{"as_of":"2026-08-13T22:17:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:64dc30d0e57de06b0a1c8924ca6998242a3b509c5b65938d6557d60819122f1c","coverage":[{"denominator":74,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":74,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-12T22:01:13.146022Z","state":"measured"},{"denominator":74,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":74,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-13T06:32:02.005865+00:00","state":"measured"},{"denominator":0,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":0,"source":"paper_references, paper_reference_links","source_observed_at":null,"state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"cited_works","source_observed_at":null,"state":"measured"}],"external_citation_measurements":[],"inbound":[],"links":{"evidence":"/evidence","html":"/paper/2411.08023/citation-record","integrity":"/paper/2411.08023/integrity","json":"/paper/2411.08023/citation-record.json","paper":"/paper/2411.08023"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-12T22:01:14.349780Z","title":null,"venue":null,"work_id":"76dd5aa5-381c-404d-9b97-8e610f91dd55","year":null},"citing_paper":{"arxiv_id":"2411.08023","last_updated":"2025-01-21T17:34:00Z","snapshot_observed_at":"2026-08-12T21:57:43.085949Z","submitted_at":"2024-11-12T18:54:12Z","title":"How neutron star properties disfavor a nuclear chiral density wave","version":2},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-12T22:01:12.789869Z"},"links":{"citing_paper":"/paper/2411.08023"},"observation_digest":"sha256:35cd8aa379810f286de4596fab2cbe97d2f78c06fd991e7865a87c8199657708","observation_id":"5b5e049a-5d03-4e32-916e-6da12cb0f67a","resolution":{"observed_at":"2026-08-12T22:01:14.354921Z","resolver_source":"raw_fallback","status":"malformed_identifier"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+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":"2026-08-12T22:01:14.334570Z","title":"(48) Using the numerical values of all fixed physical parameters, the relations (46) yield functions gω = gω(dω, M0) , g ρ = gρ(dω, dωρ, M0)","venue":null,"work_id":"d6921842-822b-4d39-99c2-2eacdc903bb3","year":null},"citing_paper":{"arxiv_id":"2411.08023","last_updated":"2025-01-21T17:34:00Z","snapshot_observed_at":"2026-08-12T21:57:43.085949Z","submitted_at":"2024-11-12T18:54:12Z","title":"How neutron star properties disfavor a nuclear chiral density wave","version":2},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-12T22:01:12.795451Z"},"links":{"citing_paper":"/paper/2411.08023"},"observation_digest":"sha256:c713a2ebbf49cb99842014c388ea978cbaf0502b6af866d765ecb769662e4e65","observation_id":"e6ff1c95-92bf-44a9-b84e-1cfb3b1dd6af","resolution":{"observed_at":"2026-08-12T22:01:14.340148Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+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":"2026-08-12T22:01:14.319381Z","title":"reasonable","venue":null,"work_id":"5d45310b-0e72-4571-932b-e7e24ddca718","year":2000},"citing_paper":{"arxiv_id":"2411.08023","last_updated":"2025-01-21T17:34:00Z","snapshot_observed_at":"2026-08-12T21:57:43.085949Z","submitted_at":"2024-11-12T18:54:12Z","title":"How neutron star properties disfavor a nuclear chiral density wave","version":2},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-12T22:01:12.800480Z"},"links":{"citing_paper":"/paper/2411.08023"},"observation_digest":"sha256:53ca8da95e04887c7250259a671af299d82fce97694321ecba8f4a62ad03cfed","observation_id":"d4d4ee36-2c41-4128-b058-1eddae04abc8","resolution":{"observed_at":"2026-08-12T22:01:14.324448Z","resolver_source":"raw_fallback","status":"malformed_identifier"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1406.1367","last_updated":"2014-10-07T17:30:41Z","snapshot_observed_at":"2026-08-06T22:25:16.003511Z","submitted_at":"2014-06-05T12:50:35Z","title":"Inhomogeneous chiral condensates","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1406.1367","snapshot_observed_at":"2026-08-12T22:01:12.825851Z","title":"Buballa and S","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2411.08023","last_updated":"2025-01-21T17:34:00Z","snapshot_observed_at":"2026-08-12T21:57:43.085949Z","submitted_at":"2024-11-12T18:54:12Z","title":"How neutron star properties disfavor a nuclear chiral density wave","version":2},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-12T22:01:12.825851Z"},"links":{"cited_paper":"/paper/1406.1367","citing_paper":"/paper/2411.08023"},"observation_digest":"sha256:c4abb39a80f5bb0184a473f45d959940007ea99b0f09667740506c45d688baf7","observation_id":"061b4ae4-9f6b-467e-8fca-0211a252abd8","resolution":{"observed_at":"2026-08-12T22:01:12.825851Z","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":"2026-08-12T22:01:14.287664Z","title":"Dautry and E","venue":null,"work_id":"f51e4f95-0bb2-46a9-a39e-658678e4c619","year":1979},"citing_paper":{"arxiv_id":"2411.08023","last_updated":"2025-01-21T17:34:00Z","snapshot_observed_at":"2026-08-12T21:57:43.085949Z","submitted_at":"2024-11-12T18:54:12Z","title":"How neutron star properties disfavor a nuclear chiral density wave","version":2},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-12T22:01:12.811784Z"},"links":{"citing_paper":"/paper/2411.08023"},"observation_digest":"sha256:948688dd33632cf72111f0c15c16687145e99a137e08b1e5099d1082065ffbe4","observation_id":"9cf1b234-63f3-4ed5-8cc2-ea2b30c03dfa","resolution":{"observed_at":"2026-08-12T22:01:14.292534Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+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":"2026-08-12T22:01:14.272303Z","title":"Takahashi and T","venue":null,"work_id":"02f12f53-684a-4354-8984-1c1208fc37a0","year":2001},"citing_paper":{"arxiv_id":"2411.08023","last_updated":"2025-01-21T17:34:00Z","snapshot_observed_at":"2026-08-12T21:57:43.085949Z","submitted_at":"2024-11-12T18:54:12Z","title":"How neutron star properties disfavor a nuclear chiral density wave","version":2},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-12T22:01:12.816503Z"},"links":{"citing_paper":"/paper/2411.08023"},"observation_digest":"sha256:330203581b8f67b6f81ea1eadf4b5a23dedb0cd0677385a579308bc43dcc3dc2","observation_id":"112ab610-c523-4368-a413-1dd63903e48a","resolution":{"observed_at":"2026-08-12T22:01:14.277780Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+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":"2026-08-12T22:01:14.256673Z","title":"Takahashi, Phys","venue":null,"work_id":"0a8a29a6-8834-4f07-b2b9-ef2b588ac63a","year":2002},"citing_paper":{"arxiv_id":"2411.08023","last_updated":"2025-01-21T17:34:00Z","snapshot_observed_at":"2026-08-12T21:57:43.085949Z","submitted_at":"2024-11-12T18:54:12Z","title":"How neutron star properties disfavor a nuclear chiral density wave","version":2},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-12T22:01:12.821279Z"},"links":{"citing_paper":"/paper/2411.08023"},"observation_digest":"sha256:1534551faaa488ddf2c4dea7f8a622d3584eabe2985dd0ecbef3ea0e0085b55d","observation_id":"d4aa51e5-bf1d-406d-b92b-b3dbeb791367","resolution":{"observed_at":"2026-08-12T22:01:14.262154Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"0709.4635","last_updated":"2008-01-21T08:57:17Z","snapshot_observed_at":"2026-07-06T01:34:39.570334Z","submitted_at":"2007-09-28T18:31:24Z","title":"Color superconductivity in dense quark matter","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0709.4635","snapshot_observed_at":"2026-08-12T22:01:12.846694Z","title":null,"venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2411.08023","last_updated":"2025-01-21T17:34:00Z","snapshot_observed_at":"2026-08-12T21:57:43.085949Z","submitted_at":"2024-11-12T18:54:12Z","title":"How neutron star properties disfavor a nuclear chiral density wave","version":2},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-12T22:01:12.846694Z"},"links":{"cited_paper":"/paper/0709.4635","citing_paper":"/paper/2411.08023"},"observation_digest":"sha256:e386ee656abaa41b2a07cec08d8a7afb267c31552f8fa1c45fef5cd09574f235","observation_id":"78958cdc-bdb6-4dd4-b8e4-924bd0eba3c8","resolution":{"observed_at":"2026-08-12T22:01:12.846694Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"hep-ph/0008208","last_updated":"2001-01-06T19:59:03Z","snapshot_observed_at":"2026-08-12T11:24:41.977482Z","submitted_at":"2000-08-19T18:23:31Z","title":"Crystalline Color Superconductivity","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-ph/0008208","snapshot_observed_at":"2026-08-12T22:01:12.831163Z","title":null,"venue":null,"work_id":null,"year":2001},"citing_paper":{"arxiv_id":"2411.08023","last_updated":"2025-01-21T17:34:00Z","snapshot_observed_at":"2026-08-12T21:57:43.085949Z","submitted_at":"2024-11-12T18:54:12Z","title":"How neutron star properties disfavor a nuclear chiral density wave","version":2},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-12T22:01:12.831163Z"},"links":{"cited_paper":"/paper/hep-ph/0008208","citing_paper":"/paper/2411.08023"},"observation_digest":"sha256:10bda6ceb24b354960c89486329f2d93deca1576c74fb54285cfb21376275508","observation_id":"dda9d8b8-9f23-4b4c-92eb-f090eeb054ff","resolution":{"observed_at":"2026-08-12T22:01:12.831163Z","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":"2026-08-12T22:01:14.304109Z","title":"Therefore, a controlled approximation would require more sophisticated (strong-coupling) methods beyond our one-loop calculation of the pressure","venue":null,"work_id":"6920ca96-c870-4431-aeac-c4f9861beb99","year":null},"citing_paper":{"arxiv_id":"2411.08023","last_updated":"2025-01-21T17:34:00Z","snapshot_observed_at":"2026-08-12T21:57:43.085949Z","submitted_at":"2024-11-12T18:54:12Z","title":"How neutron star properties disfavor a nuclear chiral density