{"as_of":"2026-08-14T15:52:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:7aa3f4f204b3ff627c5057add5cb5e8984326b8f3ded54686ac8a50c2485db02","coverage":[{"denominator":39,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":39,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-07T14:39:35.565620Z","state":"measured"},{"denominator":39,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":39,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-14T06:32:32.682623+00:00","state":"measured"},{"denominator":0,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":0,"source":"paper_references, paper_reference_links","source_observed_at":null,"state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"cited_works","source_observed_at":null,"state":"measured"}],"external_citation_measurements":[],"inbound":[],"links":{"evidence":"/evidence","html":"/paper/2505.18309/citation-record","integrity":"/paper/2505.18309/integrity","json":"/paper/2505.18309/citation-record.json","paper":"/paper/2505.18309"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T14:39:30.653829Z","title":null,"venue":null,"work_id":null,"year":1971},"citing_paper":{"arxiv_id":"2505.18309","last_updated":"2025-05-23T19:07:16Z","snapshot_observed_at":"2026-08-10T00:56:21.283944Z","submitted_at":"2025-05-23T19:07:16Z","title":"Filling fractions for the formation of nuclear pasta in neutron stars: semiclassical vs liquid-drop predictions","version":1},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-07T14:39:30.653829Z"},"links":{"citing_paper":"/paper/2505.18309"},"observation_digest":"sha256:3f03d4f3744042cf9b853a0ec9c239108ffcd537585a1bf761810b2c59c25699","observation_id":"4fefb948-84ac-43da-ae65-70115e4b68b5","resolution":{"observed_at":"2026-08-07T14:39:30.653829Z","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":"2026-08-07T14:39:30.790209Z","title":null,"venue":null,"work_id":null,"year":1983},"citing_paper":{"arxiv_id":"2505.18309","last_updated":"2025-05-23T19:07:16Z","snapshot_observed_at":"2026-08-10T00:56:21.283944Z","submitted_at":"2025-05-23T19:07:16Z","title":"Filling fractions for the formation of nuclear pasta in neutron stars: semiclassical vs liquid-drop predictions","version":1},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-07T14:39:30.790209Z"},"links":{"citing_paper":"/paper/2505.18309"},"observation_digest":"sha256:b844ce4d3ffb99ca889b71e4405b8e7faae0baccd918ce7172ae6325883dc0f2","observation_id":"f223f807-20c5-4bcb-9d05-5f8d4ae61408","resolution":{"observed_at":"2026-08-07T14:39:30.790209Z","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":"2026-08-07T14:39:41.800039Z","title":"Progress of Theoretical Physics 71(2), 320–326 (1984) https://doi.org/10","venue":null,"work_id":"f6ab982d-6b82-46ab-8424-4e3cd73d5299","year":1984},"citing_paper":{"arxiv_id":"2505.18309","last_updated":"2025-05-23T19:07:16Z","snapshot_observed_at":"2026-08-10T00:56:21.283944Z","submitted_at":"2025-05-23T19:07:16Z","title":"Filling fractions for the formation of nuclear pasta in neutron stars: semiclassical vs liquid-drop predictions","version":1},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-07T14:39:30.927287Z"},"links":{"citing_paper":"/paper/2505.18309"},"observation_digest":"sha256:fe336220c81b770edd0ff2c9f5a00443344ade0cbf3ae187a3bf0669a0067fd9","observation_id":"323a7531-eeca-4a14-aba3-e7514c42a706","resolution":{"observed_at":"2026-08-07T14:39:41.910922Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1143/ptp.72.373","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T05:30:23.456663Z","title":"Progress of Theoretical Physics 72(2), 373–375 (1984) https://doi.org/10.1143/PTP.72.373","venue":"Progress of Theoretical Physics","work_id":"75c37e15-fbeb-4e52-a74a-b14d2dd5a4bf","year":1984},"citing_paper":{"arxiv_id":"2505.18309","last_updated":"2025-05-23T19:07:16Z","snapshot_observed_at":"2026-08-10T00:56:21.283944Z","submitted_at":"2025-05-23T19:07:16Z","title":"Filling fractions for the formation of nuclear pasta in neutron stars: semiclassical vs liquid-drop predictions","version":1},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-07T14:39:31.046528Z"},"links":{"citing_paper":"/paper/2505.18309"},"observation_digest":"sha256:63c63ff42dd57621f82999f5f3403f633f217f55fdf2a8976a7652ec5302804a","observation_id":"808842af-b4b2-4fbb-9d38-64a74863921e","resolution":{"observed_at":"2026-08-07T14:39:38.609669Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"0195.00224","doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T14:39:39.115248Z","title":"Annual