{"as_of":"2026-08-07T19:37:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:7c4335dec57b9885e00dd12e8d255d9954563cab69e8fd86492f66ed5a9952d4","coverage":[{"denominator":67,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":67,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-06T16:29:19.198119Z","state":"measured"},{"denominator":69,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":69,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-07T06:34:17.273281+00:00","state":"measured"},{"denominator":2,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":2,"source":"paper_references, paper_reference_links","source_observed_at":"2026-05-09T23:09:39.154108Z","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":"2026-05-12T00:01:13.950102Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2507.13429","last_updated":"2025-09-03T15:30:02Z","snapshot_observed_at":"2026-08-07T09:33:37.858372Z","submitted_at":"2025-07-17T18:00:00Z","title":"Electron-neutrino lepton number crossings: Variations with the supernova core physics","version":2},"cited_work":{"arxiv_id":"2507.13429","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2507.13429","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Cornelius, I","venue":null,"work_id":"54346459-df73-4929-9cfd-c9548494a8a6","year":2025},"citing_paper":{"arxiv_id":"2604.21081","last_updated":"2026-04-24T18:33:29Z","snapshot_observed_at":"2026-08-02T17:34:31.644360Z","submitted_at":"2026-04-22T20:47:33Z","title":"An Analytic Threshold for LESA-Driven Negative ELN Flux Directions in Core-Collapse Supernovae: Derivation and Population Census","version":2},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-05-09T23:09:39.154108Z"},"links":{"cited_paper":"/paper/2507.13429","citing_paper":"/paper/2604.21081"},"observation_digest":"sha256:857ee9329d61a1f414c8452a6cf118885f9c9899c1f6635d09bbfe150d26daea","observation_id":"db7538ac-3be3-4594-b723-5acf3904464c","resolution":{"observed_at":"2026-05-11T14:16:04.250051Z","resolver_source":"arxiv_id","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2507.13429","last_updated":"2025-09-03T15:30:02Z","snapshot_observed_at":"2026-08-07T09:33:37.858372Z","submitted_at":"2025-07-17T18:00:00Z","title":"Electron-neutrino lepton number crossings: Variations with the supernova core physics","version":2},"cited_work":{"arxiv_id":"2507.13429","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2507.13429","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Cornelius, I","venue":null,"work_id":"54346459-df73-4929-9cfd-c9548494a8a6","year":2025},"citing_paper":{"arxiv_id":"2604.25687","last_updated":"2026-04-28T14:18:05Z","snapshot_observed_at":"2026-07-06T23:11:30.068819Z","submitted_at":"2026-04-28T14:18:05Z","title":"Collective neutrino-antineutrino pair oscillations","version":1},"reference_index":86,"source":"pdf_text","source_observed_at":"2026-05-07T15:58:06.378902Z"},"links":{"cited_paper":"/paper/2507.13429","citing_paper":"/paper/2604.25687"},"observation_digest":"sha256:2c3e27a16c70364671c21c10989fb57e7281f45632cd8672547b59c0fc1b43a9","observation_id":"513d30ed-d287-4940-ab1b-49a1c1776fea","resolution":{"observed_at":"2026-05-12T00:01:13.954868Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/2507.13429/citation-record","integrity":"/paper/2507.13429/integrity","json":"/paper/2507.13429/citation-record.json","paper":"/paper/2507.13429"},"outbound":[{"citation":{"cited_paper":{"arxiv_id":"2009.14157","last_updated":"2021-01-20T17:38:51Z","snapshot_observed_at":"2026-08-06T11:16:23.762101Z","submitted_at":"2020-09-29T17:07:40Z","title":"Core-Collapse Supernova Explosion Theory","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2009.14157","snapshot_observed_at":"2026-08-06T16:29:10.052930Z","title":"Burrows and D","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2507.13429","last_updated":"2025-09-03T15:30:02Z","snapshot_observed_at":"2026-08-07T09:33:37.858372Z","submitted_at":"2025-07-17T18:00:00Z","title":"Electron-neutrino lepton number crossings: Variations with the supernova core physics","version":2},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-06T16:29:10.052930Z"},"links":{"cited_paper":"/paper/2009.14157","citing_paper":"/paper/2507.13429"},"observation_digest":"sha256:a6ce49325b5bbb5cdf020fba955e3f19e40a8f5c480a851775ffd5421b8662b6","observation_id":"10c15729-3519-4e79-907c-47d321dc537d","resolution":{"observed_at":"2026-08-06T16:29:10.052930Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2412.09699","last_updated":"2025-06-02T07:23:00Z","snapshot_observed_at":"2026-07-06T20:06:13.565435Z","submitted_at":"2024-12-12T19:38:31Z","title":"Neutrinos from explosive transients at the dawn of multi-messenger astronomy","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2412.09699","snapshot_observed_at":"2026-08-06T16:29:10.196872Z","title":"Tamborra, Neutrinos from explosive transients at the dawn of multi-messenger astronomy, Nature Rev","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2507.13429","last_updated":"2025-09-03T15:30:02Z","snapshot_observed_at":"2026-08-07T09:33:37.858372Z","submitted_at":"2025-07-17T18:00:00Z","title":"Electron-neutrino lepton number crossings: Variations with the supernova core physics","version":2},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-06T16:29:10.196872Z"},"links":{"cited_paper":"/paper/2412.09699","citing_paper":"/paper/2507.13429"},"observation_digest":"sha256:f9b17df3258715dc430a06e8a3ad08ce666f6879d2fa545eb160560908216745","observation_id":"910c6016-64d8-4410-8040-7b0d7ae70d0e","resolution":{"observed_at":"2026-08-06T16:29:10.196872Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1910.11878","last_updated":"2020-12-10T15:31:16Z","snapshot_observed_at":"2026-07-06T08:32:20.422044Z","submitted_at":"2019-10-25T18:00:02Z","title":"Grand Unified Neutrino Spectrum at Earth: Sources and Spectral Components","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1910.11878","snapshot_observed_at":"2026-08-06T16:29:10.306944Z","title":"Vitagliano, I","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2507.13429","last_updated":"2025-09-03T15:30:02Z","snapshot_observed_at":"2026-08-07T09:33:37.858372Z","submitted_at":"2025-07-17T18:00:00Z","title":"Electron-neutrino lepton number crossings: Variations with the supernova core physics","version":2},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-06T16:29:10.306944Z"},"links":{"cited_paper":"/paper/1910.11878","citing_paper":"/paper/2507.13429"},"observation_digest":"sha256:d2e389a3af627671e0283e8c18acd37936f59a062cf3cc1c4d925803da50a5d2","observation_id":"c6800bf0-d19d-4b04-9d24-ef02257ddb79","resolution":{"observed_at":"2026-08-06T16:29:10.306944Z","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":"2026-08-06T16:29:10.438163Z","title":"Janka, Long-Term Multidimensional Models of Core-Collapse Supernovae: Progress and Challenges (2025), arXiv:2502.14836 [astro-ph.HE]","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2507.13429","last_updated":"2025-09-03T15:30:02Z","snapshot_observed_at":"2026-08-07T09:33:37.858372Z","submitted_at":"2025-07-17T18:00:00Z","title":"Electron-neutrino lepton number crossings: Variations with the supernova core physics","version":2},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-06T16:29:10.438163Z"},"links":{"citing_paper":"/paper/2507.13429"},"observation_digest":"sha256:b4a44585c9cad6075435db4ee78d72d661d5fc36ae0c3c21c474140bf5115441","observation_id":"b29cb31a-a940-4161-9ab8-be54399b0388","resolution":{"observed_at":"2026-08-06T16:29:10.438163Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1611.05859","last_updated":"2018-01-26T20:32:55Z","snapshot_observed_at":"2026-08-07T15:32:07.324339Z","submitted_at":"2016-11-17T20:59:59Z","title":"Crucial Physical Dependencies of the Core-Collapse Supernova Mechanism","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1611.05859","snapshot_observed_at":"2026-08-06T16:29:10.631374Z","title":"Burrows, D","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2507.13429","last_updated":"2025-09-03T15:30:02Z","snapshot_observed_at":"2026-08-07T09:33:37.858372Z","submitted_at":"2025-07-17T18:00:00Z","title":"Electron-neutrino lepton number crossings: Variations with the supernova core physics","version":2},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-06T16:29:10.631374Z"},"links":{"cited_paper":"/paper/1611.05859","citing_paper":"/paper/2507.13429"},"observation_digest":"sha256:4e3c96950a3a5d0e4af5f754b3e3efa70c4fc9212b7263c2088abc1db1a2e1eb","observation_id":"c94bae55-76f9-4385-a500-73f284d21fc7","resolution":{"observed_at":"2026-08-06T16:29:10.631374Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2010.09013","last_updated":"2020-10-18T16:03:48Z","snapshot_observed_at":"2026-07-06T10:05:29.439402Z","submitted_at":"2020-10-18T16:03:48Z","title":"Physical, numerical, and computational challenges of modeling neutrino transport in core-collapse supernovae","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2010.09013","snapshot_observed_at":"2026-08-06T16:29:10.752525Z","title":"Mezzacappa, E","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2507.13429","last_updated":"2025-09-03T15:30:02Z","snapshot_observed_at":"2026-08-07T09:33:37.858372Z","submitted_at":"2025-07-17T18:00:00Z","title":"Electron-neutrino lepton number crossings: Variations with the supernova core