wave","version":2},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-12T22:01:12.806609Z"},"links":{"citing_paper":"/paper/2411.08023"},"observation_digest":"sha256:2827bf460b3c18724b9b251972625dcb2aae31df0a532f6cc5d1fe0d3f9f234e","observation_id":"558b5542-693a-4900-bb97-60b7b88dcc46","resolution":{"observed_at":"2026-08-12T22:01:14.308989Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"hep-ph/0508190","last_updated":"2006-01-24T16:09:45Z","snapshot_observed_at":"2026-07-07T04:08:21.729706Z","submitted_at":"2005-08-17T19:03:30Z","title":"Meson Supercurrent State in High Density QCD","version":2},"cited_work":{"arxiv_id":"hep-ph/0508190","doi":null,"metadata_source":"pith","pith_arxiv_id":"hep-ph/0508190","snapshot_observed_at":"2026-08-12T22:01:14.023842Z","title":"Meson Supercurrent State in High Density QCD","venue":"hep-ph","work_id":"0c2879cb-7f77-4050-bb39-0d0361248443","year":2005},"citing_paper":{"arxiv_id":"2411.08023","last_updated":"2025-01-21T17:34:00Z","snapshot_observed_at":"2026-08-12T21:57:43.085949Z","submitted_at":"2024-11-12T18:54:12Z","title":"How neutron star properties disfavor a nuclear chiral density wave","version":2},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-12T22:01:12.836696Z"},"links":{"cited_paper":"/paper/hep-ph/0508190","citing_paper":"/paper/2411.08023"},"observation_digest":"sha256:799e36360690e35a99ee703eaff1c885b480c7fee4c74b2d97188d7cde6558b9","observation_id":"ea409658-1913-4274-b5cc-ca297064bfdd","resolution":{"observed_at":"2026-08-12T22:01:14.028332Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"hep-ph/0508180","last_updated":"2007-12-13T04:10:07Z","snapshot_observed_at":"2026-07-07T04:08:21.729706Z","submitted_at":"2005-08-16T18:26:27Z","title":"Spontaneous Superfluid Current Generation in CFL at Nonzero Strange Quark Mass","version":2},"cited_work":{"arxiv_id":"hep-ph/0508180","doi":null,"metadata_source":"pith","pith_arxiv_id":"hep-ph/0508180","snapshot_observed_at":"2026-08-12T22:01:14.002300Z","title":"Spontaneous Superfluid Current Generation in CFL at Nonzero Strange Quark Mass","venue":"hep-ph","work_id":"f80de012-3b86-4e38-9da0-b2d0f717e000","year":2005},"citing_paper":{"arxiv_id":"2411.08023","last_updated":"2025-01-21T17:34:00Z","snapshot_observed_at":"2026-08-12T21:57:43.085949Z","submitted_at":"2024-11-12T18:54:12Z","title":"How neutron star properties disfavor a nuclear chiral density wave","version":2},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-12T22:01:12.841778Z"},"links":{"cited_paper":"/paper/hep-ph/0508180","citing_paper":"/paper/2411.08023"},"observation_digest":"sha256:057d43eca6c048896f2c70fae12ff25b3b6c372951f60373d6ed4fae575d1ed0","observation_id":"8bdbf003-2ae6-476f-bf5a-1dc2b160f9f0","resolution":{"observed_at":"2026-08-12T22:01:14.007698Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2309.01603","last_updated":"2024-04-22T15:08:37Z","snapshot_observed_at":"2026-08-13T10:20:46.710006Z","submitted_at":"2023-09-04T13:38:33Z","title":"Chiral crossover vs chiral density wave in dense nuclear matter","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2309.01603","snapshot_observed_at":"2026-08-12T22:01:12.851700Z","title":"Pitsinigkos and A","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2411.08023","last_updated":"2025-01-21T17:34:00Z","snapshot_observed_at":"2026-08-12T21:57:43.085949Z","submitted_at":"2024-11-12T18:54:12Z","title":"How neutron star properties disfavor a nuclear chiral density wave","version":2},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-12T22:01:12.851700Z"},"links":{"cited_paper":"/paper/2309.01603","citing_paper":"/paper/2411.08023"},"observation_digest":"sha256:31b8958c4ab0e8b5caabb1d1126e0cefc2c91bfa5f9d7102187d8796eb67c0eb","observation_id":"dc118d7e-db51-4ca5-9663-2f47f2bae719","resolution":{"observed_at":"2026-08-12T22:01:12.851700Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0906.5295","last_updated":"2009-06-29T15:22:51Z","snapshot_observed_at":"2026-07-06T01:54:49.154542Z","submitted_at":"2009-06-29T15:22:51Z","title":"Inhomogeneous phases in the Nambu-Jona-Lasino and quark-meson model","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0906.5295","snapshot_observed_at":"2026-08-12T22:01:12.856688Z","title":"Nickel, Phys.Rev","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2411.08023","last_updated":"2025-01-21T17:34:00Z","snapshot_observed_at":"2026-08-12T21:57:43.085949Z","submitted_at":"2024-11-12T18:54:12Z","title":"How neutron star properties disfavor a nuclear chiral density wave","version":2},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-12T22:01:12.856688Z"},"links":{"cited_paper":"/paper/0906.5295","citing_paper":"/paper/2411.08023"},"observation_digest":"sha256:c464c9b7d5564fe1fda6094dd390e22d05e6a9115b19c5e63effe7db1ad9c502","observation_id":"02bc4a08-989a-4e24-a93b-d004e880f4e3","resolution":{"observed_at":"2026-08-12T22:01:12.856688Z","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":"2026-08-12T22:01:14.240880Z","title":"Boguta, Phys","venue":null,"work_id":"169153a2-4be4-48fb-bf9a-1247f52f93e9","year":1983},"citing_paper":{"arxiv_id":"2411.08023","last_updated":"2025-01-21T17:34:00Z","snapshot_observed_at":"2026-08-12T21:57:43.085949Z","submitted_at":"2024-11-12T18:54:12Z","title":"How neutron star properties disfavor a nuclear chiral density wave","version":2},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-12T22:01:12.861644Z"},"links":{"citing_paper":"/paper/2411.08023"},"observation_digest":"sha256:566c141652a09f2b6550ec5b338bd2f5fbe163a9691202bdedf4f450158f0812","observation_id":"74321a6b-4b8b-4a24-96cf-92971ac8c299","resolution":{"observed_at":"2026-08-12T22:01:14.245774Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+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":"2026-08-12T22:01:14.224475Z","title":"Boguta and J","venue":null,"work_id":"b886af14-6303-4c2d-afb4-e1d259e5d001","year":1989},"citing_paper":{"arxiv_id":"2411.08023","last_updated":"2025-01-21T17:34:00Z","snapshot_observed_at":"2026-08-12T21:57:43.085949Z","submitted_at":"2024-11-12T18:54:12Z","title":"How neutron star properties disfavor a nuclear chiral density wave","version":2},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-12T22:01:12.866280Z"},"links":{"citing_paper":"/paper/2411.08023"},"observation_digest":"sha256:a71066113b5fdbbce952e7a0fe6cb627380b294b11cebe7d42657382322c91c3","observation_id":"0867892e-a9a5-4163-8639-de68e0849a08","resolution":{"observed_at":"2026-08-12T22:01:14.230425Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1202.1671","last_updated":"2012-08-17T12:32:46Z","snapshot_observed_at":"2026-08-07T16:40:13.968507Z","submitted_at":"2012-02-08T12:19:47Z","title":"Chemical freeze-out in heavy ion collisions at large baryon densities","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1202.1671","snapshot_observed_at":"2026-08-12T22:01:12.870714Z","title":"Floerchinger and C","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2411.08023","last_updated":"2025-01-21T17:34:00Z","snapshot_observed_at":"2026-08-12T21:57:43.085949Z","submitted_at":"2024-11-12T18:54:12Z","title":"How neutron star properties disfavor a nuclear chiral density wave","version":2},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-12T22:01:12.870714Z"},"links":{"cited_paper":"/paper/1202.1671","citing_paper":"/paper/2411.08023"},"observation_digest":"sha256:96a92fc450ef839704465ab5e0386fd2d3ba8b242a3a9a0ae28e1365fb09ea25","observation_id":"68093b25-aa81-4038-af91-1b8cd22322ea","resolution":{"observed_at":"2026-08-12T22:01:12.870714Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1308.5596","last_updated":"2013-11-19T13:11:08Z","snapshot_observed_at":"2026-07-06T03:21:27.896144Z","submitted_at":"2013-08-26T14:25:10Z","title":"Thermodynamic phases and mesonic fluctuations in a chiral nucleon-meson model","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1308.5596","snapshot_observed_at":"2026-08-12T22:01:12.875471Z","title":"Drews, T","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2411.08023","last_updated":"2025-01-21T17:34:00Z","snapshot_observed_at":"2026-08-12T21:57:43.085949Z","submitted_at":"2024-11-12T18:54:12Z","title":"How neutron star properties disfavor a nuclear chiral density wave","version":2},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-12T22:01:12.875471Z"},"links":{"cited_paper":"/paper/1308.5596","citing_paper":"/paper/2411.08023"},"observation_digest":"sha256:c092513a3f54e83a5761b4146baf2167856ee0108cb68d6272a8ade5e05b4fbc","observation_id":"335cc154-e066-4abe-96be-dd1cb8905437","resolution":{"observed_at":"2026-08-12T22:01:12.875471Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1412.7655","last_updated":"2015-02-22T10:33:43Z","snapshot_observed_at":"2026-07-06T04:04:38.985181Z","submitted_at":"2014-12-24T12:40:39Z","title":"From asymmetric nuclear matter to neutron stars: a functional renormalization group study","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1412.7655","snapshot_observed_at":"2026-08-12T22:01:12.880190Z","title":"Drews and W","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2411.08023","last_updated":"2025-01-21T17:34:00Z","snapshot_observed_at":"2026-08-12T21:57:43.085949Z","submitted_at":"2024-11-12T18:54:12Z","title":"How neutron star properties disfavor a nuclear chiral density wave","version":2},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-12T22:01:12.880190Z"},"links":{"cited_paper":"/paper/1412.7655","citing_paper":"/paper/2411.08023"},"observation_digest":"sha256:2b745e362ced3a16190015bdbe37cc8d1ba99672a23eef9d6a72a3c03770d49f","observation_id":"ac9e4c3d-e064-4fd7-aea1-493c7dc961a1","resolution":{"observed_at":"2026-08-12T22:01:12.880190Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1810.13226","last_updated":"2019-01-23T10:55:35Z","snapshot_observed_at":"2026-08-06T07:47:49.741333Z","submitted_at":"2018-10-31T11:45:43Z","title":"Surface