{"as_of":"2026-08-07T02:29:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:215e922b1d8a6d2cba5bfd6abcb38dc4a9bf55776a50480f99eb6efcb7ce4170","coverage":[{"denominator":0,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":0,"source":"paper_references, paper_reference_links","source_observed_at":null,"state":"measured"},{"denominator":21,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":21,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-06T06:34:29.942622+00:00","state":"measured"},{"denominator":21,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":21,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-05T15:54:20.945129Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"pith","source_observed_at":"2026-07-10T02:26:43.016930Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"1904.00984","last_updated":"2019-11-14T11:42:21Z","snapshot_observed_at":"2026-08-05T18:53:21.194461Z","submitted_at":"2019-04-01T17:46:05Z","title":"Primordial black hole formation and abundance: contribution from the non-linear relation between the density and curvature perturbation","version":2},"cited_work":{"arxiv_id":"1904.00984","doi":null,"metadata_source":"pith","pith_arxiv_id":"1904.00984","snapshot_observed_at":"2026-07-10T02:26:43.016930Z","title":"Young, I","venue":"astro-ph.CO","work_id":"1ba0f722-9b79-4407-8a4f-20872bf16ce5","year":2019},"citing_paper":{"arxiv_id":"2109.01398","last_updated":"2021-11-05T08:11:41Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2021-09-03T09:44:21Z","title":"Scalar induced gravitational waves review","version":2},"reference_index":222,"source":"pdf_text","source_observed_at":"2026-05-17T07:57:52.725198Z"},"links":{"cited_paper":"/paper/1904.00984","citing_paper":"/paper/2109.01398"},"observation_digest":"sha256:bd7f216aaa32483e5630c1ea565e5b2e58f26614a62000b5037823317cef26da","observation_id":"9a22626b-8e7a-4857-803b-1ad8b93bbacc","resolution":{"observed_at":"2026-05-17T07:59:16.888026Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1904.00984","last_updated":"2019-11-14T11:42:21Z","snapshot_observed_at":"2026-08-05T18:53:21.194461Z","submitted_at":"2019-04-01T17:46:05Z","title":"Primordial black hole formation and abundance: contribution from the non-linear relation between the density and curvature perturbation","version":2},"cited_work":{"arxiv_id":"1904.00984","doi":null,"metadata_source":"pith","pith_arxiv_id":"1904.00984","snapshot_observed_at":"2026-07-10T02:26:43.016930Z","title":"Young, I","venue":"astro-ph.CO","work_id":"1ba0f722-9b79-4407-8a4f-20872bf16ce5","year":2019},"citing_paper":{"arxiv_id":"2503.01962","last_updated":"2026-05-06T17:35:03Z","snapshot_observed_at":"2026-07-06T20:45:59.818273Z","submitted_at":"2025-03-03T19:00:01Z","title":"Curvature Perturbations from First-Order Phase Transitions: Implications to Black Holes and Gravitational Waves","version":2},"reference_index":77,"source":"pdf_text","source_observed_at":"2026-05-23T01:19:15.263346Z"},"links":{"cited_paper":"/paper/1904.00984","citing_paper":"/paper/2503.01962"},"observation_digest":"sha256:e65cd9995a6488ca77d3cbfd9e38232c596a7ff4dd87c1286bac500e7d7a62f3","observation_id":"2ff4de64-8548-404f-8d60-5b354960277e","resolution":{"observed_at":"2026-05-23T01:22:21.040494Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1904.00984","last_updated":"2019-11-14T11:42:21Z","snapshot_observed_at":"2026-08-05T18:53:21.194461Z","submitted_at":"2019-04-01T17:46:05Z","title":"Primordial black hole formation and abundance: contribution from the non-linear relation between the density and curvature perturbation","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1904.00984","snapshot_observed_at":"2026-08-05T15:54:20.945129Z","title":"Young, I","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2508.19328","last_updated":"2026-06-02T10:21:11Z","snapshot_observed_at":"2026-08-06T11:12:02.586056Z","submitted_at":"2025-08-26T18:00:00Z","title":"Implications