{"as_of":"2026-08-16T12:31:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:8318dd8bf2eb23c26a4580353d7d6ef639519336b1f2399869f0fbab83ef62d0","coverage":[{"denominator":108,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":100,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-15T22:51:47.316903Z","state":"measured"},{"denominator":100,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":100,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-16T06:30:59.297886+00:00","state":"measured"},{"denominator":0,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":0,"source":"paper_references, paper_reference_links","source_observed_at":null,"state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"cited_works","source_observed_at":null,"state":"measured"}],"external_citation_measurements":[],"inbound":[],"links":{"evidence":"/evidence","html":"/paper/2505.06382/citation-record","integrity":"/paper/2505.06382/integrity","json":"/paper/2505.06382/citation-record.json","paper":"/paper/2505.06382"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T22:51:46.803732Z","title":"(42) The photon sphere radius and shadow radius squared for this model thus become rph = 3M− 35G2 Fα 324π3M 4, (43) R2 sh = 27M 2− 5G2 Fα 6π3M 3","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2505.06382","last_updated":"2025-05-28T06:37:40Z","snapshot_observed_at":"2026-08-16T09:42:46.840892Z","submitted_at":"2025-05-09T19:03:38Z","title":"Probing Weak-Force Corrections to Black Hole Geometry via Long Range Potentials: Feinberg-Sucher and Ferrer-Nowakowski Potentials","version":2},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-15T22:51:46.803732Z"},"links":{"citing_paper":"/paper/2505.06382"},"observation_digest":"sha256:75b5b61bdda75e8f8bb59b27371b759dc4899a6dd07852482f70503b2f0df9bf","observation_id":"976e90a5-c521-41c1-9dde-dfc414977b5b","resolution":{"observed_at":"2026-08-15T22:51:46.803732Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T22:51:46.808078Z","title":"(46) The corresponding photon sphere radius and shadow radius squared yield rph = 3M + 5β 16π3M 2, (47) R2 sh = 27M 2 + 27β 8π3M","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2505.06382","last_updated":"2025-05-28T06:37:40Z","snapshot_observed_at":"2026-08-16T09:42:46.840892Z","submitted_at":"2025-05-09T19:03:38Z","title":"Probing Weak-Force Corrections to Black Hole Geometry via Long Range Potentials: Feinberg-Sucher and Ferrer-Nowakowski Potentials","version":2},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-15T22:51:46.808078Z"},"links":{"citing_paper":"/paper/2505.06382"},"observation_digest":"sha256:5dc1cd51573a0ac76e24f58e35bcfbbc97c354b69ad27f1e922161ffcf3a4ee3","observation_id":"bb20e8f7-fe98-4835-9336-bd9982622a0e","resolution":{"observed_at":"2026-08-15T22:51:46.808078Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2205.07787","last_updated":"2023-05-26T11:55:37Z","snapshot_observed_at":"2026-08-12T14:53:38.917068Z","submitted_at":"2022-05-16T16:22:56Z","title":"Horizon-scale tests of gravity theories and fundamental physics from the Event Horizon Telescope image of Sagittarius A$^*$","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2205.07787","snapshot_observed_at":"2026-08-15T22:51:46.840177Z","title":"Vagnozzi et al., Class","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2505.06382","last_updated":"2025-05-28T06:37:40Z","snapshot_observed_at":"2026-08-16T09:42:46.840892Z","submitted_at":"2025-05-09T19:03:38Z","title":"Probing Weak-Force Corrections to Black Hole Geometry via Long Range Potentials: Feinberg-Sucher and Ferrer-Nowakowski Potentials","version":2},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-15T22:51:46.840177Z"},"links":{"cited_paper":"/paper/2205.07787","citing_paper":"/paper/2505.06382"},"observation_digest":"sha256:14d6b84251bb9bc6e7db8f96060f124a39c01c59137368cd3c829350282bf5ed","observation_id":"521cfc7d-53bc-418f-8652-90e2ba0b7a5f","resolution":{"observed_at":"2026-08-15T22:51:46.840177Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T22:51:46.815842Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2505.06382","last_updated":"2025-05-28T06:37:40Z","snapshot_observed_at":"2026-08-16T09:42:46.840892Z","submitted_at":"2025-05-09T19:03:38Z","title":"Probing Weak-Force Corrections to Black Hole Geometry via Long Range Potentials: Feinberg-Sucher and Ferrer-Nowakowski Potentials","version":2},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-15T22:51:46.815842Z"},"links":{"citing_paper":"/paper/2505.06382"},"observation_digest":"sha256:b6186564a6249493d35b03fefadb927e2a802851153a82597d504dc6d27b7628","observation_id":"357e9a11-44c7-48d7-aaa5-61f43fbc6700","resolution":{"observed_at":"2026-08-15T22:51:46.815842Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T22:51:46.821060Z","title":"R2 s = r2 p A(rp)","venue":null,"work_id":null,"year":1946},"citing_paper":{"arxiv_id":"2505.06382","last_updated":"2025-05-28T06:37:40Z","snapshot_observed_at":"2026-08-16T09:42:46.840892Z","submitted_at":"2025-05-09T19:03:38Z","title":"Probing Weak-Force Corrections to Black Hole Geometry via Long Range Potentials: Feinberg-Sucher and Ferrer-Nowakowski Potentials","version":2},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-15T22:51:46.821060Z"},"links":{"citing_paper":"/paper/2505.06382"},"observation_digest":"sha256:3370186186b70202a3831adf9f877362d68edff5bb53b7808767b93fd970265d","observation_id":"15eddb21-f5be-4d8f-a4c8-27b8791ebcbe","resolution":{"observed_at":"2026-08-15T22:51:46.821060Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1906.11238","last_updated":"2019-06-26T18:06:46Z","snapshot_observed_at":"2026-08-13T13:53:05.353909Z","submitted_at":"2019-06-26T18:06:46Z","title":"First M87 Event Horizon Telescope Results. I. The Shadow of the Supermassive Black Hole","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1906.11238","snapshot_observed_at":"2026-08-15T22:51:46.827065Z","title":"Akiyama et al","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2505.06382","last_updated":"2025-05-28T06:37:40Z","snapshot_observed_at":"2026-08-16T09:42:46.840892Z","submitted_at":"2025-05-09T19:03:38Z","title":"Probing Weak-Force Corrections to Black Hole Geometry via Long Range Potentials: Feinberg-Sucher and Ferrer-Nowakowski Potentials","version":2},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-15T22:51:46.827065Z"},"links":{"cited_paper":"/paper/1906.11238","citing_paper":"/paper/2505.06382"},"observation_digest":"sha256:ff5121bef42c7fe85794f287535c46a3bc55a301b6b7d6ccb0f80a0f888e20b7","observation_id":"d4deceab-88f7-41be-82ef-156a8a50a13f","resolution":{"observed_at":"2026-08-15T22:51:46.827065Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2311.09484","last_updated":"2023-11-16T01:08:55Z","snapshot_observed_at":"2026-08-13T05:24:17.499350Z","submitted_at":"2023-11-16T01:08:55Z","title":"First Sagittarius A* Event Horizon Telescope Results. VI: Testing the Black Hole Metric","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2311.09484","snapshot_observed_at":"2026-08-15T22:51:46.833625Z","title":"Akiyama et al","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2505.06382","last_updated":"2025-05-28T06:37:40Z","snapshot_observed_at":"2026-08-16T09:42:46.840892Z","submitted_at":"2025-05-09T19:03:38Z","title":"Probing Weak-Force Corrections to Black Hole Geometry via Long Range Potentials: Feinberg-Sucher and Ferrer-Nowakowski Potentials","version":2},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-15T22:51:46.833625Z"},"links":{"cited_paper":"/paper/2311.09484","citing_paper":"/paper/2505.06382"},"observation_digest":"sha256:58e0b1aac52dfc6d33121277393880bcc5eccde3601774afd34cfe74397aa555","observation_id":"f42baaaf-b7c0-4726-bf03-31ccac3116ad","resolution":{"observed_at":"2026-08-15T22:51:46.833625Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1904.12983","last_updated":"2019-08-15T12:36:19Z","snapshot_observed_at":"2026-08-14T16:39:42.819066Z","submitted_at":"2019-04-29T23:04:12Z","title":"Testing the rotational nature of the supermassive object M87* from the circularity and size of its first image","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1904.12983","snapshot_observed_at":"2026-08-15T22:51:46.866646Z","title":"Bambi, K","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2505.06382","last_updated":"2025-05-28T06:37:40Z","snapshot_observed_at":"2026-08-16T09:42:46.840892Z","submitted_at":"2025-05-09T19:03:38Z","title":"Probing Weak-Force Corrections to Black Hole Geometry via Long Range Potentials: Feinberg-Sucher and Ferrer-Nowakowski Potentials","version":2},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-15T22:51:46.866646Z"},"links":{"cited_paper":"/paper/1904.12983","citing_paper":"/paper/2505.06382"},"observation_digest":"sha256:c43e6b8f5179e76ffe01e957702798c17b22c6bb7686a4765004c8c63e4eae11","observation_id":"2fd97e7d-fdb1-45a3-8703-4e5bc36f6f02","resolution":{"observed_at":"2026-08-15T22:51:46.866646Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9912263","last_updated":"1999-12-14T09:29:57Z","snapshot_observed_at":"2026-07-07T01:30:29.466209Z","submitted_at":"1999-12-14T09:29:57Z","title":"Viewing the Shadow of the Black Hole at the Galactic Center","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9912263","snapshot_observed_at":"2026-08-15T22:51:46.846089Z","title":"Falcke, F","venue":null,"work_id":null,"year":2000},"citing_paper":{"arxiv_id":"2505.06382","last_updated":"2025-05-28T06:37:40Z","snapshot_observed_at":"2026-08-16T09:42:46.840892Z","submitted_at":"2025-05-09T19:03:38Z","title":"Probing Weak-Force Corrections to Black Hole Geometry via Long Range Potentials: Feinberg-Sucher and Ferrer-Nowakowski Potentials","version":2},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-15T22:51:46.846089Z"},"links":{"cited_paper":"/paper/astro-ph/9912263","citing_paper":"/paper/2505.06382"},"observation_digest":"sha256:204434bcf77b6addbfebcebbacde47e0dbd9518e34dc57187675a0b846c71dee","observation_id":"025f4c09-a507-4de6-9cca-fe8bcf9bf1cd","resolution":{"observed_at":"2026-08-15T22:51:46.846089Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2205.06238","last_updated":"2022-08-24T15:36:10Z","snapshot_observed_at":"2026-08-13T15:44:59.332141Z","submitted_at":"2022-05-12T17:36:42Z","title":"Superradiant evolution of the shadow and photon ring of Sgr A$^\\star$","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2205.06238","snapshot_observed_at":"2026-08-15T22:51:46.851212Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2505.06382","last_updated":"2025-05-28T06:37:40Z","snapshot_observed_at":"2026-08-16T09:42:46.840892Z","submitted_at":"2025-05-09T19:03:38Z","title":"Probing Weak-Force Corrections to Black Hole Geometry via Long Range Potentials: Feinberg-Sucher and Ferrer-Nowakowski Potentials","version":2},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-15T22:51:46.851212Z"},"links":{"cited_paper":"/paper/2205.06238","citing_paper":"/paper/2505.06382"},"observation_digest":"sha256:e030c643abef45c140aa11dc7c56b6f66c77117f7b9af7c78349db74c200fcc9","observation_id":"c7547649-73e6-4ecc-8710-ad17d9d2e7a8","resolution":{"observed_at":"2026-08-15T22:51:46.851212Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1801.09920","last_updated":"2018-02-11T15:07:49Z","snapshot_observed_at":"2026-08-14T19:50:46.053053Z","submitted_at":"2018-01-30T10:10:01Z","title":"The black hole at the Galactic Center: observations and models","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1801.09920","snapshot_observed_at":"2026-08-15T22:51:46.857329Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2505.06382","last_updated":"2025-05-28T06:37:40Z","snapshot_observed_at":"2026-08-16T09:42:46.840892Z","submitted_at":"2025-05-09T19:03:38Z","title":"Probing Weak-Force Corrections to Black Hole Geometry via Long Range Potentials: Feinberg-Sucher and Ferrer-Nowakowski Potentials","version":2},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-15T22:51:46.857329Z"},"links":{"cited_paper":"/paper/1801.09920","citing_paper":"/paper/2505.06382"},"observation_digest":"sha256:8d3241a5aefc3d2754f3c703b63e6485d58f26b82b879a4b4badffc19790d36a","observation_id":"3b3da6a8-1cf0-4d2b-b927-5150a83a7263","resolution":{"observed_at":"2026-08-15T22:51:46.857329Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1407.7457","last_updated":"2014-07-24T15:11:34Z","snapshot_observed_at":"2026-08-14T23:25:31.063319Z","submitted_at":"2014-07-24T15:11:34Z","title":"Constraints on a charge in the Reissner--Nordstr\\\"om metric for the black hole at the Galactic Center","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1407.7457","snapshot_observed_at":"2026-08-15T22:51:46.862405Z","title":null,"venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2505.06382","last_updated":"2025-05-28T06:37:40Z","snapshot_observed_at":"2026-08-16T09:42:46.840892Z","submitted_at":"2025-05-09T19:03:38Z","title":"Probing Weak-Force Corrections to Black Hole Geometry via Long Range Potentials: Feinberg-Sucher and Ferrer-Nowakowski Potentials","version":2},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-15T22:51:46.862405Z"},"links":{"cited_paper":"/paper/1407.7457","citing_paper":"/paper/2505.06382"},"observation_digest":"sha256:0ff75e37e46c9dde0883e6b419b2d0ba4cc88759f53a81f9c261f21cb73cc522","observation_id":"8354c2c7-3f79-4913-b93d-ba615a414e3d","resolution":{"observed_at":"2026-08-15T22:51:46.862405Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1801.00860","last_updated":"2019-02-11T12:21:47Z","snapshot_observed_at":"2026-08-14T19:58:26.924480Z","submitted_at":"2018-01-02T23:22:42Z","title":"Shadows and strong gravitational lensing: a brief review","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1801.00860","snapshot_observed_at":"2026-08-15T22:51:46.889595Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2505.06382","last_updated":"2025-05-28T06:37:40Z","snapshot_observed_at":"2026-08-16T09:42:46.840892Z","submitted_at":"2025-05-09T19:03:38Z","title":"Probing