{"as_of":"2026-08-17T16:30:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:d00b9b4d925794d2fddd9d551b17f885617c2b71517f43600b7b985cc838f90b","coverage":[{"denominator":63,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":63,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-15T21:01:48.011553Z","state":"measured"},{"denominator":63,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":63,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-17T06:30:58.91139+00:00","state":"measured"},{"denominator":0,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":0,"source":"paper_references, paper_reference_links","source_observed_at":null,"state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"cited_works","source_observed_at":null,"state":"measured"}],"external_citation_measurements":[],"inbound":[],"links":{"evidence":"/evidence","html":"/paper/2505.11591/citation-record","integrity":"/paper/2505.11591/integrity","json":"/paper/2505.11591/citation-record.json","paper":"/paper/2505.11591"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T21:01:48.524431Z","title":"We consider now the generic behavior of the Einstein frame EoS in the case of positiveq","venue":null,"work_id":"38592026-88a8-4181-92cb-88b19daf6d0a","year":2025},"citing_paper":{"arxiv_id":"2505.11591","last_updated":"2025-05-16T18:00:09Z","snapshot_observed_at":"2026-08-17T13:41:03.609315Z","submitted_at":"2025-05-16T18:00:09Z","title":"Dust stars in the minimal exponential measure model","version":1},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-15T21:01:47.815206Z"},"links":{"citing_paper":"/paper/2505.11591"},"observation_digest":"sha256:3022ace8ac162c08ef9902feb2df8004f5f7990ef91fb382d9d84066ea32b8be","observation_id":"311f8dd0-0705-476c-9a17-84dc39feeb47","resolution":{"observed_at":"2026-08-15T21:01:48.527167Z","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":"2026-08-15T21:01:48.515911Z","title":"Although we must choose a value for the parameterq to proceed with numerical solutions, we found that the qualitative properties of the solutions are insensitive to variations inq","venue":null,"work_id":"57e7b3e4-93f9-4ca6-ab91-d76e450a392e","year":null},"citing_paper":{"arxiv_id":"2505.11591","last_updated":"2025-05-16T18:00:09Z","snapshot_observed_at":"2026-08-17T13:41:03.609315Z","submitted_at":"2025-05-16T18:00:09Z","title":"Dust stars in the minimal exponential measure model","version":1},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-15T21:01:47.819499Z"},"links":{"citing_paper":"/paper/2505.11591"},"observation_digest":"sha256:65e82f8c3b4ce3a361226d41e6a4b41eda2b0f30aff1177e11f41c2e27c19522","observation_id":"19429e2c-ea00-404b-938c-a30a352d58b8","resolution":{"observed_at":"2026-08-15T21:01:48.519289Z","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":"1707.03021","last_updated":"2019-04-12T05:01:20Z","snapshot_observed_at":"2026-08-14T20:48:32.547366Z","submitted_at":"2017-07-10T18:56:24Z","title":"The observational evidence for horizons: from echoes to precision gravitational-wave physics","version":5},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1707.03021","snapshot_observed_at":"2026-08-15T21:01:47.823192Z","title":"Cardoso and P","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2505.11591","last_updated":"2025-05-16T18:00:09Z","snapshot_observed_at":"2026-08-17T13:41:03.609315Z","submitted_at":"2025-05-16T18:00:09Z","title":"Dust stars in the minimal exponential measure model","version":1},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-15T21:01:47.823192Z"},"links":{"cited_paper":"/paper/1707.03021","citing_paper":"/paper/2505.11591"},"observation_digest":"sha256:442290cb198bcca0390a2954d899d5b45478b740d39492ceb7413130e1df40a7","observation_id":"50ac3c86-f7da-4cc2-93b9-0864d9d537f2","resolution":{"observed_at":"2026-08-15T21:01:47.823192Z","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":"2026-08-15T21:01:48.507174Z","title":null,"venue":null,"work_id":"f73296ce-ecf6-4e37-81be-edbaaa73c2dc","year":1972},"citing_paper":{"arxiv_id":"2505.11591","last_updated":"2025-05-16T18:00:09Z","snapshot_observed_at":"2026-08-17T13:41:03.609315Z","submitted_at":"2025-05-16T18:00:09Z","title":"Dust stars in the minimal exponential measure model","version":1},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-15T21:01:47.826341Z"},"links":{"citing_paper":"/paper/2505.11591"},"observation_digest":"sha256:ca17010ed6a7f579f445c26181be39520c87eb6e3a3b3ea6d671f6dd30ee6ecb","observation_id":"9a7569e3-aca8-4019-84ec-f5e7394ab96c","resolution":{"observed_at":"2026-08-15T21:01:48.510631Z","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":{"arxiv_id":"0812.1806","last_updated":"2009-03-12T00:13:05Z","snapshot_observed_at":"2026-08-15T05:59:41.571134Z","submitted_at":"2008-12-09T21:38:26Z","title":"Geodesic stability, Lyapunov exponents and quasinormal modes","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0812.1806","snapshot_observed_at":"2026-08-15T21:01:47.829039Z","title":"Cardoso, A","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2505.11591","last_updated":"2025-05-16T18:00:09Z","snapshot_observed_at":"2026-08-17T13:41:03.609315Z","submitted_at":"2025-05-16T18:00:09Z","title":"Dust stars in the minimal exponential measure model","version":1},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-15T21:01:47.829039Z"},"links":{"cited_paper":"/paper/0812.1806","citing_paper":"/paper/2505.11591"},"observation_digest":"sha256:44074e0434b6285f20fa6d7f980f54389d2fa1c7fd79bd65729fb3ecd96d93b8","observation_id":"cb21a83c-b3cc-4160-b523-e7be4edfba69","resolution":{"observed_at":"2026-08-15T21:01:47.829039Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1410.4481","last_updated":"2014-10-22T00:39:28Z","snapshot_observed_at":"2026-08-17T13:41:47.766037Z","submitted_at":"2014-10-16T16:08:55Z","title":"A Black-Hole Primer: Particles, Waves, Critical Phenomena and Superradiant Instabilities","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1410.4481","snapshot_observed_at":"2026-08-15T21:01:47.832240Z","title":"Berti (2014) arXiv:1410.4481 [gr-qc]","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2505.11591","last_updated":"2025-05-16T18:00:09Z","snapshot_observed_at":"2026-08-17T13:41:03.609315Z","submitted_at":"2025-05-16T18:00:09Z","title":"Dust stars in the minimal exponential measure model","version":1},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-15T21:01:47.832240Z"},"links":{"cited_paper":"/paper/1410.4481","citing_paper":"/paper/2505.11591"},"observation_digest":"sha256:86b5c7113945bf6cadc34e5ac89f4c8ad7f7a9ba51c23d8a43be338c26a49da4","observation_id":"0ba06c5f-5776-4753-ad13-0622c0af2ff0","resolution":{"observed_at":"2026-08-15T21:01:47.832240Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1706.07658","last_updated":"2017-06-23T12:17:31Z","snapshot_observed_at":"2026-08-14T20:52:05.267488Z","submitted_at":"2017-06-23T12:17:31Z","title":"Post-Kerr black hole spectroscopy","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1706.07658","snapshot_observed_at":"2026-08-15T21:01:47.835695Z","title":"Glampedakis, G","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2505.11591","last_updated":"2025-05-16T18:00:09Z","snapshot_observed_at":"2026-08-17T13:41:03.609315Z","submitted_at":"2025-05-16T18:00:09Z","title":"Dust stars in the minimal exponential measure