physics","version":2},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-06T16:29:10.752525Z"},"links":{"cited_paper":"/paper/2010.09013","citing_paper":"/paper/2507.13429"},"observation_digest":"sha256:b04e823bd83116e27b68e945e0742d0dff1c29df5784694afdbf31812d6dfe71","observation_id":"983c7231-d6d7-4de7-88d6-81ccc1e6e59e","resolution":{"observed_at":"2026-08-06T16:29:10.752525Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2011.01948","last_updated":"2021-01-13T08:21:02Z","snapshot_observed_at":"2026-07-06T10:11:26.758341Z","submitted_at":"2020-11-03T19:00:04Z","title":"New Developments in Flavor Evolution of a Dense Neutrino Gas","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2011.01948","snapshot_observed_at":"2026-08-06T16:29:10.888462Z","title":"Tamborra and S","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2507.13429","last_updated":"2025-09-03T15:30:02Z","snapshot_observed_at":"2026-08-07T09:33:37.858372Z","submitted_at":"2025-07-17T18:00:00Z","title":"Electron-neutrino lepton number crossings: Variations with the supernova core physics","version":2},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-06T16:29:10.888462Z"},"links":{"cited_paper":"/paper/2011.01948","citing_paper":"/paper/2507.13429"},"observation_digest":"sha256:1a77d4bedf3f89a87b4c14b51e3d101369a165088b2a3e6a456cd615aa177c50","observation_id":"c20a5b54-d335-4db6-904a-e37071a8237f","resolution":{"observed_at":"2026-08-06T16:29:10.888462Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2301.11814","last_updated":"2024-10-10T08:14:47Z","snapshot_observed_at":"2026-08-04T22:49:23.565473Z","submitted_at":"2023-01-27T16:07:03Z","title":"Neutrinos from dense environments : Flavor mechanisms, theoretical approaches, observations, and new directions","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2301.11814","snapshot_observed_at":"2026-08-06T16:29:11.055507Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2507.13429","last_updated":"2025-09-03T15:30:02Z","snapshot_observed_at":"2026-08-07T09:33:37.858372Z","submitted_at":"2025-07-17T18:00:00Z","title":"Electron-neutrino lepton number crossings: Variations with the supernova core physics","version":2},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-06T16:29:11.055507Z"},"links":{"cited_paper":"/paper/2301.11814","citing_paper":"/paper/2507.13429"},"observation_digest":"sha256:9c93d21e2cb742cb558f8c8cc567497f2f6d16b2bf3cbb4e6d3715e10807afe9","observation_id":"3d2be127-db9a-4b3c-b642-f6994f84da7c","resolution":{"observed_at":"2026-08-06T16:29:11.055507Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2503.05959","last_updated":"2025-08-28T14:27:45Z","snapshot_observed_at":"2026-08-07T17:21:01.381506Z","submitted_at":"2025-03-07T21:54:01Z","title":"Neutrino Oscillations in Core-Collapse Supernovae and Neutron Star Mergers","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2503.05959","snapshot_observed_at":"2026-08-06T16:29:11.163601Z","title":"Johns, S","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2507.13429","last_updated":"2025-09-03T15:30:02Z","snapshot_observed_at":"2026-08-07T09:33:37.858372Z","submitted_at":"2025-07-17T18:00:00Z","title":"Electron-neutrino lepton number crossings: Variations with the supernova core physics","version":2},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-06T16:29:11.163601Z"},"links":{"cited_paper":"/paper/2503.05959","citing_paper":"/paper/2507.13429"},"observation_digest":"sha256:380968d26aa30af2f87090441f354d18c6971e8ab10e3ea3e21d76f076083193","observation_id":"1e98e6d8-7139-4c6a-8810-cc52168766f0","resolution":{"observed_at":"2026-08-06T16:29:11.163601Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2301.10785","last_updated":"2023-05-11T02:04:06Z","snapshot_observed_at":"2026-07-06T14:44:38.168186Z","submitted_at":"2023-01-25T19:00:04Z","title":"Roles of fast neutrino-flavor conversion on the neutrino-heating mechanism of core-collapse supernova","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2301.10785","snapshot_observed_at":"2026-08-06T16:29:11.258011Z","title":"Nagakura, Roles of Fast Neutrino-Flavor Conver- sion on the Neutrino-Heating Mechanism of Core- Collapse Supernova, Phys","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2507.13429","last_updated":"2025-09-03T15:30:02Z","snapshot_observed_at":"2026-08-07T09:33:37.858372Z","submitted_at":"2025-07-17T18:00:00Z","title":"Electron-neutrino lepton number crossings: Variations with the supernova core physics","version":2},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-06T16:29:11.258011Z"},"links":{"cited_paper":"/paper/2301.10785","citing_paper":"/paper/2507.13429"},"observation_digest":"sha256:b428b8506fa47ce7a99b188f4d0f9f88a030537198fe98543f0688db8aee8838","observation_id":"c2bb820f-5dca-487d-be30-956ed2935139","resolution":{"observed_at":"2026-08-06T16:29:11.258011Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2305.11207","last_updated":"2025-01-02T07:41:55Z","snapshot_observed_at":"2026-08-06T19:00:16.615204Z","submitted_at":"2023-05-18T18:00:00Z","title":"Fast Neutrino Flavor Conversions can Help and Hinder Neutrino-Driven Explosions","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2305.11207","snapshot_observed_at":"2026-08-06T16:29:11.382664Z","title":"Ehring, S","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2507.13429","last_updated":"2025-09-03T15:30:02Z","snapshot_observed_at":"2026-08-07T09:33:37.858372Z","submitted_at":"2025-07-17T18:00:00Z","title":"Electron-neutrino lepton number crossings: Variations with the supernova core physics","version":2},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-06T16:29:11.382664Z"},"links":{"cited_paper":"/paper/2305.11207","citing_paper":"/paper/2507.13429"},"observation_digest":"sha256:8391c17d2069172331b7b560095558c0d2423a97d57aec23b09cb257dad73d5c","observation_id":"8e76a3eb-04b3-407d-9c63-57349ff666e5","resolution":{"observed_at":"2026-08-06T16:29:11.382664Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2301.11938","last_updated":"2023-04-02T10:26:12Z","snapshot_observed_at":"2026-07-06T14:45:26.549421Z","submitted_at":"2023-01-27T19:00:00Z","title":"Fast Neutrino Flavor Conversion in Core-Collapse Supernovae: A Parametric Study in 1D Models","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2301.11938","snapshot_observed_at":"2026-08-06T16:29:11.530218Z","title":"Ehring, S","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2507.13429","last_updated":"2025-09-03T15:30:02Z","snapshot_observed_at":"2026-08-07T09:33:37.858372Z","submitted_at":"2025-07-17T18:00:00Z","title":"Electron-neutrino lepton number crossings: Variations with the supernova core physics","version":2},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-06T16:29:11.530218Z"},"links":{"cited_paper":"/paper/2301.11938","citing_paper":"/paper/2507.13429"},"observation_digest":"sha256:24172a0e3add34533ec76dd58239ef7e9db55932e76aded9d0aebf91aeb62b74","observation_id":"035c8853-7da3-42ab-a2b4-412d7ff694b4","resolution":{"observed_at":"2026-08-06T16:29:11.530218Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2501.15256","last_updated":"2025-03-04T05:03:37Z","snapshot_observed_at":"2026-07-06T20:26:07.715114Z","submitted_at":"2025-01-25T16:04:00Z","title":"Three-dimensional core-collapse supernova models with phenomenological treatment of neutrino flavor conversions","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2501.15256","snapshot_observed_at":"2026-08-06T16:29:11.631155Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2507.13429","last_updated":"2025-09-03T15:30:02Z","snapshot_observed_at":"2026-08-07T09:33:37.858372Z","submitted_at":"2025-07-17T18:00:00Z","title":"Electron-neutrino lepton number crossings: Variations with the supernova core physics","version":2},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-06T16:29:11.631155Z"},"links":{"cited_paper":"/paper/2501.15256","citing_paper":"/paper/2507.13429"},"observation_digest":"sha256:d9349b3eaddd0e52af394880b97d79c32d00f3451fba8c59497837a1dd14549c","observation_id":"66d0eb99-8e7c-422c-84cb-118a90299d08","resolution":{"observed_at":"2026-08-06T16:29:11.631155Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2503.04896","last_updated":"2025-05-13T04:37:57Z","snapshot_observed_at":"2026-08-07T17:23:45.385035Z","submitted_at":"2025-03-06T19:00:03Z","title":"The Effect of the Fast-Flavor Instability on Core-Collapse Supernova Models","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2503.04896","snapshot_observed_at":"2026-08-06T16:29:11.748471Z","title":"Wang and A","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2507.13429","last_updated":"2025-09-03T15:30:02Z","snapshot_observed_at":"2026-08-07T09:33:37.858372Z","submitted_at":"2025-07-17T18:00:00Z","title":"Electron-neutrino lepton number crossings: Variations with the supernova core physics","version":2},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-06T16:29:11.748471Z"},"links":{"cited_paper":"/paper/2503.04896","citing_paper":"/paper/2507.13429"},"observation_digest":"sha256:829d5309248b7893bad5dd1972eed9e95f750f89bd971bbfa065c48ebd78794a","observation_id":"b93a67a6-fc3b-4edf-aaf3-2d85918279df","resolution":{"observed_at":"2026-08-06T16:29:11.748471Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"hep-ph/0503013","last_updated":"2005-03-01T17:35:27Z","snapshot_observed_at":"2026-07-07T04:06:47.589680Z","submitted_at":"2005-03-01T17:35:27Z","title":"Speed-up of neutrino transformations in a supernova