{"as_of":"2026-08-21T10:50:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:39a265a48840c625e4a53a5f1604fe1070634bf04a03181fc5583f4d438c2b13","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":"2026-08-12T14:48:39.985824Z","state":"measured"},{"denominator":82,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":82,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-21T06:32:19.484+00:00","state":"measured"},{"denominator":3,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":3,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-07T14:28:07.416341Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"arxiv_reference","source_observed_at":"2026-05-22T22:47:13.386560Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2411.14930","last_updated":"2025-04-02T10:48:19Z","snapshot_observed_at":"2026-08-17T16:07:02.156639Z","submitted_at":"2024-11-22T13:39:01Z","title":"Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state","version":2},"cited_work":{"arxiv_id":"2411.14930","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2411.14930","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Kunkel, S","venue":null,"work_id":"d1411cf5-4af7-4ed6-b05f-cef9cd225829","year":null},"citing_paper":{"arxiv_id":"2503.19691","last_updated":"2026-03-04T15:53:07Z","snapshot_observed_at":"2026-07-06T20:58:27.929311Z","submitted_at":"2025-03-25T14:18:06Z","title":"Strongly Interacting Dark Matter admixed Neutron Stars","version":4},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-05-22T22:45:48.648963Z"},"links":{"cited_paper":"/paper/2411.14930","citing_paper":"/paper/2503.19691"},"observation_digest":"sha256:634d3d54050b61bf065adaeea48485ea37f7b0f05e064d7cd617fff546efcc22","observation_id":"f01a286e-88d8-41ea-806f-82b5b98d0a6a","resolution":{"observed_at":"2026-05-22T22:47:13.389016Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2411.14930","last_updated":"2025-04-02T10:48:19Z","snapshot_observed_at":"2026-08-17T16:07:02.156639Z","submitted_at":"2024-11-22T13:39:01Z","title":"Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2411.14930","snapshot_observed_at":"2026-08-07T14:28:07.416341Z","title":"Kunkel, S","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2505.18888","last_updated":"2025-05-24T22:16:54Z","snapshot_observed_at":"2026-08-14T04:25:22.251818Z","submitted_at":"2025-05-24T22:16:54Z","title":"Constraints on maximum neutron star mass from proto-neutron star evolution","version":1},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-07T14:28:07.416341Z"},"links":{"cited_paper":"/paper/2411.14930","citing_paper":"/paper/2505.18888"},"observation_digest":"sha256:03b1405b8d04b8b60288f7d911449326bc84c3e1c8640a80c0aaf2e427be7a9a","observation_id":"b777e559-8910-49d8-ac41-b57bbc7e6727","resolution":{"observed_at":"2026-08-07T14:28:07.416341Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2411.14930","last_updated":"2025-04-02T10:48:19Z","snapshot_observed_at":"2026-08-17T16:07:02.156639Z","submitted_at":"2024-11-22T13:39:01Z","title":"Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2411.14930","snapshot_observed_at":"2026-07-14T04:54:21.953406Z","title":"Kunkel, S","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.11537","last_updated":"2026-07-13T13:19:56Z","snapshot_observed_at":"2026-08-15T18:05:25.066238Z","submitted_at":"2026-07-13T13:19:56Z","title":"The petit four of color-superconducting phases in proto-neutron star evolution","version":1},"reference_index":59,"source":"pdf_text","source_observed_at":"2026-07-14T04:54:21.953406Z"},"links":{"cited_paper":"/paper/2411.14930","citing_paper":"/paper/2607.11537"},"observation_digest":"sha256:fab9a4a7185a03ad0febdcb5079e5cf97c78f0245c39fbfecc92da9a6bcc7d7b","observation_id":"67f55096-33ec-4304-9abf-5827ab0f3811","resolution":{"observed_at":"2026-07-14T04:54:21.953406Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2411.14930/citation-record","integrity":"/paper/2411.14930/integrity","json":"/paper/2411.14930/citation-record.json","paper":"/paper/2411.14930"},"outbound":[{"citation":{"cited_paper":{"arxiv_id":"1803.00549","last_updated":"2018-05-31T11:15:49Z","snapshot_observed_at":"2026-08-17T12:34:09.096492Z","submitted_at":"2018-03-01T18:36:24Z","title":"New constraints on radii and tidal deformabilities of neutron stars from GW170817","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1803.00549","snapshot_observed_at":"2026-08-12T14:48:39.623289Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2411.14930","last_updated":"2025-04-02T10:48:19Z","snapshot_observed_at":"2026-08-17T16:07:02.156639Z","submitted_at":"2024-11-22T13:39:01Z","title":"Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state","version":2},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-12T14:48:39.623289Z"},"links":{"cited_paper":"/paper/1803.00549","citing_paper":"/paper/2411.14930"},"observation_digest":"sha256:87f81e330fea3fa5448e0affaffc3f15bc2693a9554991b2e96c95c5b1337ea5","observation_id":"79ff458c-20cc-4965-a5bb-d9a900eef2e5","resolution":{"observed_at":"2026-08-12T14:48:39.623289Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2402.04172","last_updated":"2025-04-15T09:06:55Z","snapshot_observed_at":"2026-08-16T14:20:55.786725Z","submitted_at":"2024-02-06T17:27:09Z","title":"From existing and new nuclear and astrophysical constraints to stringent limits on the equation of state of neutron-rich dense matter","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2402.04172","snapshot_observed_at":"2026-08-12T14:48:39.628866Z","title":"Koehn et al., (2024), arXiv:2402.04172 [astro-ph.HE]","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2411.14930","last_updated":"2025-04-02T10:48:19Z","snapshot_observed_at":"2026-08-17T16:07:02.156639Z","submitted_at":"2024-11-22T13:39:01Z","title":"Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state","version":2},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-12T14:48:39.628866Z"},"links":{"cited_paper":"/paper/2402.04172","citing_paper":"/paper/2411.14930"},"observation_digest":"sha256:693ead3e5bb3e4a68e2a52135ec8652c2229b38e4312d958af4d0a9e5c918434","observation_id":"5f4c1195-e3d6-4002-ae07-0a51655d24cd","resolution":{"observed_at":"2026-08-12T14:48:39.628866Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1311.5154","last_updated":"2014-02-26T14:40:45Z","snapshot_observed_at":"2026-08-14T23:54:33.762402Z","submitted_at":"2013-11-20T18:10:27Z","title":"Interacting quark matter equation of state for compact stars","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1311.5154","snapshot_observed_at":"2026-08-12T14:48:39.633221Z","title":null,"venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2411.14930","last_updated":"2025-04-02T10:48:19Z","snapshot_observed_at":"2026-08-17T16:07:02.156639Z","submitted_at":"2024-11-22T13:39:01Z","title":"Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state","version":2},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-12T14:48:39.633221Z"},"links":{"cited_paper":"/paper/1311.5154","citing_paper":"/paper/2411.14930"},"observation_digest":"sha256:844614a08bc4931facdb5ae6ffda1f253238f1877c5fccd4946b84ac5265bbbd","observation_id":"14584ece-9cfb-4694-840a-1bf10f48763e","resolution":{"observed_at":"2026-08-12T14:48:39.633221Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1402.6618","last_updated":"2014-02-26T17:35:50Z","snapshot_observed_at":"2026-08-15T23:45:06.219059Z","submitted_at":"2014-02-26T17:35:50Z","title":"Constraining neutron star matter with QCD","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1402.6618","snapshot_observed_at":"2026-08-12T14:48:39.637758Z","title":"Kurkela, E","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2411.14930","last_updated":"2025-04-02T10:48:19Z","snapshot_observed_at":"2026-08-17T16:07:02.156639Z","submitted_at":"2024-11-22T13:39:01Z","title":"Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state","version":2},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-12T14:48:39.637758Z"},"links":{"cited_paper":"/paper/1402.6618","citing_paper":"/paper/2411.14930"},"observation_digest":"sha256:2abe4e3aadc0b85d84c8d9762f68cadcb17ea954cfbc121fba484cae43a0a8ae","observation_id":"241f6fc9-4125-40ab-8bf1-87e5a07d8a07","resolution":{"observed_at":"2026-08-12T14:48:39.637758Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1303.4662","last_updated":"2013-07-22T10:12:05Z","snapshot_observed_at":"2026-08-15T00:24:38.471934Z","submitted_at":"2013-03-19T16:57:33Z","title":"Equation of state and neutron star properties constrained by nuclear physics and observation","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1303.4662","snapshot_observed_at":"2026-08-12T14:48:39.642359Z","title":"Hebeler, J","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2411.14930","last_updated":"2025-04-02T10:48:19Z","snapshot_observed_at":"2026-08-17T16:07:02.156639Z","submitted_at":"2024-11-22T13:39:01Z","title":"Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state","version":2},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-12T14:48:39.642359Z"},"links":{"cited_paper":"/paper/1303.4662","citing_paper":"/paper/2411.14930"},"observation_digest":"sha256:2f8d380799e9c0b074acdbb0bf1c279c30b62610dfbc8dbabb314f2640d92e6a","observation_id":"fee429bc-a871-4cb0-b324-37f14bb31ede","resolution":{"observed_at":"2026-08-12T14:48:39.642359Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1710.08220","last_updated":"2019-02-02T04:36:38Z","snapshot_observed_at":"2026-08-19T16:53:29.201159Z","submitted_at":"2017-10-23T11:56:20Z","title":"Chiral interactions up to next-to-next-to-next-to-leading order and nuclear saturation","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1710.08220","snapshot_observed_at":"2026-08-12T14:48:39.647554Z","title":"Drischler, K","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2411.14930","last_updated":"2025-04-02T10:48:19Z","snapshot_observed_at":"2026-08-17T16:07:02.156639Z","submitted_at":"2024-11-22T13:39:01Z","title":"Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state","version":2},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-12T14:48:39.647554Z"},"links":{"cited_paper":"/paper/1710.08220","citing_paper":"/paper/2411.14930"},"observation_digest":"sha256:275667a4c9fd166ca635ff14a9ccb723a90477f3e4885783cd25fe4897729121","observation_id":"23e6d826-57f2-45e4-b3e3-d46edd2b0da5","resolution":{"observed_at":"2026-08-12T14:48:39.647554Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0911.4073","last_updated":"2009-11-20T18:41:34Z","snapshot_observed_at":"2026-08-16T17:45:23.823475Z","submitted_at":"2009-11-20T18:41:34Z","title":"Statistical