{"as_of":"2026-08-10T09:37:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:c6a99782ec28e208ef4865b11fdb1bd8cf863c37ea13a22fa54ac73b7faa67fa","coverage":[{"denominator":79,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":79,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-08T10:10:48.516830Z","state":"measured"},{"denominator":79,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":79,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-10T06:31:04.303077+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/2608.05582/citation-record","integrity":"/paper/2608.05582/integrity","json":"/paper/2608.05582/citation-record.json","paper":"/paper/2608.05582"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-08T10:10:50.683775Z","title":"We show in Fig","venue":null,"work_id":"01c97a59-69d2-47c7-9678-55cdd0f66a50","year":null},"citing_paper":{"arxiv_id":"2608.05582","last_updated":"2026-08-06T04:10:03Z","snapshot_observed_at":"2026-08-09T23:11:06.657264Z","submitted_at":"2026-08-06T04:10:03Z","title":"Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects","version":1},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-08T10:10:48.142680Z"},"links":{"citing_paper":"/paper/2608.05582"},"observation_digest":"sha256:913b6be2ce406338dfb9f4b1ccb2de000d44540cfc9ad412023eced89d4969c0","observation_id":"6cd2c01e-4600-4cfe-823f-1312e0f030aa","resolution":{"observed_at":"2026-08-08T10:10:50.688569Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+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":"2026-08-08T10:10:50.665809Z","title":"After the core bounce, the shock wave stalls and recedes as a result of intense mass accretion","venue":null,"work_id":"428ca43d-1603-44b9-b30f-8d9574167499","year":null},"citing_paper":{"arxiv_id":"2608.05582","last_updated":"2026-08-06T04:10:03Z","snapshot_observed_at":"2026-08-09T23:11:06.657264Z","submitted_at":"2026-08-06T04:10:03Z","title":"Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects","version":1},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-08T10:10:48.147849Z"},"links":{"citing_paper":"/paper/2608.05582"},"observation_digest":"sha256:4cb5570432a1eacb9fd878515866c163f63ed279d888c73fba4fd55f6f9b7054","observation_id":"67323f27-3e6b-45e8-8b01-741ae74bccf3","resolution":{"observed_at":"2026-08-08T10:10:50.671883Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+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":"2026-08-08T10:10:48.164310Z","title":null,"venue":null,"work_id":null,"year":1990},"citing_paper":{"arxiv_id":"2608.05582","last_updated":"2026-08-06T04:10:03Z","snapshot_observed_at":"2026-08-09T23:11:06.657264Z","submitted_at":"2026-08-06T04:10:03Z","title":"Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects","version":1},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-08T10:10:48.164310Z"},"links":{"citing_paper":"/paper/2608.05582"},"observation_digest":"sha256:e391f6e7eeec5f8cfd7e15cfce22235fffbbeb4ec2ab5876bd5f4d6710537a68","observation_id":"1846ad84-f6a5-4bc1-8440-610e1fa2932f","resolution":{"observed_at":"2026-08-08T10:10:48.164310Z","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":"2026-08-08T10:10:50.640085Z","title":null,"venue":null,"work_id":"0b4e31ce-85be-41a6-9bf8-87a0db6f4fe2","year":1985},"citing_paper":{"arxiv_id":"2608.05582","last_updated":"2026-08-06T04:10:03Z","snapshot_observed_at":"2026-08-09T23:11:06.657264Z","submitted_at":"2026-08-06T04:10:03Z","title":"Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects","version":1},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-08T10:10:48.169585Z"},"links":{"citing_paper":"/paper/2608.05582"},"observation_digest":"sha256:7ca533c1f5c7317dc6b8e13eb573d0a7878953c8090104c5d33b9b0b12297eac","observation_id":"d1059002-d89b-4e2b-a4b3-19bc9635c699","resolution":{"observed_at":"2026-08-08T10:10:50.645202Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1610.03361","last_updated":"2016-10-11T14:29:10Z","snapshot_observed_at":"2026-07-06T05:14:11.208979Z","submitted_at":"2016-10-11T14:29:10Z","title":"Equations of state for supernovae and compact stars","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1610.03361","snapshot_observed_at":"2026-08-08T10:10:48.153127Z","title":"Oertel, M","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2608.05582","last_updated":"2026-08-06T04:10:03Z","snapshot_observed_at":"2026-08-09T23:11:06.657264Z","submitted_at":"2026-08-06T04:10:03Z","title":"Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects","version":1},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-08T10:10:48.153127Z"},"links":{"cited_paper":"/paper/1610.03361","citing_paper":"/paper/2608.05582"},"observation_digest":"sha256:bbc2fdbb7f92d903d36ffe7e80aae4e76e52b8fb021d505d877738130fe3fdc3","observation_id":"4f1d3d30-437b-4eba-8fc9-13d25f32152c","resolution":{"observed_at":"2026-08-08T10:10:48.153127Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2207.00033","last_updated":"2022-06-30T18:01:15Z","snapshot_observed_at":"2026-07-06T13:26:33.250328Z","submitted_at":"2022-06-30T18:01:15Z","title":"Equation of state in neutron stars and supernovae","version":1},"cited_work":{"arxiv_id":"2207.00033","doi":null,"metadata_source":"pith","pith_arxiv_id":"2207.00033","snapshot_observed_at":"2026-08-08T10:10:50.404657Z","title":"Equation of state in neutron stars and supernovae","venue":"nucl-th","work_id":"a38eb1b6-8366-4b60-ab0c-450c87d439a2","year":2022},"citing_paper":{"arxiv_id":"2608.05582","last_updated":"2026-08-06T04:10:03Z","snapshot_observed_at":"2026-08-09T23:11:06.657264Z","submitted_at":"2026-08-06T04:10:03Z","title":"Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects","version":1},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-08T10:10:48.158615Z"},"links":{"cited_paper":"/paper/2207.00033","citing_paper":"/paper/2608.05582"},"observation_digest":"sha256:b240edb86374fc82ca82a5a5d8a73ba4f30b0a07352b0ae8788c6b9847ddb457","observation_id":"c256ca78-6fae-46ab-a186-8eb1d12d4d13","resolution":{"observed_at":"2026-08-08T10:10:50.409889Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1110.5107","last_updated":"2012-04-10T05:49:55Z","snapshot_observed_at":"2026-07-06T02:36:17.251994Z","submitted_at":"2011-10-24T01:15:32Z","title":"Multiple physical elements to determine the gravitational-wave signatures of core-collapse supernovae","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1110.5107","snapshot_observed_at":"2026-08-08T10:10:48.183848Z","title":null,"venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2608.05582","last_updated":"2026-08-06T04:10:03Z","snapshot_observed_at":"2026-08-09T23:11:06.657264Z","submitted_at":"2026-08-06T04:10:03Z","title":"Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects","version":1},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-08T10:10:48.183848Z"},"links":{"cited_paper":"/paper/1110.5107","citing_paper":"/paper/2608.05582"},"observation_digest":"sha256:9ffe2eef5b186f2c468087f1629ab4a54be0c049df8fff0042cf16b8dbce228e","observation_id":"39ab832f-d9e2-4ee9-aeb2-475895606fdf","resolution":{"observed_at":"2026-08-08T10:10:48.183848Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1602.05576","last_updated":"2016-02-17T21:00:01Z","snapshot_observed_at":"2026-07-06T04:46:31.221295Z","submitted_at":"2016-02-17T21:00:01Z","title":"Physics of Core-Collapse Supernovae in Three Dimensions: a Sneak Preview","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1602.05576","snapshot_observed_at":"2026-08-08T10:10:48.188277Z","title":"Janka, T","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2608.05582","last_updated":"2026-08-06T04:10:03Z","snapshot_observed_at":"2026-08-09T23:11:06.657264Z","submitted_at":"2026-08-06T04:10:03Z","title":"Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects","version":1},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-08T10:10:48.188277Z"},"links":{"cited_paper":"/paper/1602.05576","citing_paper":"/paper/2608.05582"},"observation_digest":"sha256:b3a153ffc65e7256d38c93d57fa37b5312e8758a99fd6fae635efcba80b2e5dc","observation_id":"d5c0d76b-fbe5-4e89-a410-04c10027ca91","resolution":{"observed_at":"2026-08-08T10:10:48.188277Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1206.2503","last_updated":"2012-06-12T12:12:02Z","snapshot_observed_at":"2026-08-04T00:00:05.427259Z","submitted_at":"2012-06-12T12:12:02Z","title":"Explosion Mechanisms of Core-Collapse Supernovae","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1206.2503","snapshot_observed_at":"2026-08-08T10:10:48.174417Z","title":"Janka, Explosion Mechanisms of Core-Collapse Supernovae, Annual Review of Nuclear and Particle Science62, 407 (2012), arXiv:1206.2503 [astro-ph.SR]","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2608.05582","last_updated":"2026-08-06T04:10:03Z","snapshot_observed_at":"2026-08-09T23:11:06.657264Z","submitted_at":"2026-08-06T04:10:03Z","title":"Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects","version":1},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-08T10:10:48.174417Z"},"links":{"cited_paper":"/paper/1206.2503","citing_paper":"/paper/2608.05582"},"observation_digest":"sha256:1c787360eb5ed7080a319ebeceddc16092ba616f00fbbad4b4217b41e789f600","observation_id":"6d802845-6f1f-40cf-84d2-b4fcf1470284","resolution":{"observed_at":"2026-08-08T10:10:48.174417Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1210.4921","last_updated":"2012-10-17T20:00:00Z","snapshot_observed_at":"2026-08-02T00:23:24.554538Z","submitted_at":"2012-10-17T20:00:00Z","title":"Perspectives on Core-Collapse Supernova Theory","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1210.4921","snapshot_observed_at":"2026-08-08T10:10:48.179004Z","title":"Burrows, Colloquium: Perspectives on core-collapse supernova theory, Reviews of Modern Physics85, 245 (2013), arXiv:1210.4921 [astro-ph.SR]","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2608.05582","last_updated":"2026-08-06T04:10:03Z","snapshot_observed_at":"2026-08-09T23:11:06.657264Z","submitted_at":"2026-08-06T04:10:03Z","title":"Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects","version":1},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-08T10:10:48.179004Z"},"links":{"cited_paper":"/paper/1210.4921","citing_paper":"/paper/2608.05582"},"observation_digest":"sha256:1ed8a4de87b6fa1062ab8cc3691070b04f9fa17fe93780f3ecfb95bc54be4170","observation_id":"2b2d01d3-0982-404d-8f21-f6df25de01e2","resolution":{"observed_at":"2026-08-08T10:10:48.179004Z","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":"2026-08-08T10:10:50.715911Z","title":null,"venue":null,"work_id":"b136a95d-bd58-49fd-aeaa-cb5c97b1e785","year":null},"citing_paper":{"arxiv_id":"2608.05582","last_updated":"2026-08-06T04:10:03Z","snapshot_observed_at":"2026-08-09T23:11:06.657264Z","submitted_at":"2026-08-06T04:10:03Z","title":"Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects","version":1},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-08T10:10:48.130700Z"},"links":{"citing_paper":"/paper/2608.05582"},"observation_digest":"sha256:b6ab520561f28323e5d3074fa94aff490de206ece4766c4325fdee596ace9fcc","observation_id":"dfba1bbe-0bda-444e-b1f7-14562c122844","resolution":{"observed_at":"2026-08-08T10:10:50.720854Z","resolver_source":"raw_fallback","status":"malformed_identifier"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+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":"2026-08-08T10:10:50.595408Z","title":null,"venue":null,"work_id":"63734759-6eaa-4ff5-aaed-1e7f72ab413c","year":2021},"citing_paper":{"arxiv_id":"2608.05582","last_updated":"2026-08-06T04:10:03Z","snapshot_observed_at":"2026-08-09T23:11:06.657264Z","submitted_at":"2026-08-06T04:10:03Z","title":"Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects","version":1},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-08T10:10:48.213248Z"},"links":{"citing_paper":"/paper/2608.05582"},"observation_digest":"sha256:eab85ef099a4640a8a077311d734846b7a5e92ed85c5361e0942fa4f488e7aa5","observation_id":"c8edc849-b621-44f0-a197-30cf57b8b6ba","resolution":{"observed_at":"2026-08-08T10:10:50.599935Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+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":"2026-08-08T10:10:50.624754Z","title":"Janka, Neutrino-Driven Explosions, inHandbook of Supernovae, ISBN 978-3-319-21845-","venue":null,"work_id":"47847e4b-9737-4c63-86c1-d27608088b4a","year":null},"citing_paper":{"arxiv_id":"2608.05582","last_updated":"2026-08-06T04:10:03Z","snapshot_observed_at":"2026-08-09T23:11:06.657264Z","submitted_at":"2026-08-06T04:10:03Z","title":"Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects","version":1},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-08T10:10:48.192798Z"},"links":{"citing_paper":"/paper/2608.05582"},"observation_digest":"sha256:11d7940e4bcb99e64988def065c66a530343c56fc515fa69d89edfe8b62816c1","observation_id":"5bc72b79-e6d3-4632-adb9-2251da272fbc","resolution":{"observed_at":"2026-08-08T10:10:50.629557Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+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":"2026-08-08T10:10:50.610117Z","title":"1095(Springer, 2017) p","venue":null,"work_id":"3f63d979-60d7-4b44-ad65-ea5684190265","year":2017},"citing_paper":{"arxiv_id":"2608.05582","last_updated":"2026-08-06T04:10:03Z","snapshot_observed_at":"2026-08-09T23:11:06.657264Z","submitted_at":"2026-08-06T04:10:03Z","title":"Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects","version":1},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-08T10:10:48.198268Z"},"links":{"citing_paper":"/paper/2608.05582"},"observation_digest":"sha256:7b022fd9787eb2608b1c5dc45754374c98b9608e1571e54cc2c8bbba543447f3","observation_id":"37387fa7-5d7d-431d-ba0c-2ad2da3277d5","resolution":{"observed_at":"2026-08-08T10:10:50.614843Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+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":"2026-08-08T10:10:48.203104Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2608.05582","last_updated":"2026-08-06T04:10:03Z","snapshot_observed_at":"2026-08-09T23:11:06.657264Z","submitted_at":"2026-08-06T04:10:03Z","title":"Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects","version":1},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-08T10:10:48.203104Z"},"links":{"citing_paper":"/paper/2608.05582"},"observation_digest":"sha256:855c6f009a07a0cd586a1fba225a221624260a5ff587df20637ee69b81cf6849","observation_id":"b6063a1c-0102-472c-88a3-963acd992809","resolution":{"observed_at":"2026-08-08T10:10:48.203104Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2212.07498","last_updated":"2023-02-20T17:31:23Z","snapshot_observed_at":"2026-07-06T14:30:44.117201Z","submitted_at":"2022-12-14T20:37:45Z","title":"Dynamics and Equation of State Dependencies of Relevance for Nucleosynthesis in Supernovae and Neutron Star Mergers","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2212.07498","snapshot_observed_at":"2026-08-08T10:10:48.207933Z","title":"Janka and A","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2608.05582","last_updated":"2026-08-06T04:10:03Z","snapshot_observed_at":"2026-08-09T23:11:06.657264Z","submitted_at":"2026-08-06T04:10:03Z","title":"Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects","version":1},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-08T10:10:48.207933Z"},"links":{"cited_paper":"/paper/2212.07498","citing_paper":"/paper/2608.05582"},"observation_digest":"sha256:fc0cb455e3e31bd13d26076d4a244c35673f92428600eff36bfb9ccdb7d5dc4e","observation_id":"d15a13d8-fc0f-461d-bba0-213ca3cb75d4","resolution":{"observed_at":"2026-08-08T10:10:48.207933Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1904.11067","last_updated":"2019-04-24T21:01:24Z","snapshot_observed_at":"2026-07-06T07:48:11.809456Z","submitted_at":"2019-04-24T21:01:24Z","title":"Neutrino Emission as Diagnostics of Core-Collapse Supernovae","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1904.11067","snapshot_observed_at":"2026-08-08T10:10:48.238282Z","title":"M¨ uller, Neutrino Emission as Diagnostics of Core-Collapse Supernovae, Annual Review of Nuclear and Particle Science69, 253 (2019), arXiv:1904.11067 [astro-ph.HE]","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2608.05582","last_updated":"2026-08-06T04:10:03Z","snapshot_observed_at":"2026-08-09T23:11:06.657264Z","submitted_at":"2026-08-06T04:10:03Z","title":"Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects","version":1},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-08T10:10:48.238282Z"},"links":{"cited_paper":"/paper/1904.11067","citing_paper":"/paper/2608.05582"},"observation_digest":"sha256:612b3c79c22255ce73663c066f3c428cdfcaa61715ad6893173a0435a06fc49c","observation_id":"146e1608-5ef8-40bb-afcd-14b4d6e9cc74","resolution":{"observed_at":"2026-08-08T10:10:48.238282Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2105.03747","last_updated":"2021-05-08T17:25:09Z","snapshot_observed_at":"2026-07-06T11:07:31.660804Z","submitted_at":"2021-05-08T17:25:09Z","title":"Neutron Stars and the Nuclear Equation of State","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2105.03747","snapshot_observed_at":"2026-08-08T10:10:48.217883Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2608.05582","last_updated":"2026-08-06T04:10:03Z","snapshot_observed_at":"2026-08-09T23:11:06.657264Z","submitted_at":"2026-08-06T04:10:03Z","title":"Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects","version":1},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-08T10:10:48.217883Z"},"links":{"cited_paper":"/paper/2105.03747","citing_paper":"/paper/2608.05582"},"observation_digest":"sha256:aec253988f99858d4d8c2eb799b5260633ca51ebfd7d1239ee50464a4de86e1b","observation_id":"ad6e2985-55be-42e7-b53f-66edf7bb903c","resolution":{"observed_at":"2026-08-08T10:10:48.217883Z","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":"2026-08-08T10:10:48.222733Z","title":"Chatziioannou, H","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2608.05582","last_updated":"2026-08-06T04:10:03Z","snapshot_observed_at":"2026-08-09T23:11:06.657264Z","submitted_at":"2026-08-06T04:10:03Z","title":"Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects","version":1},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-08T10:10:48.222733Z"},"links":{"citing_paper":"/paper/2608.05582"},"observation_digest":"sha256:943bd36fd567bf17d2c117d9dffc986b916efdc5cc9a8ecf1a81ba95918f1e5a","observation_id":"a2f91066-4f6e-460a-b2bd-5cc52669b300","resolution":{"observed_at":"2026-08-08T10:10:48.222733Z","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":"ph/0509456","doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-08T10:10:49.907492Z","title":"Kotake, K","venue":null,"work_id":"0fe68430-d4f8-454d-8071-6c158a6d95a2","year":2006},"citing_paper":{"arxiv_id":"2608.05582","last_updated":"2026-08-06T04:10:03Z","snapshot_observed_at":"2026-08-09T23:11:06.657264Z","submitted_at":"2026-08-06T04:10:03Z","title":"Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects","version":1},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-08T10:10:48.227411Z"},"links":{"citing_paper":"/paper/2608.05582"},"observation_digest":"sha256:82437656ff74ca2e462d4717e41307207bf87dc62de6edde7eebfb17d43f5e68","observation_id":"19608c22-78e8-4856-940c-ce1ee9a9a42b","resolution":{"observed_at":"2026-08-08T10:10:49.915232Z","resolver_source":"raw_fallback","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1508.00785","last_updated":"2016-02-05T10:48:32Z","snapshot_observed_at":"2026-07-06T04:25:46.543674Z","submitted_at":"2015-07-31T20:09:50Z","title":"Supernova Neutrinos: Production, Oscillations and Detection","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1508.00785","snapshot_observed_at":"2026-08-08T10:10:48.232689Z","title":"Mirizzi, I","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2608.05582","last_updated":"2026-08-06T04:10:03Z","snapshot_observed_at":"2026-08-09T23:11:06.657264Z","submitted_at":"2026-08-06T04:10:03Z","title":"Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects","version":1},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-08T10:10:48.232689Z"},"links":{"cited_paper":"/paper/1508.00785","citing_paper":"/paper/2608.05582"},"observation_digest":"sha256:fa027a2e031d92431e34fd61a2643f9d19dbd4d7c3b337bee8a065264fb312af","observation_id":"7ffa1408-a212-4347-89d1-967876a35168","resolution":{"observed_at":"2026-08-08T10:10:48.232689Z","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":"2026-08-08T10:10:50.550041Z","title":"Takahara and