{"as_of":"2026-08-17T22:25:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:8651694b1e94b3dde3a8b6c9327eed403aa41ff186ceae3c62aee1162cec3698","coverage":[{"denominator":53,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":53,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-16T04:57:01.316472Z","state":"measured"},{"denominator":54,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":54,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-17T06:30:58.91139+00:00","state":"measured"},{"denominator":1,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":1,"source":"paper_references, paper_reference_links","source_observed_at":"2026-06-30T05:26:28.825729Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"arxiv_reference","source_observed_at":"2026-06-30T14:34:45.798905Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2505.00366","last_updated":"2025-05-01T07:37:06Z","snapshot_observed_at":"2026-08-16T11:18:43.918864Z","submitted_at":"2025-05-01T07:37:06Z","title":"Primordial black hole formation from a type II perturbation in the absence and presence of pressure","version":1},"cited_work":{"arxiv_id":"2505.00366","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2505.00366","snapshot_observed_at":"2026-06-30T14:34:45.798905Z","title":"Uehara, A","venue":null,"work_id":"f4758dc1-9d77-400f-aeb1-0e536d68e023","year":2025},"citing_paper":{"arxiv_id":"2606.30087","last_updated":"2026-06-29T10:27:35Z","snapshot_observed_at":"2026-08-04T09:16:17.016040Z","submitted_at":"2026-06-29T10:27:35Z","title":"Compaction function in stochastic inflation: a \\texttt{FOREST} of type I and II primordial black holes","version":1},"reference_index":71,"source":"pdf_text","source_observed_at":"2026-06-30T05:26:28.825729Z"},"links":{"cited_paper":"/paper/2505.00366","citing_paper":"/paper/2606.30087"},"observation_digest":"sha256:1b34b928d847632217729bad249fa8cd4dc0fa2b67b19033d620a7ff39599e2f","observation_id":"d9146483-36bf-4587-8fb3-b2b606dd4ed8","resolution":{"observed_at":"2026-06-30T14:34:45.800158Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/2505.00366/citation-record","integrity":"/paper/2505.00366/integrity","json":"/paper/2505.00366/citation-record.json","paper":"/paper/2505.00366"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T04:57:02.716945Z","title":"Oppenheimer and H","venue":null,"work_id":"fc9a4c47-eb7d-4d34-9f1c-112bae3bf0eb","year":1939},"citing_paper":{"arxiv_id":"2505.00366","last_updated":"2025-05-01T07:37:06Z","snapshot_observed_at":"2026-08-16T11:18:43.918864Z","submitted_at":"2025-05-01T07:37:06Z","title":"Primordial black hole formation from a type II perturbation in the absence and presence of pressure","version":1},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-16T04:57:00.863242Z"},"links":{"citing_paper":"/paper/2505.00366"},"observation_digest":"sha256:8be12fcf3594ad2ab4c8079601e041d8a2c040f6c636768ddc6b278a92ea6149","observation_id":"2582c97b-262f-44a7-86d4-f6a8823fa4f9","resolution":{"observed_at":"2026-08-16T04:57:02.722026Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-16T04:57:02.696451Z","title":"Zel’dovich and I.D","venue":null,"work_id":"3b61f811-fd04-48fc-900c-f5966dfb0e15","year":1967},"citing_paper":{"arxiv_id":"2505.00366","last_updated":"2025-05-01T07:37:06Z","snapshot_observed_at":"2026-08-16T11:18:43.918864Z","submitted_at":"2025-05-01T07:37:06Z","title":"Primordial black hole formation from a type II perturbation in the absence and presence of pressure","version":1},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-16T04:57:00.871147Z"},"links":{"citing_paper":"/paper/2505.00366"},"observation_digest":"sha256:b0c4eb3f12a0a356a408e22b4466c6fb2ff94e4b7795a497fb1d1722bfe7081c","observation_id":"ca1ec4a7-873e-4138-a572-13eb322f29d6","resolution":{"observed_at":"2026-08-16T04:57:02.702380Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-16T04:57:02.670485Z","title":null,"venue":null,"work_id":"33f20c47-6e5c-4d89-b674-a1efe9da433b","year":1971},"citing_paper":{"arxiv_id":"2505.00366","last_updated":"2025-05-01T07:37:06Z","snapshot_observed_at":"2026-08-16T11:18:43.918864Z","submitted_at":"2025-05-01T07:37:06Z","title":"Primordial black hole formation from a type II perturbation in the absence and presence of pressure","version":1},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-16T04:57:00.882437Z"},"links":{"citing_paper":"/paper/2505.00366"},"observation_digest":"sha256:da0aa3d3a586e78953f2508f23c1435aeaa8702ea5d7d212cee4b2351dfb1564","observation_id":"59c26877-220f-4d50-8a57-595243daab7c","resolution":{"observed_at":"2026-08-16T04:57:02.677606Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-16T04:57:02.652998Z","title":"Carr and S.W","venue":null,"work_id":"d975b400-1402-4d50-b225-70af5c7213e9","year":1974},"citing_paper":{"arxiv_id":"2505.00366","last_updated":"2025-05-01T07:37:06Z","snapshot_observed_at":"2026-08-16T11:18:43.918864Z","submitted_at":"2025-05-01T07:37:06Z","title":"Primordial black hole formation from a type II perturbation in the absence and presence of pressure","version":1},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-16T04:57:01.026893Z"},"links":{"citing_paper":"/paper/2505.00366"},"observation_digest":"sha256:91ba8c2250d1e73862acbf6a2a91500d0baec1152d563486fce3433c317a2303","observation_id":"67e9be74-0c86-41e7-83cb-32ccc6baaa5e","resolution":{"observed_at":"2026-08-16T04:57:02.657971Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-16T04:57:01.033507Z","title":"Carr, The Primordial black hole mass spectrum , Astrophys","venue":null,"work_id":null,"year":1975},"citing_paper":{"arxiv_id":"2505.00366","last_updated":"2025-05-01T07:37:06Z","snapshot_observed_at":"2026-08-16T11:18:43.918864Z","submitted_at":"2025-05-01T07:37:06Z","title":"Primordial black hole formation from a type II perturbation in the absence and presence of pressure","version":1},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-16T04:57:01.033507Z"},"links":{"citing_paper":"/paper/2505.00366"},"observation_digest":"sha256:18a00400d73d67a54f09f8c52cd2e9566f1912e77c1e4de84d7bc182d0060cf3","observation_id":"a4278572-915d-4a52-8301-b6473d3fedc3","resolution":{"observed_at":"2026-08-16T04:57:01.033507Z","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":"2026-08-16T04:57:02.608655Z","title":"Harada