{"as_of":"2026-08-16T08:12:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:76cc41f1fbc6e1a2fff1cb78fee703288c9751da3b96588c339ef47e9cd89ac4","coverage":[{"denominator":67,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":67,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-14T13:38:02.173264Z","state":"measured"},{"denominator":67,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":67,"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/1908.04961/citation-record","integrity":"/paper/1908.04961/integrity","json":"/paper/1908.04961/citation-record.json","paper":"/paper/1908.04961"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T13:38:03.681162Z","title":"(14), we ﬁnd the same solution for the potential as in [29],i.e., (dV dφ )2 = 3µ4V , (34) V = 3µ4 4 (φ−V0)2 , (35) and it is then seen that the entire system is consistent","venue":null,"work_id":"f4976f33-e655-4f2e-bce5-b1463a9a1c2f","year":null},"citing_paper":{"arxiv_id":"1908.04961","last_updated":"2019-08-15T16:41:53Z","snapshot_observed_at":"2026-08-16T03:37:35.803409Z","submitted_at":"2019-08-14T05:23:32Z","title":"Charged cosmological black holes: a thorough study of a family of solutions","version":2},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-14T13:38:01.847757Z"},"links":{"citing_paper":"/paper/1908.04961"},"observation_digest":"sha256:fc7e9db38345c00e15cfd42384f03d646e0ed76bb3eaefaccb45a2af5957155a","observation_id":"562beb12-b43f-41ec-9073-612dec94b274","resolution":{"observed_at":"2026-08-14T13:38:03.686109Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"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":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T13:38:03.666424Z","title":"Hence, considering that the isotropic coordinate is real, the domain of the areal radius coordi- nateR should be restricted to the intervalsR+≤R< ∞ and 0≤R≤R−","venue":null,"work_id":"6b562d99-8130-450a-a3da-c8ed04ea0666","year":null},"citing_paper":{"arxiv_id":"1908.04961","last_updated":"2019-08-15T16:41:53Z","snapshot_observed_at":"2026-08-16T03:37:35.803409Z","submitted_at":"2019-08-14T05:23:32Z","title":"Charged cosmological black holes: a thorough study of a family of solutions","version":2},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-14T13:38:01.853278Z"},"links":{"citing_paper":"/paper/1908.04961"},"observation_digest":"sha256:68d8505f90307c2ed4a2a7b31004fdcdc871790989c80e610b8744e1f80092d4","observation_id":"c59d24ae-872e-4038-b08b-08472b093cbc","resolution":{"observed_at":"2026-08-14T13:38:03.671212Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"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":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T13:38:03.652191Z","title":"We then conclude that, form2 =q2, theisotropiccoordinate r covers(once) all the range ofR","venue":null,"work_id":"d4b63606-e497-4311-b726-dd6a586bc985","year":null},"citing_paper":{"arxiv_id":"1908.04961","last_updated":"2019-08-15T16:41:53Z","snapshot_observed_at":"2026-08-16T03:37:35.803409Z","submitted_at":"2019-08-14T05:23:32Z","title":"Charged cosmological black holes: a thorough study of a family of solutions","version":2},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-14T13:38:01.859068Z"},"links":{"citing_paper":"/paper/1908.04961"},"observation_digest":"sha256:c8e70ee0e252880d7cfaac003a269118dc98e5ed9143d33d11b2e4af457d7e43","observation_id":"e1738693-9660-4ffa-b812-b081d58c3fe6","resolution":{"observed_at":"2026-08-14T13:38:03.656894Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"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":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T13:38:03.637817Z","title":"Therefore, form2 <q 2, the isotropic coordinate r covers (twice) all the range ofR","venue":null,"work_id":"71825cb0-d693-4539-9aed-f528df3ae9f6","year":null},"citing_paper":{"arxiv_id":"1908.04961","last_updated":"2019-08-15T16:41:53Z","snapshot_observed_at":"2026-08-16T03:37:35.803409Z","submitted_at":"2019-08-14T05:23:32Z","title":"Charged cosmological black holes: a thorough study of a family of solutions","version":2},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-14T13:38:01.863951Z"},"links":{"citing_paper":"/paper/1908.04961"},"observation_digest":"sha256:5c95984ce7124346a8c85242ac4ae8e2dbf4b272f7dc54cd8669c4b9f0ceb2ae","observation_id":"bcbbc0eb-632d-41e2-ac99-6ef98974f09c","resolution":{"observed_at":"2026-08-14T13:38:03.642494Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"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":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T13:38:03.622587Z","title":"(36) and (39)] for which the a(t)r→ 0 limit corresponds toR→∞ , whileR = 0 cor- responds to a(t)r = (−m±|q|)/2, where the isotropic coordinater is allowed to assume negative values","venue":null,"work_id":"dfa8e508-bd28-4de1-9162-0bb5003a08ce","year":null},"citing_paper":{"arxiv_id":"1908.04961","last_updated":"2019-08-15T16:41:53Z","snapshot_observed_at":"2026-08-16T03:37:35.803409Z","submitted_at":"2019-08-14T05:23:32Z","title":"Charged cosmological black holes: a thorough study of a family of solutions","version":2},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-14T13:38:01.869196Z"},"links":{"citing_paper":"/paper/1908.04961"},"observation_digest":"sha256:cedf0c5bcd6de490efb625fb529719e814586610b9751d86ebe21f32cc979b57","observation_id":"36660726-d1e7-4113-b52f-426e5f303ea6","resolution":{"observed_at":"2026-08-14T13:38:03.628129Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"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":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T13:38:03.608709Z","title":"First of all, Eq","venue":null,"work_id":"521806f4-9c0d-4d9a-aaab-a3d2cb845dc7","year":null},"citing_paper":{"arxiv_id":"1908.04961","last_updated":"2019-08-15T16:41:53Z","snapshot_observed_at":"2026-08-16T03:37:35.803409Z","submitted_at":"2019-08-14T05:23:32Z","title":"Charged cosmological black holes: a thorough study of a family of solutions","version":2},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-14T13:38:01.874061Z"},"links":{"citing_paper":"/paper/1908.04961"},"observation_digest":"sha256:41c44f0c598eb51e96cd2bccd019a5f5e65cd09fb5c652246969f2385de293cb","observation_id":"4e378244-e652-4c80-be2a-0b41ff2cb717","resolution":{"observed_at":"2026-08-14T13:38:03.613131Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"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":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T13:38:03.594114Z","title":"The spacetime de- scribed by the overcharged SV metric includes all the range of the radial coordinate0<R< ∞and is bounded by a singular timelike surface atR = 0","venue":null,"work_id":"b2b8d37d-6e87-4bf6-80c9-963ee812d26c","year":null},"citing_paper":{"arxiv_id":"1908.04961","last_updated":"2019-08-15T16:41:53Z","snapshot_observed_at":"2026-08-16T03:37:35.803409Z","submitted_at":"2019-08-14T05:23:32Z","title":"Charged cosmological black holes: a thorough study of a family of solutions","version":2},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-14T13:38:01.879461Z"},"links":{"citing_paper":"/paper/1908.04961"},"observation_digest":"sha256:cc325ae61f2946336dd4ee12406b2de400b14a11312ecf0f1ceec81c0824dd83","observation_id":"f0be2620-5bb3-41f7-a5dd-a7800134fd76","resolution":{"observed_at":"2026-08-14T13:38:03.599129Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"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":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T13:38:03.579028Z","title":null,"venue":null,"work_id":"ced036d5-9896-4321-80c1-e9ab1c2fef73","year":null},"citing_paper":{"arxiv_id":"1908.04961","last_updated":"2019-08-15T16:41:53Z","snapshot_observed_at":"2026-08-16T03:37:35.803409Z","submitted_at":"2019-08-14T05:23:32Z","title":"Charged cosmological black holes: a thorough study of a family of solutions","version":2},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-14T13:38:01.884305Z"},"links":{"citing_paper":"/paper/1908.04961"},"observation_digest":"sha256:d99815dfbe079a66f6474cab8c47edc1483c6c7e8189691586dfe0236b8b8c10","observation_id":"3e09c21e-e1e4-4eb0-8efe-d9d7142678cb","resolution":{"observed_at":"2026-08-14T13:38:03.583668Z","resolver_source":"raw_fallback","status":"unresolved"},"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":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T13:38:03.564136Z","title":"In this case, theAHscorrespondtorootsofthetwosecond-order polynomials, HR 2 +R−m = 0, HR 2−R +m = 0, (49) which can be easily computed","venue":null,"work_id":"ebc02237-891f-4203-8936-5d0b7534a60e","year":null},"citing_paper":{"arxiv_id":"1908.04961","last_updated":"2019-08-15T16:41:53Z","snapshot_observed_at":"2026-08-16T03:37:35.803409Z","submitted_at":"2019-08-14T05:23:32Z","title":"Charged cosmological black holes: a thorough study of a family of solutions","version":2},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-14T13:38:01.889052Z"},"links":{"citing_paper":"/paper/1908.04961"},"observation_digest":"sha256:e44b5c951fc1fce569107049f4257df3b1f1d3199b79015b5a9e4c96e982792a","observation_id":"a29c56af-adf2-4c5c-a601-b77ee4635a4b","resolution":{"observed_at":"2026-08-14T13:38:03.569209Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"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":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T13:38:03.549480Z","title":"It is bounded from below by the lineσ2 = 1, from above by the curve forσ2 c+, and from the right by the curve for σ2 c−","venue":null,"work_id":"c413969d-e481-4918-a114-c6a4d735c357","year":null},"citing_paper":{"arxiv_id":"1908.04961","last_updated":"2019-08-15T16:41:53Z","snapshot_observed_at":"2026-08-16T03:37:35.803409Z","submitted_at":"2019-08-14T05:23:32Z","title":"Charged cosmological black holes: a thorough study of a family of solutions","version":2},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-14T13:38:01.893570Z"},"links":{"citing_paper":"/paper/1908.04961"},"observation_digest":"sha256:ae8e54dcee3bbe34195bc7fd8abbc14b5c5048f7f5704c1f6b2ce7c8de6fa128","observation_id":"518269d5-868b-4eb9-ac61-f99acda1d1b2","resolution":{"observed_at":"2026-08-14T13:38:03.554516Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"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":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T13:38:03.535227Z","title":"An analysis of the roots of Eq","venue":null,"work_id":"ed7bf981-8355-45f0-9b92-7d619477d551","year":null},"citing_paper":{"arxiv_id":"1908.04961","last_updated":"2019-08-15T16:41:53Z","snapshot_observed_at":"2026-08-16T03:37:35.803409Z","submitted_at":"2019-08-14T05:23:32Z","title":"Charged cosmological black holes: a thorough study of a family of solutions","version":2},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-14T13:38:01.898284Z"},"links":{"citing_paper":"/paper/1908.04961"},"observation_digest":"sha256:729816c6c50ec9642099f65bdc6480caabb51220c26bc873b6b9925e8e3ac63a","observation_id":"dcc0a6b4-a692-48bf-be9c-7211360a5ee4","resolution":{"observed_at":"2026-08-14T13:38:03.539719Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"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":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T13:38:03.520416Z","title":null,"venue":null,"work_id":"120b703a-3d43-439f-8976-8afee04330cd","year":null},"citing_paper":{"arxiv_id":"1908.04961","last_updated":"2019-08-15T16:41:53Z","snapshot_observed_at":"2026-08-16T03:37:35.803409Z","submitted_at":"2019-08-14T05:23:32Z","title":"Charged cosmological black holes: a thorough study of a family of solutions","version":2},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-14T13:38:01.903132Z"},"links":{"citing_paper":"/paper/1908.04961"},"observation_digest":"sha256:e5f7212d6702086cbad10ec77d3b55fe2558045297fa373a5682c34b12ff5969","observation_id":"1eb20afb-5c92-4ec9-b748-a4ba8fd5e974","resolution":{"observed_at":"2026-08-14T13:38:03.525539Z","resolver_source":"raw_fallback","status":"unresolved"},"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":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T13:38:03.505737Z","title":"Analogously, if there existsδ >0 such that Fδ +(ti,t ) = ∫ t ti e(B+δ)u∆H(u) du, (71) converges ast→∞ , then a black-hole/white-hole pair is present","venue":null,"work_id":"55114b94-2508-4d52-89f5-a65a00f13306","year":null},"citing_paper":{"arxiv_id":"1908.04961","last_updated":"2019-08-15T16:41:53Z","snapshot_observed_at":"2026-08-16T03:37:35.803409Z","submitted_at":"2019-08-14T05:23:32Z","title":"Charged cosmological black holes: a thorough study of a family of solutions","version":2},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-14T13:38:01.907706Z"},"links":{"citing_paper":"/paper/1908.04961"},"observation_digest":"sha256:58d9306de08b9016f0c5a6d6ad4365ec4fc829d028bd583774ec8f6538160bfa","observation_id":"2b8ca0ed-3db9-4023-91d9-5af01e261adb","resolution":{"observed_at":"2026-08-14T13:38:03.510949Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"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":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T13:38:03.490522Z","title":null,"venue":null,"work_id":"b1e4db7a-4af8-40ca-8897-41fa7ab14b4d","year":null},"citing_paper":{"arxiv_id":"1908.04961","last_updated":"2019-08-15T16:41:53Z","snapshot_observed_at":"2026-08-16T03:37:35.803409Z","submitted_at":"2019-08-14T05:23:32Z","title":"Charged cosmological black holes: a thorough study of a family of solutions","version":2},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-14T13:38:01.912164Z"},"links":{"citing_paper":"/paper/1908.04961"},"observation_digest":"sha256:6a9541f48244e4cc10be3fc0e124e6c5351a5a2e50f0bfce621e2bf6b50c75d5","observation_id":"c35703fe-358d-4b90-bb5f-499d64afaa6f","resolution":{"observed_at":"2026-08-14T13:38:03.495159Z","resolver_source":"raw_fallback","status":"unresolved"},"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":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T13:38:03.474828Z","title":"In spacetimes represented by Region II there is no AH, and the patch covered by the coordinates is anti-trapped everywhere, therefore there is no doubt about the causal structure","venue":null,"work_id":"c8af277d-c308-4f82-8957-95a43fe5a20a","year":null},"citing_paper":{"arxiv_id":"1908.04961","last_updated":"2019-08-15T16:41:53Z","snapshot_observed_at":"2026-08-16T03:37:35.803409Z","submitted_at":"2019-08-14T05:23:32Z","title":"Charged cosmological black holes: a thorough study of a family of solutions","version":2},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-14T13:38:01.916580Z"},"links":{"citing_paper":"/paper/1908.04961"},"observation_digest":"sha256:af1e692ad83bc938f41e6ad4811c9db7163c89f30b897cdd1efff652f543ce20","observation_id":"40b4ee97-6288-42b9-a872-012c41968f2a","resolution":{"observed_at":"2026-08-14T13:38:03.480287Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"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":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T13:38:03.457683Z","title":"Following the reasoning of Sec","venue":null,"work_id":"e855baf0-91e1-4017-b355-239ba6bd7801","year":null},"citing_paper":{"arxiv_id":"1908.04961","last_updated":"2019-08-15T16:41:53Z","snapshot_observed_at":"2026-08-16T03:37:35.803409Z","submitted_at":"2019-08-14T05:23:32Z","title":"Charged cosmological black holes: a thorough study of a family of solutions","version":2},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-14T13:38:01.921371Z"},"links":{"citing_paper":"/paper/1908.04961"},"observation_digest":"sha256:db144c21c15a4feba20b74090fd14f4b87dd294dcd842827110918053bf9b280","observation_id":"554d9f7f-1af6-4267-adb2-236fd101442f","resolution":{"observed_at":"2026-08-14T13:38:03.462927Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"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":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T13:38:03.442327Z","title":"2, represents an undercharged case with q < mand small mH0","venue":null,"work_id":"4d320e8d-97c4-4267-8719-13c04d765f4a","year":null},"citing_paper":{"arxiv_id":"1908.04961","last_updated":"2019-08-15T16:41:53Z","snapshot_observed_at":"2026-08-16T03:37:35.803409Z","submitted_at":"2019-08-14T05:23:32Z","title":"Charged cosmological black holes: a thorough study of a family of solutions","version":2},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-14T13:38:01.926488Z"},"links":{"citing_paper":"/paper/1908.04961"},"observation_digest":"sha256:c366341eea5447423c57f989baf9c72243c724ba7c9b01667b6699e3d3e772c9","observation_id":"0cb675d2-2279-4262-9488-cad3d0fc0739","resolution":{"observed_at":"2026-08-14T13:38:03.447603Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"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":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T13:38:03.426340Z","title":"The singularity at R = m +√ m2−q2 is still present, however no AH is formed and the singularity is naked, as can be seen in