Review of Nuclear and Particle Science 45(45), 429–484 (1995) https://doi.org/10.1146/annurev.ns.45.120195.002241","venue":null,"work_id":"dda73c8b-5c44-43a1-af75-031d72ec64f4","year":1995},"citing_paper":{"arxiv_id":"2505.18309","last_updated":"2025-05-23T19:07:16Z","snapshot_observed_at":"2026-08-10T00:56:21.283944Z","submitted_at":"2025-05-23T19:07:16Z","title":"Filling fractions for the formation of nuclear pasta in neutron stars: semiclassical vs liquid-drop predictions","version":1},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-07T14:39:31.126967Z"},"links":{"citing_paper":"/paper/2505.18309"},"observation_digest":"sha256:1d12a29cc07a80e37962c073a7112ac305e1897acf0fe8c41e803414bdfce5db","observation_id":"f0a133ea-5dea-4837-9a8d-3a6589b46b75","resolution":{"observed_at":"2026-08-07T14:39:39.250207Z","resolver_source":"raw_fallback","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+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":"2026-08-07T14:39:41.585199Z","title":"Particles 5(3), 225–234 (2022) https://doi.org/10.3390/ particles5030020","venue":null,"work_id":"2a02b437-4a94-4f5e-922e-29f8f06aa9da","year":2022},"citing_paper":{"arxiv_id":"2505.18309","last_updated":"2025-05-23T19:07:16Z","snapshot_observed_at":"2026-08-10T00:56:21.283944Z","submitted_at":"2025-05-23T19:07:16Z","title":"Filling fractions for the formation of nuclear pasta in neutron stars: semiclassical vs liquid-drop predictions","version":1},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-07T14:39:31.274535Z"},"links":{"citing_paper":"/paper/2505.18309"},"observation_digest":"sha256:b80eafba7d03b59f64f890dc6da015c3d77df3fe89be50d9ad7658375878bd29","observation_id":"aa5b0ff4-140b-495a-87ac-96cd58652669","resolution":{"observed_at":"2026-08-07T14:39:41.692308Z","resolver_source":"raw_fallback","status":"malformed_identifier"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+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":"2026-08-07T14:39:31.393699Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2505.18309","last_updated":"2025-05-23T19:07:16Z","snapshot_observed_at":"2026-08-10T00:56:21.283944Z","submitted_at":"2025-05-23T19:07:16Z","title":"Filling fractions for the formation of nuclear pasta in neutron stars: semiclassical vs liquid-drop predictions","version":1},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-07T14:39:31.393699Z"},"links":{"citing_paper":"/paper/2505.18309"},"observation_digest":"sha256:8a674ca28524e451fd320685765c2fc0031a85a8a5a87468ebfe975935e6a1a2","observation_id":"d8ca59d2-73d1-401f-9e33-f35f6e1eb426","resolution":{"observed_at":"2026-08-07T14:39:31.393699Z","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":"10.1016/0370-2693(83)90376-3","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T05:30:23.456663Z","title":"Physics Letters B 128(3), 137–140 (1983) https://doi.org/10.1016/0370-2693(83)90376-3","venue":"Physics Letters B","work_id":"517d0644-3269-4808-920f-e15cd6ba4ca6","year":1983},"citing_paper":{"arxiv_id":"2505.18309","last_updated":"2025-05-23T19:07:16Z","snapshot_observed_at":"2026-08-10T00:56:21.283944Z","submitted_at":"2025-05-23T19:07:16Z","title":"Filling fractions for the formation of nuclear pasta in neutron stars: semiclassical vs liquid-drop predictions","version":1},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-07T14:39:31.504675Z"},"links":{"citing_paper":"/paper/2505.18309"},"observation_digest":"sha256:497720abc752b60ad4ca1546a0d30f848b76582142d806149c3bafbdb7dac420","observation_id":"03152e02-cd10-454b-a8b2-5b01bcf7189c","resolution":{"observed_at":"2026-08-07T14:39:38.353268Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1103/physrevc.83.065811","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T05:30:23.456663Z","title":null,"venue":"Physical Review C","work_id":"ae3e47e3-85f1-4083-b031-da21e79c92e0","year":2011},"citing_paper":{"arxiv_id":"2505.18309","last_updated":"2025-05-23T19:07:16Z","snapshot_observed_at":"2026-08-10T00:56:21.283944Z","submitted_at":"2025-05-23T19:07:16Z","title":"Filling fractions for the formation of nuclear pasta in neutron stars: semiclassical vs liquid-drop predictions","version":1},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-07T14:39:31.631893Z"},"links":{"citing_paper":"/paper/2505.18309"},"observation_digest":"sha256:30fdee606dcf651f976baf918676c74c09743c0f27f7fc7eb5279c59275237f4","observation_id":"09f6d3f8-da57-46f2-a199-f353a1ca7889","resolution":{"observed_at":"2026-08-07T14:39:38.139986Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+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":"2026-08-07T14:39:41.350116Z","title":"Compressible 