and B.J","venue":null,"work_id":"1c9af0e6-9441-4275-b37d-0edfe9eda3d3","year":2005},"citing_paper":{"arxiv_id":"2505.00366","last_updated":"2025-05-01T07:37:06Z","snapshot_observed_at":"2026-08-16T11:18:43.918864Z","submitted_at":"2025-05-01T07:37:06Z","title":"Primordial black hole formation from a type II perturbation in the absence and presence of pressure","version":1},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-16T04:57:01.039356Z"},"links":{"citing_paper":"/paper/2505.00366"},"observation_digest":"sha256:0afa40f27e9e86e4593f3a5f0418bec6f904793c1ecc6af599face51f1c3fb6f","observation_id":"d7694530-22fc-4fe4-a554-24b18a3ef634","resolution":{"observed_at":"2026-08-16T04:57:02.614216Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-16T04:57:02.588990Z","title":null,"venue":null,"work_id":"45e78cd0-d018-40dc-84d4-9205a60ff0d9","year":2011},"citing_paper":{"arxiv_id":"2505.00366","last_updated":"2025-05-01T07:37:06Z","snapshot_observed_at":"2026-08-16T11:18:43.918864Z","submitted_at":"2025-05-01T07:37:06Z","title":"Primordial black hole formation from a type II perturbation in the absence and presence of pressure","version":1},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-16T04:57:01.044816Z"},"links":{"citing_paper":"/paper/2505.00366"},"observation_digest":"sha256:f2984fca68195d7a4b249fe4c7f0660071a5e52c3da9ddd63213b87ad0a813cc","observation_id":"c2594a10-0b54-4dd8-ac26-82f951823eae","resolution":{"observed_at":"2026-08-16T04:57:02.595236Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-16T04:57:02.573196Z","title":"Misner, Gravitational collapse., pp 115-215 of Astrophysics and General Relativity","venue":null,"work_id":"40316551-9d73-43c0-830e-90fb142db742","year":1969},"citing_paper":{"arxiv_id":"2505.00366","last_updated":"2025-05-01T07:37:06Z","snapshot_observed_at":"2026-08-16T11:18:43.918864Z","submitted_at":"2025-05-01T07:37:06Z","title":"Primordial black hole formation from a type II perturbation in the absence and presence of pressure","version":1},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-16T04:57:01.049805Z"},"links":{"citing_paper":"/paper/2505.00366"},"observation_digest":"sha256:60a044ee882af5dee28c9ad56353736da556d58762d94996900d4de46e3ffc42","observation_id":"a070ac97-fe18-4156-b230-28ab004f0dac","resolution":{"observed_at":"2026-08-16T04:57:02.578303Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-16T04:57:02.553168Z","title":"Barnes, On gravitational collapse against a cosmological background , Journal of Physics A: General Physics 3 (1970) 653","venue":null,"work_id":"e9bdb10c-6c8a-4d31-8125-4b2023835c18","year":1970},"citing_paper":{"arxiv_id":"2505.00366","last_updated":"2025-05-01T07:37:06Z","snapshot_observed_at":"2026-08-16T11:18:43.918864Z","submitted_at":"2025-05-01T07:37:06Z","title":"Primordial black hole formation from a type II perturbation in the absence and presence of pressure","version":1},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-16T04:57:01.054505Z"},"links":{"citing_paper":"/paper/2505.00366"},"observation_digest":"sha256:844e1c43e95a61090df52ff4b64cd37ae43b9f038e26b52cbf5116451b0ffb25","observation_id":"cde27f96-55b5-46c8-95b9-a8a7f21fa3c7","resolution":{"observed_at":"2026-08-16T04:57:02.561172Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"p/1822381","doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T04:57:02.050272Z","title":"Zel’dovich and L.P","venue":null,"work_id":"4fec397e-4c9e-402a-b26d-d2d22839ec14","year":1984},"citing_paper":{"arxiv_id":"2505.00366","last_updated":"2025-05-01T07:37:06Z","snapshot_observed_at":"2026-08-16T11:18:43.918864Z","submitted_at":"2025-05-01T07:37:06Z","title":"Primordial black hole formation from a type II perturbation in the absence and presence of pressure","version":1},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-16T04:57:01.059994Z"},"links":{"citing_paper":"/paper/2505.00366"},"observation_digest":"sha256:fd3c51c144a41da65e5c170fc9516fb4cb5460a3e9ba067c21cd25c07f46ed44","observation_id":"f92267b4-a11e-4155-b60e-2e8eb3b8cec8","resolution":{"observed_at":"2026-08-16T04:57:02.058975Z","resolver_source":"raw_fallback","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-16T04:57:02.532765Z","title":null,"venue":null,"work_id":"10b53c5d-d76f-4caf-8049-eaec8c89822b","year":1984},"citing_paper":{"arxiv_id":"2505.00366","last_updated":"2025-05-01T07:37:06Z","snapshot_observed_at":"2026-08-16T11:18:43.918864Z","submitted_at":"2025-05-01T07:37:06Z","title":"Primordial black hole formation from a type II perturbation in the absence and presence of pressure","version":1},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-16T04:57:01.065011Z"},"links":{"citing_paper":"/paper/2505.00366"},"observation_digest":"sha256:3651620962af6261969504f4bb159b4d6164ce771c2fd7b31690684b0e934b63","observation_id":"56d5aba8-f63b-413c-bd3a-c5400e145a52","resolution":{"observed_at":"2026-08-16T04:57:02.537112Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-16T04:57:02.506558Z","title":"Sussman, Conformal structure of a Schwarzschild black hole immersed in a Friedmann universe., General Relativity and Gravitation 17 (1985) 251","venue":null,"work_id":"e5bf4c54-646a-448f-94dc-0020f339369e","year":1985},"citing_paper":{"arxiv_id":"2505.00366","last_updated":"2025-05-01T07:37:06Z","snapshot_observed_at":"2026-08-16T11:18:43.918864Z","submitted_at":"2025-05-01T07:37:06Z","title":"Primordial black hole formation from a type II perturbation in the absence and presence of pressure","version":1},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-16T04:57:01.070258Z"},"links":{"citing_paper":"/paper/2505.00366"},"observation_digest":"sha256:6f48d98d101dceed0cffe3ab07ea4e3fa50d37781a9f69e0b3972e52d409e53f","observation_id":"b5a2b8bd-c20e-4d00-a8c6-ca9a1bf16002","resolution":{"observed_at":"2026-08-16T04:57:02.520431Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-16T04:57:02.472903Z","title":"Hellaby and K","venue":null,"work_id":"8b1be226-d786-4edf-a3cf-df6455af5306","year":1985},"citing_paper":{"arxiv_id":"2505.00366","last_updated":"2025-05-01T07:37:06Z","snapshot_observed_at":"2026-08-16T11:18:43.918864Z","submitted_at":"2025-05-01T07:37:06Z","title":"Primordial black hole formation from a type II perturbation in the absence and presence of