model","version":1},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-15T21:01:47.835695Z"},"links":{"cited_paper":"/paper/1706.07658","citing_paper":"/paper/2505.11591"},"observation_digest":"sha256:9aa84e6280369851621514b9fb58ff9edb4d131356cdf5ede10af4876f1b6506","observation_id":"a34e52db-9cc9-4b6f-a304-e98a284d75c8","resolution":{"observed_at":"2026-08-15T21:01:47.835695Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2204.06533","last_updated":"2022-04-13T17:24:31Z","snapshot_observed_at":"2026-08-16T17:07:07.929245Z","submitted_at":"2022-04-13T17:24:31Z","title":"Modified theories of Gravity: Why, How and What?","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2204.06533","snapshot_observed_at":"2026-08-15T21:01:47.839045Z","title":"Shankaranarayanan and J","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2505.11591","last_updated":"2025-05-16T18:00:09Z","snapshot_observed_at":"2026-08-17T13:41:03.609315Z","submitted_at":"2025-05-16T18:00:09Z","title":"Dust stars in the minimal exponential measure model","version":1},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-15T21:01:47.839045Z"},"links":{"cited_paper":"/paper/2204.06533","citing_paper":"/paper/2505.11591"},"observation_digest":"sha256:dff9a2b44490230af5922800b492a70d0a0f91aaf71e4c0abace26875d1dcc49","observation_id":"fb3dd8ab-53e7-409e-811d-c44702056f98","resolution":{"observed_at":"2026-08-15T21:01:47.839045Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1708.03757","last_updated":"2017-08-12T09:31:49Z","snapshot_observed_at":"2026-08-17T03:05:59.600301Z","submitted_at":"2017-08-12T09:31:49Z","title":"A Class of Minimally Modified Gravity Theories","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1708.03757","snapshot_observed_at":"2026-08-15T21:01:47.842105Z","title":"Lin and S","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2505.11591","last_updated":"2025-05-16T18:00:09Z","snapshot_observed_at":"2026-08-17T13:41:03.609315Z","submitted_at":"2025-05-16T18:00:09Z","title":"Dust stars in the minimal exponential measure model","version":1},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-15T21:01:47.842105Z"},"links":{"cited_paper":"/paper/1708.03757","citing_paper":"/paper/2505.11591"},"observation_digest":"sha256:3c7f2701a1cfd3a101185359b054d7e5d9abd3f48fa9a32be9273da8ecc5ae3d","observation_id":"ad3b2e35-efce-49b6-b0b3-0d5099bcda61","resolution":{"observed_at":"2026-08-15T21:01:47.842105Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2011.04188","last_updated":"2020-11-09T04:49:16Z","snapshot_observed_at":"2026-08-16T19:07:18.254546Z","submitted_at":"2020-11-09T04:49:16Z","title":"Weakening gravity for dark matter in a type-II minimally modified gravity","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2011.04188","snapshot_observed_at":"2026-08-15T21:01:47.845434Z","title":"De Felice and S","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2505.11591","last_updated":"2025-05-16T18:00:09Z","snapshot_observed_at":"2026-08-17T13:41:03.609315Z","submitted_at":"2025-05-16T18:00:09Z","title":"Dust stars in the minimal exponential measure model","version":1},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-15T21:01:47.845434Z"},"links":{"cited_paper":"/paper/2011.04188","citing_paper":"/paper/2505.11591"},"observation_digest":"sha256:6e8f4a014250112740e0595b4f31cbec808944ac8933cdb3011cdaa1d4cde8d5","observation_id":"1bf04981-3ff7-4493-8ad1-d773ec42eb6f","resolution":{"observed_at":"2026-08-15T21:01:47.845434Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2004.12549","last_updated":"2020-09-16T16:13:19Z","snapshot_observed_at":"2026-08-10T19:45:13.051378Z","submitted_at":"2020-04-27T02:27:05Z","title":"A theory of type-II minimally modified gravity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2004.12549","snapshot_observed_at":"2026-08-15T21:01:47.848393Z","title":"De Felice, A","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2505.11591","last_updated":"2025-05-16T18:00:09Z","snapshot_observed_at":"2026-08-17T13:41:03.609315Z","submitted_at":"2025-05-16T18:00:09Z","title":"Dust stars in the minimal exponential measure model","version":1},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-15T21:01:47.848393Z"},"links":{"cited_paper":"/paper/2004.12549","citing_paper":"/paper/2505.11591"},"observation_digest":"sha256:8970a38b87b23b7c01574398415ee7efb46d5a1df53e83f84a922bc38ca42579","observation_id":"241fc8d6-ecc0-4f6d-83f4-9467dac8d6fa","resolution":{"observed_at":"2026-08-15T21:01:47.848393Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1810.01047","last_updated":"2019-01-04T14:00:35Z","snapshot_observed_at":"2026-08-14T18:20:48.335256Z","submitted_at":"2018-10-02T03:07:23Z","title":"Phenomenology in type-I minimally modified gravity","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1810.01047","snapshot_observed_at":"2026-08-15T21:01:47.851494Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2505.11591","last_updated":"2025-05-16T18:00:09Z","snapshot_observed_at":"2026-08-17T13:41:03.609315Z","submitted_at":"2025-05-16T18:00:09Z","title":"Dust stars in the minimal exponential measure model","version":1},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-15T21:01:47.851494Z"},"links":{"cited_paper":"/paper/1810.01047","citing_paper":"/paper/2505.11591"},"observation_digest":"sha256:87e040446d6b2c0ca923825ddf4ccb2d707f627ac3cb1aeb1035d899fa4d2cd5","observation_id":"774d7f64-cb0d-4fcc-a946-de6ab0fc927d","resolution":{"observed_at":"2026-08-15T21:01:47.851494Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1804.03902","last_updated":"2020-03-07T01:37:47Z","snapshot_observed_at":"2026-08-17T07:18:17.954336Z","submitted_at":"2018-04-11T09:49:02Z","title":"Novel matter coupling in general relativity via canonical transformation","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1804.03902","snapshot_observed_at":"2026-08-15T21:01:47.854901Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2505.11591","last_updated":"2025-05-16T18:00:09Z","snapshot_observed_at":"2026-08-17T13:41:03.609315Z","submitted_at":"2025-05-16T18:00:09Z","title":"Dust stars in the minimal exponential measure model","version":1},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-15T21:01:47.854901Z"},"links":{"cited_paper":"/paper/1804.03902","citing_paper":"/paper/2505.11591"},"observation_digest":"sha256:c943416583c6585fca0466a8e2710d4c5bbe4365a6f6910a69398228108ffce2","observation_id":"86677145-1d5c-4f27-ab39-45f14d2c68be","resolution":{"observed_at":"2026-08-15T21:01:47.854901Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1905.02000","last_updated":"2019-05-06T12:47:57Z","snapshot_observed_at":"2026-08-14T16:36:46.361555Z","submitted_at":"2019-05-06T12:47:57Z","title":"Minimally Modified Gravity: a Hamiltonian Construction","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1905.02000","snapshot_observed_at":"2026-08-15T21:01:47.857778Z","title":"Mukohyama and K","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2505.11591","last_updated":"2025-05-16T18:00:09Z","snapshot_observed_at":"2026-08-17T13:41:03.609315Z","submitted_at":"2025-05-16T18:00:09Z","title":"Dust stars in the minimal exponential measure model","version":1},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-15T21:01:47.857778Z"},"links":{"cited_paper":"/paper/1905.02000","citing_paper":"/paper/2505.11591"},"observation_digest":"sha256:931308919ebef833a2995a4c3917c6a5df039323b235a7912e8a8afa0bfed7e6","observation_id":"b16cb305-6fae-4b2a-89ee-07ea89030279","resolution":{"observed_at":"2026-08-15T21:01:47.857778Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2005.13972","last_updated":"2020-08-09T16:21:22Z","snapshot_observed_at":"2026-07-06T09:24:06.815308Z","submitted_at":"2020-05-28T13:24:19Z","title":"Minimally Modified Gravity fitting Planck data better than $\\Lambda$CDM","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2005.13972","snapshot_observed_at":"2026-08-15T21:01:47.860772Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2505.11591","last_updated":"2025-05-16T18:00:09Z","snapshot_observed_at":"2026-08-17T13:41:03.609315Z","submitted_at":"2025-05-16T18:00:09Z","title":"Dust stars in the minimal exponential measure model","version":1},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-15T21:01:47.860772Z"},"links":{"cited_paper":"/paper/2005.13972","citing_paper":"/paper/2505.11591"},"observation_digest":"sha256:f243cdf1e203e9cccd1f68baa6b23e62f2b19d17a42cf7bf5d446b4211ba0a1c","observation_id":"68b8d9b5-0d28-472a-b526-39c4960aeaeb","resolution":{"observed_at":"2026-08-15T21:01:47.860772Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1910.06978","last_updated":"2020-03-03T20:30:41Z","snapshot_observed_at":"2026-08-02T15:45:31.268920Z","submitted_at":"2019-10-15T18:00:06Z","title":"New class of generalized coupling theories","version":2},"cited_work":{"arxiv_id":"1910.06978","doi":null,"metadata_source":"pith","pith_arxiv_id":"1910.06978","snapshot_observed_at":"2026-08-15T21:01:48.277409Z","title":"New class of generalized coupling theories","venue":"gr-qc","work_id":"dc9c6087-58c6-4e84-ae7e-445e58afd682","year":2019},"citing_paper":{"arxiv_id":"2505.11591","last_updated":"2025-05-16T18:00:09Z","snapshot_observed_at":"2026-08-17T13:41:03.609315Z","submitted_at":"2025-05-16T18:00:09Z","title":"Dust stars in the minimal exponential measure model","version":1},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-15T21:01:47.863520Z"},"links":{"cited_paper":"/paper/1910.06978","citing_paper":"/paper/2505.11591"},"observation_digest":"sha256:ef901a28e32385d84aec0e91ff5573b0e8b2f59e577d1f4cd63130b329c54718","observation_id":"d07746e7-55c1-4415-b0bb-d3362ad881c7","resolution":{"observed_at":"2026-08-15T21:01:48.281249Z","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":{"arxiv_id":"2011.12305","last_updated":"2021-04-29T16:09:49Z","snapshot_observed_at":"2026-08-16T19:03:33.685831Z","submitted_at":"2020-11-24T19:00:01Z","title":"Minimal exponential measure model in the post-Newtonian limit","version":2},"cited_work":{"arxiv_id":"2011.12305","doi":null,"metadata_source":"pith","pith_arxiv_id":"2011.12305","snapshot_observed_at":"2026-08-15T21:01:48.265529Z","title":"Minimal exponential measure model in the post-Newtonian limit","venue":"gr-qc","work_id":"c3b53f80-0983-4d72-8ab0-b40324594e55","year":2020},"citing_paper":{"arxiv_id":"2505.11591","last_updated":"2025-05-16T18:00:09Z","snapshot_observed_at":"2026-08-17T13:41:03.609315Z","submitted_at":"2025-05-16T18:00:09Z","title":"Dust stars in the minimal exponential measure model","version":1},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-15T21:01:47.866612Z"},"links":{"cited_paper":"/paper/2011.12305","citing_paper":"/paper/2505.11591"},"observation_digest":"sha256:91ab0984d4803dfb2bbd30d4f1418430edeab027b4d8818420463ad1dedfb8b3","observation_id":"6c901a25-8da8-4ff2-ba63-349543e1d5a6","resolution":{"observed_at":"2026-08-15T21:01:48.269722Z","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":"2026-08-15T21:01:48.498225Z","title":null,"venue":null,"work_id":"65722922-6717-4a78-b642-2cfe4a52dfa0","year":2023},"citing_paper":{"arxiv_id":"2505.11591","last_updated":"2025-05-16T18:00:09Z","snapshot_observed_at":"2026-08-17T13:41:03.609315Z","submitted_at":"2025-05-16T18:00:09Z","title":"Dust stars in the minimal exponential measure model","version":1},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-15T21:01:47.870084Z"},"links":{"citing_paper":"/paper/2505.11591"},"observation_digest":"sha256:779fd1863e41897badebf19d8daab8fe51ef0c6e07e1e24b08827953b705346b","observation_id":"fbfbba43-2274-4fc5-8614-e26b2479bab3","resolution":{"observed_at":"2026-08-15T21:01:48.501201Z","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":"2026-08-15T21:01:48.489811Z","title":"Troisi and S","venue":null,"work_id":"168b8d4b-34c6-400f-849d-c1642966cdf8","year":2025},"citing_paper":{"arxiv_id":"2505.11591","last_updated":"2025-05-16T18:00:09Z","snapshot_observed_at":"2026-08-17T13:41:03.609315Z","submitted_at":"2025-05-16T18:00:09Z","title":"Dust stars in the minimal exponential measure model","version":1},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-15T21:01:47.873081Z"},"links":{"citing_paper":"/paper/2505.11591"},"observation_digest":"sha256:76bc54b19382963f7f47733c275b424c0f42df12e6fedd2a02de71a193d9dbee","observation_id":"bfd35a04-3cfd-4dc2-a14f-90f6cd7fdf19","resolution":{"observed_at":"2026-08-15T21:01:48.493441Z","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":"2111.08086","last_updated":"2021-11-15T21:18:39Z","snapshot_observed_at":"2026-08-16T17:41:38.554696Z","submitted_at":"2021-11-15T21:18:39Z","title":"Alternatives to $\\Lambda$: Torsion, Generalized Couplings, and Scale Invariance","version":1},"cited_work":{"arxiv_id":"2111.08086","doi":null,"metadata_source":"pith","pith_arxiv_id":"2111.08086","snapshot_observed_at":"2026-08-15T21:01:48.253107Z","title":"Alternatives to $\\Lambda$: Torsion, Generalized Couplings, and Scale Invariance","venue":"astro-ph.CO","work_id":"f1b0e6ab-24be-4f4e-801d-9f92a0ec7406","year":2021},"citing_paper":{"arxiv_id":"2505.11591","last_updated":"2025-05-16T18:00:09Z","snapshot_observed_at":"2026-08-17T13:41:03.609315Z","submitted_at":"2025-05-16T18:00:09Z","title":"Dust stars in the minimal exponential measure model","version":1},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-15T21:01:47.875658Z"},"links":{"cited_paper":"/paper/2111.08086","citing_paper":"/paper/2505.11591"},"observation_digest":"sha256:28c98efaf6fb95e1179cd7b9e31a0d81168898085c2d4cce008700d478b613ac","observation_id":"f9a91872-a360-4ba5-b0a9-78afbe0d73f9","resolution":{"observed_at":"2026-08-15T21:01:48.257192Z","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":{"arxiv_id":"2012.10513","last_updated":"2020-12-18T21:08:03Z","snapshot_observed_at":"2026-08-16T18:57:23.713076Z","submitted_at":"2020-12-18T21:08:03Z","title":"Constraining alternatives to a cosmological constant: generalized couplings and scale invariance","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2012.10513","snapshot_observed_at":"2026-08-15T21:01:47.882179Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2505.11591","last_updated":"2025-05-16T18:00:09Z","snapshot_observed_at":"2026-08-17T13:41:03.609315Z","submitted_at":"2025-05-16T18:00:09Z","title":"Dust stars in the minimal exponential measure model","version":1},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-15T21:01:47.882179Z"},"links":{"cited_paper":"/paper/2012.10513","citing_paper":"/paper/2505.11591"},"observation_digest":"sha256:7716f21c52d3a05abe253e705f301db081bf0583cff5c57bb0dde27abb9e60a3","observation_id":"a74addd4-8f8e-4440-9bf3-db3f56ca0c8c","resolution":{"observed_at":"2026-08-15T21:01:47.882179Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2203.00011","last_updated":"2022-05-17T15:20:24Z","snapshot_observed_at":"2026-08-16T17:18:00.797832Z","submitted_at":"2022-02-28T19:00:00Z","title":"Junction conditions and sharp gradients in generalized coupling theories","version":2},"cited_work":{"arxiv_id":"2203.00011","doi":null,"metadata_source":"pith","pith_arxiv_id":"2203.00011","snapshot_observed_at":"2026-08-15T21:01:48.233977Z","title":"Junction conditions and sharp gradients in generalized coupling theories","venue":"gr-qc","work_id":"702e8e46-2441-4ec5-92f0-6beb899bac89","year":2022},"citing_paper":{"arxiv_id":"2505.11591","last_updated":"2025-05-16T18:00:09Z","snapshot_observed_at":"2026-08-17T13:41:03.609315Z","submitted_at":"2025-05-16T18:00:09Z","title":"Dust