environment","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-ph/0503013","snapshot_observed_at":"2026-08-06T16:29:11.865834Z","title":null,"venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2507.13429","last_updated":"2025-09-03T15:30:02Z","snapshot_observed_at":"2026-08-07T09:33:37.858372Z","submitted_at":"2025-07-17T18:00:00Z","title":"Electron-neutrino lepton number crossings: Variations with the supernova core physics","version":2},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-06T16:29:11.865834Z"},"links":{"cited_paper":"/paper/hep-ph/0503013","citing_paper":"/paper/2507.13429"},"observation_digest":"sha256:196152b8d0c68ec8266ba3d80daefc7671576687c659f5639e0d3eaac5ac796c","observation_id":"d8147f57-f6de-4cd0-9b8a-717162b337ff","resolution":{"observed_at":"2026-08-06T16:29:11.865834Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1509.03323","last_updated":"2016-01-14T01:11:52Z","snapshot_observed_at":"2026-07-06T04:29:32.165102Z","submitted_at":"2015-09-10T20:10:05Z","title":"Neutrino cloud instabilities just above the neutrino sphere of a supernova","version":6},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1509.03323","snapshot_observed_at":"2026-08-06T16:29:11.975259Z","title":null,"venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2507.13429","last_updated":"2025-09-03T15:30:02Z","snapshot_observed_at":"2026-08-07T09:33:37.858372Z","submitted_at":"2025-07-17T18:00:00Z","title":"Electron-neutrino lepton number crossings: Variations with the supernova core physics","version":2},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-06T16:29:11.975259Z"},"links":{"cited_paper":"/paper/1509.03323","citing_paper":"/paper/2507.13429"},"observation_digest":"sha256:0c9da6288abfa025633de2e53b4233d7cb6958c9369a18bd2ad51bc92ef6a438","observation_id":"8dd1afdf-8e99-4f16-bbf6-e97cb27c317d","resolution":{"observed_at":"2026-08-06T16:29:11.975259Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1602.02766","last_updated":"2016-02-08T21:00:07Z","snapshot_observed_at":"2026-08-02T18:34:50.997907Z","submitted_at":"2016-02-08T21:00:07Z","title":"Collective neutrino flavor conversion: Recent developments","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1602.02766","snapshot_observed_at":"2026-08-06T16:29:12.134723Z","title":"Chakraborty, R","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2507.13429","last_updated":"2025-09-03T15:30:02Z","snapshot_observed_at":"2026-08-07T09:33:37.858372Z","submitted_at":"2025-07-17T18:00:00Z","title":"Electron-neutrino lepton number crossings: Variations with the supernova core physics","version":2},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-06T16:29:12.134723Z"},"links":{"cited_paper":"/paper/1602.02766","citing_paper":"/paper/2507.13429"},"observation_digest":"sha256:df64d9182024be8da2d3ca568289bfe4111026794492237326954b880e008232","observation_id":"aa3e53ef-8e40-4d59-b23a-31166b72da9d","resolution":{"observed_at":"2026-08-06T16:29:12.134723Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1602.00698","last_updated":"2016-03-24T16:28:09Z","snapshot_observed_at":"2026-07-06T04:44:47.916674Z","submitted_at":"2016-02-01T21:00:09Z","title":"Self-induced neutrino flavor conversion without flavor mixing","version":2},"cited_work":{"arxiv_id":"1602.00698","doi":null,"metadata_source":"pith","pith_arxiv_id":"1602.00698","snapshot_observed_at":"2026-08-06T16:29:21.830623Z","title":"Self-induced neutrino flavor conversion without flavor mixing","venue":"hep-ph","work_id":"14bc2c47-17cf-42f4-ab4f-07725500a89f","year":2016},"citing_paper":{"arxiv_id":"2507.13429","last_updated":"2025-09-03T15:30:02Z","snapshot_observed_at":"2026-08-07T09:33:37.858372Z","submitted_at":"2025-07-17T18:00:00Z","title":"Electron-neutrino lepton number crossings: Variations with the supernova core physics","version":2},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-06T16:29:12.295918Z"},"links":{"cited_paper":"/paper/1602.00698","citing_paper":"/paper/2507.13429"},"observation_digest":"sha256:76d96aba415c50b396d29c3cf044edb6f8ff7491530605db5d3d17bbd46e4a2e","observation_id":"d1c6c736-5cba-4ce9-92b6-7e94fa001568","resolution":{"observed_at":"2026-08-06T16:29:21.933022Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1610.01612","last_updated":"2017-01-11T10:19:08Z","snapshot_observed_at":"2026-08-07T10:54:32.618198Z","submitted_at":"2016-10-05T20:00:05Z","title":"Fast Pairwise Conversion of Supernova Neutrinos: A Dispersion-Relation Approach","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1610.01612","snapshot_observed_at":"2026-08-06T16:29:12.451492Z","title":"Izaguirre, G","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2507.13429","last_updated":"2025-09-03T15:30:02Z","snapshot_observed_at":"2026-08-07T09:33:37.858372Z","submitted_at":"2025-07-17T18:00:00Z","title":"Electron-neutrino lepton number crossings: Variations with the supernova core physics","version":2},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-06T16:29:12.451492Z"},"links":{"cited_paper":"/paper/1610.01612","citing_paper":"/paper/2507.13429"},"observation_digest":"sha256:bf36cf03cd8828bc7d7d94cd0712516e3d65c86c85074b517847e563628c0940","observation_id":"bbf23685-033f-49eb-9546-56753da810bc","resolution":{"observed_at":"2026-08-06T16:29:12.451492Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2103.15267","last_updated":"2022-03-28T23:50:50Z","snapshot_observed_at":"2026-07-06T10:54:11.548426Z","submitted_at":"2021-03-29T01:39:32Z","title":"Fast neutrino flavor instability and neutrino flavor lepton number crossings","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2103.15267","snapshot_observed_at":"2026-08-06T16:29:12.586994Z","title":"Morinaga, Fast neutrino flavor instability and neu- trino flavor lepton number crossings, Phys","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2507.13429","last_updated":"2025-09-03T15:30:02Z","snapshot_observed_at":"2026-08-07T09:33:37.858372Z","submitted_at":"2025-07-17T18:00:00Z","title":"Electron-neutrino lepton number crossings: Variations with the supernova core physics","version":2},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-06T16:29:12.586994Z"},"links":{"cited_paper":"/paper/2103.15267","citing_paper":"/paper/2507.13429"},"observation_digest":"sha256:a044e8a0179be55e0761ba2677623273e91ba05cb6e221dce977c424328c51f7","observation_id":"38f198a4-9be3-41c3-b86c-cf1b061ba084","resolution":{"observed_at":"2026-08-06T16:29:12.586994Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2109.14627","last_updated":"2022-11-07T19:10:00Z","snapshot_observed_at":"2026-07-06T11:52:46.440188Z","submitted_at":"2021-09-29T18:00:03Z","title":"Neutrino Flavor Pendulum Reloaded: The Case of Fast Pairwise Conversion","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2109.14627","snapshot_observed_at":"2026-08-06T16:29:12.697830Z","title":"Padilla-Gay, I","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2507.13429","last_updated":"2025-09-03T15:30:02Z","snapshot_observed_at":"2026-08-07T09:33:37.858372Z","submitted_at":"2025-07-17T18:00:00Z","title":"Electron-neutrino lepton number crossings: Variations with the supernova core physics","version":2},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-06T16:29:12.697830Z"},"links":{"cited_paper":"/paper/2109.14627","citing_paper":"/paper/2507.13429"},"observation_digest":"sha256:babeffa8dd55d08bc444807b849dff930e6d55b699898cb4c04f44bc5256da4f","observation_id":"fb28548f-90bb-4479-a845-95bcb4d1c0b7","resolution":{"observed_at":"2026-08-06T16:29:12.697830Z","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":"2026-08-06T16:29:12.833578Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2507.13429","last_updated":"2025-09-03T15:30:02Z","snapshot_observed_at":"2026-08-07T09:33:37.858372Z","submitted_at":"2025-07-17T18:00:00Z","title":"Electron-neutrino lepton number crossings: Variations with the supernova core physics","version":2},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-06T16:29:12.833578Z"},"links":{"citing_paper":"/paper/2507.13429"},"observation_digest":"sha256:42048d5d03168a3ddd4056f61c6e299679c9387b01b170f2a649413fbc442294","observation_id":"38229f74-deb8-44a1-b4a5-47b1a6a24ef3","resolution":{"observed_at":"2026-08-06T16:29:12.833578Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1702.00060","last_updated":"2017-03-24T16:39:15Z","snapshot_observed_at":"2026-07-06T05:28:17.715340Z","submitted_at":"2017-01-31T21:31:58Z","title":"Flavor-dependent neutrino angular distribution in core-collapse supernovae","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1702.00060","snapshot_observed_at":"2026-08-06T16:29:13.002537Z","title":"Tamborra, L","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2507.13429","last_updated":"2025-09-03T15:30:02Z","snapshot_observed_at":"2026-08-07T09:33:37.858372Z","submitted_at":"2025-07-17T18:00:00Z","title":"Electron-neutrino lepton number crossings: Variations with the supernova core physics","version":2},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-06T16:29:13.002537Z"},"links":{"cited_paper":"/paper/1702.00060","citing_paper":"/paper/2507.13429"},"observation_digest":"sha256:e78af8fd984635d93bb26f80e978dd06e592df58e9f9ee82072954acaa1c9754","observation_id":"dce48aae-1c21-4892-9e29-a31482284584","resolution":{"observed_at":"2026-08-06T16:29:13.002537Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1009.4654","last_updated":"2010-12-01T21:09:47Z","snapshot_observed_at":"2026-08-03T05:35:57.717907Z","submitted_at":"2010-09-23T16:30:38Z","title":"Results