Fig","venue":null,"work_id":"e1cbacfd-ecbd-474a-8dc4-fa589e35e017","year":null},"citing_paper":{"arxiv_id":"1908.04961","last_updated":"2019-08-15T16:41:53Z","snapshot_observed_at":"2026-08-16T03:37:35.803409Z","submitted_at":"2019-08-14T05:23:32Z","title":"Charged cosmological black holes: a thorough study of a family of solutions","version":2},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-14T13:38:01.931431Z"},"links":{"citing_paper":"/paper/1908.04961"},"observation_digest":"sha256:623fb221b637c57fba1600af58ed5f4ee629a8b19d33cba58b665d3b092f0127","observation_id":"51a55c35-cf63-497f-ba49-1b0b45b275f0","resolution":{"observed_at":"2026-08-14T13:38:03.431841Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"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":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T13:38:03.410799Z","title":"They present three AHs, a singularity at 14 R = 0 and an initial singularity att = 0, as shown in Fig","venue":null,"work_id":"c46c8706-088b-433d-80f4-c1b5960442be","year":null},"citing_paper":{"arxiv_id":"1908.04961","last_updated":"2019-08-15T16:41:53Z","snapshot_observed_at":"2026-08-16T03:37:35.803409Z","submitted_at":"2019-08-14T05:23:32Z","title":"Charged cosmological black holes: a thorough study of a family of solutions","version":2},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-14T13:38:01.936231Z"},"links":{"citing_paper":"/paper/1908.04961"},"observation_digest":"sha256:96ad84e116fff6531fca899863c78fa4ff887e4a484400bc3380c9a13cfe1e61","observation_id":"feaee9cc-fd0c-4675-ad8a-9a2ff72a870c","resolution":{"observed_at":"2026-08-14T13:38:03.415883Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"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":"8881.06499","doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T13:38:03.113287Z","title":"The Cauchy surface is not present either, as it can be seen in Fig","venue":null,"work_id":"87072fc8-6ecb-4601-9478-633a04f6fbf7","year":2014},"citing_paper":{"arxiv_id":"1908.04961","last_updated":"2019-08-15T16:41:53Z","snapshot_observed_at":"2026-08-16T03:37:35.803409Z","submitted_at":"2019-08-14T05:23:32Z","title":"Charged cosmological black holes: a thorough study of a family of solutions","version":2},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-14T13:38:01.940896Z"},"links":{"citing_paper":"/paper/1908.04961"},"observation_digest":"sha256:f1dbaa030ab5c10bceb43f08d2526f38f2355e55362b3aeab9728349b14164cf","observation_id":"86bdaf21-dc1c-43cf-8d86-2f6fbcf93193","resolution":{"observed_at":"2026-08-14T13:38:03.121036Z","resolver_source":"raw_fallback","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":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T13:38:03.395605Z","title":null,"venue":null,"work_id":"b783e937-a103-44a8-ba74-17f672a24106","year":2017},"citing_paper":{"arxiv_id":"1908.04961","last_updated":"2019-08-15T16:41:53Z","snapshot_observed_at":"2026-08-16T03:37:35.803409Z","submitted_at":"2019-08-14T05:23:32Z","title":"Charged cosmological black holes: a thorough study of a family of solutions","version":2},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-14T13:38:01.945765Z"},"links":{"citing_paper":"/paper/1908.04961"},"observation_digest":"sha256:de73eed993e0bb640ba2aec42b935b8c6e3cc1a1c214158aaf940c30f6e04da9","observation_id":"022bd807-569c-49c3-8455-c4a1e9109905","resolution":{"observed_at":"2026-08-14T13:38:03.400625Z","resolver_source":"raw_fallback","status":"unresolved"},"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":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T13:38:03.379061Z","title":"This case correspondstotheverticalaxisinFig.1, andtheSVmet- ric (37) asymptotes to the Reissner–Nordström metric at large times","venue":null,"work_id":"e998fbf3-2291-4061-9998-6fe7c0a11220","year":null},"citing_paper":{"arxiv_id":"1908.04961","last_updated":"2019-08-15T16:41:53Z","snapshot_observed_at":"2026-08-16T03:37:35.803409Z","submitted_at":"2019-08-14T05:23:32Z","title":"Charged cosmological black holes: a thorough study of a family of solutions","version":2},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-14T13:38:01.950506Z"},"links":{"citing_paper":"/paper/1908.04961"},"observation_digest":"sha256:4da3a2d43d621e21d80f93016cbfa81cf9e52b5093abba3744052a21b83221f2","observation_id":"d7577cbe-cd50-4028-9b45-266fe1117844","resolution":{"observed_at":"2026-08-14T13:38:03.384972Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"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":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T13:38:03.363175Z","title":"The ﬁrst case, for values ofm2 > q2, presents two apparent horizons R+ and R− and an initial singular- ity atS+","venue":null,"work_id":"20843432-5a26-4f58-9c62-9a68ef477f92","year":null},"citing_paper":{"arxiv_id":"1908.04961","last_updated":"2019-08-15T16:41:53Z","snapshot_observed_at":"2026-08-16T03:37:35.803409Z","submitted_at":"2019-08-14T05:23:32Z","title":"Charged cosmological black holes: a thorough study of a family of solutions","version":2},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-14T13:38:01.955032Z"},"links":{"citing_paper":"/paper/1908.04961"},"observation_digest":"sha256:2e9860099bba2d17e9ce8a2426309335a9e9907321bc1d31e2fa13fbb281518c","observation_id":"00a8eba1-1591-4fdd-b37f-a07f41841a5f","resolution":{"observed_at":"2026-08-14T13:38:03.368742Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"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":"1606.04855","last_updated":"2016-06-15T16:44:04Z","snapshot_observed_at":"2026-08-14T21:52:35.855236Z","submitted_at":"2016-06-15T16:44:04Z","title":"GW151226: Observation of Gravitational Waves from a 22-Solar-Mass Binary Black Hole Coalescence","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1606.04855","snapshot_observed_at":"2026-08-14T13:38:01.959861Z","title":null,"venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"1908.04961","last_updated":"2019-08-15T16:41:53Z","snapshot_observed_at":"2026-08-16T03:37:35.803409Z","submitted_at":"2019-08-14T05:23:32Z","title":"Charged cosmological black holes: a thorough study of a family of solutions","version":2},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-14T13:38:01.959861Z"},"links":{"cited_paper":"/paper/1606.04855","citing_paper":"/paper/1908.04961"},"observation_digest":"sha256:7bd34ac8c59fc3507b0b2826bd10c62a624321388d0d6df1c972f3b8c849c6a4","observation_id":"fb664ad0-12ee-4810-a31a-5ea1c186c061","resolution":{"observed_at":"2026-08-14T13:38:01.959861Z","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":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T13:38:03.348717Z","title":"Akiyamaet al","venue":null,"work_id":"4f7e7b18-6693-4dc1-a174-b37169783458","year":2019},"citing_paper":{"arxiv_id":"1908.04961","last_updated":"2019-08-15T16:41:53Z","snapshot_observed_at":"2026-08-16T03:37:35.803409Z","submitted_at":"2019-08-14T05:23:32Z","title":"Charged cosmological black holes: a thorough study of a family of solutions","version":2},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-14T13:38:01.965008Z"},"links":{"citing_paper":"/paper/1908.04961"},"observation_digest":"sha256:898ddf4630faee51fb61558ba2b8c930ac059e78a25078e86d253d60c7248fc1","observation_id":"a6b61b3d-1c8b-4965-916c-c486148f0db3","resolution":{"observed_at":"2026-08-14T13:38:03.353303Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"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":"1501.06570","last_updated":"2021-01-08T08:19:41Z","snapshot_observed_at":"2026-08-11T07:07:02.101103Z","submitted_at":"2015-01-26T21:00:09Z","title":"Superradiance -- the 2020 Edition","version":8},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1501.06570","snapshot_observed_at":"2026-08-14T13:38:01.969881Z","title":"Carlip, Int","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"1908.04961","last_updated":"2019-08-15T16:41:53Z","snapshot_observed_at":"2026-08-16T03:37:35.803409Z","submitted_at":"2019-08-14T05:23:32Z","title":"Charged cosmological black holes: a thorough study of a family of solutions","version":2},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-14T13:38:01.969881Z"},"links":{"cited_paper":"/paper/1501.06570","citing_paper":"/paper/1908.04961"},"observation_digest":"sha256:d3ff060c97ee02a5c9f414aa177e900868d7f6be9a8196fcfd01fcd334ea1561","observation_id":"41eb5fb4-4e58-4dbf-83cc-801b2105f360","resolution":{"observed_at":"2026-08-14T13:38:01.969881Z","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":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T13:38:03.332999Z","title":null,"venue":null,"work_id":"b2203023-67b9-4e63-a9db-848706821427","year":1981},"citing_paper":{"arxiv_id":"1908.04961","last_updated":"2019-08-15T16:41:53Z","snapshot_observed_at":"2026-08-16T03:37:35.803409Z","submitted_at":"2019-08-14T05:23:32Z","title":"Charged