tension of dense matter at the chiral phase transition","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1810.13226","snapshot_observed_at":"2026-08-12T22:01:12.884691Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2411.08023","last_updated":"2025-01-21T17:34:00Z","snapshot_observed_at":"2026-08-12T21:57:43.085949Z","submitted_at":"2024-11-12T18:54:12Z","title":"How neutron star properties disfavor a nuclear chiral density wave","version":2},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-12T22:01:12.884691Z"},"links":{"cited_paper":"/paper/1810.13226","citing_paper":"/paper/2411.08023"},"observation_digest":"sha256:4064c42f51d9d16c8fd7d17e87eb686134bc1a5c85d924930af1890f3f4e3a84","observation_id":"cc0252ee-1233-43b6-a608-83211b4a6736","resolution":{"observed_at":"2026-08-12T22:01:12.884691Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2002.01451","last_updated":"2020-03-30T12:24:03Z","snapshot_observed_at":"2026-08-13T21:35:53.644752Z","submitted_at":"2020-02-04T18:27:22Z","title":"Chiral pasta","version":2},"cited_work":{"arxiv_id":"2002.01451","doi":null,"metadata_source":"pith","pith_arxiv_id":"2002.01451","snapshot_observed_at":"2026-08-12T22:01:13.880111Z","title":"Chiral pasta","venue":"hep-ph","work_id":"a78f4533-1d13-4afa-b22c-4afa0b697e06","year":2020},"citing_paper":{"arxiv_id":"2411.08023","last_updated":"2025-01-21T17:34:00Z","snapshot_observed_at":"2026-08-12T21:57:43.085949Z","submitted_at":"2024-11-12T18:54:12Z","title":"How neutron star properties disfavor a nuclear chiral density wave","version":2},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-12T22:01:12.889486Z"},"links":{"cited_paper":"/paper/2002.01451","citing_paper":"/paper/2411.08023"},"observation_digest":"sha256:ab459bbcbf0271594a33f480578a4796601fb0da445dfe1f4268f9ba8a599685","observation_id":"572612bf-15de-4cd6-a34f-6e07514a30c8","resolution":{"observed_at":"2026-08-12T22:01:13.885428Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2206.09219","last_updated":"2022-09-27T16:57:49Z","snapshot_observed_at":"2026-08-13T15:20:55.830962Z","submitted_at":"2022-06-18T14:48:00Z","title":"Strange quark matter from a baryonic approach","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2206.09219","snapshot_observed_at":"2026-08-12T22:01:12.894061Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2411.08023","last_updated":"2025-01-21T17:34:00Z","snapshot_observed_at":"2026-08-12T21:57:43.085949Z","submitted_at":"2024-11-12T18:54:12Z","title":"How neutron star properties disfavor a nuclear chiral density wave","version":2},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-12T22:01:12.894061Z"},"links":{"cited_paper":"/paper/2206.09219","citing_paper":"/paper/2411.08023"},"observation_digest":"sha256:bd0b6ac87c6501be237cbd05c02163d1ce8f5a40e0e8c2a455286b9503bc4461","observation_id":"c6e84612-97ac-417f-8e4c-011107a5e8d7","resolution":{"observed_at":"2026-08-12T22:01:12.894061Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"hep-ph/0411350","last_updated":"2005-05-21T07:26:51Z","snapshot_observed_at":"2026-07-07T04:05:47.156737Z","submitted_at":"2004-11-27T05:24:59Z","title":"Chiral symmetry and density wave in quark matter","version":5},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-ph/0411350","snapshot_observed_at":"2026-08-12T22:01:12.898800Z","title":"Nakano and T","venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2411.08023","last_updated":"2025-01-21T17:34:00Z","snapshot_observed_at":"2026-08-12T21:57:43.085949Z","submitted_at":"2024-11-12T18:54:12Z","title":"How neutron star properties disfavor a nuclear chiral density wave","version":2},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-12T22:01:12.898800Z"},"links":{"cited_paper":"/paper/hep-ph/0411350","citing_paper":"/paper/2411.08023"},"observation_digest":"sha256:5ffbe99fc7b8d18db30db1b803fa6b904d0f4f7594a86a0214b6a7bef5d7edaf","observation_id":"103a0a9c-727b-4c81-ac88-f7210af1d9a6","resolution":{"observed_at":"2026-08-12T22:01:12.898800Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1007.2984","last_updated":"2010-10-11T19:57:42Z","snapshot_observed_at":"2026-07-06T02:13:01.945417Z","submitted_at":"2010-07-18T09:51:19Z","title":"Chiral density waves in quark matter within the Nambu--Jona-Lasinio model in an external magnetic field","version":3},"cited_work":{"arxiv_id":"1007.2984","doi":null,"metadata_source":"pith","pith_arxiv_id":"1007.2984","snapshot_observed_at":"2026-08-12T22:01:13.830063Z","title":"Chiral density waves in quark matter within the Nambu--Jona-Lasinio model in an external magnetic field","venue":"hep-ph","work_id":"23770c32-6063-4e2c-ba39-2cb9be6dfa4a","year":2010},"citing_paper":{"arxiv_id":"2411.08023","last_updated":"2025-01-21T17:34:00Z","snapshot_observed_at":"2026-08-12T21:57:43.085949Z","submitted_at":"2024-11-12T18:54:12Z","title":"How neutron star properties disfavor a nuclear chiral density wave","version":2},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-12T22:01:12.903815Z"},"links":{"cited_paper":"/paper/1007.2984","citing_paper":"/paper/2411.08023"},"observation_digest":"sha256:b1f510b40eab6ecba549c8d3b99478fc6a3a393cfc310e77e3b60dfa4dfb9ae5","observation_id":"a6d7bd9f-e518-4068-8e2b-5f627f65920c","resolution":{"observed_at":"2026-08-12T22:01:13.835066Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1111.4400","last_updated":"2012-03-01T16:05:27Z","snapshot_observed_at":"2026-07-06T02:37:49.738393Z","submitted_at":"2011-11-18T15:44:21Z","title":"Inhomogeneous islands and continents in the Nambu--Jona-Lasinio model","version":2},"cited_work":{"arxiv_id":"1111.4400","doi":null,"metadata_source":"pith","pith_arxiv_id":"1111.4400","snapshot_observed_at":"2026-08-12T22:01:13.809455Z","title":"Inhomogeneous islands and continents in the Nambu--Jona-Lasinio model","venue":"hep-ph","work_id":"9c9e6f48-fa0f-4950-99bf-4b8fcbf43afc","year":2011},"citing_paper":{"arxiv_id":"2411.08023","last_updated":"2025-01-21T17:34:00Z","snapshot_observed_at":"2026-08-12T21:57:43.085949Z","submitted_at":"2024-11-12T18:54:12Z","title":"How neutron star properties disfavor a nuclear chiral density wave","version":2},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-12T22:01:12.908832Z"},"links":{"cited_paper":"/paper/1111.4400","citing_paper":"/paper/2411.08023"},"observation_digest":"sha256:dcabc0ba33f948980b7b17f96876277416654d9a168da44e2c3b3071b494dc26","observation_id":"9472cb21-8085-48f0-92d1-f12494ba3b38","resolution":{"observed_at":"2026-08-12T22:01:13.814276Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1404.0057","last_updated":"2014-07-09T23:53:21Z","snapshot_observed_at":"2026-07-06T03:40:00.436979Z","submitted_at":"2014-03-31T22:43:42Z","title":"Inhomogeneous phases in the quark-meson model with vacuum fluctuations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1404.0057","snapshot_observed_at":"2026-08-12T22:01:12.913524Z","title":"Carignano, M","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2411.08023","last_updated":"2025-01-21T17:34:00Z","snapshot_observed_at":"2026-08-12T21:57:43.085949Z","submitted_at":"2024-11-12T18:54:12Z","title":"How neutron star properties disfavor a nuclear chiral density wave","version":2},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-12T22:01:12.913524Z"},"links":{"cited_paper":"/paper/1404.0057","citing_paper":"/paper/2411.08023"},"observation_digest":"sha256:c4123513627218d3ff3760f5cc2955e13d59859b7626daac21f62b6317a18af9","observation_id":"1f3965be-f604-410f-9b5e-30a63c6303b0","resolution":{"observed_at":"2026-08-12T22:01:12.913524Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1508.04361","last_updated":"2016-04-29T15:23:10Z","snapshot_observed_at":"2026-07-06T04:27:00.684723Z","submitted_at":"2015-08-18T15:47:12Z","title":"Inhomogeneous chiral symmetry breaking in dense neutron-star matter","version":2},"cited_work":{"arxiv_id":"1508.04361","doi":null,"metadata_source":"pith","pith_arxiv_id":"1508.04361","snapshot_observed_at":"2026-08-12T22:01:13.772738Z","title":"Inhomogeneous chiral symmetry breaking in dense neutron-star matter","venue":"nucl-th","work_id":"3504207c-535b-4bd2-a244-8389ba236d42","year":2015},"citing_paper":{"arxiv_id":"2411.08023","last_updated":"2025-01-21T17:34:00Z","snapshot_observed_at":"2026-08-12T21:57:43.085949Z","submitted_at":"2024-11-12T18:54:12Z","title":"How neutron star properties disfavor a nuclear chiral density wave","version":2},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-12T22:01:12.918375Z"},"links":{"cited_paper":"/paper/1508.04361","citing_paper":"/paper/2411.08023"},"observation_digest":"sha256:d817d458522e6cdfc92d1fc1433e7653f66c5a8ffed73ad55469e2816d6e8815","observation_id":"f926aa54-31bf-4d09-b745-d36988dae4e4","resolution":{"observed_at":"2026-08-12T22:01:13.777949Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1702.01324","last_updated":"2017-10-06T09:54:52Z","snapshot_observed_at":"2026-07-06T05:28:49.510456Z","submitted_at":"2017-02-04T18:52:00Z","title":"Inhomogeneous chiral condensate in the quark-meson model","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1702.01324","snapshot_observed_at":"2026-08-12T22:01:12.923359Z","title":"Adhikari, J","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2411.08023","last_updated":"2025-01-21T17:34:00Z","snapshot_observed_at":"2026-08-12T21:57:43.085949Z","submitted_at":"2024-11-12T18:54:12Z","title":"How neutron star properties disfavor a nuclear chiral density