for Pulsar Timing Arrays of Sub-solar Black Hole Detections: From LVK to Einstein Telescope and Cosmic Explorer","version":2},"reference_index":138,"source":"pdf_text","source_observed_at":"2026-08-05T15:54:20.945129Z"},"links":{"cited_paper":"/paper/1904.00984","citing_paper":"/paper/2508.19328"},"observation_digest":"sha256:eb55d9621ab33c01fe9e1d949b7138dbf58d0d50728cdc776890a9f2202540ad","observation_id":"33d8bbc9-fa1e-4e27-ba07-a27aa10bb757","resolution":{"observed_at":"2026-08-05T15:54:20.945129Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1904.00984","last_updated":"2019-11-14T11:42:21Z","snapshot_observed_at":"2026-08-05T18:53:21.194461Z","submitted_at":"2019-04-01T17:46:05Z","title":"Primordial black hole formation and abundance: contribution from the non-linear relation between the density and curvature perturbation","version":2},"cited_work":{"arxiv_id":"1904.00984","doi":null,"metadata_source":"pith","pith_arxiv_id":"1904.00984","snapshot_observed_at":"2026-07-10T02:26:43.016930Z","title":"Young, I","venue":"astro-ph.CO","work_id":"1ba0f722-9b79-4407-8a4f-20872bf16ce5","year":2019},"citing_paper":{"arxiv_id":"2512.07284","last_updated":"2026-04-07T04:55:32Z","snapshot_observed_at":"2026-07-06T22:38:03.983093Z","submitted_at":"2025-12-08T08:22:17Z","title":"Evaporation of Primordial Black Holes in a Thermal Universe: A Thermofield Dynamics Approach","version":2},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-05-17T01:22:45.340376Z"},"links":{"cited_paper":"/paper/1904.00984","citing_paper":"/paper/2512.07284"},"observation_digest":"sha256:b7e5050a4eae9a9df561c638f2b2b36bb52dcb03a0402072abda7ac388eb4691","observation_id":"c6d17d90-ad4b-420b-b619-df89013d373a","resolution":{"observed_at":"2026-05-17T01:23:49.348782Z","resolver_source":"arxiv_id","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1904.00984","last_updated":"2019-11-14T11:42:21Z","snapshot_observed_at":"2026-08-05T18:53:21.194461Z","submitted_at":"2019-04-01T17:46:05Z","title":"Primordial black hole formation and abundance: contribution from the non-linear relation between the density and curvature perturbation","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1904.00984","snapshot_observed_at":"2026-08-03T18:08:22.564763Z","title":"Primordial black hole formation and abundance: contribution from the non-linear relation between the density and curvature perturbation,","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2512.07291","last_updated":"2026-07-24T05:07:32Z","snapshot_observed_at":"2026-08-04T03:47:00.493724Z","submitted_at":"2025-12-08T08:31:25Z","title":"Revisiting PBH accretion, evaporation and their cosmological consequences","version":2},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-03T18:08:22.564763Z"},"links":{"cited_paper":"/paper/1904.00984","citing_paper":"/paper/2512.07291"},"observation_digest":"sha256:4d4549da33b77166cfef6d5051b6903b101db621a53318a2c8ed6e894654d890","observation_id":"0ecd09e0-fe40-4df6-98e6-8cc1d60d67fc","resolution":{"observed_at":"2026-08-03T18:08:22.564763Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1904.00984","last_updated":"2019-11-14T11:42:21Z","snapshot_observed_at":"2026-08-05T18:53:21.194461Z","submitted_at":"2019-04-01T17:46:05Z","title":"Primordial black hole formation and abundance: contribution from the non-linear relation between the density and curvature perturbation","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1904.00984","snapshot_observed_at":"2026-08-03T14:43:18.066415Z","title":"Young, I","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2512.19668","last_updated":"2026-06-01T10:28:28Z","snapshot_observed_at":"2026-08-05T18:41:19.493542Z","submitted_at":"2025-12-22T18:48:00Z","title":"Are Primordial Black Holes Truly