stars in the minimal exponential measure model","version":1},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-15T21:01:47.885350Z"},"links":{"cited_paper":"/paper/2203.00011","citing_paper":"/paper/2505.11591"},"observation_digest":"sha256:de3f1c22b9154a45a4f51686204ae7532ff58dbc38a789891a93e9f4db64dbe7","observation_id":"d6bdea8b-971e-4e66-9101-e006e7f7905d","resolution":{"observed_at":"2026-08-15T21:01:48.239065Z","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":"2026-08-15T21:01:48.481874Z","title":null,"venue":null,"work_id":"80df3c85-e7b8-4205-a2f4-4630d823432a","year":2023},"citing_paper":{"arxiv_id":"2505.11591","last_updated":"2025-05-16T18:00:09Z","snapshot_observed_at":"2026-08-17T13:41:03.609315Z","submitted_at":"2025-05-16T18:00:09Z","title":"Dust stars in the minimal exponential measure model","version":1},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-15T21:01:47.888293Z"},"links":{"citing_paper":"/paper/2505.11591"},"observation_digest":"sha256:6cc8505d3051bf9b1f278062efecf551a3cb1ba398a92d976f315ffb42442a7d","observation_id":"e545cc93-9d7d-4f43-be8d-bb89d39c8ada","resolution":{"observed_at":"2026-08-15T21:01:48.484598Z","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":"2026-08-15T21:01:48.473103Z","title":"Chandrasekhar, inGeneral relativity: papers in honour of J","venue":null,"work_id":"4c4b5c7f-a555-4ab6-b1bc-90632b83a152","year":1972},"citing_paper":{"arxiv_id":"2505.11591","last_updated":"2025-05-16T18:00:09Z","snapshot_observed_at":"2026-08-17T13:41:03.609315Z","submitted_at":"2025-05-16T18:00:09Z","title":"Dust stars in the minimal exponential measure model","version":1},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-15T21:01:47.891359Z"},"links":{"citing_paper":"/paper/2505.11591"},"observation_digest":"sha256:0417a53878c8547b20bedfb658e2f3d67eec0faf0212f8a49ffb925f409fb89d","observation_id":"8b39ed39-721b-4fd4-9c45-749552a30575","resolution":{"observed_at":"2026-08-15T21:01:48.476018Z","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":"2026-08-15T21:01:48.463698Z","title":"Chavanis, Astronomy & Astrophysics381, 709 (2002)","venue":null,"work_id":"d1778b9e-63d6-4924-83df-39918ccc0e92","year":2002},"citing_paper":{"arxiv_id":"2505.11591","last_updated":"2025-05-16T18:00:09Z","snapshot_observed_at":"2026-08-17T13:41:03.609315Z","submitted_at":"2025-05-16T18:00:09Z","title":"Dust stars in the minimal exponential measure model","version":1},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-15T21:01:47.893944Z"},"links":{"citing_paper":"/paper/2505.11591"},"observation_digest":"sha256:76129028dd6833521869820a73ddbc113423c745975fe44fa1c2958a468331ca","observation_id":"689e61f0-e8e2-43eb-b7f6-334fe296c872","resolution":{"observed_at":"2026-08-15T21:01:48.466457Z","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":"2026-08-15T21:01:47.896710Z","title":"Weinberg, Rev","venue":null,"work_id":null,"year":1989},"citing_paper":{"arxiv_id":"2505.11591","last_updated":"2025-05-16T18:00:09Z","snapshot_observed_at":"2026-08-17T13:41:03.609315Z","submitted_at":"2025-05-16T18:00:09Z","title":"Dust stars in the minimal exponential measure model","version":1},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-15T21:01:47.896710Z"},"links":{"citing_paper":"/paper/2505.11591"},"observation_digest":"sha256:533f0506b494e6ca36d2a5357084d3eb68e0544778787eac38df7a21f3a1cc8c","observation_id":"452f2080-4edf-4d3c-913f-58b8b86f9645","resolution":{"observed_at":"2026-08-15T21:01:47.896710Z","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":"2026-08-15T21:01:48.450436Z","title":"Chandrasekhar,An introduction to the study of stellar structure(Chicago Univ","venue":null,"work_id":"532295a8-419f-421e-884f-cb1865729f54","year":1939},"citing_paper":{"arxiv_id":"2505.11591","last_updated":"2025-05-16T18:00:09Z","snapshot_observed_at":"2026-08-17T13:41:03.609315Z","submitted_at":"2025-05-16T18:00:09Z","title":"Dust stars in the minimal exponential measure model","version":1},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-15T21:01:47.900337Z"},"links":{"citing_paper":"/paper/2505.11591"},"observation_digest":"sha256:e15146efe935cce3a672c1022ce1508f0a420efdf9aba90cc0d3f179cc54eb3f","observation_id":"f230d789-f859-4822-aa4a-f8dec98a39d2","resolution":{"observed_at":"2026-08-15T21:01:48.453905Z","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":"1611.01533","last_updated":"2017-01-26T19:10:07Z","snapshot_observed_at":"2026-08-14T21:31:53.782514Z","submitted_at":"2016-11-04T20:58:37Z","title":"Phenomenological Review on Quark-Gluon Plasma: Concepts vs. Observations","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1611.01533","snapshot_observed_at":"2026-08-15T21:01:47.902625Z","title":"Pasechnik and M","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2505.11591","last_updated":"2025-05-16T18:00:09Z","snapshot_observed_at":"2026-08-17T13:41:03.609315Z","submitted_at":"2025-05-16T18:00:09Z","title":"Dust stars in the minimal exponential measure model","version":1},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-15T21:01:47.902625Z"},"links":{"cited_paper":"/paper/1611.01533","citing_paper":"/paper/2505.11591"},"observation_digest":"sha256:c213b0a548b61f9d541268c5d4065e06fbcedf489a2adc6d5dfe27f13433cade","observation_id":"249cd214-4dc8-4ae7-a07b-d5a7b9c88e61","resolution":{"observed_at":"2026-08-15T21:01:47.902625Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2002.12778","last_updated":"2021-05-09T18:33:50Z","snapshot_observed_at":"2026-08-15T00:15:00.732047Z","submitted_at":"2020-02-27T05:17:54Z","title":"Constraints on Primordial Black Holes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2002.12778","snapshot_observed_at":"2026-08-15T21:01:47.905318Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2505.11591","last_updated":"2025-05-16T18:00:09Z","snapshot_observed_at":"2026-08-17T13:41:03.609315Z","submitted_at":"2025-05-16T18:00:09Z","title":"Dust stars in the minimal exponential measure model","version":1},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-15T21:01:47.905318Z"},"links":{"cited_paper":"/paper/2002.12778","citing_paper":"/paper/2505.11591"},"observation_digest":"sha256:851382229c47dd47193874a81941dc0d5c16127c1aaf69bd0ba8ad350fccb53c","observation_id":"b103832f-aa36-4806-ac00-4500141b8f99","resolution":{"observed_at":"2026-08-15T21:01:47.905318Z","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":"2026-08-15T21:01:47.908835Z","title":null,"venue":null,"work_id":null,"year":1989},"citing_paper":{"arxiv_id":"2505.11591","last_updated":"2025-05-16T18:00:09Z","snapshot_observed_at":"2026-08-17T13:41:03.609315Z","submitted_at":"2025-05-16T18:00:09Z","title":"Dust stars in the minimal exponential measure model","version":1},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-15T21:01:47.908835Z"},"links":{"citing_paper":"/paper/2505.11591"},"observation_digest":"sha256:5b1c0fc760ebc65aad214a421d63e3f88d9b9de969d89070e37c627f718781bb","observation_id":"86b57491-62c3-4d43-8065-f81d810a31b6","resolution":{"observed_at":"2026-08-15T21:01:47.908835Z","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":"2026-08-15T21:01:48.438210Z","title":null,"venue":null,"work_id":"ce4dbbad-a128-454d-9472-ee360be3a387","year":1992},"citing_paper":{"arxiv_id":"2505.11591","last_updated":"2025-05-16T18:00:09Z","snapshot_observed_at":"2026-08-17T13:41:03.609315Z","submitted_at":"2025-05-16T18:00:09Z","title":"Dust stars in the minimal exponential measure