cosmological black holes: a thorough study of a family of solutions","version":2},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-14T13:38:01.975180Z"},"links":{"citing_paper":"/paper/1908.04961"},"observation_digest":"sha256:ddc0c2241b6fbb4d78802a08fd9811f3dd1fd924172f07b7b53de3e6770c1cc1","observation_id":"b59039c7-09be-4fc2-b9b8-5816ec2d9c94","resolution":{"observed_at":"2026-08-14T13:38:03.337828Z","resolver_source":"raw_fallback","status":"unresolved"},"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":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T13:38:03.318678Z","title":null,"venue":null,"work_id":"412c8e31-ac39-4ab0-bf3c-4fc76ec8bc29","year":2006},"citing_paper":{"arxiv_id":"1908.04961","last_updated":"2019-08-15T16:41:53Z","snapshot_observed_at":"2026-08-16T03:37:35.803409Z","submitted_at":"2019-08-14T05:23:32Z","title":"Charged cosmological black holes: a thorough study of a family of solutions","version":2},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-14T13:38:01.980379Z"},"links":{"citing_paper":"/paper/1908.04961"},"observation_digest":"sha256:aec0ed7f12e843b75ea66842dab59d0e88366efd424ac64ec7faa223ef8bc91b","observation_id":"2fc98a25-c284-41ed-904f-7ba00d99ea81","resolution":{"observed_at":"2026-08-14T13:38:03.323136Z","resolver_source":"raw_fallback","status":"unresolved"},"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":"1309.4915","last_updated":"2013-09-19T09:52:03Z","snapshot_observed_at":"2026-08-15T00:02:36.792572Z","submitted_at":"2013-09-19T09:52:03Z","title":"Evolving black hole horizons in General Relativity and alternative gravity","version":1},"cited_work":{"arxiv_id":"1309.4915","doi":null,"metadata_source":"pith","pith_arxiv_id":"1309.4915","snapshot_observed_at":"2026-08-14T13:38:02.844136Z","title":"Evolving black hole horizons in General Relativity and alternative gravity","venue":"gr-qc","work_id":"aaf22d81-e516-48f1-9988-906be71bfb64","year":2013},"citing_paper":{"arxiv_id":"1908.04961","last_updated":"2019-08-15T16:41:53Z","snapshot_observed_at":"2026-08-16T03:37:35.803409Z","submitted_at":"2019-08-14T05:23:32Z","title":"Charged cosmological black holes: a thorough study of a family of solutions","version":2},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-14T13:38:01.985554Z"},"links":{"cited_paper":"/paper/1309.4915","citing_paper":"/paper/1908.04961"},"observation_digest":"sha256:9148ae1f4b449bbd3e1aa3e80ed51e9cc5e612a7283a0de7316ac84ad649124e","observation_id":"b9dd6e21-11d9-4f92-82be-3bcef932db24","resolution":{"observed_at":"2026-08-14T13:38:02.849335Z","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":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T13:38:03.303265Z","title":null,"venue":null,"work_id":"cb0aa5e0-712f-40e2-b89c-e4598c0dc19f","year":1932},"citing_paper":{"arxiv_id":"1908.04961","last_updated":"2019-08-15T16:41:53Z","snapshot_observed_at":"2026-08-16T03:37:35.803409Z","submitted_at":"2019-08-14T05:23:32Z","title":"Charged cosmological black holes: a thorough study of a family of solutions","version":2},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-14T13:38:01.990640Z"},"links":{"citing_paper":"/paper/1908.04961"},"observation_digest":"sha256:ac598c43ca8451fc830291a616a614c3c3fbe00356767f2f669e8ae64bd4191b","observation_id":"21da5c37-df2c-4d26-8eec-5d11ee4511ac","resolution":{"observed_at":"2026-08-14T13:38:03.308210Z","resolver_source":"raw_fallback","status":"unresolved"},"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":"2026-08-14T13:38:01.995192Z","title":null,"venue":null,"work_id":null,"year":1994},"citing_paper":{"arxiv_id":"1908.04961","last_updated":"2019-08-15T16:41:53Z","snapshot_observed_at":"2026-08-16T03:37:35.803409Z","submitted_at":"2019-08-14T05:23:32Z","title":"Charged cosmological black holes: a thorough study of a family of solutions","version":2},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-08-14T13:38:01.995192Z"},"links":{"citing_paper":"/paper/1908.04961"},"observation_digest":"sha256:9bd78b01db3e577d98413194335cef165e74bd8abb5029ad616d5924eb1c0b27","observation_id":"e0b222a0-733a-47d1-aecf-b31ab2d9a7cc","resolution":{"observed_at":"2026-08-14T13:38:01.995192Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1107.1344","last_updated":"2011-09-14T14:53:38Z","snapshot_observed_at":"2026-08-15T16:23:57.285990Z","submitted_at":"2011-07-07T11:09:30Z","title":"Trapped surfaces","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1107.1344","snapshot_observed_at":"2026-08-14T13:38:01.999667Z","title":null,"venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"1908.04961","last_updated":"2019-08-15T16:41:53Z","snapshot_observed_at":"2026-08-16T03:37:35.803409Z","submitted_at":"2019-08-14T05:23:32Z","title":"Charged cosmological black holes: a thorough study of a family of solutions","version":2},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-14T13:38:01.999667Z"},"links":{"cited_paper":"/paper/1107.1344","citing_paper":"/paper/1908.04961"},"observation_digest":"sha256:7e415b9bc006b6f3a8886f8b8148587d1e131b9cfcf79b27770c6ea659f63576","observation_id":"212535a2-4ab0-4bc4-a204-2f72462700f1","resolution":{"observed_at":"2026-08-14T13:38:01.999667Z","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":"2026-08-14T13:38:02.004662Z","title":null,"venue":null,"work_id":null,"year":1998},"citing_paper":{"arxiv_id":"1908.04961","last_updated":"2019-08-15T16:41:53Z","snapshot_observed_at":"2026-08-16T03:37:35.803409Z","submitted_at":"2019-08-14T05:23:32Z","title":"Charged cosmological black holes: a thorough study of a family of solutions","version":2},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-14T13:38:02.004662Z"},"links":{"citing_paper":"/paper/1908.04961"},"observation_digest":"sha256:b92124dec7393e2dad27acdd2d90bdc7b7e13e1b512b291a28fe4b8cd6e08666","observation_id":"a6e8b481-906d-47a3-bc49-3e0eac374e9b","resolution":{"observed_at":"2026-08-14T13:38:02.004662Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0908.3101","last_updated":"2009-08-21T11:25:39Z","snapshot_observed_at":"2026-08-15T05:40:52.262738Z","submitted_at":"2009-08-21T11:25:39Z","title":"On the generalization of McVittie's model for an inhomogeneity in a cosmological spacetime","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0908.3101","snapshot_observed_at":"2026-08-14T13:38:02.009114Z","title":"Carrera and D","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"1908.04961","last_updated":"2019-08-15T16:41:53Z","snapshot_observed_at":"2026-08-16T03:37:35.803409Z","submitted_at":"2019-08-14T05:23:32Z","title":"Charged cosmological black holes: a thorough study of a family of solutions","version":2},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-14T13:38:02.009114Z"},"links":{"cited_paper":"/paper/0908.3101","citing_paper":"/paper/1908.04961"},"observation_digest":"sha256:0c3a96ec6863ac29d6d5a0c84d9f9645dfb15e6a4aa22a8c43cc8353d8ac6db4","observation_id":"f9a872c8-e9de-480f-bc22-988e192bda5a","resolution":{"observed_at":"2026-08-14T13:38:02.009114Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1003.4777","last_updated":"2010-07-28T16:03:39Z","snapshot_observed_at":"2026-08-15T05:23:22.613717Z","submitted_at":"2010-03-24T23:49:48Z","title":"McVittie's Legacy: Black Holes in an Expanding Universe","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1003.4777","snapshot_observed_at":"2026-08-14T13:38:02.014463Z","title":"Kaloper, M","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"1908.04961","last_updated":"2019-08-15T16:41:53Z","snapshot_observed_at":"2026-08-16T03:37:35.803409Z","submitted_at":"2019-08-14T05:23:32Z","title":"Charged cosmological black holes: a thorough study of a family of solutions","version":2},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-14T13:38:02.014463Z"},"links":{"cited_paper":"/paper/1003.4777","citing_paper":"/paper/1908.04961"},"observation_digest":"sha256:7822597408bbf1355bde9be529d0816111a6c2f669deae2661513303c27f328d","observation_id":"f67f3857-8d1d-4d72-bb07-94073ce55ded","resolution":{"observed_at":"2026-08-14T13:38:02.014463Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1106.3666","last_updated":"2011-07-29T18:25:56Z","snapshot_observed_at":"2026-08-15T04:43:33.731941Z","submitted_at":"2011-06-18T16:07:03Z","title":"More