wave","version":2},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-12T22:01:12.923359Z"},"links":{"cited_paper":"/paper/1702.01324","citing_paper":"/paper/2411.08023"},"observation_digest":"sha256:7fa36545f2991fe012569f9ccc614fa1b7feda460d0801f0562a48bdd0287993","observation_id":"4e6c0c07-9a4b-4529-b772-f1b15aedf92e","resolution":{"observed_at":"2026-08-12T22:01:12.923359Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1802.01832","last_updated":"2018-04-17T15:47:00Z","snapshot_observed_at":"2026-07-06T06:21:56.000483Z","submitted_at":"2018-02-06T07:48:45Z","title":"Chiral density wave versus pion condensation at finite density","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1802.01832","snapshot_observed_at":"2026-08-12T22:01:12.928103Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2411.08023","last_updated":"2025-01-21T17:34:00Z","snapshot_observed_at":"2026-08-12T21:57:43.085949Z","submitted_at":"2024-11-12T18:54:12Z","title":"How neutron star properties disfavor a nuclear chiral density wave","version":2},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-12T22:01:12.928103Z"},"links":{"cited_paper":"/paper/1802.01832","citing_paper":"/paper/2411.08023"},"observation_digest":"sha256:6a728629892d0c4688604bd59e4a25d27a2b02172f8dc4d561b827f46cb8d6e1","observation_id":"1c6e3bf0-5974-4474-a746-06f6f1a652ea","resolution":{"observed_at":"2026-08-12T22:01:12.928103Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1902.06810","last_updated":"2020-05-09T23:17:19Z","snapshot_observed_at":"2026-08-04T18:29:36.685454Z","submitted_at":"2019-02-18T21:51:50Z","title":"Absence of Landau-Peierls Instability in the Magnetic Dual Chiral Density Wave Phase of Dense QCD","version":3},"cited_work":{"arxiv_id":"1902.06810","doi":null,"metadata_source":"pith","pith_arxiv_id":"1902.06810","snapshot_observed_at":"2026-08-12T22:01:13.723343Z","title":"Absence of Landau-Peierls Instability in the Magnetic Dual Chiral Density Wave Phase of Dense QCD","venue":"nucl-th","work_id":"706d33c4-d5b9-499b-b54c-e6ad298f337a","year":2019},"citing_paper":{"arxiv_id":"2411.08023","last_updated":"2025-01-21T17:34:00Z","snapshot_observed_at":"2026-08-12T21:57:43.085949Z","submitted_at":"2024-11-12T18:54:12Z","title":"How neutron star properties disfavor a nuclear chiral density wave","version":2},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-12T22:01:12.932897Z"},"links":{"cited_paper":"/paper/1902.06810","citing_paper":"/paper/2411.08023"},"observation_digest":"sha256:8cd27bfca8d2bb53e182a5e340ce2dde90d36026e9aeb3b3de4ca002849b94fe","observation_id":"72b1cbbe-9387-49bb-af2e-384847af98c2","resolution":{"observed_at":"2026-08-12T22:01:13.728222Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1910.03604","last_updated":"2020-02-10T16:38:02Z","snapshot_observed_at":"2026-07-06T08:27:52.322036Z","submitted_at":"2019-10-08T18:00:14Z","title":"Inhomogeneous chiral condensates in three-flavor quark matter","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1910.03604","snapshot_observed_at":"2026-08-12T22:01:12.938004Z","title":"Carignano and M","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2411.08023","last_updated":"2025-01-21T17:34:00Z","snapshot_observed_at":"2026-08-12T21:57:43.085949Z","submitted_at":"2024-11-12T18:54:12Z","title":"How neutron star properties disfavor a nuclear chiral density wave","version":2},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-08-12T22:01:12.938004Z"},"links":{"cited_paper":"/paper/1910.03604","citing_paper":"/paper/2411.08023"},"observation_digest":"sha256:3ba7b2b705cf8380bcf0883c76b1885a4677bff22ce7ae56c318cf70724a8661","observation_id":"bba199cb-4769-47c0-b5e2-3bba7110caab","resolution":{"observed_at":"2026-08-12T22:01:12.938004Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2012.07520","last_updated":"2020-12-14T13:52:20Z","snapshot_observed_at":"2026-07-06T10:24:12.354087Z","submitted_at":"2020-12-14T13:52:20Z","title":"Competition of inhomogeneous chiral phases and two-flavor color superconductivity in the NJL model","version":1},"cited_work":{"arxiv_id":"2012.07520","doi":null,"metadata_source":"pith","pith_arxiv_id":"2012.07520","snapshot_observed_at":"2026-08-12T22:01:13.688100Z","title":"Competition of inhomogeneous chiral phases and two-flavor color superconductivity in the NJL model","venue":"hep-ph","work_id":"56937952-d5dc-4181-8771-bb9548224c67","year":2020},"citing_paper":{"arxiv_id":"2411.08023","last_updated":"2025-01-21T17:34:00Z","snapshot_observed_at":"2026-08-12T21:57:43.085949Z","submitted_at":"2024-11-12T18:54:12Z","title":"How neutron star properties disfavor a nuclear chiral density wave","version":2},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-12T22:01:12.942962Z"},"links":{"cited_paper":"/paper/2012.07520","citing_paper":"/paper/2411.08023"},"observation_digest":"sha256:a13ebdf6d141f5ac211dfca527c04062ad0299ce64f9c34785023d2941fb6557","observation_id":"c7e31a8d-4e2c-4d32-bdaf-1b249f13ae29","resolution":{"observed_at":"2026-08-12T22:01:13.693154Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2006.02133","last_updated":"2021-01-05T16:50:07Z","snapshot_observed_at":"2026-08-13T19:49:48.366032Z","submitted_at":"2020-06-03T10:01:20Z","title":"Inhomogeneous phases in the quark-meson model with explicit chiral-symmetry breaking","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2006.02133","snapshot_observed_at":"2026-08-12T22:01:12.948155Z","title":"Buballa, S","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2411.08023","last_updated":"2025-01-21T17:34:00Z","snapshot_observed_at":"2026-08-12T21:57:43.085949Z","submitted_at":"2024-11-12T18:54:12Z","title":"How neutron star properties disfavor a nuclear chiral density wave","version":2},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-12T22:01:12.948155Z"},"links":{"cited_paper":"/paper/2006.02133","citing_paper":"/paper/2411.08023"},"observation_digest":"sha256:19686857a0eddfafa1658684009395d23774158467332174f3e181e0214355bb","observation_id":"70546367-29fa-49a2-9937-3f503ebd9dbd","resolution":{"observed_at":"2026-08-12T22:01:12.948155Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1312.3244","last_updated":"2014-12-19T15:01:35Z","snapshot_observed_at":"2026-07-06T03:30:37.076367Z","submitted_at":"2013-12-11T17:04:12Z","title":"Chiral density wave in nuclear matter","version":2},"cited_work":{"arxiv_id":"1312.3244","doi":null,"metadata_source":"pith","pith_arxiv_id":"1312.3244","snapshot_observed_at":"2026-08-12T22:01:13.653122Z","title":"Chiral density wave in nuclear matter","venue":"nucl-th","work_id":"c4cfca90-53ef-4c5a-b723-615a44c378b6","year":2013},"citing_paper":{"arxiv_id":"2411.08023","last_updated":"2025-01-21T17:34:00Z","snapshot_observed_at":"2026-08-12T21:57:43.085949Z","submitted_at":"2024-11-12T18:54:12Z","title":"How neutron star properties disfavor a nuclear chiral density wave","version":2},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-12T22:01:12.953106Z"},"links":{"cited_paper":"/paper/1312.3244","citing_paper":"/paper/2411.08023"},"observation_digest":"sha256:d5c0121cc9ec40ff64dd1a872d51d3828ceaa8769b27aa8c210107fe7ffbb67d","observation_id":"069e3c51-5115-4983-b289-1a67d7bac726","resolution":{"observed_at":"2026-08-12T22:01:13.657978Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1803.06779","last_updated":"2018-03-19T01:46:16Z","snapshot_observed_at":"2026-07-06T06:28:55.242298Z","submitted_at":"2018-03-19T01:46:16Z","title":"A novel Dual Chiral Density Wave in nuclear matter based on a parity doublet structure","version":1},"cited_work":{"arxiv_id":"1803.06779","doi":null,"metadata_source":"pith","pith_arxiv_id":"1803.06779","snapshot_observed_at":"2026-08-12T22:01:13.632921Z","title":"A novel Dual Chiral Density Wave in nuclear matter based on a parity doublet structure","venue":"hep-ph","work_id":"1a25d547-8ab5-4b46-bb0d-ac90e9a2c377","year":2018},"citing_paper":{"arxiv_id":"2411.08023","last_updated":"2025-01-21T17:34:00Z","snapshot_observed_at":"2026-08-12T21:57:43.085949Z","submitted_at":"2024-11-12T18:54:12Z","title":"How neutron star properties disfavor a nuclear chiral density wave","version":2},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-12T22:01:12.958143Z"},"links":{"cited_paper":"/paper/1803.06779","citing_paper":"/paper/2411.08023"},"observation_digest":"sha256:736854ffb91dd960ae67b57c13caf2f12ed9f3f576f5e891db3396efbdded9ec","observation_id":"f7b1eb96-f749-4e15-9fbd-743f90909daf","resolution":{"observed_at":"2026-08-12T22:01:13.638148Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1109.1615","last_updated":"2012-03-30T02:16:03Z","snapshot_observed_at":"2026-07-06T02:33:40.228653Z","submitted_at":"2011-09-08T02:44:59Z","title":"Crystalline chiral condensates off the tricritical point in a generalized Ginzburg-Landau approach","version":3},"cited_work":{"arxiv_id":"1109.1615","doi":null,"metadata_source":"pith","pith_arxiv_id":"1109.1615","snapshot_observed_at":"2026-08-12T22:01:13.612687Z","title":"Crystalline chiral condensates off the tricritical point in a generalized Ginzburg-Landau approach","venue":"hep-ph","work_id":"4db825d6-2cfc-4dbe-ae31-c09b6de98992","year":2011},"citing_paper":{"arxiv_id":"2411.08023","last_updated":"2025-01-21T17:34:00Z","snapshot_observed_at":"2026-08-12T21:57:43.085949Z","submitted_at":"2024-11-12T18:54:12Z","title":"How neutron star properties disfavor a nuclear chiral density wave","version":2},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-12T22:01:12.962941Z"},"links":{"cited_paper":"/paper/1109.1615","citing_paper":"/paper/2411.08023"},"observation_digest":"sha256:a92151211781d2a8c62b2ec6e3c5ae7edd0e30dde9681b5eb555325c325e7876","observation_id":"8f6c5713-a00a-4fc8-baf0-0942c2620ca7","resolution":{"observed_at":"2026-08-12T22:01:13.617782Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1203.5343","last_updated":"2012-10-31T18:08:59Z","snapshot_observed_at":"2026-07-06T02:45:07.089504Z","submitted_at":"2012-03-23T20:00:27Z","title":"Two-dimensional