Weak-Force Corrections to Black Hole Geometry via Long Range Potentials: Feinberg-Sucher and Ferrer-Nowakowski Potentials","version":2},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-15T22:51:46.889595Z"},"links":{"cited_paper":"/paper/1801.00860","citing_paper":"/paper/2505.06382"},"observation_digest":"sha256:f9c75449ff55fedd4e76d447a4d885a7e90222766bc94c83ec175126d9a6361d","observation_id":"f89ebe00-1091-4c8b-b897-d9f2faa46a69","resolution":{"observed_at":"2026-08-15T22:51:46.889595Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1906.00873","last_updated":"2019-06-17T16:03:08Z","snapshot_observed_at":"2026-08-14T16:21:49.374613Z","submitted_at":"2019-06-03T15:29:09Z","title":"Black Hole Shadows, Photon Rings, and Lensing Rings","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1906.00873","snapshot_observed_at":"2026-08-15T22:51:46.870874Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2505.06382","last_updated":"2025-05-28T06:37:40Z","snapshot_observed_at":"2026-08-16T09:42:46.840892Z","submitted_at":"2025-05-09T19:03:38Z","title":"Probing Weak-Force Corrections to Black Hole Geometry via Long Range Potentials: Feinberg-Sucher and Ferrer-Nowakowski Potentials","version":2},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-15T22:51:46.870874Z"},"links":{"cited_paper":"/paper/1906.00873","citing_paper":"/paper/2505.06382"},"observation_digest":"sha256:09d985f08885966f8e13fa8a60cef7f0605696044caced3e359fa22bc5a106a6","observation_id":"c62433c8-8932-49db-9a70-42e6f6366560","resolution":{"observed_at":"2026-08-15T22:51:46.870874Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1005.1931","last_updated":"2010-06-01T20:11:42Z","snapshot_observed_at":"2026-08-15T05:19:20.350915Z","submitted_at":"2010-05-11T20:01:20Z","title":"Testing the No-Hair Theorem with Observations in the Electromagnetic Spectrum: II. Black-Hole Images","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1005.1931","snapshot_observed_at":"2026-08-15T22:51:46.875777Z","title":"Johannsen and D","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2505.06382","last_updated":"2025-05-28T06:37:40Z","snapshot_observed_at":"2026-08-16T09:42:46.840892Z","submitted_at":"2025-05-09T19:03:38Z","title":"Probing Weak-Force Corrections to Black Hole Geometry via Long Range Potentials: Feinberg-Sucher and Ferrer-Nowakowski Potentials","version":2},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-15T22:51:46.875777Z"},"links":{"cited_paper":"/paper/1005.1931","citing_paper":"/paper/2505.06382"},"observation_digest":"sha256:d21f3f224ecfb0bf11767eb61c66ad294bcc354c8a0feb1584b30341986d7000","observation_id":"2a835609-9351-40a6-b382-d9c62a609c56","resolution":{"observed_at":"2026-08-15T22:51:46.875777Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1607.03133","last_updated":"2016-07-11T20:11:37Z","snapshot_observed_at":"2026-08-14T21:48:52.257173Z","submitted_at":"2016-07-11T20:11:37Z","title":"Testing the black hole \"no-hair\" hypothesis","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1607.03133","snapshot_observed_at":"2026-08-15T22:51:46.880077Z","title":"Cardoso and L","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2505.06382","last_updated":"2025-05-28T06:37:40Z","snapshot_observed_at":"2026-08-16T09:42:46.840892Z","submitted_at":"2025-05-09T19:03:38Z","title":"Probing Weak-Force Corrections to Black Hole Geometry via Long Range Potentials: Feinberg-Sucher and Ferrer-Nowakowski Potentials","version":2},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-15T22:51:46.880077Z"},"links":{"cited_paper":"/paper/1607.03133","citing_paper":"/paper/2505.06382"},"observation_digest":"sha256:98636de8c80bfe97630d94d21b78f3086dbb6e6671a70bb90f0204caba2ef8b3","observation_id":"08a7b3a0-c3b1-4b5e-b162-3e5b41f83987","resolution":{"observed_at":"2026-08-15T22:51:46.880077Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2206.05878","last_updated":"2022-09-17T12:59:04Z","snapshot_observed_at":"2026-08-13T15:25:12.242164Z","submitted_at":"2022-06-13T02:12:23Z","title":"Constraining a modified gravity theory in strong gravitational lensing and black hole shadow observations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2206.05878","snapshot_observed_at":"2026-08-15T22:51:46.885250Z","title":"Kuang, Z.-Y","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2505.06382","last_updated":"2025-05-28T06:37:40Z","snapshot_observed_at":"2026-08-16T09:42:46.840892Z","submitted_at":"2025-05-09T19:03:38Z","title":"Probing Weak-Force Corrections to Black Hole Geometry via Long Range Potentials: Feinberg-Sucher and Ferrer-Nowakowski Potentials","version":2},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-15T22:51:46.885250Z"},"links":{"cited_paper":"/paper/2206.05878","citing_paper":"/paper/2505.06382"},"observation_digest":"sha256:c095eff86e32b4fda4e89f9dd99d58eeaf3b81455af40ba15ac41dfff8f85e3d","observation_id":"f4db8ca9-b6c7-4c35-a38b-ac303ffce32a","resolution":{"observed_at":"2026-08-15T22:51:46.885250Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1705.05461","last_updated":"2017-05-15T21:47:26Z","snapshot_observed_at":"2026-08-14T21:00:32.435818Z","submitted_at":"2017-05-15T21:47:26Z","title":"Fundamental photon orbits: black hole shadows and spacetime instabilities","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1705.05461","snapshot_observed_at":"2026-08-15T22:51:46.913016Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2505.06382","last_updated":"2025-05-28T06:37:40Z","snapshot_observed_at":"2026-08-16T09:42:46.840892Z","submitted_at":"2025-05-09T19:03:38Z","title":"Probing Weak-Force Corrections to Black Hole Geometry via Long Range Potentials: Feinberg-Sucher and Ferrer-Nowakowski Potentials","version":2},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-15T22:51:46.913016Z"},"links":{"cited_paper":"/paper/1705.05461","citing_paper":"/paper/2505.06382"},"observation_digest":"sha256:6fff26a57cfc0ee5cc78a334458f32685ce9086e4b1eda25ded883e8f2ff30d8","observation_id":"5edbd2f4-bbb5-4b9b-85e8-2fd764474a0c","resolution":{"observed_at":"2026-08-15T22:51:46.913016Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1701.00079","last_updated":"2017-03-15T22:45:11Z","snapshot_observed_at":"2026-08-14T21:23:02.592881Z","submitted_at":"2016-12-31T09:26:51Z","title":"Shadows of Einstein-dilaton-Gauss-Bonnet black holes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1701.00079","snapshot_observed_at":"2026-08-15T22:51:46.894379Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2505.06382","last_updated":"2025-05-28T06:37:40Z","snapshot_observed_at":"2026-08-16T09:42:46.840892Z","submitted_at":"2025-05-09T19:03:38Z","title":"Probing Weak-Force Corrections to Black Hole Geometry via Long Range Potentials: Feinberg-Sucher and Ferrer-Nowakowski Potentials","version":2},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-15T22:51:46.894379Z"},"links":{"cited_paper":"/paper/1701.00079","citing_paper":"/paper/2505.06382"},"observation_digest":"sha256:7594a552f8bd2a95b4724876a4b3e09a3c2555a3ca153960daa505195e2f2c23","observation_id":"dca80292-2295-427b-a01d-106416d2aae7","resolution":{"observed_at":"2026-08-15T22:51:46.894379Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2105.07101","last_updated":"2022-01-25T21:06:30Z","snapshot_observed_at":"2026-08-13T19:22:38.874754Z","submitted_at":"2021-05-15T00:00:17Z","title":"Calculating black hole shadows: Review of analytical studies","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2105.07101","snapshot_observed_at":"2026-08-15T22:51:46.898848Z","title":"Perlick and O","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2505.06382","last_updated":"2025-05-28T06:37:40Z","snapshot_observed_at":"2026-08-16T09:42:46.840892Z","submitted_at":"2025-05-09T19:03:38Z","title":"Probing Weak-Force Corrections to Black Hole Geometry via Long Range Potentials: Feinberg-Sucher and Ferrer-Nowakowski Potentials","version":2},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-15T22:51:46.898848Z"},"links":{"cited_paper":"/paper/2105.07101","citing_paper":"/paper/2505.06382"},"observation_digest":"sha256:9eb519560c4e7b0438a6745877aec510ae0387f478f0bde0136fca9a6c196f5a","observation_id":"dbe64801-14e0-42d4-8eeb-112dcdd2f733","resolution":{"observed_at":"2026-08-15T22:51:46.898848Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1811.00047","last_updated":"2019-02-11T19:57:00Z","snapshot_observed_at":"2026-08-14T18:06:08.760303Z","submitted_at":"2018-10-31T18:19:59Z","title":"Intrinsic curvature and topology of shadows in Kerr spacetime","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1811.00047","snapshot_observed_at":"2026-08-15T22:51:46.904328Z","title":"Wei, Y.-X","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2505.06382","last_updated":"2025-05-28T06:37:40Z","snapshot_observed_at":"2026-08-16T09:42:46.840892Z","submitted_at":"2025-05-09T19:03:38Z","title":"Probing Weak-Force Corrections to Black Hole Geometry via Long Range Potentials: Feinberg-Sucher and Ferrer-Nowakowski Potentials","version":2},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-15T22:51:46.904328Z"},"links":{"cited_paper":"/paper/1811.00047","citing_paper":"/paper/2505.06382"},"observation_digest":"sha256:cbecff7af07a6c66cf0ccd5d36a2e68a4200c8a9f88953b95803369c76ffe620","observation_id":"7bcb512a-9e5c-4e0f-a271-7c3babb71de5","resolution":{"observed_at":"2026-08-15T22:51:46.904328Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2003.01188","last_updated":"2020-11-13T06:46:13Z","snapshot_observed_at":"2026-08-16T05:03:16.774289Z","submitted_at":"2020-03-02T21:01:48Z","title":"Quasinormal modes, stability and shadows of a black hole in the 4D Einstein-Gauss-Bonnet gravity","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2003.01188","snapshot_observed_at":"2026-08-15T22:51:46.908855Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2505.06382","last_updated":"2025-05-28T06:37:40Z","snapshot_observed_at":"2026-08-16T09:42:46.840892Z","submitted_at":"2025-05-09T19:03:38Z","title":"Probing Weak-Force Corrections to Black Hole Geometry via Long Range Potentials: Feinberg-Sucher and Ferrer-Nowakowski Potentials","version":2},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-15T22:51:46.908855Z"},"links":{"cited_paper":"/paper/2003.01188","citing_paper":"/paper/2505.06382"},"observation_digest":"sha256:1b0aee886fef35155410f4fabad8406cf27c0b923ebdb03a73c0cf8471d0850f","observation_id":"00a47a2f-d0c6-4500-a3d1-65868daa899e","resolution":{"observed_at":"2026-08-15T22:51:46.908855Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1802.08060","last_updated":"2018-10-30T11:30:40Z","snapshot_observed_at":"2026-08-14T19:43:18.502723Z","submitted_at":"2018-02-22T14:33:43Z","title":"Shadows of spherically symmetric black holes and naked singularities","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1802.08060","snapshot_observed_at":"2026-08-15T22:51:46.935142Z","title":"Shaikh, P","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2505.06382","last_updated":"2025-05-28T06:37:40Z","snapshot_observed_at":"2026-08-16T09:42:46.840892Z","submitted_at":"2025-05-09T19:03:38Z","title":"Probing Weak-Force Corrections to Black Hole Geometry via Long Range Potentials: Feinberg-Sucher and Ferrer-Nowakowski Potentials","version":2},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-15T22:51:46.935142Z"},"links":{"cited_paper":"/paper/1802.08060","citing_paper":"/paper/2505.06382"},"observation_digest":"sha256:a44e7e2d060c15cb5877e9a99536a0638558f8ce16480f94d6998564cdb0f064","observation_id":"7fcd75a6-d875-42af-b09f-f21102986bd5","resolution":{"observed_at":"2026-08-15T22:51:46.935142Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2108.07766","last_updated":"2022-01-04T20:57:09Z","snapshot_observed_at":"2026-08-13T18:27:27.874952Z","submitted_at":"2021-08-17T17:17:19Z","title":"Nonlinear electrodynamics effects on the black hole shadow, deflection angle, quasinormal modes and greybody factors","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2108.07766","snapshot_observed_at":"2026-08-15T22:51:46.917333Z","title":"Okyay and A","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2505.06382","last_updated":"2025-05-28T06:37:40Z","snapshot_observed_at":"2026-08-16T09:42:46.840892Z","submitted_at":"2025-05-09T19:03:38Z","title":"Probing Weak-Force Corrections to Black Hole Geometry via Long Range Potentials: Feinberg-Sucher and Ferrer-Nowakowski Potentials","version":2},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-15T22:51:46.917333Z"},"links":{"cited_paper":"/paper/2108.07766","citing_paper":"/paper/2505.06382"},"observation_digest":"sha256:0df77414c2cf2fbe21eb86c2148302e4087a274c68cafcebe66685ae1842fa11","observation_id":"51dab512-3633-4f17-902d-8ff59d18e22c","resolution":{"observed_at":"2026-08-15T22:51:46.917333Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2010.05755","last_updated":"2021-02-24T16:14:23Z","snapshot_observed_at":"2026-08-11T16:53:43.020517Z","submitted_at":"2020-10-08T09:48:51Z","title":"Shadow, deflection angle and quasinormal modes of Born-Infeld charged black holes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2010.05755","snapshot_observed_at":"2026-08-15T22:51:46.922118Z","title":"Jafarzade, M","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2505.06382","last_updated":"2025-05-28T06:37:40Z","snapshot_observed_at":"2026-08-16T09:42:46.840892Z","submitted_at":"2025-05-09T19:03:38Z","title":"Probing Weak-Force Corrections to Black Hole Geometry via Long Range Potentials: Feinberg-Sucher and Ferrer-Nowakowski