on McVittie's Legacy: A Schwarzschild - de Sitter black and white hole embedded in an asymptotically $\\Lambda$CDM cosmology","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1106.3666","snapshot_observed_at":"2026-08-14T13:38:02.019741Z","title":"Lake and M","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"1908.04961","last_updated":"2019-08-15T16:41:53Z","snapshot_observed_at":"2026-08-16T03:37:35.803409Z","submitted_at":"2019-08-14T05:23:32Z","title":"Charged cosmological black holes: a thorough study of a family of solutions","version":2},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-14T13:38:02.019741Z"},"links":{"cited_paper":"/paper/1106.3666","citing_paper":"/paper/1908.04961"},"observation_digest":"sha256:16d83cb80a004d7553d89f56d142b119f6d8e6d1990ba2711a69c43d92dbe555","observation_id":"c8b90be0-ceff-4295-a57a-3cefb052ed0c","resolution":{"observed_at":"2026-08-14T13:38:02.019741Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1212.0155","last_updated":"2013-03-27T13:05:40Z","snapshot_observed_at":"2026-08-15T00:37:27.390554Z","submitted_at":"2012-12-01T20:31:37Z","title":"How the expansion of the universe determines the causal structure of McVittie spacetimes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1212.0155","snapshot_observed_at":"2026-08-14T13:38:02.025008Z","title":"daSilva, M","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"1908.04961","last_updated":"2019-08-15T16:41:53Z","snapshot_observed_at":"2026-08-16T03:37:35.803409Z","submitted_at":"2019-08-14T05:23:32Z","title":"Charged cosmological black holes: a thorough study of a family of solutions","version":2},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-14T13:38:02.025008Z"},"links":{"cited_paper":"/paper/1212.0155","citing_paper":"/paper/1908.04961"},"observation_digest":"sha256:64000ab9b5521b7fdeed4fd4939256c64773e28f52e5ed98c69638fb1dc6c5dd","observation_id":"78384d07-4f57-4e87-b934-caf7ea17169a","resolution":{"observed_at":"2026-08-14T13:38:02.025008Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1207.6350","last_updated":"2012-09-04T19:45:43Z","snapshot_observed_at":"2026-08-15T00:51:57.350861Z","submitted_at":"2012-07-26T17:51:44Z","title":"The McVittie solution with a negative cosmological constant","version":3},"cited_work":{"arxiv_id":"1207.6350","doi":null,"metadata_source":"pith","pith_arxiv_id":"1207.6350","snapshot_observed_at":"2026-08-14T13:38:02.570274Z","title":"The McVittie solution with a negative cosmological constant","venue":"gr-qc","work_id":"1ec29628-f558-43ef-a489-167366e224ba","year":2012},"citing_paper":{"arxiv_id":"1908.04961","last_updated":"2019-08-15T16:41:53Z","snapshot_observed_at":"2026-08-16T03:37:35.803409Z","submitted_at":"2019-08-14T05:23:32Z","title":"Charged cosmological black holes: a thorough study of a family of solutions","version":2},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-14T13:38:02.030250Z"},"links":{"cited_paper":"/paper/1207.6350","citing_paper":"/paper/1908.04961"},"observation_digest":"sha256:5fa084fa683e6aa2438bc4321ca1402cfaa94e44eddfbc070d7bac76cc7baba3","observation_id":"981b7a63-f90c-4cd9-861a-40c1948dc7f1","resolution":{"observed_at":"2026-08-14T13:38:02.575757Z","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":"1202.0719","last_updated":"2012-02-03T14:41:52Z","snapshot_observed_at":"2026-08-15T04:20:22.230723Z","submitted_at":"2012-02-03T14:41:52Z","title":"Making sense of the bizarre behaviour of horizons in the McVittie spacetime","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1202.0719","snapshot_observed_at":"2026-08-14T13:38:02.035418Z","title":"Faraoni, A","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"1908.04961","last_updated":"2019-08-15T16:41:53Z","snapshot_observed_at":"2026-08-16T03:37:35.803409Z","submitted_at":"2019-08-14T05:23:32Z","title":"Charged cosmological black holes: a thorough study of a family of solutions","version":2},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-08-14T13:38:02.035418Z"},"links":{"cited_paper":"/paper/1202.0719","citing_paper":"/paper/1908.04961"},"observation_digest":"sha256:d59f5ea83603266d34b92d444e0c7f082d1549204ec76752b32eb34123f05d97","observation_id":"1d1afaef-e1dc-4826-a00e-90ad43707695","resolution":{"observed_at":"2026-08-14T13:38:02.035418Z","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":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T13:38:03.287674Z","title":"19,191(1968)","venue":null,"work_id":"64311791-001e-42de-bc5d-888d3a30f596","year":1968},"citing_paper":{"arxiv_id":"1908.04961","last_updated":"2019-08-15T16:41:53Z","snapshot_observed_at":"2026-08-16T03:37:35.803409Z","submitted_at":"2019-08-14T05:23:32Z","title":"Charged cosmological black holes: a thorough study of a family of solutions","version":2},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-08-14T13:38:02.040476Z"},"links":{"citing_paper":"/paper/1908.04961"},"observation_digest":"sha256:7150c524a89e49277df4f4c837f568327f8a61631802cbea4f2001140203d512","observation_id":"182a54e3-08ca-4bb6-8880-88fa7dc0da86","resolution":{"observed_at":"2026-08-14T13:38:03.292610Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"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":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T13:38:03.272708Z","title":"Kastor and J","venue":null,"work_id":"af90bb98-9256-4ab0-9a2d-70778058560f","year":1993},"citing_paper":{"arxiv_id":"1908.04961","last_updated":"2019-08-15T16:41:53Z","snapshot_observed_at":"2026-08-16T03:37:35.803409Z","submitted_at":"2019-08-14T05:23:32Z","title":"Charged cosmological black holes: a thorough study of a family of solutions","version":2},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-08-14T13:38:02.045072Z"},"links":{"citing_paper":"/paper/1908.04961"},"observation_digest":"sha256:b88ad3c230dc0324d7f47d5cf830c381b05c5f082699e4624df1cd91a73ae29c","observation_id":"6b08faaf-9bd0-4810-87f6-b06b337acc13","resolution":{"observed_at":"2026-08-14T13:38:03.277479Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"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":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T13:38:03.255539Z","title":null,"venue":null,"work_id":"6ab4349c-7a24-4b22-acea-2c51788e4c53","year":1972},"citing_paper":{"arxiv_id":"1908.04961","last_updated":"2019-08-15T16:41:53Z","snapshot_observed_at":"2026-08-16T03:37:35.803409Z","submitted_at":"2019-08-14T05:23:32Z","title":"Charged cosmological black holes: a thorough study of a family of solutions","version":2},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-08-14T13:38:02.049782Z"},"links":{"citing_paper":"/paper/1908.04961"},"observation_digest":"sha256:610a754216b9d90e2e6c85c2d09dde0d977ac02bd314d0a163911e30be44f6aa","observation_id":"bdebeee8-e67b-4035-bfbb-c465e21f88a9","resolution":{"observed_at":"2026-08-14T13:38:03.261340Z","resolver_source":"raw_fallback","status":"unresolved"},"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":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T13:38:03.238955Z","title":"Nakao, T","venue":null,"work_id":"5d1bac2c-3606-4ca4-9d3b-906a9190f206","year":1995},"citing_paper":{"arxiv_id":"1908.04961","last_updated":"2019-08-15T16:41:53Z","snapshot_observed_at":"2026-08-16T03:37:35.803409Z","submitted_at":"2019-08-14T05:23:32Z","title":"Charged cosmological black holes: a thorough study of a family of solutions","version":2},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-08-14T13:38:02.054772Z"},"links":{"citing_paper":"/paper/1908.04961"},"observation_digest":"sha256:02defa3f9d56657a62c9a37e90f82ba577d4008b4ce7ae860f21c05104bd7070","observation_id":"a9af7940-2af7-421b-8e7a-ade53ee285ea","resolution":{"observed_at":"2026-08-14T13:38:03.243791Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"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":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T13:38:03.223405Z","title":"Chimento and D","venue":null,"work_id":"c2f34c5d-b34a-4429-ac4d-c3be0a23d373","year":2013},"citing_paper":{"arxiv_id":"1908.04961","last_updated":"2019-08-15T16:41:53Z","snapshot_observed_at":"2026-08-16T03:37:35.803409Z","submitted_at":"2019-08-14T05:23:32Z","title":"Charged cosmological black holes: a thorough study of a family of