chiral crystals in the NJL model","version":2},"cited_work":{"arxiv_id":"1203.5343","doi":null,"metadata_source":"pith","pith_arxiv_id":"1203.5343","snapshot_observed_at":"2026-08-12T22:01:13.591504Z","title":"Two-dimensional chiral crystals in the NJL model","venue":"hep-ph","work_id":"863fda2a-c803-4fe2-827c-5d4bfb0c6881","year":2012},"citing_paper":{"arxiv_id":"2411.08023","last_updated":"2025-01-21T17:34:00Z","snapshot_observed_at":"2026-08-12T21:57:43.085949Z","submitted_at":"2024-11-12T18:54:12Z","title":"How neutron star properties disfavor a nuclear chiral density wave","version":2},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-12T22:01:12.967814Z"},"links":{"cited_paper":"/paper/1203.5343","citing_paper":"/paper/2411.08023"},"observation_digest":"sha256:663274c37a4369c0a4cedc4bd63e06010166e952f863a4b09236150e07e1793a","observation_id":"29c8508c-1840-43bf-a2c8-0e30c7eab238","resolution":{"observed_at":"2026-08-12T22:01:13.596482Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2005.10259","last_updated":"2020-06-09T20:22:41Z","snapshot_observed_at":"2026-08-12T05:26:34.229949Z","submitted_at":"2020-05-20T18:00:01Z","title":"How transverse thermal fluctuations disorder a condensate of chiral spirals into a quantum spin liquid","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2005.10259","snapshot_observed_at":"2026-08-12T22:01:12.972886Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2411.08023","last_updated":"2025-01-21T17:34:00Z","snapshot_observed_at":"2026-08-12T21:57:43.085949Z","submitted_at":"2024-11-12T18:54:12Z","title":"How neutron star properties disfavor a nuclear chiral density wave","version":2},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-12T22:01:12.972886Z"},"links":{"cited_paper":"/paper/2005.10259","citing_paper":"/paper/2411.08023"},"observation_digest":"sha256:bd4b0ed9012fd3ad5a4ae3ef4c5f9a169208f824868ed83e9d9365ed9e3508f1","observation_id":"de4a136b-7d40-4787-a56b-9d6e93dc8053","resolution":{"observed_at":"2026-08-12T22:01:12.972886Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2403.18640","last_updated":"2024-03-27T14:45:05Z","snapshot_observed_at":"2026-08-13T19:52:55.097087Z","submitted_at":"2024-03-27T14:45:05Z","title":"Lattice study of disordering of inhomogeneous condensates and the Quantum Pion Liquid in effective $O(N)$ model","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2403.18640","snapshot_observed_at":"2026-08-12T22:01:12.977745Z","title":"Winstel and S","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2411.08023","last_updated":"2025-01-21T17:34:00Z","snapshot_observed_at":"2026-08-12T21:57:43.085949Z","submitted_at":"2024-11-12T18:54:12Z","title":"How neutron star properties disfavor a nuclear chiral density wave","version":2},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-08-12T22:01:12.977745Z"},"links":{"cited_paper":"/paper/2403.18640","citing_paper":"/paper/2411.08023"},"observation_digest":"sha256:29d5c46e781d1036addc4719e75463b476b312e39aeca465b4eab1b02f87be32","observation_id":"25786b87-60a3-4fb0-bdfc-b421555985cc","resolution":{"observed_at":"2026-08-12T22:01:12.977745Z","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":"2026-08-12T22:01:12.983024Z","title":null,"venue":null,"work_id":null,"year":1992},"citing_paper":{"arxiv_id":"2411.08023","last_updated":"2025-01-21T17:34:00Z","snapshot_observed_at":"2026-08-12T21:57:43.085949Z","submitted_at":"2024-11-12T18:54:12Z","title":"How neutron star properties disfavor a nuclear chiral density wave","version":2},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-08-12T22:01:12.983024Z"},"links":{"citing_paper":"/paper/2411.08023"},"observation_digest":"sha256:59b9d61f9fc9f35083ad0d15268c18c2c0c60b39219fc1ab501d814414b6a55d","observation_id":"eef89f60-6a6c-4aa7-8331-62a990bbf0f5","resolution":{"observed_at":"2026-08-12T22:01:12.983024Z","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":"2026-08-12T22:01:14.201274Z","title":"Heiselberg, C","venue":null,"work_id":"1f35899d-2071-4ab3-9344-e1d12c6b824f","year":1993},"citing_paper":{"arxiv_id":"2411.08023","last_updated":"2025-01-21T17:34:00Z","snapshot_observed_at":"2026-08-12T21:57:43.085949Z","submitted_at":"2024-11-12T18:54:12Z","title":"How neutron star properties disfavor a nuclear chiral density wave","version":2},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-08-12T22:01:12.987832Z"},"links":{"citing_paper":"/paper/2411.08023"},"observation_digest":"sha256:735ded1cbf9210d8022c6c789a5df5ce825d33c70a4ca312157a7d826b6ad0fd","observation_id":"90452c11-20ed-45fb-aca9-fc2b407fc5b5","resolution":{"observed_at":"2026-08-12T22:01:14.205727Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1505.05094","last_updated":"2015-11-04T17:48:35Z","snapshot_observed_at":"2026-07-06T04:18:19.357036Z","submitted_at":"2015-05-19T17:27:47Z","title":"Crystalline chiral condensates as a component of compact stars","version":2},"cited_work":{"arxiv_id":"1505.05094","doi":null,"metadata_source":"pith","pith_arxiv_id":"1505.05094","snapshot_observed_at":"2026-08-12T22:01:13.539885Z","title":"Crystalline chiral condensates as a component of compact stars","venue":"nucl-th","work_id":"b6e77ab2-e213-421b-80df-8730f781b745","year":2015},"citing_paper":{"arxiv_id":"2411.08023","last_updated":"2025-01-21T17:34:00Z","snapshot_observed_at":"2026-08-12T21:57:43.085949Z","submitted_at":"2024-11-12T18:54:12Z","title":"How neutron star properties disfavor a nuclear chiral density wave","version":2},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-08-12T22:01:12.992861Z"},"links":{"cited_paper":"/paper/1505.05094","citing_paper":"/paper/2411.08023"},"observation_digest":"sha256:e4a994d77dc01dd8baad01e6ddfda032fcc50851185a5890b62b24d4211b0f67","observation_id":"7a12b478-ddc5-4dd8-ba26-30d9189e4a46","resolution":{"observed_at":"2026-08-12T22:01:13.545830Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2201.04032","last_updated":"2022-01-11T16:28:02Z","snapshot_observed_at":"2026-08-13T17:00:42.344740Z","submitted_at":"2022-01-11T16:28:02Z","title":"Magnetic Dual Chiral Density Wave: A Candidate Quark Matter Phase for the Interior of Neutron Stars","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2201.04032","snapshot_observed_at":"2026-08-12T22:01:12.997901Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2411.08023","last_updated":"2025-01-21T17:34:00Z","snapshot_observed_at":"2026-08-12T21:57:43.085949Z","submitted_at":"2024-11-12T18:54:12Z","title":"How neutron star properties disfavor a nuclear chiral density wave","version":2},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-08-12T22:01:12.997901Z"},"links":{"cited_paper":"/paper/2201.04032","citing_paper":"/paper/2411.08023"},"observation_digest":"sha256:09b76caaf475e5c33f17f681fd52d2e53b13dbcf0b7504e2de112102e9e50d73","observation_id":"57bbd09f-2b3d-45dd-af45-ac7f0fd62bea","resolution":{"observed_at":"2026-08-12T22:01:12.997901Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1403.1927","last_updated":"2014-03-08T03:47:59Z","snapshot_observed_at":"2026-07-06T03:37:56.276162Z","submitted_at":"2014-03-08T03:47:59Z","title":"Quark beta decay in the inhomogeneous chiral phase and cooling of compact stars","version":1},"cited_work":{"arxiv_id":"1403.1927","doi":null,"metadata_source":"pith","pith_arxiv_id":"1403.1927","snapshot_observed_at":"2026-08-12T22:01:13.504440Z","title":"Quark beta decay in the inhomogeneous chiral phase and cooling of compact stars","venue":"nucl-th","work_id":"7f4c857c-1de8-4e07-8925-62e09eb2c6a0","year":2014},"citing_paper":{"arxiv_id":"2411.08023","last_updated":"2025-01-21T17:34:00Z","snapshot_observed_at":"2026-08-12T21:57:43.085949Z","submitted_at":"2024-11-12T18:54:12Z","title":"How neutron star properties disfavor a nuclear chiral density wave","version":2},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-08-12T22:01:13.002692Z"},"links":{"cited_paper":"/paper/1403.1927","citing_paper":"/paper/2411.08023"},"observation_digest":"sha256:5adf7f638acee795648cc97523f29616d34cfd3c44d8fd8f3733890f6fb23c2e","observation_id":"74d812d6-8b05-417b-98c3-fca0a73bec33","resolution":{"observed_at":"2026-08-12T22:01:13.509673Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1801.01923","last_updated":"2018-06-25T20:56:27Z","snapshot_observed_at":"2026-08-13T20:54:00.304892Z","submitted_at":"2018-01-05T21:28:09Z","title":"Constraining the speed of sound inside neutron stars with chiral effective field theory interactions and observations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1801.01923","snapshot_observed_at":"2026-08-12T22:01:13.007330Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2411.08023","last_updated":"2025-01-21T17:34:00Z","snapshot_observed_at":"2026-08-12T21:57:43.085949Z","submitted_at":"2024-11-12T18:54:12Z","title":"How neutron star properties disfavor a nuclear chiral density wave","version":2},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-08-12T22:01:13.007330Z"},"links":{"cited_paper":"/paper/1801.01923","citing_paper":"/paper/2411.08023"},"observation_digest":"sha256:3c7dc03def6afb9a457c922a0adbdb8d82b875e1110601f988e5da3bee4467e5","observation_id":"afccc97c-7982-4367-9d5a-6aa1a2ee1664","resolution":{"observed_at":"2026-08-12T22:01:13.007330Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2205.10283","last_updated":"2022-11-21T21:18:21Z","snapshot_observed_at":"2026-08-13T15:39:56.567643Z","submitted_at":"2022-05-20T16:28:37Z","title":"Relativistic mean-field theories for neutron-star physics based on chiral effective field