14 Liquid Drop Approaches","venue":null,"work_id":"af4b3a60-c906-4e14-aab1-1826766de8c3","year":2022},"citing_paper":{"arxiv_id":"2505.18309","last_updated":"2025-05-23T19:07:16Z","snapshot_observed_at":"2026-08-10T00:56:21.283944Z","submitted_at":"2025-05-23T19:07:16Z","title":"Filling fractions for the formation of nuclear pasta in neutron stars: semiclassical vs liquid-drop predictions","version":1},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-07T14:39:31.764197Z"},"links":{"citing_paper":"/paper/2505.18309"},"observation_digest":"sha256:44c91124f1614c7e2759315a25f10e5e82f69fa6fc38d794d3fdc98959586d57","observation_id":"732942fe-5a7c-4865-b4b8-0d9af9f0dca7","resolution":{"observed_at":"2026-08-07T14:39:41.471562Z","resolver_source":"raw_fallback","status":"malformed_identifier"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+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":"2026-08-07T14:39:31.894820Z","title":"European Physical Journal A 57(10), 296 (2021) https://doi.org/10.1140/epja/s10050-021-00605-6","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2505.18309","last_updated":"2025-05-23T19:07:16Z","snapshot_observed_at":"2026-08-10T00:56:21.283944Z","submitted_at":"2025-05-23T19:07:16Z","title":"Filling fractions for the formation of nuclear pasta in neutron stars: semiclassical vs liquid-drop predictions","version":1},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-07T14:39:31.894820Z"},"links":{"citing_paper":"/paper/2505.18309"},"observation_digest":"sha256:fda1f11a5089c3f71e7ba57fea0f0aa8dedcb56abedb807d868ffd8047d97576","observation_id":"212e6705-fd89-4e0d-96e3-047049eb5900","resolution":{"observed_at":"2026-08-07T14:39:31.894820Z","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":"2026-08-07T14:39:32.000010Z","title":"The Astrophysical Journal Supplement Series 204(1), 9 (2012) https://doi.org/ 10.1088/0067-0049/204/1/9","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2505.18309","last_updated":"2025-05-23T19:07:16Z","snapshot_observed_at":"2026-08-10T00:56:21.283944Z","submitted_at":"2025-05-23T19:07:16Z","title":"Filling fractions for the formation of nuclear pasta in neutron stars: semiclassical vs liquid-drop predictions","version":1},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-07T14:39:32.000010Z"},"links":{"citing_paper":"/paper/2505.18309"},"observation_digest":"sha256:031ea5d228c878e4b1e18547f14bad30a4878057e84a39dca7cbbbaa3e4b01a6","observation_id":"fce2f14a-4d65-4017-bb0b-98702d302526","resolution":{"observed_at":"2026-08-07T14:39:32.000010Z","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":"10.1016/s0375-9474(99)00397-8","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T05:30:23.456663Z","title":null,"venue":"Nuclear Physics A","work_id":"cbb84820-1cc7-44ac-84a0-c6b4b5503cfe","year":2000},"citing_paper":{"arxiv_id":"2505.18309","last_updated":"2025-05-23T19:07:16Z","snapshot_observed_at":"2026-08-10T00:56:21.283944Z","submitted_at":"2025-05-23T19:07:16Z","title":"Filling fractions for the formation of nuclear pasta in neutron stars: semiclassical vs liquid-drop predictions","version":1},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-07T14:39:32.109193Z"},"links":{"citing_paper":"/paper/2505.18309"},"observation_digest":"sha256:3d16a62f71156faa94ce107a7836a80af5f722824adc7f406db3f2326406d2db","observation_id":"878ccb52-68a9-43b8-8711-a5f293796400","resolution":{"observed_at":"2026-08-07T14:39:37.878919Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1016/s0370-2693(00)00672-9","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T05:30:23.456663Z","title":"Physics Letters B 485(1-3), 107–114 (2000) https: //doi.org/10.1016/S0370-2693(00)00672-9","venue":"Physics Letters B","work_id":"f38b485b-cf73-40df-9cc0-99fba3d4840e","year":2000},"citing_paper":{"arxiv_id":"2505.18309","last_updated":"2025-05-23T19:07:16Z","snapshot_observed_at":"2026-08-10T00:56:21.283944Z","submitted_at":"2025-05-23T19:07:16Z","title":"Filling fractions for the formation of nuclear pasta in neutron stars: semiclassical vs liquid-drop