Model for a Complete Supernova Equation of State","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0911.4073","snapshot_observed_at":"2026-08-12T14:48:39.653024Z","title":"Hempel and J","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2411.14930","last_updated":"2025-04-02T10:48:19Z","snapshot_observed_at":"2026-08-17T16:07:02.156639Z","submitted_at":"2024-11-22T13:39:01Z","title":"Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state","version":2},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-12T14:48:39.653024Z"},"links":{"cited_paper":"/paper/0911.4073","citing_paper":"/paper/2411.14930"},"observation_digest":"sha256:39f942555b43013f22676825f3c0ba05891450290b4cb9b8cf1d9286cb5679e0","observation_id":"031384af-8701-424e-a890-324de4420957","resolution":{"observed_at":"2026-08-12T14:48:39.653024Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1108.0848","last_updated":"2012-11-22T15:11:18Z","snapshot_observed_at":"2026-08-18T13:49:02.027374Z","submitted_at":"2011-08-03T14:08:54Z","title":"New Equations of State in Simulations of Core-Collapse Supernovae","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1108.0848","snapshot_observed_at":"2026-08-12T14:48:39.657712Z","title":"Hempel, T","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2411.14930","last_updated":"2025-04-02T10:48:19Z","snapshot_observed_at":"2026-08-17T16:07:02.156639Z","submitted_at":"2024-11-22T13:39:01Z","title":"Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state","version":2},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-12T14:48:39.657712Z"},"links":{"cited_paper":"/paper/1108.0848","citing_paper":"/paper/2411.14930"},"observation_digest":"sha256:3c2a7cda84b25c295065d06d552e650c366f138af38d38c9a43800f6f2e2ad3c","observation_id":"4b9310ad-36e0-447e-8812-e8fa182ef2e9","resolution":{"observed_at":"2026-08-12T14:48:39.657712Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2011.05855","last_updated":"2021-05-17T14:54:59Z","snapshot_observed_at":"2026-08-16T19:06:34.152422Z","submitted_at":"2020-11-11T15:43:07Z","title":"Neutron matter at finite temperature based on chiral effective field theory interactions","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2011.05855","snapshot_observed_at":"2026-08-12T14:48:39.662690Z","title":"Keller, C","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2411.14930","last_updated":"2025-04-02T10:48:19Z","snapshot_observed_at":"2026-08-17T16:07:02.156639Z","submitted_at":"2024-11-22T13:39:01Z","title":"Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state","version":2},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-12T14:48:39.662690Z"},"links":{"cited_paper":"/paper/2011.05855","citing_paper":"/paper/2411.14930"},"observation_digest":"sha256:1bfee9c9c1f8c877db83b7f52d37db9cb081edd00e6fa29173a59fc60c59a1e9","observation_id":"01247319-fe17-440d-8022-99aa9201593c","resolution":{"observed_at":"2026-08-12T14:48:39.662690Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2204.14016","last_updated":"2023-02-20T13:50:33Z","snapshot_observed_at":"2026-08-19T23:49:39.510270Z","submitted_at":"2022-04-29T11:04:31Z","title":"Nuclear equation of state for arbitrary proton fraction and temperature based on chiral effective field theory and a Gaussian process emulator","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2204.14016","snapshot_observed_at":"2026-08-12T14:48:39.667616Z","title":"Keller, K","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2411.14930","last_updated":"2025-04-02T10:48:19Z","snapshot_observed_at":"2026-08-17T16:07:02.156639Z","submitted_at":"2024-11-22T13:39:01Z","title":"Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state","version":2},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-12T14:48:39.667616Z"},"links":{"cited_paper":"/paper/2204.14016","citing_paper":"/paper/2411.14930"},"observation_digest":"sha256:bb57c5a8f1c59fc5dd37d00979d4f3d543a8e2377abaf7adc90e5330911a292d","observation_id":"08459f19-4e3d-4524-98e5-9bd796b5e18c","resolution":{"observed_at":"2026-08-12T14:48:39.667616Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2304.07836","last_updated":"2023-11-17T21:57:53Z","snapshot_observed_at":"2026-08-18T06:45:12.664400Z","submitted_at":"2023-04-16T17:17:11Z","title":"Tabulated Equations of State From Models Informed by Chiral Effective Field Theory","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2304.07836","snapshot_observed_at":"2026-08-12T14:48:39.672354Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2411.14930","last_updated":"2025-04-02T10:48:19Z","snapshot_observed_at":"2026-08-17T16:07:02.156639Z","submitted_at":"2024-11-22T13:39:01Z","title":"Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state","version":2},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-12T14:48:39.672354Z"},"links":{"cited_paper":"/paper/2304.07836","citing_paper":"/paper/2411.14930"},"observation_digest":"sha256:78d2295e78812e4eae33e047cd74729130e9f9c5574658ca8e3c133cf7789301","observation_id":"943c4443-37d0-41b6-97c4-bb09831ec596","resolution":{"observed_at":"2026-08-12T14:48:39.672354Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1509.08805","last_updated":"2015-09-29T15:31:15Z","snapshot_observed_at":"2026-08-20T01:30:03.224757Z","submitted_at":"2015-09-29T15:31:15Z","title":"Pulsar J0453+1559: A Double Neutron Star System with a Large Mass Asymmetry","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1509.08805","snapshot_observed_at":"2026-08-12T14:48:39.677149Z","title":null,"venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2411.14930","last_updated":"2025-04-02T10:48:19Z","snapshot_observed_at":"2026-08-17T16:07:02.156639Z","submitted_at":"2024-11-22T13:39:01Z","title":"Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state","version":2},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-12T14:48:39.677149Z"},"links":{"cited_paper":"/paper/1509.08805","citing_paper":"/paper/2411.14930"},"observation_digest":"sha256:57a6d3d6aedfcb9fb5bb61411e7518cc3585685fe9049d971706e06ddc4e4c23","observation_id":"39e321b7-4b22-4e1f-b00a-d567849dc0da","resolution":{"observed_at":"2026-08-12T14:48:39.677149Z","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":"2026-08-12T14:48:42.009907Z","title":"Doroshenko, V","venue":null,"work_id":"2d5d645c-4337-4747-a864-eb6c7a58e510","year":2022},"citing_paper":{"arxiv_id":"2411.14930","last_updated":"2025-04-02T10:48:19Z","snapshot_observed_at":"2026-08-17T16:07:02.156639Z","submitted_at":"2024-11-22T13:39:01Z","title":"Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state","version":2},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-12T14:48:39.681836Z"},"links":{"citing_paper":"/paper/2411.14930"},"observation_digest":"sha256:f1e3a5c9aa753abc3afb4ab8024fc22dc513b916e467a39819bfc5dead6dd0a1","observation_id":"9f7245e6-58ff-4846-8d17-780fb74ebe84","resolution":{"observed_at":"2026-08-12T14:48:42.014097Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1808.02328","last_updated":"2019-04-10T15:31:53Z","snapshot_observed_at":"2026-08-14T18:43:46.264982Z","submitted_at":"2018-08-07T12:52:32Z","title":"On the minimum mass of neutron stars","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1808.02328","snapshot_observed_at":"2026-08-12T14:48:39.686203Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2411.14930","last_updated":"2025-04-02T10:48:19Z","snapshot_observed_at":"2026-08-17T16:07:02.156639Z","submitted_at":"2024-11-22T13:39:01Z","title":"Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state","version":2},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-12T14:48:39.686203Z"},"links":{"cited_paper":"/paper/1808.02328","citing_paper":"/paper/2411.14930"},"observation_digest":"sha256:999c3e21a406b814383d0a2bc014260e3beea67849415a5080ec609936bb0c36","observation_id":"318aa8cd-6f6e-485e-9e79-4d6af992b4b5","resolution":{"observed_at":"2026-08-12T14:48:39.686203Z","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":"2026-08-12T14:48:39.691139Z","title":"Stockinger et al., Mon","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2411.14930","last_updated":"2025-04-02T10:48:19Z","snapshot_observed_at":"2026-08-17T16:07:02.156639Z","submitted_at":"2024-11-22T13:39:01Z","title":"Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state","version":2},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-12T14:48:39.691139Z"},"links":{"citing_paper":"/paper/2411.14930"},"observation_digest":"sha256:aa1d1b6fb77b5cef9c007239b3eaea6a38d18cca4b8c5ccca56fa78cb81d18ce","observation_id":"e15ae581-ac13-423a-a31e-4609666f1f39","resolution":{"observed_at":"2026-08-12T14:48:39.691139Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2407.08407","last_updated":"2025-01-15T00:17:09Z","snapshot_observed_at":"2026-08-16T13:35:07.442373Z","submitted_at":"2024-07-11T11:20:50Z","title":"The minimum neutron star mass in neutrino-driven supernova explosions","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2407.08407","snapshot_observed_at":"2026-08-12T14:48:39.695483Z","title":"M¨ uller, A","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2411.14930","last_updated":"2025-04-02T10:48:19Z","snapshot_observed_at":"2026-08-17T16:07:02.156639Z","submitted_at":"2024-11-22T13:39:01Z","title":"Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state","version":2},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-12T14:48:39.695483Z"},"links":{"cited_paper":"/paper/2407.08407","citing_paper":"/paper/2411.14930"},"observation_digest":"sha256:e371923d616aa41407aece9d46a11d5ca0164b4c44cc225204dd2f3ee937535d","observation_id":"4e2a8791-2773-48a1-bc8d-4578da5bc581","resolution":{"observed_at":"2026-08-12T14:48:39.695483Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2409.14923","last_updated":"2024-11-20T16:53:28Z","snapshot_observed_at":"2026-08-16T22:15:15.605765Z","submitted_at":"2024-09-23T11:19:19Z","title":"A NICER View of PSR J1231$-$1411: A Complex