Fine-Tuned?","version":2},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-08-03T14:43:18.066415Z"},"links":{"cited_paper":"/paper/1904.00984","citing_paper":"/paper/2512.19668"},"observation_digest":"sha256:fcc905a533512521d7500a6735cca2e29a288123c56928c8207098948b80c336","observation_id":"d8c64898-d26d-4b52-8d50-00cd72633721","resolution":{"observed_at":"2026-08-03T14:43:18.066415Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1904.00984","last_updated":"2019-11-14T11:42:21Z","snapshot_observed_at":"2026-08-05T18:53:21.194461Z","submitted_at":"2019-04-01T17:46:05Z","title":"Primordial black hole formation and abundance: contribution from the non-linear relation between the density and curvature perturbation","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1904.00984","snapshot_observed_at":"2026-08-04T06:39:32.059192Z","title":"Young, I","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2512.25044","last_updated":"2026-08-01T19:36:03Z","snapshot_observed_at":"2026-08-06T23:24:03.575290Z","submitted_at":"2025-12-31T18:39:54Z","title":"Primordial black hole dark matter from ultra-slow-roll inflation in Horndeski gravity","version":2},"reference_index":77,"source":"pdf_text","source_observed_at":"2026-08-04T06:39:32.059192Z"},"links":{"cited_paper":"/paper/1904.00984","citing_paper":"/paper/2512.25044"},"observation_digest":"sha256:33fc6aec2eec33f95d969f63db4c8617216ea496bc30222772a6b241f5773b2e","observation_id":"dabfc401-f271-4dce-b550-7db5158e981c","resolution":{"observed_at":"2026-08-04T06:39:32.059192Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1904.00984","last_updated":"2019-11-14T11:42:21Z","snapshot_observed_at":"2026-08-05T18:53:21.194461Z","submitted_at":"2019-04-01T17:46:05Z","title":"Primordial black hole formation and abundance: contribution from the non-linear relation between the density and curvature perturbation","version":2},"cited_work":{"arxiv_id":"1904.00984","doi":null,"metadata_source":"pith","pith_arxiv_id":"1904.00984","snapshot_observed_at":"2026-07-10T02:26:43.016930Z","title":"Young, I","venue":"astro-ph.CO","work_id":"1ba0f722-9b79-4407-8a4f-20872bf16ce5","year":2019},"citing_paper":{"arxiv_id":"2604.20063","last_updated":"2026-07-24T11:06:14Z","snapshot_observed_at":"2026-08-02T15:56:53.680056Z","submitted_at":"2026-04-21T23:58:51Z","title":"Purely quadratic non-Gaussianity from tachyonic instability: Primordial black holes and scalar-induced gravitational waves","version":2},"reference_index":127,"source":"pdf_text","source_observed_at":"2026-05-10T00:55:18.764549Z"},"links":{"cited_paper":"/paper/1904.00984","citing_paper":"/paper/2604.20063"},"observation_digest":"sha256:043dfc4222abbf34ce6844f265219bfa5e25c09e0cca16a0a5dddeeb753a5f2b","observation_id":"12050c95-6923-4847-b8ca-a4bf9b517ac4","resolution":{"observed_at":"2026-05-10T01:04:50.530492Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1904.00984","last_updated":"2019-11-14T11:42:21Z","snapshot_observed_at":"2026-08-05T18:53:21.194461Z","submitted_at":"2019-04-01T17:46:05Z","title":"Primordial black hole formation and abundance: contribution from the non-linear relation between the density and curvature perturbation","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1904.00984","snapshot_observed_at":"2026-08-02T15:57:06.860244Z","title":"Young, I","venue":null,"work_id":null,"year":1904},"citing_paper":{"arxiv_id":"2604.20063","last_updated":"2026-07-24T11:06:14Z","snapshot_observed_at":"2026-08-02T15:56:53.680056Z","submitted_at":"2026-04-21T23:58:51Z","title":"Purely quadratic non-Gaussianity from tachyonic instability: Primordial black holes and scalar-induced gravitational waves","version":3},"reference_index":127,"source":"pdf_text","source_observed_at":"2026-08-02T15:57:06.860244Z"},"links":{"cited_paper":"/paper/1904.00984","citing_paper":"/paper/2604.20063"},"observation_digest":"sha256:845ad28735a2491ba146968b82f57872f714d6c01fa3dd384caa5200f68b2442","observation_id":"9b5b8553-c744-4970-92c8-92d588db2b9a","resolution":{"observed_at":"2026-08-02T15:57:06.860244Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1904.00984","last_updated":"2019-11-14T11:42:21Z","snapshot_observed_at":"2026-08-05T18:53:21.194461Z","submitted_at":"2019-04-01T17:46:05Z","title":"Primordial