predictions","version":1},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-07T14:39:32.278511Z"},"links":{"citing_paper":"/paper/2505.18309"},"observation_digest":"sha256:93aaa79afe0835f15225ab46b193f65afc9957f7d492b69ea37ef5e12ad2f50e","observation_id":"5f119055-18b5-4f8c-b273-7427a78f87a3","resolution":{"observed_at":"2026-08-07T14:39:37.632553Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+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":"2026-08-07T14:39:41.116828Z","title":null,"venue":null,"work_id":"75c2e977-5273-4462-b991-405967a8586f","year":2001},"citing_paper":{"arxiv_id":"2505.18309","last_updated":"2025-05-23T19:07:16Z","snapshot_observed_at":"2026-08-10T00:56:21.283944Z","submitted_at":"2025-05-23T19:07:16Z","title":"Filling fractions for the formation of nuclear pasta in neutron stars: semiclassical vs liquid-drop predictions","version":1},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-07T14:39:32.389090Z"},"links":{"citing_paper":"/paper/2505.18309"},"observation_digest":"sha256:e36426b72a1f4f1ad6311abe43f8a50b3336d3631f99fd99464d3fac058c66f6","observation_id":"2aa32f42-f4ff-47e6-b4a8-5fb0d7308b2f","resolution":{"observed_at":"2026-08-07T14:39:41.220363Z","resolver_source":"raw_fallback","status":"malformed_identifier"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+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":"2026-08-07T14:39:40.881619Z","title":null,"venue":null,"work_id":"cd59a94a-4ca1-413f-85cc-3cb768db1f21","year":2007},"citing_paper":{"arxiv_id":"2505.18309","last_updated":"2025-05-23T19:07:16Z","snapshot_observed_at":"2026-08-10T00:56:21.283944Z","submitted_at":"2025-05-23T19:07:16Z","title":"Filling fractions for the formation of nuclear pasta in neutron stars: semiclassical vs liquid-drop predictions","version":1},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-07T14:39:32.490874Z"},"links":{"citing_paper":"/paper/2505.18309"},"observation_digest":"sha256:81d9fb61108a562ab266fe4979509cb4e649e2f96cd2f51895ab65447f5e9803","observation_id":"49130aaf-6c76-48a6-9ac4-2ff41e058884","resolution":{"observed_at":"2026-08-07T14:39:40.989559Z","resolver_source":"raw_fallback","status":"malformed_identifier"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+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":"2026-08-07T14:39:32.611544Z","title":null,"venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2505.18309","last_updated":"2025-05-23T19:07:16Z","snapshot_observed_at":"2026-08-10T00:56:21.283944Z","submitted_at":"2025-05-23T19:07:16Z","title":"Filling fractions for the formation of nuclear pasta in neutron stars: semiclassical vs liquid-drop predictions","version":1},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-07T14:39:32.611544Z"},"links":{"citing_paper":"/paper/2505.18309"},"observation_digest":"sha256:6a3d21b1cbbeaac04e86903874ba8cee5886ba2ea14501c393cce3821230b75b","observation_id":"43404348-3648-4fd6-96b7-8d24724f860f","resolution":{"observed_at":"2026-08-07T14:39:32.611544Z","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":"10.1103/physrevc.88.025801","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T05:30:23.456663Z","title":null,"venue":"Physical Review C","work_id":"bc08b50c-c737-4715-915b-240dd7c2ca22","year":2013},"citing_paper":{"arxiv_id":"2505.18309","last_updated":"2025-05-23T19:07:16Z","snapshot_observed_at":"2026-08-10T00:56:21.283944Z","submitted_at":"2025-05-23T19:07:16Z","title":"Filling fractions for the formation of nuclear pasta in neutron stars: semiclassical vs liquid-drop predictions","version":1},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-07T14:39:32.739497Z"},"links":{"citing_paper":"/paper/2505.18309"},"observation_digest":"sha256:6701c72322f4aeaef3b53dff75b9c8451f4c7ce370fe077593da442353704696","observation_id":"79cb0843-bd07-462d-8e3d-d46bfbebbf27","resolution":{"observed_at":"2026-08-07T14:39:37.407758Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1103/physrevc.101.015802","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T05:30:23.456663Z","title":null,"venue":"Physical review. C","work_id":"d170cf72-f450-41b3-aa12-62084394e7f3","year":2020},"citing_paper":{"arxiv_id":"2505.18309","last_updated":"2025-05-23T19:07:16Z","snapshot_observed_at":"2026-08-10T00:56:21.283944Z","submitted_at":"2025-05-23T19:07:16Z","title":"Filling fractions for the formation of nuclear pasta in neutron stars: semiclassical vs liquid-drop predictions","version":1},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-07T14:39:32.871810Z"},"links":{"citing_paper":"/paper/2505.18309"},"observation_digest":"sha256:7aade9892f542b905afd335f50076c20af47927206924db08e17b391879601df","observation_id":"c70c7e4b-6d0b-4fe4-a342-4d23be0d21e2","resolution":{"observed_at":"2026-08-07T14:39:37.149587Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+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":"2026-08-07T14:39:40.666952Z","title":null,"venue":null,"work_id":"b0886375-6ee8-4a14-8144-93f2f5890806","year":2013},"citing_paper":{"arxiv_id":"2505.18309","last_updated":"2025-05-23T19:07:16Z","snapshot_observed_at":"2026-08-10T00:56:21.283944Z","submitted_at":"2025-05-23T19:07:16Z","title":"Filling