K","venue":null,"work_id":"98a638c5-f1ce-446c-ac07-9ed8b5481506","year":1988},"citing_paper":{"arxiv_id":"2608.05582","last_updated":"2026-08-06T04:10:03Z","snapshot_observed_at":"2026-08-09T23:11:06.657264Z","submitted_at":"2026-08-06T04:10:03Z","title":"Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects","version":1},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-08T10:10:48.263442Z"},"links":{"citing_paper":"/paper/2608.05582"},"observation_digest":"sha256:4bcf8233c38f63eda16b2c650b0c3b0026562f28dd5314a0f90c356e96b629ab","observation_id":"3de72a04-1357-49f3-9a9a-2610068bdd57","resolution":{"observed_at":"2026-08-08T10:10:50.554654Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2010.04356","last_updated":"2022-01-01T08:33:41Z","snapshot_observed_at":"2026-07-06T10:02:51.179347Z","submitted_at":"2020-10-09T03:56:02Z","title":"Gravitational Waves from Core-Collapse Supernovae","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2010.04356","snapshot_observed_at":"2026-08-08T10:10:48.244041Z","title":"Abdikamalov, G","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2608.05582","last_updated":"2026-08-06T04:10:03Z","snapshot_observed_at":"2026-08-09T23:11:06.657264Z","submitted_at":"2026-08-06T04:10:03Z","title":"Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects","version":1},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-08T10:10:48.244041Z"},"links":{"cited_paper":"/paper/2010.04356","citing_paper":"/paper/2608.05582"},"observation_digest":"sha256:7efd6bfd33ac90b7750432d9efebdef209f0e06b9a9395bb3fa365ef28ceb5d5","observation_id":"7fdb5981-ff61-495c-987b-3bf708815cb6","resolution":{"observed_at":"2026-08-08T10:10:48.244041Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2603.24243","last_updated":"2026-07-15T03:34:44Z","snapshot_observed_at":"2026-08-07T17:37:37.761675Z","submitted_at":"2026-03-25T12:29:39Z","title":"Core-Collapse Supernovae and their Gravitational Wave Signals: The Status of Theory and Modeling","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2603.24243","snapshot_observed_at":"2026-08-08T10:10:48.248912Z","title":null,"venue":null,"work_id":null,"year":2026},"citing_paper":{"arxiv_id":"2608.05582","last_updated":"2026-08-06T04:10:03Z","snapshot_observed_at":"2026-08-09T23:11:06.657264Z","submitted_at":"2026-08-06T04:10:03Z","title":"Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects","version":1},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-08T10:10:48.248912Z"},"links":{"cited_paper":"/paper/2603.24243","citing_paper":"/paper/2608.05582"},"observation_digest":"sha256:6d58c9fea01af68574500f1729bc4a128d75442075a4005733ffffa5624a9c75","observation_id":"e0d3b64a-fb2d-4c49-9244-0a31f3fe0d63","resolution":{"observed_at":"2026-08-08T10:10:48.248912Z","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":"2026-08-08T10:10:50.580833Z","title":"Sotani, Understanding supernova gravitational waves with protoneutron star asteroseis- mology, Classical and Quantum Gravity43, 093001 (2026)","venue":null,"work_id":"9d44f242-c3b6-4b88-9152-a999aec2ba56","year":2026},"citing_paper":{"arxiv_id":"2608.05582","last_updated":"2026-08-06T04:10:03Z","snapshot_observed_at":"2026-08-09T23:11:06.657264Z","submitted_at":"2026-08-06T04:10:03Z","title":"Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects","version":1},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-08T10:10:48.253931Z"},"links":{"citing_paper":"/paper/2608.05582"},"observation_digest":"sha256:24b2211e6dc63f8abd43b9a427bd03e8aa2bb94662db2cc34c73b78e433e70c1","observation_id":"9daffa2e-0a9e-4156-8d80-f9db6b0fe185","resolution":{"observed_at":"2026-08-08T10:10:50.585537Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+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":"2026-08-08T10:10:50.565743Z","title":"Baron, J","venue":null,"work_id":"8e84cf96-5dc1-4fd3-b414-4b7e3eb4e917","year":1985},"citing_paper":{"arxiv_id":"2608.05582","last_updated":"2026-08-06T04:10:03Z","snapshot_observed_at":"2026-08-09T23:11:06.657264Z","submitted_at":"2026-08-06T04:10:03Z","title":"Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects","version":1},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-08T10:10:48.258735Z"},"links":{"citing_paper":"/paper/2608.05582"},"observation_digest":"sha256:68286e42571c93beac02f5cbe4b5198c29e4fc3f81f7890c76a0eeca09f0f2fe","observation_id":"a59a8034-ff33-4888-8972-0efe12632551","resolution":{"observed_at":"2026-08-08T10:10:50.570557Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1207.2184","last_updated":"2012-07-09T21:00:43Z","snapshot_observed_at":"2026-08-10T06:35:57.906968Z","submitted_at":"2012-07-09T21:00:43Z","title":"Core-collapse supernova equations of state based on neutron star observations","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1207.2184","snapshot_observed_at":"2026-08-08T10:10:48.287208Z","title":null,"venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2608.05582","last_updated":"2026-08-06T04:10:03Z","snapshot_observed_at":"2026-08-09T23:11:06.657264Z","submitted_at":"2026-08-06T04:10:03Z","title":"Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects","version":1},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-08T10:10:48.287208Z"},"links":{"cited_paper":"/paper/1207.2184","citing_paper":"/paper/2608.05582"},"observation_digest":"sha256:70541e589569f1994cb0cf52148c74b3d08d1ff3b21c70f141fb465159e946d0","observation_id":"11d8c854-4776-48bd-9331-11aa89e577ef","resolution":{"observed_at":"2026-08-08T10:10:48.287208Z","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":"2026-08-08T10:10:50.534838Z","title":null,"venue":null,"work_id":"073ef985-17a0-4048-b2d3-ed2f5bf9f4ef","year":1994},"citing_paper":{"arxiv_id":"2608.05582","last_updated":"2026-08-06T04:10:03Z","snapshot_observed_at":"2026-08-09T23:11:06.657264Z","submitted_at":"2026-08-06T04:10:03Z","title":"Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects","version":1},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-08T10:10:48.268204Z"},"links":{"citing_paper":"/paper/2608.05582"},"observation_digest":"sha256:d408428ae4d7efdc1c64161a075e71f7d0fe23be43f4144b5d7200672fb569c2","observation_id":"b5158629-9ad1-4b54-9bbc-a05d92144dd6","resolution":{"observed_at":"2026-08-08T10:10:50.539735Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0211194","last_updated":"2003-04-02T18:22:46Z","snapshot_observed_at":"2026-08-09T19:33:15.757974Z","submitted_at":"2002-11-10T22:15:02Z","title":"Shock Breakout in Core-Collapse Supernovae and its Neutrino Signature","version":2},"cited_work":{"arxiv_id":"astro-ph/0211194","doi":null,"metadata_source":"pith","pith_arxiv_id":"astro-ph/0211194","snapshot_observed_at":"2026-08-08T10:10:49.693989Z","title":"Shock Breakout in Core-Collapse Supernovae and its Neutrino Signature","venue":"astro-ph","work_id":"8b23bf45-1353-4e7e-b35f-a5a8506a201a","year":2002},"citing_paper":{"arxiv_id":"2608.05582","last_updated":"2026-08-06T04:10:03Z","snapshot_observed_at":"2026-08-09T23:11:06.657264Z","submitted_at":"2026-08-06T04:10:03Z","title":"Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects","version":1},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-08T10:10:48.272671Z"},"links":{"cited_paper":"/paper/astro-ph/0211194","citing_paper":"/paper/2608.05582"},"observation_digest":"sha256:e6b2a4289f9401983c64552bafd24412d9f83533f8a5271cf5d903a7cca79fd1","observation_id":"d84080b8-8c5d-4cbd-b7f0-0ca2dc2a37ac","resolution":{"observed_at":"2026-08-08T10:10:49.699501Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0506620","last_updated":"2005-06-25T04:26:39Z","snapshot_observed_at":"2026-07-07T00:51:43.193510Z","submitted_at":"2005-06-25T04:26:39Z","title":"Postbounce evolution of core-collapse supernovae: Long-term effects of equation of state","version":1},"cited_work":{"arxiv_id":"astro-ph/0506620","doi":null,"metadata_source":"pith","pith_arxiv_id":"astro-ph/0506620","snapshot_observed_at":"2026-08-08T10:10:49.672179Z","title":"Postbounce evolution of core-collapse supernovae: Long-term effects of equation of state","venue":"astro-ph","work_id":"e24739ea-6549-435e-9559-6800d68491d1","year":2005},"citing_paper":{"arxiv_id":"2608.05582","last_updated":"2026-08-06T04:10:03Z","snapshot_observed_at":"2026-08-09T23:11:06.657264Z","submitted_at":"2026-08-06T04:10:03Z","title":"Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects","version":1},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-08T10:10:48.277374Z"},"links":{"cited_paper":"/paper/astro-ph/0506620","citing_paper":"/paper/2608.05582"},"observation_digest":"sha256:8f10f176980b7ab3ae08d46e06f84345ecd1a258ad92e70b39d78972b86e5dbc","observation_id":"d1a55cbf-f2fb-4621-a0bd-0711205814c5","resolution":{"observed_at":"2026-08-08T10:10:49.677150Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1011.3409","last_updated":"2011-04-14T09:41:16Z","snapshot_observed_at":"2026-08-05T02:08:27.962255Z","submitted_at":"2010-11-10T16:31:00Z","title":"Core-collapse supernova explosions triggered by a quark-hadron phase transition during the early post-bounce phase","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1011.3409","snapshot_observed_at":"2026-08-08T10:10:48.282144Z","title":"Fischer, I","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2608.05582","last_updated":"2026-08-06T04:10:03Z","snapshot_observed_at":"2026-08-09T23:11:06.657264Z","submitted_at":"2026-08-06T04:10:03Z","title":"Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects","version":1},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-08-08T10:10:48.282144Z"},"links":{"cited_paper":"/paper/1011.3409","citing_paper":"/paper/2608.05582"},"observation_digest":"sha256:0d9d129dfb74cb35f6d53481758bb75b312e3e6e89f0c824d692f8fbe9f22308","observation_id":"db00897c-9ee9-4363-9353-6b81f5cf0b5c","resolution":{"observed_at":"2026-08-08T10:10:48.282144Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1701.02752","last_updated":"2017-03-03T18:51:23Z","snapshot_observed_at":"2026-08-09T00:35:56.931029Z","submitted_at":"2017-01-10T19:01:10Z","title":"Equation of State Effects on Gravitational Waves from Rotating Core Collapse","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1701.02752","snapshot_observed_at":"2026-08-08T10:10:48.310511Z","title":"Richers, C","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2608.05582","last_updated":"2026-08-06T04:10:03Z","snapshot_observed_at":"2026-08-09T23:11:06.657264Z","submitted_at":"2026-08-06T04:10:03Z","title":"Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects","version":1},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-08T10:10:48.310511Z"},"links":{"cited_paper":"/paper/1701.02752","citing_paper":"/paper/2608.05582"},"observation_digest":"sha256:3c591a02154f62d3079b89e9291148908e4e4ba60806b002ad955a78b93b0ac1","observation_id":"18f01174-ae34-4000-8595-64b4dfa10700","resolution":{"observed_at":"2026-08-08T10:10:48.310511Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0808.4136","last_updated":"2009-03-06T15:12:11Z","snapshot_observed_at":"2026-07-06T01:42:46.952168Z","submitted_at":"2008-08-29T17:31:19Z","title":"Equation-of-State