black hole formation and abundance: contribution from the non-linear relation between the density and curvature perturbation","version":2},"cited_work":{"arxiv_id":"1904.00984","doi":null,"metadata_source":"pith","pith_arxiv_id":"1904.00984","snapshot_observed_at":"2026-07-10T02:26:43.016930Z","title":"Young, I","venue":"astro-ph.CO","work_id":"1ba0f722-9b79-4407-8a4f-20872bf16ce5","year":2019},"citing_paper":{"arxiv_id":"2604.26005","last_updated":"2026-04-28T18:00:03Z","snapshot_observed_at":"2026-07-06T23:11:43.764239Z","submitted_at":"2026-04-28T18:00:03Z","title":"Asteroid-mass Primordial Black Holes as Dark Matter from Supersymmetry","version":1},"reference_index":87,"source":"pdf_text","source_observed_at":"2026-05-07T15:51:05.674217Z"},"links":{"cited_paper":"/paper/1904.00984","citing_paper":"/paper/2604.26005"},"observation_digest":"sha256:44bf2a5ba54b1a53141e9ed12c7b1c79e9accb427d89bc583283b2faa3258f6b","observation_id":"89c1a69d-9ea1-41fc-944b-c91ace42c0f0","resolution":{"observed_at":"2026-05-12T00:06:16.482512Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1904.00984","last_updated":"2019-11-14T11:42:21Z","snapshot_observed_at":"2026-08-05T18:53:21.194461Z","submitted_at":"2019-04-01T17:46:05Z","title":"Primordial black hole formation and abundance: contribution from the non-linear relation between the density and curvature perturbation","version":2},"cited_work":{"arxiv_id":"1904.00984","doi":null,"metadata_source":"pith","pith_arxiv_id":"1904.00984","snapshot_observed_at":"2026-07-10T02:26:43.016930Z","title":"Young, I","venue":"astro-ph.CO","work_id":"1ba0f722-9b79-4407-8a4f-20872bf16ce5","year":2019},"citing_paper":{"arxiv_id":"2604.27496","last_updated":"2026-04-30T06:49:42Z","snapshot_observed_at":"2026-07-06T23:12:57.730833Z","submitted_at":"2026-04-30T06:49:42Z","title":"Primordial black hole dark matter from axion inflation","version":1},"reference_index":56,"source":"pdf_text","source_observed_at":"2026-05-07T09:07:09.900700Z"},"links":{"cited_paper":"/paper/1904.00984","citing_paper":"/paper/2604.27496"},"observation_digest":"sha256:b835eae4a1393a60da951d34ede58c4c271f1d00fd329ff19633c7d2bce5397c","observation_id":"aa2afe38-6a3b-439c-a815-fbe34e7575af","resolution":{"observed_at":"2026-05-12T09:51:26.976402Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1904.00984","last_updated":"2019-11-14T11:42:21Z","snapshot_observed_at":"2026-08-05T18:53:21.194461Z","submitted_at":"2019-04-01T17:46:05Z","title":"Primordial black hole formation and abundance: contribution from the non-linear relation between the density and curvature perturbation","version":2},"cited_work":{"arxiv_id":"1904.00984","doi":null,"metadata_source":"pith","pith_arxiv_id":"1904.00984","snapshot_observed_at":"2026-07-10T02:26:43.016930Z","title":"Young, I","venue":"astro-ph.CO","work_id":"1ba0f722-9b79-4407-8a4f-20872bf16ce5","year":2019},"citing_paper":{"arxiv_id":"2605.13042","last_updated":"2026-05-13T05:54:23Z","snapshot_observed_at":"2026-07-06T23:24:37.915639Z","submitted_at":"2026-05-13T05:54:23Z","title":"The Gravitational Spectral Radio Forest: A Signature of Primordial Black Holes","version":1},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-05-14T19:08:52.224510Z"},"links":{"cited_paper":"/paper/1904.00984","citing_paper":"/paper/2605.13042"},"observation_digest":"sha256:1263609c1082b1b92de30da3204804f4e6d5b5f9c18c353a55846aa3628cf5f3","observation_id":"4793d45e-8e0d-4ecc-ad36-43dfa3945498","resolution":{"observed_at":"2026-05-14T19:09:23.114398Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1904.00984","last_updated":"2019-11-14T11:42:21Z","snapshot_observed_at":"2026-08-05T18:53:21.194461Z","submitted_at":"2019-04-01T17:46:05Z","title":"Primordial black hole formation and