pressure","version":1},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-16T04:57:01.077333Z"},"links":{"citing_paper":"/paper/2505.00366"},"observation_digest":"sha256:83096c0f96161c96836aadedee9c0017aa7886874e5ff30b2d79913d33b976a0","observation_id":"2acaf064-f197-4267-b069-c54267ae36cf","resolution":{"observed_at":"2026-08-16T04:57:02.482230Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-16T04:57:02.453321Z","title":"Hellaby, A kruskal-like model with finite density , Classical and Quantum Gravity 4 (1987) 635","venue":null,"work_id":"493c2abf-3bdf-4508-ac4d-ea9a349f6da4","year":1987},"citing_paper":{"arxiv_id":"2505.00366","last_updated":"2025-05-01T07:37:06Z","snapshot_observed_at":"2026-08-16T11:18:43.918864Z","submitted_at":"2025-05-01T07:37:06Z","title":"Primordial black hole formation from a type II perturbation in the absence and presence of pressure","version":1},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-16T04:57:01.082730Z"},"links":{"citing_paper":"/paper/2505.00366"},"observation_digest":"sha256:d5c547a87199357ea5186a0f0c63558f07b9cdc6ef3a6fc1d229038456c3e246","observation_id":"cdb5c8d1-23e4-49f4-8202-d5cfb10cc055","resolution":{"observed_at":"2026-08-16T04:57:02.459918Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-16T04:57:02.429352Z","title":"Krasi´ nski and C","venue":null,"work_id":"f9030aa3-79d9-46c9-8977-76b2e4c538af","year":2004},"citing_paper":{"arxiv_id":"2505.00366","last_updated":"2025-05-01T07:37:06Z","snapshot_observed_at":"2026-08-16T11:18:43.918864Z","submitted_at":"2025-05-01T07:37:06Z","title":"Primordial black hole formation from a type II perturbation in the absence and presence of pressure","version":1},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-16T04:57:01.087567Z"},"links":{"citing_paper":"/paper/2505.00366"},"observation_digest":"sha256:ce30562d6531c90b258a60a987b4588d9bc28aa9bb0a101e2c24fbe356ee71c5","observation_id":"25d571f5-e0b7-49cc-b7ab-42cb7dd2723c","resolution":{"observed_at":"2026-08-16T04:57:02.435633Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/0206052","last_updated":"2002-08-27T14:52:31Z","snapshot_observed_at":"2026-07-07T03:15:59.460346Z","submitted_at":"2002-06-18T13:27:29Z","title":"You Can't Get Through Szekeres Wormholes - or - Regularity, Topology and Causality in Quasi-Spherical Szekeres Models","version":4},"cited_work":{"arxiv_id":"gr-qc/0206052","doi":null,"metadata_source":"pith","pith_arxiv_id":"gr-qc/0206052","snapshot_observed_at":"2026-08-16T04:57:01.974957Z","title":"You Can't Get Through Szekeres Wormholes - or - Regularity, Topology and Causality in Quasi-Spherical Szekeres Models","venue":"gr-qc","work_id":"c30482ea-c5a8-4420-abf2-7f64fa90c4c8","year":2002},"citing_paper":{"arxiv_id":"2505.00366","last_updated":"2025-05-01T07:37:06Z","snapshot_observed_at":"2026-08-16T11:18:43.918864Z","submitted_at":"2025-05-01T07:37:06Z","title":"Primordial black hole formation from a type II perturbation in the absence and presence of pressure","version":1},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-16T04:57:01.092213Z"},"links":{"cited_paper":"/paper/gr-qc/0206052","citing_paper":"/paper/2505.00366"},"observation_digest":"sha256:3d4bd69d18425c59c139f76186a2763dacc15ee560b1763d3f44f158f1b9a6ca","observation_id":"82eda7ce-4576-43e2-b49e-4426e42c83e1","resolution":{"observed_at":"2026-08-16T04:57:01.980641Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-16T04:57:02.403190Z","title":"Plebanski and A","venue":null,"work_id":"08f080b9-4efe-4345-a911-2baf4955d4b5","year":2006},"citing_paper":{"arxiv_id":"2505.00366","last_updated":"2025-05-01T07:37:06Z","snapshot_observed_at":"2026-08-16T11:18:43.918864Z","submitted_at":"2025-05-01T07:37:06Z","title":"Primordial black hole formation from a type II perturbation in the absence and presence of pressure","version":1},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-16T04:57:01.097670Z"},"links":{"citing_paper":"/paper/2505.00366"},"observation_digest":"sha256:2d1f02f6019df65d743f52293ab9870a483763855e0318ee20dfa44032297c25","observation_id":"607d7f9a-e9e5-41c4-a53a-06126490a2a8","resolution":{"observed_at":"2026-08-16T04:57:02.409102Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-16T04:57:02.387395Z","title":null,"venue":null,"work_id":"01ca44cb-d1c8-4ba3-824e-450a319a9642","year":2023},"citing_paper":{"arxiv_id":"2505.00366","last_updated":"2025-05-01T07:37:06Z","snapshot_observed_at":"2026-08-16T11:18:43.918864Z","submitted_at":"2025-05-01T07:37:06Z","title":"Primordial black hole formation from a type II perturbation in the absence and presence of pressure","version":1},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-16T04:57:01.102675Z"},"links":{"citing_paper":"/paper/2505.00366"},"observation_digest":"sha256:4dc97a49f927f460ebda0eeeffd059231f58f4f42699a8b828ccfd7ae56d6619","observation_id":"fbbeb60d-24ba-493c-8782-5b3c9d62df42","resolution":{"observed_at":"2026-08-16T04:57:02.392382Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-16T04:57:01.108390Z","title":"Escriv` a, V","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2505.00366","last_updated":"2025-05-01T07:37:06Z","snapshot_observed_at":"2026-08-16T11:18:43.918864Z","submitted_at":"2025-05-01T07:37:06Z","title":"Primordial black hole formation from a type II perturbation in the absence and presence of pressure","version":1},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-16T04:57:01.108390Z"},"links":{"citing_paper":"/paper/2505.00366"},"observation_digest":"sha256:8135b197c17f725cb2ef383dea47da8b487b8e7bd1fb5655acba95f0001ac6bf","observation_id":"c4593292-d32e-41f8-af77-ac8ebf350e10","resolution":{"observed_at":"2026-08-16T04:57:01.108390Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2411.07648","last_updated":"2024-11-12T08:55:45Z","snapshot_observed_at":"2026-08-16T13:00:53.320537Z","submitted_at":"2024-11-12T08:55:45Z","title":"Primordial Black Hole Formation from Type II Fluctuations with Primordial Non-Gaussianity","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2411.07648","snapshot_observed_at":"2026-08-16T04:57:01.113531Z","title":"Shimada, A","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2505.00366","last_updated":"2025-05-01T07:37:06Z","snapshot_observed_at":"2026-08-16T11:18:43.918864Z","submitted_at":"2025-05-01T07:37:06Z","title":"Primordial