum fluctuations of a quantum field, from Rindler modified Schwarzschild black hole. Rindler acceleration is used to produce the post-general relativistic theory of gravity for the distant field of a point mass. The gravitational lensing problem of the Rindler modified Schwarzschild black hole is also studied. We compute the deflection angle for the IR region (large distance limit as infrared) by using the Gaussian curvature of the optical metric of this back hole. Our investigations clarify how th"},"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":"1702.04636","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"physics.gen-ph","submitted_at":"2017-02-14T01:41:06Z","cross_cats_sorted":[],"title_canon_sha256":"8d728f128e4b1d0d907e6b95edf25a081beacd7f3886652b63c67dc6e3672a4e","abstract_canon_sha256":"76390d21af3a2346cf418d2bdf22b32590eba8e6301656a6105e38bc4054e673"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:36:09.183030Z","signature_b64":"KbXnVeEgUOJAJCmtXPLvS0GVew3OwP0SQFZrea/RK4wrB7CS6rtsS5yC3tnLmh6tUdEn0o/IxwOoKYU4zzD5CQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"6f46f7961d0b733695f429621c3e47c74c31eb35b7ba44df700997b0cde823fe","last_reissued_at":"2026-05-18T00:36:09.182439Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:36:09.182439Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Hawking Radiation and Deflection of Light from Rindler Modified Schwarzschild Black Hole","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"physics.gen-ph","authors_text":"A. Ovgun, I. Sakalli","submitted_at":"2017-02-14T01:41:06Z","abstract_excerpt":"We investigate the Hawking radiation of massive spin-1 vector particles, which are coupled to vacuum fluctuations of a quantum field, from Rindler modified Schwarzschild black hole. Rindler acceleration is used to produce the post-general relativistic theory of gravity for the distant field of a point mass. The gravitational lensing problem of the Rindler modified Schwarzschild black hole is also studied. We compute the deflection angle for the IR region (large distance limit as infrared) by using the Gaussian curvature of the optical metric of this back hole. Our investigations clarify how th"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1702.04636","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":""},"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":"1702.04636","created_at":"2026-05-18T00:36:09.182545+00:00"},{"alias_kind":"arxiv_version","alias_value":"1702.04636v2","created_at":"2026-05-18T00:36:09.182545+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1702.04636","created_at":"2026-05-18T00:36:09.182545+00:00"},{"alias_kind":"pith_short_12","alias_value":"N5DPPFQ5BNZT","created_at":"2026-05-18T12:31:31.346846+00:00"},{"alias_kind":"pith_short_16","alias_value":"N5DPPFQ5BNZTNFPU","created_at":"2026-05-18T12:31:31.346846+00:00"},{"alias_kind":"pith_short_8","alias_value":"N5DPPFQ5","created_at":"2026-05-18T12:31:31.346846+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2205.07787","citing_title":"Horizon-scale tests of gravity theories and fundamental physics from the Event Horizon Telescope image of Sagittarius A$^*$","ref_index":255,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/N5DPPFQ5BNZTNFPUFFRBYPSHY5","json":"https://pith.science/pith/N5DPPFQ5BNZTNFPUFFRBYPSHY5.json","graph_json":"https://pith.science/api/pith-number/N5DPPFQ5BNZTNFPUFFRBYPSHY5/graph.json","events_json":"https://pith.science/api/pith-number/N5DPPFQ5BNZTNFPUFFRBYPSHY5/events.json","paper":"https://pith.science/paper/N5DPPFQ5"},"agent_actions":{"view_html":"https://pith.science/pith/N5DPPFQ5BNZTNFPUFFRBYPSHY5","download_json":"https://pith.science/pith/N5DPPFQ5BNZTNFPUFFRBYPSHY5.json","view_paper":"https://pith.science/paper/N5DPPFQ5","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1702.04636&json=true","fetch_graph":"https://pith.science/api/pith-number/N5DPPFQ5BNZTNFPUFFRBYPSHY5/graph.json","fetch_events":"https://pith.science/api/pith-number/N5DPPFQ5BNZTNFPUFFRBYPSHY5/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/N5DPPFQ5BNZTNFPUFFRBYPSHY5/action/timestamp_anchor","attest_storage":"https://pith.science/pith/N5DPPFQ5BNZTNFPUFFRBYPSHY5/action/storage_attestation","attest_author":"https://pith.science/pith/N5DPPFQ5BNZTNFPUFFRBYPSHY5/action/author_attestation","sign_citation":"https://pith.science/pith/N5DPPFQ5BNZTNFPUFFRBYPSHY5/action/citation_signature","submit_replication":"https://pith.science/pith/N5DPPFQ5BNZTNFPUFFRBYPSHY5/action/replication_record"}},"created_at":"2026-05-18T00:36:09.182545+00:00","updated_at":"2026-05-18T00:36:09.182545+00:00"}