abundance: contribution from the non-linear relation between the density and curvature perturbation","version":2},"cited_work":{"arxiv_id":"1904.00984","doi":null,"metadata_source":"pith","pith_arxiv_id":"1904.00984","snapshot_observed_at":"2026-07-10T02:26:43.016930Z","title":"Young, I","venue":"astro-ph.CO","work_id":"1ba0f722-9b79-4407-8a4f-20872bf16ce5","year":2019},"citing_paper":{"arxiv_id":"2605.15197","last_updated":"2026-07-29T13:49:49Z","snapshot_observed_at":"2026-08-02T14:03:29.096476Z","submitted_at":"2026-05-14T17:59:55Z","title":"Primordial Black Hole from Tensor-induced Density Fluctuation: First-order Phase Transitions and Domain Walls","version":1},"reference_index":158,"source":"pdf_text","source_observed_at":"2026-05-15T02:53:41.149271Z"},"links":{"cited_paper":"/paper/1904.00984","citing_paper":"/paper/2605.15197"},"observation_digest":"sha256:7c7d58aacf115866acea6bfa6eda413b886ea8848aa180501dab116dcecde753","observation_id":"c2a9fe5b-e0d4-461d-a0a1-083653126318","resolution":{"observed_at":"2026-05-15T02:59:41.894699Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1904.00984","last_updated":"2019-11-14T11:42:21Z","snapshot_observed_at":"2026-08-05T18:53:21.194461Z","submitted_at":"2019-04-01T17:46:05Z","title":"Primordial black hole formation and abundance: contribution from the non-linear relation between the density and curvature perturbation","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1904.00984","snapshot_observed_at":"2026-08-02T14:03:44.623702Z","title":"Young, I","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2605.15197","last_updated":"2026-07-29T13:49:49Z","snapshot_observed_at":"2026-08-02T14:03:29.096476Z","submitted_at":"2026-05-14T17:59:55Z","title":"Primordial Black Hole from Tensor-induced Density Fluctuation: First-order Phase Transitions and Domain Walls","version":2},"reference_index":158,"source":"pdf_text","source_observed_at":"2026-08-02T14:03:44.623702Z"},"links":{"cited_paper":"/paper/1904.00984","citing_paper":"/paper/2605.15197"},"observation_digest":"sha256:0254dc6125ebaee6c080667150a52054116f85178ee667490f88136f62aa1281","observation_id":"ff8bbcf0-f0b5-49e4-8c45-faf6b68846f3","resolution":{"observed_at":"2026-08-02T14:03:44.623702Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1904.00984","last_updated":"2019-11-14T11:42:21Z","snapshot_observed_at":"2026-08-05T18:53:21.194461Z","submitted_at":"2019-04-01T17:46:05Z","title":"Primordial black hole formation and abundance: contribution from the non-linear relation between the density and curvature perturbation","version":2},"cited_work":{"arxiv_id":"1904.00984","doi":null,"metadata_source":"pith","pith_arxiv_id":"1904.00984","snapshot_observed_at":"2026-07-10T02:26:43.016930Z","title":"Young, I","venue":"astro-ph.CO","work_id":"1ba0f722-9b79-4407-8a4f-20872bf16ce5","year":2019},"citing_paper":{"arxiv_id":"2605.21474","last_updated":"2026-05-20T17:55:24Z","snapshot_observed_at":"2026-08-02T11:46:02.728077Z","submitted_at":"2026-05-20T17:55:24Z","title":"Gravitational Waves from Black Hole Reheating: The Scalar-Induced Component","version":1},"reference_index":267,"source":"pdf_text","source_observed_at":"2026-05-21T03:29:26.870369Z"},"links":{"cited_paper":"/paper/1904.00984","citing_paper":"/paper/2605.21474"},"observation_digest":"sha256:8df85d560e2233b4391f1e9dfc1286c88ac28da47a2b2c0db14d69a7f038610d","observation_id":"0e3f97c7-205a-4449-9725-308c4acfd49d","resolution":{"observed_at":"2026-05-21T03:29:29.109670Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1904.00984","last_updated":"2019-11-14T11:42:21Z","snapshot_observed_at":"2026-08-05T18:53:21.194461Z","submitted_at":"2019-04-01T17:46:05Z","title":"Primordial black hole formation and abundance: contribution from the non-linear relation between the density and curvature