Case","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2409.14923","snapshot_observed_at":"2026-08-12T14:48:39.700322Z","title":"Salmi, J","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2411.14930","last_updated":"2025-04-02T10:48:19Z","snapshot_observed_at":"2026-08-17T16:07:02.156639Z","submitted_at":"2024-11-22T13:39:01Z","title":"Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state","version":2},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-12T14:48:39.700322Z"},"links":{"cited_paper":"/paper/2409.14923","citing_paper":"/paper/2411.14930"},"observation_digest":"sha256:a8fea977f2c13e7d51eb844c00b85d7d7a9adb58cb18f88d00e6c91af095df65","observation_id":"e3e12da0-e2f5-410e-90ec-d8517b5e3fc0","resolution":{"observed_at":"2026-08-12T14:48:39.700322Z","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":"2026-08-12T14:48:41.994124Z","title":"Burrows and J","venue":null,"work_id":"c72a23d4-c029-4ad1-9694-7a725d184906","year":1986},"citing_paper":{"arxiv_id":"2411.14930","last_updated":"2025-04-02T10:48:19Z","snapshot_observed_at":"2026-08-17T16:07:02.156639Z","submitted_at":"2024-11-22T13:39:01Z","title":"Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state","version":2},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-12T14:48:39.705307Z"},"links":{"citing_paper":"/paper/2411.14930"},"observation_digest":"sha256:4dbe09df1b4a75ff1c322d6b19878067f5616acd555775567245b2bf35d124c3","observation_id":"d032ea5f-b7f1-4da4-8e3b-17407340f0e9","resolution":{"observed_at":"2026-08-12T14:48:41.999806Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+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":"2026-08-12T14:48:41.979063Z","title":"Burrows and J","venue":null,"work_id":"d249268b-66cf-47aa-a901-2f1d54f36db9","year":1988},"citing_paper":{"arxiv_id":"2411.14930","last_updated":"2025-04-02T10:48:19Z","snapshot_observed_at":"2026-08-17T16:07:02.156639Z","submitted_at":"2024-11-22T13:39:01Z","title":"Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state","version":2},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-12T14:48:39.709948Z"},"links":{"citing_paper":"/paper/2411.14930"},"observation_digest":"sha256:714591b2a47b5c9c6273e25315a7bbc8d1ed4bcda1fea39364164407c122f072","observation_id":"25d2db5e-ac24-4a34-801b-606f7c573714","resolution":{"observed_at":"2026-08-12T14:48:41.983914Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9610203","last_updated":"1996-10-25T08:47:28Z","snapshot_observed_at":"2026-07-07T01:14:50.921706Z","submitted_at":"1996-10-25T08:47:28Z","title":"Ledoux-Convection in Protoneutron Stars --- a Clue to Supernova Nucleosynthesis?","version":1},"cited_work":{"arxiv_id":"astro-ph/9610203","doi":null,"metadata_source":"pith","pith_arxiv_id":"astro-ph/9610203","snapshot_observed_at":"2026-08-12T14:48:41.109967Z","title":"Ledoux-Convection in Protoneutron Stars --- a Clue to Supernova Nucleosynthesis?","venue":"astro-ph","work_id":"6521a34c-3d5b-46be-96c7-4fd11f5131ff","year":1996},"citing_paper":{"arxiv_id":"2411.14930","last_updated":"2025-04-02T10:48:19Z","snapshot_observed_at":"2026-08-17T16:07:02.156639Z","submitted_at":"2024-11-22T13:39:01Z","title":"Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state","version":2},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-12T14:48:39.713951Z"},"links":{"cited_paper":"/paper/astro-ph/9610203","citing_paper":"/paper/2411.14930"},"observation_digest":"sha256:6907d3aa95f851232f2be385f995eb95c06ff955581fc6ab83f5fa54b17a3871","observation_id":"f02b0ce6-5d3d-4bf7-b671-0fe37e2ad8a0","resolution":{"observed_at":"2026-08-12T14:48:41.115370Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2201.01955","last_updated":"2022-01-06T07:48:33Z","snapshot_observed_at":"2026-08-16T17:29:58.372809Z","submitted_at":"2022-01-06T07:48:33Z","title":"Proto-neutron star evolution with improved charged-current neutrino-nucleon interactions","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2201.01955","snapshot_observed_at":"2026-08-12T14:48:39.718061Z","title":"Pascal, J","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2411.14930","last_updated":"2025-04-02T10:48:19Z","snapshot_observed_at":"2026-08-17T16:07:02.156639Z","submitted_at":"2024-11-22T13:39:01Z","title":"Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state","version":2},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-12T14:48:39.718061Z"},"links":{"cited_paper":"/paper/2201.01955","citing_paper":"/paper/2411.14930"},"observation_digest":"sha256:3132dac44eae7a26fda75f48d91815923353369b679a211bf6faeebc188ae2e7","observation_id":"fe1730c3-80dd-4eeb-bcdf-f81d283ab87b","resolution":{"observed_at":"2026-08-12T14:48:39.718061Z","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":"2026-08-15T04:27:04.533554Z","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":"2026-08-12T14:48:39.722077Z","title":null,"venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2411.14930","last_updated":"2025-04-02T10:48:19Z","snapshot_observed_at":"2026-08-17T16:07:02.156639Z","submitted_at":"2024-11-22T13:39:01Z","title":"Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state","version":2},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-12T14:48:39.722077Z"},"links":{"cited_paper":"/paper/1112.0335","citing_paper":"/paper/2411.14930"},"observation_digest":"sha256:a06523af204cf11bf459cb2b55788150c3e92b870119b35995a607c668f7edc5","observation_id":"da2f933d-db03-43db-9a83-606f83773d87","resolution":{"observed_at":"2026-08-12T14:48:39.722077Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1508.00785","last_updated":"2016-02-05T10:48:32Z","snapshot_observed_at":"2026-08-15T15:11:13.854972Z","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":"2026-08-12T14:48:39.726108Z","title":"Mirizzi, I","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2411.14930","last_updated":"2025-04-02T10:48:19Z","snapshot_observed_at":"2026-08-17T16:07:02.156639Z","submitted_at":"2024-11-22T13:39:01Z","title":"Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state","version":2},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-12T14:48:39.726108Z"},"links":{"cited_paper":"/paper/1508.00785","citing_paper":"/paper/2411.14930"},"observation_digest":"sha256:eb31aa8d12cdf59f24460fb258230cf061efd277646905f9825c9027c0d65c5f","observation_id":"b439c242-b05f-4a44-8048-9f9a1c4dbdc7","resolution":{"observed_at":"2026-08-12T14:48:39.726108Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1912.07615","last_updated":"2020-01-24T12:06:36Z","snapshot_observed_at":"2026-08-13T06:59:27.481419Z","submitted_at":"2019-12-16T19:00:03Z","title":"A systematic study of proto-neutron star convection in three-dimensional core-collapse supernova simulations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1912.07615","snapshot_observed_at":"2026-08-12T14:48:39.730285Z","title":"Nagakura, A","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2411.14930","last_updated":"2025-04-02T10:48:19Z","snapshot_observed_at":"2026-08-17T16:07:02.156639Z","submitted_at":"2024-11-22T13:39:01Z","title":"Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state","version":2},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-12T14:48:39.730285Z"},"links":{"cited_paper":"/paper/1912.07615","citing_paper":"/paper/2411.14930"},"observation_digest":"sha256:5ee89633535e5e46459af0dab34680484b457a409d0caff4c1b2b3db7eb515df","observation_id":"00ee69cb-307c-4d5a-89a3-2948804c7f8b","resolution":{"observed_at":"2026-08-12T14:48:39.730285Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2308.01403","last_updated":"2023-10-03T09:36:44Z","snapshot_observed_at":"2026-08-16T15:11:13.928870Z","submitted_at":"2023-08-02T19:53:40Z","title":"Supernova Simulations Confront SN 1987A Neutrinos","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2308.01403","snapshot_observed_at":"2026-08-12T14:48:39.734986Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2411.14930","last_updated":"2025-04-02T10:48:19Z","snapshot_observed_at":"2026-08-17T16:07:02.156639Z","submitted_at":"2024-11-22T13:39:01Z","title":"Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state","version":2},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-12T14:48:39.734986Z"},"links":{"cited_paper":"/paper/2308.01403","citing_paper":"/paper/2411.14930"},"observation_digest":"sha256:4d557b5aadcb21b30954aab77e41f775a781340c487b33e8f52a568270d7969a","observation_id":"b918648c-c52a-4fdd-9e42-1ff4bc4f51e5","resolution":{"observed_at":"2026-08-12T14:48:39.734986Z","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":"2026-08-12T14:48:41.852297Z","title":"Haines et al","venue":null,"work_id":"3e559d15-b018-4caa-b9d6-ef408cdfad9f","year":1988},"citing_paper":{"arxiv_id":"2411.14930","last_updated":"2025-04-02T10:48:19Z","snapshot_observed_at":"2026-08-17T16:07:02.156639Z","submitted_at":"2024-11-22T13:39:01Z","title":"Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state","version":2},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-12T14:48:39.740174Z"},"links":{"citing_paper":"/paper/2411.14930"},"observation_digest":"sha256:0cf3c6fa20012b94b080bfed62aca3f454f5b4093c23f905cf411b9fdef907cc","observation_id":"cbbc7ba9-9d7d-4856-950e-9a5639601af4","resolution":{"observed_at":"2026-08-12T14:48:41.895876Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"ph/0510229","doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-12T14:48:40.968994Z","title":"Dessart, A","venue":null,"work_id":"2561f34c-6f1b-4e80-8f75-c42344144fb5","year":2006},"citing_paper":{"arxiv_id":"2411.14930","last_updated":"2025-04-02T10:48:19Z","snapshot_observed_at":"2026-08-17T16:07:02.156639Z","submitted_at":"2024-11-22T13:39:01Z","title":"Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state","version":2},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-12T14:48:39.744756Z"},"links":{"citing_paper":"/paper/2411.14930"},"observation_digest":"sha256:07ec43cf4e68d64b4899703ce36e3e8bc247145226efeab64e0af016d5835a09","observation_id":"2b65fb69-81de-4272-a0df-55f210fdcfe9","resolution":{"observed_at":"2026-08-12T14:48:40.996537Z","resolver_source":"raw_fallback","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1801.01350","last_updated":"2018-01-04T13:52:20Z","snapshot_observed_at":"2026-08-14T19:58:02.316111Z","submitted_at":"2018-01-04T13:52:20Z","title":"Early evolution of newly born proto-neutron stars","version":1},"cited_work":{"arxiv_id":"1801.01350","doi":null,"metadata_source":"pith","pith_arxiv_id":"1801.01350","snapshot_observed_at":"2026-08-12T14:48:40.887424Z","title":"Early