black hole formation from a type II perturbation in the absence and presence of pressure","version":1},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-16T04:57:01.113531Z"},"links":{"cited_paper":"/paper/2411.07648","citing_paper":"/paper/2505.00366"},"observation_digest":"sha256:38aa29479350b3fd3cf8ba9b220c0eb6cc6f1875221c90b0b873fbdce9533d0d","observation_id":"e6e59ca6-0dcc-4978-9f66-5f029e79841a","resolution":{"observed_at":"2026-08-16T04:57:01.113531Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2411.07647","last_updated":"2025-04-09T03:37:05Z","snapshot_observed_at":"2026-08-16T13:00:53.772218Z","submitted_at":"2024-11-12T08:55:44Z","title":"Primordial black holes and induced gravitational waves from logarithmic non-Gaussianity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2411.07647","snapshot_observed_at":"2026-08-16T04:57:01.121313Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2505.00366","last_updated":"2025-05-01T07:37:06Z","snapshot_observed_at":"2026-08-16T11:18:43.918864Z","submitted_at":"2025-05-01T07:37:06Z","title":"Primordial black hole formation from a type II perturbation in the absence and presence of pressure","version":1},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-16T04:57:01.121313Z"},"links":{"cited_paper":"/paper/2411.07647","citing_paper":"/paper/2505.00366"},"observation_digest":"sha256:b2712c96da02b2e77a3d77e63ddb21236e57ad54db2490b86c94d49e945468cb","observation_id":"e87382d2-091f-4706-8538-f73620d6c608","resolution":{"observed_at":"2026-08-16T04:57:01.121313Z","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":"2026-08-16T04:57:01.127170Z","title":"Escriv` a,The threshold for PBH formation in the type-II region and its analytical estimation , 2504.05814","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2505.00366","last_updated":"2025-05-01T07:37:06Z","snapshot_observed_at":"2026-08-16T11:18:43.918864Z","submitted_at":"2025-05-01T07:37:06Z","title":"Primordial black hole formation from a type II perturbation in the absence and presence of pressure","version":1},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-16T04:57:01.127170Z"},"links":{"citing_paper":"/paper/2505.00366"},"observation_digest":"sha256:b8ad5bfea76fc01711ed2bf391cd384fdee984c1f87ccb356d6ceee2ef5d6599","observation_id":"735cd81f-1fbb-4e9f-b59e-13473726f428","resolution":{"observed_at":"2026-08-16T04:57:01.127170Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1612.03753","last_updated":"2017-03-21T19:56:30Z","snapshot_observed_at":"2026-08-14T21:25:52.053348Z","submitted_at":"2016-12-12T21:34:51Z","title":"Primordial black hole and wormhole formation by domain walls","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1612.03753","snapshot_observed_at":"2026-08-16T04:57:01.131757Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2505.00366","last_updated":"2025-05-01T07:37:06Z","snapshot_observed_at":"2026-08-16T11:18:43.918864Z","submitted_at":"2025-05-01T07:37:06Z","title":"Primordial black hole formation from a type II perturbation in the absence and presence of pressure","version":1},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-16T04:57:01.131757Z"},"links":{"cited_paper":"/paper/1612.03753","citing_paper":"/paper/2505.00366"},"observation_digest":"sha256:e3467489f4b5c4642124200e3dec18f58f5c9f0bee30e1a2e25dd4a358270c03","observation_id":"e036c4c5-1e62-40e7-9c11-aa7c22973c70","resolution":{"observed_at":"2026-08-16T04:57:01.131757Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1710.02865","last_updated":"2018-03-10T05:12:50Z","snapshot_observed_at":"2026-08-14T20:25:49.810935Z","submitted_at":"2017-10-08T18:04:57Z","title":"Primordial black hole formation by vacuum bubbles","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1710.02865","snapshot_observed_at":"2026-08-16T04:57:01.137029Z","title":"Deng and A","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2505.00366","last_updated":"2025-05-01T07:37:06Z","snapshot_observed_at":"2026-08-16T11:18:43.918864Z","submitted_at":"2025-05-01T07:37:06Z","title":"Primordial black hole formation from a type II perturbation in the absence and presence of pressure","version":1},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-16T04:57:01.137029Z"},"links":{"cited_paper":"/paper/1710.02865","citing_paper":"/paper/2505.00366"},"observation_digest":"sha256:11f266deec4ba329881bdc46bf2a31b842fb94d7668a478afbaf655305ba6288","observation_id":"b80e95ed-b915-43b4-9d6d-4c94f9e63417","resolution":{"observed_at":"2026-08-16T04:57:01.137029Z","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":"2026-08-16T04:57:01.142621Z","title":"Uehara, A","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2505.00366","last_updated":"2025-05-01T07:37:06Z","snapshot_observed_at":"2026-08-16T11:18:43.918864Z","submitted_at":"2025-05-01T07:37:06Z","title":"Primordial black hole formation from a type II perturbation in the absence and presence of pressure","version":1},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-16T04:57:01.142621Z"},"links":{"citing_paper":"/paper/2505.00366"},"observation_digest":"sha256:500003815d2b753a92809695758bd3ff1dba41119f15cc624484c580c33184c9","observation_id":"372780fa-2711-4be7-bbec-aef698bdc2cf","resolution":{"observed_at":"2026-08-16T04:57:01.142621Z","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":"2026-08-16T04:57:01.147134Z","title":"Hayward, General laws of black hole dynamics , Phys","venue":null,"work_id":null,"year":1994},"citing_paper":{"arxiv_id":"2505.00366","last_updated":"2025-05-01T07:37:06Z","snapshot_observed_at":"2026-08-16T11:18:43.918864Z","submitted_at":"2025-05-01T07:37:06Z","title":"Primordial black hole formation from a type II perturbation in the absence and presence of pressure","version":1},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-16T04:57:01.147134Z"},"links":{"citing_paper":"/paper/2505.00366"},"observation_digest":"sha256:9edfd3c80d68c0929520241fc6642117e26ff0ced1d33c731af43dfcc21b317c","observation_id":"3489b15d-d48d-4563-9ad4-3b1f98744714","resolution":{"observed_at":"2026-08-16T04:57:01.147134Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/9408002","last_updated":"2002-02-17T05:04:07Z","snapshot_observed_at":"2026-07-07T03:24:51.075694Z","submitted_at":"1994-08-02T06:46:48Z","title":"Gravitational