Potentials","version":2},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-15T22:51:46.922118Z"},"links":{"cited_paper":"/paper/2010.05755","citing_paper":"/paper/2505.06382"},"observation_digest":"sha256:79a8680256348c81724098e3c8ddb94a587024f4bdbad21e01152b65028ada8c","observation_id":"afb75d8d-3074-4eb7-9a34-41482a4bdce9","resolution":{"observed_at":"2026-08-15T22:51:46.922118Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1112.6349","last_updated":"2012-03-16T15:08:01Z","snapshot_observed_at":"2026-08-15T04:24:17.075933Z","submitted_at":"2011-12-29T17:09:00Z","title":"Shadow of a rotating braneworld black hole","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1112.6349","snapshot_observed_at":"2026-08-15T22:51:46.926395Z","title":"Amarilla and E","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2505.06382","last_updated":"2025-05-28T06:37:40Z","snapshot_observed_at":"2026-08-16T09:42:46.840892Z","submitted_at":"2025-05-09T19:03:38Z","title":"Probing Weak-Force Corrections to Black Hole Geometry via Long Range Potentials: Feinberg-Sucher and Ferrer-Nowakowski Potentials","version":2},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-15T22:51:46.926395Z"},"links":{"cited_paper":"/paper/1112.6349","citing_paper":"/paper/2505.06382"},"observation_digest":"sha256:2659a4b0233dc47c9e91fde54a43e1a8d28d5a10d1b4c88d734ec2d561bacc1f","observation_id":"09d015b2-7749-46d1-8ba4-647e0a708412","resolution":{"observed_at":"2026-08-15T22:51:46.926395Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1801.03223","last_updated":"2018-04-12T08:17:50Z","snapshot_observed_at":"2026-08-14T19:56:28.485039Z","submitted_at":"2018-01-10T02:49:02Z","title":"Shadows, Signals, and Stability in Einsteinian Cubic Gravity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1801.03223","snapshot_observed_at":"2026-08-15T22:51:46.930776Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2505.06382","last_updated":"2025-05-28T06:37:40Z","snapshot_observed_at":"2026-08-16T09:42:46.840892Z","submitted_at":"2025-05-09T19:03:38Z","title":"Probing Weak-Force Corrections to Black Hole Geometry via Long Range Potentials: Feinberg-Sucher and Ferrer-Nowakowski Potentials","version":2},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-15T22:51:46.930776Z"},"links":{"cited_paper":"/paper/1801.03223","citing_paper":"/paper/2505.06382"},"observation_digest":"sha256:9cf9b1732800171585ab92bca19894b9c3f91cb8a227e11c15bfada4f62b25e7","observation_id":"89e8990d-7b95-4b56-985e-49ef97b83625","resolution":{"observed_at":"2026-08-15T22:51:46.930776Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1905.12421","last_updated":"2019-07-12T14:32:43Z","snapshot_observed_at":"2026-08-14T16:24:29.405115Z","submitted_at":"2019-05-29T13:26:48Z","title":"Hunting for extra dimensions in the shadow of M87*","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1905.12421","snapshot_observed_at":"2026-08-15T22:51:46.957245Z","title":"Vagnozzi and L","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2505.06382","last_updated":"2025-05-28T06:37:40Z","snapshot_observed_at":"2026-08-16T09:42:46.840892Z","submitted_at":"2025-05-09T19:03:38Z","title":"Probing Weak-Force Corrections to Black Hole Geometry via Long Range Potentials: Feinberg-Sucher and Ferrer-Nowakowski Potentials","version":2},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-15T22:51:46.957245Z"},"links":{"cited_paper":"/paper/1905.12421","citing_paper":"/paper/2505.06382"},"observation_digest":"sha256:0b5f8dadc8f72a98be5a5cec1032f5fd2aef7f48382cd474601930b264ce7fb7","observation_id":"b7e2b307-2783-4a4c-9bfb-d2541b0b3701","resolution":{"observed_at":"2026-08-15T22:51:46.957245Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1905.00064","last_updated":"2019-06-04T14:46:43Z","snapshot_observed_at":"2026-08-14T16:39:06.449186Z","submitted_at":"2019-04-30T19:08:54Z","title":"Shadow of a black hole surrounded by dark matter","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1905.00064","snapshot_observed_at":"2026-08-15T22:51:46.940603Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2505.06382","last_updated":"2025-05-28T06:37:40Z","snapshot_observed_at":"2026-08-16T09:42:46.840892Z","submitted_at":"2025-05-09T19:03:38Z","title":"Probing Weak-Force Corrections to Black Hole Geometry via Long Range Potentials: Feinberg-Sucher and Ferrer-Nowakowski Potentials","version":2},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-15T22:51:46.940603Z"},"links":{"cited_paper":"/paper/1905.00064","citing_paper":"/paper/2505.06382"},"observation_digest":"sha256:b4fa42458d095da64ca912574d7f0b49c2421d6056bd7b7cf3df1f443b4c8b3e","observation_id":"5da00929-c018-4894-b45a-c06d9dedb43c","resolution":{"observed_at":"2026-08-15T22:51:46.940603Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2005.05992","last_updated":"2020-08-09T12:55:45Z","snapshot_observed_at":"2026-07-06T09:19:47.840044Z","submitted_at":"2020-05-12T18:03:40Z","title":"Black holes with scalar hair in light of the Event Horizon Telescope","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2005.05992","snapshot_observed_at":"2026-08-15T22:51:46.944227Z","title":"Khodadi, A","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2505.06382","last_updated":"2025-05-28T06:37:40Z","snapshot_observed_at":"2026-08-16T09:42:46.840892Z","submitted_at":"2025-05-09T19:03:38Z","title":"Probing Weak-Force Corrections to Black Hole Geometry via Long Range Potentials: Feinberg-Sucher and Ferrer-Nowakowski Potentials","version":2},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-15T22:51:46.944227Z"},"links":{"cited_paper":"/paper/2005.05992","citing_paper":"/paper/2505.06382"},"observation_digest":"sha256:c8324583a3479f932e91b77fe5286d9df5943dbf548242082431457ba98600de","observation_id":"91205507-7f47-4d38-a7de-b1d1c398fcf6","resolution":{"observed_at":"2026-08-15T22:51:46.944227Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2103.11417","last_updated":"2021-05-31T16:40:34Z","snapshot_observed_at":"2026-08-14T23:42:34.519803Z","submitted_at":"2021-03-21T15:08:25Z","title":"Parameter estimation of hairy Kerr black holes from its shadow and constraints from M87*","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2103.11417","snapshot_observed_at":"2026-08-15T22:51:46.949561Z","title":"Afrin, R","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2505.06382","last_updated":"2025-05-28T06:37:40Z","snapshot_observed_at":"2026-08-16T09:42:46.840892Z","submitted_at":"2025-05-09T19:03:38Z","title":"Probing Weak-Force Corrections to Black Hole Geometry via Long Range Potentials: Feinberg-Sucher and Ferrer-Nowakowski Potentials","version":2},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-08-15T22:51:46.949561Z"},"links":{"cited_paper":"/paper/2103.11417","citing_paper":"/paper/2505.06382"},"observation_digest":"sha256:729402a24ddee5f965056365c403b7606a796931c2195ac38a4d7d5b0eb1a2d2","observation_id":"ee90147d-2a15-460b-9509-d877ab217098","resolution":{"observed_at":"2026-08-15T22:51:46.949561Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2004.12074","last_updated":"2020-09-26T11:06:19Z","snapshot_observed_at":"2026-08-14T07:44:01.493804Z","submitted_at":"2020-04-25T07:45:05Z","title":"Shadows and photon spheres with spherical accretions in the four-dimensional Gauss-Bonnet black hole","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2004.12074","snapshot_observed_at":"2026-08-15T22:51:46.953622Z","title":"Zeng, H.-Q","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2505.06382","last_updated":"2025-05-28T06:37:40Z","snapshot_observed_at":"2026-08-16T09:42:46.840892Z","submitted_at":"2025-05-09T19:03:38Z","title":"Probing Weak-Force Corrections to Black Hole Geometry via Long Range Potentials: Feinberg-Sucher and Ferrer-Nowakowski Potentials","version":2},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-15T22:51:46.953622Z"},"links":{"cited_paper":"/paper/2004.12074","citing_paper":"/paper/2505.06382"},"observation_digest":"sha256:47185bcf622231d8fc807aaa6e48a03c9085a71f5781a112e1474f758f9afbc8","observation_id":"b3515dd5-510d-4cbc-9d0f-6240d46612c8","resolution":{"observed_at":"2026-08-15T22:51:46.953622Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T22:51:46.978648Z","title":"Vertogradov and A.¨Ovg ¨un, (2024), arXiv:2412.10930 [gr-qc]","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2505.06382","last_updated":"2025-05-28T06:37:40Z","snapshot_observed_at":"2026-08-16T09:42:46.840892Z","submitted_at":"2025-05-09T19:03:38Z","title":"Probing Weak-Force Corrections to Black Hole Geometry via Long Range Potentials: Feinberg-Sucher and Ferrer-Nowakowski Potentials","version":2},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-15T22:51:46.978648Z"},"links":{"citing_paper":"/paper/2505.06382"},"observation_digest":"sha256:d4568686d048a9d8fc44af8aba608f9bec04d128976bc28c282b3807035e4110","observation_id":"0bc5d054-dfd6-4adf-9a2a-14654742a309","resolution":{"observed_at":"2026-08-15T22:51:46.978648Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1912.08231","last_updated":"2020-01-20T12:22:02Z","snapshot_observed_at":"2026-08-14T07:12:52.846599Z","submitted_at":"2019-12-17T19:06:18Z","title":"Magnetically charged black holes from non-linear electrodynamics and the Event Horizon Telescope","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1912.08231","snapshot_observed_at":"2026-08-15T22:51:46.961624Z","title":"Allahyari, M","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2505.06382","last_updated":"2025-05-28T06:37:40Z","snapshot_observed_at":"2026-08-16T09:42:46.840892Z","submitted_at":"2025-05-09T19:03:38Z","title":"Probing Weak-Force Corrections to Black Hole Geometry via Long Range Potentials: Feinberg-Sucher and Ferrer-Nowakowski Potentials","version":2},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-15T22:51:46.961624Z"},"links":{"cited_paper":"/paper/1912.08231","citing_paper":"/paper/2505.06382"},"observation_digest":"sha256:7dd978ed0f386587a1b8841851821dc5e119ebef61016738d54df3d544e2a125","observation_id":"ca433eea-abe1-4564-a961-3e22ad25ba5f","resolution":{"observed_at":"2026-08-15T22:51:46.961624Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1311.4251","last_updated":"2013-12-02T06:18:16Z","snapshot_observed_at":"2026-08-14T23:54:59.003143Z","submitted_at":"2013-11-18T03:11:21Z","title":"Observing the shadow of Einstein-Maxwell-Dilaton-Axion black hole","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1311.4251","snapshot_observed_at":"2026-08-15T22:51:46.965251Z","title":"Wei and Y.-X","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2505.06382","last_updated":"2025-05-28T06:37:40Z","snapshot_observed_at":"2026-08-16T09:42:46.840892Z","submitted_at":"2025-05-09T19:03:38Z","title":"Probing Weak-Force Corrections to Black Hole Geometry via Long Range Potentials: Feinberg-Sucher and Ferrer-Nowakowski Potentials","version":2},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-15T22:51:46.965251Z"},"links":{"cited_paper":"/paper/1311.4251","citing_paper":"/paper/2505.06382"},"observation_digest":"sha256:cb291a9478c415b987b3ab7f366593decea367c1593a11fc445676b6539c6de1","observation_id":"c7dbc683-c504-468d-b4c5-e9dde19eba5e","resolution":{"observed_at":"2026-08-15T22:51:46.965251Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2008.13478","last_updated":"2020-08-31T10:43:11Z","snapshot_observed_at":"2026-08-16T09:43:06.606455Z","submitted_at":"2020-08-31T10:43:11Z","title":"Shadows of 5D Black Holes from String Theory","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2008.13478","snapshot_observed_at":"2026-08-15T22:51:46.969369Z","title":"Belhaj, H","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2505.06382","last_updated":"2025-05-28T06:37:40Z","snapshot_observed_at":"2026-08-16T09:42:46.840892Z","submitted_at":"2025-05-09T19:03:38Z","title":"Probing Weak-Force Corrections to Black Hole Geometry via Long Range Potentials: Feinberg-Sucher and Ferrer-Nowakowski Potentials","version":2},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-15T22:51:46.969369Z"},"links":{"cited_paper":"/paper/2008.13478","citing_paper":"/paper/2505.06382"},"observation_digest":"sha256:849c871b33db385286890912457f10c945e05281611205b3fa49d90367845536","observation_id":"0af8315b-049a-44c6-ae63-c5a0bf4ea688","resolution":{"observed_at":"2026-08-15T22:51:46.969369Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2502.00521","last_updated":"2025-06-18T05:58:38Z","snapshot_observed_at":"2026-08-12T13:32:12.008207Z","submitted_at":"2025-02-01T18:49:33Z","title":"Formation of regular black hole from baryonic matter","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2502.00521","snapshot_observed_at":"2026-08-15T22:51:46.973513Z","title":"Vertogradov, A","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2505.06382","last_updated":"2025-05-28T06:37:40Z","snapshot_observed_at":"2026-08-16T09:42:46.840892Z","submitted_at":"2025-05-09T19:03:38Z","title":"Probing Weak-Force Corrections to Black Hole Geometry via Long Range Potentials: Feinberg-Sucher and Ferrer-Nowakowski Potentials","version":2},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-15T22:51:46.973513Z"},"links":{"cited_paper":"/paper/2502.00521","citing_paper":"/paper/2505.06382"},"observation_digest":"sha256:8e1dcfc57415d6cffa0e877e346442db7b1fe3a2a943eb23a1878b4c08f7e6f3","observation_id":"74119965-1bfc-4a8b-8141-4fcd0e593eb2","resolution":{"observed_at":"2026-08-15T22:51:46.973513Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2403.16743","last_updated":"2024-05-12T12:56:09Z","snapshot_observed_at":"2026-08-13T00:45:42.154822Z","submitted_at":"2024-03-25T13:15:00Z","title":"Influence of primary hair and plasma on intensity distribution of black hole shadows","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2403.16743","snapshot_observed_at":"2026-08-15T22:51:47.001337Z","title":"Vertogradov, M","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2505.06382","last_updated":"2025-05-28T06:37:40Z","snapshot_observed_at":"2026-08-16T09:42:46.840892Z","submitted_at":"2025-05-09T19:03:38Z","title":"Probing Weak-Force Corrections to Black Hole Geometry via Long Range Potentials: Feinberg-Sucher and