Dependent Features in Shock-Oscillation Modulated Neutrino and Gravitational-Wave Signals from Supernovae","version":2},"cited_work":{"arxiv_id":"0808.4136","doi":null,"metadata_source":"pith","pith_arxiv_id":"0808.4136","snapshot_observed_at":"2026-08-08T10:10:49.616242Z","title":"Equation-of-State Dependent Features in Shock-Oscillation Modulated Neutrino and Gravitational-Wave Signals from Supernovae","venue":"astro-ph","work_id":"395c768a-7692-40e4-a3c1-35e59b4c9a4a","year":2008},"citing_paper":{"arxiv_id":"2608.05582","last_updated":"2026-08-06T04:10:03Z","snapshot_observed_at":"2026-08-09T23:11:06.657264Z","submitted_at":"2026-08-06T04:10:03Z","title":"Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects","version":1},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-08T10:10:48.292375Z"},"links":{"cited_paper":"/paper/0808.4136","citing_paper":"/paper/2608.05582"},"observation_digest":"sha256:30e914e6d22b5819937833a8b087b67908490e5f4fa9c1ed46cbd1005d12a9d5","observation_id":"3db554e0-5c14-40b9-9fed-bbc98e13f76b","resolution":{"observed_at":"2026-08-08T10:10:49.621720Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1206.6101","last_updated":"2012-12-12T00:10:07Z","snapshot_observed_at":"2026-07-06T02:50:42.941440Z","submitted_at":"2012-06-26T20:00:00Z","title":"On the Importance of the Equation of State for the Neutrino-Driven Supernova Explosion Mechanism","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1206.6101","snapshot_observed_at":"2026-08-08T10:10:48.296909Z","title":null,"venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2608.05582","last_updated":"2026-08-06T04:10:03Z","snapshot_observed_at":"2026-08-09T23:11:06.657264Z","submitted_at":"2026-08-06T04:10:03Z","title":"Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects","version":1},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-08T10:10:48.296909Z"},"links":{"cited_paper":"/paper/1206.6101","citing_paper":"/paper/2608.05582"},"observation_digest":"sha256:3cb9dcde9f924a123f78032fd19b0ac8be6f4000879e80038ea2a2dc72d62b30","observation_id":"a5359e8d-c1be-4711-8f2e-daea73d0e775","resolution":{"observed_at":"2026-08-08T10:10:48.296909Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1206.4724","last_updated":"2012-06-20T21:18:12Z","snapshot_observed_at":"2026-07-06T02:50:20.241587Z","submitted_at":"2012-06-20T21:18:12Z","title":"The Dependence of the Neutrino Mechanism of Core-Collapse Supernovae on the Equation of State","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1206.4724","snapshot_observed_at":"2026-08-08T10:10:48.301302Z","title":null,"venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2608.05582","last_updated":"2026-08-06T04:10:03Z","snapshot_observed_at":"2026-08-09T23:11:06.657264Z","submitted_at":"2026-08-06T04:10:03Z","title":"Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects","version":1},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-08T10:10:48.301302Z"},"links":{"cited_paper":"/paper/1206.4724","citing_paper":"/paper/2608.05582"},"observation_digest":"sha256:ddf8e154a95a72727d4d63c4ebd2e3e77562ffc85f06392d69e827bc73a08534","observation_id":"3ece6e91-ba00-4560-9107-45b8b32fe479","resolution":{"observed_at":"2026-08-08T10:10:48.301302Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1307.6190","last_updated":"2014-02-05T12:50:56Z","snapshot_observed_at":"2026-07-06T03:19:00.026073Z","submitted_at":"2013-07-23T18:55:29Z","title":"Symmetry energy impact in simulations of core-collapse supernovae","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1307.6190","snapshot_observed_at":"2026-08-08T10:10:48.305670Z","title":"Fischer, M","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2608.05582","last_updated":"2026-08-06T04:10:03Z","snapshot_observed_at":"2026-08-09T23:11:06.657264Z","submitted_at":"2026-08-06T04:10:03Z","title":"Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects","version":1},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-08T10:10:48.305670Z"},"links":{"cited_paper":"/paper/1307.6190","citing_paper":"/paper/2608.05582"},"observation_digest":"sha256:695b8b61e63bd7f8979ff623e2044b71852213e18273a63d0e765bba50b01b16","observation_id":"66bd71d1-0e95-4d7f-9a35-8f7cd66736b4","resolution":{"observed_at":"2026-08-08T10:10:48.305670Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2106.09734","last_updated":"2021-06-17T18:00:03Z","snapshot_observed_at":"2026-08-04T11:56:40.981387Z","submitted_at":"2021-06-17T18:00:03Z","title":"Equation of State Dependence of Gravitational Waves in Core-Collapse Supernovae","version":1},"cited_work":{"arxiv_id":"2106.09734","doi":null,"metadata_source":"pith","pith_arxiv_id":"2106.09734","snapshot_observed_at":"2026-08-08T10:10:49.458201Z","title":"Equation of State Dependence of Gravitational Waves in Core-Collapse Supernovae","venue":"astro-ph.HE","work_id":"f759fb3d-b8ee-4014-a28b-a7fdcd80fab4","year":2021},"citing_paper":{"arxiv_id":"2608.05582","last_updated":"2026-08-06T04:10:03Z","snapshot_observed_at":"2026-08-09T23:11:06.657264Z","submitted_at":"2026-08-06T04:10:03Z","title":"Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects","version":1},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-08T10:10:48.337836Z"},"links":{"cited_paper":"/paper/2106.09734","citing_paper":"/paper/2608.05582"},"observation_digest":"sha256:4ca68975118d676b6d4fb00a051f888ca8907618d02238789f4677f0e84764ab","observation_id":"862588a6-6815-4b12-a607-66ade24a8f91","resolution":{"observed_at":"2026-08-08T10:10:49.463662Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1611.05859","last_updated":"2018-01-26T20:32:55Z","snapshot_observed_at":"2026-08-07T15:32:07.324339Z","submitted_at":"2016-11-17T20:59:59Z","title":"Crucial Physical Dependencies of the Core-Collapse Supernova Mechanism","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1611.05859","snapshot_observed_at":"2026-08-08T10:10:48.315594Z","title":"Burrows, D","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2608.05582","last_updated":"2026-08-06T04:10:03Z","snapshot_observed_at":"2026-08-09T23:11:06.657264Z","submitted_at":"2026-08-06T04:10:03Z","title":"Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects","version":1},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-08T10:10:48.315594Z"},"links":{"cited_paper":"/paper/1611.05859","citing_paper":"/paper/2608.05582"},"observation_digest":"sha256:322efef8d0c09a9010d0a51714732d69f99d37de7eb2e95fb16f313b0a7ede54","observation_id":"5debfae9-d802-49d8-94ea-bb2dd31440e8","resolution":{"observed_at":"2026-08-08T10:10:48.315594Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1702.01752","last_updated":"2018-02-12T23:32:25Z","snapshot_observed_at":"2026-07-06T05:29:01.228177Z","submitted_at":"2017-02-06T19:00:01Z","title":"Simulations of core-collapse supernovae in spatial axisymmetry with full Boltzmann neutrino transport","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1702.01752","snapshot_observed_at":"2026-08-08T10:10:48.321873Z","title":"Nagakura, W","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2608.05582","last_updated":"2026-08-06T04:10:03Z","snapshot_observed_at":"2026-08-09T23:11:06.657264Z","submitted_at":"2026-08-06T04:10:03Z","title":"Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects","version":1},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-08-08T10:10:48.321873Z"},"links":{"cited_paper":"/paper/1702.01752","citing_paper":"/paper/2608.05582"},"observation_digest":"sha256:22a39be8710a30d88409133f36745ca091c9a44c11a8afc591b66935b6ee4fe2","observation_id":"544aa46f-8789-434d-9059-e4fed400a0bf","resolution":{"observed_at":"2026-08-08T10:10:48.321873Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1810.12316","last_updated":"2019-03-07T02:41:33Z","snapshot_observed_at":"2026-07-06T07:11:16.512397Z","submitted_at":"2018-10-29T18:00:16Z","title":"On the Neutrino Distributions in Phase Space for the Rotating Core-collapse Supernova Simulated with a Boltzmann-neutrino-radiation-hydrodynamics Code","version":2},"cited_work":{"arxiv_id":"1810.12316","doi":null,"metadata_source":"pith","pith_arxiv_id":"1810.12316","snapshot_observed_at":"2026-08-08T10:10:49.496910Z","title":"On the Neutrino Distributions in Phase Space for the Rotating Core-collapse Supernova Simulated with a Boltzmann-neutrino-radiation-hydrodynamics Code","venue":"astro-ph.HE","work_id":"63264a69-f90b-45f7-9a75-67070bf198ad","year":2018},"citing_paper":{"arxiv_id":"2608.05582","last_updated":"2026-08-06T04:10:03Z","snapshot_observed_at":"2026-08-09T23:11:06.657264Z","submitted_at":"2026-08-06T04:10:03Z","title":"Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects","version":1},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-08-08T10:10:48.327321Z"},"links":{"cited_paper":"/paper/1810.12316","citing_paper":"/paper/2608.05582"},"observation_digest":"sha256:6b1760859792720c970546184596aec4d781531d9051d431047034a3fb6679c5","observation_id":"1b6b3ebb-2507-4598-95e0-904e9c720a65","resolution":{"observed_at":"2026-08-08T10:10:49.502056Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1906.02009","last_updated":"2019-06-05T13:02:15Z","snapshot_observed_at":"2026-08-08T14:39:19.032576Z","submitted_at":"2019-06-05T13:02:15Z","title":"Equation of state effects in the core collapse of a $20$-$M_\\odot$ star","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1906.02009","snapshot_observed_at":"2026-08-08T10:10:48.332913Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2608.05582","last_updated":"2026-08-06T04:10:03Z","snapshot_observed_at":"2026-08-09T23:11:06.657264Z","submitted_at":"2026-08-06T04:10:03Z","title":"Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects","version":1},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-08-08T10:10:48.332913Z"},"links":{"cited_paper":"/paper/1906.02009","citing_paper":"/paper/2608.05582"},"observation_digest":"sha256:551ba60e6ec2282a0eadcbf006c488440c8bb25b6005366342ec1693a2b19650","observation_id":"da0cd4d4-93eb-4e4a-a9a2-62fbf1dce8ff","resolution":{"observed_at":"2026-08-08T10:10:48.332913Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0706.3762","last_updated":"2007-06-26T06:58:20Z","snapshot_observed_at":"2026-07-06T01:28:43.804135Z","submitted_at":"2007-06-26T06:58:20Z","title":"Dynamics