From Core-Collapse Simulations with Multi-Dimensional, Multi-Angle Neutrino Transport","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1009.4654","snapshot_observed_at":"2026-08-06T16:29:13.130352Z","title":null,"venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2507.13429","last_updated":"2025-09-03T15:30:02Z","snapshot_observed_at":"2026-08-07T09:33:37.858372Z","submitted_at":"2025-07-17T18:00:00Z","title":"Electron-neutrino lepton number crossings: Variations with the supernova core physics","version":2},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-06T16:29:13.130352Z"},"links":{"cited_paper":"/paper/1009.4654","citing_paper":"/paper/2507.13429"},"observation_digest":"sha256:6f0cb2ffe0a77133daf0d0107a3df82ee8a7def07e880c797ad4f7f0166a1b40","observation_id":"a2b5e984-c3a3-495b-b691-3ae40907a9b4","resolution":{"observed_at":"2026-08-06T16:29:13.130352Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1904.07236","last_updated":"2019-09-03T14:54:46Z","snapshot_observed_at":"2026-07-06T07:46:14.077705Z","submitted_at":"2019-04-15T18:00:00Z","title":"On the Occurrence of Crossings Between the Angular Distributions of Electron Neutrinos and Antineutrinos in the Supernova Core","version":2},"cited_work":{"arxiv_id":"1904.07236","doi":null,"metadata_source":"pith","pith_arxiv_id":"1904.07236","snapshot_observed_at":"2026-08-06T16:29:21.479896Z","title":"On the Occurrence of Crossings Between the Angular Distributions of Electron Neutrinos and Antineutrinos in the Supernova Core","venue":"astro-ph.HE","work_id":"080dd44c-cc7f-4a26-a6c4-30c936960012","year":2019},"citing_paper":{"arxiv_id":"2507.13429","last_updated":"2025-09-03T15:30:02Z","snapshot_observed_at":"2026-08-07T09:33:37.858372Z","submitted_at":"2025-07-17T18:00:00Z","title":"Electron-neutrino lepton number crossings: Variations with the supernova core physics","version":2},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-06T16:29:13.260913Z"},"links":{"cited_paper":"/paper/1904.07236","citing_paper":"/paper/2507.13429"},"observation_digest":"sha256:a4d9011518c744aa294b9c00b37cc2608f883fb829625097ce4349ca8674d613","observation_id":"912c122b-8ba2-43a1-b15d-142240f36dd7","resolution":{"observed_at":"2026-08-06T16:29:21.554718Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1201.2244","last_updated":"2012-01-11T05:39:28Z","snapshot_observed_at":"2026-07-31T12:40:22.521535Z","submitted_at":"2012-01-11T05:39:28Z","title":"Neutrino Transfer in Three Dimensions for Core-Collapse Supernovae. I. Static Configurations","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1201.2244","snapshot_observed_at":"2026-08-06T16:29:13.373289Z","title":"Sumiyoshi and S","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2507.13429","last_updated":"2025-09-03T15:30:02Z","snapshot_observed_at":"2026-08-07T09:33:37.858372Z","submitted_at":"2025-07-17T18:00:00Z","title":"Electron-neutrino lepton number crossings: Variations with the supernova core physics","version":2},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-06T16:29:13.373289Z"},"links":{"cited_paper":"/paper/1201.2244","citing_paper":"/paper/2507.13429"},"observation_digest":"sha256:3fd73d7eabaec72b77721152414f797032147db02a3d2c64b830b7dc83b99059","observation_id":"4befe1de-5221-4f82-8b76-fe0dd5022709","resolution":{"observed_at":"2026-08-06T16:29:13.373289Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2010.10780","last_updated":"2021-03-19T12:39:05Z","snapshot_observed_at":"2026-07-06T10:06:31.697461Z","submitted_at":"2020-10-21T06:17:07Z","title":"Multidimensional Boltzmann Neutrino Transport Code in Full General Relativity for Core-collapse Simulations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2010.10780","snapshot_observed_at":"2026-08-06T16:29:13.479092Z","title":"Akaho, A","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2507.13429","last_updated":"2025-09-03T15:30:02Z","snapshot_observed_at":"2026-08-07T09:33:37.858372Z","submitted_at":"2025-07-17T18:00:00Z","title":"Electron-neutrino lepton number crossings: Variations with the supernova core physics","version":2},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-06T16:29:13.479092Z"},"links":{"cited_paper":"/paper/2010.10780","citing_paper":"/paper/2507.13429"},"observation_digest":"sha256:338e588fd36e2161301a09568b3e867c5566fd64c94bc921d65933459438cf50","observation_id":"c7e9ebc4-ba1f-4090-999e-e3c0169b61e6","resolution":{"observed_at":"2026-08-06T16:29:13.479092Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1702.01752","last_updated":"2018-02-12T23:32:25Z","snapshot_observed_at":"2026-07-06T05:29:01.228177Z","submitted_at":"2017-02-06T19:00:01Z","title":"Simulations of core-collapse supernovae in spatial axisymmetry with full Boltzmann neutrino transport","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1702.01752","snapshot_observed_at":"2026-08-06T16:29:13.589862Z","title":"Nagakura, W","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2507.13429","last_updated":"2025-09-03T15:30:02Z","snapshot_observed_at":"2026-08-07T09:33:37.858372Z","submitted_at":"2025-07-17T18:00:00Z","title":"Electron-neutrino lepton number crossings: Variations with the supernova core physics","version":2},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-06T16:29:13.589862Z"},"links":{"cited_paper":"/paper/1702.01752","citing_paper":"/paper/2507.13429"},"observation_digest":"sha256:b82a9b679b7fdaa5c82fb46d36889d6dc1f402b18609d9e7d9510fb9f94c6718","observation_id":"f6cd3d95-db09-4b00-adf3-e9056f9b0404","resolution":{"observed_at":"2026-08-06T16:29:13.589862Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0908.1871","last_updated":"2010-10-20T09:57:12Z","snapshot_observed_at":"2026-07-06T01:59:43.508271Z","submitted_at":"2009-08-13T11:08:08Z","title":"Protoneutron star evolution and the neutrino driven wind in general relativistic neutrino radiation hydrodynamics simulations","version":5},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0908.1871","snapshot_observed_at":"2026-08-06T16:29:13.702024Z","title":"Fischer, S","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2507.13429","last_updated":"2025-09-03T15:30:02Z","snapshot_observed_at":"2026-08-07T09:33:37.858372Z","submitted_at":"2025-07-17T18:00:00Z","title":"Electron-neutrino lepton number crossings: Variations with the supernova core physics","version":2},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-06T16:29:13.702024Z"},"links":{"cited_paper":"/paper/0908.1871","citing_paper":"/paper/2507.13429"},"observation_digest":"sha256:97b28a9f95193761dc78c04814123b744e89f9b09493208ca7452ae513b7092c","observation_id":"a456c099-218a-4b81-a620-53e32c0cc55c","resolution":{"observed_at":"2026-08-06T16:29:13.702024Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2003.00969","last_updated":"2020-05-21T15:09:38Z","snapshot_observed_at":"2026-07-06T09:01:33.241690Z","submitted_at":"2020-03-02T15:32:46Z","title":"Searching for Fast Neutrino Flavor Conversion Modes in Core-collapse Supernova Simulations","version":2},"cited_work":{"arxiv_id":"2003.00969","doi":null,"metadata_source":"pith","pith_arxiv_id":"2003.00969","snapshot_observed_at":"2026-08-06T16:29:21.203911Z","title":"Searching for Fast Neutrino Flavor Conversion Modes in Core-collapse Supernova Simulations","venue":"astro-ph.HE","work_id":"f608e203-38be-4a1f-9922-24afb7437649","year":2020},"citing_paper":{"arxiv_id":"2507.13429","last_updated":"2025-09-03T15:30:02Z","snapshot_observed_at":"2026-08-07T09:33:37.858372Z","submitted_at":"2025-07-17T18:00:00Z","title":"Electron-neutrino lepton number crossings: Variations with the supernova core physics","version":2},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-06T16:29:13.854009Z"},"links":{"cited_paper":"/paper/2003.00969","citing_paper":"/paper/2507.13429"},"observation_digest":"sha256:d0abc3f3fcbc7a347ac738f4fd933506778feffb4e48f1bd786f93d559cd3499","observation_id":"aeb96d91-b47c-40f6-9bd8-01b58ee9fcde","resolution":{"observed_at":"2026-08-06T16:29:21.279643Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2012.06594","last_updated":"2021-03-11T21:04:26Z","snapshot_observed_at":"2026-07-06T10:23:40.025224Z","submitted_at":"2020-12-11T19:00:47Z","title":"On the characteristics of fast neutrino flavor instabilities in three-dimensional core-collapse supernova models","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2012.06594","snapshot_observed_at":"2026-08-06T16:29:13.985390Z","title":"Abbar, F","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2507.13429","last_updated":"2025-09-03T15:30:02Z","snapshot_observed_at":"2026-08-07T09:33:37.858372Z","submitted_at":"2025-07-17T18:00:00Z","title":"Electron-neutrino lepton number crossings: Variations with the supernova core physics","version":2},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-08-06T16:29:13.985390Z"},"links":{"cited_paper":"/paper/2012.06594","citing_paper":"/paper/2507.13429"},"observation_digest":"sha256:fe6f961b3827e02ba57642d448bd79831e0470a1acc5a3e4db17757bbe18ea45","observation_id":"64a5847c-153e-45df-a733-1adb6754c65e","resolution":{"observed_at":"2026-08-06T16:29:13.985390Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2012.08525","last_updated":"2021-03-11T16:17:18Z","snapshot_observed_at":"2026-08-05T19:22:53.068225Z","submitted_at":"2020-12-15T19:00:01Z","title":"Fast neutrino flavor conversions in one-dimensional