model","version":1},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-08-15T21:01:47.911315Z"},"links":{"citing_paper":"/paper/2505.11591"},"observation_digest":"sha256:23b2b665112e92a2a2afc357e52092e30dea95c2edbfaecc52842a5cac00de52","observation_id":"943eec7f-99c2-4b3f-a8dc-c92cdf888abc","resolution":{"observed_at":"2026-08-15T21:01:48.441222Z","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":{"arxiv_id":"gr-qc/9904013","last_updated":"1999-04-06T14:47:05Z","snapshot_observed_at":"2026-07-07T03:30:20.599489Z","submitted_at":"1999-04-06T14:47:05Z","title":"Gravitational Collapse of Gravitational Waves in 3D Numerical Relativity","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"gr-qc/9904013","snapshot_observed_at":"2026-08-15T21:01:47.914430Z","title":"Alcubierre, G","venue":null,"work_id":null,"year":2000},"citing_paper":{"arxiv_id":"2505.11591","last_updated":"2025-05-16T18:00:09Z","snapshot_observed_at":"2026-08-17T13:41:03.609315Z","submitted_at":"2025-05-16T18:00:09Z","title":"Dust stars in the minimal exponential measure model","version":1},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-15T21:01:47.914430Z"},"links":{"cited_paper":"/paper/gr-qc/9904013","citing_paper":"/paper/2505.11591"},"observation_digest":"sha256:d1a958677bd70bdf68a924402e219f0d2dae225f8cbe1bb22133fe539dd58cf9","observation_id":"ef2d9b73-4ca2-4d33-a441-6c7879ef3fad","resolution":{"observed_at":"2026-08-15T21:01:47.914430Z","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":"2026-08-15T21:01:47.917407Z","title":null,"venue":null,"work_id":null,"year":2001},"citing_paper":{"arxiv_id":"2505.11591","last_updated":"2025-05-16T18:00:09Z","snapshot_observed_at":"2026-08-17T13:41:03.609315Z","submitted_at":"2025-05-16T18:00:09Z","title":"Dust stars in the minimal exponential measure model","version":1},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-15T21:01:47.917407Z"},"links":{"citing_paper":"/paper/2505.11591"},"observation_digest":"sha256:f5a1d5f36a300932e382c67c09083ee8edf01fe4375e6c18c75ddfeb44dfae81","observation_id":"2aae36c5-22de-4d04-adab-972d59fa96d1","resolution":{"observed_at":"2026-08-15T21:01:47.917407Z","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":"2026-08-15T21:01:48.425962Z","title":"Chen and R","venue":null,"work_id":"93b09434-56a2-4209-89d7-c66d1ad1b185","year":2003},"citing_paper":{"arxiv_id":"2505.11591","last_updated":"2025-05-16T18:00:09Z","snapshot_observed_at":"2026-08-17T13:41:03.609315Z","submitted_at":"2025-05-16T18:00:09Z","title":"Dust stars in the minimal exponential measure model","version":1},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-15T21:01:47.920542Z"},"links":{"citing_paper":"/paper/2505.11591"},"observation_digest":"sha256:cd1812f9e3231a23dfcb803438c395a1571518889838ed48592d6f1f27153434","observation_id":"4ff1746b-a15b-4760-9b5a-12f1daa10b50","resolution":{"observed_at":"2026-08-15T21:01:48.428803Z","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":"2026-08-15T21:01:48.417758Z","title":"bradkav/pbhbounds: Release version,","venue":null,"work_id":"7d793dec-11e2-40ff-af36-dbe8bb8d06f5","year":2019},"citing_paper":{"arxiv_id":"2505.11591","last_updated":"2025-05-16T18:00:09Z","snapshot_observed_at":"2026-08-17T13:41:03.609315Z","submitted_at":"2025-05-16T18:00:09Z","title":"Dust stars in the minimal exponential measure model","version":1},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-15T21:01:47.923055Z"},"links":{"citing_paper":"/paper/2505.11591"},"observation_digest":"sha256:253c59a493725a6dfec4d37e93facb108cdc461f9c70e9659cceff163595a36d","observation_id":"34898e2a-6087-4fd7-af51-3e672cc3f12c","resolution":{"observed_at":"2026-08-15T21:01:48.420787Z","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":"2026-08-15T21:01:47.926496Z","title":"Rackauckas and Q","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2505.11591","last_updated":"2025-05-16T18:00:09Z","snapshot_observed_at":"2026-08-17T13:41:03.609315Z","submitted_at":"2025-05-16T18:00:09Z","title":"Dust stars in the minimal exponential measure model","version":1},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-15T21:01:47.926496Z"},"links":{"citing_paper":"/paper/2505.11591"},"observation_digest":"sha256:d4eb0d7ba9acd6139fbe1f078ba4ee19d11dde99fd0983413b2342ed9e55f18b","observation_id":"175ac9fc-87b6-47f9-aa0f-ed9fa03f6456","resolution":{"observed_at":"2026-08-15T21:01:47.926496Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2008.05331","last_updated":"2020-08-12T14:12:05Z","snapshot_observed_at":"2026-08-13T21:52:44.056245Z","submitted_at":"2020-08-12T14:12:05Z","title":"Equilibrium, radial stability and non-adiabatic gravitational collapse of anisotropic neutron stars","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2008.05331","snapshot_observed_at":"2026-08-15T21:01:47.929081Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2505.11591","last_updated":"2025-05-16T18:00:09Z","snapshot_observed_at":"2026-08-17T13:41:03.609315Z","submitted_at":"2025-05-16T18:00:09Z","title":"Dust stars in the minimal exponential measure model","version":1},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-15T21:01:47.929081Z"},"links":{"cited_paper":"/paper/2008.05331","citing_paper":"/paper/2505.11591"},"observation_digest":"sha256:1f78a65d70d7732ac9eab70b1dddd9994e31a88e23ff00458215e05b066ba2c0","observation_id":"983a26b6-afb5-4812-a11d-4712a9d9c397","resolution":{"observed_at":"2026-08-15T21:01:47.929081Z","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":"2026-08-15T21:01:47.932318Z","title":null,"venue":null,"work_id":null,"year":1983},"citing_paper":{"arxiv_id":"2505.11591","last_updated":"2025-05-16T18:00:09Z","snapshot_observed_at":"2026-08-17T13:41:03.609315Z","submitted_at":"2025-05-16T18:00:09Z","title":"Dust stars in the minimal exponential measure model","version":1},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-15T21:01:47.932318Z"},"links":{"citing_paper":"/paper/2505.11591"},"observation_digest":"sha256:d02c9801cdb2a557e12bb56cecafd2a5b801972cb6f858577c83f370e099c980","observation_id":"1eb213d9-bc2b-4b98-b953-396d9dda6cad","resolution":{"observed_at":"2026-08-15T21:01:47.932318Z","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":"2026-08-15T21:01:48.404702Z","title":"Chandrasekhar, Astrophys","venue":null,"work_id":"254c284d-7b43-4491-b061-7fc85130d5f5","year":1964},"citing_paper":{"arxiv_id":"2505.11591","last_updated":"2025-05-16T18:00:09Z","snapshot_observed_at":"2026-08-17T13:41:03.609315Z","submitted_at":"2025-05-16T18:00:09Z","title":"Dust stars in the minimal exponential measure model","version":1},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-08-15T21:01:47.934636Z"},"links":{"citing_paper":"/paper/2505.11591"},"observation_digest":"sha256:b43ee48b4e20855bf0ee48097d505d4c248319b6ee0c898e10247f02d4f848bb","observation_id":"8f6950b4-d617-4060-a010-909ac7c46fcc","resolution":{"observed_at":"2026-08-15T21:01:48.407919Z","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":"2026-08-15T21:01:48.396350Z","title":"Chandrasekhar, Phys","venue":null,"work_id":"e7900608-1bad-43a3-98a2-ec16de012483","year":1964},"citing_paper":{"arxiv_id":"2505.11591","last_updated":"2025-05-16T18:00:09Z","snapshot_observed_at":"2026-08-17T13:41:03.609315Z","submitted_at":"2025-05-16T18:00:09Z","title":"Dust stars in the minimal exponential measure model","version":1},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-08-15T21:01:47.937064Z"},"links":{"citing_paper":"/paper/2505.11591"},"observation_digest":"sha256:16ca7baa36ba80f65c1001d333946591467742c26dfd266d2d01778de8e153d0","observation_id":"c98da218-16f1-4cf2-b90a-1a7e6b45d58f","resolution":{"observed_at":"2026-08-15T21:01:48.399180Z","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":"2026-08-15T21:01:48.388088Z","title":"Chanmugam, Astrophys","venue":null,"work_id":"11cefa9d-e62e-4857-a9a4-75b8d994eeae","year":1977},"citing_paper":{"arxiv_id":"2505.11591","last_updated":"2025-05-16T18:00:09Z","snapshot_observed_at":"2026-08-17T13:41:03.609315Z","submitted_at":"2025-05-16T18:00:09Z","title":"Dust