Ferrer-Nowakowski Potentials","version":2},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-15T22:51:47.001337Z"},"links":{"cited_paper":"/paper/2403.16743","citing_paper":"/paper/2505.06382"},"observation_digest":"sha256:0c8d624e8fc5d10a7554f905cdd53360a59fbf31250223f00b53fac6c4e78b6a","observation_id":"f7fc4dfd-877f-4c7f-82eb-c40ac132fbd6","resolution":{"observed_at":"2026-08-15T22:51:47.001337Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2408.02699","last_updated":"2024-12-06T16:18:49Z","snapshot_observed_at":"2026-08-12T23:08:53.100100Z","submitted_at":"2024-08-04T15:28:02Z","title":"Exact Regular Black Hole Solutions with de Sitter Cores and Hagedorn Fluid","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2408.02699","snapshot_observed_at":"2026-08-15T22:51:46.984326Z","title":"Vertogradov and A","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2505.06382","last_updated":"2025-05-28T06:37:40Z","snapshot_observed_at":"2026-08-16T09:42:46.840892Z","submitted_at":"2025-05-09T19:03:38Z","title":"Probing Weak-Force Corrections to Black Hole Geometry via Long Range Potentials: Feinberg-Sucher and Ferrer-Nowakowski Potentials","version":2},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-08-15T22:51:46.984326Z"},"links":{"cited_paper":"/paper/2408.02699","citing_paper":"/paper/2505.06382"},"observation_digest":"sha256:0766219e2cb2502802b44a2fc7ffe02384265c31291da60156999983610cc88b","observation_id":"ee94f8dd-8e84-41e4-bbd0-bbf77db276a0","resolution":{"observed_at":"2026-08-15T22:51:46.984326Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2405.05077","last_updated":"2024-05-08T14:21:46Z","snapshot_observed_at":"2026-08-13T00:12:19.341684Z","submitted_at":"2024-05-08T14:21:46Z","title":"Analyzing the Influence of Geometrical Deformation on Photon Sphere and Shadow Radius: A New Analytical Approach -Stationary, and Axisymmetric Spacetime","version":1},"cited_work":{"arxiv_id":"2405.05077","doi":null,"metadata_source":"pith","pith_arxiv_id":"2405.05077","snapshot_observed_at":"2026-08-15T22:51:48.615952Z","title":"Analyzing the Influence of Geometrical Deformation on Photon Sphere and Shadow Radius: A New Analytical Approach -Stationary, and Axisymmetric Spacetime","venue":"gr-qc","work_id":"949f7da9-d7a7-464c-849f-6216a864b1b7","year":2024},"citing_paper":{"arxiv_id":"2505.06382","last_updated":"2025-05-28T06:37:40Z","snapshot_observed_at":"2026-08-16T09:42:46.840892Z","submitted_at":"2025-05-09T19:03:38Z","title":"Probing Weak-Force Corrections to Black Hole Geometry via Long Range Potentials: Feinberg-Sucher and Ferrer-Nowakowski Potentials","version":2},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-08-15T22:51:46.988311Z"},"links":{"cited_paper":"/paper/2405.05077","citing_paper":"/paper/2505.06382"},"observation_digest":"sha256:4dee0cab8b51b8b8362363d97b482bccf3e303a6413c032af79d5f4ded62a218","observation_id":"7ec91e96-01bc-4078-8737-6a2a817777a1","resolution":{"observed_at":"2026-08-15T22:51:48.620865Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2404.04046","last_updated":"2024-06-01T18:36:26Z","snapshot_observed_at":"2026-08-13T00:37:08.130929Z","submitted_at":"2024-04-05T11:59:47Z","title":"Analyzing the Influence of Geometrical Deformation on Photon Sphere and Shadow Radius: A New Analytical Approach -- Spherically Symmetric Spacetimes","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.04046","snapshot_observed_at":"2026-08-15T22:51:46.993170Z","title":"Vertogradov and A","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2505.06382","last_updated":"2025-05-28T06:37:40Z","snapshot_observed_at":"2026-08-16T09:42:46.840892Z","submitted_at":"2025-05-09T19:03:38Z","title":"Probing Weak-Force Corrections to Black Hole Geometry via Long Range Potentials: Feinberg-Sucher and Ferrer-Nowakowski Potentials","version":2},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-08-15T22:51:46.993170Z"},"links":{"cited_paper":"/paper/2404.04046","citing_paper":"/paper/2505.06382"},"observation_digest":"sha256:ac3688269383b66476b63dcd9497a0e959e670f3d7cb6ef1002380590757da90","observation_id":"ab1155b2-7edb-4f39-8d0b-34a8db6f39cc","resolution":{"observed_at":"2026-08-15T22:51:46.993170Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2404.18536","last_updated":"2024-06-01T18:46:01Z","snapshot_observed_at":"2026-08-13T00:19:39.569829Z","submitted_at":"2024-04-29T09:27:15Z","title":"General Approach on Shadow Radius and Photon Spheres in Asymptotically Flat Spacetimes and the Impact of Mass-Dependent Variations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.18536","snapshot_observed_at":"2026-08-15T22:51:46.997007Z","title":"Vertogradov and A.¨Ovg ¨un, Phys","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2505.06382","last_updated":"2025-05-28T06:37:40Z","snapshot_observed_at":"2026-08-16T09:42:46.840892Z","submitted_at":"2025-05-09T19:03:38Z","title":"Probing Weak-Force Corrections to Black Hole Geometry via Long Range Potentials: Feinberg-Sucher and Ferrer-Nowakowski Potentials","version":2},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-08-15T22:51:46.997007Z"},"links":{"cited_paper":"/paper/2404.18536","citing_paper":"/paper/2505.06382"},"observation_digest":"sha256:8b82c6e09c761c22d99bfcc99a06a0c73ab626c34eee829981239219a1aa9f62","observation_id":"29295edb-ea88-4aa2-a278-bad3fc927ee6","resolution":{"observed_at":"2026-08-15T22:51:46.997007Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2305.14305","last_updated":"2023-08-09T00:45:20Z","snapshot_observed_at":"2026-08-13T11:35:17.414780Z","submitted_at":"2023-05-23T17:45:06Z","title":"Observational constraints on Yukawa cosmology and connection with black hole shadows","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2305.14305","snapshot_observed_at":"2026-08-15T22:51:47.023041Z","title":"Gonz´alez, K","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2505.06382","last_updated":"2025-05-28T06:37:40Z","snapshot_observed_at":"2026-08-16T09:42:46.840892Z","submitted_at":"2025-05-09T19:03:38Z","title":"Probing Weak-Force Corrections to Black Hole Geometry via Long Range Potentials: Feinberg-Sucher and Ferrer-Nowakowski Potentials","version":2},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-08-15T22:51:47.023041Z"},"links":{"cited_paper":"/paper/2305.14305","citing_paper":"/paper/2505.06382"},"observation_digest":"sha256:99abab1b8cbc0719b81fd4599f5550448fbdca42251344e6b41b667ae1c4876d","observation_id":"5ba0e155-f69a-4c78-90f7-5b00d30e52c5","resolution":{"observed_at":"2026-08-15T22:51:47.023041Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2311.08930","last_updated":"2024-09-10T12:37:24Z","snapshot_observed_at":"2026-08-13T19:23:53.989168Z","submitted_at":"2023-11-15T13:02:07Z","title":"Dynamical Photon Spheres in Charged Black Holes and Naked Singularities","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2311.08930","snapshot_observed_at":"2026-08-15T22:51:47.005418Z","title":"Heydarzade and V","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2505.06382","last_updated":"2025-05-28T06:37:40Z","snapshot_observed_at":"2026-08-16T09:42:46.840892Z","submitted_at":"2025-05-09T19:03:38Z","title":"Probing Weak-Force Corrections to Black Hole Geometry via Long Range Potentials: Feinberg-Sucher and Ferrer-Nowakowski Potentials","version":2},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-08-15T22:51:47.005418Z"},"links":{"cited_paper":"/paper/2311.08930","citing_paper":"/paper/2505.06382"},"observation_digest":"sha256:6a8220f7bda30b6094a4ed48bd97adfe7a4ed106be23b27d5a5a82195b74fc5c","observation_id":"bc5ec8cc-944a-487d-ae64-9446a01fb809","resolution":{"observed_at":"2026-08-15T22:51:47.005418Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/0510112","last_updated":"2005-11-12T07:59:01Z","snapshot_observed_at":"2026-08-11T10:35:24.971521Z","submitted_at":"2005-10-26T09:55:41Z","title":"Noncommutative geometry inspired Schwarzschild black hole","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"gr-qc/0510112","snapshot_observed_at":"2026-08-15T22:51:47.009424Z","title":"Nicolini, A","venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"2505.06382","last_updated":"2025-05-28T06:37:40Z","snapshot_observed_at":"2026-08-16T09:42:46.840892Z","submitted_at":"2025-05-09T19:03:38Z","title":"Probing Weak-Force Corrections to Black Hole Geometry via Long Range Potentials: Feinberg-Sucher and Ferrer-Nowakowski Potentials","version":2},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-08-15T22:51:47.009424Z"},"links":{"cited_paper":"/paper/gr-qc/0510112","citing_paper":"/paper/2505.06382"},"observation_digest":"sha256:690ff35722a36de02b0583e75acd64efe6ed3003d1d3af01fc5e45c73121c3a3","observation_id":"10d31bc0-bfce-45ab-987d-dd2104788734","resolution":{"observed_at":"2026-08-15T22:51:47.009424Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2401.15211","last_updated":"2024-03-12T00:03:14Z","snapshot_observed_at":"2026-08-13T04:33:46.190116Z","submitted_at":"2024-01-26T21:21:00Z","title":"Charged Black Holes with Yukawa Potential","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2401.15211","snapshot_observed_at":"2026-08-15T22:51:47.013432Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2505.06382","last_updated":"2025-05-28T06:37:40Z","snapshot_observed_at":"2026-08-16T09:42:46.840892Z","submitted_at":"2025-05-09T19:03:38Z","title":"Probing Weak-Force Corrections to Black Hole Geometry via Long Range Potentials: Feinberg-Sucher and Ferrer-Nowakowski Potentials","version":2},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-08-15T22:51:47.013432Z"},"links":{"cited_paper":"/paper/2401.15211","citing_paper":"/paper/2505.06382"},"observation_digest":"sha256:3f4fc87b7b7a1aac4d391b4544afcaef049b18407e46734246bbb938861ac7dc","observation_id":"d9dfc736-de16-4162-ad29-7b279b90df69","resolution":{"observed_at":"2026-08-15T22:51:47.013432Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2402.05344","last_updated":"2024-02-08T01:23:22Z","snapshot_observed_at":"2026-08-13T04:23:46.927537Z","submitted_at":"2024-02-08T01:23:22Z","title":"Dark matter effects of a black hole with nonsingular Yukawa-modified potential in Einstein-Gauss-Bonnet Gravity","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2402.05344","snapshot_observed_at":"2026-08-15T22:51:47.018009Z","title":"Sekhmani, A","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2505.06382","last_updated":"2025-05-28T06:37:40Z","snapshot_observed_at":"2026-08-16T09:42:46.840892Z","submitted_at":"2025-05-09T19:03:38Z","title":"Probing Weak-Force Corrections to Black Hole Geometry via Long Range Potentials: Feinberg-Sucher and Ferrer-Nowakowski Potentials","version":2},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-08-15T22:51:47.018009Z"},"links":{"cited_paper":"/paper/2402.05344","citing_paper":"/paper/2505.06382"},"observation_digest":"sha256:737d50397104bac75d561e237469aa42ce1a5ad117996b0dc0213399f1040f92","observation_id":"2674e49d-0375-43c0-9d53-1ec13430bace","resolution":{"observed_at":"2026-08-15T22:51:47.018009Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"hep-ph/9710204","last_updated":"1997-11-12T10:29:30Z","snapshot_observed_at":"2026-07-07T04:27:05.538853Z","submitted_at":"1997-10-01T10:37:14Z","title":"Millimetre-Range Forces in Superstring Theories with Weak-Scale Compactification","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-ph/9710204","snapshot_observed_at":"2026-08-15T22:51:47.047731Z","title":"Antoniadis, S","venue":null,"work_id":null,"year":1998},"citing_paper":{"arxiv_id":"2505.06382","last_updated":"2025-05-28T06:37:40Z","snapshot_observed_at":"2026-08-16T09:42:46.840892Z","submitted_at":"2025-05-09T19:03:38Z","title":"Probing Weak-Force Corrections to Black Hole Geometry via Long Range Potentials: Feinberg-Sucher and Ferrer-Nowakowski Potentials","version":2},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-08-15T22:51:47.047731Z"},"links":{"cited_paper":"/paper/hep-ph/9710204","citing_paper":"/paper/2505.06382"},"observation_digest":"sha256:9b8622790a66e897f001c6b877bc90234bf9ab76502727f04c7f4dc0ecf85a31","observation_id":"96285f9f-41c1-402d-bb5f-40b8a541dd5c","resolution":{"observed_at":"2026-08-15T22:51:47.047731Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2304.11492","last_updated":"2024-08-21T13:10:50Z","snapshot_observed_at":"2026-08-13T11:57:33.365802Z","submitted_at":"2023-04-22T22:55:59Z","title":"Dark Universe Phenomenology from Yukawa Potential?","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2304.11492","snapshot_observed_at":"2026-08-15T22:51:47.028301Z","title":"Jusufi, G","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2505.06382","last_updated":"2025-05-28T06:37:40Z","snapshot_observed_at":"2026-08-16T09:42:46.840892Z","submitted_at":"2025-05-09T19:03:38Z","title":"Probing Weak-Force Corrections to Black Hole Geometry via Long Range Potentials: Feinberg-Sucher and Ferrer-Nowakowski Potentials","version":2},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-08-15T22:51:47.028301Z"},"links":{"cited_paper":"/paper/2304.11492","citing_paper":"/paper/2505.06382"},"observation_digest":"sha256:0e7342d03f86d7553089004cb64816fcb90035558bc343a9b4c42b29bd60658a","observation_id":"f0f4465e-4941-4366-b5f7-a537ab8879ad","resolution":{"observed_at":"2026-08-15T22:51:47.028301Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1902.11242","last_updated":"2019-08-27T19:27:20Z","snapshot_observed_at":"2026-08-14T17:09:27.655909Z","submitted_at":"2019-02-28T17:44:00Z","title":"Quantum Corrected Black Holes from String T-Duality","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1902.11242","snapshot_observed_at":"2026-08-15T22:51:47.033408Z","title":"Nicolini, E","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2505.06382","last_updated":"2025-05-28T06:37:40Z","snapshot_observed_at":"2026-08-16T09:42:46.840892Z","submitted_at":"2025-05-09T19:03:38Z","title":"Probing Weak-Force