core-collapse supernova models with and without muon creation","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2012.08525","snapshot_observed_at":"2026-08-06T16:29:14.182091Z","title":"Capozzi, S","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2507.13429","last_updated":"2025-09-03T15:30:02Z","snapshot_observed_at":"2026-08-07T09:33:37.858372Z","submitted_at":"2025-07-17T18:00:00Z","title":"Electron-neutrino lepton number crossings: Variations with the supernova core physics","version":2},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-06T16:29:14.182091Z"},"links":{"cited_paper":"/paper/2012.08525","citing_paper":"/paper/2507.13429"},"observation_digest":"sha256:6fa3f2d2cae6b093b59c047e14e298a5c2aa55bcf6c7e874e8871b0fd55bd80b","observation_id":"a365258e-16db-4340-a561-51e5e8562c4c","resolution":{"observed_at":"2026-08-06T16:29:14.182091Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1807.03322","last_updated":"2018-11-05T20:11:50Z","snapshot_observed_at":"2026-08-02T08:00:36.786513Z","submitted_at":"2018-07-09T18:06:01Z","title":"A few moments to diagnose fast flavor conversions of supernova neutrinos","version":2},"cited_work":{"arxiv_id":"1807.03322","doi":null,"metadata_source":"pith","pith_arxiv_id":"1807.03322","snapshot_observed_at":"2026-08-06T16:29:20.910284Z","title":"A few moments to diagnose fast flavor conversions of supernova neutrinos","venue":"hep-ph","work_id":"2465b043-fa11-4d20-adcc-22d729f5beba","year":2018},"citing_paper":{"arxiv_id":"2507.13429","last_updated":"2025-09-03T15:30:02Z","snapshot_observed_at":"2026-08-07T09:33:37.858372Z","submitted_at":"2025-07-17T18:00:00Z","title":"Electron-neutrino lepton number crossings: Variations with the supernova core physics","version":2},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-06T16:29:14.357864Z"},"links":{"cited_paper":"/paper/1807.03322","citing_paper":"/paper/2507.13429"},"observation_digest":"sha256:ce334081fa99ccf89d30994bbe98dffe4740d3d802ac6ca2618e5792583b9d39","observation_id":"1181e554-84f8-41a4-964f-6f63ee38de73","resolution":{"observed_at":"2026-08-06T16:29:21.046067Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T16:29:14.453094Z","title":"Glas, H.-T","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2507.13429","last_updated":"2025-09-03T15:30:02Z","snapshot_observed_at":"2026-08-07T09:33:37.858372Z","submitted_at":"2025-07-17T18:00:00Z","title":"Electron-neutrino lepton number crossings: Variations with the supernova core physics","version":2},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-06T16:29:14.453094Z"},"links":{"citing_paper":"/paper/2507.13429"},"observation_digest":"sha256:317bf462d4ded8d7eb675eae2712a2f4b1ed256b2e9218c2c8d68e1fce88decc","observation_id":"af28f6de-8f4a-4616-bac3-303b9ee708e2","resolution":{"observed_at":"2026-08-06T16:29:14.453094Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2108.07281","last_updated":"2021-08-24T04:07:41Z","snapshot_observed_at":"2026-07-06T11:38:45.947453Z","submitted_at":"2021-08-16T18:00:04Z","title":"Where, when and why: occurrence of fast-pairwise collective neutrino oscillation in three-dimensional core-collapse supernova models","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2108.07281","snapshot_observed_at":"2026-08-06T16:29:14.568876Z","title":"Nagakura, L","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2507.13429","last_updated":"2025-09-03T15:30:02Z","snapshot_observed_at":"2026-08-07T09:33:37.858372Z","submitted_at":"2025-07-17T18:00:00Z","title":"Electron-neutrino lepton number crossings: Variations with the supernova core physics","version":2},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-06T16:29:14.568876Z"},"links":{"cited_paper":"/paper/2108.07281","citing_paper":"/paper/2507.13429"},"observation_digest":"sha256:a3b94f42deaa60f52ca68a8966c954fa5b463fbe81d3544b664339939477f22c","observation_id":"70501120-4883-47e3-82ab-1766cc00c2b2","resolution":{"observed_at":"2026-08-06T16:29:14.568876Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2104.04106","last_updated":"2021-04-15T18:58:05Z","snapshot_observed_at":"2026-07-06T10:57:51.456986Z","submitted_at":"2021-04-08T22:59:16Z","title":"Fast flavor instabilities and the search for neutrino angular crossings","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2104.04106","snapshot_observed_at":"2026-08-06T16:29:14.673312Z","title":"Johns and H","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2507.13429","last_updated":"2025-09-03T15:30:02Z","snapshot_observed_at":"2026-08-07T09:33:37.858372Z","submitted_at":"2025-07-17T18:00:00Z","title":"Electron-neutrino lepton number crossings: Variations with the supernova core physics","version":2},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-06T16:29:14.673312Z"},"links":{"cited_paper":"/paper/2104.04106","citing_paper":"/paper/2507.13429"},"observation_digest":"sha256:7f29f2d0ec5dd0e140b77f0008686cd37369bc2bbfecf0938ac0d18375404315","observation_id":"f22dbcc5-1fd1-4cba-ad4e-024292c0de27","resolution":{"observed_at":"2026-08-06T16:29:14.673312Z","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":"2026-08-06T16:29:14.844421Z","title":"Cornelius, I","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2507.13429","last_updated":"2025-09-03T15:30:02Z","snapshot_observed_at":"2026-08-07T09:33:37.858372Z","submitted_at":"2025-07-17T18:00:00Z","title":"Electron-neutrino lepton number crossings: Variations with the supernova core physics","version":2},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-06T16:29:14.844421Z"},"links":{"citing_paper":"/paper/2507.13429"},"observation_digest":"sha256:4761962da9d1ad0cb206107f5e2132ac5b4096565cc8259a637fd8d1312aa284","observation_id":"0ba599ad-8de6-4c1a-8b28-94dc42ea666a","resolution":{"observed_at":"2026-08-06T16:29:14.844421Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2307.10366","last_updated":"2024-04-15T11:51:47Z","snapshot_observed_at":"2026-07-06T15:56:07.787414Z","submitted_at":"2023-07-19T18:00:01Z","title":"Do Neutrinos Become Flavor Unstable Due to Collisions with Matter in the Supernova Decoupling Region?","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2307.10366","snapshot_observed_at":"2026-08-06T16:29:14.997843Z","title":"Shalgar and I","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2507.13429","last_updated":"2025-09-03T15:30:02Z","snapshot_observed_at":"2026-08-07T09:33:37.858372Z","submitted_at":"2025-07-17T18:00:00Z","title":"Electron-neutrino lepton number crossings: Variations with the supernova core physics","version":2},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-06T16:29:14.997843Z"},"links":{"cited_paper":"/paper/2307.10366","citing_paper":"/paper/2507.13429"},"observation_digest":"sha256:ca05bdf0c72df60d0a13deae2257e8f22fe9d89bd8a35a214b6355f7c5784017","observation_id":"ded915fc-4628-4de9-8e37-a48f1bf5fa3f","resolution":{"observed_at":"2026-08-06T16:29:14.997843Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2406.09504","last_updated":"2024-08-15T14:29:45Z","snapshot_observed_at":"2026-07-06T18:30:37.311343Z","submitted_at":"2024-06-13T18:00:02Z","title":"Neutrino quantum kinetics in a core-collapse supernova","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2406.09504","snapshot_observed_at":"2026-08-06T16:29:15.136093Z","title":"Shalgar and I","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2507.13429","last_updated":"2025-09-03T15:30:02Z","snapshot_observed_at":"2026-08-07T09:33:37.858372Z","submitted_at":"2025-07-17T18:00:00Z","title":"Electron-neutrino lepton number crossings: Variations with the supernova core physics","version":2},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-08-06T16:29:15.136093Z"},"links":{"cited_paper":"/paper/2406.09504","citing_paper":"/paper/2507.13429"},"observation_digest":"sha256:2f418079d4b871e20a048f1080c796be4baa354af3a911adf112dd5a942d4020","observation_id":"9bda2834-3919-4158-a09e-2f3d0005a9dd","resolution":{"observed_at":"2026-08-06T16:29:15.136093Z","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":"2026-08-06T16:29:15.287580Z","title":"Shalgar and I","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2507.13429","last_updated":"2025-09-03T15:30:02Z","snapshot_observed_at":"2026-08-07T09:33:37.858372Z","submitted_at":"2025-07-17T18:00:00Z","title":"Electron-neutrino lepton number crossings: Variations with the supernova core physics","version":2},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-08-06T16:29:15.287580Z"},"links":{"citing_paper":"/paper/2507.13429"},"observation_digest":"sha256:6b7abe267c485d634386a76e6fca0320f25e4b8f80799cf6b422b95ec13dbc5a","observation_id":"67a21784-7d41-4378-bc37-f41e6ccdbd3d","resolution":{"observed_at":"2026-08-06T16:29:15.287580Z","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":"2026-08-06T16:29:22.680342Z","title":null,"venue":null,"work_id":"64c2a19d-5364-4409-b843-fa8a47b91f77","year":null},"citing_paper":{"arxiv_id":"2507.13429","last_updated":"2025-09-03T15:30:02Z","snapshot_observed_at":"2026-08-07T09:33:37.858372Z","submitted_at":"2025-07-17T18:00:00Z","title":"Electron-neutrino lepton number crossings: Variations with the supernova core