and neutrino signal of black hole formation in non-rotating failed supernovae. I. EOS dependence","version":1},"cited_work":{"arxiv_id":"0706.3762","doi":null,"metadata_source":"pith","pith_arxiv_id":"0706.3762","snapshot_observed_at":"2026-08-08T10:10:49.353439Z","title":"Dynamics and neutrino signal of black hole formation in non-rotating failed supernovae. I. EOS dependence","venue":"astro-ph","work_id":"081656b2-1e41-43f2-88f9-b8b51e9e2120","year":2007},"citing_paper":{"arxiv_id":"2608.05582","last_updated":"2026-08-06T04:10:03Z","snapshot_observed_at":"2026-08-09T23:11:06.657264Z","submitted_at":"2026-08-06T04:10:03Z","title":"Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects","version":1},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-08-08T10:10:48.362562Z"},"links":{"cited_paper":"/paper/0706.3762","citing_paper":"/paper/2608.05582"},"observation_digest":"sha256:be7e2c9c24029f69cde662329cb3ba3025744a0c9429f7ccb08fdec4444b364e","observation_id":"81991be8-58ab-47f8-b2d0-e6fa9bae2500","resolution":{"observed_at":"2026-08-08T10:10:49.359729Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2110.05544","last_updated":"2022-01-17T09:02:47Z","snapshot_observed_at":"2026-08-02T20:53:12.783503Z","submitted_at":"2021-10-11T18:29:53Z","title":"Effect of the Nuclear Equation of State on Relativistic-Turbulence Induced Core-Collapse Supernovae","version":2},"cited_work":{"arxiv_id":"2110.05544","doi":null,"metadata_source":"pith","pith_arxiv_id":"2110.05544","snapshot_observed_at":"2026-08-08T10:10:49.435341Z","title":"Effect of the Nuclear Equation of State on Relativistic-Turbulence Induced Core-Collapse Supernovae","venue":"astro-ph.HE","work_id":"76e2f5ba-b409-47f9-b3fd-16dd3b3120ae","year":2021},"citing_paper":{"arxiv_id":"2608.05582","last_updated":"2026-08-06T04:10:03Z","snapshot_observed_at":"2026-08-09T23:11:06.657264Z","submitted_at":"2026-08-06T04:10:03Z","title":"Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects","version":1},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-08-08T10:10:48.342848Z"},"links":{"cited_paper":"/paper/2110.05544","citing_paper":"/paper/2608.05582"},"observation_digest":"sha256:32c35b82d474d79e06236950966ba19a515e1caee5f4398b71279bfcc92da549","observation_id":"a4d82a53-0c11-4efd-9d51-c765a53f33fa","resolution":{"observed_at":"2026-08-08T10:10:49.440379Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2510.20076","last_updated":"2026-06-22T02:19:09Z","snapshot_observed_at":"2026-08-08T14:40:22.642242Z","submitted_at":"2025-10-22T23:21:03Z","title":"Impact of the nuclear equation of state on the explodability of massive stars","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2510.20076","snapshot_observed_at":"2026-08-08T10:10:48.347874Z","title":"Powell and B","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2608.05582","last_updated":"2026-08-06T04:10:03Z","snapshot_observed_at":"2026-08-09T23:11:06.657264Z","submitted_at":"2026-08-06T04:10:03Z","title":"Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects","version":1},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-08-08T10:10:48.347874Z"},"links":{"cited_paper":"/paper/2510.20076","citing_paper":"/paper/2608.05582"},"observation_digest":"sha256:665430ef6d4de452f38621c00d9271761106695f976cb96d8f0a26c76866b35b","observation_id":"bcd3eeb4-edb0-462e-84f9-39e8a6dc6c50","resolution":{"observed_at":"2026-08-08T10:10:48.347874Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2602.09025","last_updated":"2026-04-19T19:44:04Z","snapshot_observed_at":"2026-07-06T22:45:11.110274Z","submitted_at":"2026-02-09T18:59:59Z","title":"An Exploration of the Equation of State Dependence of Core-Collapse Supernova Explosion Outcomes and Signatures","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2602.09025","snapshot_observed_at":"2026-08-08T10:10:48.352788Z","title":"Rusakov, A","venue":null,"work_id":null,"year":2026},"citing_paper":{"arxiv_id":"2608.05582","last_updated":"2026-08-06T04:10:03Z","snapshot_observed_at":"2026-08-09T23:11:06.657264Z","submitted_at":"2026-08-06T04:10:03Z","title":"Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects","version":1},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-08-08T10:10:48.352788Z"},"links":{"cited_paper":"/paper/2602.09025","citing_paper":"/paper/2608.05582"},"observation_digest":"sha256:da54ce161038f28eeddcf68643be9d59e861b050b8b196a313dac87a4e56a72d","observation_id":"183113f8-8959-4568-9d2b-4e62186362b7","resolution":{"observed_at":"2026-08-08T10:10:48.352788Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0608509","last_updated":"2006-08-24T08:11:52Z","snapshot_observed_at":"2026-08-02T19:12:36.275175Z","submitted_at":"2006-08-24T08:11:52Z","title":"Neutrino signals from the formation of black hole: a probe of equation of state of dense matter","version":1},"cited_work":{"arxiv_id":"astro-ph/0608509","doi":null,"metadata_source":"pith","pith_arxiv_id":"astro-ph/0608509","snapshot_observed_at":"2026-08-08T10:10:49.378040Z","title":"Neutrino signals from the formation of black hole: a probe of equation of state of dense matter","venue":"astro-ph","work_id":"8fcbf6cd-68c0-41ff-888b-2d25f8987937","year":2006},"citing_paper":{"arxiv_id":"2608.05582","last_updated":"2026-08-06T04:10:03Z","snapshot_observed_at":"2026-08-09T23:11:06.657264Z","submitted_at":"2026-08-06T04:10:03Z","title":"Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects","version":1},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-08-08T10:10:48.357788Z"},"links":{"cited_paper":"/paper/astro-ph/0608509","citing_paper":"/paper/2608.05582"},"observation_digest":"sha256:f2e10b0c6330d24d4a385544a5fe81035d41a513fc025627be3f38aee1bac826","observation_id":"22b08f20-900a-41d9-8ae8-b258d011b9d0","resolution":{"observed_at":"2026-08-08T10:10:49.383558Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2411.11969","last_updated":"2024-11-18T19:00:33Z","snapshot_observed_at":"2026-07-06T19:52:11.774784Z","submitted_at":"2024-11-18T19:00:33Z","title":"Black Hole Supernovae, their Equation of State Dependence and Ejecta Composition","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2411.11969","snapshot_observed_at":"2026-08-08T10:10:48.386268Z","title":"Eggenberger Andersen, E","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2608.05582","last_updated":"2026-08-06T04:10:03Z","snapshot_observed_at":"2026-08-09T23:11:06.657264Z","submitted_at":"2026-08-06T04:10:03Z","title":"Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects","version":1},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-08-08T10:10:48.386268Z"},"links":{"cited_paper":"/paper/2411.11969","citing_paper":"/paper/2608.05582"},"observation_digest":"sha256:9197cb9980ff1bae4d9230505fb0c1cafeabe527d36290c789420783d5d90088","observation_id":"8dd864b9-1cda-4771-ab62-6cd3a84708b0","resolution":{"observed_at":"2026-08-08T10:10:48.386268Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1010.5550","last_updated":"2011-03-10T19:59:16Z","snapshot_observed_at":"2026-07-06T02:18:15.737750Z","submitted_at":"2010-10-27T02:07:41Z","title":"Black Hole Formation in Failing Core-Collapse Supernovae","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1010.5550","snapshot_observed_at":"2026-08-08T10:10:48.367527Z","title":"O’Connor and C","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2608.05582","last_updated":"2026-08-06T04:10:03Z","snapshot_observed_at":"2026-08-09T23:11:06.657264Z","submitted_at":"2026-08-06T04:10:03Z","title":"Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects","version":1},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-08-08T10:10:48.367527Z"},"links":{"cited_paper":"/paper/1010.5550","citing_paper":"/paper/2608.05582"},"observation_digest":"sha256:d2dd921b9a770f3bc01dc1bfaabe577a967a6f424b8099f5e3c8097fec7408af","observation_id":"c59e2286-b317-4dd5-afdf-dfd9565d62e8","resolution":{"observed_at":"2026-08-08T10:10:48.367527Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1508.01854","last_updated":"2015-08-08T05:14:09Z","snapshot_observed_at":"2026-07-06T04:26:08.135890Z","submitted_at":"2015-08-08T05:14:09Z","title":"A Comparative study of hyperon equations of state in supernova simulations","version":1},"cited_work":{"arxiv_id":"1508.01854","doi":null,"metadata_source":"pith","pith_arxiv_id":"1508.01854","snapshot_observed_at":"2026-08-08T10:10:49.311819Z","title":"A Comparative study of hyperon equations of state in supernova simulations","venue":"astro-ph.HE","work_id":"b05ba5f1-ae01-4c8a-b9a4-44d0f71b2bf4","year":2015},"citing_paper":{"arxiv_id":"2608.05582","last_updated":"2026-08-06T04:10:03Z","snapshot_observed_at":"2026-08-09T23:11:06.657264Z","submitted_at":"2026-08-06T04:10:03Z","title":"Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects","version":1},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-08-08T10:10:48.372761Z"},"links":{"cited_paper":"/paper/1508.01854","citing_paper":"/paper/2608.05582"},"observation_digest":"sha256:0a80453401686041ae22d45a228f46a297f2a4669acac2b672a8b876439c7501","observation_id":"86e850bd-0c03-4baf-864b-2644572152ce","resolution":{"observed_at":"2026-08-08T10:10:49.317228Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1710.01690","last_updated":"2018-04-09T15:41:19Z","snapshot_observed_at":"2026-08-10T09:07:07.312984Z","submitted_at":"2017-10-04T16:47:51Z","title":"Equation of State Dependent Dynamics and Multimessenger Signals from Stellar-mass Black Hole Formation","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1710.01690","snapshot_observed_at":"2026-08-08T10:10:48.377694Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2608.05582","last_updated":"2026-08-06T04:10:03Z","snapshot_observed_at":"2026-08-09T23:11:06.657264Z","submitted_at":"2026-08-06T04:10:03Z","title":"Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects","version":1},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-08-08T10:10:48.377694Z"},"links":{"cited_paper":"/paper/1710.01690","citing_paper":"/paper/2608.05582"},"observation_digest":"sha256:806f133d213867e763730d9cd4f2bcf3834ffbe939787b37a1c4366ebebd20c7","observation_id":"70982369-a516-4646-8b85-5d5fa6737d41","resolution":{"observed_at":"2026-08-08T10:10:48.377694Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2001.10434","last_updated":"2020-01-28T16:09:54Z","snapshot_observed_at":"2026-08-09T07:05:43.510781Z","submitted_at":"2020-01-28T16:09:54Z","title":"Equation