Corrections to Black Hole Geometry via Long Range Potentials: Feinberg-Sucher and Ferrer-Nowakowski Potentials","version":2},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-08-15T22:51:47.033408Z"},"links":{"cited_paper":"/paper/1902.11242","citing_paper":"/paper/2505.06382"},"observation_digest":"sha256:3c84817c1b6a25eb53df70889288b746a8b4f2b0bfd7d0eb4a1c6e855fb94fb0","observation_id":"44178b51-3880-4e32-a6b3-3c163f37141f","resolution":{"observed_at":"2026-08-15T22:51:47.033408Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T22:51:47.038072Z","title":null,"venue":null,"work_id":null,"year":1948},"citing_paper":{"arxiv_id":"2505.06382","last_updated":"2025-05-28T06:37:40Z","snapshot_observed_at":"2026-08-16T09:42:46.840892Z","submitted_at":"2025-05-09T19:03:38Z","title":"Probing Weak-Force Corrections to Black Hole Geometry via Long Range Potentials: Feinberg-Sucher and Ferrer-Nowakowski Potentials","version":2},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-08-15T22:51:47.038072Z"},"links":{"citing_paper":"/paper/2505.06382"},"observation_digest":"sha256:04e34b13c8df7b6534babef19a96a0846d9b1cfe0830faf3c81c91bdbbf388c2","observation_id":"b8dfa1a2-d45f-4aba-8add-7d6501d976dc","resolution":{"observed_at":"2026-08-15T22:51:47.038072Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T22:51:47.043437Z","title":"Feinberg and J","venue":null,"work_id":null,"year":1968},"citing_paper":{"arxiv_id":"2505.06382","last_updated":"2025-05-28T06:37:40Z","snapshot_observed_at":"2026-08-16T09:42:46.840892Z","submitted_at":"2025-05-09T19:03:38Z","title":"Probing Weak-Force Corrections to Black Hole Geometry via Long Range Potentials: Feinberg-Sucher and Ferrer-Nowakowski Potentials","version":2},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-08-15T22:51:47.043437Z"},"links":{"citing_paper":"/paper/2505.06382"},"observation_digest":"sha256:6c97bb70a582a9e194d2c23c777ace93e39a1475ce46722cf21933a23a30b3cc","observation_id":"a00a3a34-79c3-420c-a8ef-88ab4b315126","resolution":{"observed_at":"2026-08-15T22:51:47.043437Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2311.07764","last_updated":"2024-03-26T00:30:26Z","snapshot_observed_at":"2026-08-15T04:33:26.373430Z","submitted_at":"2023-11-13T21:28:14Z","title":"Gravitational Aharonov-Bohm Effect","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2311.07764","snapshot_observed_at":"2026-08-15T22:51:47.072817Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2505.06382","last_updated":"2025-05-28T06:37:40Z","snapshot_observed_at":"2026-08-16T09:42:46.840892Z","submitted_at":"2025-05-09T19:03:38Z","title":"Probing Weak-Force Corrections to Black Hole Geometry via Long Range Potentials: Feinberg-Sucher and Ferrer-Nowakowski Potentials","version":2},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-08-15T22:51:47.072817Z"},"links":{"cited_paper":"/paper/2311.07764","citing_paper":"/paper/2505.06382"},"observation_digest":"sha256:c2e3a89f3c84d30e82fb868981777ee7f6a9338358e2a228ba42c39e8160d9a8","observation_id":"563f1a80-d661-4db3-8394-2df9c129941f","resolution":{"observed_at":"2026-08-15T22:51:47.072817Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"hep-ph/0007226","last_updated":"2000-07-20T15:42:22Z","snapshot_observed_at":"2026-08-12T08:46:33.794948Z","submitted_at":"2000-07-20T15:42:22Z","title":"Large Dimensions and String Physics in Future Colliders","version":1},"cited_work":{"arxiv_id":"hep-ph/0007226","doi":null,"metadata_source":"pith","pith_arxiv_id":"hep-ph/0007226","snapshot_observed_at":"2026-08-15T22:51:48.475632Z","title":"Large Dimensions and String Physics in Future Colliders","venue":"hep-ph","work_id":"6238fc5f-8bab-42cb-8faf-e2402762e068","year":2000},"citing_paper":{"arxiv_id":"2505.06382","last_updated":"2025-05-28T06:37:40Z","snapshot_observed_at":"2026-08-16T09:42:46.840892Z","submitted_at":"2025-05-09T19:03:38Z","title":"Probing Weak-Force Corrections to Black Hole Geometry via Long Range Potentials: Feinberg-Sucher and Ferrer-Nowakowski Potentials","version":2},"reference_index":54,"source":"pdf_text","source_observed_at":"2026-08-15T22:51:47.052391Z"},"links":{"cited_paper":"/paper/hep-ph/0007226","citing_paper":"/paper/2505.06382"},"observation_digest":"sha256:7e26173be7cb0645a891a3445b3b133bc0b4687976000c90733d0a8b7b0e7e93","observation_id":"db746ee1-eab1-4d4d-b80b-baf9f2a57943","resolution":{"observed_at":"2026-08-15T22:51:48.479750Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T22:51:47.058846Z","title":"Antoniadis, C","venue":null,"work_id":null,"year":1987},"citing_paper":{"arxiv_id":"2505.06382","last_updated":"2025-05-28T06:37:40Z","snapshot_observed_at":"2026-08-16T09:42:46.840892Z","submitted_at":"2025-05-09T19:03:38Z","title":"Probing Weak-Force Corrections to Black Hole Geometry via Long Range Potentials: Feinberg-Sucher and Ferrer-Nowakowski Potentials","version":2},"reference_index":55,"source":"pdf_text","source_observed_at":"2026-08-15T22:51:47.058846Z"},"links":{"citing_paper":"/paper/2505.06382"},"observation_digest":"sha256:c96e1023d1508f55b3e963ebdb2e1c54adf1716f73581e71e9f23aa3094914c1","observation_id":"2fbe27dc-863b-45b3-8337-fde5cb74a4f5","resolution":{"observed_at":"2026-08-15T22:51:47.058846Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"hep-ph/9601367","last_updated":"1996-07-02T04:47:57Z","snapshot_observed_at":"2026-08-14T13:59:52.775998Z","submitted_at":"1996-01-30T07:04:28Z","title":"Experimental Signatures of Low Energy Gauge Mediated Supersymmetry Breaking","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-ph/9601367","snapshot_observed_at":"2026-08-15T22:51:47.064184Z","title":"Dimopoulos, M","venue":null,"work_id":null,"year":1996},"citing_paper":{"arxiv_id":"2505.06382","last_updated":"2025-05-28T06:37:40Z","snapshot_observed_at":"2026-08-16T09:42:46.840892Z","submitted_at":"2025-05-09T19:03:38Z","title":"Probing Weak-Force Corrections to Black Hole Geometry via Long Range Potentials: Feinberg-Sucher and Ferrer-Nowakowski Potentials","version":2},"reference_index":56,"source":"pdf_text","source_observed_at":"2026-08-15T22:51:47.064184Z"},"links":{"cited_paper":"/paper/hep-ph/9601367","citing_paper":"/paper/2505.06382"},"observation_digest":"sha256:c9e1038684dbe6c8e3c75fe24e4180e66a4442d37f8dc0ea13cd873e2b6f4355","observation_id":"1634585b-5377-4778-b32f-b8e63f4facda","resolution":{"observed_at":"2026-08-15T22:51:47.064184Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2409.13780","last_updated":"2024-09-19T20:44:57Z","snapshot_observed_at":"2026-08-12T22:41:27.121968Z","submitted_at":"2024-09-19T20:44:57Z","title":"Temporal Pound-Rebka experiment as gravitational Aharonov-Bohm effect","version":1},"cited_work":{"arxiv_id":"2409.13780","doi":null,"metadata_source":"pith","pith_arxiv_id":"2409.13780","snapshot_observed_at":"2026-08-15T22:51:48.444653Z","title":"Temporal Pound-Rebka experiment as gravitational Aharonov-Bohm effect","venue":"gr-qc","work_id":"241f4da2-11cd-4653-92c6-fe0ab46872da","year":2024},"citing_paper":{"arxiv_id":"2505.06382","last_updated":"2025-05-28T06:37:40Z","snapshot_observed_at":"2026-08-16T09:42:46.840892Z","submitted_at":"2025-05-09T19:03:38Z","title":"Probing Weak-Force Corrections to Black Hole Geometry via Long Range Potentials: Feinberg-Sucher and Ferrer-Nowakowski Potentials","version":2},"reference_index":57,"source":"pdf_text","source_observed_at":"2026-08-15T22:51:47.068241Z"},"links":{"cited_paper":"/paper/2409.13780","citing_paper":"/paper/2505.06382"},"observation_digest":"sha256:10054e419b05bda9bf02c6bbb7523fabfad8ae6f41695bff9882df418f978d9f","observation_id":"f7b73909-0537-4df2-b0dc-e1fbe6915d48","resolution":{"observed_at":"2026-08-15T22:51:48.449364Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T22:51:47.148249Z","title":"Tan et al., Phys","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2505.06382","last_updated":"2025-05-28T06:37:40Z","snapshot_observed_at":"2026-08-16T09:42:46.840892Z","submitted_at":"2025-05-09T19:03:38Z","title":"Probing Weak-Force Corrections to Black Hole Geometry via Long Range Potentials: Feinberg-Sucher and Ferrer-Nowakowski Potentials","version":2},"reference_index":58,"source":"pdf_text","source_observed_at":"2026-08-15T22:51:47.148249Z"},"links":{"citing_paper":"/paper/2505.06382"},"observation_digest":"sha256:7f32007c406728023af2ae8e6c2fb13300b388693283d938cb68df961a01a5ad","observation_id":"8679a166-2c07-4496-9eb4-86851ec00f1b","resolution":{"observed_at":"2026-08-15T22:51:47.148249Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"hep-ph/9810550","last_updated":"1998-10-30T17:26:44Z","snapshot_observed_at":"2026-07-07T04:31:13.333117Z","submitted_at":"1998-10-30T17:26:44Z","title":"Higgs- and Goldstone bosons-mediated long range forces","version":1},"cited_work":{"arxiv_id":"hep-ph/9810550","doi":null,"metadata_source":"pith","pith_arxiv_id":"hep-ph/9810550","snapshot_observed_at":"2026-08-15T22:51:48.413732Z","title":"Higgs- and Goldstone bosons-mediated long range forces","venue":"hep-ph","work_id":"a0206d11-4ab1-4486-b38d-c50bd2fdae3f","year":1998},"citing_paper":{"arxiv_id":"2505.06382","last_updated":"2025-05-28T06:37:40Z","snapshot_observed_at":"2026-08-16T09:42:46.840892Z","submitted_at":"2025-05-09T19:03:38Z","title":"Probing Weak-Force Corrections to Black Hole Geometry via Long Range Potentials: Feinberg-Sucher and Ferrer-Nowakowski Potentials","version":2},"reference_index":59,"source":"pdf_text","source_observed_at":"2026-08-15T22:51:47.077459Z"},"links":{"cited_paper":"/paper/hep-ph/9810550","citing_paper":"/paper/2505.06382"},"observation_digest":"sha256:43bc87a3d05f8ecab283d787844887499afed6bac4eeeb536f91acdc06dc59f9","observation_id":"2851aa65-7dc6-46c4-b7a9-ca9da101e755","resolution":{"observed_at":"2026-08-15T22:51:48.417945Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"hep-ph/9602350","last_updated":"1996-02-20T15:43:33Z","snapshot_observed_at":"2026-08-06T11:38:10.209350Z","submitted_at":"1996-02-20T15:43:33Z","title":"Macroscopic Forces from Supersymmetry","version":1},"cited_work":{"arxiv_id":"hep-ph/9602350","doi":null,"metadata_source":"pith","pith_arxiv_id":"hep-ph/9602350","snapshot_observed_at":"2026-08-15T22:51:48.399089Z","title":"Macroscopic Forces from Supersymmetry","venue":"hep-ph","work_id":"1ff79d2e-3263-4b06-aaa0-d71138effc76","year":1996},"citing_paper":{"arxiv_id":"2505.06382","last_updated":"2025-05-28T06:37:40Z","snapshot_observed_at":"2026-08-16T09:42:46.840892Z","submitted_at":"2025-05-09T19:03:38Z","title":"Probing Weak-Force Corrections to Black Hole Geometry via Long Range Potentials: Feinberg-Sucher and Ferrer-Nowakowski Potentials","version":2},"reference_index":60,"source":"pdf_text","source_observed_at":"2026-08-15T22:51:47.081536Z"},"links":{"cited_paper":"/paper/hep-ph/9602350","citing_paper":"/paper/2505.06382"},"observation_digest":"sha256:beb50bd26b909b4305d59d5c6f345e534eee141786551f3831febb8e8018ca6a","observation_id":"564b04a3-c0fb-46e9-9ecb-9af8671e8e8a","resolution":{"observed_at":"2026-08-15T22:51:48.402821Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2312.01422","last_updated":"2023-12-03T15:00:42Z","snapshot_observed_at":"2026-08-13T05:10:56.682773Z","submitted_at":"2023-12-03T15:00:42Z","title":"Testing Gravity and Predictions Beyond the Standard Model at Short Distances: The Casimir Effect","version":1},"cited_work":{"arxiv_id":"2312.01422","doi":null,"metadata_source":"pith","pith_arxiv_id":"2312.01422","snapshot_observed_at":"2026-08-15T22:51:48.382782Z","title":"Testing Gravity and Predictions Beyond the Standard Model at Short Distances: The Casimir Effect","venue":"hep-ph","work_id":"b7ce55d8-3797-4c20-b0f0-edc986141bfb","year":2023},"citing_paper":{"arxiv_id":"2505.06382","last_updated":"2025-05-28T06:37:40Z","snapshot_observed_at":"2026-08-16T09:42:46.840892Z","submitted_at":"2025-05-09T19:03:38Z","title":"Probing Weak-Force Corrections to Black Hole Geometry via Long Range Potentials: Feinberg-Sucher and Ferrer-Nowakowski Potentials","version":2},"reference_index":61,"source":"pdf_text","source_observed_at":"2026-08-15T22:51:47.085640Z"},"links":{"cited_paper":"/paper/2312.01422","citing_paper":"/paper/2505.06382"},"observation_digest":"sha256:3ee840299809be41f7866ca1e80abb55e5e4432d24a49f80f532bc78f8f7be96","observation_id":"319f383f-6982-43bd-b70f-b9d9da7607b0","resolution":{"observed_at":"2026-08-15T22:51:48.387296Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2003.00948","last_updated":"2020-03-02T14:50:28Z","snapshot_observed_at":"2026-08-13T23:22:44.696945Z","submitted_at":"2020-03-02T14:50:28Z","title":"Constraints on non-Newtonian gravity and axionlike particles from measuring the Casimir force in nanometer separation range","version":1},"cited_work":{"arxiv_id":"2003.00948","doi":null,"metadata_source":"pith","pith_arxiv_id":"2003.00948","snapshot_observed_at":"2026-08-15T22:51:48.363366Z","title":"Constraints on non-Newtonian gravity and axionlike particles from measuring the Casimir force in nanometer separation range","venue":"hep-ph","work_id":"fba964df-6e37-45ef-be90-5dd75bb331d9","year":2020},"citing_paper":{"arxiv_id":"2505.06382","last_updated":"2025-05-28T06:37:40Z","snapshot_observed_at":"2026-08-16T09:42:46.840892Z","submitted_at":"2025-05-09T19:03:38Z","title":"Probing Weak-Force Corrections to Black Hole Geometry via Long Range Potentials: Feinberg-Sucher and Ferrer-Nowakowski Potentials","version":2},"reference_index":62,"source":"pdf_text","source_observed_at":"2026-08-15T22:51:47.100763Z"},"links":{"cited_paper":"/paper/2003.00948","citing_paper":"/paper/2505.06382"},"observation_digest":"sha256:8176074c12ba16ecbad3ff3050e310085f506268f528f8d7c86f36d538c4a5c9","observation_id":"8787862c-4cf4-4bb5-bb4f-fb2ac1ee4226","resolution":{"observed_at":"2026-08-15T22:51:48.367930Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T22:51:46.796941Z","title":"In parallel, theoretical investigations have explored how