evolution of newly born proto-neutron stars","venue":"gr-qc","work_id":"1542060c-8c2a-4168-a150-389dab5496da","year":2018},"citing_paper":{"arxiv_id":"2411.14930","last_updated":"2025-04-02T10:48:19Z","snapshot_observed_at":"2026-08-17T16:07:02.156639Z","submitted_at":"2024-11-22T13:39:01Z","title":"Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state","version":2},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-12T14:48:39.749262Z"},"links":{"cited_paper":"/paper/1801.01350","citing_paper":"/paper/2411.14930"},"observation_digest":"sha256:f362c483a279592d1253dec2e0fb0608015d226995f442b46517e3338632d1e0","observation_id":"2f005126-0064-4964-8660-eab6b7ea5c52","resolution":{"observed_at":"2026-08-12T14:48:40.892481Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"ph/0512189","doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-12T14:48:40.861798Z","title":"Buras, H","venue":null,"work_id":"01b722fe-7b26-44be-90eb-03199573f214","year":2006},"citing_paper":{"arxiv_id":"2411.14930","last_updated":"2025-04-02T10:48:19Z","snapshot_observed_at":"2026-08-17T16:07:02.156639Z","submitted_at":"2024-11-22T13:39:01Z","title":"Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state","version":2},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-12T14:48:39.754054Z"},"links":{"citing_paper":"/paper/2411.14930"},"observation_digest":"sha256:ad079767de71b7996a9c640cee958ae00514225e3a49fb6d3e1026814d6e6292","observation_id":"4ac5d841-c449-43bf-a67f-9da2855f8b51","resolution":{"observed_at":"2026-08-12T14:48:40.870546Z","resolver_source":"raw_fallback","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"nucl-th/9603042","last_updated":"1996-03-27T22:26:14Z","snapshot_observed_at":"2026-08-15T13:09:34.785965Z","submitted_at":"1996-03-27T22:26:14Z","title":"Composition and Structure of Protoneutron Stars","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"nucl-th/9603042","snapshot_observed_at":"2026-08-12T14:48:39.758517Z","title":"Prakash, I","venue":null,"work_id":null,"year":1997},"citing_paper":{"arxiv_id":"2411.14930","last_updated":"2025-04-02T10:48:19Z","snapshot_observed_at":"2026-08-17T16:07:02.156639Z","submitted_at":"2024-11-22T13:39:01Z","title":"Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state","version":2},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-12T14:48:39.758517Z"},"links":{"cited_paper":"/paper/nucl-th/9603042","citing_paper":"/paper/2411.14930"},"observation_digest":"sha256:037e98635a0350911f55a6c8c5bc4969e1e3a03e14ad5fb97babc241607f6b67","observation_id":"8b73ccbd-591e-4c56-8a1e-412265c96ba2","resolution":{"observed_at":"2026-08-12T14:48:39.758517Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"hep-ph/0005228","last_updated":"2000-05-23T21:35:12Z","snapshot_observed_at":"2026-07-07T03:48:37.017164Z","submitted_at":"2000-05-23T21:35:12Z","title":"Neutrino Propagation In Color Superconducting Quark Matter","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-ph/0005228","snapshot_observed_at":"2026-08-12T14:48:39.763216Z","title":null,"venue":null,"work_id":null,"year":2000},"citing_paper":{"arxiv_id":"2411.14930","last_updated":"2025-04-02T10:48:19Z","snapshot_observed_at":"2026-08-17T16:07:02.156639Z","submitted_at":"2024-11-22T13:39:01Z","title":"Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state","version":2},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-08-12T14:48:39.763216Z"},"links":{"cited_paper":"/paper/hep-ph/0005228","citing_paper":"/paper/2411.14930"},"observation_digest":"sha256:1a4d065a4e1c438e8a6d8b8cfa414f31843273b075db59de9b8be42ba06560ac","observation_id":"6261fb97-9170-4272-8f5e-7b8e0f126169","resolution":{"observed_at":"2026-08-12T14:48:39.763216Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0407155","last_updated":"2004-09-27T15:41:29Z","snapshot_observed_at":"2026-08-06T21:42:30.929605Z","submitted_at":"2004-07-07T20:16:59Z","title":"Strange Quark Matter and Compact Stars","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0407155","snapshot_observed_at":"2026-08-12T14:48:39.767801Z","title":"Weber, Prog","venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2411.14930","last_updated":"2025-04-02T10:48:19Z","snapshot_observed_at":"2026-08-17T16:07:02.156639Z","submitted_at":"2024-11-22T13:39:01Z","title":"Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state","version":2},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-12T14:48:39.767801Z"},"links":{"cited_paper":"/paper/astro-ph/0407155","citing_paper":"/paper/2411.14930"},"observation_digest":"sha256:29b3a7195aedf8e44e00317cfc2f5d9d1f1fa4166553307512fe7b548872ee7c","observation_id":"2ace2905-0bce-4907-8057-24582db13299","resolution":{"observed_at":"2026-08-12T14:48:39.767801Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"hep-ph/0402234","last_updated":"2005-01-27T09:45:51Z","snapshot_observed_at":"2026-08-19T10:56:45.440668Z","submitted_at":"2004-02-23T09:53:49Z","title":"NJL-model analysis of dense quark matter","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-ph/0402234","snapshot_observed_at":"2026-08-12T14:48:39.772258Z","title":"Buballa, Phys","venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2411.14930","last_updated":"2025-04-02T10:48:19Z","snapshot_observed_at":"2026-08-17T16:07:02.156639Z","submitted_at":"2024-11-22T13:39:01Z","title":"Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state","version":2},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-12T14:48:39.772258Z"},"links":{"cited_paper":"/paper/hep-ph/0402234","citing_paper":"/paper/2411.14930"},"observation_digest":"sha256:eacedf9e3ced93b1ddc140cabcb82a7b173011b00501c119e1e71fc846677b70","observation_id":"5e4a8bbd-11d4-4b7c-8d49-b7973ef1193a","resolution":{"observed_at":"2026-08-12T14:48:39.772258Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0809.4225","last_updated":"2008-09-24T16:25:08Z","snapshot_observed_at":"2026-08-15T10:06:09.401772Z","submitted_at":"2008-09-24T16:25:08Z","title":"Signals of the QCD phase transition in core-collapse supernovae","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0809.4225","snapshot_observed_at":"2026-08-12T14:48:39.777106Z","title":"Sagert, T","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2411.14930","last_updated":"2025-04-02T10:48:19Z","snapshot_observed_at":"2026-08-17T16:07:02.156639Z","submitted_at":"2024-11-22T13:39:01Z","title":"Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state","version":2},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-12T14:48:39.777106Z"},"links":{"cited_paper":"/paper/0809.4225","citing_paper":"/paper/2411.14930"},"observation_digest":"sha256:59f4de95ff2ccd343a31f9e9bfe484574320f9581a9f10502079d078f8a16402","observation_id":"cf9ce2c1-e442-440f-8d90-a7fb89f7dabf","resolution":{"observed_at":"2026-08-12T14:48:39.777106Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1510.06306","last_updated":"2015-11-06T16:07:42Z","snapshot_observed_at":"2026-08-18T20:49:48.796507Z","submitted_at":"2015-10-21T15:46:47Z","title":"Do hyperons exist in the interior of neutron stars ?","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1510.06306","snapshot_observed_at":"2026-08-12T14:48:39.781871Z","title":"Chatterjee and I","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2411.14930","last_updated":"2025-04-02T10:48:19Z","snapshot_observed_at":"2026-08-17T16:07:02.156639Z","submitted_at":"2024-11-22T13:39:01Z","title":"Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state","version":2},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-12T14:48:39.781871Z"},"links":{"cited_paper":"/paper/1510.06306","citing_paper":"/paper/2411.14930"},"observation_digest":"sha256:4021fb8fef25fafb0ce499cc6f38f0859390d4a682e4e0895c815944e59d9a45","observation_id":"674c47ff-75c9-404c-9319-413cefeaeb46","resolution":{"observed_at":"2026-08-12T14:48:39.781871Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2003.00972","last_updated":"2020-05-07T10:03:48Z","snapshot_observed_at":"2026-08-09T17:13:14.626265Z","submitted_at":"2020-03-02T15:42:25Z","title":"Core-collapse Supernova Explosions Driven by the Hadron-quark Phase Transition as a Rare $r$-process Site","version":2},"cited_work":{"arxiv_id":"2003.00972","doi":null,"metadata_source":"pith","pith_arxiv_id":"2003.00972","snapshot_observed_at":"2026-08-12T14:48:40.697864Z","title":"Core-collapse Supernova Explosions Driven by the Hadron-quark Phase Transition as a Rare $r$-process Site","venue":"astro-ph.HE","work_id":"4c3f394e-eb14-4c85-a18c-bb3033571836","year":2020},"citing_paper":{"arxiv_id":"2411.14930","last_updated":"2025-04-02T10:48:19Z","snapshot_observed_at":"2026-08-17T16:07:02.156639Z","submitted_at":"2024-11-22T13:39:01Z","title":"Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state","version":2},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-12T14:48:39.786380Z"},"links":{"cited_paper":"/paper/2003.00972","citing_paper":"/paper/2411.14930"},"observation_digest":"sha256:6cc8de37325a0c6a85809d2276f5b11811c1ce099befdfceff7c5fc1fa26f248","observation_id":"fc790462-d27a-466d-a66a-6eed57f75243","resolution":{"observed_at":"2026-08-12T14:48:40.703414Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"ph/9705157","doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-12T14:48:40.672017Z","title":"Gondek, P","venue":null,"work_id":"8ae1848a-8cdf-4cf0-a87d-366f096553ad","year":1997},"citing_paper":{"arxiv_id":"2411.14930","last_updated":"2025-04-02T10:48:19Z","snapshot_observed_at":"2026-08-17T16:07:02.156639Z","submitted_at":"2024-11-22T13:39:01Z","title":"Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state","version":2},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-12T14:48:39.791105Z"},"links":{"citing_paper":"/paper/2411.14930"},"observation_digest":"sha256:ec9832adef57262b7ec7b12d9ed97e628a134beb49e804d462e96cde4df5f410","observation_id":"70fe3a06-4c48-44b0-b45f-4dd33b5aa7b0","resolution":{"observed_at":"2026-08-12T14:48:40.679991Z","resolver_source":"raw_fallback","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"0802.1999","last_updated":"2008-07-16T12:33:41Z","snapshot_observed_at":"2026-08-15T10:21:40.519784Z","submitted_at":"2008-02-14T10:46:38Z","title":"Proto-Neutron and Neutron Stars in a Chiral