theory","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2205.10283","snapshot_observed_at":"2026-08-12T22:01:13.012097Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2411.08023","last_updated":"2025-01-21T17:34:00Z","snapshot_observed_at":"2026-08-12T21:57:43.085949Z","submitted_at":"2024-11-12T18:54:12Z","title":"How neutron star properties disfavor a nuclear chiral density wave","version":2},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-08-12T22:01:13.012097Z"},"links":{"cited_paper":"/paper/2205.10283","citing_paper":"/paper/2411.08023"},"observation_digest":"sha256:0a1420cdfb8a3f18cb1a4a4dc8d6a37d0689d14011462fef44a16160f859fdcf","observation_id":"4e1f0027-277c-42b8-9699-7db0d7d8b8f0","resolution":{"observed_at":"2026-08-12T22:01:13.012097Z","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":"2026-08-12T22:01:14.187601Z","title":null,"venue":null,"work_id":"d24339a1-adef-4394-9eff-32840e664873","year":2000},"citing_paper":{"arxiv_id":"2411.08023","last_updated":"2025-01-21T17:34:00Z","snapshot_observed_at":"2026-08-12T21:57:43.085949Z","submitted_at":"2024-11-12T18:54:12Z","title":"How neutron star properties disfavor a nuclear chiral density wave","version":2},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-08-12T22:01:13.016967Z"},"links":{"citing_paper":"/paper/2411.08023"},"observation_digest":"sha256:a9af1ee376e4a87992fac0457bcefa9a9206679fa6d451b85d7d1f905b6a4799","observation_id":"d16b0192-02ed-4d18-8588-8a713edbdf15","resolution":{"observed_at":"2026-08-12T22:01:14.191982Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"nucl-th/0410066","last_updated":"2005-02-17T21:00:17Z","snapshot_observed_at":"2026-07-07T06:34:46.907694Z","submitted_at":"2004-10-14T14:36:38Z","title":"Isospin Asymmetry in Nuclei and Neutron Stars","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"nucl-th/0410066","snapshot_observed_at":"2026-08-12T22:01:13.021490Z","title":null,"venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2411.08023","last_updated":"2025-01-21T17:34:00Z","snapshot_observed_at":"2026-08-12T21:57:43.085949Z","submitted_at":"2024-11-12T18:54:12Z","title":"How neutron star properties disfavor a nuclear chiral density wave","version":2},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-08-12T22:01:13.021490Z"},"links":{"cited_paper":"/paper/nucl-th/0410066","citing_paper":"/paper/2411.08023"},"observation_digest":"sha256:86073e120da52f6dfe412a3ef74e547db61ff4ff5e2691f18b6b7e97218121e8","observation_id":"1b4ed410-07a1-43ee-8106-f06576de7d3e","resolution":{"observed_at":"2026-08-12T22:01:13.021490Z","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":"2026-08-12T22:01:14.171874Z","title":"Kapusta and C","venue":null,"work_id":"0e3704bb-0ddd-4130-b409-e2863d74948e","year":2023},"citing_paper":{"arxiv_id":"2411.08023","last_updated":"2025-01-21T17:34:00Z","snapshot_observed_at":"2026-08-12T21:57:43.085949Z","submitted_at":"2024-11-12T18:54:12Z","title":"How neutron star properties disfavor a nuclear chiral density wave","version":2},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-08-12T22:01:13.026542Z"},"links":{"citing_paper":"/paper/2411.08023"},"observation_digest":"sha256:dd6e6d9d448a33ea5cd49fce30e9e5c776b964dbc872fcf268345ddccd686337","observation_id":"5c860be7-02c3-4167-a4fb-64da051c6945","resolution":{"observed_at":"2026-08-12T22:01:14.177058Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"0912.1856","last_updated":"2010-01-29T21:04:06Z","snapshot_observed_at":"2026-08-04T19:04:54.313386Z","submitted_at":"2009-12-10T19:08:28Z","title":"Cold Quark Matter","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0912.1856","snapshot_observed_at":"2026-08-12T22:01:13.031273Z","title":"Kurkela, P","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2411.08023","last_updated":"2025-01-21T17:34:00Z","snapshot_observed_at":"2026-08-12T21:57:43.085949Z","submitted_at":"2024-11-12T18:54:12Z","title":"How neutron star properties disfavor a nuclear chiral density wave","version":2},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-08-12T22:01:13.031273Z"},"links":{"cited_paper":"/paper/0912.1856","citing_paper":"/paper/2411.08023"},"observation_digest":"sha256:0813d4cb823c16cc3225206441ca22c84e3a2fe04e17d7cab9aee58447940a70","observation_id":"f5c53f80-acc4-41e4-82f7-1b91e94ccd61","resolution":{"observed_at":"2026-08-12T22:01:13.031273Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2303.12140","last_updated":"2023-09-14T14:15:15Z","snapshot_observed_at":"2026-08-13T12:19:40.421001Z","submitted_at":"2023-03-21T18:57:46Z","title":"Hot perturbative QCD in a very strong magnetic background","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2303.12140","snapshot_observed_at":"2026-08-12T22:01:13.036314Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2411.08023","last_updated":"2025-01-21T17:34:00Z","snapshot_observed_at":"2026-08-12T21:57:43.085949Z","submitted_at":"2024-11-12T18:54:12Z","title":"How neutron star properties disfavor a nuclear chiral density wave","version":2},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-08-12T22:01:13.036314Z"},"links":{"cited_paper":"/paper/2303.12140","citing_paper":"/paper/2411.08023"},"observation_digest":"sha256:85bf2a126ce6b9b301d45f21e619e2cef0944792609bebcda526429438f91969","observation_id":"622e5a0d-c19b-46af-b5d7-56d5d5756440","resolution":{"observed_at":"2026-08-12T22:01:13.036314Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1001.3294","last_updated":"2010-06-25T11:33:20Z","snapshot_observed_at":"2026-07-06T02:06:41.679342Z","submitted_at":"2010-01-19T13:18:09Z","title":"Dense matter in compact stars - A pedagogical introduction","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1001.3294","snapshot_observed_at":"2026-08-12T22:01:13.041255Z","title":"Schmitt, Lect","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2411.08023","last_updated":"2025-01-21T17:34:00Z","snapshot_observed_at":"2026-08-12T21:57:43.085949Z","submitted_at":"2024-11-12T18:54:12Z","title":"How neutron star properties disfavor a nuclear chiral density wave","version":2},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-08-12T22:01:13.041255Z"},"links":{"cited_paper":"/paper/1001.3294","citing_paper":"/paper/2411.08023"},"observation_digest":"sha256:0713622788f007e4a2a6c6eb36ef6a96860f684537c714b86d8aa9e00b9151fe","observation_id":"565e54ed-fb73-4e3f-9f8b-08ab03ea6394","resolution":{"observed_at":"2026-08-12T22:01:13.041255Z","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":"2026-08-12T22:01:14.156168Z","title":null,"venue":null,"work_id":"74844086-87d5-4404-8047-5d62f6efc0d5","year":1995},"citing_paper":{"arxiv_id":"2411.08023","last_updated":"2025-01-21T17:34:00Z","snapshot_observed_at":"2026-08-12T21:57:43.085949Z","submitted_at":"2024-11-12T18:54:12Z","title":"How neutron star properties disfavor a nuclear chiral density wave","version":2},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-08-12T22:01:13.045840Z"},"links":{"citing_paper":"/paper/2411.08023"},"observation_digest":"sha256:d0f9729bb979fa15fdb755f026c462c5a6c0cb2c748aa7f965c741f3fb78ade7","observation_id":"81f2104a-ad67-4fc6-afd0-6152f4010254","resolution":{"observed_at":"2026-08-12T22:01:14.160882Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"nucl-th/0302070","last_updated":"2003-02-24T15:27:27Z","snapshot_observed_at":"2026-07-07T06:32:38.552250Z","submitted_at":"2003-02-24T15:27:27Z","title":"A microscopic estimate of the nuclear matter compressibility and symmetry energy in relativistic mean-field models","version":1},"cited_work":{"arxiv_id":"nucl-th/0302070","doi":null,"metadata_source":"pith","pith_arxiv_id":"nucl-th/0302070","snapshot_observed_at":"2026-08-12T22:01:13.395893Z","title":"A microscopic estimate of the nuclear matter compressibility and symmetry energy in relativistic mean-field models","venue":"nucl-th","work_id":"c9ff83e7-4e17-4a6e-9e76-726aec949521","year":2003},"citing_paper":{"arxiv_id":"2411.08023","last_updated":"2025-01-21T17:34:00Z","snapshot_observed_at":"2026-08-12T21:57:43.085949Z","submitted_at":"2024-11-12T18:54:12Z","title":"How neutron star properties disfavor a nuclear chiral density wave","version":2},"reference_index":54,"source":"pdf_text","source_observed_at":"2026-08-12T22:01:13.050353Z"},"links":{"cited_paper":"/paper/nucl-th/0302070","citing_paper":"/paper/2411.08023"},"observation_digest":"sha256:af2babbcd29c705cbd14fd87ae02099386252beb7f2aef78b6a527674a46ca98","observation_id":"d0a864a2-d2f9-45b6-a0a7-f69e5bd72f87","resolution":{"observed_at":"2026-08-12T22:01:13.401173Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+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":"2026-08-12T22:01:14.142095Z","title":null,"venue":null,"work_id":"1d4881b5-2f20-4719-a93c-fe2fd15082dd","year":2004},"citing_paper":{"arxiv_id":"2411.08023","last_updated":"2025-01-21T17:34:00Z","snapshot_observed_at":"2026-08-12T21:57:43.085949Z","submitted_at":"2024-11-12T18:54:12Z","title":"How neutron star properties disfavor a nuclear chiral density wave","version":2},"reference_index":55,"source":"pdf_text","source_observed_at":"2026-08-12T22:01:13.055112Z"},"links":{"citing_paper":"/paper/2411.08023"},"observation_digest":"sha256:43623feb73a09c76126532163dd9b4e6e8b51f1124d93259c9b5bba8b29af584","observation_id":"8955a64c-2290-4ab9-813f-946fb14370a9","resolution":{"observed_at":"2026-08-12T22:01:14.146602Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+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":"2026-08-12T22:01:14.127404Z","title":"Shlomo, V","venue":null,"work_id":"a99b9fe2-ee95-4f4d-a2f6-d52860ff656e","year":2006},"citing_paper":{"arxiv_id":"2411.08023","last_updated":"2025-01-21T17:34:00Z","snapshot_observed_at":"2026-08-12T21:57:43.085949Z","submitted_at":"2024-11-12T18:54:12Z","title":"How neutron star properties disfavor a nuclear chiral density wave","version":2},"reference_index":56,"source":"pdf_text","source_observed_at":"2026-08-12T22:01:13.059572Z"},"links":{"citing_paper":"/paper/2411.08023"},"observation_digest":"sha256:1c01d9e03d66579133aa7d56de72cc8e604f18fc969411bc2f2464add8a06214","observation_id":"df170901-a6ee-46cd-b6ea-f4a79f3b0b21","resolution":{"observed_at":"2026-08-12T22:01:14.132111Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+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":"2026-08-12T22:01:14.112596Z","title":"Liu, J.