stars in the minimal exponential measure model","version":1},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-08-15T21:01:47.939859Z"},"links":{"citing_paper":"/paper/2505.11591"},"observation_digest":"sha256:215ab81d1494a237744501183b5f08abebb69d96ed91c4b488e048655547c74a","observation_id":"1fa145b0-d015-45e7-b26d-5605fde416fd","resolution":{"observed_at":"2026-08-15T21:01:48.390724Z","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":"2405.10359","last_updated":"2024-05-16T18:00:00Z","snapshot_observed_at":"2026-08-16T20:57:34.892843Z","submitted_at":"2024-05-16T18:00:00Z","title":"Non-comoving description of adiabatic radial perturbations of relativistic stars","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2405.10359","snapshot_observed_at":"2026-08-15T21:01:47.942839Z","title":"Luz and S","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2505.11591","last_updated":"2025-05-16T18:00:09Z","snapshot_observed_at":"2026-08-17T13:41:03.609315Z","submitted_at":"2025-05-16T18:00:09Z","title":"Dust stars in the minimal exponential measure model","version":1},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-08-15T21:01:47.942839Z"},"links":{"cited_paper":"/paper/2405.10359","citing_paper":"/paper/2505.11591"},"observation_digest":"sha256:2918ffdfe59a6cda019bf1c38974f526a7ebe4e0463b25bfdae1264e612b2162","observation_id":"03fe9b29-be0c-4573-bd65-eed7ade7358a","resolution":{"observed_at":"2026-08-15T21:01:47.942839Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2405.06740","last_updated":"2024-05-10T18:00:01Z","snapshot_observed_at":"2026-08-16T13:53:39.925905Z","submitted_at":"2024-05-10T18:00:01Z","title":"Adiabatic radial perturbations of relativistic stars: analytic solutions to an old problem","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2405.06740","snapshot_observed_at":"2026-08-15T21:01:47.945888Z","title":"Luz and S","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2505.11591","last_updated":"2025-05-16T18:00:09Z","snapshot_observed_at":"2026-08-17T13:41:03.609315Z","submitted_at":"2025-05-16T18:00:09Z","title":"Dust stars in the minimal exponential measure model","version":1},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-08-15T21:01:47.945888Z"},"links":{"cited_paper":"/paper/2405.06740","citing_paper":"/paper/2505.11591"},"observation_digest":"sha256:1409d12c19db10029d89f1bd292ab85a3f3fcf1ff919d8d8d3fc276148c06e3b","observation_id":"1c97a8da-aa94-4002-9ea9-482cf53e5b91","resolution":{"observed_at":"2026-08-15T21:01:47.945888Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2405.05321","last_updated":"2024-05-08T18:00:06Z","snapshot_observed_at":"2026-08-16T13:54:15.248020Z","submitted_at":"2024-05-08T18:00:06Z","title":"Gauge invariant perturbations of static spatially compact LRS II spacetimes","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2405.05321","snapshot_observed_at":"2026-08-15T21:01:47.948938Z","title":"Luz and S","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2505.11591","last_updated":"2025-05-16T18:00:09Z","snapshot_observed_at":"2026-08-17T13:41:03.609315Z","submitted_at":"2025-05-16T18:00:09Z","title":"Dust stars in the minimal exponential measure model","version":1},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-08-15T21:01:47.948938Z"},"links":{"cited_paper":"/paper/2405.05321","citing_paper":"/paper/2505.11591"},"observation_digest":"sha256:ae18c2ea17659121f085cb91210e5a53821e9e3c1d961c242e369b40711b3f5b","observation_id":"9b4a6d90-50ae-42b1-97ae-477feef3e1a4","resolution":{"observed_at":"2026-08-15T21:01:47.948938Z","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":"2026-08-15T21:01:47.952724Z","title":"Santiago, J","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2505.11591","last_updated":"2025-05-16T18:00:09Z","snapshot_observed_at":"2026-08-17T13:41:03.609315Z","submitted_at":"2025-05-16T18:00:09Z","title":"Dust stars in the minimal exponential measure model","version":1},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-08-15T21:01:47.952724Z"},"links":{"citing_paper":"/paper/2505.11591"},"observation_digest":"sha256:d9cb29465c4c445b0a80cf7066b27d43a75e1e22764e6f597e77fafebdf5b6dc","observation_id":"3d060c04-5e83-494e-aced-59e64d046dd5","resolution":{"observed_at":"2026-08-15T21:01:47.952724Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2410.21577","last_updated":"2025-05-03T17:10:06Z","snapshot_observed_at":"2026-08-16T13:05:11.243942Z","submitted_at":"2024-10-28T22:16:37Z","title":"Nonsingular black holes as dark matter","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2410.21577","snapshot_observed_at":"2026-08-15T21:01:47.955567Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2505.11591","last_updated":"2025-05-16T18:00:09Z","snapshot_observed_at":"2026-08-17T13:41:03.609315Z","submitted_at":"2025-05-16T18:00:09Z","title":"Dust stars in the minimal exponential measure model","version":1},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-08-15T21:01:47.955567Z"},"links":{"cited_paper":"/paper/2410.21577","citing_paper":"/paper/2505.11591"},"observation_digest":"sha256:dff0bbb604cb566ec875ee0519265fe7a84144c0abad982a96fa4a8fbc831205","observation_id":"5772652e-7550-4363-8a53-791f9ad118a0","resolution":{"observed_at":"2026-08-15T21:01:47.955567Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2110.02821","last_updated":"2022-05-02T09:01:34Z","snapshot_observed_at":"2026-08-16T21:59:16.332490Z","submitted_at":"2021-10-06T14:46:37Z","title":"Primordial Black Holes as Dark Matter Candidates","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2110.02821","snapshot_observed_at":"2026-08-15T21:01:47.958095Z","title":"Carr and F","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2505.11591","last_updated":"2025-05-16T18:00:09Z","snapshot_observed_at":"2026-08-17T13:41:03.609315Z","submitted_at":"2025-05-16T18:00:09Z","title":"Dust stars in the minimal exponential measure model","version":1},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-08-15T21:01:47.958095Z"},"links":{"cited_paper":"/paper/2110.02821","citing_paper":"/paper/2505.11591"},"observation_digest":"sha256:184c5767018a95e8ebe3c0d82ddc32601d7dff81b5a6565068d3d954aae07554","observation_id":"301b233d-95e6-4f40-82f3-e68f35337c0f","resolution":{"observed_at":"2026-08-15T21:01:47.958095Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1906.04858","last_updated":"2019-06-11T23:14:26Z","snapshot_observed_at":"2026-08-17T14:29:51.665845Z","submitted_at":"2019-06-11T23:14:26Z","title":"Primordial Extremal Black Holes as Dark Matter","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1906.04858","snapshot_observed_at":"2026-08-15T21:01:47.961815Z","title":"Bai and N","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2505.11591","last_updated":"2025-05-16T18:00:09Z","snapshot_observed_at":"2026-08-17T13:41:03.609315Z","submitted_at":"2025-05-16T18:00:09Z","title":"Dust stars in the minimal exponential measure model","version":1},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-08-15T21:01:47.961815Z"},"links":{"cited_paper":"/paper/1906.04858","citing_paper":"/paper/2505.11591"},"observation_digest":"sha256:a710c8d638e9c20f6d799a553dd86d995b187d3fa887d269512c98d42f394d51","observation_id":"75abdd9d-6299-4e10-8bfa-b751131e31af","resolution":{"observed_at":"2026-08-15T21:01:47.961815Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/0205106","last_updated":"2002-05-24T19:30:09Z","snapshot_observed_at":"2026-08-12T20:13:11.825713Z","submitted_at":"2002-05-24T19:30:09Z","title":"Black