physics","version":2},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-08-06T16:29:15.437245Z"},"links":{"citing_paper":"/paper/2507.13429"},"observation_digest":"sha256:a3470a20db8a8dc7cf455c52633d2ec33ba7917500e0d0c23352d2d2cf7f9929","observation_id":"f4ab263a-e3b7-4f5e-8787-5f94e1a70cbf","resolution":{"observed_at":"2026-08-06T16:29:22.774250Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+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":"2026-08-06T16:29:22.396650Z","title":null,"venue":null,"work_id":"defa4c89-6d8d-45ea-8fe7-de0b1094f437","year":1991},"citing_paper":{"arxiv_id":"2507.13429","last_updated":"2025-09-03T15:30:02Z","snapshot_observed_at":"2026-08-07T09:33:37.858372Z","submitted_at":"2025-07-17T18:00:00Z","title":"Electron-neutrino lepton number crossings: Variations with the supernova core physics","version":2},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-08-06T16:29:15.616357Z"},"links":{"citing_paper":"/paper/2507.13429"},"observation_digest":"sha256:671f1d1dc150942e61df0f5690f992ac945e4a6b2018148c36c5267b41f46894","observation_id":"f87ebf18-3ee0-4575-9cdb-88a32f82e777","resolution":{"observed_at":"2026-08-06T16:29:22.554873Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1207.2184","last_updated":"2012-07-09T21:00:43Z","snapshot_observed_at":"2026-07-06T02:51:32.421947Z","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":"2026-08-06T16:29:15.785047Z","title":null,"venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2507.13429","last_updated":"2025-09-03T15:30:02Z","snapshot_observed_at":"2026-08-07T09:33:37.858372Z","submitted_at":"2025-07-17T18:00:00Z","title":"Electron-neutrino lepton number crossings: Variations with the supernova core physics","version":2},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-08-06T16:29:15.785047Z"},"links":{"cited_paper":"/paper/1207.2184","citing_paper":"/paper/2507.13429"},"observation_digest":"sha256:c7398dcb35e1528f26024006b6dabe05b0cd185112c03c9f7614c3dd29aa90e3","observation_id":"a40eb5e7-fa4a-487c-81f5-f61c750a93a1","resolution":{"observed_at":"2026-08-06T16:29:15.785047Z","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":"2026-07-06T02:00:40.912171Z","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":"2026-08-06T16:29:15.908494Z","title":"Hempel and J","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2507.13429","last_updated":"2025-09-03T15:30:02Z","snapshot_observed_at":"2026-08-07T09:33:37.858372Z","submitted_at":"2025-07-17T18:00:00Z","title":"Electron-neutrino lepton number crossings: Variations with the supernova core physics","version":2},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-08-06T16:29:15.908494Z"},"links":{"cited_paper":"/paper/0911.4073","citing_paper":"/paper/2507.13429"},"observation_digest":"sha256:be4d86f3900244b1c97d84820497e14833d3e28360d7fa9ede57c6261a746922","observation_id":"d5c8a786-e13b-43a4-b130-4608f8a4d280","resolution":{"observed_at":"2026-08-06T16:29:15.908494Z","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":"2026-07-31T19:37:08.721893Z","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":"2026-08-06T16:29:16.057758Z","title":"Typel, G","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2507.13429","last_updated":"2025-09-03T15:30:02Z","snapshot_observed_at":"2026-08-07T09:33:37.858372Z","submitted_at":"2025-07-17T18:00:00Z","title":"Electron-neutrino lepton number crossings: Variations with the supernova core physics","version":2},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-08-06T16:29:16.057758Z"},"links":{"cited_paper":"/paper/0908.2344","citing_paper":"/paper/2507.13429"},"observation_digest":"sha256:fb8389061305ead9aa0884c2de523a3612277ada0de1a6099ef5bcb0de72f46a","observation_id":"162cd553-e529-459b-bd20-1a0bcb83513e","resolution":{"observed_at":"2026-08-06T16:29:16.057758Z","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":"2026-07-06T02:31:53.409694Z","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":"2026-08-06T16:29:16.191928Z","title":"Hempel, T","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2507.13429","last_updated":"2025-09-03T15:30:02Z","snapshot_observed_at":"2026-08-07T09:33:37.858372Z","submitted_at":"2025-07-17T18:00:00Z","title":"Electron-neutrino lepton number crossings: Variations with the supernova core physics","version":2},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-08-06T16:29:16.191928Z"},"links":{"cited_paper":"/paper/1108.0848","citing_paper":"/paper/2507.13429"},"observation_digest":"sha256:e2e377c1506fc8b36d7ee821e7eb4c7a7b7f15cb102e021ad5f8a9616e4820fc","observation_id":"3eec8acf-5820-4b16-b111-317a79839d34","resolution":{"observed_at":"2026-08-06T16:29:16.191928Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1706.04630","last_updated":"2017-11-17T19:28:21Z","snapshot_observed_at":"2026-07-06T05:46:53.851774Z","submitted_at":"2017-06-14T18:34:23Z","title":"Muon Creation in Supernova Matter Facilitates Neutrino-driven Explosions","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1706.04630","snapshot_observed_at":"2026-08-06T16:29:16.303968Z","title":"Bollig, H.-T","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2507.13429","last_updated":"2025-09-03T15:30:02Z","snapshot_observed_at":"2026-08-07T09:33:37.858372Z","submitted_at":"2025-07-17T18:00:00Z","title":"Electron-neutrino lepton number crossings: Variations with the supernova core physics","version":2},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-08-06T16:29:16.303968Z"},"links":{"cited_paper":"/paper/1706.04630","citing_paper":"/paper/2507.13429"},"observation_digest":"sha256:56a7fd695d27d2a6131cb7ac859c79d66c0b6078904d21a9f459c6c5da8d5d0d","observation_id":"3e2906bf-1fc0-48ba-9c7a-51b0b0b9d36a","resolution":{"observed_at":"2026-08-06T16:29:16.303968Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1112.0335","last_updated":"2011-12-01T21:40:23Z","snapshot_observed_at":"2026-07-06T02:38:39.668767Z","submitted_at":"2011-12-01T21:40:23Z","title":"Proto-Neutron Star Cooling with Convection: The Effect of the Symmetry Energy","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1112.0335","snapshot_observed_at":"2026-08-06T16:29:16.436568Z","title":null,"venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2507.13429","last_updated":"2025-09-03T15:30:02Z","snapshot_observed_at":"2026-08-07T09:33:37.858372Z","submitted_at":"2025-07-17T18:00:00Z","title":"Electron-neutrino lepton number crossings: Variations with the supernova core physics","version":2},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-08-06T16:29:16.436568Z"},"links":{"cited_paper":"/paper/1112.0335","citing_paper":"/paper/2507.13429"},"observation_digest":"sha256:c75a9704ed50fead9e56eb6b2bda687d1bc4a1bb174b187e4a5e4707376339f8","observation_id":"139ab658-b1f5-445f-880a-18019ab7074f","resolution":{"observed_at":"2026-08-06T16:29:16.436568Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2201.01955","last_updated":"2022-01-06T07:48:33Z","snapshot_observed_at":"2026-08-07T14:57:58.658441Z","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":"2026-08-06T16:29:16.559957Z","title":"Pascal, J","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2507.13429","last_updated":"2025-09-03T15:30:02Z","snapshot_observed_at":"2026-08-07T09:33:37.858372Z","submitted_at":"2025-07-17T18:00:00Z","title":"Electron-neutrino lepton number crossings: Variations with the supernova core physics","version":2},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-08-06T16:29:16.559957Z"},"links":{"cited_paper":"/paper/2201.01955","citing_paper":"/paper/2507.13429"},"observation_digest":"sha256:ccdf965129a23aa92d87b42e98f42b184ea249c7ab36bc74320c4229cd9a0d42","observation_id":"ecb36ca3-962c-4b11-bb73-1b484335e889","resolution":{"observed_at":"2026-08-06T16:29:16.559957Z","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":"2026-07-06T04:25:46.543674Z","submitted_at":"2015-07-31T20:09:50Z","title":"Supernova Neutrinos: Production, Oscillations and Detection","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1508.00785","snapshot_observed_at":"2026-08-06T16:29:16.691255Z","title":"Mirizzi, I","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2507.13429","last_updated":"2025-09-03T15:30:02Z","snapshot_observed_at":"2026-08-07T09:33:37.858372Z","submitted_at":"2025-07-17T18:00:00Z","title":"Electron-neutrino lepton number crossings: Variations with the supernova core physics","version":2},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-08-06T16:29:16.691255Z"},"links":{"cited_paper":"/paper/1508.00785","citing_paper":"/paper/2507.13429"},"observation_digest":"sha256:83477302dc8282f523ce06cbfdd201696aec889896509b66f4acda988d0382d6","observation_id":"85fd1a19-cf3d-4b7e-be37-e2d182044faf","resolution":{"observed_at":"2026-08-06T16:29:16.691255Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0203101","last_updated":"2002-10-01T09:51:41Z","snapshot_observed_at":"2026-07-07T00:25:23.256370Z","submitted_at":"2002-03-07T10:22:33Z","title":"Radiation hydrodynamics with neutrinos: Variable Eddington factor method for core-collapse supernova simulations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0203101","snapshot_observed_at":"2026-08-06T16:29:16.875154Z","title":"Rampp and H.