Energy in Spherical Symmetry","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"gr-qc/9408002","snapshot_observed_at":"2026-08-16T04:57:01.152204Z","title":"Hayward, Gravitational energy in spherical symmetry , Phys","venue":null,"work_id":null,"year":1996},"citing_paper":{"arxiv_id":"2505.00366","last_updated":"2025-05-01T07:37:06Z","snapshot_observed_at":"2026-08-16T11:18:43.918864Z","submitted_at":"2025-05-01T07:37:06Z","title":"Primordial black hole formation from a type II perturbation in the absence and presence of pressure","version":1},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-16T04:57:01.152204Z"},"links":{"cited_paper":"/paper/gr-qc/9408002","citing_paper":"/paper/2505.00366"},"observation_digest":"sha256:58d195c825ac11d8597317e3e42c03316010286bd45e5979e2b47407039d1575","observation_id":"19128323-05c9-4c32-a3dc-90b5459c9157","resolution":{"observed_at":"2026-08-16T04:57:01.152204Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0901.1153","last_updated":"2009-03-03T20:27:57Z","snapshot_observed_at":"2026-08-15T05:57:49.724420Z","submitted_at":"2009-01-08T23:43:09Z","title":"Cosmological wormholes","version":3},"cited_work":{"arxiv_id":"0901.1153","doi":null,"metadata_source":"pith","pith_arxiv_id":"0901.1153","snapshot_observed_at":"2026-08-16T04:57:01.621729Z","title":"Cosmological wormholes","venue":"gr-qc","work_id":"9f9c71f6-26b1-4b68-946f-9a375a1fb276","year":2009},"citing_paper":{"arxiv_id":"2505.00366","last_updated":"2025-05-01T07:37:06Z","snapshot_observed_at":"2026-08-16T11:18:43.918864Z","submitted_at":"2025-05-01T07:37:06Z","title":"Primordial black hole formation from a type II perturbation in the absence and presence of pressure","version":1},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-16T04:57:01.157413Z"},"links":{"cited_paper":"/paper/0901.1153","citing_paper":"/paper/2505.00366"},"observation_digest":"sha256:5d3d589ab15b18df7049bd20fc716a36fc7750172860e6e29fc870efdcd962b4","observation_id":"1acf86bf-ed47-48c4-987e-56d63407a655","resolution":{"observed_at":"2026-08-16T04:57:01.630507Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-16T04:57:01.165068Z","title":"Escriv` a,A new approach for simulating PBH formation from generic curvature fluctuations with the Misner-Sharp formalism , 2504.05813","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2505.00366","last_updated":"2025-05-01T07:37:06Z","snapshot_observed_at":"2026-08-16T11:18:43.918864Z","submitted_at":"2025-05-01T07:37:06Z","title":"Primordial black hole formation from a type II perturbation in the absence and presence of pressure","version":1},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-16T04:57:01.165068Z"},"links":{"citing_paper":"/paper/2505.00366"},"observation_digest":"sha256:ab2214294f3fb7b45eeecf7dc1e53a25cf6e2ace9788805411d4c67b5383b029","observation_id":"377c8bd0-35a4-4939-8e4e-fd02b64aaee0","resolution":{"observed_at":"2026-08-16T04:57:01.165068Z","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":"2026-08-16T04:57:02.358768Z","title":"Shibata and M","venue":null,"work_id":"51c18c1e-2e5b-473d-b707-d071190711ba","year":1999},"citing_paper":{"arxiv_id":"2505.00366","last_updated":"2025-05-01T07:37:06Z","snapshot_observed_at":"2026-08-16T11:18:43.918864Z","submitted_at":"2025-05-01T07:37:06Z","title":"Primordial black hole formation from a type II perturbation in the absence and presence of pressure","version":1},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-16T04:57:01.171340Z"},"links":{"citing_paper":"/paper/2505.00366"},"observation_digest":"sha256:fbc358e98bbb3b87d803f7b08fff0f0d4081676c228e3dd3b488eef8c0e3db98","observation_id":"d2895480-c379-4c6c-8a07-8ef003c0250e","resolution":{"observed_at":"2026-08-16T04:57:02.363465Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-16T04:57:02.341716Z","title":"Lyth, K.A","venue":null,"work_id":"0ad35598-fb20-4f16-b94f-b0b6080e9945","year":2005},"citing_paper":{"arxiv_id":"2505.00366","last_updated":"2025-05-01T07:37:06Z","snapshot_observed_at":"2026-08-16T11:18:43.918864Z","submitted_at":"2025-05-01T07:37:06Z","title":"Primordial black hole formation from a type II perturbation in the absence and presence of pressure","version":1},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-08-16T04:57:01.178998Z"},"links":{"citing_paper":"/paper/2505.00366"},"observation_digest":"sha256:c792c47b67eccdbbbf0943011b0f326c18687dd3962431541349466d0d533dc6","observation_id":"01f47034-c591-4a84-8b92-17a47c547f13","resolution":{"observed_at":"2026-08-16T04:57:02.347839Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1512.08639","last_updated":"2016-09-15T02:52:29Z","snapshot_observed_at":"2026-08-14T22:16:43.421368Z","submitted_at":"2015-12-29T09:57:11Z","title":"Spherical and nonspherical models of primordial black hole formation: exact solutions","version":2},"cited_work":{"arxiv_id":"1512.08639","doi":null,"metadata_source":"pith","pith_arxiv_id":"1512.08639","snapshot_observed_at":"2026-08-16T04:57:01.495145Z","title":"Spherical and nonspherical models of primordial black hole formation: exact solutions","venue":"gr-qc","work_id":"cb848e99-339f-425e-8f51-904371140a5d","year":2015},"citing_paper":{"arxiv_id":"2505.00366","last_updated":"2025-05-01T07:37:06Z","snapshot_observed_at":"2026-08-16T11:18:43.918864Z","submitted_at":"2025-05-01T07:37:06Z","title":"Primordial black hole formation from a type II perturbation in the absence and presence of pressure","version":1},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-16T04:57:01.184308Z"},"links":{"cited_paper":"/paper/1512.08639","citing_paper":"/paper/2505.00366"},"observation_digest":"sha256:47ff6937b322555d8a7bf0591c0403353004f3e050f90732a91921e8c934f4b5","observation_id":"5ad6f80b-f499-46df-b3cb-ad4347b14c62","resolution":{"observed_at":"2026-08-16T04:57:01.503754Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-16T04:57:02.317648Z","title":"Tolman, Effect of imhomogeneity on cosmological models , Proc","venue":null,"work_id":"dd48a05a-8911-493d-abdb-dd1970207b6a","year":1934},"citing_paper":{"arxiv_id":"2505.00366","last_updated":"2025-05-01T07:37:06Z","snapshot_observed_at":"2026-08-16T11:18:43.918864Z","submitted_at":"2025-05-01T07:37:06Z","title":"Primordial black hole formation from a type II perturbation