neutrino backgrounds and finite temperature effects can induce long-range forces [ 64, 65]","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2505.06382","last_updated":"2025-05-28T06:37:40Z","snapshot_observed_at":"2026-08-16T09:42:46.840892Z","submitted_at":"2025-05-09T19:03:38Z","title":"Probing Weak-Force Corrections to Black Hole Geometry via Long Range Potentials: Feinberg-Sucher and Ferrer-Nowakowski Potentials","version":2},"reference_index":63,"source":"pdf_text","source_observed_at":"2026-08-15T22:51:46.796941Z"},"links":{"citing_paper":"/paper/2505.06382"},"observation_digest":"sha256:fe04e60d4675e91d00878c468819a277913ea3183eb29e4ddcd80403b5b085fa","observation_id":"4336a4e6-2bb2-4355-bcdd-2cc012d8d377","resolution":{"observed_at":"2026-08-15T22:51:46.796941Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T22:51:47.151920Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2505.06382","last_updated":"2025-05-28T06:37:40Z","snapshot_observed_at":"2026-08-16T09:42:46.840892Z","submitted_at":"2025-05-09T19:03:38Z","title":"Probing Weak-Force Corrections to Black Hole Geometry via Long Range Potentials: Feinberg-Sucher and Ferrer-Nowakowski Potentials","version":2},"reference_index":64,"source":"pdf_text","source_observed_at":"2026-08-15T22:51:47.151920Z"},"links":{"citing_paper":"/paper/2505.06382"},"observation_digest":"sha256:7254e1c04d412238e68dc57a562fa5e3c32ff306553a40e9479b1d7370ef1886","observation_id":"153ca721-d356-44f6-8466-f53e9e27030c","resolution":{"observed_at":"2026-08-15T22:51:47.151920Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2110.01582","last_updated":"2022-05-23T22:33:06Z","snapshot_observed_at":"2026-08-14T23:48:31.612008Z","submitted_at":"2021-10-04T17:25:39Z","title":"New Constraints on Dark Photon Dark Matter with Superconducting Nanowire Detectors in an Optical Haloscope","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2110.01582","snapshot_observed_at":"2026-08-15T22:51:47.155838Z","title":"Chiles et al","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2505.06382","last_updated":"2025-05-28T06:37:40Z","snapshot_observed_at":"2026-08-16T09:42:46.840892Z","submitted_at":"2025-05-09T19:03:38Z","title":"Probing Weak-Force Corrections to Black Hole Geometry via Long Range Potentials: Feinberg-Sucher and Ferrer-Nowakowski Potentials","version":2},"reference_index":65,"source":"pdf_text","source_observed_at":"2026-08-15T22:51:47.155838Z"},"links":{"cited_paper":"/paper/2110.01582","citing_paper":"/paper/2505.06382"},"observation_digest":"sha256:baa4ce830fa2f70ac6498b7a5d5de5e8650015fd975f8359746dad82f56533b6","observation_id":"d3eb37e5-4e9e-476d-aebe-4d964fae07b3","resolution":{"observed_at":"2026-08-15T22:51:47.155838Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1908.11785","last_updated":"2019-12-12T14:42:46Z","snapshot_observed_at":"2026-08-14T10:04:53.283381Z","submitted_at":"2019-08-30T15:24:19Z","title":"Exploring the Foundations of the Universe with Space Tests of the Equivalence Principle","version":3},"cited_work":{"arxiv_id":"1908.11785","doi":null,"metadata_source":"pith","pith_arxiv_id":"1908.11785","snapshot_observed_at":"2026-08-15T22:51:48.334912Z","title":"Exploring the Foundations of the Universe with Space Tests of the Equivalence Principle","venue":"physics.space-ph","work_id":"a475a043-1aa8-40c1-bb7b-faed32096d58","year":2019},"citing_paper":{"arxiv_id":"2505.06382","last_updated":"2025-05-28T06:37:40Z","snapshot_observed_at":"2026-08-16T09:42:46.840892Z","submitted_at":"2025-05-09T19:03:38Z","title":"Probing Weak-Force Corrections to Black Hole Geometry via Long Range Potentials: Feinberg-Sucher and Ferrer-Nowakowski Potentials","version":2},"reference_index":66,"source":"pdf_text","source_observed_at":"2026-08-15T22:51:47.160440Z"},"links":{"cited_paper":"/paper/1908.11785","citing_paper":"/paper/2505.06382"},"observation_digest":"sha256:2902a838a68e79714571411520efe9baeac00ec42c840a6883ba25a90e57d659","observation_id":"eddb2326-fdaf-454e-a9a9-671514a1c9d5","resolution":{"observed_at":"2026-08-15T22:51:48.339322Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2102.04070","last_updated":"2021-02-08T09:10:37Z","snapshot_observed_at":"2026-08-15T11:19:57.654029Z","submitted_at":"2021-02-08T09:10:37Z","title":"Leptonic CP and Flavor Violations in SUSY GUT with Right-handed Neutrinos","version":1},"cited_work":{"arxiv_id":"2102.04070","doi":null,"metadata_source":"pith","pith_arxiv_id":"2102.04070","snapshot_observed_at":"2026-08-15T22:51:48.318875Z","title":"Leptonic CP and Flavor Violations in SUSY GUT with Right-handed Neutrinos","venue":"hep-ph","work_id":"0905b1c7-f3be-4115-9b7d-bbf9f2235bd7","year":2021},"citing_paper":{"arxiv_id":"2505.06382","last_updated":"2025-05-28T06:37:40Z","snapshot_observed_at":"2026-08-16T09:42:46.840892Z","submitted_at":"2025-05-09T19:03:38Z","title":"Probing Weak-Force Corrections to Black Hole Geometry via Long Range Potentials: Feinberg-Sucher and Ferrer-Nowakowski Potentials","version":2},"reference_index":67,"source":"pdf_text","source_observed_at":"2026-08-15T22:51:47.164625Z"},"links":{"cited_paper":"/paper/2102.04070","citing_paper":"/paper/2505.06382"},"observation_digest":"sha256:4c40ff41bb0a0d76140271852937f5914a1950eb8f4ea386baa7c2c52f1159db","observation_id":"806f3de1-a145-4bf4-83be-7c389d4f41d5","resolution":{"observed_at":"2026-08-15T22:51:48.322936Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T22:51:47.168891Z","title":null,"venue":null,"work_id":null,"year":1993},"citing_paper":{"arxiv_id":"2505.06382","last_updated":"2025-05-28T06:37:40Z","snapshot_observed_at":"2026-08-16T09:42:46.840892Z","submitted_at":"2025-05-09T19:03:38Z","title":"Probing Weak-Force Corrections to Black Hole Geometry via Long Range Potentials: Feinberg-Sucher and Ferrer-Nowakowski Potentials","version":2},"reference_index":68,"source":"pdf_text","source_observed_at":"2026-08-15T22:51:47.168891Z"},"links":{"citing_paper":"/paper/2505.06382"},"observation_digest":"sha256:2a8a01f0389ab1f0e6ab37c39e306bdf63de6cefff9166858b2ffb4c189ef518","observation_id":"7d6985f4-8226-4118-bce3-ddbf0e11053e","resolution":{"observed_at":"2026-08-15T22:51:47.168891Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"hep-ph/9806438","last_updated":"1998-06-22T13:49:42Z","snapshot_observed_at":"2026-07-07T04:29:48.448431Z","submitted_at":"1998-06-22T13:49:42Z","title":"Long range forces induced by neutrinos at finite temperature","version":1},"cited_work":{"arxiv_id":"hep-ph/9806438","doi":null,"metadata_source":"pith","pith_arxiv_id":"hep-ph/9806438","snapshot_observed_at":"2026-08-15T22:51:48.303620Z","title":"Long range forces induced by neutrinos at finite temperature","venue":"hep-ph","work_id":"f946db8a-3063-498e-b72a-cd2315d0d4a8","year":1998},"citing_paper":{"arxiv_id":"2505.06382","last_updated":"2025-05-28T06:37:40Z","snapshot_observed_at":"2026-08-16T09:42:46.840892Z","submitted_at":"2025-05-09T19:03:38Z","title":"Probing Weak-Force Corrections to Black Hole Geometry via Long Range Potentials: Feinberg-Sucher and Ferrer-Nowakowski Potentials","version":2},"reference_index":69,"source":"pdf_text","source_observed_at":"2026-08-15T22:51:47.172913Z"},"links":{"cited_paper":"/paper/hep-ph/9806438","citing_paper":"/paper/2505.06382"},"observation_digest":"sha256:f41e7d4ebf47753f7ce236d3add6359b5bdbfeb6b4a613295faab8a06bce3557","observation_id":"207709fc-1281-4441-bb8e-2fc8da466e96","resolution":{"observed_at":"2026-08-15T22:51:48.307741Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"hep-ph/9906463","last_updated":"1999-06-23T10:58:23Z","snapshot_observed_at":"2026-07-07T04:33:32.996165Z","submitted_at":"1999-06-23T10:58:23Z","title":"Long range neutrino forces in the cosmic relic neutrino background","version":1},"cited_work":{"arxiv_id":"hep-ph/9906463","doi":null,"metadata_source":"pith","pith_arxiv_id":"hep-ph/9906463","snapshot_observed_at":"2026-08-15T22:51:48.282925Z","title":"Long range neutrino forces in the cosmic relic neutrino background","venue":"hep-ph","work_id":"223a0228-d8aa-4b5a-baa6-36277022cc25","year":1999},"citing_paper":{"arxiv_id":"2505.06382","last_updated":"2025-05-28T06:37:40Z","snapshot_observed_at":"2026-08-16T09:42:46.840892Z","submitted_at":"2025-05-09T19:03:38Z","title":"Probing Weak-Force Corrections to Black Hole Geometry via Long Range Potentials: Feinberg-Sucher and Ferrer-Nowakowski Potentials","version":2},"reference_index":70,"source":"pdf_text","source_observed_at":"2026-08-15T22:51:47.177192Z"},"links":{"cited_paper":"/paper/hep-ph/9906463","citing_paper":"/paper/2505.06382"},"observation_digest":"sha256:0efd0e183ccd4fb2fdd8a70031b99afaeb27f1600afae7b66cc9c3da7ce00581","observation_id":"38255ef6-3602-4f7e-91ae-b56ce1e3008c","resolution":{"observed_at":"2026-08-15T22:51:48.288887Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T22:51:47.181750Z","title":"Ghosh, Y","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2505.06382","last_updated":"2025-05-28T06:37:40Z","snapshot_observed_at":"2026-08-16T09:42:46.840892Z","submitted_at":"2025-05-09T19:03:38Z","title":"Probing Weak-Force Corrections to Black Hole Geometry via Long Range Potentials: Feinberg-Sucher and Ferrer-Nowakowski Potentials","version":2},"reference_index":71,"source":"pdf_text","source_observed_at":"2026-08-15T22:51:47.181750Z"},"links":{"citing_paper":"/paper/2505.06382"},"observation_digest":"sha256:f4976ef7a184ec84324a7f65255e07c1ef2cf9aeea1cc3cda423362e81cc87ee","observation_id":"9126786d-ca8b-463f-b23a-3c9ddaae4b50","resolution":{"observed_at":"2026-08-15T22:51:47.181750Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2403.13894","last_updated":"2025-01-06T17:45:52Z","snapshot_observed_at":"2026-08-13T00:49:14.174910Z","submitted_at":"2024-03-20T18:05:57Z","title":"Background-Induced Forces from Dark Relics","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2403.13894","snapshot_observed_at":"2026-08-15T22:51:47.185639Z","title":"Barbosa and S","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2505.06382","last_updated":"2025-05-28T06:37:40Z","snapshot_observed_at":"2026-08-16T09:42:46.840892Z","submitted_at":"2025-05-09T19:03:38Z","title":"Probing Weak-Force Corrections to Black Hole Geometry via Long Range Potentials: Feinberg-Sucher and Ferrer-Nowakowski Potentials","version":2},"reference_index":72,"source":"pdf_text","source_observed_at":"2026-08-15T22:51:47.185639Z"},"links":{"cited_paper":"/paper/2403.13894","citing_paper":"/paper/2505.06382"},"observation_digest":"sha256:bb63b55885bf7f47c5be5de967a8229d831ea44ff1f21273b9620ca792b816ca","observation_id":"9697ffac-9709-43aa-b53b-a7790246000c","resolution":{"observed_at":"2026-08-15T22:51:47.185639Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2212.03889","last_updated":"2023-09-17T15:46:25Z","snapshot_observed_at":"2026-08-13T13:25:46.357246Z","submitted_at":"2022-12-07T19:00:02Z","title":"On neutrino-mediated potentials in a neutrino background","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2212.03889","snapshot_observed_at":"2026-08-15T22:51:47.189629Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2505.06382","last_updated":"2025-05-28T06:37:40Z","snapshot_observed_at":"2026-08-16T09:42:46.840892Z","submitted_at":"2025-05-09T19:03:38Z","title":"Probing Weak-Force Corrections to Black Hole Geometry via Long Range Potentials: Feinberg-Sucher and Ferrer-Nowakowski Potentials","version":2},"reference_index":73,"source":"pdf_text","source_observed_at":"2026-08-15T22:51:47.189629Z"},"links":{"cited_paper":"/paper/2212.03889","citing_paper":"/paper/2505.06382"},"observation_digest":"sha256:441e1db398eff233b1b28d1bb83c2fd33451b81749c28b598ff6a0265929e279","observation_id":"867db8b5-fc6b-472c-bb42-d81fc66229da","resolution":{"observed_at":"2026-08-15T22:51:47.189629Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1912.09444","last_updated":"2020-09-03T22:46:45Z","snapshot_observed_at":"2026-08-15T10:04:44.022570Z","submitted_at":"2019-12-19T18:22:14Z","title":"Probing the two-neutrino exchange force using atomic parity violation","version":3},"cited_work":{"arxiv_id":"1912.09444","doi":null,"metadata_source":"pith","pith_arxiv_id":"1912.09444","snapshot_observed_at":"2026-08-15T22:51:48.183376Z","title":"Probing the two-neutrino exchange force using atomic parity violation","venue":"hep-ph","work_id":"392bec6f-7a2c-4597-a5da-4125659e187b","year":2019},"citing_paper":{"arxiv_id":"2505.06382","last_updated":"2025-05-28T06:37:40Z","snapshot_observed_at":"2026-08-16T09:42:46.840892Z","submitted_at":"2025-05-09T19:03:38Z","title":"Probing Weak-Force Corrections to Black Hole Geometry via Long Range Potentials: Feinberg-Sucher and Ferrer-Nowakowski Potentials","version":2},"reference_index":74,"source":"pdf_text","source_observed_at":"2026-08-15T22:51:47.209087Z"},"links":{"cited_paper":"/paper/1912.09444","citing_paper":"/paper/2505.06382"},"observation_digest":"sha256:192bb25ac3eacbcd586739462f4dd56d244e8bddb85c6127c7d4543ec23c6208","observation_id":"7ff485da-1d0c-447f-9e38-29d1fd60974a","resolution":{"observed_at":"2026-08-15T22:51:48.188007Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"ph/0407532","doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T22:51:48.162560Z","title":"Ferrer and J","venue":null,"work_id":"40e16fe4-3dae-4e12-b1d8-da75643f2e0c","year":2004},"citing_paper":{"arxiv_id":"2505.06382","last_updated":"2025-05-28T06:37:40Z","snapshot_observed_at":"2026-08-16T09:42:46.840892Z","submitted_at":"2025-05-09T19:03:38Z","title":"Probing Weak-Force Corrections to Black Hole Geometry via Long Range Potentials: Feinberg-Sucher and Ferrer-Nowakowski Potentials","version":2},"reference_index":75,"source":"pdf_text","source_observed_at":"2026-08-15T22:51:47.217429Z"},"links":{"citing_paper":"/paper/2505.06382"},"observation_digest":"sha256:75a2a9f98b9420d6ca13e7f476ea0049a58bb0b6e0a93b6c70dfbc4b022b7610","observation_id":"a0208ef3-e6ee-4676-837a-87c98bf9447c","resolution":{"observed_at":"2026-08-15T22:51:48.168669Z","resolver_source":"raw_fallback","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"ph/0009157","doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T22:51:48.094595Z","title":"Nowakowski, PoS