-T","venue":null,"work_id":null,"year":2002},"citing_paper":{"arxiv_id":"2507.13429","last_updated":"2025-09-03T15:30:02Z","snapshot_observed_at":"2026-08-07T09:33:37.858372Z","submitted_at":"2025-07-17T18:00:00Z","title":"Electron-neutrino lepton number crossings: Variations with the supernova core physics","version":2},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-08-06T16:29:16.875154Z"},"links":{"cited_paper":"/paper/astro-ph/0203101","citing_paper":"/paper/2507.13429"},"observation_digest":"sha256:e2266591c31d7a6ae4b2f9d4f73414b6130de89e91c4d01f8bf35dd5646334bf","observation_id":"40c31648-e37e-47e7-bdb6-150629a6fb69","resolution":{"observed_at":"2026-08-06T16:29:16.875154Z","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":"2026-07-06T16:01:50.107288Z","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":"2026-08-06T16:29:17.015115Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2507.13429","last_updated":"2025-09-03T15:30:02Z","snapshot_observed_at":"2026-08-07T09:33:37.858372Z","submitted_at":"2025-07-17T18:00:00Z","title":"Electron-neutrino lepton number crossings: Variations with the supernova core physics","version":2},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-08-06T16:29:17.015115Z"},"links":{"cited_paper":"/paper/2308.01403","citing_paper":"/paper/2507.13429"},"observation_digest":"sha256:f51ebe00c1f7d1c53c392e714a5fc1af3a11364a80b44b9168ff6cb1e7aeb9d9","observation_id":"e97ac9bc-71d7-4b54-8982-869de04d43b3","resolution":{"observed_at":"2026-08-06T16:29:17.015115Z","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":"2026-08-06T16:29:22.268278Z","title":"Sigl and G","venue":null,"work_id":"754c2730-59a3-48c6-ae0f-0aa95e87e856","year":1993},"citing_paper":{"arxiv_id":"2507.13429","last_updated":"2025-09-03T15:30:02Z","snapshot_observed_at":"2026-08-07T09:33:37.858372Z","submitted_at":"2025-07-17T18:00:00Z","title":"Electron-neutrino lepton number crossings: Variations with the supernova core physics","version":2},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-08-06T16:29:17.142005Z"},"links":{"citing_paper":"/paper/2507.13429"},"observation_digest":"sha256:039f34969727d6c378e3dc0dde24761ff06b15e93101793665aa6a652818293f","observation_id":"c48a4584-226a-4722-8abb-be30e45679ed","resolution":{"observed_at":"2026-08-06T16:29:22.334067Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1411.7058","last_updated":"2015-10-01T21:11:22Z","snapshot_observed_at":"2026-07-06T04:01:43.228675Z","submitted_at":"2014-11-25T22:25:53Z","title":"An Open-Source Neutrino Radiation Hydrodynamics Code for Core-Collapse Supernovae","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1411.7058","snapshot_observed_at":"2026-08-06T16:29:17.246787Z","title":"O’Connor, An Open-Source Neutrino Radiation Hy- drodynamics Code for Core-Collapse Supernovae, Astro- phys","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2507.13429","last_updated":"2025-09-03T15:30:02Z","snapshot_observed_at":"2026-08-07T09:33:37.858372Z","submitted_at":"2025-07-17T18:00:00Z","title":"Electron-neutrino lepton number crossings: Variations with the supernova core physics","version":2},"reference_index":54,"source":"pdf_text","source_observed_at":"2026-08-06T16:29:17.246787Z"},"links":{"cited_paper":"/paper/1411.7058","citing_paper":"/paper/2507.13429"},"observation_digest":"sha256:4581de770a4673797715ccef21145979ac1a1de24a4ae2c240e5849563fb40d0","observation_id":"1260b1f5-4d11-483f-aa74-fe94c39c6f0a","resolution":{"observed_at":"2026-08-06T16:29:17.246787Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0507135","last_updated":"2005-10-31T17:05:06Z","snapshot_observed_at":"2026-08-01T19:27:07.322068Z","submitted_at":"2005-07-06T15:58:38Z","title":"Two-dimensional hydrodynamic core-collapse supernova simulations with spectral neutrino transport. I. Numerical method and results for a 15 M_sun star","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0507135","snapshot_observed_at":"2026-08-06T16:29:17.367914Z","title":"Buras, M","venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"2507.13429","last_updated":"2025-09-03T15:30:02Z","snapshot_observed_at":"2026-08-07T09:33:37.858372Z","submitted_at":"2025-07-17T18:00:00Z","title":"Electron-neutrino lepton number crossings: Variations with the supernova core physics","version":2},"reference_index":55,"source":"pdf_text","source_observed_at":"2026-08-06T16:29:17.367914Z"},"links":{"cited_paper":"/paper/astro-ph/0507135","citing_paper":"/paper/2507.13429"},"observation_digest":"sha256:f21ec3d8ec28fb7f89a96f90ef804db492c0c5115365465b85847ef19ee8441d","observation_id":"ca95c755-f00a-4db5-b476-de2e09efec33","resolution":{"observed_at":"2026-08-06T16:29:17.367914Z","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":"2026-08-06T16:29:17.489757Z","title":"Janka, K","venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2507.13429","last_updated":"2025-09-03T15:30:02Z","snapshot_observed_at":"2026-08-07T09:33:37.858372Z","submitted_at":"2025-07-17T18:00:00Z","title":"Electron-neutrino lepton number crossings: Variations with the supernova core physics","version":2},"reference_index":56,"source":"pdf_text","source_observed_at":"2026-08-06T16:29:17.489757Z"},"links":{"citing_paper":"/paper/2507.13429"},"observation_digest":"sha256:8bb03fb2bfd168c903cd1cf1da9e95a70cd1ee17bc18a2d42f959b16924e3699","observation_id":"b3ed0bc4-9a87-438b-97fe-74b05abaa513","resolution":{"observed_at":"2026-08-06T16:29:17.489757Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1206.2503","last_updated":"2012-06-12T12:12:02Z","snapshot_observed_at":"2026-08-04T00:00:05.427259Z","submitted_at":"2012-06-12T12:12:02Z","title":"Explosion Mechanisms of Core-Collapse Supernovae","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1206.2503","snapshot_observed_at":"2026-08-06T16:29:17.649538Z","title":"Janka, Explosion Mechanisms of Core-Collapse Su- pernovae, Ann","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2507.13429","last_updated":"2025-09-03T15:30:02Z","snapshot_observed_at":"2026-08-07T09:33:37.858372Z","submitted_at":"2025-07-17T18:00:00Z","title":"Electron-neutrino lepton number crossings: Variations with the supernova core physics","version":2},"reference_index":57,"source":"pdf_text","source_observed_at":"2026-08-06T16:29:17.649538Z"},"links":{"cited_paper":"/paper/1206.2503","citing_paper":"/paper/2507.13429"},"observation_digest":"sha256:913355da3493a3ab1cc5066b8a120cfee6dc0b0a22bce1000816b3360786d846","observation_id":"b65fbf0f-9237-4449-8df3-98771f5cdc1b","resolution":{"observed_at":"2026-08-06T16:29:17.649538Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1910.06176","last_updated":"2020-01-15T05:17:08Z","snapshot_observed_at":"2026-08-03T04:15:43.162009Z","submitted_at":"2019-10-14T14:36:06Z","title":"Fast collective neutrino oscillations inside the neutrino sphere in core-collapse supernovae","version":3},"cited_work":{"arxiv_id":"1910.06176","doi":null,"metadata_source":"pith","pith_arxiv_id":"1910.06176","snapshot_observed_at":"2026-08-06T16:29:20.218021Z","title":"Fast collective neutrino oscillations inside the neutrino sphere in core-collapse supernovae","venue":"astro-ph.HE","work_id":"19c973c8-575c-401c-9d5d-e9d05efa2997","year":2019},"citing_paper":{"arxiv_id":"2507.13429","last_updated":"2025-09-03T15:30:02Z","snapshot_observed_at":"2026-08-07T09:33:37.858372Z","submitted_at":"2025-07-17T18:00:00Z","title":"Electron-neutrino lepton number crossings: Variations with the supernova core physics","version":2},"reference_index":58,"source":"pdf_text","source_observed_at":"2026-08-06T16:29:17.833610Z"},"links":{"cited_paper":"/paper/1910.06176","citing_paper":"/paper/2507.13429"},"observation_digest":"sha256:a8ce6eaa666cf28b9cfd1e4ef9aa4d0a21d85ab8ec3be82e4c8528a3d91efb6e","observation_id":"bf27f8b8-efb4-450a-aba5-8cc0d17c9bcc","resolution":{"observed_at":"2026-08-06T16:29:20.323431Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2206.01673","last_updated":"2022-12-20T06:46:40Z","snapshot_observed_at":"2026-07-06T13:17:15.959025Z","submitted_at":"2022-06-03T16:36:47Z","title":"Protoneutron Star Convection Simulated with a New General Relativistic Boltzmann Neutrino Radiation-Hydrodynamics Code","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2206.01673","snapshot_observed_at":"2026-08-06T16:29:17.984814Z","title":"Akaho, A","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2507.13429","last_updated":"2025-09-03T15:30:02Z","snapshot_observed_at":"2026-08-07T09:33:37.858372Z","submitted_at":"2025-07-17T18:00:00Z","title":"Electron-neutrino lepton number crossings: Variations with the supernova core physics","version":2},"reference_index":59,"source":"pdf_text","source_observed_at":"2026-08-06T16:29:17.984814Z"},"links":{"cited_paper":"/paper/2206.01673","citing_paper":"/paper/2507.13429"},"observation_digest":"sha256:fb3f1c01075be9db3d86020c247a3e28c804970b164b014a265314e3313851ad","observation_id":"ee6fba47-f2db-4552-9beb-68e4406b803d","resolution":{"observed_at":"2026-08-06T16:29:17.984814Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2311.11272","last_updated":"2024-01-09T11:33:39Z","snapshot_observed_at":"2026-07-06T16:49:33.776407Z","submitted_at":"2023-11-19T09:02:45Z","title":"Collisional and Fast Neutrino Flavor Instabilities in Two-dimensional Core-collapse Supernova Simulation with Boltzmann Neutrino Transport","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2311.11272","snapshot_observed_at":"2026-08-06T16:29:18.145109Z","title":"Akaho, J","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2507.13429","last_updated":"2025-09-03T15:30:02Z","snapshot_observed_at":"2026-08-07T09:33:37.858372Z","submitted_at":"2025-07-17T18:00:00Z","title":"Electron-neutrino lepton number crossings: Variations with the supernova core