SU(3) Model","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0802.1999","snapshot_observed_at":"2026-08-12T14:48:39.795384Z","title":"Dexheimer and S","venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2411.14930","last_updated":"2025-04-02T10:48:19Z","snapshot_observed_at":"2026-08-17T16:07:02.156639Z","submitted_at":"2024-11-22T13:39:01Z","title":"Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state","version":2},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-12T14:48:39.795384Z"},"links":{"cited_paper":"/paper/0802.1999","citing_paper":"/paper/2411.14930"},"observation_digest":"sha256:97b16a346facd023c3fd1cfbcf8ff46f8849d10cec44ae5ec71ef6675c3cbcae","observation_id":"516cce95-2a01-40d3-93fb-66d1393ac3a8","resolution":{"observed_at":"2026-08-12T14:48:39.795384Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1002.4497","last_updated":"2010-08-25T08:53:03Z","snapshot_observed_at":"2026-08-19T08:19:26.101635Z","submitted_at":"2010-02-24T09:31:30Z","title":"The maximum and minimum mass of protoneutron stars in the Brueckner theory","version":2},"cited_work":{"arxiv_id":"1002.4497","doi":null,"metadata_source":"pith","pith_arxiv_id":"1002.4497","snapshot_observed_at":"2026-08-12T14:48:40.577387Z","title":"The maximum and minimum mass of protoneutron stars in the Brueckner theory","venue":"astro-ph.SR","work_id":"de9a3ad5-3907-4f91-8865-752d012ca3c3","year":2010},"citing_paper":{"arxiv_id":"2411.14930","last_updated":"2025-04-02T10:48:19Z","snapshot_observed_at":"2026-08-17T16:07:02.156639Z","submitted_at":"2024-11-22T13:39:01Z","title":"Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state","version":2},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-08-12T14:48:39.799988Z"},"links":{"cited_paper":"/paper/1002.4497","citing_paper":"/paper/2411.14930"},"observation_digest":"sha256:72ce538f91934b07bc5993a91d5e32d44d820a2cc0ffc13646629fd1d52b01be","observation_id":"63300a19-4693-494c-b4e2-de2858bad8f0","resolution":{"observed_at":"2026-08-12T14:48:40.582602Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2007.10424","last_updated":"2021-05-10T18:45:25Z","snapshot_observed_at":"2026-08-15T22:12:54.717320Z","submitted_at":"2020-07-20T19:28:45Z","title":"Thermodynamical Description of Hot, Rapidly Rotating Neutron Stars, Protoneutron Stars, and Neutron Star Merger Remnants","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2007.10424","snapshot_observed_at":"2026-08-12T14:48:39.804693Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2411.14930","last_updated":"2025-04-02T10:48:19Z","snapshot_observed_at":"2026-08-17T16:07:02.156639Z","submitted_at":"2024-11-22T13:39:01Z","title":"Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state","version":2},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-08-12T14:48:39.804693Z"},"links":{"cited_paper":"/paper/2007.10424","citing_paper":"/paper/2411.14930"},"observation_digest":"sha256:956ee456c25b917efbc17e6c803ff2454b6dd4aae0972d72c9f30a5be775327f","observation_id":"21658481-ff74-4f13-b81f-90c51a02d7c9","resolution":{"observed_at":"2026-08-12T14:48:39.804693Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1304.2212","last_updated":"2013-08-12T12:23:41Z","snapshot_observed_at":"2026-08-15T00:22:15.735297Z","submitted_at":"2013-04-08T14:04:39Z","title":"Neutron matter from chiral effective field theory interactions","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1304.2212","snapshot_observed_at":"2026-08-12T14:48:39.809400Z","title":"Kr¨ uger, I","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2411.14930","last_updated":"2025-04-02T10:48:19Z","snapshot_observed_at":"2026-08-17T16:07:02.156639Z","submitted_at":"2024-11-22T13:39:01Z","title":"Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state","version":2},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-08-12T14:48:39.809400Z"},"links":{"cited_paper":"/paper/1304.2212","citing_paper":"/paper/2411.14930"},"observation_digest":"sha256:bf529a056eec3fa124c8f10b4aaca83956783a3cdb085e81549c5d62863c4676","observation_id":"6844ff18-cdb4-4ed8-a2ee-f4873e405d12","resolution":{"observed_at":"2026-08-12T14:48:39.809400Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0908.2344","last_updated":"2009-12-18T08:33:35Z","snapshot_observed_at":"2026-08-15T05:41:22.815319Z","submitted_at":"2009-08-17T15:33:35Z","title":"Composition and thermodynamics of nuclear matter with light clusters","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0908.2344","snapshot_observed_at":"2026-08-12T14:48:39.814232Z","title":"Typel, G","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2411.14930","last_updated":"2025-04-02T10:48:19Z","snapshot_observed_at":"2026-08-17T16:07:02.156639Z","submitted_at":"2024-11-22T13:39:01Z","title":"Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state","version":2},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-08-12T14:48:39.814232Z"},"links":{"cited_paper":"/paper/0908.2344","citing_paper":"/paper/2411.14930"},"observation_digest":"sha256:c38835a3a2911be8db48b6471a6a8bc9db0c6fbd35878c3e49316bb2650b3b31","observation_id":"849f06c2-53e2-46af-91f0-71d581a2fc9e","resolution":{"observed_at":"2026-08-12T14:48:39.814232Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1207.2184","last_updated":"2012-07-09T21:00:43Z","snapshot_observed_at":"2026-08-15T00:53:51.994483Z","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":"2026-08-12T14:48:39.818546Z","title":null,"venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2411.14930","last_updated":"2025-04-02T10:48:19Z","snapshot_observed_at":"2026-08-17T16:07:02.156639Z","submitted_at":"2024-11-22T13:39:01Z","title":"Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state","version":2},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-08-12T14:48:39.818546Z"},"links":{"cited_paper":"/paper/1207.2184","citing_paper":"/paper/2411.14930"},"observation_digest":"sha256:78c00562691f24e9bf26125f85032f93ac9adf7a77747f12e6a4b3d4326a3751","observation_id":"afda7189-a8ae-48ae-a03a-641dc8c762db","resolution":{"observed_at":"2026-08-12T14:48:39.818546Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1702.08713","last_updated":"2017-02-28T09:40:19Z","snapshot_observed_at":"2026-08-20T15:20:01.803549Z","submitted_at":"2017-02-28T09:40:19Z","title":"Neutrino Emission from Supernovae","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1702.08713","snapshot_observed_at":"2026-08-12T14:48:39.823073Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2411.14930","last_updated":"2025-04-02T10:48:19Z","snapshot_observed_at":"2026-08-17T16:07:02.156639Z","submitted_at":"2024-11-22T13:39:01Z","title":"Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state","version":2},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-08-12T14:48:39.823073Z"},"links":{"cited_paper":"/paper/1702.08713","citing_paper":"/paper/2411.14930"},"observation_digest":"sha256:d7434381cce8e7467a5a0004be032feeebfdd2a5f97913b8684c10c1721d8d93","observation_id":"b87bc62e-b19b-4ef2-ac02-d0dbfce35a2b","resolution":{"observed_at":"2026-08-12T14:48:39.823073Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1505.02513","last_updated":"2015-11-30T12:34:19Z","snapshot_observed_at":"2026-08-14T22:49:08.537107Z","submitted_at":"2015-05-11T08:06:56Z","title":"Two-Dimensional Core-Collapse Supernova Simulations with the Isotropic Diffusion Source Approximation for Neutrino Transport","version":3},"cited_work":{"arxiv_id":"1505.02513","doi":null,"metadata_source":"pith","pith_arxiv_id":"1505.02513","snapshot_observed_at":"2026-08-12T14:48:40.426037Z","title":"Two-Dimensional Core-Collapse Supernova Simulations with the Isotropic Diffusion Source Approximation for Neutrino Transport","venue":"astro-ph.HE","work_id":"067a562f-7afa-4134-a843-5bda894502cf","year":2015},"citing_paper":{"arxiv_id":"2411.14930","last_updated":"2025-04-02T10:48:19Z","snapshot_observed_at":"2026-08-17T16:07:02.156639Z","submitted_at":"2024-11-22T13:39:01Z","title":"Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state","version":2},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-08-12T14:48:39.827627Z"},"links":{"cited_paper":"/paper/1505.02513","citing_paper":"/paper/2411.14930"},"observation_digest":"sha256:7f1d1a72fcad145d37d32fc3b489430a8793167b8626b3ba21b80ec776da1f22","observation_id":"cd970559-05f6-4d1f-a4f5-cafdbe4e9336","resolution":{"observed_at":"2026-08-12T14:48:40.450433Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2408.01406","last_updated":"2025-01-14T18:17:43Z","snapshot_observed_at":"2026-08-18T16:58:49.329260Z","submitted_at":"2024-08-02T17:31:36Z","title":"Hyperons during proto-neutron star deleptonization and the emission of dark flavoured particles","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2408.01406","snapshot_observed_at":"2026-08-12T14:48:39.832369Z","title":"Fischer, J","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2411.14930","last_updated":"2025-04-02T10:48:19Z","snapshot_observed_at":"2026-08-17T16:07:02.156639Z","submitted_at":"2024-11-22T13:39:01Z","title":"Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state","version":2},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-08-12T14:48:39.832369Z"},"links":{"cited_paper":"/paper/2408.01406","citing_paper":"/paper/2411.14930"},"observation_digest":"sha256:d120a386ba844aed19380d3ca50d08ff13eb5651310fdf635b25dc3baa7fe5bd","observation_id":"556760d5-51b9-401a-9eca-abb5d438c522","resolution":{"observed_at":"2026-08-12T14:48:39.832369Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2401.13728","last_updated":"2024-03-12T17:38:28Z","snapshot_observed_at":"2026-08-16T23:22:59.822526Z","submitted_at":"2024-01-24T19:00:00Z","title":"Astrophysical Axion Bounds: The 2024 Edition","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2401.13728","snapshot_observed_at":"2026-08-12T14:48:39.837207Z","title":"Caputo and