fractions for the formation of nuclear pasta in neutron stars: semiclassical vs liquid-drop predictions","version":1},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-07T14:39:33.005945Z"},"links":{"citing_paper":"/paper/2505.18309"},"observation_digest":"sha256:a46a111b21ee1a20035b494e4ec9434439ec43193347faeccbb4bfe4ba5b7937","observation_id":"b49680c0-cbed-4c42-a55c-fe3abdf4c178","resolution":{"observed_at":"2026-08-07T14:39:40.774704Z","resolver_source":"raw_fallback","status":"malformed_identifier"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+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":"2026-08-07T14:39:40.400754Z","title":"Nuclei far from stabilities","venue":null,"work_id":"1c7be405-7900-4dc1-8456-2ebb8e2283fa","year":1998},"citing_paper":{"arxiv_id":"2505.18309","last_updated":"2025-05-23T19:07:16Z","snapshot_observed_at":"2026-08-10T00:56:21.283944Z","submitted_at":"2025-05-23T19:07:16Z","title":"Filling fractions for the formation of nuclear pasta in neutron stars: semiclassical vs liquid-drop predictions","version":1},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-07T14:39:33.158592Z"},"links":{"citing_paper":"/paper/2505.18309"},"observation_digest":"sha256:be9f4817bb70cb4140ca95873c47782db0baad063a9ab070ad6b8693d2a077d6","observation_id":"ebc26839-7c6c-477e-a698-44131341b5ac","resolution":{"observed_at":"2026-08-07T14:39:40.514921Z","resolver_source":"raw_fallback","status":"malformed_identifier"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1103/physrevc.108.025805","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T05:30:23.456663Z","title":null,"venue":"Physical review. C","work_id":"1e60206a-42d4-46be-b69b-f180f322b52b","year":2023},"citing_paper":{"arxiv_id":"2505.18309","last_updated":"2025-05-23T19:07:16Z","snapshot_observed_at":"2026-08-10T00:56:21.283944Z","submitted_at":"2025-05-23T19:07:16Z","title":"Filling fractions for the formation of nuclear pasta in neutron stars: semiclassical vs liquid-drop predictions","version":1},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-07T14:39:33.322534Z"},"links":{"citing_paper":"/paper/2505.18309"},"observation_digest":"sha256:3984f594af6ab83455773148f5c15f81118611ad13a37b8cdf6ce9e760ac85f4","observation_id":"df5a75ca-0d99-456e-aaa9-a774a85ba199","resolution":{"observed_at":"2026-08-07T14:39:36.919116Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+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":"2026-08-07T14:39:33.480446Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2505.18309","last_updated":"2025-05-23T19:07:16Z","snapshot_observed_at":"2026-08-10T00:56:21.283944Z","submitted_at":"2025-05-23T19:07:16Z","title":"Filling fractions for the formation of nuclear pasta in neutron stars: semiclassical vs liquid-drop predictions","version":1},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-07T14:39:33.480446Z"},"links":{"citing_paper":"/paper/2505.18309"},"observation_digest":"sha256:bc338f001bcd488c6e14cb7e9ed44a0bb7ee3095fcd3befa10c1634ccdc66a19","observation_id":"c4cf044f-7e06-4b4a-9472-f29211affce1","resolution":{"observed_at":"2026-08-07T14:39:33.480446Z","resolver_source":null,"status":"malformed_identifier"},"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":"2026-08-07T14:39:33.604553Z","title":null,"venue":null,"work_id":null,"year":1985},"citing_paper":{"arxiv_id":"2505.18309","last_updated":"2025-05-23T19:07:16Z","snapshot_observed_at":"2026-08-10T00:56:21.283944Z","submitted_at":"2025-05-23T19:07:16Z","title":"Filling fractions for the formation of nuclear pasta in neutron stars: semiclassical vs liquid-drop predictions","version":1},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-07T14:39:33.604553Z"},"links":{"citing_paper":"/paper/2505.18309"},"observation_digest":"sha256:ac6a91b31483264b4cbc2617df2b992e40105cc916a705b3bd0418d90c1bdc74","observation_id":"7692e3e9-8599-4b9b-9654-f7ac6c02768e","resolution":{"observed_at":"2026-08-07T14:39:33.604553Z","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":"2026-08-07T14:39:33.725889Z","title":"Role of symmetry