solutions","version":2},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-08-14T13:38:02.059630Z"},"links":{"citing_paper":"/paper/1908.04961"},"observation_digest":"sha256:296d18bc8c93f76871675579d85d93499c054141037e744aede442c6461d4dbb","observation_id":"e9576baa-f481-487d-bd53-92d1522ebcfd","resolution":{"observed_at":"2026-08-14T13:38:03.228745Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"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":"0911.3849","last_updated":"2010-01-12T12:23:24Z","snapshot_observed_at":"2026-08-15T05:33:28.730161Z","submitted_at":"2009-11-19T17:53:49Z","title":"Static Charged Black Hole Solutions in Horava-Lifshitz Gravity","version":2},"cited_work":{"arxiv_id":"0911.3849","doi":null,"metadata_source":"pith","pith_arxiv_id":"0911.3849","snapshot_observed_at":"2026-08-14T13:38:02.531638Z","title":"Static Charged Black Hole Solutions in Horava-Lifshitz Gravity","venue":"hep-th","work_id":"f3397f0e-9f88-483e-bf1e-84482ce076dc","year":2009},"citing_paper":{"arxiv_id":"1908.04961","last_updated":"2019-08-15T16:41:53Z","snapshot_observed_at":"2026-08-16T03:37:35.803409Z","submitted_at":"2019-08-14T05:23:32Z","title":"Charged cosmological black holes: a thorough study of a family of solutions","version":2},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-08-14T13:38:02.064026Z"},"links":{"cited_paper":"/paper/0911.3849","citing_paper":"/paper/1908.04961"},"observation_digest":"sha256:ac32a15231741acef8265ea79e66ddcafdf0d89d0177e2c483277a436c29c407","observation_id":"803130a9-a6da-4ee2-9079-b54c3c43a22b","resolution":{"observed_at":"2026-08-14T13:38:02.536904Z","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":"1404.3929","last_updated":"2014-04-15T14:35:42Z","snapshot_observed_at":"2026-08-14T23:37:27.259013Z","submitted_at":"2014-04-15T14:35:42Z","title":"The charged McVittie spacetime","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1404.3929","snapshot_observed_at":"2026-08-14T13:38:02.069191Z","title":null,"venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"1908.04961","last_updated":"2019-08-15T16:41:53Z","snapshot_observed_at":"2026-08-16T03:37:35.803409Z","submitted_at":"2019-08-14T05:23:32Z","title":"Charged cosmological black holes: a thorough study of a family of solutions","version":2},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-08-14T13:38:02.069191Z"},"links":{"cited_paper":"/paper/1404.3929","citing_paper":"/paper/1908.04961"},"observation_digest":"sha256:dc745332bfadd4688f43374f1f2f790aa77f37019af6d83886d600c8b7a46cfd","observation_id":"9320a9c0-2bc7-4003-9be7-715abef20731","resolution":{"observed_at":"2026-08-14T13:38:02.069191Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1502.00688","last_updated":"2015-05-09T15:02:04Z","snapshot_observed_at":"2026-08-14T23:01:39.789461Z","submitted_at":"2015-02-02T23:53:12Z","title":"Charged black holes in expanding Einstein-de Sitter universes","version":2},"cited_work":{"arxiv_id":"1502.00688","doi":null,"metadata_source":"pith","pith_arxiv_id":"1502.00688","snapshot_observed_at":"2026-08-14T13:38:02.492542Z","title":"Charged black holes in expanding Einstein-de Sitter universes","venue":"gr-qc","work_id":"9e0eebf1-91df-4394-a0df-a277e37cece6","year":2015},"citing_paper":{"arxiv_id":"1908.04961","last_updated":"2019-08-15T16:41:53Z","snapshot_observed_at":"2026-08-16T03:37:35.803409Z","submitted_at":"2019-08-14T05:23:32Z","title":"Charged cosmological black holes: a thorough study of a family of solutions","version":2},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-08-14T13:38:02.074230Z"},"links":{"cited_paper":"/paper/1502.00688","citing_paper":"/paper/1908.04961"},"observation_digest":"sha256:34f5d258f0272f61b4b48b72cb0de3206e70bcb010f19f37b389c5ab1bd9bf9a","observation_id":"f75866a3-e0c8-461e-a719-577e47dc342f","resolution":{"observed_at":"2026-08-14T13:38:02.498195Z","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":"1705.01892","last_updated":"2017-06-30T08:56:55Z","snapshot_observed_at":"2026-08-14T21:02:47.377888Z","submitted_at":"2017-05-04T16:06:21Z","title":"Cosmological Solutions with Charged Black Holes","version":2},"cited_work":{"arxiv_id":"1705.01892","doi":null,"metadata_source":"pith","pith_arxiv_id":"1705.01892","snapshot_observed_at":"2026-08-14T13:38:02.469208Z","title":"Cosmological Solutions with Charged Black Holes","venue":"gr-qc","work_id":"1f36bb23-6817-4cf5-9d78-2eb3f03f0bfd","year":2017},"citing_paper":{"arxiv_id":"1908.04961","last_updated":"2019-08-15T16:41:53Z","snapshot_observed_at":"2026-08-16T03:37:35.803409Z","submitted_at":"2019-08-14T05:23:32Z","title":"Charged cosmological black holes: a thorough study of a family of solutions","version":2},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-08-14T13:38:02.079113Z"},"links":{"cited_paper":"/paper/1705.01892","citing_paper":"/paper/1908.04961"},"observation_digest":"sha256:daf3a72cb0ce42ff2ffbc1ee771e00e1863b659c58b4362a818b0f1f820bdd27","observation_id":"2af3148b-d82e-45fa-a42b-3cdf2a09bac3","resolution":{"observed_at":"2026-08-14T13:38:02.474684Z","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-th/0609150","last_updated":"2007-04-28T01:08:21Z","snapshot_observed_at":"2026-07-07T04:58:32.532377Z","submitted_at":"2006-09-21T21:18:54Z","title":"Cuscuton: A Causal Field Theory with an Infinite Speed of Sound","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-th/0609150","snapshot_observed_at":"2026-08-14T13:38:02.084318Z","title":"Afshordi, D","venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"1908.04961","last_updated":"2019-08-15T16:41:53Z","snapshot_observed_at":"2026-08-16T03:37:35.803409Z","submitted_at":"2019-08-14T05:23:32Z","title":"Charged cosmological black holes: a thorough study of a family of solutions","version":2},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-08-14T13:38:02.084318Z"},"links":{"cited_paper":"/paper/hep-th/0609150","citing_paper":"/paper/1908.04961"},"observation_digest":"sha256:fad7754b921a761a13b046a12261b2d9a8499313e5bd39e02509755b726abc70","observation_id":"745b468c-3c72-45b9-ad2c-aaa1f44094f9","resolution":{"observed_at":"2026-08-14T13:38:02.084318Z","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":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T13:38:03.207614Z","title":null,"venue":null,"work_id":"535ef9ce-8314-477e-85a4-8d089acd105f","year":1987},"citing_paper":{"arxiv_id":"1908.04961","last_updated":"2019-08-15T16:41:53Z","snapshot_observed_at":"2026-08-16T03:37:35.803409Z","submitted_at":"2019-08-14T05:23:32Z","title":"Charged cosmological black holes: a thorough study of a family of solutions","version":2},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-08-14T13:38:02.089948Z"},"links":{"citing_paper":"/paper/1908.04961"},"observation_digest":"sha256:20a0c14db2493876d26e33cfd88a1a82b62b0a5c2d364226368e8491797ba5f2","observation_id":"1e6944b4-6571-4ef9-a003-3af338b32639","resolution":{"observed_at":"2026-08-14T13:38:03.212206Z","resolver_source":"raw_fallback","status":"unresolved"},"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":"gr-qc/0407045","last_updated":"2004-11-17T07:58:14Z","snapshot_observed_at":"2026-08-15T01:02:52.161542Z","submitted_at":"2004-07-13T08:00:07Z","title":"Reissner-Nordstr\\\"om Metric in the Friedman-Robertson-Walker Universe","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"gr-qc/0407045","snapshot_observed_at":"2026-08-14T13:38:02.094732Z","title":null,"venue":null,"work_id":null,"year":2004},"citing_paper":{"arxiv_id":"1908.04961","last_updated":"2019-08-15T16:41:53Z","snapshot_observed_at":"2026-08-16T03:37:35.803409Z","submitted_at":"2019-08-14T05:23:32Z","title":"Charged cosmological black holes: a thorough study of a family of solutions","version":2},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-08-14T13:38:02.094732Z"},"links":{"cited_paper":"/paper/gr-qc/0407045","citing_paper":"/paper/1908.04961"},"observation_digest":"sha256:4318d839f90f9e49ecb1c98521f30b58b36612962158dc362e0b9b3f254729de","observation_id":"7fa81f86-38d2-46b1-a76d-c5ebcf5cf803","resolution":{"observed_at":"2026-08-14T13:38:02.094732Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1312.3682","last_updated":"2014-05-15T13:27:13Z","snapshot_observed_at":"2026-08-14T23:51:49.515291Z","submitted_at":"2013-12-13T00:07:06Z","title":"Cosmological black holes from self-gravitating fields","version":2},"cited_work":{"arxiv_id":"1312.3682","doi":null,"metadata_source":"pith","pith_arxiv_id":"1312.3682","snapshot_observed_at":"2026-08-14T13:38:02.412669Z","title":"Cosmological black holes from self-gravitating fields","venue":"gr-qc","work_id":"91785229-c3e5-420a-884d-575707da4b62","year":2013},"citing_paper":{"arxiv_id":"1908.04961","last_updated":"2019-08-15T16:41:53Z","snapshot_observed_at":"2026-08-16T03:37:35.803409Z","submitted_at":"2019-08-14T05:23:32Z","title":"Charged