silafae-III, 025 (2000), arXiv:hep- ph/0009157","venue":null,"work_id":"212825fe-46c9-44de-8d4e-78cbf253f78b","year":2000},"citing_paper":{"arxiv_id":"2505.06382","last_updated":"2025-05-28T06:37:40Z","snapshot_observed_at":"2026-08-16T09:42:46.840892Z","submitted_at":"2025-05-09T19:03:38Z","title":"Probing Weak-Force Corrections to Black Hole Geometry via Long Range Potentials: Feinberg-Sucher and Ferrer-Nowakowski Potentials","version":2},"reference_index":76,"source":"pdf_text","source_observed_at":"2026-08-15T22:51:47.221542Z"},"links":{"citing_paper":"/paper/2505.06382"},"observation_digest":"sha256:67e41b17b8c580acb81b32c9a3d91576d968befb91f5042407e8c9a455ad8140","observation_id":"40aab0af-dcaa-4052-9b04-f3880b202a6a","resolution":{"observed_at":"2026-08-15T22:51:48.100720Z","resolver_source":"raw_fallback","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"ph/9904394","doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T22:51:48.014809Z","title":"Ferrer and J","venue":null,"work_id":"0166aaf0-29d9-446f-a594-7e21890ba81c","year":1999},"citing_paper":{"arxiv_id":"2505.06382","last_updated":"2025-05-28T06:37:40Z","snapshot_observed_at":"2026-08-16T09:42:46.840892Z","submitted_at":"2025-05-09T19:03:38Z","title":"Probing Weak-Force Corrections to Black Hole Geometry via Long Range Potentials: Feinberg-Sucher and Ferrer-Nowakowski Potentials","version":2},"reference_index":77,"source":"pdf_text","source_observed_at":"2026-08-15T22:51:47.224637Z"},"links":{"citing_paper":"/paper/2505.06382"},"observation_digest":"sha256:4a536a5987540df4b4ce5149dc704f5789e6b41d366b46c9ead09fb44771538a","observation_id":"472170c5-336f-4dbb-8abe-f586a317063d","resolution":{"observed_at":"2026-08-15T22:51:48.022339Z","resolver_source":"raw_fallback","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"hep-ph/9707536","last_updated":"1997-08-04T12:55:06Z","snapshot_observed_at":"2026-08-02T07:31:13.407583Z","submitted_at":"1997-07-31T16:35:29Z","title":"Gravitinos from Gravitational Collapse","version":2},"cited_work":{"arxiv_id":"hep-ph/9707536","doi":null,"metadata_source":"pith","pith_arxiv_id":"hep-ph/9707536","snapshot_observed_at":"2026-08-15T22:51:47.950146Z","title":"Gravitinos from Gravitational Collapse","venue":"hep-ph","work_id":"7823de1c-b12e-4f8f-bc78-659bf7fc326b","year":1997},"citing_paper":{"arxiv_id":"2505.06382","last_updated":"2025-05-28T06:37:40Z","snapshot_observed_at":"2026-08-16T09:42:46.840892Z","submitted_at":"2025-05-09T19:03:38Z","title":"Probing Weak-Force Corrections to Black Hole Geometry via Long Range Potentials: Feinberg-Sucher and Ferrer-Nowakowski Potentials","version":2},"reference_index":78,"source":"pdf_text","source_observed_at":"2026-08-15T22:51:47.227847Z"},"links":{"cited_paper":"/paper/hep-ph/9707536","citing_paper":"/paper/2505.06382"},"observation_digest":"sha256:7fdba6ec62f75462077d1e23ec6b9cc695481731c8f0d6b60874955ea987b98f","observation_id":"32e945c6-77cd-4d57-994c-857a52b2452d","resolution":{"observed_at":"2026-08-15T22:51:47.954513Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"hep-ph/9306222","last_updated":"1993-06-03T21:51:35Z","snapshot_observed_at":"2026-08-06T18:01:29.248910Z","submitted_at":"1993-06-03T21:51:35Z","title":"Long Range Forces from the Cosmological Neutrino Background","version":1},"cited_work":{"arxiv_id":"hep-ph/9306222","doi":null,"metadata_source":"pith","pith_arxiv_id":"hep-ph/9306222","snapshot_observed_at":"2026-08-15T22:51:47.934422Z","title":"Long Range Forces from the Cosmological Neutrino Background","venue":"hep-ph","work_id":"a8a01943-74da-4cf4-b911-befae022f700","year":1993},"citing_paper":{"arxiv_id":"2505.06382","last_updated":"2025-05-28T06:37:40Z","snapshot_observed_at":"2026-08-16T09:42:46.840892Z","submitted_at":"2025-05-09T19:03:38Z","title":"Probing Weak-Force Corrections to Black Hole Geometry via Long Range Potentials: Feinberg-Sucher and Ferrer-Nowakowski Potentials","version":2},"reference_index":79,"source":"pdf_text","source_observed_at":"2026-08-15T22:51:47.232839Z"},"links":{"cited_paper":"/paper/hep-ph/9306222","citing_paper":"/paper/2505.06382"},"observation_digest":"sha256:269387ae3dd81f26803a1cde6f405cdbbb957a0bdf59e033fced81c40973b5c0","observation_id":"3d768b44-5560-424d-b4a4-95d189665d80","resolution":{"observed_at":"2026-08-15T22:51:47.939057Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T22:51:47.237859Z","title":"Wilczek, Phys","venue":null,"work_id":null,"year":1982},"citing_paper":{"arxiv_id":"2505.06382","last_updated":"2025-05-28T06:37:40Z","snapshot_observed_at":"2026-08-16T09:42:46.840892Z","submitted_at":"2025-05-09T19:03:38Z","title":"Probing Weak-Force Corrections to Black Hole Geometry via Long Range Potentials: Feinberg-Sucher and Ferrer-Nowakowski Potentials","version":2},"reference_index":80,"source":"pdf_text","source_observed_at":"2026-08-15T22:51:47.237859Z"},"links":{"citing_paper":"/paper/2505.06382"},"observation_digest":"sha256:e35013b5a323a9ce9ef103095d61c4ecb0a344719310099d33bc3cd23bce6d86","observation_id":"a5598692-3641-446e-a502-bfef4e1eb89c","resolution":{"observed_at":"2026-08-15T22:51:47.237859Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2409.16367","last_updated":"2024-12-31T14:38:07Z","snapshot_observed_at":"2026-08-12T22:38:23.498021Z","submitted_at":"2024-09-24T18:01:31Z","title":"The Unknowns of the Diffuse Supernova Neutrino Background Hinder New Physics Searches","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2409.16367","snapshot_observed_at":"2026-08-15T22:51:47.241487Z","title":"MacDonald, P","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2505.06382","last_updated":"2025-05-28T06:37:40Z","snapshot_observed_at":"2026-08-16T09:42:46.840892Z","submitted_at":"2025-05-09T19:03:38Z","title":"Probing Weak-Force Corrections to Black Hole Geometry via Long Range Potentials: Feinberg-Sucher and Ferrer-Nowakowski Potentials","version":2},"reference_index":81,"source":"pdf_text","source_observed_at":"2026-08-15T22:51:47.241487Z"},"links":{"cited_paper":"/paper/2409.16367","citing_paper":"/paper/2505.06382"},"observation_digest":"sha256:0e53e8a63aa90bea6db717572656a13a88244bb50571dab539ec9331a44a06ea","observation_id":"1070f15b-5568-459e-8b5c-91c404c5503f","resolution":{"observed_at":"2026-08-15T22:51:47.241487Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2408.04234","last_updated":"2025-03-18T14:30:53Z","snapshot_observed_at":"2026-08-14T22:36:19.287760Z","submitted_at":"2024-08-08T05:40:21Z","title":"Distinguishing Beyond-Standard Model Effects in Neutrino Oscillation","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2408.04234","snapshot_observed_at":"2026-08-15T22:51:47.245506Z","title":"Calatayud-Cadenillas, A","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2505.06382","last_updated":"2025-05-28T06:37:40Z","snapshot_observed_at":"2026-08-16T09:42:46.840892Z","submitted_at":"2025-05-09T19:03:38Z","title":"Probing Weak-Force Corrections to Black Hole Geometry via Long Range Potentials: Feinberg-Sucher and Ferrer-Nowakowski Potentials","version":2},"reference_index":82,"source":"pdf_text","source_observed_at":"2026-08-15T22:51:47.245506Z"},"links":{"cited_paper":"/paper/2408.04234","citing_paper":"/paper/2505.06382"},"observation_digest":"sha256:e256ce0717fa11a33b458354248fdc088af2828c0ddf2aba864bb510438f83a4","observation_id":"fe129285-1511-43a6-883c-a88ec038baba","resolution":{"observed_at":"2026-08-15T22:51:47.245506Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2402.00116","last_updated":"2024-03-20T16:09:38Z","snapshot_observed_at":"2026-08-13T04:29:48.208836Z","submitted_at":"2024-01-31T19:00:03Z","title":"The Sun and core-collapse supernovae are leading probes of the neutrino lifetime","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2402.00116","snapshot_observed_at":"2026-08-15T22:51:47.249318Z","title":"Mart´ınez-Mirav´e, I","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2505.06382","last_updated":"2025-05-28T06:37:40Z","snapshot_observed_at":"2026-08-16T09:42:46.840892Z","submitted_at":"2025-05-09T19:03:38Z","title":"Probing Weak-Force Corrections to Black Hole Geometry via Long Range Potentials: Feinberg-Sucher and Ferrer-Nowakowski Potentials","version":2},"reference_index":83,"source":"pdf_text","source_observed_at":"2026-08-15T22:51:47.249318Z"},"links":{"cited_paper":"/paper/2402.00116","citing_paper":"/paper/2505.06382"},"observation_digest":"sha256:caceb9363bfae2701588574839c8156cd829beec5895b83b242fc87910a2f85a","observation_id":"a0821e2b-6d96-42e6-a35c-44659744c7ce","resolution":{"observed_at":"2026-08-15T22:51:47.249318Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2203.07377","last_updated":"2023-12-26T23:27:42Z","snapshot_observed_at":"2026-08-16T04:11:04.410210Z","submitted_at":"2022-03-14T18:13:30Z","title":"Synergy between cosmological and laboratory searches in neutrino physics","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2203.07377","snapshot_observed_at":"2026-08-15T22:51:47.253300Z","title":"Gerbino et al","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2505.06382","last_updated":"2025-05-28T06:37:40Z","snapshot_observed_at":"2026-08-16T09:42:46.840892Z","submitted_at":"2025-05-09T19:03:38Z","title":"Probing Weak-Force Corrections to Black Hole Geometry via Long Range Potentials: Feinberg-Sucher and Ferrer-Nowakowski Potentials","version":2},"reference_index":84,"source":"pdf_text","source_observed_at":"2026-08-15T22:51:47.253300Z"},"links":{"cited_paper":"/paper/2203.07377","citing_paper":"/paper/2505.06382"},"observation_digest":"sha256:6876f60cc9dfce3353b44da013872ea68182d247ff20c7e6f5322923daa40ac8","observation_id":"083c5313-d75a-42b5-8265-935a2c6648bb","resolution":{"observed_at":"2026-08-15T22:51:47.253300Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2503.02940","last_updated":"2025-06-24T18:01:35Z","snapshot_observed_at":"2026-08-11T17:07:06.497943Z","submitted_at":"2025-03-04T19:00:07Z","title":"Impact of the cosmic neutrino background on black hole superradiance","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2503.02940","snapshot_observed_at":"2026-08-15T22:51:47.257142Z","title":"Lambiase, T","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2505.06382","last_updated":"2025-05-28T06:37:40Z","snapshot_observed_at":"2026-08-16T09:42:46.840892Z","submitted_at":"2025-05-09T19:03:38Z","title":"Probing Weak-Force Corrections to Black Hole Geometry via Long Range Potentials: Feinberg-Sucher and Ferrer-Nowakowski Potentials","version":2},"reference_index":85,"source":"pdf_text","source_observed_at":"2026-08-15T22:51:47.257142Z"},"links":{"cited_paper":"/paper/2503.02940","citing_paper":"/paper/2505.06382"},"observation_digest":"sha256:a000344f2c031b01c1a2adfda14855b2b828586d9a79138e628b83cdc02079f4","observation_id":"f32f7420-d3d0-48fb-826c-94f585c6a4b7","resolution":{"observed_at":"2026-08-15T22:51:47.257142Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2412.09575","last_updated":"2024-12-12T18:53:22Z","snapshot_observed_at":"2026-08-11T18:33:48.371596Z","submitted_at":"2024-12-12T18:53:22Z","title":"Limits on dark matter, ultralight scalars, and cosmic neutrinos with gyroscope spin and precision clocks","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2412.09575","snapshot_observed_at":"2026-08-15T22:51:47.261002Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2505.06382","last_updated":"2025-05-28T06:37:40Z","snapshot_observed_at":"2026-08-16T09:42:46.840892Z","submitted_at":"2025-05-09T19:03:38Z","title":"Probing Weak-Force Corrections to Black Hole Geometry via Long Range Potentials: Feinberg-Sucher and Ferrer-Nowakowski Potentials","version":2},"reference_index":86,"source":"pdf_text","source_observed_at":"2026-08-15T22:51:47.261002Z"},"links":{"cited_paper":"/paper/2412.09575","citing_paper":"/paper/2505.06382"},"observation_digest":"sha256:ad399add5dbe9e07b1b44af54b44bb3d33ca546b8c29e59bc5c0a6de2b0e3a43","observation_id":"9a3f8acb-26f8-4f9f-963e-150726c5568f","resolution":{"observed_at":"2026-08-15T22:51:47.261002Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2407.16742","last_updated":"2025-01-26T08:51:26Z","snapshot_observed_at":"2026-08-14T14:40:07.513673Z","submitted_at":"2024-07-23T17:53:33Z","title":"Quantum coherence in neutrino spin-flavor oscillations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2407.16742","snapshot_observed_at":"2026-08-15T22:51:47.265229Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2505.06382","last_updated":"2025-05-28T06:37:40Z","snapshot_observed_at":"2026-08-16T09:42:46.840892Z","submitted_at":"2025-05-09T19:03:38Z","title":"Probing Weak-Force Corrections to Black Hole Geometry via Long Range Potentials: Feinberg-Sucher and Ferrer-Nowakowski Potentials","version":2},"reference_index":87,"source":"pdf_text","source_observed_at":"2026-08-15T22:51:47.265229Z"},"links":{"cited_paper":"/paper/2407.16742","citing_paper":"/paper/2505.06382"},"observation_digest":"sha256:65032ed21befb1fd9e462801b4bdbfe8ea1d4cbe04efd58f9e7d84993e5524cb","observation_id":"35247d05-46a2-4fc5-b506-d9875f575a02","resolution":{"observed_at":"2026-08-15T22:51:47.265229Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2306.16977","last_updated":"2023-12-11T04:42:38Z","snapshot_observed_at":"2026-08-15T07:31:18.813617Z","submitted_at":"2023-06-29T14:31:39Z","title":"Astrophysical neutrino oscillations after pulsar timing array analyses","version":2},"cited_work":{"arxiv_id":"2306.16977","doi":null,"metadata_source":"pith","pith_arxiv_id":"2306.16977","snapshot_observed_at":"2026-08-15T22:51:47.846483Z","title":"Astrophysical neutrino oscillations after pulsar timing array