energy","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2505.18309","last_updated":"2025-05-23T19:07:16Z","snapshot_observed_at":"2026-08-10T00:56:21.283944Z","submitted_at":"2025-05-23T19:07:16Z","title":"Filling fractions for the formation of nuclear pasta in neutron stars: semiclassical vs liquid-drop predictions","version":1},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-07T14:39:33.725889Z"},"links":{"citing_paper":"/paper/2505.18309"},"observation_digest":"sha256:5cbf1406ebde94646042411434a1ad07ad0a8e9cc3469b047783f0b4dd359751","observation_id":"4a6f5742-5aa0-4eff-b2a6-b1b0fcb380fb","resolution":{"observed_at":"2026-08-07T14:39:33.725889Z","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":"10.1209/0295-5075/91/32001","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T05:30:23.456663Z","title":"EPL (Europhysics Letters) 91(3), 32001 (2010) https://doi.org/10.1209/0295-5075/91/32001","venue":"Europhysics Letters (EPL)","work_id":"3c218d4b-385f-498c-b434-f69fa3dfdac5","year":2010},"citing_paper":{"arxiv_id":"2505.18309","last_updated":"2025-05-23T19:07:16Z","snapshot_observed_at":"2026-08-10T00:56:21.283944Z","submitted_at":"2025-05-23T19:07:16Z","title":"Filling fractions for the formation of nuclear pasta in neutron stars: semiclassical vs liquid-drop predictions","version":1},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-07T14:39:33.839042Z"},"links":{"citing_paper":"/paper/2505.18309"},"observation_digest":"sha256:7baa5f5bee84f924f79352146ad648102455182af19cea813e58e600012e5a43","observation_id":"e4b8709a-4529-4e91-98b6-28d8bef5ff60","resolution":{"observed_at":"2026-08-07T14:39:36.625057Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+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":"2026-08-07T14:39:33.990038Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2505.18309","last_updated":"2025-05-23T19:07:16Z","snapshot_observed_at":"2026-08-10T00:56:21.283944Z","submitted_at":"2025-05-23T19:07:16Z","title":"Filling fractions for the formation of nuclear pasta in neutron stars: semiclassical vs liquid-drop predictions","version":1},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-07T14:39:33.990038Z"},"links":{"citing_paper":"/paper/2505.18309"},"observation_digest":"sha256:89ecf09c93cd991a122b9d145fa64358ede73f8f8aee93383f2d6a570e680d04","observation_id":"4ed993b5-2d8f-4190-bdc7-79acc0f5d9c6","resolution":{"observed_at":"2026-08-07T14:39:33.990038Z","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":"10.1016/s0375-9474(98)00167-5","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T05:30:23.456663Z","title":null,"venue":"Nuclear Physics A","work_id":"c2942459-05ec-4552-a6b7-c27d99643783","year":1998},"citing_paper":{"arxiv_id":"2505.18309","last_updated":"2025-05-23T19:07:16Z","snapshot_observed_at":"2026-08-10T00:56:21.283944Z","submitted_at":"2025-05-23T19:07:16Z","title":"Filling fractions for the formation of nuclear pasta in neutron stars: semiclassical vs liquid-drop predictions","version":1},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-07T14:39:34.162289Z"},"links":{"citing_paper":"/paper/2505.18309"},"observation_digest":"sha256:4c7835df6dae4f1940293a5a9b3fc3b8d3fcf2d86ed0b4b38d6e51f0f40e7f97","observation_id":"c9e29e70-aaf3-4bfd-aeaa-d96a5dc27eef","resolution":{"observed_at":"2026-08-07T14:39:36.413519Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+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":"2026-08-07T14:39:34.286657Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2505.18309","last_updated":"2025-05-23T19:07:16Z","snapshot_observed_at":"2026-08-10T00:56:21.283944Z","submitted_at":"2025-05-23T19:07:16Z","title":"Filling fractions for the formation of nuclear pasta in neutron stars: semiclassical vs liquid-drop predictions","version":1},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-07T14:39:34.286657Z"},"links":{"citing_paper":"/paper/2505.18309"},"observation_digest":"sha256:a3bac6f399f5c9b2910f26f9821e2f5a5d3299a9ac19cf9cfb9149228313385a","observation_id":"c06b72b6-8fbe-453e-a27f-f153737abb4e","resolution":{"observed_at":"2026-08-07T14:39:34.286657Z","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":"10.1088/1742-6596/1697/1/012025","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T05:30:23.456663Z","title":"In: Journal of Physics Conference Series","venue":"Journal of Physics Conference Series","work_id":"2c9fbcfd-f7a3-4e47-8da9-b7f200d055c6","year":2020},"citing_paper":{"arxiv_id":"2505.18309","last_updated":"2025-05-23T19:07:16Z","snapshot_observed_at":"2026-08-10T00:56:21.283944Z","submitted_at":"2025-05-23T19:07:16Z","title":"Filling