perturbation","version":2},"cited_work":{"arxiv_id":"1904.00984","doi":null,"metadata_source":"pith","pith_arxiv_id":"1904.00984","snapshot_observed_at":"2026-07-10T02:26:43.016930Z","title":"Young, I","venue":"astro-ph.CO","work_id":"1ba0f722-9b79-4407-8a4f-20872bf16ce5","year":2019},"citing_paper":{"arxiv_id":"2605.21477","last_updated":"2026-05-20T17:57:36Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-05-20T17:57:36Z","title":"Opening the Window of Ultra-Light PBHs by Exorcising the Poltergeist","version":1},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-05-21T03:23:33.652171Z"},"links":{"cited_paper":"/paper/1904.00984","citing_paper":"/paper/2605.21477"},"observation_digest":"sha256:0d4a723a88801fc7e30853bed891f44c7e92b1839b5ff6e20dce536583a10ec3","observation_id":"121bfe10-08da-4b29-9965-9225320f98a4","resolution":{"observed_at":"2026-05-21T03:23:55.476655Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1904.00984","last_updated":"2019-11-14T11:42:21Z","snapshot_observed_at":"2026-08-05T18:53:21.194461Z","submitted_at":"2019-04-01T17:46:05Z","title":"Primordial black hole formation and abundance: contribution from the non-linear relation between the density and curvature perturbation","version":2},"cited_work":{"arxiv_id":"1904.00984","doi":null,"metadata_source":"pith","pith_arxiv_id":"1904.00984","snapshot_observed_at":"2026-07-10T02:26:43.016930Z","title":"Young, I","venue":"astro-ph.CO","work_id":"1ba0f722-9b79-4407-8a4f-20872bf16ce5","year":2019},"citing_paper":{"arxiv_id":"2606.23846","last_updated":"2026-08-04T11:29:48Z","snapshot_observed_at":"2026-08-07T02:25:40.431062Z","submitted_at":"2026-06-22T18:29:10Z","title":"Primordial Black Holes: A Review of Formation and Evolution","version":1},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-06-26T07:13:12.429183Z"},"links":{"cited_paper":"/paper/1904.00984","citing_paper":"/paper/2606.23846"},"observation_digest":"sha256:fc1773a5d602d77b03686a9ea5ce4d0829f4eaa8b7920c0dbb83401ca4f00269","observation_id":"2a47726a-6cf6-4c13-8dd6-750a3c794b7c","resolution":{"observed_at":"2026-07-04T12:09:49.028890Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1904.00984","last_updated":"2019-11-14T11:42:21Z","snapshot_observed_at":"2026-08-05T18:53:21.194461Z","submitted_at":"2019-04-01T17:46:05Z","title":"Primordial black hole formation and abundance: contribution from the non-linear relation between the density and curvature perturbation","version":2},"cited_work":{"arxiv_id":"1904.00984","doi":null,"metadata_source":"pith","pith_arxiv_id":"1904.00984","snapshot_observed_at":"2026-07-10T02:26:43.016930Z","title":"Young, I","venue":"astro-ph.CO","work_id":"1ba0f722-9b79-4407-8a4f-20872bf16ce5","year":2019},"citing_paper":{"arxiv_id":"2607.01818","last_updated":"2026-07-17T07:29:52Z","snapshot_observed_at":"2026-08-03T17:46:08.224981Z","submitted_at":"2026-07-02T07:30:54Z","title":"Gravitational Waves from Primordial Black Holes: Connecting Low-Frequency Scalar-Induced Signatures to High-Frequency Binary Mergers","version":1},"reference_index":58,"source":"pdf_text","source_observed_at":"2026-07-03T07:00:45.003745Z"},"links":{"cited_paper":"/paper/1904.00984","citing_paper":"/paper/2607.01818"},"observation_digest":"sha256:2369715cc56ca8945cd25be58330f1d2fd7dd13dd98b547fb5bbf35a577cecc2","observation_id":"aa71c761-3d7c-4020-a035-d78bae5618a0","resolution":{"observed_at":"2026-07-03T07:07:44.390420Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1904.00984","last_updated":"2019-11-14T11:42:21Z","snapshot_observed_at":"2026-08-05T18:53:21.194461Z","submitted_at":"2019-04-01T17:46:05Z","title":"Primordial black hole formation and abundance: contribution from the non-linear relation between the density and curvature perturbation","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1904.00984","snapshot_observed_at":"2026-08-02T09:09:17.229883Z","title":"Young, I","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2607.01818","last_updated":"2026-07-17T07:29:52Z","snapshot_observed_at":"2026-08-03T17:46:08.224981Z","submitted_at":"2026-07-02T07:30:54Z","title":"Gravitational