Hole Remnants and Dark Matter","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"gr-qc/0205106","snapshot_observed_at":"2026-08-15T21:01:47.965608Z","title":"Chen and R","venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2505.11591","last_updated":"2025-05-16T18:00:09Z","snapshot_observed_at":"2026-08-17T13:41:03.609315Z","submitted_at":"2025-05-16T18:00:09Z","title":"Dust stars in the minimal exponential measure model","version":1},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-08-15T21:01:47.965608Z"},"links":{"cited_paper":"/paper/gr-qc/0205106","citing_paper":"/paper/2505.11591"},"observation_digest":"sha256:7166b33b5bbfab057b558a86b2b7af194c366ac21e3c231d63ae19c29911213c","observation_id":"7eab04a4-9649-432e-a973-e3a8623ba659","resolution":{"observed_at":"2026-08-15T21:01:47.965608Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/0106080","last_updated":"2001-06-26T00:09:55Z","snapshot_observed_at":"2026-08-17T16:09:31.440315Z","submitted_at":"2001-06-26T00:09:55Z","title":"The Generalized Uncertainty Principle and Black Hole Remnants","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"gr-qc/0106080","snapshot_observed_at":"2026-08-15T21:01:47.969632Z","title":null,"venue":null,"work_id":null,"year":2001},"citing_paper":{"arxiv_id":"2505.11591","last_updated":"2025-05-16T18:00:09Z","snapshot_observed_at":"2026-08-17T13:41:03.609315Z","submitted_at":"2025-05-16T18:00:09Z","title":"Dust stars in the minimal exponential measure model","version":1},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-08-15T21:01:47.969632Z"},"links":{"cited_paper":"/paper/gr-qc/0106080","citing_paper":"/paper/2505.11591"},"observation_digest":"sha256:039dfa93a5e9b4f9d70869671e42b73fdf11e158d8935f51db4ce54c08e33a70","observation_id":"4ae819c6-017b-45a7-9cf2-80949ccd78a2","resolution":{"observed_at":"2026-08-15T21:01:47.969632Z","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":"2026-08-15T21:01:48.379635Z","title":null,"venue":null,"work_id":"dac8ff33-869d-49f9-93cb-506f1373d9a0","year":1992},"citing_paper":{"arxiv_id":"2505.11591","last_updated":"2025-05-16T18:00:09Z","snapshot_observed_at":"2026-08-17T13:41:03.609315Z","submitted_at":"2025-05-16T18:00:09Z","title":"Dust stars in the minimal exponential measure model","version":1},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-08-15T21:01:47.972597Z"},"links":{"citing_paper":"/paper/2505.11591"},"observation_digest":"sha256:b5c3fa4bdd5f0e6d94a39828926809c633998926ff9e30cdbd524d3340131b18","observation_id":"d8685e7b-f66e-4210-8117-872cf5e8e5fe","resolution":{"observed_at":"2026-08-15T21:01:48.383120Z","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":"2026-08-15T21:01:48.370943Z","title":null,"venue":null,"work_id":"8343bcb9-6de7-4a9a-8f28-f44f1eb5b074","year":1992},"citing_paper":{"arxiv_id":"2505.11591","last_updated":"2025-05-16T18:00:09Z","snapshot_observed_at":"2026-08-17T13:41:03.609315Z","submitted_at":"2025-05-16T18:00:09Z","title":"Dust stars in the minimal exponential measure model","version":1},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-08-15T21:01:47.974995Z"},"links":{"citing_paper":"/paper/2505.11591"},"observation_digest":"sha256:8ea8408afeb13235188ef7292f511d195976271af795e63f5b8ead185a817ffe","observation_id":"1f7d01f4-8368-45c0-8f68-3f36f238d87d","resolution":{"observed_at":"2026-08-15T21:01:48.374306Z","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":"2026-08-15T21:01:48.362749Z","title":"Aharonov, A","venue":null,"work_id":"8ef7585f-8f20-4a8c-bb79-10dfc235feb9","year":1987},"citing_paper":{"arxiv_id":"2505.11591","last_updated":"2025-05-16T18:00:09Z","snapshot_observed_at":"2026-08-17T13:41:03.609315Z","submitted_at":"2025-05-16T18:00:09Z","title":"Dust stars in the minimal exponential measure model","version":1},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-08-15T21:01:47.978616Z"},"links":{"citing_paper":"/paper/2505.11591"},"observation_digest":"sha256:9d27fd1809e347cd8245a6f5ff83223765a643729dd1f2119cfa4daa107858ec","observation_id":"105fa694-63a4-4427-98d4-6837fc123e17","resolution":{"observed_at":"2026-08-15T21:01:48.365238Z","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":"2503.21740","last_updated":"2025-03-27T17:51:05Z","snapshot_observed_at":"2026-08-16T12:46:12.349012Z","submitted_at":"2025-03-27T17:51:05Z","title":"Transitioning to Memory Burden: Detectable Small Primordial Black Holes as Dark Matter","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2503.21740","snapshot_observed_at":"2026-08-15T21:01:47.982112Z","title":"Dvali, M","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2505.11591","last_updated":"2025-05-16T18:00:09Z","snapshot_observed_at":"2026-08-17T13:41:03.609315Z","submitted_at":"2025-05-16T18:00:09Z","title":"Dust stars in the minimal exponential measure model","version":1},"reference_index":54,"source":"pdf_text","source_observed_at":"2026-08-15T21:01:47.982112Z"},"links":{"cited_paper":"/paper/2503.21740","citing_paper":"/paper/2505.11591"},"observation_digest":"sha256:50bc88a58ebdf756c4ee75f1a6bdf727c40d132db842f0140f88983c555aac85","observation_id":"c8ab4bf4-2f89-4d57-93d4-bc310622d4df","resolution":{"observed_at":"2026-08-15T21:01:47.982112Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0001272","last_updated":"2000-01-15T22:28:48Z","snapshot_observed_at":"2026-07-07T00:09:31.766167Z","submitted_at":"2000-01-15T22:28:48Z","title":"The MACHO Project: Microlensing Results from 5.7 Years of LMC Observations","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0001272","snapshot_observed_at":"2026-08-15T21:01:47.985692Z","title":"Alcocket al.(MACHO), Astrophys","venue":null,"work_id":null,"year":2000},"citing_paper":{"arxiv_id":"2505.11591","last_updated":"2025-05-16T18:00:09Z","snapshot_observed_at":"2026-08-17T13:41:03.609315Z","submitted_at":"2025-05-16T18:00:09Z","title":"Dust stars in the minimal exponential measure model","version":1},"reference_index":55,"source":"pdf_text","source_observed_at":"2026-08-15T21:01:47.985692Z"},"links":{"cited_paper":"/paper/astro-ph/0001272","citing_paper":"/paper/2505.11591"},"observation_digest":"sha256:76c8f0330a65ee8dbc882141b53b0483b37768fad7ece40f800664c8d545bc8d","observation_id":"e02ace71-a24f-4876-920b-7747e733e574","resolution":{"observed_at":"2026-08-15T21:01:47.985692Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2109.06456","last_updated":"2022-02-23T04:17:52Z","snapshot_observed_at":"2026-08-16T17:56:48.830381Z","submitted_at":"2021-09-14T05:52:55Z","title":"Constraints on compact dark matter from gravitational wave microlensing","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2109.06456","snapshot_observed_at":"2026-08-15T21:01:47.989206Z","title":"Basak, A","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2505.11591","last_updated":"2025-05-16T18:00:09Z","snapshot_observed_at":"2026-08-17T13:41:03.609315Z","submitted_at":"2025-05-16T18:00:09Z","title":"Dust stars in the minimal exponential measure model","version":1},"reference_index":56,"source":"pdf_text","source_observed_at":"2026-08-15T21:01:47.989206Z"},"links":{"cited_paper":"/paper/2109.06456","citing_paper":"/paper/2505.11591"},"observation_digest":"sha256:4cf4073b468d94c05c72c138209dbed2653afcc0b4959653e0c586cc309ad60d","observation_id":"86e57b44-1dec-4f94-81b8-f932b84cffed","resolution":{"observed_at":"2026-08-15T21:01:47.989206Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2002.12533","last_updated":"2020-09-09T01:17:18Z","snapshot_observed_at":"2026-08-15T03:28:05.756941Z","submitted_at":"2020-02-28T03:59:54Z","title":"First