fractions for the formation of nuclear pasta in neutron stars: semiclassical vs liquid-drop predictions","version":1},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-07T14:39:34.416682Z"},"links":{"citing_paper":"/paper/2505.18309"},"observation_digest":"sha256:47832fe9ef661e8af9221f3e1b773e9561fdf3aa8f191ee527860f1ab1e79df8","observation_id":"f70381db-ee11-4de2-ad4a-9dc737a99ab9","resolution":{"observed_at":"2026-08-07T14:39:36.196260Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1016/0375-9474(85)90425-7","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T05:30:23.456663Z","title":null,"venue":"Nuclear Physics A","work_id":"449dbcbb-b5f3-419e-9d09-7456ce768abf","year":1985},"citing_paper":{"arxiv_id":"2505.18309","last_updated":"2025-05-23T19:07:16Z","snapshot_observed_at":"2026-08-10T00:56:21.283944Z","submitted_at":"2025-05-23T19:07:16Z","title":"Filling fractions for the formation of nuclear pasta in neutron stars: semiclassical vs liquid-drop predictions","version":1},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-08-07T14:39:34.559514Z"},"links":{"citing_paper":"/paper/2505.18309"},"observation_digest":"sha256:b918b3dc21c26af01920063c107011b1c4fc385147a5e93cd5c94e929ae6f72a","observation_id":"d0668016-e33e-49f3-b5e4-55976ebeca3f","resolution":{"observed_at":"2026-08-07T14:39:35.917443Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+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":"2026-08-07T14:39:40.123107Z","title":null,"venue":null,"work_id":"42a78bec-9192-4f91-bb5a-556f2d74841e","year":1983},"citing_paper":{"arxiv_id":"2505.18309","last_updated":"2025-05-23T19:07:16Z","snapshot_observed_at":"2026-08-10T00:56:21.283944Z","submitted_at":"2025-05-23T19:07:16Z","title":"Filling fractions for the formation of nuclear pasta in neutron stars: semiclassical vs liquid-drop predictions","version":1},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-07T14:39:34.725371Z"},"links":{"citing_paper":"/paper/2505.18309"},"observation_digest":"sha256:68e69c5ec44c91bcc9d2afd3d777df1361d9bba2c56603df34ebc2be7dd94eba","observation_id":"9ac0c1a0-f714-4bbc-ac74-fd27495c0a62","resolution":{"observed_at":"2026-08-07T14:39:40.234897Z","resolver_source":"raw_fallback","status":"malformed_identifier"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+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":"2026-08-07T14:39:34.841073Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2505.18309","last_updated":"2025-05-23T19:07:16Z","snapshot_observed_at":"2026-08-10T00:56:21.283944Z","submitted_at":"2025-05-23T19:07:16Z","title":"Filling fractions for the formation of nuclear pasta in neutron stars: semiclassical vs liquid-drop predictions","version":1},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-07T14:39:34.841073Z"},"links":{"citing_paper":"/paper/2505.18309"},"observation_digest":"sha256:e74724ea097ba40395cf76b867e6ac34f9e5c2e918d3604b496e651a3601fe61","observation_id":"c5a9f651-2888-447e-9afb-74dd32b81b00","resolution":{"observed_at":"2026-08-07T14:39:34.841073Z","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":"2026-08-07T14:39:39.859433Z","title":null,"venue":null,"work_id":"51549bb1-aac3-4e0a-bb55-8a3588f64214","year":2022},"citing_paper":{"arxiv_id":"2505.18309","last_updated":"2025-05-23T19:07:16Z","snapshot_observed_at":"2026-08-10T00:56:21.283944Z","submitted_at":"2025-05-23T19:07:16Z","title":"Filling fractions for the formation of nuclear pasta in neutron stars: semiclassical vs liquid-drop predictions","version":1},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-07T14:39:34.937462Z"},"links":{"citing_paper":"/paper/2505.18309"},"observation_digest":"sha256:72eb09b8afb3d215161ac6d27e2e248da223952a6697cc5f2f1c5bef4199447c","observation_id":"a58d2a82-6ce6-4442-bff0-7d11ad98be8b","resolution":{"observed_at":"2026-08-07T14:39:39.979873Z","resolver_source":"raw_fallback","status":"malformed_identifier"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"2502.19762","doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T14:39:38.853314Z","title":"arXiv e-prints, 2502–19762 (2025) arXiv:2502.19762","venue":null,"work_id":"53abdf36-0db4-4f55-a340-6438ac404af0","year":2025},"citing_paper":{"arxiv_id":"2505.18309","last_updated":"2025-05-23T19:07:16Z","snapshot_observed_at":"2026-08-10T00:56:21.283944Z","submitted_at":"2025-05-23T19:07:16Z","title":"Filling fractions for the formation of nuclear pasta in neutron stars: semiclassical vs liquid-drop