-D","venue":null,"work_id":"b520976a-8146-4fa5-8a53-577ae9eb9f2e","year":2024},"citing_paper":{"arxiv_id":"2411.08023","last_updated":"2025-01-21T17:34:00Z","snapshot_observed_at":"2026-08-12T21:57:43.085949Z","submitted_at":"2024-11-12T18:54:12Z","title":"How neutron star properties disfavor a nuclear chiral density wave","version":2},"reference_index":57,"source":"pdf_text","source_observed_at":"2026-08-12T22:01:13.064286Z"},"links":{"citing_paper":"/paper/2411.08023"},"observation_digest":"sha256:a782f96f284f70221704ec00b3d2b079f5c7dca04b63bf83d29c4b2e5c84ae8a","observation_id":"62737647-3647-404e-94df-9c45fd13ecec","resolution":{"observed_at":"2026-08-12T22:01:14.117300Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1005.3166","last_updated":"2010-05-18T12:01:34Z","snapshot_observed_at":"2026-08-10T08:15:41.108751Z","submitted_at":"2010-05-18T12:01:34Z","title":"Vacuum fluctuations and the thermodynamics of chiral models","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1005.3166","snapshot_observed_at":"2026-08-12T22:01:13.068916Z","title":"Skokov, B","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2411.08023","last_updated":"2025-01-21T17:34:00Z","snapshot_observed_at":"2026-08-12T21:57:43.085949Z","submitted_at":"2024-11-12T18:54:12Z","title":"How neutron star properties disfavor a nuclear chiral density wave","version":2},"reference_index":58,"source":"pdf_text","source_observed_at":"2026-08-12T22:01:13.068916Z"},"links":{"cited_paper":"/paper/1005.3166","citing_paper":"/paper/2411.08023"},"observation_digest":"sha256:749280411b411690aca1377f2c986977944f6bfd145b4fd3ad073f2399e15ea6","observation_id":"e06be52d-1c26-426d-82d2-425a43af3ad4","resolution":{"observed_at":"2026-08-12T22:01:13.068916Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2102.10767","last_updated":"2021-04-27T02:57:40Z","snapshot_observed_at":"2026-08-13T20:10:41.019800Z","submitted_at":"2021-02-22T04:33:39Z","title":"Accurate Determination of the Neutron Skin Thickness of $^{208}$Pb through Parity-Violation in Electron Scattering","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2102.10767","snapshot_observed_at":"2026-08-12T22:01:13.073686Z","title":"Adhikari et al","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2411.08023","last_updated":"2025-01-21T17:34:00Z","snapshot_observed_at":"2026-08-12T21:57:43.085949Z","submitted_at":"2024-11-12T18:54:12Z","title":"How neutron star properties disfavor a nuclear chiral density wave","version":2},"reference_index":59,"source":"pdf_text","source_observed_at":"2026-08-12T22:01:13.073686Z"},"links":{"cited_paper":"/paper/2102.10767","citing_paper":"/paper/2411.08023"},"observation_digest":"sha256:a27eca309bd1373da9920a74fd6f0272dda13d64a030795d52045e6f7178c895","observation_id":"71d24700-9236-438c-a3d4-9d0b5bda8e35","resolution":{"observed_at":"2026-08-12T22:01:13.073686Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2112.01125","last_updated":"2022-08-22T15:41:09Z","snapshot_observed_at":"2026-08-13T17:23:14.264753Z","submitted_at":"2021-12-02T11:01:07Z","title":"Ab initio predictions link the neutron skin of ${}^{208}$Pb to nuclear forces","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2112.01125","snapshot_observed_at":"2026-08-12T22:01:13.078813Z","title":"Hu et al., Nature Phys","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2411.08023","last_updated":"2025-01-21T17:34:00Z","snapshot_observed_at":"2026-08-12T21:57:43.085949Z","submitted_at":"2024-11-12T18:54:12Z","title":"How neutron star properties disfavor a nuclear chiral density wave","version":2},"reference_index":60,"source":"pdf_text","source_observed_at":"2026-08-12T22:01:13.078813Z"},"links":{"cited_paper":"/paper/2112.01125","citing_paper":"/paper/2411.08023"},"observation_digest":"sha256:6995b33e8e28f5c4805e317075c2509330538c4eb4ee22def7c7c2a7d8c497eb","observation_id":"764b6e31-e59f-4239-a28b-0911617b1420","resolution":{"observed_at":"2026-08-12T22:01:13.078813Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2203.05410","last_updated":"2022-03-17T01:36:47Z","snapshot_observed_at":"2026-08-13T16:37:55.765733Z","submitted_at":"2022-02-20T06:07:39Z","title":"New constraints on the neutron-star mass and radius relation from terrestrial nuclear experiments","version":2},"cited_work":{"arxiv_id":"2203.05410","doi":null,"metadata_source":"pith","pith_arxiv_id":"2203.05410","snapshot_observed_at":"2026-08-12T22:01:13.327966Z","title":"New constraints on the neutron-star mass and radius relation from terrestrial nuclear experiments","venue":"nucl-th","work_id":"56361716-e3f9-4c64-9673-df86df4bff20","year":2022},"citing_paper":{"arxiv_id":"2411.08023","last_updated":"2025-01-21T17:34:00Z","snapshot_observed_at":"2026-08-12T21:57:43.085949Z","submitted_at":"2024-11-12T18:54:12Z","title":"How neutron star properties disfavor a nuclear chiral density wave","version":2},"reference_index":61,"source":"pdf_text","source_observed_at":"2026-08-12T22:01:13.083519Z"},"links":{"cited_paper":"/paper/2203.05410","citing_paper":"/paper/2411.08023"},"observation_digest":"sha256:ee29cf9617b3732eb849f56159b2825e270e4b524978168ce7265c779be89716","observation_id":"c176f4d3-6c5c-460c-b571-2cfec3ff8bac","resolution":{"observed_at":"2026-08-12T22:01:13.333261Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2205.11593","last_updated":"2022-06-16T21:20:56Z","snapshot_observed_at":"2026-08-13T15:38:35.501836Z","submitted_at":"2022-05-23T19:46:18Z","title":"Precision Determination of the Neutral Weak Form Factor of $^{48}$Ca","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2205.11593","snapshot_observed_at":"2026-08-12T22:01:13.088171Z","title":"Adhikari et al","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2411.08023","last_updated":"2025-01-21T17:34:00Z","snapshot_observed_at":"2026-08-12T21:57:43.085949Z","submitted_at":"2024-11-12T18:54:12Z","title":"How neutron star properties disfavor a nuclear chiral density wave","version":2},"reference_index":62,"source":"pdf_text","source_observed_at":"2026-08-12T22:01:13.088171Z"},"links":{"cited_paper":"/paper/2205.11593","citing_paper":"/paper/2411.08023"},"observation_digest":"sha256:a2e5e47ddfe6559140151342f3cb6995cb2cf9ce6f709ffa4ca2a9a4a115bc33","observation_id":"4f7691e1-5162-438d-b371-a96533b863c7","resolution":{"observed_at":"2026-08-12T22:01:13.088171Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2301.03666","last_updated":"2023-01-09T20:29:41Z","snapshot_observed_at":"2026-08-13T13:07:31.934208Z","submitted_at":"2023-01-09T20:29:41Z","title":"Constraints on Nuclear Symmetry Energy Parameters","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2301.03666","snapshot_observed_at":"2026-08-12T22:01:13.093131Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2411.08023","last_updated":"2025-01-21T17:34:00Z","snapshot_observed_at":"2026-08-12T21:57:43.085949Z","submitted_at":"2024-11-12T18:54:12Z","title":"How neutron star properties disfavor a nuclear chiral density wave","version":2},"reference_index":63,"source":"pdf_text","source_observed_at":"2026-08-12T22:01:13.093131Z"},"links":{"cited_paper":"/paper/2301.03666","citing_paper":"/paper/2411.08023"},"observation_digest":"sha256:a5ab98312bc99dda5c5d584fe1344dd08ce7153233cb02764d242b555b077148","observation_id":"e73b6d56-9f2c-4373-a41a-eab7d1e0e0f7","resolution":{"observed_at":"2026-08-12T22:01:13.093131Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2305.00015","last_updated":"2023-12-01T13:19:37Z","snapshot_observed_at":"2026-08-13T11:52:57.454845Z","submitted_at":"2023-04-28T18:00:00Z","title":"Determination of the neutron skin of $^{208}$Pb from ultrarelativistic nuclear collisions","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2305.00015","snapshot_observed_at":"2026-08-12T22:01:13.097839Z","title":"Giacalone, G","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2411.08023","last_updated":"2025-01-21T17:34:00Z","snapshot_observed_at":"2026-08-12T21:57:43.085949Z","submitted_at":"2024-11-12T18:54:12Z","title":"How neutron star properties disfavor a nuclear chiral density wave","version":2},"reference_index":64,"source":"pdf_text","source_observed_at":"2026-08-12T22:01:13.097839Z"},"links":{"cited_paper":"/paper/2305.00015","citing_paper":"/paper/2411.08023"},"observation_digest":"sha256:027b46186c008955a9b18ab3082b55f2c34648a8e8169ded76fbc91a78fd3740","observation_id":"7d506ba2-430b-44ee-82ea-c618c0c6815c","resolution":{"observed_at":"2026-08-12T22:01:13.097839Z","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":"2026-08-12T22:01:14.096379Z","title":null,"venue":null,"work_id":"4926bf91-19c2-48a0-92e3-560b480a9f99","year":1934},"citing_paper":{"arxiv_id":"2411.08023","last_updated":"2025-01-21T17:34:00Z","snapshot_observed_at":"2026-08-12T21:57:43.085949Z","submitted_at":"2024-11-12T18:54:12Z","title":"How neutron star properties disfavor a nuclear chiral density