Waves from Primordial Black Holes: Connecting Low-Frequency Scalar-Induced Signatures to High-Frequency Binary Mergers","version":2},"reference_index":158,"source":"pdf_text","source_observed_at":"2026-08-02T09:09:17.229883Z"},"links":{"cited_paper":"/paper/1904.00984","citing_paper":"/paper/2607.01818"},"observation_digest":"sha256:b81c7ef94403e269d8f58e1b7d7dac5fd1da22b858130b694ad2df35e45e19a5","observation_id":"dd1caf1b-78ad-4f17-bd8f-be5219f21a1e","resolution":{"observed_at":"2026-08-02T09:09:17.229883Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1904.00984","last_updated":"2019-11-14T11:42:21Z","snapshot_observed_at":"2026-08-05T18:53:21.194461Z","submitted_at":"2019-04-01T17:46:05Z","title":"Primordial black hole formation and abundance: contribution from the non-linear relation between the density and curvature perturbation","version":2},"cited_work":{"arxiv_id":"1904.00984","doi":null,"metadata_source":"pith","pith_arxiv_id":"1904.00984","snapshot_observed_at":"2026-07-10T02:26:43.016930Z","title":"Young, I","venue":"astro-ph.CO","work_id":"1ba0f722-9b79-4407-8a4f-20872bf16ce5","year":2019},"citing_paper":{"arxiv_id":"2607.08738","last_updated":"2026-07-30T05:09:26Z","snapshot_observed_at":"2026-08-06T23:53:21.521039Z","submitted_at":"2026-07-09T17:39:27Z","title":"The statistics of curvature-profile dispersion in primordial black hole formation","version":1},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-07-10T02:22:09.448925Z"},"links":{"cited_paper":"/paper/1904.00984","citing_paper":"/paper/2607.08738"},"observation_digest":"sha256:5425043f04035f662ce569d4cd0848bcd1c6a63abafc3d4b1ce57aab968bc02d","observation_id":"b7e8a989-5d84-4902-b1b6-b074e1d4524d","resolution":{"observed_at":"2026-07-10T02:26:43.018253Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1904.00984","last_updated":"2019-11-14T11:42:21Z","snapshot_observed_at":"2026-08-05T18:53:21.194461Z","submitted_at":"2019-04-01T17:46:05Z","title":"Primordial black hole formation and abundance: contribution from the non-linear relation between the density and curvature perturbation","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1904.00984","snapshot_observed_at":"2026-08-02T07:53:09.540521Z","title":"Young, I","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2607.08738","last_updated":"2026-07-30T05:09:26Z","snapshot_observed_at":"2026-08-06T23:53:21.521039Z","submitted_at":"2026-07-09T17:39:27Z","title":"The statistics of curvature-profile dispersion in primordial black hole formation","version":2},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-08-02T07:53:09.540521Z"},"links":{"cited_paper":"/paper/1904.00984","citing_paper":"/paper/2607.08738"},"observation_digest":"sha256:c2711a1fbb7cc6a9ba50d0620d9c8e90e33577bbf9414a83729e4fb2828369a8","observation_id":"961b1d5a-546f-4933-ab59-d9156bfb36e4","resolution":{"observed_at":"2026-08-02T07:53:09.540521Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/1904.00984/citation-record","integrity":"/paper/1904.00984/integrity","json":"/paper/1904.00984/citation-record.json","paper":"/paper/1904.00984"},"outbound":[],"paper":{"arxiv_id":"1904.00984","last_updated":"2019-11-14T11:42:21Z","latest_version":2,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-08-05T18:53:21.194461Z","submitted_at":"2019-04-01T17:46:05Z","title":"Primordial black hole formation and abundance: contribution from the non-linear relation between the density and curvature perturbation"},"reference_resolution":{"displayed":0,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":0,"verified_exact":0,"verified_fuzzy":0},"total_outbound_references":0},"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":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"thesis":"As of 7 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 21 inbound Pith citation observations for arXiv:1904.00984."}