predictions","version":1},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-07T14:39:35.081158Z"},"links":{"citing_paper":"/paper/2505.18309"},"observation_digest":"sha256:4326b8e73090581e4b48872aa3e4a48b55f652304b1f08b8554205d01424725e","observation_id":"c951a1f3-2393-4f57-be3f-67a4eb25cad9","resolution":{"observed_at":"2026-08-07T14:39:38.955274Z","resolver_source":"raw_fallback","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+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":"2026-08-07T14:39:35.215346Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2505.18309","last_updated":"2025-05-23T19:07:16Z","snapshot_observed_at":"2026-08-10T00:56:21.283944Z","submitted_at":"2025-05-23T19:07:16Z","title":"Filling fractions for the formation of nuclear pasta in neutron stars: semiclassical vs liquid-drop predictions","version":1},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-07T14:39:35.215346Z"},"links":{"citing_paper":"/paper/2505.18309"},"observation_digest":"sha256:74f4b9a235cea4109ec20fdb5892d671a6b2209ffde4622110985cf54a723590","observation_id":"626e70d7-1730-4b1f-9781-438ca36a8283","resolution":{"observed_at":"2026-08-07T14:39:35.215346Z","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":"2026-08-07T14:39:39.592446Z","title":"PhD thesis, University of Illinois, Urbana-Champaign (February 1991)","venue":null,"work_id":"91290b95-e966-4ef4-80c2-c5cc2d201c36","year":1991},"citing_paper":{"arxiv_id":"2505.18309","last_updated":"2025-05-23T19:07:16Z","snapshot_observed_at":"2026-08-10T00:56:21.283944Z","submitted_at":"2025-05-23T19:07:16Z","title":"Filling fractions for the formation of nuclear pasta in neutron stars: semiclassical vs liquid-drop predictions","version":1},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-07T14:39:35.381625Z"},"links":{"citing_paper":"/paper/2505.18309"},"observation_digest":"sha256:480a2a6923e626d5dbc360e1528050fa4705ec9e9ecd2a34008991c4cb7775a4","observation_id":"7e6b8014-c204-4a8c-b0af-cc0779eec665","resolution":{"observed_at":"2026-08-07T14:39:39.734973Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+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":"2026-08-07T14:39:39.374734Z","title":"Theses, Normandie Universit´ e (September 2023)","venue":null,"work_id":"b062098a-cf30-46d7-b8ff-f391f88a6c0a","year":2023},"citing_paper":{"arxiv_id":"2505.18309","last_updated":"2025-05-23T19:07:16Z","snapshot_observed_at":"2026-08-10T00:56:21.283944Z","submitted_at":"2025-05-23T19:07:16Z","title":"Filling fractions for the formation of nuclear pasta in neutron stars: semiclassical vs liquid-drop predictions","version":1},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-07T14:39:35.470800Z"},"links":{"citing_paper":"/paper/2505.18309"},"observation_digest":"sha256:7cabcb547f5c5e8f05ce99f70cb32f23093d8383a72270bb46cf548b507c8260","observation_id":"99ab0f79-d762-4ffb-9f8e-e00018ec4a28","resolution":{"observed_at":"2026-08-07T14:39:39.479996Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+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":"2026-08-07T14:39:35.565620Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2505.18309","last_updated":"2025-05-23T19:07:16Z","snapshot_observed_at":"2026-08-10T00:56:21.283944Z","submitted_at":"2025-05-23T19:07:16Z","title":"Filling fractions for the formation of nuclear pasta in neutron stars: semiclassical vs liquid-drop predictions","version":1},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-08-07T14:39:35.565620Z"},"links":{"citing_paper":"/paper/2505.18309"},"observation_digest":"sha256:67e4603a11d9cea58a767562f0181e1c7d7dccdd84a54d601fdb674cc484660c","observation_id":"fad8b1aa-4c13-4ff1-a07a-03d97e1ecc2c","resolution":{"observed_at":"2026-08-07T14:39:35.565620Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"2505.18309","last_updated":"2025-05-23T19:07:16Z","latest_version":1,"primary_category":"astro-ph.HE","snapshot_observed_at":"2026-08-10T00:56:21.283944Z","submitted_at":"2025-05-23T19:07:16Z","title":"Filling fractions for the formation of nuclear pasta in neutron stars: semiclassical vs liquid-drop predictions"},"reference_resolution":{"displayed":39,"state_counts":{"malformed_identifier":9,"metadata_mismatch":1,"parse_uncertain":0,"unresolved":13,"verified_exact":13,"verified_fuzzy":3},"total_outbound_references":39},"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":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"thesis":"As of 14 August 2026, this Paper Citation Record lists 39 of 39 outbound references and 0 inbound Pith citation observations for arXiv:2505.18309."}