G","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2411.14930","last_updated":"2025-04-02T10:48:19Z","snapshot_observed_at":"2026-08-17T16:07:02.156639Z","submitted_at":"2024-11-22T13:39:01Z","title":"Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state","version":2},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-08-12T14:48:39.837207Z"},"links":{"cited_paper":"/paper/2401.13728","citing_paper":"/paper/2411.14930"},"observation_digest":"sha256:4de1a5ab3210bf697317f5904d2f03eb7f5c30ce1fc0033d2859bf141367d3fa","observation_id":"3bbd90c6-82bd-46f5-8c74-a1dcfcb54c11","resolution":{"observed_at":"2026-08-12T14:48:39.837207Z","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":"2026-08-20T12:13:52.892033Z","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":"2026-08-12T14:48:39.842810Z","title":"Fischer, M","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2411.14930","last_updated":"2025-04-02T10:48:19Z","snapshot_observed_at":"2026-08-17T16:07:02.156639Z","submitted_at":"2024-11-22T13:39:01Z","title":"Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state","version":2},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-08-12T14:48:39.842810Z"},"links":{"cited_paper":"/paper/1307.6190","citing_paper":"/paper/2411.14930"},"observation_digest":"sha256:ca8d0251f2cc9f96591a51fc0078fab9486a35306cc8550d1cac4ebddc53d7a2","observation_id":"d8c73d6d-a6c9-49c6-a4a3-77b1c15b4e6e","resolution":{"observed_at":"2026-08-12T14:48:39.842810Z","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":"2026-08-12T14:48:39.847368Z","title":null,"venue":null,"work_id":null,"year":1990},"citing_paper":{"arxiv_id":"2411.14930","last_updated":"2025-04-02T10:48:19Z","snapshot_observed_at":"2026-08-17T16:07:02.156639Z","submitted_at":"2024-11-22T13:39:01Z","title":"Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state","version":2},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-08-12T14:48:39.847368Z"},"links":{"citing_paper":"/paper/2411.14930"},"observation_digest":"sha256:14cdd4ad9f2563c2b530f1cdc76ae1622760d11ef37b566399cbdf7ee2b96a21","observation_id":"93f0ac9a-6754-4106-a524-8ffa27e3fd63","resolution":{"observed_at":"2026-08-12T14:48:39.847368Z","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":"2026-08-12T14:48:41.787388Z","title":null,"venue":null,"work_id":"f1329cc0-ac2b-4b7a-bbae-9739c9fedc22","year":1966},"citing_paper":{"arxiv_id":"2411.14930","last_updated":"2025-04-02T10:48:19Z","snapshot_observed_at":"2026-08-17T16:07:02.156639Z","submitted_at":"2024-11-22T13:39:01Z","title":"Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state","version":2},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-08-12T14:48:39.852016Z"},"links":{"citing_paper":"/paper/2411.14930"},"observation_digest":"sha256:06322e046cb6083551c9c4b1c25477e02b6467038132ebb515de7d53fed44b07","observation_id":"81a3a3fe-e276-4daf-9a3e-f40fa004592d","resolution":{"observed_at":"2026-08-12T14:48:41.792295Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+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":"2026-08-12T14:48:41.772712Z","title":null,"venue":null,"work_id":"709dc4e8-35c6-4eeb-a52f-2ac2d3f02c46","year":1966},"citing_paper":{"arxiv_id":"2411.14930","last_updated":"2025-04-02T10:48:19Z","snapshot_observed_at":"2026-08-17T16:07:02.156639Z","submitted_at":"2024-11-22T13:39:01Z","title":"Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state","version":2},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-08-12T14:48:39.857143Z"},"links":{"citing_paper":"/paper/2411.14930"},"observation_digest":"sha256:cd14429f5c4999e6dfeacc6ee7ce49c8bc1e981a39f17faaf31678c7bc3b17cf","observation_id":"9bbf6308-7ed5-4d4e-82f3-18760c11ca72","resolution":{"observed_at":"2026-08-12T14:48:41.777028Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0512065","last_updated":"2006-01-02T14:05:46Z","snapshot_observed_at":"2026-08-07T17:07:19.834377Z","submitted_at":"2005-12-02T17:38:12Z","title":"Explosions of O-Ne-Mg Cores, the Crab Supernova, and Subluminous Type II-P Supernovae","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0512065","snapshot_observed_at":"2026-08-12T14:48:39.861567Z","title":null,"venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"2411.14930","last_updated":"2025-04-02T10:48:19Z","snapshot_observed_at":"2026-08-17T16:07:02.156639Z","submitted_at":"2024-11-22T13:39:01Z","title":"Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state","version":2},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-08-12T14:48:39.861567Z"},"links":{"cited_paper":"/paper/astro-ph/0512065","citing_paper":"/paper/2411.14930"},"observation_digest":"sha256:8a259df13741ea54bdc9f432524730469943331511a4db859d7fe3a35171cd33","observation_id":"3c7c5c40-bf49-464a-b402-e430825bd805","resolution":{"observed_at":"2026-08-12T14:48:39.861567Z","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":"2026-08-19T21:00:00.465635Z","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":"2026-08-12T14:48:39.866293Z","title":"Janka, Ann","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2411.14930","last_updated":"2025-04-02T10:48:19Z","snapshot_observed_at":"2026-08-17T16:07:02.156639Z","submitted_at":"2024-11-22T13:39:01Z","title":"Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state","version":2},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-08-12T14:48:39.866293Z"},"links":{"cited_paper":"/paper/1206.2503","citing_paper":"/paper/2411.14930"},"observation_digest":"sha256:fc5119fa086f2f0c3f92f141bb10536531ac909e1e4b46429360a02d1a6aedae","observation_id":"ecc7033b-ad3a-4d60-b053-6cf20dd7264a","resolution":{"observed_at":"2026-08-12T14:48:39.866293Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9812058","last_updated":"1998-12-02T20:40:20Z","snapshot_observed_at":"2026-08-14T09:57:08.192342Z","submitted_at":"1998-12-02T20:40:20Z","title":"What Can the Accretion Induced Collapse of White Dwarfs Really Explain?","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9812058","snapshot_observed_at":"2026-08-12T14:48:39.871151Z","title":null,"venue":null,"work_id":null,"year":1999},"citing_paper":{"arxiv_id":"2411.14930","last_updated":"2025-04-02T10:48:19Z","snapshot_observed_at":"2026-08-17T16:07:02.156639Z","submitted_at":"2024-11-22T13:39:01Z","title":"Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state","version":2},"reference_index":54,"source":"pdf_text","source_observed_at":"2026-08-12T14:48:39.871151Z"},"links":{"cited_paper":"/paper/astro-ph/9812058","citing_paper":"/paper/2411.14930"},"observation_digest":"sha256:fc4ef7c7746a7639afe16c45d4f70f6b793782227445b45a413a15784964cabf","observation_id":"df5be244-a8ed-4364-bdef-40b5d0a73d80","resolution":{"observed_at":"2026-08-12T14:48:39.871151Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2005.01880","last_updated":"2020-07-10T07:04:38Z","snapshot_observed_at":"2026-08-02T08:52:24.771535Z","submitted_at":"2020-05-04T22:57:32Z","title":"The formation of neutron star systems through accretion-induced collapse in white-dwarf binaries","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2005.01880","snapshot_observed_at":"2026-08-12T14:48:39.875749Z","title":"Wang and D","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2411.14930","last_updated":"2025-04-02T10:48:19Z","snapshot_observed_at":"2026-08-17T16:07:02.156639Z","submitted_at":"2024-11-22T13:39:01Z","title":"Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state","version":2},"reference_index":55,"source":"pdf_text","source_observed_at":"2026-08-12T14:48:39.875749Z"},"links":{"cited_paper":"/paper/2005.01880","citing_paper":"/paper/2411.14930"},"observation_digest":"sha256:71e8697d0fe45ea6891d0fdc643f8894955a7a59e93ba03b90b97e160c26911a","observation_id":"48a70c58-5602-4b0b-91e0-a54dfef3e612","resolution":{"observed_at":"2026-08-12T14:48:39.875749Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2306.04711","last_updated":"2023-08-03T19:36:26Z","snapshot_observed_at":"2026-08-16T15:25:43.190741Z","submitted_at":"2023-06-07T18:23:02Z","title":"Multimessenger Emission from the Accretion Induced Collapse of White Dwarfs","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2306.04711","snapshot_observed_at":"2026-08-12T14:48:39.880455Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2411.14930","last_updated":"2025-04-02T10:48:19Z","snapshot_observed_at":"2026-08-17T16:07:02.156639Z","submitted_at":"2024-11-22T13:39:01Z","title":"Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state","version":2},"reference_index":56,"source":"pdf_text","source_observed_at":"2026-08-12T14:48:39.880455Z"},"links":{"cited_paper":"/paper/2306.04711","citing_paper":"/paper/2411.14930"},"observation_digest":"sha256:0923d4159914b0baef31b3ae6e06049cbde61b76e44836a8afe7754718ddf927","observation_id":"471ed481-24ae-4dc9-904b-3c7335481227","resolution":{"observed_at":"2026-08-12T14:48:39.880455Z","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":"2026-08-12T14:48:39.884595Z","title":null,"venue":null,"work_id":null,"year":1930},"citing_paper":{"arxiv_id":"2411.14930","last_updated":"2025-04-02T10:48:19Z","snapshot_observed_at":"2026-08-17T16:07:02.156639Z","submitted_at":"2024-11-22T13:39:01Z","title":"Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state","version":2},"reference_index":57,"source":"pdf_text","source_observed_at":"2026-08-12T14:48:39.884595Z"},"links":{"citing_paper":"/paper/2411.14930"},"observation_digest":"sha256:2dc40b5b1a16430dde36176cc92a16eec9fde341180ff6c72ad1ff94e7a0a7c0","observation_id":"11f78fc8-8810-4c87-b647-6601faaa04d9","resolution":{"observed_at":"2026-08-12T14:48:39.884595Z","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":"2026-08-12T14:48:39.888737Z","title":"Tolman and P","venue":null,"work_id":null,"year":1930},"citing_paper":{"arxiv_id":"2411.14930","last_updated":"2025-04-02T10:48:19Z","snapshot_observed_at":"2026-08-17T16:07:02.156639Z","submitted_at":"2024-11-22T13:39:01Z","title":"Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state","version":2},"reference_index":58,"source":"pdf_text","source_observed_at":"2026-08-12T14:48:39.888737Z"},"links":{"citing_paper":"/paper/2411.14930"},"observation_digest":"sha256:e74190c84e9e9fab90deb89f2318d6538740168868d930ef411a8bf104322e54","observation_id":"b187d420-1360-4090-abfa-152ecb15ec72","resolution":{"observed_at":"2026-08-12T14:48:39.888737Z","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":"2026-08-12T14:48:41.737344Z","title":"Klein, Reviews of Modern Physics 21, 531 (1949)","venue":null,"work_id":"83f4a685-a1a8-4286-a28f-68307198a08c","year":1949},"citing_paper":{"arxiv_id":"2411.14930","last_updated":"2025-04-02T10:48:19Z","snapshot_observed_at":"2026-08-17T16:07:02.156639Z","submitted_at":"2024-11-22T13:39:01Z","title":"Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state","version":2},"reference_index":59,"source":"pdf_text","source_observed_at":"2026-08-12T14:48:39.892554Z"},"links":{"citing_paper":"/paper/2411.14930"},"observation_digest":"sha256:786a953d9e2225bba4e5271d033d25c8c512a2b4b5f43dd41c47a38a8f0ebbe1","observation_id":"b542c2cd-65db-435d-871f-af9b60e02794","resolution":{"observed_at":"2026-08-12T14:48:41.742474Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1911.09060","last_updated":"2019-11-23T17:53:43Z","snapshot_observed_at":"2026-08-12T19:34:21.106619Z","submitted_at":"2019-11-20T17:44:36Z","title":"Thermodynamic Equilibrium in General Relativity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1911.09060","snapshot_observed_at":"2026-08-12T14:48:39.896975Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2411.14930","last_updated":"2025-04-02T10:48:19Z","snapshot_observed_at":"2026-08-17T16:07:02.156639Z","submitted_at":"2024-11-22T13:39:01Z","title":"Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state","version":2},"reference_index":60,"source":"pdf_text","source_observed_at":"2026-08-12T14:48:39.896975Z"},"links":{"cited_paper":"/paper/1911.09060","citing_paper":"/paper/2411.14930"},"observation_digest":"sha256:dcc55e82693d9a674192e9b0c862051e6b3d354b2a321b3bc99ea0fa3efdc925","observation_id":"0ff211e5-6f98-4378-ade9-56a989fad9cd","resolution":{"observed_at":"2026-08-12T14:48:39.896975Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1706.02913","last_updated":"2017-10-04T13:39:38Z","snapshot_observed_at":"2026-08-14T20:55:05.055120Z","submitted_at":"2017-06-09T12:03:46Z","title":"A new temperature dependent hyperonic equation of state: application to rotating neutron star models and I-Q-relations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1706.02913","snapshot_observed_at":"2026-08-12T14:48:39.901830Z","title":"Marques, M","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2411.14930","last_updated":"2025-04-02T10:48:19Z","snapshot_observed_at":"2026-08-17T16:07:02.156639Z","submitted_at":"2024-11-22T13:39:01Z","title":"Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state","version":2},"reference_index":61,"source":"pdf_text","source_observed_at":"2026-08-12T14:48:39.901830Z"},"links":{"cited_paper":"/paper/1706.02913","citing_paper":"/paper/2411.14930"},"observation_digest":"sha256:d6206a53c9dc4ae83c8cff9997709410d373654cd4a04fea8b6265cb1949e22d","observation_id":"241407b3-7bbc-4ce8-b81b-8f19bad07cec","resolution":{"observed_at":"2026-08-12T14:48:39.901830Z","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/9610265","doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-12T14:48:40.237210Z","title":"Goussard, P","venue":null,"work_id":"2b31bbf6-93d0-4ee9-bf1d-6d11385851d8","year":1997},"citing_paper":{"arxiv_id":"2411.14930","last_updated":"2025-04-02T10:48:19Z","snapshot_observed_at":"2026-08-17T16:07:02.156639Z","submitted_at":"2024-11-22T13:39:01Z","title":"Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state","version":2},"reference_index":62,"source":"pdf_text","source_observed_at":"2026-08-12T14:48:39.906564Z"},"links":{"citing_paper":"/paper/2411.14930"},"observation_digest":"sha256:4ffba03a0a6a78f7c892f7940741eac4b2f9fb73c5bc0e9439cf1a8a7c103baa","observation_id":"f772cbd7-db97-42d2-b4da-e6bb9bc0bcfe","resolution":{"observed_at":"2026-08-12T14:48:40.246074Z","resolver_source":"raw_fallback","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+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":"2026-08-12T14:48:41.722856Z","title":"Keil and H","venue":null,"work_id":"72c9dcbb-a393-493a-9feb-cdb98910e7ea","year":1995},"citing_paper":{"arxiv_id":"2411.14930","last_updated":"2025-04-02T10:48:19Z","snapshot_observed_at":"2026-08-17T16:07:02.156639Z","submitted_at":"2024-11-22T13:39:01Z","title":"Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state","version":2},"reference_index":63,"source":"pdf_text","source_observed_at":"2026-08-12T14:48:39.911146Z"},"links":{"citing_paper":"/paper/2411.14930"},"observation_digest":"sha256:dd33683f9f1bdd0f7831801920812ec62fb8933c7546dc7ed1e64b81cc9a38ec","observation_id":"25bd8d13-e3aa-49e2-8755-e0d44635e9e1","resolution":{"observed_at":"2026-08-12T14:48:41.727070Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+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":"2026-08-12T14:48:41.706669Z","title":"Prakash, J","venue":null,"work_id":"a5ede874-c2f9-40f8-8e1a-372f3c79542b","year":1995},"citing_paper":{"arxiv_id":"2411.14930","last_updated":"2025-04-02T10:48:19Z","snapshot_observed_at":"2026-08-17T16:07:02.156639Z","submitted_at":"2024-11-22T13:39:01Z","title":"Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state","version":2},"reference_index":64,"source":"pdf_text","source_observed_at":"2026-08-12T14:48:39.915500Z"},"links":{"citing_paper":"/paper/2411.14930"},"observation_digest":"sha256:3e674c5cdaba9a806c846017b040c74a92324a0631e16e5b69ce4f900d306423","observation_id":"3ecd46ac-aaf6-41da-85b1-fbb046e9fe19","resolution":{"observed_at":"2026-08-12T14:48:41.711900Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+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":"2026-08-12T14:48:41.643376Z","title":null,"venue":null,"work_id":"acded6de-966d-4082-980d-96649da91bb1","year":1995},"citing_paper":{"arxiv_id":"2411.14930","last_updated":"2025-04-02T10:48:19Z","snapshot_observed_at":"2026-08-17T16:07:02.156639Z","submitted_at":"2024-11-22T13:39:01Z","title":"Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state","version":2},"reference_index":65,"source":"pdf_text","source_observed_at":"2026-08-12T14:48:39.919951Z"},"links":{"citing_paper":"/paper/2411.14930"},"observation_digest":"sha256:58e25ac47514038a7cc2ca2fb5ded2cd5ff2975e27362453151408025d881e99","observation_id":"bf07ceff-d0d7-4863-af91-d64ffa84405c","resolution":{"observed_at":"2026-08-12T14:48:41.694883Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+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":"2026-08-12T14:48:41.532309Z","title":null,"venue":null,"work_id":"90b0ef6b-5d15-434f-9fc6-41399b7f33f3","year":1996},"citing_paper":{"arxiv_id":"2411.14930","last_updated":"2025-04-02T10:48:19Z","snapshot_observed_at":"2026-08-17T16:07:02.156639Z","submitted_at":"2024-11-22T13:39:01Z","title":"Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state","version":2},"reference_index":66,"source":"pdf_text","source_observed_at":"2026-08-12T14:48:39.924536Z"},"links":{"citing_paper":"/paper/2411.14930"},"observation_digest":"sha256:6d8c48efe62b57816a7dc7c9dc4438fc58561e6c5e5657ba2b0c7c096f189990","observation_id":"cabe3c65-6aba-402d-82f8-bcda3806c535","resolution":{"observed_at":"2026-08-12T14:48:41.578867Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+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":"2026-08-12T14:48:41.513375Z","title":null,"venue":null,"work_id":"dd4336c3-7618-4534-b87b-f8c9ec821494","year":1966},"citing_paper":{"arxiv_id":"2411.14930","last_updated":"2025-04-02T10:48:19Z","snapshot_observed_at":"2026-08-17T16:07:02.156639Z","submitted_at":"2024-11-22T13:39:01Z","title":"Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state","version":2},"reference_index":67,"source":"pdf_text","source_observed_at":"2026-08-12T14:48:39.929082Z"},"links":{"citing_paper":"/paper/2411.14930"},"observation_digest":"sha256:9c39dbcd0dc4500cf89e1fc78c13e054004420d130a33742fde0990358d155d9","observation_id":"d43fc115-7d89-4db1-baa2-4dbb493d5568","resolution":{"observed_at":"2026-08-12T14:48:41.517994Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+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":"2026-08-12T14:48:41.498582Z","title":null,"venue":null,"work_id":"a827ddb9-4911-4c00-b5e8-72b014af64a9","year":1968},"citing_paper":{"arxiv_id":"2411.14930","last_updated":"2025-04-02T10:48:19Z","snapshot_observed_at":"2026-08-17T16:07:02.156639Z","submitted_at":"2024-11-22T13:39:01Z","title":"Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state","version":2},"reference_index":68,"source":"pdf_text","source_observed_at":"2026-08-12T14:48:39.933545Z"},"links":{"citing_paper":"/paper/2411.14930"},"observation_digest":"sha256:7d644480e4686ebbd0af5de3680ce9fb45ace296517f724f05ee49cd911c5c39","observation_id":"dae236d2-991d-4193-8e73-38d33db55a33","resolution":{"observed_at":"2026-08-12T14:48:41.503813Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+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":"2026-08-12T14:48:41.484849Z","title":"Kampfer, J","venue":null,"work_id":"5e87f214-b0d7-4988-bb2c-e43fb1f79b90","year":1981},"citing_paper":{"arxiv_id":"2411.14930","last_updated":"2025-04-02T10:48:19Z","snapshot_observed_at":"2026-08-17T16:07:02.156639Z","submitted_at":"2024-11-22T13:39:01Z","title":"Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state","version":2},"reference_index":69,"source":"pdf_text","source_observed_at":"2026-08-12T14:48:39.937966Z"},"links":{"citing_paper":"/paper/2411.14930"},"observation_digest":"sha256:909c8a07f1e8e2de544e443be9200c32b46736350aba3d6ae222b78cdc5b48b0","observation_id":"9535502e-0e94-44df-9bf3-755909f9582c","resolution":{"observed_at":"2026-08-12T14:48:41.488902Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9807155","last_updated":"1998-10-22T19:43:44Z","snapshot_observed_at":"2026-08-20T01:22:21.129419Z","submitted_at":"1998-07-15T16:14:13Z","title":"Non-Identical Neutron Star Twins","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9807155","snapshot_observed_at":"2026-08-12T14:48:39.942790Z","title":null,"venue":null,"work_id":null,"year":2000},"citing_paper":{"arxiv_id":"2411.14930","last_updated":"2025-04-02T10:48:19Z","snapshot_observed_at":"2026-08-17T16:07:02.156639Z","submitted_at":"2024-11-22T13:39:01Z","title":"Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state","version":2},"reference_index":70,"source":"pdf_text","source_observed_at":"2026-08-12T14:48:39.942790Z"},"links":{"cited_paper":"/paper/astro-ph/9807155","citing_paper":"/paper/2411.14930"},"observation_digest":"sha256:a5a7244faa1e520dc8817fad6bb6c46beee69dd33837a999a6f2a19e0263d0da","observation_id":"0557b78c-6818-4b7c-8155-4ec2695a12ec","resolution":{"observed_at":"2026-08-12T14:48:39.942790Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0001467","last_updated":"2000-01-26T20:43:12Z","snapshot_observed_at":"2026-07-07T00:09:41.792896Z","submitted_at":"2000-01-26T20:43:12Z","title":"Quark