of State and Progenitor Dependence of Stellar-Mass Black-Hole Formation","version":1},"cited_work":{"arxiv_id":"2001.10434","doi":null,"metadata_source":"pith","pith_arxiv_id":"2001.10434","snapshot_observed_at":"2026-08-08T10:10:49.271696Z","title":"Equation of State and Progenitor Dependence of Stellar-Mass Black-Hole Formation","venue":"astro-ph.HE","work_id":"1355f5ff-be7f-4054-afd2-3b165a744e09","year":2020},"citing_paper":{"arxiv_id":"2608.05582","last_updated":"2026-08-06T04:10:03Z","snapshot_observed_at":"2026-08-09T23:11:06.657264Z","submitted_at":"2026-08-06T04:10:03Z","title":"Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects","version":1},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-08-08T10:10:48.381836Z"},"links":{"cited_paper":"/paper/2001.10434","citing_paper":"/paper/2608.05582"},"observation_digest":"sha256:19e1a37b8de26e1e3eea88bb94e769a1e8d3c72ba6a79e2ebb3f715ed0f7f43c","observation_id":"80035027-3353-4264-bc41-f19f52a78451","resolution":{"observed_at":"2026-08-08T10:10:49.277902Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+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":"2026-08-08T10:10:50.485294Z","title":"Suzuki, inPhysics and Astrophysics of Neutrinos, edited by M","venue":null,"work_id":"4b100918-4151-4dda-b4ff-974c55db382c","year":1994},"citing_paper":{"arxiv_id":"2608.05582","last_updated":"2026-08-06T04:10:03Z","snapshot_observed_at":"2026-08-09T23:11:06.657264Z","submitted_at":"2026-08-06T04:10:03Z","title":"Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects","version":1},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-08-08T10:10:48.409188Z"},"links":{"citing_paper":"/paper/2608.05582"},"observation_digest":"sha256:7cbee5ccf16f03a57731cf36e8a56d228ca44a4d0b44c4c59cb00f400d3972e4","observation_id":"0f78a5ee-1f4e-474e-9f84-bb0b752751b8","resolution":{"observed_at":"2026-08-08T10:10:50.490199Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+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":"2026-08-08T10:10:50.518103Z","title":"Yasin, S","venue":null,"work_id":"2a5c9d22-7546-4c78-a6b2-fffcdd30e4a2","year":2020},"citing_paper":{"arxiv_id":"2608.05582","last_updated":"2026-08-06T04:10:03Z","snapshot_observed_at":"2026-08-09T23:11:06.657264Z","submitted_at":"2026-08-06T04:10:03Z","title":"Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects","version":1},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-08-08T10:10:48.390471Z"},"links":{"citing_paper":"/paper/2608.05582"},"observation_digest":"sha256:3ca1fcccbc6331632c25643394cdf12807d29054d8bcb3e5d81ad8caf9a6bb4d","observation_id":"714a6978-9349-4ec1-b31e-1f8bd8a4d395","resolution":{"observed_at":"2026-08-08T10:10:50.524049Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1901.09652","last_updated":"2019-01-28T14:03:26Z","snapshot_observed_at":"2026-08-09T01:22:27.638452Z","submitted_at":"2019-01-28T14:03:26Z","title":"The APR equation of state for simulations of supernovae, neutron stars and binary mergers","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1901.09652","snapshot_observed_at":"2026-08-08T10:10:48.394357Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2608.05582","last_updated":"2026-08-06T04:10:03Z","snapshot_observed_at":"2026-08-09T23:11:06.657264Z","submitted_at":"2026-08-06T04:10:03Z","title":"Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects","version":1},"reference_index":54,"source":"pdf_text","source_observed_at":"2026-08-08T10:10:48.394357Z"},"links":{"cited_paper":"/paper/1901.09652","citing_paper":"/paper/2608.05582"},"observation_digest":"sha256:804200d8efddad1c084e0ad1197494826008c63d2dcecee2b39b541b55ae6404","observation_id":"67468d6e-2422-4d0c-94b3-4708d0dce7b4","resolution":{"observed_at":"2026-08-08T10:10:48.394357Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2503.13963","last_updated":"2025-03-18T06:56:17Z","snapshot_observed_at":"2026-08-07T16:55:45.422480Z","submitted_at":"2025-03-18T06:56:17Z","title":"Influence of the effective mass on the properties of nuclear matter at finite density and temperature","version":1},"cited_work":{"arxiv_id":"2503.13963","doi":null,"metadata_source":"pith","pith_arxiv_id":"2503.13963","snapshot_observed_at":"2026-08-08T10:10:49.215265Z","title":"Influence of the effective mass on the properties of nuclear matter at finite density and temperature","venue":"nucl-th","work_id":"079f153d-c7d8-4083-a5bd-f28af5f1ce0b","year":2025},"citing_paper":{"arxiv_id":"2608.05582","last_updated":"2026-08-06T04:10:03Z","snapshot_observed_at":"2026-08-09T23:11:06.657264Z","submitted_at":"2026-08-06T04:10:03Z","title":"Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects","version":1},"reference_index":55,"source":"pdf_text","source_observed_at":"2026-08-08T10:10:48.399200Z"},"links":{"cited_paper":"/paper/2503.13963","citing_paper":"/paper/2608.05582"},"observation_digest":"sha256:f1fe2b6086cfaba4b463a00640046eed5dd5d35d0737086e7d201355139f244e","observation_id":"e8171e5f-39e4-4cb3-a375-cf5935379b9c","resolution":{"observed_at":"2026-08-08T10:10:49.220576Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+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":"2026-08-08T10:10:50.500919Z","title":"Burrows and J","venue":null,"work_id":"3b5a0094-9c72-4247-817d-5cdb3a7bcc70","year":1986},"citing_paper":{"arxiv_id":"2608.05582","last_updated":"2026-08-06T04:10:03Z","snapshot_observed_at":"2026-08-09T23:11:06.657264Z","submitted_at":"2026-08-06T04:10:03Z","title":"Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects","version":1},"reference_index":56,"source":"pdf_text","source_observed_at":"2026-08-08T10:10:48.404240Z"},"links":{"citing_paper":"/paper/2608.05582"},"observation_digest":"sha256:aa6d21211b005c766875dad849b4126ddf6f754ba21b5a24d349cf362573ff39","observation_id":"388ca1a0-dd90-4225-923e-32f6372e1730","resolution":{"observed_at":"2026-08-08T10:10:50.505621Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1905.00014","last_updated":"2019-04-30T18:00:00Z","snapshot_observed_at":"2026-07-06T07:49:36.138512Z","submitted_at":"2019-04-30T18:00:00Z","title":"Cooling timescale for protoneutron stars and properties of nuclear matter: Effective mass and symmetry energy at high densities","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1905.00014","snapshot_observed_at":"2026-08-08T10:10:48.432957Z","title":"Nakazato and H","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2608.05582","last_updated":"2026-08-06T04:10:03Z","snapshot_observed_at":"2026-08-09T23:11:06.657264Z","submitted_at":"2026-08-06T04:10:03Z","title":"Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects","version":1},"reference_index":57,"source":"pdf_text","source_observed_at":"2026-08-08T10:10:48.432957Z"},"links":{"cited_paper":"/paper/1905.00014","citing_paper":"/paper/2608.05582"},"observation_digest":"sha256:4122bf8fca73469619395fad267861b72d2fb1925a6dc82c7bc687e4b9b705b6","observation_id":"859fb60d-e572-4906-a0a2-da85b3a3defa","resolution":{"observed_at":"2026-08-08T10:10:48.432957Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9506024","last_updated":"1995-06-07T00:43:29Z","snapshot_observed_at":"2026-07-07T01:11:17.861816Z","submitted_at":"1995-06-05T14:12:47Z","title":"Influence of the symmetry energy on the birth of neutron stars and supernova neutrinos","version":2},"cited_work":{"arxiv_id":"astro-ph/9506024","doi":null,"metadata_source":"pith","pith_arxiv_id":"astro-ph/9506024","snapshot_observed_at":"2026-08-08T10:10:49.190753Z","title":"Influence of the symmetry energy on the birth of neutron stars and supernova neutrinos","venue":"astro-ph","work_id":"27ee6de8-99bf-495e-b15d-522550c192ee","year":1995},"citing_paper":{"arxiv_id":"2608.05582","last_updated":"2026-08-06T04:10:03Z","snapshot_observed_at":"2026-08-09T23:11:06.657264Z","submitted_at":"2026-08-06T04:10:03Z","title":"Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects","version":1},"reference_index":58,"source":"pdf_text","source_observed_at":"2026-08-08T10:10:48.413664Z"},"links":{"cited_paper":"/paper/astro-ph/9506024","citing_paper":"/paper/2608.05582"},"observation_digest":"sha256:b2717a642c9ed759d1c4b9d9c3f5faab662efc0e34be2b43635045c623a7ae8a","observation_id":"4a3d64b1-4fac-4af3-813c-752a080443d5","resolution":{"observed_at":"2026-08-08T10:10:49.196300Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9807040","last_updated":"1998-07-03T16:37:44Z","snapshot_observed_at":"2026-07-07T01:21:25.090997Z","submitted_at":"1998-07-03T16:37:44Z","title":"Evolution of Protoneutron Stars","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9807040","snapshot_observed_at":"2026-08-08T10:10:48.418288Z","title":null,"venue":null,"work_id":null,"year":1999},"citing_paper":{"arxiv_id":"2608.05582","last_updated":"2026-08-06T04:10:03Z","snapshot_observed_at":"2026-08-09T23:11:06.657264Z","submitted_at":"2026-08-06T04:10:03Z","title":"Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects","version":1},"reference_index":59,"source":"pdf_text","source_observed_at":"2026-08-08T10:10:48.418288Z"},"links":{"cited_paper":"/paper/astro-ph/9807040","citing_paper":"/paper/2608.05582"},"observation_digest":"sha256:afc960a069cb8ba3d83f5f2959d4b6c92616665b45884d01c601fc56daf8dbdf","observation_id":"fdf88342-7a89-45a1-a412-cb85fd52011a","resolution":{"observed_at":"2026-08-08T10:10:48.418288Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1112.0335","last_updated":"2011-12-01T21:40:23Z","snapshot_observed_at":"2026-07-06T02:38:39.668767Z","submitted_at":"2011-12-01T21:40:23Z","title":"Proto-Neutron Star Cooling with Convection: The Effect of the Symmetry Energy","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1112.0335","snapshot_observed_at":"2026-08-08T10:10:48.423272Z","title":null,"venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2608.05582","last_updated":"2026-08-06T04:10:03Z","snapshot_observed_at":"2026-08-09T23:11:06.657264Z","submitted_at":"2026-08-06T04:10:03Z","title":"Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects","version":1},"reference_index":60,"source":"pdf_text","source_observed_at":"2026-08-08T10:10:48.423272Z"},"links":{"cited_paper":"/paper/1112.0335","citing_paper":"/paper/2608.05582"},"observation_digest":"sha256:c4bfae07ac410c3908587222f6ad16c3c93a6c25c8fe003f2ede5e8a7c697f06","observation_id":"ebff9801-c6aa-4aac-823f-713c0032a254","resolution":{"observed_at":"2026-08-08T10:10:48.423272Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1210.6841","last_updated":"2013-01-09T12:05:03Z","snapshot_observed_at":"2026-07-06T02:58:27.249808Z","submitted_at":"2012-10-25T13:47:26Z","title":"Supernova