in the absence and presence of pressure","version":1},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-16T04:57:01.194425Z"},"links":{"citing_paper":"/paper/2505.00366"},"observation_digest":"sha256:d6921e525180fd0e3e0a6f8f299b23e78fccad87de75259293b319577490abac","observation_id":"feb06f18-71e8-4a0c-8b52-2a4d76aa2636","resolution":{"observed_at":"2026-08-16T04:57:02.323712Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/0605122","last_updated":"2006-07-16T22:03:51Z","snapshot_observed_at":"2026-08-05T21:52:25.215338Z","submitted_at":"2006-05-24T18:00:09Z","title":"Curvature profiles as initial conditions for primordial black hole formation","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"gr-qc/0605122","snapshot_observed_at":"2026-08-16T04:57:01.202277Z","title":"Polnarev and I","venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2505.00366","last_updated":"2025-05-01T07:37:06Z","snapshot_observed_at":"2026-08-16T11:18:43.918864Z","submitted_at":"2025-05-01T07:37:06Z","title":"Primordial black hole formation from a type II perturbation in the absence and presence of pressure","version":1},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-16T04:57:01.202277Z"},"links":{"cited_paper":"/paper/gr-qc/0605122","citing_paper":"/paper/2505.00366"},"observation_digest":"sha256:ff0b6ae3653b39d9132eb4dc025a21a755b7e195cd64f4c868f5f0b1830887b8","observation_id":"0c59bab1-fa03-4317-ac53-19b375ecd3f6","resolution":{"observed_at":"2026-08-16T04:57:01.202277Z","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":"2026-08-16T04:57:02.296908Z","title":"Harada, C.-M","venue":null,"work_id":"b12191f1-6e61-4b58-a066-035f69f6ac10","year":2015},"citing_paper":{"arxiv_id":"2505.00366","last_updated":"2025-05-01T07:37:06Z","snapshot_observed_at":"2026-08-16T11:18:43.918864Z","submitted_at":"2025-05-01T07:37:06Z","title":"Primordial black hole formation from a type II perturbation in the absence and presence of pressure","version":1},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-16T04:57:01.208856Z"},"links":{"citing_paper":"/paper/2505.00366"},"observation_digest":"sha256:ff1a06cc043652c032d24b0b16a6b9df9ab52c51c29a2d2d2ba712416155af0d","observation_id":"966ab50b-0ddf-4adc-a178-2549402519d4","resolution":{"observed_at":"2026-08-16T04:57:02.301569Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-16T04:57:01.213378Z","title":"Lemaitre, The expanding universe , Annales Soc","venue":null,"work_id":null,"year":1933},"citing_paper":{"arxiv_id":"2505.00366","last_updated":"2025-05-01T07:37:06Z","snapshot_observed_at":"2026-08-16T11:18:43.918864Z","submitted_at":"2025-05-01T07:37:06Z","title":"Primordial black hole formation from a type II perturbation in the absence and presence of pressure","version":1},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-16T04:57:01.213378Z"},"links":{"citing_paper":"/paper/2505.00366"},"observation_digest":"sha256:c217613a6bdc3855d4cde7d9ab01b2dcafd088a2e9f9ac965ea358f258c729f3","observation_id":"c9d7c415-913e-42de-b910-1b5644539c95","resolution":{"observed_at":"2026-08-16T04:57:01.213378Z","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":"2026-08-16T04:57:01.218331Z","title":"Misner, K.S","venue":null,"work_id":null,"year":1973},"citing_paper":{"arxiv_id":"2505.00366","last_updated":"2025-05-01T07:37:06Z","snapshot_observed_at":"2026-08-16T11:18:43.918864Z","submitted_at":"2025-05-01T07:37:06Z","title":"Primordial black hole formation from a type II perturbation in the absence and presence of pressure","version":1},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-16T04:57:01.218331Z"},"links":{"citing_paper":"/paper/2505.00366"},"observation_digest":"sha256:0b405f1e493220fe197f09f3db7b162cbe357af746ff85ab8a5b847927238c26","observation_id":"a30a5db4-a6f9-45c4-9d59-1865fd2879ff","resolution":{"observed_at":"2026-08-16T04:57:01.218331Z","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":"2026-08-16T04:57:02.258098Z","title":"Yoo, The basics of primordial black hole formation and abundance estimation , Galaxies 10 (2022)","venue":null,"work_id":"f9971f49-6df1-4f28-9c9a-1e370691fe6a","year":2022},"citing_paper":{"arxiv_id":"2505.00366","last_updated":"2025-05-01T07:37:06Z","snapshot_observed_at":"2026-08-16T11:18:43.918864Z","submitted_at":"2025-05-01T07:37:06Z","title":"Primordial black hole formation from a type II perturbation in the absence and presence of pressure","version":1},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-16T04:57:01.223828Z"},"links":{"citing_paper":"/paper/2505.00366"},"observation_digest":"sha256:abbaf1dc50a15244b6b3992b4f91db562d73b7fca79a1fef1a1dbf509ade5e93","observation_id":"9b0329e2-c2e1-4d6d-8977-8717c4f43a9d","resolution":{"observed_at":"2026-08-16T04:57:02.262505Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-16T04:57:02.240640Z","title":"Silk, Large-scale inhomogeneity of the universe: spherically symmetric models","venue":null,"work_id":"a75647f2-1d7f-44db-8a29-841e2c85abf6","year":1977},"citing_paper":{"arxiv_id":"2505.00366","last_updated":"2025-05-01T07:37:06Z","snapshot_observed_at":"2026-08-16T11:18:43.918864Z","submitted_at":"2025-05-01T07:37:06Z","title":"Primordial black hole formation from a type II perturbation in the absence and presence of pressure","version":1},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-08-16T04:57:01.228465Z"},"links":{"citing_paper":"/paper/2505.00366"},"observation_digest":"sha256:e29ea138e2a27bedf7a9b94cd11dff93df4ed11c0a11c912b94903207006793e","observation_id":"f7204342-dc16-45e4-b470-1c294a572172","resolution":{"observed_at":"2026-08-16T04:57:02.245724Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-16T04:57:02.225136Z","title":"Hayward, General laws of black-hole dynamics , Phys","venue":null,"work_id":"3108a0c3-e693-4f01-96d6-caafb2d16e9a","year":1994},"citing_paper":{"arxiv_id":"2505.00366","last_updated":"2025-05-01T07:37:06Z","snapshot_observed_at":"2026-08-16T11:18:43.918864Z","submitted_at":"2025-05-01T07:37:06Z","title":"Primordial black hole formation from a type II perturbation in the absence and presence of