phases in neutron stars and a \"third family\" of compact stars as a signature for phase transitions","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0001467","snapshot_observed_at":"2026-08-12T14:48:39.947665Z","title":"Schertler, C","venue":null,"work_id":null,"year":2000},"citing_paper":{"arxiv_id":"2411.14930","last_updated":"2025-04-02T10:48:19Z","snapshot_observed_at":"2026-08-17T16:07:02.156639Z","submitted_at":"2024-11-22T13:39:01Z","title":"Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state","version":2},"reference_index":71,"source":"pdf_text","source_observed_at":"2026-08-12T14:48:39.947665Z"},"links":{"cited_paper":"/paper/astro-ph/0001467","citing_paper":"/paper/2411.14930"},"observation_digest":"sha256:c446d24326bd5a5815da606d92169e2496790ea2d51e343ba834080360a1f5f2","observation_id":"a0645001-5f0e-4e9c-b039-48e808fabc88","resolution":{"observed_at":"2026-08-12T14:48:39.947665Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1612.06167","last_updated":"2016-12-19T13:17:27Z","snapshot_observed_at":"2026-08-14T21:24:46.905238Z","submitted_at":"2016-12-19T13:17:27Z","title":"Twin Stars within the SU(3) Chiral Quark-Meson Model","version":1},"cited_work":{"arxiv_id":"1612.06167","doi":null,"metadata_source":"pith","pith_arxiv_id":"1612.06167","snapshot_observed_at":"2026-08-12T14:48:40.124045Z","title":"Twin Stars within the SU(3) Chiral Quark-Meson Model","venue":"astro-ph.HE","work_id":"603df848-9f74-4a2a-927e-176fd59f45e9","year":2016},"citing_paper":{"arxiv_id":"2411.14930","last_updated":"2025-04-02T10:48:19Z","snapshot_observed_at":"2026-08-17T16:07:02.156639Z","submitted_at":"2024-11-22T13:39:01Z","title":"Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state","version":2},"reference_index":72,"source":"pdf_text","source_observed_at":"2026-08-12T14:48:39.952465Z"},"links":{"cited_paper":"/paper/1612.06167","citing_paper":"/paper/2411.14930"},"observation_digest":"sha256:2389596270a705e278882d45a1039b50c40d4790df9d62c1bf965745fa6db46e","observation_id":"a8e08668-66e4-4296-be93-5203ed6bb27f","resolution":{"observed_at":"2026-08-12T14:48:40.128928Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1707.07524","last_updated":"2017-07-24T12:49:14Z","snapshot_observed_at":"2026-08-19T19:10:55.116226Z","submitted_at":"2017-07-24T12:49:14Z","title":"Classifications of Twin Star Solutions for a Constant Speed of Sound Parameterized Equation of State","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1707.07524","snapshot_observed_at":"2026-08-12T14:48:39.957220Z","title":"Christian, A","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2411.14930","last_updated":"2025-04-02T10:48:19Z","snapshot_observed_at":"2026-08-17T16:07:02.156639Z","submitted_at":"2024-11-22T13:39:01Z","title":"Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state","version":2},"reference_index":73,"source":"pdf_text","source_observed_at":"2026-08-12T14:48:39.957220Z"},"links":{"cited_paper":"/paper/1707.07524","citing_paper":"/paper/2411.14930"},"observation_digest":"sha256:422711906664a2c858728abb03351b55a63ff486b423276285482f7bffecd2aa","observation_id":"21e25015-a89c-480c-8fbf-eec1e76dfa67","resolution":{"observed_at":"2026-08-12T14:48:39.957220Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0005490","last_updated":"2002-09-19T21:10:48Z","snapshot_observed_at":"2026-08-10T10:14:01.862496Z","submitted_at":"2000-05-24T17:24:54Z","title":"Phase Transition to Hyperon Matter in Neutron Stars","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0005490","snapshot_observed_at":"2026-08-12T14:48:39.962435Z","title":"Schaffner-Bielich, M","venue":null,"work_id":null,"year":2002},"citing_paper":{"arxiv_id":"2411.14930","last_updated":"2025-04-02T10:48:19Z","snapshot_observed_at":"2026-08-17T16:07:02.156639Z","submitted_at":"2024-11-22T13:39:01Z","title":"Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state","version":2},"reference_index":74,"source":"pdf_text","source_observed_at":"2026-08-12T14:48:39.962435Z"},"links":{"cited_paper":"/paper/astro-ph/0005490","citing_paper":"/paper/2411.14930"},"observation_digest":"sha256:bcef94c7693471ee6a970cc1f7278b63915caea26c07cd2817ecbf5458591d75","observation_id":"51a165d6-1815-4150-9c89-4b488be6c318","resolution":{"observed_at":"2026-08-12T14:48:39.962435Z","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":"2026-08-12T14:48:41.470513Z","title":"Chabanat, J","venue":null,"work_id":"873554d6-a721-4d63-b4b9-8455fd419def","year":1997},"citing_paper":{"arxiv_id":"2411.14930","last_updated":"2025-04-02T10:48:19Z","snapshot_observed_at":"2026-08-17T16:07:02.156639Z","submitted_at":"2024-11-22T13:39:01Z","title":"Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state","version":2},"reference_index":75,"source":"pdf_text","source_observed_at":"2026-08-12T14:48:39.967244Z"},"links":{"citing_paper":"/paper/2411.14930"},"observation_digest":"sha256:9febfee1c43b4ab0dedd56a90a82a30140c6a3acc164f3edf7cace2914409cc0","observation_id":"8c3a60e4-59fb-4a74-80f8-ab82b8a9199a","resolution":{"observed_at":"2026-08-12T14:48:41.474949Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"0907.2680","last_updated":"2009-07-15T18:49:03Z","snapshot_observed_at":"2026-08-18T11:13:06.432090Z","submitted_at":"2009-07-15T18:49:03Z","title":"Conditions for Phase Equilibrium in Supernovae, Proto-Neutron and Neutron Stars","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0907.2680","snapshot_observed_at":"2026-08-12T14:48:39.971866Z","title":"Hempel, G","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2411.14930","last_updated":"2025-04-02T10:48:19Z","snapshot_observed_at":"2026-08-17T16:07:02.156639Z","submitted_at":"2024-11-22T13:39:01Z","title":"Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state","version":2},"reference_index":76,"source":"pdf_text","source_observed_at":"2026-08-12T14:48:39.971866Z"},"links":{"cited_paper":"/paper/0907.2680","citing_paper":"/paper/2411.14930"},"observation_digest":"sha256:f5adac959d11aacefda826420f3e0df82e0c3db229cf7350b9e168407b88607f","observation_id":"9f0677df-f4ed-45ab-9eea-c35c5897e7e5","resolution":{"observed_at":"2026-08-12T14:48:39.971866Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0907.3075","last_updated":"2009-07-17T13:44:25Z","snapshot_observed_at":"2026-08-15T05:43:27.337323Z","submitted_at":"2009-07-17T13:44:25Z","title":"A new possible quark-hadron mixed phase in protoneutron stars","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0907.3075","snapshot_observed_at":"2026-08-12T14:48:39.976765Z","title":"Pagliara, M","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2411.14930","last_updated":"2025-04-02T10:48:19Z","snapshot_observed_at":"2026-08-17T16:07:02.156639Z","submitted_at":"2024-11-22T13:39:01Z","title":"Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state","version":2},"reference_index":77,"source":"pdf_text","source_observed_at":"2026-08-12T14:48:39.976765Z"},"links":{"cited_paper":"/paper/0907.3075","citing_paper":"/paper/2411.14930"},"observation_digest":"sha256:dc747212ced8b33da208b02f770687347b6981f82bef9a226df41ef9eb20c6c6","observation_id":"31ef2cdd-eb5d-4455-9528-d535eb65681b","resolution":{"observed_at":"2026-08-12T14:48:39.976765Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1511.06551","last_updated":"2016-11-11T15:25:33Z","snapshot_observed_at":"2026-08-14T22:22:04.249529Z","submitted_at":"2015-11-20T10:36:16Z","title":"Hot third family of compact stars and the possibility of core-collapse supernova explosions","version":2},"cited_work":{"arxiv_id":"1511.06551","doi":null,"metadata_source":"pith","pith_arxiv_id":"1511.06551","snapshot_observed_at":"2026-08-12T14:48:40.040488Z","title":"Hot third family of compact stars and the possibility of core-collapse supernova explosions","venue":"nucl-th","work_id":"b3114c54-d849-495f-b051-688552afc796","year":2015},"citing_paper":{"arxiv_id":"2411.14930","last_updated":"2025-04-02T10:48:19Z","snapshot_observed_at":"2026-08-17T16:07:02.156639Z","submitted_at":"2024-11-22T13:39:01Z","title":"Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state","version":2},"reference_index":78,"source":"pdf_text","source_observed_at":"2026-08-12T14:48:39.981339Z"},"links":{"cited_paper":"/paper/1511.06551","citing_paper":"/paper/2411.14930"},"observation_digest":"sha256:7a2dff87a5f7d68a15e2863f01896d58179b86bd523331430cd4112dbaf1d4e4","observation_id":"1d723bca-f28c-44e5-b9e3-f8ec9179290a","resolution":{"observed_at":"2026-08-12T14:48:40.046932Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2312.01975","last_updated":"2024-03-01T13:25:32Z","snapshot_observed_at":"2026-08-16T14:37:49.687624Z","submitted_at":"2023-12-04T15:43:43Z","title":"Thermal twin stars within a hybrid equation of state based on a nonlocal chiral quark model compatible with modern astrophysical observations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2312.01975","snapshot_observed_at":"2026-08-12T14:48:39.985824Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2411.14930","last_updated":"2025-04-02T10:48:19Z","snapshot_observed_at":"2026-08-17T16:07:02.156639Z","submitted_at":"2024-11-22T13:39:01Z","title":"Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state","version":2},"reference_index":79,"source":"pdf_text","source_observed_at":"2026-08-12T14:48:39.985824Z"},"links":{"cited_paper":"/paper/2312.01975","citing_paper":"/paper/2411.14930"},"observation_digest":"sha256:cd8f28e560de3760096b985b44ccf1a5f17895b648313dcba6cf50064dd77589","observation_id":"1c47bb8d-4575-400a-9e41-4c94448da071","resolution":{"observed_at":"2026-08-12T14:48:39.985824Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"2411.14930","last_updated":"2025-04-02T10:48:19Z","latest_version":2,"primary_category":"nucl-th","snapshot_observed_at":"2026-08-17T16:07:02.156639Z","submitted_at":"2024-11-22T13:39:01Z","title":"Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state"},"reference_resolution":{"displayed":79,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":59,"verified_exact":11,"verified_fuzzy":9},"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":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"thesis":"As of 21 August 2026, this Paper Citation Record lists 79 of 79 outbound references and 3 inbound Pith citation observations for arXiv:2411.14930."}