Neutrino Light Curves and Spectra for Various Progenitor Stars: From Core Collapse to Proto-neutron Star Cooling","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1210.6841","snapshot_observed_at":"2026-08-08T10:10:48.428124Z","title":"Nakazato, K","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2608.05582","last_updated":"2026-08-06T04:10:03Z","snapshot_observed_at":"2026-08-09T23:11:06.657264Z","submitted_at":"2026-08-06T04:10:03Z","title":"Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects","version":1},"reference_index":61,"source":"pdf_text","source_observed_at":"2026-08-08T10:10:48.428124Z"},"links":{"cited_paper":"/paper/1210.6841","citing_paper":"/paper/2608.05582"},"observation_digest":"sha256:3407387631dcd4f49f5cb57f6303ef0244ff2195c639762beb58c43da890e065","observation_id":"c41d4d0a-8fe2-407e-a926-8a7147727498","resolution":{"observed_at":"2026-08-08T10:10:48.428124Z","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":"th/9806095","doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-08T10:10:48.931418Z","title":null,"venue":null,"work_id":"99a220f6-1038-4383-a0b9-3ae28e0b68a8","year":1998},"citing_paper":{"arxiv_id":"2608.05582","last_updated":"2026-08-06T04:10:03Z","snapshot_observed_at":"2026-08-09T23:11:06.657264Z","submitted_at":"2026-08-06T04:10:03Z","title":"Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects","version":1},"reference_index":62,"source":"pdf_text","source_observed_at":"2026-08-08T10:10:48.459870Z"},"links":{"citing_paper":"/paper/2608.05582"},"observation_digest":"sha256:abded4b6323d174dee515410a5678c46eeb2e836480cc662be893ab267fcef74","observation_id":"1370749a-7e78-4e45-b66d-c66179833d06","resolution":{"observed_at":"2026-08-08T10:10:48.938612Z","resolver_source":"raw_fallback","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2407.18739","last_updated":"2025-02-14T13:46:35Z","snapshot_observed_at":"2026-07-06T18:52:25.478047Z","submitted_at":"2024-07-26T13:51:05Z","title":"Influence of effective nucleon mass on equation of state for supernova simulations and neutron stars","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2407.18739","snapshot_observed_at":"2026-08-08T10:10:48.437906Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2608.05582","last_updated":"2026-08-06T04:10:03Z","snapshot_observed_at":"2026-08-09T23:11:06.657264Z","submitted_at":"2026-08-06T04:10:03Z","title":"Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects","version":1},"reference_index":63,"source":"pdf_text","source_observed_at":"2026-08-08T10:10:48.437906Z"},"links":{"cited_paper":"/paper/2407.18739","citing_paper":"/paper/2608.05582"},"observation_digest":"sha256:6344fd2da472c776651551fdfc651e1c83731f697227217cd93b7e1d40a79c05","observation_id":"191392c5-bab0-42f7-9eb7-ee8cbb5288f8","resolution":{"observed_at":"2026-08-08T10:10:48.437906Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2001.10143","last_updated":"2020-01-28T02:16:17Z","snapshot_observed_at":"2026-08-04T23:23:52.874666Z","submitted_at":"2020-01-28T02:16:17Z","title":"Effects of symmetry energy on equation of state for simulations of core-collapse supernovae and neutron-star mergers","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2001.10143","snapshot_observed_at":"2026-08-08T10:10:48.443532Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2608.05582","last_updated":"2026-08-06T04:10:03Z","snapshot_observed_at":"2026-08-09T23:11:06.657264Z","submitted_at":"2026-08-06T04:10:03Z","title":"Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects","version":1},"reference_index":64,"source":"pdf_text","source_observed_at":"2026-08-08T10:10:48.443532Z"},"links":{"cited_paper":"/paper/2001.10143","citing_paper":"/paper/2608.05582"},"observation_digest":"sha256:9a7d6b963907247165058d717997616ab77bab3cc458f04781faaada95091a80","observation_id":"76e79414-a315-489d-911f-217378c6d340","resolution":{"observed_at":"2026-08-08T10:10:48.443532Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1105.1666","last_updated":"2011-12-09T16:20:36Z","snapshot_observed_at":"2026-08-05T13:51:35.023141Z","submitted_at":"2011-05-09T13:23:13Z","title":"Relativistic Equation of State for Core-Collapse Supernova Simulations","version":2},"cited_work":{"arxiv_id":"1105.1666","doi":null,"metadata_source":"pith","pith_arxiv_id":"1105.1666","snapshot_observed_at":"2026-08-08T10:10:49.073331Z","title":"Relativistic Equation of State for Core-Collapse Supernova Simulations","venue":"astro-ph.HE","work_id":"7633428c-e457-49b9-8396-aa87b66f6566","year":2011},"citing_paper":{"arxiv_id":"2608.05582","last_updated":"2026-08-06T04:10:03Z","snapshot_observed_at":"2026-08-09T23:11:06.657264Z","submitted_at":"2026-08-06T04:10:03Z","title":"Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects","version":1},"reference_index":65,"source":"pdf_text","source_observed_at":"2026-08-08T10:10:48.449585Z"},"links":{"cited_paper":"/paper/1105.1666","citing_paper":"/paper/2608.05582"},"observation_digest":"sha256:18e898407b694829810f5e84eecd789538c5ec3a9a72e7ba63baf6073a33cb3c","observation_id":"f461c043-4b02-48c1-9d25-2db0235f25d4","resolution":{"observed_at":"2026-08-08T10:10:49.080174Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+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":"2026-08-08T10:10:50.699523Z","title":"nucleons, electrons, positrons, and photons by adding the lepton and photon contributions to the nuclear contributions for pressure, energy, and entropy","venue":null,"work_id":"677a2462-e49a-4f09-826d-de66775df46a","year":null},"citing_paper":{"arxiv_id":"2608.05582","last_updated":"2026-08-06T04:10:03Z","snapshot_observed_at":"2026-08-09T23:11:06.657264Z","submitted_at":"2026-08-06T04:10:03Z","title":"Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects","version":1},"reference_index":66,"source":"pdf_text","source_observed_at":"2026-08-08T10:10:48.137533Z"},"links":{"citing_paper":"/paper/2608.05582"},"observation_digest":"sha256:6451f37c2425fa3866bc964bbfab1a546a45b7a1bb68701103d552b5278ea575","observation_id":"3f5c7886-6e95-4b00-a7be-325ce4ab3cf5","resolution":{"observed_at":"2026-08-08T10:10:50.705197Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"th/9805035","doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-08T10:10:49.050017Z","title":null,"venue":null,"work_id":"1e3470bf-5625-4822-8def-4be79cf984b2","year":1998},"citing_paper":{"arxiv_id":"2608.05582","last_updated":"2026-08-06T04:10:03Z","snapshot_observed_at":"2026-08-09T23:11:06.657264Z","submitted_at":"2026-08-06T04:10:03Z","title":"Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects","version":1},"reference_index":67,"source":"pdf_text","source_observed_at":"2026-08-08T10:10:48.455190Z"},"links":{"citing_paper":"/paper/2608.05582"},"observation_digest":"sha256:ffd6f13205a369aecf767cc9ef862d7e58eef1bc53bdd6920ef414152ed829ce","observation_id":"ecf67bf3-95ef-4eee-818b-40e131aa6c0b","resolution":{"observed_at":"2026-08-08T10:10:49.057496Z","resolver_source":"raw_fallback","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1908.02928","last_updated":"2019-12-31T02:37:38Z","snapshot_observed_at":"2026-07-06T08:13:06.709908Z","submitted_at":"2019-08-08T04:30:06Z","title":"Influence of density dependence of symmetry energy in hot and dense matter for supernova simulations","version":2},"cited_work":{"arxiv_id":"1908.02928","doi":null,"metadata_source":"pith","pith_arxiv_id":"1908.02928","snapshot_observed_at":"2026-08-08T10:10:48.701909Z","title":"Influence of density dependence of symmetry energy in hot and dense matter for supernova simulations","venue":"astro-ph.HE","work_id":"58176073-99d3-4880-a699-996f920757fe","year":2019},"citing_paper":{"arxiv_id":"2608.05582","last_updated":"2026-08-06T04:10:03Z","snapshot_observed_at":"2026-08-09T23:11:06.657264Z","submitted_at":"2026-08-06T04:10:03Z","title":"Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects","version":1},"reference_index":68,"source":"pdf_text","source_observed_at":"2026-08-08T10:10:48.464411Z"},"links":{"cited_paper":"/paper/1908.02928","citing_paper":"/paper/2608.05582"},"observation_digest":"sha256:13ad4e37db709427d6f7e1d091b9c88acc9b25952c87a28c33e0ff3ab6a9da3d","observation_id":"c30b2efd-e21a-4817-935c-db35dc9c83c5","resolution":{"observed_at":"2026-08-08T10:10:48.707064Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+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":"2026-08-08T10:10:50.469768Z","title":"Sugahara and H","venue":null,"work_id":"25f429a4-d2df-4be0-a614-b3edf646f632","year":1994},"citing_paper":{"arxiv_id":"2608.05582","last_updated":"2026-08-06T04:10:03Z","snapshot_observed_at":"2026-08-09T23:11:06.657264Z","submitted_at":"2026-08-06T04:10:03Z","title":"Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects","version":1},"reference_index":69,"source":"pdf_text","source_observed_at":"2026-08-08T10:10:48.469499Z"},"links":{"citing_paper":"/paper/2608.05582"},"observation_digest":"sha256:c542c4bcd4295bdfe94ca7a63adb93ea5cbf81b7f40c43d040a8516ea02600d1","observation_id":"04a37a0d-1d4e-4349-a589-361c2035998a","resolution":{"observed_at":"2026-08-08T10:10:50.474729Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1805.11581","last_updated":"2018-10-15T17:59:04Z","snapshot_observed_at":"2026-08-07T22:20:24.299342Z","submitted_at":"2018-05-29T16:56:13Z","title":"GW170817: Measurements of Neutron Star Radii and Equation of State","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1805.11581","snapshot_observed_at":"2026-08-08T10:10:48.473746Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2608.05582","last_updated":"2026-08-06T04:10:03Z","snapshot_observed_at":"2026-08-09T23:11:06.657264Z","submitted_at":"2026-08-06T04:10:03Z","title":"Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects","version":1},"reference_index":70,"source":"pdf_text","source_observed_at":"2026-08-08T10:10:48.473746Z"},"links":{"cited_paper":"/paper/1805.11581","citing_paper":"/paper/2608.05582"},"observation_digest":"sha256:fbf1f98c13c04b1f3ef8d18e0f7878c6a9844beb7fbfa24584ad99d43587c69f","observation_id":"a91b7ff0-e7d6-4b2f-976a-2abe64a9a25f","resolution":{"observed_at":"2026-08-08T10:10:48.473746Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1912.05702","last_updated":"2019-12-12T00:04:38Z","snapshot_observed_at":"2026-07-06T08:43:55.093635Z","submitted_at":"2019-12-12T00:04:38Z","title":"A