Constraints on Compact Dark Matter from Fast Radio Burst Microstructure","version":5},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2002.12533","snapshot_observed_at":"2026-08-15T21:01:47.992151Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2505.11591","last_updated":"2025-05-16T18:00:09Z","snapshot_observed_at":"2026-08-17T13:41:03.609315Z","submitted_at":"2025-05-16T18:00:09Z","title":"Dust stars in the minimal exponential measure model","version":1},"reference_index":57,"source":"pdf_text","source_observed_at":"2026-08-15T21:01:47.992151Z"},"links":{"cited_paper":"/paper/2002.12533","citing_paper":"/paper/2505.11591"},"observation_digest":"sha256:680a3e8b84220eba8cb0959e3140a2d639220e06e7ba3bb4bd526c0dfad6a80c","observation_id":"125583b5-540e-491c-a126-592644a71b84","resolution":{"observed_at":"2026-08-15T21:01:47.992151Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2410.07956","last_updated":"2024-11-20T12:08:23Z","snapshot_observed_at":"2026-08-16T13:10:41.790989Z","submitted_at":"2024-10-10T14:22:24Z","title":"Constraints on compact objects from the Dark Energy Survey five-year supernova sample","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2410.07956","snapshot_observed_at":"2026-08-15T21:01:47.995167Z","title":"Shahet al.(DES), Mon","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2505.11591","last_updated":"2025-05-16T18:00:09Z","snapshot_observed_at":"2026-08-17T13:41:03.609315Z","submitted_at":"2025-05-16T18:00:09Z","title":"Dust stars in the minimal exponential measure model","version":1},"reference_index":58,"source":"pdf_text","source_observed_at":"2026-08-15T21:01:47.995167Z"},"links":{"cited_paper":"/paper/2410.07956","citing_paper":"/paper/2505.11591"},"observation_digest":"sha256:3f021e77e9a58ed1d23b1f2972bf51f0a147a34dcb25f5cd23695ec55f397b39","observation_id":"9fd42373-e314-4906-b4d5-ecaa12723028","resolution":{"observed_at":"2026-08-15T21:01:47.995167Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1605.03665","last_updated":"2016-06-09T20:04:23Z","snapshot_observed_at":"2026-08-15T11:56:43.020632Z","submitted_at":"2016-05-12T03:19:31Z","title":"Constraints on MACHO Dark Matter from Compact Stellar Systems in Ultra-Faint Dwarf Galaxies","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1605.03665","snapshot_observed_at":"2026-08-15T21:01:47.998890Z","title":null,"venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2505.11591","last_updated":"2025-05-16T18:00:09Z","snapshot_observed_at":"2026-08-17T13:41:03.609315Z","submitted_at":"2025-05-16T18:00:09Z","title":"Dust stars in the minimal exponential measure model","version":1},"reference_index":59,"source":"pdf_text","source_observed_at":"2026-08-15T21:01:47.998890Z"},"links":{"cited_paper":"/paper/1605.03665","citing_paper":"/paper/2505.11591"},"observation_digest":"sha256:a18be7a6979ffb0a5695aac911c59075c14ebee3b8d51b30e6b3e48594fd0fdc","observation_id":"8de326f3-3889-46b6-bd26-773dc0a4280e","resolution":{"observed_at":"2026-08-15T21:01:47.998890Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1202.5809","last_updated":"2023-02-11T22:07:32Z","snapshot_observed_at":"2026-08-08T15:48:17.017551Z","submitted_at":"2012-02-27T00:47:39Z","title":"Dynamical Boson Stars","version":5},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1202.5809","snapshot_observed_at":"2026-08-15T21:01:48.002120Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2505.11591","last_updated":"2025-05-16T18:00:09Z","snapshot_observed_at":"2026-08-17T13:41:03.609315Z","submitted_at":"2025-05-16T18:00:09Z","title":"Dust stars in the minimal exponential measure model","version":1},"reference_index":60,"source":"pdf_text","source_observed_at":"2026-08-15T21:01:48.002120Z"},"links":{"cited_paper":"/paper/1202.5809","citing_paper":"/paper/2505.11591"},"observation_digest":"sha256:6599895061b67b51f806eaaf04465e1bd1bc704913e886deec5784fdc957f811","observation_id":"24828d3a-8d1f-41a6-a863-9869059e66a2","resolution":{"observed_at":"2026-08-15T21:01:48.002120Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2109.05481","last_updated":"2023-01-12T05:47:33Z","snapshot_observed_at":"2026-08-16T17:57:15.134471Z","submitted_at":"2021-09-12T10:23:13Z","title":"Boson Stars and Oscillatons: A Review","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2109.05481","snapshot_observed_at":"2026-08-15T21:01:48.005705Z","title":"Visinelli, Int","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2505.11591","last_updated":"2025-05-16T18:00:09Z","snapshot_observed_at":"2026-08-17T13:41:03.609315Z","submitted_at":"2025-05-16T18:00:09Z","title":"Dust stars in the minimal exponential measure model","version":1},"reference_index":61,"source":"pdf_text","source_observed_at":"2026-08-15T21:01:48.005705Z"},"links":{"cited_paper":"/paper/2109.05481","citing_paper":"/paper/2505.11591"},"observation_digest":"sha256:f283cf15313621ecff6d0dffb0566382ca6310dc26607a2ce6f9449f59081994","observation_id":"f26f9e1c-ede5-4d5f-8787-4acef5bd4a3a","resolution":{"observed_at":"2026-08-15T21:01:48.005705Z","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":"2026-08-15T21:01:48.008981Z","title":null,"venue":null,"work_id":null,"year":1968},"citing_paper":{"arxiv_id":"2505.11591","last_updated":"2025-05-16T18:00:09Z","snapshot_observed_at":"2026-08-17T13:41:03.609315Z","submitted_at":"2025-05-16T18:00:09Z","title":"Dust stars in the minimal exponential measure model","version":1},"reference_index":62,"source":"pdf_text","source_observed_at":"2026-08-15T21:01:48.008981Z"},"links":{"citing_paper":"/paper/2505.11591"},"observation_digest":"sha256:1c9bb2d3bae11d072a4aba1936fbd104e767cb6f443412ce431bd8305f1bff40","observation_id":"6658bdbd-06ab-436a-b73f-023c0beb70b4","resolution":{"observed_at":"2026-08-15T21:01:48.008981Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2310.19857","last_updated":"2023-10-30T17:54:47Z","snapshot_observed_at":"2026-08-16T14:47:31.749285Z","submitted_at":"2023-10-30T17:54:47Z","title":"Primordial black holes and their gravitational-wave signatures","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2310.19857","snapshot_observed_at":"2026-08-15T21:01:48.011553Z","title":"Baguiet al.(LISA Cosmology Working Group), Living Rev","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2505.11591","last_updated":"2025-05-16T18:00:09Z","snapshot_observed_at":"2026-08-17T13:41:03.609315Z","submitted_at":"2025-05-16T18:00:09Z","title":"Dust stars in the minimal exponential measure model","version":1},"reference_index":63,"source":"pdf_text","source_observed_at":"2026-08-15T21:01:48.011553Z"},"links":{"cited_paper":"/paper/2310.19857","citing_paper":"/paper/2505.11591"},"observation_digest":"sha256:837c3082d0d23c5e44d670282c2ed371a9d824d5fb7a0b62745d92941259d257","observation_id":"88ef1e36-597c-4cc8-add0-7fa050375094","resolution":{"observed_at":"2026-08-15T21:01:48.011553Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"2505.11591","last_updated":"2025-05-16T18:00:09Z","latest_version":1,"primary_category":"gr-qc","snapshot_observed_at":"2026-08-17T13:41:03.609315Z","submitted_at":"2025-05-16T18:00:09Z","title":"Dust stars in the minimal exponential measure model"},"reference_resolution":{"displayed":63,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":47,"verified_exact":4,"verified_fuzzy":12},"total_outbound_references":63},"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 63 of 63 outbound references and 0 inbound Pith citation observations for arXiv:2505.11591."}