cosmological black holes: a thorough study of a family of solutions","version":2},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-08-14T13:38:02.099693Z"},"links":{"cited_paper":"/paper/1312.3682","citing_paper":"/paper/1908.04961"},"observation_digest":"sha256:c731346943e092845098c90ab09662c0115ffe2a974bf71e86a2608cbe9b0dff","observation_id":"16a389a1-c4c0-49e3-92f4-19a0bd369790","resolution":{"observed_at":"2026-08-14T13:38:02.418128Z","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":"1703.08226","last_updated":"2017-03-23T20:34:14Z","snapshot_observed_at":"2026-08-14T22:53:57.561960Z","submitted_at":"2017-03-23T20:34:14Z","title":"Hamiltonian analysis of the cuscuton","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1703.08226","snapshot_observed_at":"2026-08-14T13:38:02.104560Z","title":"Gomes and D","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"1908.04961","last_updated":"2019-08-15T16:41:53Z","snapshot_observed_at":"2026-08-16T03:37:35.803409Z","submitted_at":"2019-08-14T05:23:32Z","title":"Charged cosmological black holes: a thorough study of a family of solutions","version":2},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-08-14T13:38:02.104560Z"},"links":{"cited_paper":"/paper/1703.08226","citing_paper":"/paper/1908.04961"},"observation_digest":"sha256:f322a36dd3fd51d87c49385088e66e45caf9873c4ae3e640bc4a9afff498217d","observation_id":"93e6edc7-f8a8-41c1-95d9-3ce09e8d2dc5","resolution":{"observed_at":"2026-08-14T13:38:02.104560Z","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":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T13:38:03.191709Z","title":null,"venue":null,"work_id":"c84ba9d2-9292-46e8-a53b-6c5e5f961352","year":1984},"citing_paper":{"arxiv_id":"1908.04961","last_updated":"2019-08-15T16:41:53Z","snapshot_observed_at":"2026-08-16T03:37:35.803409Z","submitted_at":"2019-08-14T05:23:32Z","title":"Charged cosmological black holes: a thorough study of a family of solutions","version":2},"reference_index":54,"source":"pdf_text","source_observed_at":"2026-08-14T13:38:02.109420Z"},"links":{"citing_paper":"/paper/1908.04961"},"observation_digest":"sha256:0cc6ee29e540e1c85f752b96d11ea8723d5232ec8325eeac6ddcf87cf97eda39","observation_id":"84bdab68-0781-4c69-b6d2-3e215ca6e7f2","resolution":{"observed_at":"2026-08-14T13:38:03.196593Z","resolver_source":"raw_fallback","status":"unresolved"},"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":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T13:38:03.176006Z","title":"Carrera and D","venue":null,"work_id":"a4997753-6d11-44fc-9f4f-c899c2036e5b","year":2010},"citing_paper":{"arxiv_id":"1908.04961","last_updated":"2019-08-15T16:41:53Z","snapshot_observed_at":"2026-08-16T03:37:35.803409Z","submitted_at":"2019-08-14T05:23:32Z","title":"Charged cosmological black holes: a thorough study of a family of solutions","version":2},"reference_index":55,"source":"pdf_text","source_observed_at":"2026-08-14T13:38:02.113988Z"},"links":{"citing_paper":"/paper/1908.04961"},"observation_digest":"sha256:572aec6e68ab13bc9297e9aa6d36329ff2dbde85b71c7eb89dc29e9470289471","observation_id":"833937ad-fd99-46cc-ba27-6ee6e5d257c0","resolution":{"observed_at":"2026-08-14T13:38:03.180715Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"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":"1510.03789","last_updated":"2015-10-13T17:27:43Z","snapshot_observed_at":"2026-08-14T22:28:03.037105Z","submitted_at":"2015-10-13T17:27:43Z","title":"Is the Hawking quasilocal energy \"Newtonian\"?","version":1},"cited_work":{"arxiv_id":"1510.03789","doi":null,"metadata_source":"pith","pith_arxiv_id":"1510.03789","snapshot_observed_at":"2026-08-14T13:38:02.373712Z","title":"Is the Hawking quasilocal energy \"Newtonian\"?","venue":"gr-qc","work_id":"078d7d03-420c-452a-a806-ba2872183d6f","year":2015},"citing_paper":{"arxiv_id":"1908.04961","last_updated":"2019-08-15T16:41:53Z","snapshot_observed_at":"2026-08-16T03:37:35.803409Z","submitted_at":"2019-08-14T05:23:32Z","title":"Charged cosmological black holes: a thorough study of a family of solutions","version":2},"reference_index":56,"source":"pdf_text","source_observed_at":"2026-08-14T13:38:02.118503Z"},"links":{"cited_paper":"/paper/1510.03789","citing_paper":"/paper/1908.04961"},"observation_digest":"sha256:e4853d18c9ba95c298ebd67d72fddb95815b528eea6c9771270f013274eae6d5","observation_id":"d9d470e5-f7e1-49f2-a1b7-17b034a1794c","resolution":{"observed_at":"2026-08-14T13:38:02.379088Z","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":"1606.01215","last_updated":"2016-06-03T18:33:05Z","snapshot_observed_at":"2026-08-14T21:54:17.297783Z","submitted_at":"2016-06-03T18:33:05Z","title":"Self-gravitating fluid solutions of Shape Dynamics","version":1},"cited_work":{"arxiv_id":"1606.01215","doi":null,"metadata_source":"pith","pith_arxiv_id":"1606.01215","snapshot_observed_at":"2026-08-14T13:38:02.350317Z","title":"Self-gravitating fluid solutions of Shape Dynamics","venue":"gr-qc","work_id":"c915b051-c439-42d5-8f2f-a21523aaeceb","year":2016},"citing_paper":{"arxiv_id":"1908.04961","last_updated":"2019-08-15T16:41:53Z","snapshot_observed_at":"2026-08-16T03:37:35.803409Z","submitted_at":"2019-08-14T05:23:32Z","title":"Charged cosmological black holes: a thorough study of a family of solutions","version":2},"reference_index":57,"source":"pdf_text","source_observed_at":"2026-08-14T13:38:02.123423Z"},"links":{"cited_paper":"/paper/1606.01215","citing_paper":"/paper/1908.04961"},"observation_digest":"sha256:904c13f749750c941093b534d99a8bdfb1930bb6748e087a74b83c640507c708","observation_id":"b4797a19-d30e-4991-862c-436767ffbd61","resolution":{"observed_at":"2026-08-14T13:38:02.355770Z","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":"gr-qc/0403032","last_updated":"2004-11-02T15:27:26Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2004-03-08T16:22:30Z","title":"Spherically symmetric spacetimes with a trapped surface","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"gr-qc/0403032","snapshot_observed_at":"2026-08-14T13:38:02.128332Z","title":"Dafermos, Class","venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"1908.04961","last_updated":"2019-08-15T16:41:53Z","snapshot_observed_at":"2026-08-16T03:37:35.803409Z","submitted_at":"2019-08-14T05:23:32Z","title":"Charged cosmological black holes: a thorough study of a family of solutions","version":2},"reference_index":58,"source":"pdf_text","source_observed_at":"2026-08-14T13:38:02.128332Z"},"links":{"cited_paper":"/paper/gr-qc/0403032","citing_paper":"/paper/1908.04961"},"observation_digest":"sha256:feecad7c5d5d76dd22f00ac8cede82c247f6e0893ccc3c23dc77121634058c99","observation_id":"3de5d13a-4d60-4403-a0b3-6764da4a76df","resolution":{"observed_at":"2026-08-14T13:38:02.128332Z","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":"2026-08-14T13:38:02.133489Z","title":"Schnetter and B","venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"1908.04961","last_updated":"2019-08-15T16:41:53Z","snapshot_observed_at":"2026-08-16T03:37:35.803409Z","submitted_at":"2019-08-14T05:23:32Z","title":"Charged cosmological black holes: a thorough study of a family of solutions","version":2},"reference_index":59,"source":"pdf_text","source_observed_at":"2026-08-14T13:38:02.133489Z"},"links":{"citing_paper":"/paper/1908.04961"},"observation_digest":"sha256:d8491ed1b70b0039a614fe0a4c141d2c372031733eef802ea2c09aa5091a4649","observation_id":"f8195184-3185-4392-8654-7124efe4f215","resolution":{"observed_at":"2026-08-14T13:38:02.133489Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1506.07122","last_updated":"2015-06-24T18:20:51Z","snapshot_observed_at":"2026-08-14T22:43:14.044694Z","submitted_at":"2015-06-23T18:27:00Z","title":"A dual null formalism for the collapse of fluids in a cosmological background","version":2},"cited_work":{"arxiv_id":"1506.07122","doi":null,"metadata_source":"pith","pith_arxiv_id":"1506.07122","snapshot_observed_at":"2026-08-14T13:38:02.311904Z","title":"A dual null formalism for the collapse of fluids in a cosmological background","venue":"gr-qc","work_id":"14731693-3d4e-4993-9421-4e2016d6813f","year":2015},"citing_paper":{"arxiv_id":"1908.04961","last_updated":"2019-08-15T16:41:53Z","snapshot_observed_at":"2026-08-16T03:37:35.803409Z","submitted_at":"2019-08-14T05:23:32Z","title":"Charged cosmological black holes: a thorough study of a family of