physics","version":2},"reference_index":60,"source":"pdf_text","source_observed_at":"2026-08-06T16:29:18.145109Z"},"links":{"cited_paper":"/paper/2311.11272","citing_paper":"/paper/2507.13429"},"observation_digest":"sha256:0593ce0a9c5bfcd7addb9e220c4cbd445e447a78567f3498854bfefb0368466a","observation_id":"205b153b-3fb4-4a2d-9541-518e6a0400d1","resolution":{"observed_at":"2026-08-06T16:29:18.145109Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1910.04288","last_updated":"2019-10-09T22:53:22Z","snapshot_observed_at":"2026-07-06T08:28:15.985260Z","submitted_at":"2019-10-09T22:53:22Z","title":"Fast-pairwise collective neutrino oscillations associated with asymmetric neutrino emissions in core-collapse supernova","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1910.04288","snapshot_observed_at":"2026-08-06T16:29:18.321693Z","title":"Nagakura, T","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2507.13429","last_updated":"2025-09-03T15:30:02Z","snapshot_observed_at":"2026-08-07T09:33:37.858372Z","submitted_at":"2025-07-17T18:00:00Z","title":"Electron-neutrino lepton number crossings: Variations with the supernova core physics","version":2},"reference_index":61,"source":"pdf_text","source_observed_at":"2026-08-06T16:29:18.321693Z"},"links":{"cited_paper":"/paper/1910.04288","citing_paper":"/paper/2507.13429"},"observation_digest":"sha256:ba6434cfd8815e2be42af6d0e450144cba71682d790373c17dbecb4be5b421ad","observation_id":"a94bf720-9cba-47f7-819f-5a68e8583ae0","resolution":{"observed_at":"2026-08-06T16:29:18.321693Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1909.13131","last_updated":"2019-09-28T19:03:36Z","snapshot_observed_at":"2026-08-04T18:10:05.902775Z","submitted_at":"2019-09-28T19:03:36Z","title":"A new possibility of the fast neutrino-flavor conversion in the pre-shock region of core-collapse supernova","version":1},"cited_work":{"arxiv_id":"1909.13131","doi":null,"metadata_source":"pith","pith_arxiv_id":"1909.13131","snapshot_observed_at":"2026-08-06T16:29:19.902647Z","title":"A new possibility of the fast neutrino-flavor conversion in the pre-shock region of core-collapse supernova","venue":"astro-ph.HE","work_id":"ff969be3-9557-4776-afa3-e8c0377e1302","year":2019},"citing_paper":{"arxiv_id":"2507.13429","last_updated":"2025-09-03T15:30:02Z","snapshot_observed_at":"2026-08-07T09:33:37.858372Z","submitted_at":"2025-07-17T18:00:00Z","title":"Electron-neutrino lepton number crossings: Variations with the supernova core physics","version":2},"reference_index":62,"source":"pdf_text","source_observed_at":"2026-08-06T16:29:18.502725Z"},"links":{"cited_paper":"/paper/1909.13131","citing_paper":"/paper/2507.13429"},"observation_digest":"sha256:7b1753831a456d48d96cda3b09e140e26000dd3b1a3a785bb6d707b7ce2806dd","observation_id":"446b24be-3c44-4751-a9dc-8a31c00af22c","resolution":{"observed_at":"2026-08-06T16:29:20.024814Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2110.08291","last_updated":"2021-11-10T09:49:55Z","snapshot_observed_at":"2026-07-06T11:58:24.426799Z","submitted_at":"2021-10-15T18:01:06Z","title":"Prospects of fast flavor neutrino conversion in rotating core-collapse supernovae","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2110.08291","snapshot_observed_at":"2026-08-06T16:29:18.632563Z","title":"Harada and H","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2507.13429","last_updated":"2025-09-03T15:30:02Z","snapshot_observed_at":"2026-08-07T09:33:37.858372Z","submitted_at":"2025-07-17T18:00:00Z","title":"Electron-neutrino lepton number crossings: Variations with the supernova core physics","version":2},"reference_index":63,"source":"pdf_text","source_observed_at":"2026-08-06T16:29:18.632563Z"},"links":{"cited_paper":"/paper/2110.08291","citing_paper":"/paper/2507.13429"},"observation_digest":"sha256:78eb499b1de31351958b17bdb5186cc330aeb9619e9f52a3b143364f3ed420ad","observation_id":"fd7e53d5-52a9-4e6e-b4df-b9a4b5f7eeb5","resolution":{"observed_at":"2026-08-06T16:29:18.632563Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1402.5418","last_updated":"2014-07-31T05:05:30Z","snapshot_observed_at":"2026-07-06T03:36:39.153202Z","submitted_at":"2014-02-21T21:00:18Z","title":"Self-sustained asymmetry of lepton-number emission: A new phenomenon during the supernova shock-accretion phase in three dimensions","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1402.5418","snapshot_observed_at":"2026-08-06T16:29:18.803489Z","title":"Tamborra, F","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2507.13429","last_updated":"2025-09-03T15:30:02Z","snapshot_observed_at":"2026-08-07T09:33:37.858372Z","submitted_at":"2025-07-17T18:00:00Z","title":"Electron-neutrino lepton number crossings: Variations with the supernova core physics","version":2},"reference_index":64,"source":"pdf_text","source_observed_at":"2026-08-06T16:29:18.803489Z"},"links":{"cited_paper":"/paper/1402.5418","citing_paper":"/paper/2507.13429"},"observation_digest":"sha256:ca28f080117bf06ca1a9a5b8608fc6547480ce8e82d7bc7073ce44f0830e895a","observation_id":"ce67f8b1-867d-47f4-9e86-f6e3ba984c8f","resolution":{"observed_at":"2026-08-06T16:29:18.803489Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1701.06580","last_updated":"2017-05-15T09:07:26Z","snapshot_observed_at":"2026-07-06T05:27:13.416519Z","submitted_at":"2017-01-23T19:00:12Z","title":"Fast neutrino conversions: Ubiquitous in compact binary merger remnants","version":2},"cited_work":{"arxiv_id":"1701.06580","doi":null,"metadata_source":"pith","pith_arxiv_id":"1701.06580","snapshot_observed_at":"2026-08-06T16:29:19.586146Z","title":"Fast neutrino conversions: Ubiquitous in compact binary merger remnants","venue":"astro-ph.HE","work_id":"13d3d0dc-e9fd-46ee-8d67-54a1773b7ba7","year":2017},"citing_paper":{"arxiv_id":"2507.13429","last_updated":"2025-09-03T15:30:02Z","snapshot_observed_at":"2026-08-07T09:33:37.858372Z","submitted_at":"2025-07-17T18:00:00Z","title":"Electron-neutrino lepton number crossings: Variations with the supernova core physics","version":2},"reference_index":65,"source":"pdf_text","source_observed_at":"2026-08-06T16:29:18.905893Z"},"links":{"cited_paper":"/paper/1701.06580","citing_paper":"/paper/2507.13429"},"observation_digest":"sha256:3750328aa77a5c41964a5abaa715151ad8abf1da737439bb1703654941ca67a0","observation_id":"7ad648e1-2a21-4016-a65a-2b5e3776347b","resolution":{"observed_at":"2026-08-06T16:29:19.760549Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2503.23727","last_updated":"2025-03-31T05:01:52Z","snapshot_observed_at":"2026-08-07T16:26:10.907482Z","submitted_at":"2025-03-31T05:01:52Z","title":"Angle-dependent in-situ fast flavor transformations in post-neutron star merger disks","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2503.23727","snapshot_observed_at":"2026-08-06T16:29:19.030524Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2507.13429","last_updated":"2025-09-03T15:30:02Z","snapshot_observed_at":"2026-08-07T09:33:37.858372Z","submitted_at":"2025-07-17T18:00:00Z","title":"Electron-neutrino lepton number crossings: Variations with the supernova core physics","version":2},"reference_index":66,"source":"pdf_text","source_observed_at":"2026-08-06T16:29:19.030524Z"},"links":{"cited_paper":"/paper/2503.23727","citing_paper":"/paper/2507.13429"},"observation_digest":"sha256:08655590976ae0816a5d67649f27b9ea086f42e49d7559537cf4b8104e3588e9","observation_id":"8102616d-ed1a-4bfb-9fb2-283a4b62429a","resolution":{"observed_at":"2026-08-06T16:29:19.030524Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2404.17938","last_updated":"2024-04-27T15:32:24Z","snapshot_observed_at":"2026-08-06T15:19:00.896349Z","submitted_at":"2024-04-27T15:32:24Z","title":"The time evolution of fast flavor crossings in post-merger disks around a black hole remnant","version":1},"cited_work":{"arxiv_id":"2404.17938","doi":null,"metadata_source":"pith","pith_arxiv_id":"2404.17938","snapshot_observed_at":"2026-08-06T16:29:19.342636Z","title":"The time evolution of fast flavor crossings in post-merger disks around a black hole remnant","venue":"astro-ph.HE","work_id":"d7733c13-f38a-482e-9408-ce898ea6d5d9","year":2024},"citing_paper":{"arxiv_id":"2507.13429","last_updated":"2025-09-03T15:30:02Z","snapshot_observed_at":"2026-08-07T09:33:37.858372Z","submitted_at":"2025-07-17T18:00:00Z","title":"Electron-neutrino lepton number crossings: Variations with the supernova core physics","version":2},"reference_index":67,"source":"pdf_text","source_observed_at":"2026-08-06T16:29:19.198119Z"},"links":{"cited_paper":"/paper/2404.17938","citing_paper":"/paper/2507.13429"},"observation_digest":"sha256:1776b8765421f97479711c237b621d62a94822794b8ecc37439fa12a0c787b70","observation_id":"b31f6623-c8d0-446b-b0c5-0889f4ffbab2","resolution":{"observed_at":"2026-08-06T16:29:19.406727Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}}],"paper":{"arxiv_id":"2507.13429","last_updated":"2025-09-03T15:30:02Z","latest_version":2,"primary_category":"astro-ph.HE","snapshot_observed_at":"2026-08-07T09:33:37.858372Z","submitted_at":"2025-07-17T18:00:00Z","title":"Electron-neutrino lepton number crossings: Variations with the supernova core physics"},"reference_resolution":{"displayed":67,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":58,"verified_exact":8,"verified_fuzzy":1},"total_outbound_references":67},"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":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"thesis":"As of 7 August 2026, this Paper Citation Record lists 67 of 67 outbound references and 2 inbound Pith citation observations for arXiv:2507.13429."}