analyses","venue":"astro-ph.HE","work_id":"da8d004d-60e1-4bbc-8d15-2490eaecf0f2","year":2023},"citing_paper":{"arxiv_id":"2505.06382","last_updated":"2025-05-28T06:37:40Z","snapshot_observed_at":"2026-08-16T09:42:46.840892Z","submitted_at":"2025-05-09T19:03:38Z","title":"Probing Weak-Force Corrections to Black Hole Geometry via Long Range Potentials: Feinberg-Sucher and Ferrer-Nowakowski Potentials","version":2},"reference_index":88,"source":"pdf_text","source_observed_at":"2026-08-15T22:51:47.269224Z"},"links":{"cited_paper":"/paper/2306.16977","citing_paper":"/paper/2505.06382"},"observation_digest":"sha256:4ea7e121fa362c49332665bd97437c800431f3868ebcff5c27ba987fe8c498b2","observation_id":"542b987e-aa71-41c8-b1c9-d5b2bf2e14b3","resolution":{"observed_at":"2026-08-15T22:51:47.851295Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2207.08067","last_updated":"2023-01-13T18:44:13Z","snapshot_observed_at":"2026-08-15T04:13:29.241392Z","submitted_at":"2022-07-17T03:35:13Z","title":"Gravitational waves and neutrino oscillations in Chern-Simons axion gravity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2207.08067","snapshot_observed_at":"2026-08-15T22:51:47.273475Z","title":"Lambiase, L","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2505.06382","last_updated":"2025-05-28T06:37:40Z","snapshot_observed_at":"2026-08-16T09:42:46.840892Z","submitted_at":"2025-05-09T19:03:38Z","title":"Probing Weak-Force Corrections to Black Hole Geometry via Long Range Potentials: Feinberg-Sucher and Ferrer-Nowakowski Potentials","version":2},"reference_index":89,"source":"pdf_text","source_observed_at":"2026-08-15T22:51:47.273475Z"},"links":{"cited_paper":"/paper/2207.08067","citing_paper":"/paper/2505.06382"},"observation_digest":"sha256:e4552f7ab6937a121552dcd2f221c8f9e3ff235243bd36918ba6484f5a5925e5","observation_id":"64375fe0-eba9-43f6-a086-61b581210f71","resolution":{"observed_at":"2026-08-15T22:51:47.273475Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2110.02996","last_updated":"2021-10-06T18:12:35Z","snapshot_observed_at":"2026-08-13T17:58:17.171912Z","submitted_at":"2021-10-06T18:12:35Z","title":"Testing extended theories of gravity with GRBs","version":1},"cited_work":{"arxiv_id":"2110.02996","doi":null,"metadata_source":"pith","pith_arxiv_id":"2110.02996","snapshot_observed_at":"2026-08-15T22:51:47.704406Z","title":"Testing extended theories of gravity with GRBs","venue":"astro-ph.HE","work_id":"113895e8-a2a5-4a92-bf9a-b4205b704fe5","year":2021},"citing_paper":{"arxiv_id":"2505.06382","last_updated":"2025-05-28T06:37:40Z","snapshot_observed_at":"2026-08-16T09:42:46.840892Z","submitted_at":"2025-05-09T19:03:38Z","title":"Probing Weak-Force Corrections to Black Hole Geometry via Long Range Potentials: Feinberg-Sucher and Ferrer-Nowakowski Potentials","version":2},"reference_index":90,"source":"pdf_text","source_observed_at":"2026-08-15T22:51:47.277462Z"},"links":{"cited_paper":"/paper/2110.02996","citing_paper":"/paper/2505.06382"},"observation_digest":"sha256:5db2d73065a59f179a73007c9cd88501c64fd94838c11a83a6353415d25a6b90","observation_id":"8bdf07b6-bbb6-4c6d-9767-ba58a4c6e76c","resolution":{"observed_at":"2026-08-15T22:51:47.708838Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T22:51:47.281229Z","title":null,"venue":null,"work_id":null,"year":1994},"citing_paper":{"arxiv_id":"2505.06382","last_updated":"2025-05-28T06:37:40Z","snapshot_observed_at":"2026-08-16T09:42:46.840892Z","submitted_at":"2025-05-09T19:03:38Z","title":"Probing Weak-Force Corrections to Black Hole Geometry via Long Range Potentials: Feinberg-Sucher and Ferrer-Nowakowski Potentials","version":2},"reference_index":91,"source":"pdf_text","source_observed_at":"2026-08-15T22:51:47.281229Z"},"links":{"citing_paper":"/paper/2505.06382"},"observation_digest":"sha256:c98d0e5ca098ad9e4e218f14e8d64e9664f88e8c2a58e5aa63ea1c48612da1ad","observation_id":"8fc51ae5-3514-48c9-902b-0d9479c6041e","resolution":{"observed_at":"2026-08-15T22:51:47.281229Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T22:51:47.284702Z","title":null,"venue":null,"work_id":null,"year":1994},"citing_paper":{"arxiv_id":"2505.06382","last_updated":"2025-05-28T06:37:40Z","snapshot_observed_at":"2026-08-16T09:42:46.840892Z","submitted_at":"2025-05-09T19:03:38Z","title":"Probing Weak-Force Corrections to Black Hole Geometry via Long Range Potentials: Feinberg-Sucher and Ferrer-Nowakowski Potentials","version":2},"reference_index":92,"source":"pdf_text","source_observed_at":"2026-08-15T22:51:47.284702Z"},"links":{"citing_paper":"/paper/2505.06382"},"observation_digest":"sha256:f559b5e0a6892d089aeba5853d2a49a4c785306852fc799af65af953b72dee53","observation_id":"1f681e1e-03ff-4769-b81a-1b96cc9eb479","resolution":{"observed_at":"2026-08-15T22:51:47.284702Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T22:51:47.288498Z","title":null,"venue":null,"work_id":null,"year":2004},"citing_paper":{"arxiv_id":"2505.06382","last_updated":"2025-05-28T06:37:40Z","snapshot_observed_at":"2026-08-16T09:42:46.840892Z","submitted_at":"2025-05-09T19:03:38Z","title":"Probing Weak-Force Corrections to Black Hole Geometry via Long Range Potentials: Feinberg-Sucher and Ferrer-Nowakowski Potentials","version":2},"reference_index":93,"source":"pdf_text","source_observed_at":"2026-08-15T22:51:47.288498Z"},"links":{"citing_paper":"/paper/2505.06382"},"observation_digest":"sha256:ebac0e4327b9a8840352d8f5c805045f34c6de4bbb696a7ba787d8e3e3fe2cc5","observation_id":"dab80348-7f8d-4324-9302-34cf7d27aadd","resolution":{"observed_at":"2026-08-15T22:51:47.288498Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T22:51:47.291855Z","title":"Feinberg, J","venue":null,"work_id":null,"year":1989},"citing_paper":{"arxiv_id":"2505.06382","last_updated":"2025-05-28T06:37:40Z","snapshot_observed_at":"2026-08-16T09:42:46.840892Z","submitted_at":"2025-05-09T19:03:38Z","title":"Probing Weak-Force Corrections to Black Hole Geometry via Long Range Potentials: Feinberg-Sucher and Ferrer-Nowakowski Potentials","version":2},"reference_index":94,"source":"pdf_text","source_observed_at":"2026-08-15T22:51:47.291855Z"},"links":{"citing_paper":"/paper/2505.06382"},"observation_digest":"sha256:e914f0b9ecaee52d7ac171ebdb6d3179f370c8702263d8089fa184c160a53e27","observation_id":"c975cfa6-12e2-4494-a3c1-bfef63835e83","resolution":{"observed_at":"2026-08-15T22:51:47.291855Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"hep-th/0608098","last_updated":"2006-09-24T00:29:55Z","snapshot_observed_at":"2026-08-15T11:06:16.713445Z","submitted_at":"2006-08-15T05:40:35Z","title":"Hawking temperature in the tunneling picture","version":2},"cited_work":{"arxiv_id":"hep-th/0608098","doi":null,"metadata_source":"pith","pith_arxiv_id":"hep-th/0608098","snapshot_observed_at":"2026-08-15T22:51:47.482129Z","title":"Hawking temperature in the tunneling picture","venue":"hep-th","work_id":"fed56962-2de9-4518-a9fc-c0f5f339f6dd","year":2006},"citing_paper":{"arxiv_id":"2505.06382","last_updated":"2025-05-28T06:37:40Z","snapshot_observed_at":"2026-08-16T09:42:46.840892Z","submitted_at":"2025-05-09T19:03:38Z","title":"Probing Weak-Force Corrections to Black Hole Geometry via Long Range Potentials: Feinberg-Sucher and Ferrer-Nowakowski Potentials","version":2},"reference_index":95,"source":"pdf_text","source_observed_at":"2026-08-15T22:51:47.296024Z"},"links":{"cited_paper":"/paper/hep-th/0608098","citing_paper":"/paper/2505.06382"},"observation_digest":"sha256:f679da418be23c7874c9a44fcc869ce61727946713a2c5e34729303165386779","observation_id":"9a5a5381-3bb8-44cb-be6a-7f1b09c3de12","resolution":{"observed_at":"2026-08-15T22:51:47.488634Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2410.16127","last_updated":"2024-10-21T15:54:48Z","snapshot_observed_at":"2026-08-15T21:40:10.102782Z","submitted_at":"2024-10-21T15:54:48Z","title":"Perturbation theory for gravitational shadows in static spherically symmetric spacetimes","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2410.16127","snapshot_observed_at":"2026-08-15T22:51:47.301385Z","title":"Kobialko and D","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2505.06382","last_updated":"2025-05-28T06:37:40Z","snapshot_observed_at":"2026-08-16T09:42:46.840892Z","submitted_at":"2025-05-09T19:03:38Z","title":"Probing Weak-Force Corrections to Black Hole Geometry via Long Range Potentials: Feinberg-Sucher and Ferrer-Nowakowski Potentials","version":2},"reference_index":96,"source":"pdf_text","source_observed_at":"2026-08-15T22:51:47.301385Z"},"links":{"cited_paper":"/paper/2410.16127","citing_paper":"/paper/2505.06382"},"observation_digest":"sha256:8a6896bf8350ab1283ebc08bcd363ece492e3cebd48cb2d3b36e13a4c621ca44","observation_id":"a6831ea3-5d55-4ade-8b9a-b72be88bf13a","resolution":{"observed_at":"2026-08-15T22:51:47.301385Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T22:51:47.305570Z","title":"Atamurotov, A","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2505.06382","last_updated":"2025-05-28T06:37:40Z","snapshot_observed_at":"2026-08-16T09:42:46.840892Z","submitted_at":"2025-05-09T19:03:38Z","title":"Probing Weak-Force Corrections to Black Hole Geometry via Long Range Potentials: Feinberg-Sucher and Ferrer-Nowakowski Potentials","version":2},"reference_index":97,"source":"pdf_text","source_observed_at":"2026-08-15T22:51:47.305570Z"},"links":{"citing_paper":"/paper/2505.06382"},"observation_digest":"sha256:97ef3c4998fbfb35050602d896ea1eac6c5598da8a41b60960fe186e75a05862","observation_id":"7b74f792-7969-4610-b75c-62178b73a210","resolution":{"observed_at":"2026-08-15T22:51:47.305570Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1403.0371","last_updated":"2014-06-18T14:24:30Z","snapshot_observed_at":"2026-08-14T23:42:42.649804Z","submitted_at":"2014-03-03T10:24:41Z","title":"Constraining the spin and the deformation parameters from the black hole shadow","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1403.0371","snapshot_observed_at":"2026-08-15T22:51:47.309126Z","title":"Tsukamoto, Z","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2505.06382","last_updated":"2025-05-28T06:37:40Z","snapshot_observed_at":"2026-08-16T09:42:46.840892Z","submitted_at":"2025-05-09T19:03:38Z","title":"Probing Weak-Force Corrections to Black Hole Geometry via Long Range Potentials: Feinberg-Sucher and Ferrer-Nowakowski Potentials","version":2},"reference_index":98,"source":"pdf_text","source_observed_at":"2026-08-15T22:51:47.309126Z"},"links":{"cited_paper":"/paper/1403.0371","citing_paper":"/paper/2505.06382"},"observation_digest":"sha256:34e008305dd3bd8b814919e6dd63ff1074123a38d029eda48af31933f1c7e536","observation_id":"0c24ca0b-d30e-4388-be27-8bf195647b56","resolution":{"observed_at":"2026-08-15T22:51:47.309126Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1507.04217","last_updated":"2015-11-11T00:30:37Z","snapshot_observed_at":"2026-08-14T22:40:20.636846Z","submitted_at":"2015-07-15T13:48:13Z","title":"Influence of a plasma on the shadow of a spherically symmetric black hole","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1507.04217","snapshot_observed_at":"2026-08-15T22:51:47.313010Z","title":"Perlick, O","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2505.06382","last_updated":"2025-05-28T06:37:40Z","snapshot_observed_at":"2026-08-16T09:42:46.840892Z","submitted_at":"2025-05-09T19:03:38Z","title":"Probing Weak-Force Corrections to Black Hole Geometry via Long Range Potentials: Feinberg-Sucher and Ferrer-Nowakowski Potentials","version":2},"reference_index":99,"source":"pdf_text","source_observed_at":"2026-08-15T22:51:47.313010Z"},"links":{"cited_paper":"/paper/1507.04217","citing_paper":"/paper/2505.06382"},"observation_digest":"sha256:35623398e19a876e1a468d04d0c6d72934da1edfdf531beaa218eec5d057f844","observation_id":"71936bf0-cec5-47f9-8bbe-61c065333b9d","resolution":{"observed_at":"2026-08-15T22:51:47.313010Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1006.2321","last_updated":"2010-06-11T14:28:40Z","snapshot_observed_at":"2026-08-15T05:16:42.449686Z","submitted_at":"2010-06-11T14:28:40Z","title":"Gravitational lensing in a non-uniform plasma","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1006.2321","snapshot_observed_at":"2026-08-15T22:51:47.316903Z","title":null,"venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2505.06382","last_updated":"2025-05-28T06:37:40Z","snapshot_observed_at":"2026-08-16T09:42:46.840892Z","submitted_at":"2025-05-09T19:03:38Z","title":"Probing Weak-Force Corrections to Black Hole Geometry via Long Range Potentials: Feinberg-Sucher and Ferrer-Nowakowski Potentials","version":2},"reference_index":100,"source":"pdf_text","source_observed_at":"2026-08-15T22:51:47.316903Z"},"links":{"cited_paper":"/paper/1006.2321","citing_paper":"/paper/2505.06382"},"observation_digest":"sha256:6630b0210f74cb3de0aa1b83643658910fd0bb0794e905d79fce9da84a0cfa16","observation_id":"d4d47528-dd70-4521-8add-fcfa38c819c3","resolution":{"observed_at":"2026-08-15T22:51:47.316903Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"2505.06382","last_updated":"2025-05-28T06:37:40Z","latest_version":2,"primary_category":"gr-qc","snapshot_observed_at":"2026-08-16T09:42:46.840892Z","submitted_at":"2025-05-09T19:03:38Z","title":"Probing Weak-Force Corrections to Black Hole Geometry via Long Range Potentials: Feinberg-Sucher and Ferrer-Nowakowski Potentials"},"reference_resolution":{"displayed":100,"state_counts":{"malformed_identifier":0,"metadata_mismatch":1,"parse_uncertain":0,"unresolved":80,"verified_exact":19,"verified_fuzzy":0},"total_outbound_references":108},"refusal":"A citation records a reference. It does not transfer a finding from one paper to another.","schema":"pith.paper-citation-record.v1","standing_sources":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"thesis":"As of 16 August 2026, this Paper Citation Record lists 100 of 108 outbound references and 0 inbound Pith citation observations for arXiv:2505.06382."}