NICER View of PSR J0030+0451: Millisecond Pulsar Parameter Estimation","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1912.05702","snapshot_observed_at":"2026-08-08T10:10:48.478358Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2608.05582","last_updated":"2026-08-06T04:10:03Z","snapshot_observed_at":"2026-08-09T23:11:06.657264Z","submitted_at":"2026-08-06T04:10:03Z","title":"Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects","version":1},"reference_index":71,"source":"pdf_text","source_observed_at":"2026-08-08T10:10:48.478358Z"},"links":{"cited_paper":"/paper/1912.05702","citing_paper":"/paper/2608.05582"},"observation_digest":"sha256:29511f291bc51ca5d04cd143604601132f1f837e2623839adbf7a11856286b99","observation_id":"2d798ac9-d8d6-4736-a088-ddfee0553eb6","resolution":{"observed_at":"2026-08-08T10:10:48.478358Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2105.06980","last_updated":"2021-09-22T12:10:14Z","snapshot_observed_at":"2026-08-09T17:30:18.423607Z","submitted_at":"2021-05-14T17:33:33Z","title":"A NICER View of the Massive Pulsar PSR J0740+6620 Informed by Radio Timing and XMM-Newton Spectroscopy","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2105.06980","snapshot_observed_at":"2026-08-08T10:10:48.482877Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2608.05582","last_updated":"2026-08-06T04:10:03Z","snapshot_observed_at":"2026-08-09T23:11:06.657264Z","submitted_at":"2026-08-06T04:10:03Z","title":"Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects","version":1},"reference_index":72,"source":"pdf_text","source_observed_at":"2026-08-08T10:10:48.482877Z"},"links":{"cited_paper":"/paper/2105.06980","citing_paper":"/paper/2608.05582"},"observation_digest":"sha256:40c0b6af51d41bb8ba4cae0b4bb227d6c19659861a9cd3981ccca6bdd8fe791c","observation_id":"fa7a60b1-add7-4195-a4a5-286193a4ed65","resolution":{"observed_at":"2026-08-08T10:10:48.482877Z","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":"2026-08-08T10:10:50.453924Z","title":null,"venue":null,"work_id":"07f378c5-3d6d-4d03-b271-c8cf323e65e9","year":2002},"citing_paper":{"arxiv_id":"2608.05582","last_updated":"2026-08-06T04:10:03Z","snapshot_observed_at":"2026-08-09T23:11:06.657264Z","submitted_at":"2026-08-06T04:10:03Z","title":"Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects","version":1},"reference_index":73,"source":"pdf_text","source_observed_at":"2026-08-08T10:10:48.487519Z"},"links":{"citing_paper":"/paper/2608.05582"},"observation_digest":"sha256:79ad91e6733355c97ed70e901a7ace06abc8bc0016337a7e52e11e6a8777e2ab","observation_id":"c7596981-f8d3-408d-b2ef-f1f1cd5a2599","resolution":{"observed_at":"2026-08-08T10:10:50.458903Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+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":"2026-08-08T10:10:50.438725Z","title":null,"venue":null,"work_id":"60c08c72-2b0e-4e21-991a-e1795ed2c41e","year":1995},"citing_paper":{"arxiv_id":"2608.05582","last_updated":"2026-08-06T04:10:03Z","snapshot_observed_at":"2026-08-09T23:11:06.657264Z","submitted_at":"2026-08-06T04:10:03Z","title":"Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects","version":1},"reference_index":74,"source":"pdf_text","source_observed_at":"2026-08-08T10:10:48.491510Z"},"links":{"citing_paper":"/paper/2608.05582"},"observation_digest":"sha256:847028a71eb2346a10b88978b9f3c8c045feb5095b65f60d235965bc15e26f33","observation_id":"19b6a12d-28b3-4e76-9d21-80d5007a0422","resolution":{"observed_at":"2026-08-08T10:10:50.443336Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1510.04643","last_updated":"2016-02-13T11:19:23Z","snapshot_observed_at":"2026-08-08T17:52:32.514201Z","submitted_at":"2015-10-15T17:45:30Z","title":"Core-Collapse Supernovae from 9 to 120 Solar Masses Based on Neutrino-powered Explosions","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1510.04643","snapshot_observed_at":"2026-08-08T10:10:48.496159Z","title":"Sukhbold, T","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2608.05582","last_updated":"2026-08-06T04:10:03Z","snapshot_observed_at":"2026-08-09T23:11:06.657264Z","submitted_at":"2026-08-06T04:10:03Z","title":"Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects","version":1},"reference_index":75,"source":"pdf_text","source_observed_at":"2026-08-08T10:10:48.496159Z"},"links":{"cited_paper":"/paper/1510.04643","citing_paper":"/paper/2608.05582"},"observation_digest":"sha256:3dd9745b19989aa2c6817ad8d0fa17118edb213e1ed0c00ea8af7756f9658d25","observation_id":"46c87fa7-d0c6-4d45-b378-1ca46f69e852","resolution":{"observed_at":"2026-08-08T10:10:48.496159Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2209.02474","last_updated":"2022-12-09T07:50:38Z","snapshot_observed_at":"2026-07-06T13:49:19.502478Z","submitted_at":"2022-09-06T13:16:59Z","title":"Effects of nuclear matter and composition in core-collapse supernovae and long-term proto-neutron star cooling","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2209.02474","snapshot_observed_at":"2026-08-08T10:10:48.501202Z","title":"Sumiyoshi, S","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2608.05582","last_updated":"2026-08-06T04:10:03Z","snapshot_observed_at":"2026-08-09T23:11:06.657264Z","submitted_at":"2026-08-06T04:10:03Z","title":"Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects","version":1},"reference_index":76,"source":"pdf_text","source_observed_at":"2026-08-08T10:10:48.501202Z"},"links":{"cited_paper":"/paper/2209.02474","citing_paper":"/paper/2608.05582"},"observation_digest":"sha256:915689789840151a4a9655ac7cb9c3b913bdad349a9ae60e64eb6ce3b93b2291","observation_id":"a12831f2-1989-4d92-aa4c-73b6a4f951d0","resolution":{"observed_at":"2026-08-08T10:10:48.501202Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1710.10441","last_updated":"2018-03-15T04:35:02Z","snapshot_observed_at":"2026-07-06T06:06:33.136974Z","submitted_at":"2017-10-28T10:34:31Z","title":"Heavy Nuclei as Thermal Insulation for Proto-Neutron Stars","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1710.10441","snapshot_observed_at":"2026-08-08T10:10:48.506143Z","title":"Nakazato, H","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2608.05582","last_updated":"2026-08-06T04:10:03Z","snapshot_observed_at":"2026-08-09T23:11:06.657264Z","submitted_at":"2026-08-06T04:10:03Z","title":"Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects","version":1},"reference_index":77,"source":"pdf_text","source_observed_at":"2026-08-08T10:10:48.506143Z"},"links":{"cited_paper":"/paper/1710.10441","citing_paper":"/paper/2608.05582"},"observation_digest":"sha256:09670042cd7a10689ef47eb9385edbf78b502d6cbcaad3c13bf3468629a30e6c","observation_id":"fa019ef9-5427-441d-97d6-647d5ec7a3d0","resolution":{"observed_at":"2026-08-08T10:10:48.506143Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2002.03300","last_updated":"2020-02-09T06:34:27Z","snapshot_observed_at":"2026-08-09T01:54:37.645332Z","submitted_at":"2020-02-09T06:34:27Z","title":"A New Approach to Mass and Radius of Neutron Stars with Supernova Neutrinos","version":1},"cited_work":{"arxiv_id":"2002.03300","doi":null,"metadata_source":"pith","pith_arxiv_id":"2002.03300","snapshot_observed_at":"2026-08-08T10:10:48.582291Z","title":"A New Approach to Mass and Radius of Neutron Stars with Supernova Neutrinos","venue":"astro-ph.HE","work_id":"01223475-01c6-4afb-a1d5-252122031b2f","year":2020},"citing_paper":{"arxiv_id":"2608.05582","last_updated":"2026-08-06T04:10:03Z","snapshot_observed_at":"2026-08-09T23:11:06.657264Z","submitted_at":"2026-08-06T04:10:03Z","title":"Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects","version":1},"reference_index":78,"source":"pdf_text","source_observed_at":"2026-08-08T10:10:48.511234Z"},"links":{"cited_paper":"/paper/2002.03300","citing_paper":"/paper/2608.05582"},"observation_digest":"sha256:cec17ac1e681a9cf6727ea5c00136e89036ac93776be8dd2a4ad946046e914fb","observation_id":"aa45121a-3a4e-4592-b070-caf1aa670735","resolution":{"observed_at":"2026-08-08T10:10:48.587029Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2108.03009","last_updated":"2022-01-31T04:29:57Z","snapshot_observed_at":"2026-08-10T00:28:16.868184Z","submitted_at":"2021-08-06T08:57:25Z","title":"Observing Supernova Neutrino Light Curves with Super-Kamiokande. II. Impact of the Nuclear Equation of State","version":2},"cited_work":{"arxiv_id":"2108.03009","doi":null,"metadata_source":"pith","pith_arxiv_id":"2108.03009","snapshot_observed_at":"2026-08-08T10:10:48.556410Z","title":"Observing Supernova Neutrino Light Curves with Super-Kamiokande. II. Impact of the Nuclear Equation of State","venue":"astro-ph.HE","work_id":"d752e7e1-34df-49ee-8932-92f6c0513994","year":2021},"citing_paper":{"arxiv_id":"2608.05582","last_updated":"2026-08-06T04:10:03Z","snapshot_observed_at":"2026-08-09T23:11:06.657264Z","submitted_at":"2026-08-06T04:10:03Z","title":"Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects","version":1},"reference_index":79,"source":"pdf_text","source_observed_at":"2026-08-08T10:10:48.516830Z"},"links":{"cited_paper":"/paper/2108.03009","citing_paper":"/paper/2608.05582"},"observation_digest":"sha256:1715b58e5f3daf8b7b27631d6289e0ce7778a2214a4dc55bad41ba01a4f8739e","observation_id":"b51bed67-4ab0-4bfe-910a-5bb994b1dbc2","resolution":{"observed_at":"2026-08-08T10:10:48.563861Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}}],"paper":{"arxiv_id":"2608.05582","last_updated":"2026-08-06T04:10:03Z","latest_version":1,"primary_category":"astro-ph.HE","snapshot_observed_at":"2026-08-09T23:11:06.657264Z","submitted_at":"2026-08-06T04:10:03Z","title":"Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects"},"reference_resolution":{"displayed":79,"state_counts":{"malformed_identifier":1,"metadata_mismatch":2,"parse_uncertain":0,"unresolved":46,"verified_exact":18,"verified_fuzzy":12},"total_outbound_references":79},"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":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"thesis":"As of 10 August 2026, this Paper Citation Record lists 79 of 79 outbound references and 0 inbound Pith citation observations for arXiv:2608.05582."}