solutions","version":2},"reference_index":60,"source":"pdf_text","source_observed_at":"2026-08-14T13:38:02.138201Z"},"links":{"cited_paper":"/paper/1506.07122","citing_paper":"/paper/1908.04961"},"observation_digest":"sha256:e8d4a8a635d8e7208414b9e6a56b63a439e11d0e467ba1a98107bb900e7f87cb","observation_id":"792c0525-c69e-4a82-9d2d-0955165fdb4a","resolution":{"observed_at":"2026-08-14T13:38:02.317023Z","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":"1511.08663","last_updated":"2016-05-03T19:27:19Z","snapshot_observed_at":"2026-08-14T22:21:04.251593Z","submitted_at":"2015-11-27T13:30:43Z","title":"Quasilocal approach to general universal horizons","version":2},"cited_work":{"arxiv_id":"1511.08663","doi":null,"metadata_source":"pith","pith_arxiv_id":"1511.08663","snapshot_observed_at":"2026-08-14T13:38:02.288040Z","title":"Quasilocal approach to general universal horizons","venue":"gr-qc","work_id":"f91679b2-b366-4658-b68b-60985a2580bc","year":2015},"citing_paper":{"arxiv_id":"1908.04961","last_updated":"2019-08-15T16:41:53Z","snapshot_observed_at":"2026-08-16T03:37:35.803409Z","submitted_at":"2019-08-14T05:23:32Z","title":"Charged cosmological black holes: a thorough study of a family of solutions","version":2},"reference_index":61,"source":"pdf_text","source_observed_at":"2026-08-14T13:38:02.143170Z"},"links":{"cited_paper":"/paper/1511.08663","citing_paper":"/paper/1908.04961"},"observation_digest":"sha256:266874ee446850bb1fd7d220d23bfb4502cba69cece2260b09cd2409c72db65f","observation_id":"ae73261b-0299-40c8-9cf1-bedade057ff3","resolution":{"observed_at":"2026-08-14T13:38:02.294042Z","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":"1508.06849","last_updated":"2016-02-09T17:39:50Z","snapshot_observed_at":"2026-08-15T03:15:17.976718Z","submitted_at":"2015-08-27T13:22:12Z","title":"Quasilocal energy in modified gravity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1508.06849","snapshot_observed_at":"2026-08-14T13:38:02.148251Z","title":"Faraoni, (2015), arXiv:1508.06849 [gr-qc]","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"1908.04961","last_updated":"2019-08-15T16:41:53Z","snapshot_observed_at":"2026-08-16T03:37:35.803409Z","submitted_at":"2019-08-14T05:23:32Z","title":"Charged cosmological black holes: a thorough study of a family of solutions","version":2},"reference_index":62,"source":"pdf_text","source_observed_at":"2026-08-14T13:38:02.148251Z"},"links":{"cited_paper":"/paper/1508.06849","citing_paper":"/paper/1908.04961"},"observation_digest":"sha256:ddf619d7539a65c03a0d7b50ae4ad46c3aa5714b0ad18192613f49f8b88d3fb2","observation_id":"17b32d22-4716-4ff9-b91b-e958381a11ef","resolution":{"observed_at":"2026-08-14T13:38:02.148251Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1803.11547","last_updated":"2018-07-17T22:53:34Z","snapshot_observed_at":"2026-08-14T19:30:41.402963Z","submitted_at":"2018-03-30T17:35:27Z","title":"Revisiting the Birkhoff theorem from a dual null point of view","version":3},"cited_work":{"arxiv_id":"1803.11547","doi":null,"metadata_source":"pith","pith_arxiv_id":"1803.11547","snapshot_observed_at":"2026-08-14T13:38:02.246540Z","title":"Revisiting the Birkhoff theorem from a dual null point of view","venue":"gr-qc","work_id":"5b23447d-b082-48c2-9e9a-594a3768c68b","year":2018},"citing_paper":{"arxiv_id":"1908.04961","last_updated":"2019-08-15T16:41:53Z","snapshot_observed_at":"2026-08-16T03:37:35.803409Z","submitted_at":"2019-08-14T05:23:32Z","title":"Charged cosmological black holes: a thorough study of a family of solutions","version":2},"reference_index":63,"source":"pdf_text","source_observed_at":"2026-08-14T13:38:02.153512Z"},"links":{"cited_paper":"/paper/1803.11547","citing_paper":"/paper/1908.04961"},"observation_digest":"sha256:95c1f62c4152a2b2536498ebd06c5e52f1b17a06229b079c79611e0462263919","observation_id":"b87ea5da-2ac7-45a5-be3b-60b8cd656d41","resolution":{"observed_at":"2026-08-14T13:38:02.253954Z","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":"1502.01003","last_updated":"2015-02-03T20:39:53Z","snapshot_observed_at":"2026-08-14T23:01:30.863850Z","submitted_at":"2015-02-03T20:39:53Z","title":"Cosmological black holes and white holes with time-dependent mass","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1502.01003","snapshot_observed_at":"2026-08-14T13:38:02.158500Z","title":null,"venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"1908.04961","last_updated":"2019-08-15T16:41:53Z","snapshot_observed_at":"2026-08-16T03:37:35.803409Z","submitted_at":"2019-08-14T05:23:32Z","title":"Charged cosmological black holes: a thorough study of a family of solutions","version":2},"reference_index":64,"source":"pdf_text","source_observed_at":"2026-08-14T13:38:02.158500Z"},"links":{"cited_paper":"/paper/1502.01003","citing_paper":"/paper/1908.04961"},"observation_digest":"sha256:05d3d6be9db0b064aa5fb274b7667059b911e0aabf585ece068da4d8ec128c9c","observation_id":"98426cd6-3b38-4a8c-b1b5-1f8d4d1494b0","resolution":{"observed_at":"2026-08-14T13:38:02.158500Z","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":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T13:38:03.149601Z","title":"Walker, J","venue":null,"work_id":"fe41bac9-c387-40c5-b519-04c895268d26","year":1970},"citing_paper":{"arxiv_id":"1908.04961","last_updated":"2019-08-15T16:41:53Z","snapshot_observed_at":"2026-08-16T03:37:35.803409Z","submitted_at":"2019-08-14T05:23:32Z","title":"Charged cosmological black holes: a thorough study of a family of solutions","version":2},"reference_index":65,"source":"pdf_text","source_observed_at":"2026-08-14T13:38:02.163528Z"},"links":{"citing_paper":"/paper/1908.04961"},"observation_digest":"sha256:baa29b4a83dce6e45efa809811bbf03bb4782e20fdb4117f3471857161b8867a","observation_id":"94fdf1ec-3375-4537-bbe4-128baa23bf2d","resolution":{"observed_at":"2026-08-14T13:38:03.154449Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"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":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T13:38:03.132391Z","title":"Laue and M","venue":null,"work_id":"2c192f65-2259-4361-92ba-79bf4c6fb076","year":1977},"citing_paper":{"arxiv_id":"1908.04961","last_updated":"2019-08-15T16:41:53Z","snapshot_observed_at":"2026-08-16T03:37:35.803409Z","submitted_at":"2019-08-14T05:23:32Z","title":"Charged cosmological black holes: a thorough study of a family of solutions","version":2},"reference_index":66,"source":"pdf_text","source_observed_at":"2026-08-14T13:38:02.168389Z"},"links":{"citing_paper":"/paper/1908.04961"},"observation_digest":"sha256:b84235d08d7fe6d8e56aa3aae24d9e4febcf6df946fa7c32d53cdf90b02e7795","observation_id":"8cb37c5b-3886-4128-8f48-9f531b0486fc","resolution":{"observed_at":"2026-08-14T13:38:03.138525Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"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":"gr-qc/0506013","last_updated":"2005-06-08T16:57:19Z","snapshot_observed_at":"2026-07-07T03:21:04.416422Z","submitted_at":"2005-06-02T15:07:54Z","title":"Local existence of dynamical and trapping horizons","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"gr-qc/0506013","snapshot_observed_at":"2026-08-14T13:38:02.173264Z","title":"Andersson, M","venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"1908.04961","last_updated":"2019-08-15T16:41:53Z","snapshot_observed_at":"2026-08-16T03:37:35.803409Z","submitted_at":"2019-08-14T05:23:32Z","title":"Charged cosmological black holes: a thorough study of a family of solutions","version":2},"reference_index":67,"source":"pdf_text","source_observed_at":"2026-08-14T13:38:02.173264Z"},"links":{"cited_paper":"/paper/gr-qc/0506013","citing_paper":"/paper/1908.04961"},"observation_digest":"sha256:e7586892164d7603d42cfbef3be3bae10347fe267eb1e94b5ab5749cf4435e5b","observation_id":"a3cb4d22-bb59-4ef0-a09a-a84b35e27576","resolution":{"observed_at":"2026-08-14T13:38:02.173264Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"1908.04961","last_updated":"2019-08-15T16:41:53Z","latest_version":2,"primary_category":"gr-qc","snapshot_observed_at":"2026-08-16T03:37:35.803409Z","submitted_at":"2019-08-14T05:23:32Z","title":"Charged cosmological black holes: a thorough study of a family of solutions"},"reference_resolution":{"displayed":67,"state_counts":{"malformed_identifier":0,"metadata_mismatch":3,"parse_uncertain":0,"unresolved":29,"verified_exact":9,"verified_fuzzy":26},"total_outbound_references":67},"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 67 of 67 outbound references and 0 inbound Pith citation observations for arXiv:1908.04961."}