pressure","version":1},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-08-16T04:57:01.234559Z"},"links":{"citing_paper":"/paper/2505.00366"},"observation_digest":"sha256:da0cf0b4b5b0437b537e82c7a756cff0f6e898d9857076248c9ccfdd3e778bbb","observation_id":"67c5c1c2-d063-4147-baf8-36d8b9c256dd","resolution":{"observed_at":"2026-08-16T04:57:02.230969Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-16T04:57:02.207600Z","title":"Poisson, A relativist’s toolkit : the mathematics of black-hole mechanics , Cambridge University Press (2004)","venue":null,"work_id":"fecd1a7e-efad-4cbc-8af7-ce4bc9316d4e","year":2004},"citing_paper":{"arxiv_id":"2505.00366","last_updated":"2025-05-01T07:37:06Z","snapshot_observed_at":"2026-08-16T11:18:43.918864Z","submitted_at":"2025-05-01T07:37:06Z","title":"Primordial black hole formation from a type II perturbation in the absence and presence of pressure","version":1},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-08-16T04:57:01.242669Z"},"links":{"citing_paper":"/paper/2505.00366"},"observation_digest":"sha256:b8a1129260de777788896fa154035ea06974b926c2b8e216c3aaa515454c4ded","observation_id":"9c95efac-b328-43a8-bec0-afa4904a6018","resolution":{"observed_at":"2026-08-16T04:57:02.212675Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-16T04:57:02.192012Z","title":"Zeldovich and I.D","venue":null,"work_id":"cfd3e88c-2984-45ce-b773-b69226301faa","year":1983},"citing_paper":{"arxiv_id":"2505.00366","last_updated":"2025-05-01T07:37:06Z","snapshot_observed_at":"2026-08-16T11:18:43.918864Z","submitted_at":"2025-05-01T07:37:06Z","title":"Primordial black hole formation from a type II perturbation in the absence and presence of pressure","version":1},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-08-16T04:57:01.247010Z"},"links":{"citing_paper":"/paper/2505.00366"},"observation_digest":"sha256:9e88370421fd2088f6e2c3ee10602d56165456c0461342dff33e7876dfdd3fab","observation_id":"e66e50e6-7011-4d48-84e7-37a2e1a5af9e","resolution":{"observed_at":"2026-08-16T04:57:02.197039Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-16T04:57:01.252454Z","title":"Novikov and V.P","venue":null,"work_id":null,"year":1989},"citing_paper":{"arxiv_id":"2505.00366","last_updated":"2025-05-01T07:37:06Z","snapshot_observed_at":"2026-08-16T11:18:43.918864Z","submitted_at":"2025-05-01T07:37:06Z","title":"Primordial black hole formation from a type II perturbation in the absence and presence of pressure","version":1},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-08-16T04:57:01.252454Z"},"links":{"citing_paper":"/paper/2505.00366"},"observation_digest":"sha256:fc9e3435240d2d887a9bc2176c42409fc5cac8bba0589c2489e4623385584912","observation_id":"fb8873d8-50b0-40c2-9853-f0183ec6031d","resolution":{"observed_at":"2026-08-16T04:57:01.252454Z","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":"2026-08-16T04:57:01.257917Z","title":"Frolov and I.D","venue":null,"work_id":null,"year":1998},"citing_paper":{"arxiv_id":"2505.00366","last_updated":"2025-05-01T07:37:06Z","snapshot_observed_at":"2026-08-16T11:18:43.918864Z","submitted_at":"2025-05-01T07:37:06Z","title":"Primordial black hole formation from a type II perturbation in the absence and presence of pressure","version":1},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-08-16T04:57:01.257917Z"},"links":{"citing_paper":"/paper/2505.00366"},"observation_digest":"sha256:835e6d7d381c3d02f67a71fae88e32335bfd9baa3015e753ea09158adb41b97c","observation_id":"7cd418d7-9aa8-4f88-a0ea-b1d132dd827e","resolution":{"observed_at":"2026-08-16T04:57:01.257917Z","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":"2026-08-16T04:57:02.174795Z","title":"Zel’Dovich, Semiclosed Worlds in the General Theory of Relativity , Soviet Journal of Experimental and Theoretical Physics 16 (1963) 732","venue":null,"work_id":"877aac80-50cb-4b53-9845-912bbe346fce","year":1963},"citing_paper":{"arxiv_id":"2505.00366","last_updated":"2025-05-01T07:37:06Z","snapshot_observed_at":"2026-08-16T11:18:43.918864Z","submitted_at":"2025-05-01T07:37:06Z","title":"Primordial black hole formation from a type II perturbation in the absence and presence of pressure","version":1},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-08-16T04:57:01.262959Z"},"links":{"citing_paper":"/paper/2505.00366"},"observation_digest":"sha256:5f8b85a4745eb7ac61ad6509ce53f0b6a9b458ceddbfa11750b09d596604857c","observation_id":"fc1edad8-810f-4c0a-a964-a16fd2f948f8","resolution":{"observed_at":"2026-08-16T04:57:02.179967Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-16T04:57:02.156644Z","title":"Novikov, On the Evolution of a Semiclosed World , Soviet Ast","venue":null,"work_id":"b1361c1a-3fb7-4a80-8eb7-0b8aadfdee17","year":1964},"citing_paper":{"arxiv_id":"2505.00366","last_updated":"2025-05-01T07:37:06Z","snapshot_observed_at":"2026-08-16T11:18:43.918864Z","submitted_at":"2025-05-01T07:37:06Z","title":"Primordial black hole formation from a type II perturbation in the absence and presence of pressure","version":1},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-08-16T04:57:01.268206Z"},"links":{"citing_paper":"/paper/2505.00366"},"observation_digest":"sha256:e44e5d0fda9ceef6d7f8894d9c61171b658ffb889db45ef4d8a2dd39c759d670","observation_id":"16d2fabd-0b34-4be4-94b0-571d1b5f415a","resolution":{"observed_at":"2026-08-16T04:57:02.162615Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-16T04:57:02.125346Z","title":"Gourgoulhon, Geometry and physics of black holes , 2022","venue":null,"work_id":"3fe92c3d-3e84-41d2-94fd-1ea9c3ee7ca0","year":2022},"citing_paper":{"arxiv_id":"2505.00366","last_updated":"2025-05-01T07:37:06Z","snapshot_observed_at":"2026-08-16T11:18:43.918864Z","submitted_at":"2025-05-01T07:37:06Z","title":"Primordial black hole formation from a type II perturbation in the absence and presence of pressure","version":1},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-08-16T04:57:01.273980Z"},"links":{"citing_paper":"/paper/2505.00366"},"observation_digest":"sha256:61d0ae1481a3b558cb95a6db355949f75244c8cd7486af073ebcda792bfceb33","observation_id":"6ee9c934-951d-48dd-a1be-df5c6cef4bae","resolution":{"observed_at":"2026-08-16T04:57:02.142251Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2403.11147","last_updated":"2024-04-26T01:30:36Z","snapshot_observed_at":"2026-08-16T14:09:06.533684Z","submitted_at":"2024-03-17T08:53:59Z","title":"Primordial black hole formation from a nonspherical density profile with a misaligned deformation