wave","version":2},"reference_index":65,"source":"pdf_text","source_observed_at":"2026-08-12T22:01:13.102839Z"},"links":{"citing_paper":"/paper/2411.08023"},"observation_digest":"sha256:db658630c06fc95d4b1ed8aaf5dea0a4b188a92d2499bb0697ae2e08f6b6a5a1","observation_id":"80bc88dc-5967-42c6-b5e7-44205d68a7df","resolution":{"observed_at":"2026-08-12T22:01:14.101940Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+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":"2026-08-12T22:01:13.107350Z","title":null,"venue":null,"work_id":null,"year":1939},"citing_paper":{"arxiv_id":"2411.08023","last_updated":"2025-01-21T17:34:00Z","snapshot_observed_at":"2026-08-12T21:57:43.085949Z","submitted_at":"2024-11-12T18:54:12Z","title":"How neutron star properties disfavor a nuclear chiral density wave","version":2},"reference_index":66,"source":"pdf_text","source_observed_at":"2026-08-12T22:01:13.107350Z"},"links":{"citing_paper":"/paper/2411.08023"},"observation_digest":"sha256:1db4f1585e05499e0f4a72711892f6e11e30cde6bcb4ab6f8e4e7c0f097d6816","observation_id":"70021135-215f-436c-8dae-de386c7a950f","resolution":{"observed_at":"2026-08-12T22:01:13.107350Z","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":"2026-08-12T22:01:13.112086Z","title":null,"venue":null,"work_id":null,"year":1939},"citing_paper":{"arxiv_id":"2411.08023","last_updated":"2025-01-21T17:34:00Z","snapshot_observed_at":"2026-08-12T21:57:43.085949Z","submitted_at":"2024-11-12T18:54:12Z","title":"How neutron star properties disfavor a nuclear chiral density wave","version":2},"reference_index":67,"source":"pdf_text","source_observed_at":"2026-08-12T22:01:13.112086Z"},"links":{"citing_paper":"/paper/2411.08023"},"observation_digest":"sha256:e25d4932cc498b67890d357867300272c9eee0f3d629663b0ab157aa97a48953","observation_id":"2510b0f8-1f94-437d-8510-aad22df5088d","resolution":{"observed_at":"2026-08-12T22:01:13.112086Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2111.03374","last_updated":"2022-02-28T16:27:36Z","snapshot_observed_at":"2026-08-13T17:39:08.784002Z","submitted_at":"2021-11-05T10:30:05Z","title":"Building a realistic neutron star from holography","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2111.03374","snapshot_observed_at":"2026-08-12T22:01:13.116710Z","title":"Kovensky, A","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2411.08023","last_updated":"2025-01-21T17:34:00Z","snapshot_observed_at":"2026-08-12T21:57:43.085949Z","submitted_at":"2024-11-12T18:54:12Z","title":"How neutron star properties disfavor a nuclear chiral density wave","version":2},"reference_index":68,"source":"pdf_text","source_observed_at":"2026-08-12T22:01:13.116710Z"},"links":{"cited_paper":"/paper/2111.03374","citing_paper":"/paper/2411.08023"},"observation_digest":"sha256:a8a28abe9e6113444cb069e0c63a41dfa5d400914a8ab4a9d07c6acb1bcdf28c","observation_id":"f8170ada-4dac-45f9-a04a-e86158465cd9","resolution":{"observed_at":"2026-08-12T22:01:13.116710Z","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":"2026-08-12T22:01:13.121569Z","title":null,"venue":null,"work_id":null,"year":1966},"citing_paper":{"arxiv_id":"2411.08023","last_updated":"2025-01-21T17:34:00Z","snapshot_observed_at":"2026-08-12T21:57:43.085949Z","submitted_at":"2024-11-12T18:54:12Z","title":"How neutron star properties disfavor a nuclear chiral density wave","version":2},"reference_index":69,"source":"pdf_text","source_observed_at":"2026-08-12T22:01:13.121569Z"},"links":{"citing_paper":"/paper/2411.08023"},"observation_digest":"sha256:8de8f795821a5068b536701d7a7a7e89fb4a548cee21411ad217e3287de2710f","observation_id":"08debcee-dec4-43f5-bcf3-7b967eec2e18","resolution":{"observed_at":"2026-08-12T22:01:13.121569Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2104.00880","last_updated":"2021-07-06T17:59:37Z","snapshot_observed_at":"2026-08-13T19:47:08.743548Z","submitted_at":"2021-04-02T04:26:41Z","title":"Refined Mass and Geometric Measurements of the High-Mass PSR J0740+6620","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2104.00880","snapshot_observed_at":"2026-08-12T22:01:13.126491Z","title":"Fonseca et al., Astrophys","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2411.08023","last_updated":"2025-01-21T17:34:00Z","snapshot_observed_at":"2026-08-12T21:57:43.085949Z","submitted_at":"2024-11-12T18:54:12Z","title":"How neutron star properties disfavor a nuclear chiral density wave","version":2},"reference_index":70,"source":"pdf_text","source_observed_at":"2026-08-12T22:01:13.126491Z"},"links":{"cited_paper":"/paper/2104.00880","citing_paper":"/paper/2411.08023"},"observation_digest":"sha256:b5e9a28cc7cbe121cf9af5cb27844329f660974f1672eb466dc1af9ca8033a05","observation_id":"95e360e3-5dd4-483f-a4f9-4a0a5d6ec251","resolution":{"observed_at":"2026-08-12T22:01:13.126491Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2207.05124","last_updated":"2022-07-11T18:33:55Z","snapshot_observed_at":"2026-08-13T15:06:50.184744Z","submitted_at":"2022-07-11T18:33:55Z","title":"PSR J0952-0607: The Fastest and Heaviest Known Galactic Neutron Star","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2207.05124","snapshot_observed_at":"2026-08-12T22:01:13.131529Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2411.08023","last_updated":"2025-01-21T17:34:00Z","snapshot_observed_at":"2026-08-12T21:57:43.085949Z","submitted_at":"2024-11-12T18:54:12Z","title":"How neutron star properties disfavor a nuclear chiral density wave","version":2},"reference_index":71,"source":"pdf_text","source_observed_at":"2026-08-12T22:01:13.131529Z"},"links":{"cited_paper":"/paper/2207.05124","citing_paper":"/paper/2411.08023"},"observation_digest":"sha256:5f2df4bf8c3fea9517ee4a5445a5a3fdbbdd6ac51a0697b57e1dcbb8c0f16eb0","observation_id":"e2265913-c573-48c8-b1e6-027930519619","resolution":{"observed_at":"2026-08-12T22:01:13.131529Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1707.07524","last_updated":"2017-07-24T12:49:14Z","snapshot_observed_at":"2026-08-10T10:52:48.951765Z","submitted_at":"2017-07-24T12:49:14Z","title":"Classifications of Twin Star Solutions for a Constant Speed of Sound Parameterized Equation of State","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1707.07524","snapshot_observed_at":"2026-08-12T22:01:13.136140Z","title":"Christian, A","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2411.08023","last_updated":"2025-01-21T17:34:00Z","snapshot_observed_at":"2026-08-12T21:57:43.085949Z","submitted_at":"2024-11-12T18:54:12Z","title":"How neutron star properties disfavor a nuclear chiral density wave","version":2},"reference_index":72,"source":"pdf_text","source_observed_at":"2026-08-12T22:01:13.136140Z"},"links":{"cited_paper":"/paper/1707.07524","citing_paper":"/paper/2411.08023"},"observation_digest":"sha256:feaee22ab3bf9dcf9cef123ca4c253b678f854c564a94c127eba177d7868cc34","observation_id":"9728c631-ab20-48b6-aa1a-1af92802de90","resolution":{"observed_at":"2026-08-12T22:01:13.136140Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2105.03218","last_updated":"2022-02-28T16:36:07Z","snapshot_observed_at":"2026-08-03T15:15:09.501860Z","submitted_at":"2021-05-07T12:44:59Z","title":"Isospin asymmetry in holographic baryonic matter","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2105.03218","snapshot_observed_at":"2026-08-12T22:01:13.141231Z","title":"Kovensky and A","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2411.08023","last_updated":"2025-01-21T17:34:00Z","snapshot_observed_at":"2026-08-12T21:57:43.085949Z","submitted_at":"2024-11-12T18:54:12Z","title":"How neutron star properties disfavor a nuclear chiral density wave","version":2},"reference_index":73,"source":"pdf_text","source_observed_at":"2026-08-12T22:01:13.141231Z"},"links":{"cited_paper":"/paper/2105.03218","citing_paper":"/paper/2411.08023"},"observation_digest":"sha256:398d03aee47d93eddd866071f08262fedcb82a15f2f3f9efa7d3601f2d52012a","observation_id":"a03bb68d-1f84-43ed-bb26-0dd97683917a","resolution":{"observed_at":"2026-08-12T22:01:13.141231Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2302.10675","last_updated":"2023-10-04T14:26:44Z","snapshot_observed_at":"2026-08-13T12:40:12.378116Z","submitted_at":"2023-02-21T13:50:45Z","title":"Phases of cold holographic QCD: baryons, pions and rho mesons","version":3},"cited_work":{"arxiv_id":"2302.10675","doi":null,"metadata_source":"pith","pith_arxiv_id":"2302.10675","snapshot_observed_at":"2026-08-12T22:01:13.185918Z","title":"Phases of cold holographic QCD: baryons, pions and rho mesons","venue":"hep-ph","work_id":"5fd35649-9b22-461a-b2d4-a4a90de30428","year":2023},"citing_paper":{"arxiv_id":"2411.08023","last_updated":"2025-01-21T17:34:00Z","snapshot_observed_at":"2026-08-12T21:57:43.085949Z","submitted_at":"2024-11-12T18:54:12Z","title":"How neutron star properties disfavor a nuclear chiral density wave","version":2},"reference_index":74,"source":"pdf_text","source_observed_at":"2026-08-12T22:01:13.146022Z"},"links":{"cited_paper":"/paper/2302.10675","citing_paper":"/paper/2411.08023"},"observation_digest":"sha256:45a8e0ab8dfd35fc4b59ca0c10559b9605cd89e135e468cc0b5905e1157371d4","observation_id":"cc1792c2-3aaa-4ae8-beb0-f5e5054557e6","resolution":{"observed_at":"2026-08-12T22:01:13.192989Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}}],"paper":{"arxiv_id":"2411.08023","last_updated":"2025-01-21T17:34:00Z","latest_version":2,"primary_category":"nucl-th","snapshot_observed_at":"2026-08-12T21:57:43.085949Z","submitted_at":"2024-11-12T18:54:12Z","title":"How neutron star properties disfavor a nuclear chiral density wave"},"reference_resolution":{"displayed":74,"state_counts":{"malformed_identifier":2,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":44,"verified_exact":17,"verified_fuzzy":11},"total_outbound_references":74},"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":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"thesis":"As of 13 August 2026, this Paper Citation Record lists 74 of 74 outbound references and 0 inbound Pith citation observations for arXiv:2411.08023."}