tensor","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2403.11147","snapshot_observed_at":"2026-08-16T04:57:01.280071Z","title":"Yoo, Primordial black hole formation from a nonspherical density profile with a misaligned deformation tensor , Phys","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2505.00366","last_updated":"2025-05-01T07:37:06Z","snapshot_observed_at":"2026-08-16T11:18:43.918864Z","submitted_at":"2025-05-01T07:37:06Z","title":"Primordial black hole formation from a type II perturbation in the absence and presence of pressure","version":1},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-08-16T04:57:01.280071Z"},"links":{"cited_paper":"/paper/2403.11147","citing_paper":"/paper/2505.00366"},"observation_digest":"sha256:fee01158f0f7b2f0028377d964cd8949a90a13caed35418e32f7fc13a89ac523","observation_id":"969d99b9-46d8-4a5c-874d-9edb66e34e5e","resolution":{"observed_at":"2026-08-16T04:57:01.280071Z","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":"2026-08-16T04:57:02.102580Z","title":null,"venue":null,"work_id":"7e52d641-bea5-4705-be95-ad610a6f0e68","year":2022},"citing_paper":{"arxiv_id":"2505.00366","last_updated":"2025-05-01T07:37:06Z","snapshot_observed_at":"2026-08-16T11:18:43.918864Z","submitted_at":"2025-05-01T07:37:06Z","title":"Primordial black hole formation from a type II perturbation in the absence and presence of pressure","version":1},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-08-16T04:57:01.285116Z"},"links":{"citing_paper":"/paper/2505.00366"},"observation_digest":"sha256:084b26fdf20228dc58e60dee2f92d4428079ef9b09ae795fa4cb346be8499ca7","observation_id":"047be7b4-7a93-4285-9b60-236159ffd110","resolution":{"observed_at":"2026-08-16T04:57:02.108365Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-16T04:57:02.084333Z","title":null,"venue":null,"work_id":"b97a4fbf-bbad-4ce6-8cf8-928517aed67a","year":2013},"citing_paper":{"arxiv_id":"2505.00366","last_updated":"2025-05-01T07:37:06Z","snapshot_observed_at":"2026-08-16T11:18:43.918864Z","submitted_at":"2025-05-01T07:37:06Z","title":"Primordial black hole formation from a type II perturbation in the absence and presence of pressure","version":1},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-08-16T04:57:01.292393Z"},"links":{"citing_paper":"/paper/2505.00366"},"observation_digest":"sha256:afb61018b441f9511cc738372cdaad4d14cecce9f184ab0b2600a781905d5ae4","observation_id":"cf641b10-a115-420e-b53a-9340de999f9f","resolution":{"observed_at":"2026-08-16T04:57:02.089675Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-16T04:57:02.069155Z","title":"Okawa, H","venue":null,"work_id":"b5820888-face-4b6d-85be-8d510580f143","year":2014},"citing_paper":{"arxiv_id":"2505.00366","last_updated":"2025-05-01T07:37:06Z","snapshot_observed_at":"2026-08-16T11:18:43.918864Z","submitted_at":"2025-05-01T07:37:06Z","title":"Primordial black hole formation from a type II perturbation in the absence and presence of pressure","version":1},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-08-16T04:57:01.300839Z"},"links":{"citing_paper":"/paper/2505.00366"},"observation_digest":"sha256:5be45b66fb0c22819e0457ada0c1ccd18df5182ecd4255331e351b0079976457","observation_id":"c9d39f58-d4d7-4a19-9b10-200d98b9c3b6","resolution":{"observed_at":"2026-08-16T04:57:02.073503Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1201.2379","last_updated":"2013-04-11T19:25:38Z","snapshot_observed_at":"2026-08-15T04:22:44.507793Z","submitted_at":"2012-01-11T19:03:42Z","title":"Primordial black hole formation in the early universe: critical behaviour and self-similarity","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1201.2379","snapshot_observed_at":"2026-08-16T04:57:01.305509Z","title":"Musco and J.C","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2505.00366","last_updated":"2025-05-01T07:37:06Z","snapshot_observed_at":"2026-08-16T11:18:43.918864Z","submitted_at":"2025-05-01T07:37:06Z","title":"Primordial black hole formation from a type II perturbation in the absence and presence of pressure","version":1},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-08-16T04:57:01.305509Z"},"links":{"cited_paper":"/paper/1201.2379","citing_paper":"/paper/2505.00366"},"observation_digest":"sha256:97405abe9bfe66d69bd1de5900461f9f58d3d3e7408131c6759e276d2cdf42c9","observation_id":"d1f0c281-52d7-4b48-97f8-e716fe272c40","resolution":{"observed_at":"2026-08-16T04:57:01.305509Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2007.05564","last_updated":"2020-11-16T17:08:34Z","snapshot_observed_at":"2026-08-13T22:09:51.204942Z","submitted_at":"2020-07-10T18:38:51Z","title":"Analytical thresholds for black hole formation in general cosmological backgrounds","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2007.05564","snapshot_observed_at":"2026-08-16T04:57:01.316472Z","title":"Escriv` a, C","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2505.00366","last_updated":"2025-05-01T07:37:06Z","snapshot_observed_at":"2026-08-16T11:18:43.918864Z","submitted_at":"2025-05-01T07:37:06Z","title":"Primordial black hole formation from a type II perturbation in the absence and presence of pressure","version":1},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-08-16T04:57:01.316472Z"},"links":{"cited_paper":"/paper/2007.05564","citing_paper":"/paper/2505.00366"},"observation_digest":"sha256:aad8fd76e89474204aa81facbc4d5c8f77a0274f58c3a975137819550f334092","observation_id":"9fffe4ac-bc71-4449-a21b-50a21fffe089","resolution":{"observed_at":"2026-08-16T04:57:01.316472Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"2505.00366","last_updated":"2025-05-01T07:37:06Z","latest_version":1,"primary_category":"gr-qc","snapshot_observed_at":"2026-08-16T11:18:43.918864Z","submitted_at":"2025-05-01T07:37:06Z","title":"Primordial black hole formation from a type II perturbation in the absence and presence of pressure"},"reference_resolution":{"displayed":53,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":25,"verified_exact":4,"verified_fuzzy":24},"total_outbound_references":53},"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":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"thesis":"As of 17 August 2026, this Paper Citation Record lists 53 of 53 outbound references and 1 inbound Pith citation observation for arXiv:2505.00366."}