{"as_of":"2026-08-21T12:55:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:5dd96a11103a2fddcbae31f31aa3c684e48e5f7d806e9bc995eca3e5138604fe","coverage":[{"denominator":0,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":0,"source":"paper_references, paper_reference_links","source_observed_at":null,"state":"measured"},{"denominator":9,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":9,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-21T06:32:19.484+00:00","state":"measured"},{"denominator":9,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":9,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-16T00:21:42.891574Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"arxiv_reference","source_observed_at":"2026-07-04T16:19:57.284731Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2406.13717","last_updated":"2024-06-19T17:19:10Z","snapshot_observed_at":"2026-08-16T13:41:22.404359Z","submitted_at":"2024-06-19T17:19:10Z","title":"Beyond modified Urca: the nucleon width approximation for flavor-changing processes in dense matter","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2406.13717","snapshot_observed_at":"2026-08-08T11:32:34.453445Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2502.07902","last_updated":"2025-02-11T19:17:15Z","snapshot_observed_at":"2026-08-14T05:40:41.875320Z","submitted_at":"2025-02-11T19:17:15Z","title":"Building Neutron Stars with the MUSES Calculation Engine","version":1},"reference_index":66,"source":"pdf_text","source_observed_at":"2026-08-08T11:32:34.453445Z"},"links":{"cited_paper":"/paper/2406.13717","citing_paper":"/paper/2502.07902"},"observation_digest":"sha256:bc243bb6d9300da0215881f0c72ab24785ac295482a8366a1df26cc562f4eae6","observation_id":"7ce1f718-f815-4d10-87ee-1f52cd127246","resolution":{"observed_at":"2026-08-08T11:32:34.453445Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2406.13717","last_updated":"2024-06-19T17:19:10Z","snapshot_observed_at":"2026-08-16T13:41:22.404359Z","submitted_at":"2024-06-19T17:19:10Z","title":"Beyond modified Urca: the nucleon width approximation for flavor-changing processes in dense matter","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2406.13717","snapshot_observed_at":"2026-08-07T15:31:32.597991Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2505.14921","last_updated":"2025-05-20T21:15:29Z","snapshot_observed_at":"2026-08-17T17:52:18.930922Z","submitted_at":"2025-05-20T21:15:29Z","title":"An Overview of the MUSES Calculation Engine and How It Can Be Used to Describe Neutron Stars","version":1},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-07T15:31:32.597991Z"},"links":{"cited_paper":"/paper/2406.13717","citing_paper":"/paper/2505.14921"},"observation_digest":"sha256:f85a461240ff93d32f5c161dd1d7717b4225f4a36975bf1ea992816b67e6c73a","observation_id":"b0d1bec3-b832-4557-8eec-73fb886bbab8","resolution":{"observed_at":"2026-08-07T15:31:32.597991Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2406.13717","last_updated":"2024-06-19T17:19:10Z","snapshot_observed_at":"2026-08-16T13:41:22.404359Z","submitted_at":"2024-06-19T17:19:10Z","title":"Beyond modified Urca: the nucleon width approximation for flavor-changing processes in dense matter","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2406.13717","snapshot_observed_at":"2026-08-05T15:53:22.585083Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2508.19222","last_updated":"2025-08-26T17:39:15Z","snapshot_observed_at":"2026-08-09T15:15:44.935030Z","submitted_at":"2025-08-26T17:39:15Z","title":"Classification of color superconductivity by one-gluon exchange helicity amplitudes and renormalization group equations","version":1},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-05T15:53:22.585083Z"},"links":{"cited_paper":"/paper/2406.13717","citing_paper":"/paper/2508.19222"},"observation_digest":"sha256:039365ad3ed7ecdda4afe7e593d466184232500a39b846d49c29d605575a58d1","observation_id":"775af8ef-89d5-494a-a35a-fb1732c27b5b","resolution":{"observed_at":"2026-08-05T15:53:22.585083Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2406.13717","last_updated":"2024-06-19T17:19:10Z","snapshot_observed_at":"2026-08-16T13:41:22.404359Z","submitted_at":"2024-06-19T17:19:10Z","title":"Beyond modified Urca: the nucleon width approximation for flavor-changing processes in dense matter","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2406.13717","snapshot_observed_at":"2026-08-05T10:17:57.017374Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2509.04240","last_updated":"2025-09-04T14:14:59Z","snapshot_observed_at":"2026-08-16T22:43:16.818344Z","submitted_at":"2025-09-04T14:14:59Z","title":"Neutrino absorption in two-flavor color-superconducting quark matter","version":1},"reference_index":55,"source":"pdf_text","source_observed_at":"2026-08-05T10:17:57.017374Z"},"links":{"cited_paper":"/paper/2406.13717","citing_paper":"/paper/2509.04240"},"observation_digest":"sha256:0aa8e602c2961243e1dc2516cd0b9a9707af3cce744fedc02a9091b77de98683","observation_id":"5f8774cc-aa0e-4ce7-b941-0d625d6fdfc7","resolution":{"observed_at":"2026-08-05T10:17:57.017374Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2406.13717","last_updated":"2024-06-19T17:19:10Z","snapshot_observed_at":"2026-08-16T13:41:22.404359Z","submitted_at":"2024-06-19T17:19:10Z","title":"Beyond modified Urca: the nucleon width approximation for flavor-changing processes in dense matter","version":1},"cited_work":{"arxiv_id":"2406.13717","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2406.13717","snapshot_observed_at":"2026-07-04T16:19:57.284731Z","title":null,"venue":null,"work_id":"9d87ef4a-83be-4a80-b8f1-c834af3d32d7","year":2024},"citing_paper":{"arxiv_id":"2509.25838","last_updated":"2026-04-16T18:51:06Z","snapshot_observed_at":"2026-08-16T18:16:01.156053Z","submitted_at":"2025-09-30T06:23:26Z","title":"Bulk viscosity from neutron decays to dark baryons in neutron star matter","version":2},"reference_index":130,"source":"pdf_text","source_observed_at":"2026-05-18T12:44:55.766757Z"},"links":{"cited_paper":"/paper/2406.13717","citing_paper":"/paper/2509.25838"},"observation_digest":"sha256:17c2665db517db202b9dc91c97f95748e7c50af189b0c1f152d231d04970648d","observation_id":"beaedda9-c175-406d-9595-49bf1b4d7636","resolution":{"observed_at":"2026-05-18T12:46:23.853491Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2406.13717","last_updated":"2024-06-19T17:19:10Z","snapshot_observed_at":"2026-08-16T13:41:22.404359Z","submitted_at":"2024-06-19T17:19:10Z","title":"Beyond modified Urca: the nucleon width approximation for flavor-changing processes in dense matter","version":1},"cited_work":{"arxiv_id":"2406.13717","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2406.13717","snapshot_observed_at":"2026-07-04T16:19:57.284731Z","title":null,"venue":null,"work_id":"9d87ef4a-83be-4a80-b8f1-c834af3d32d7","year":2024},"citing_paper":{"arxiv_id":"2510.09104","last_updated":"2026-05-21T12:53:58Z","snapshot_observed_at":"2026-08-18T17:09:57.052389Z","submitted_at":"2025-10-10T07:58:38Z","title":"Thermal and Magnetic effects on Bulk Viscosity in Binary Neutron Star Mergers","version":3},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-05-22T12:52:58.423553Z"},"links":{"cited_paper":"/paper/2406.13717","citing_paper":"/paper/2510.09104"},"observation_digest":"sha256:fb5895418f4e81933fb5bfb0ab3347e3f48903e1b4eeb726a15230be7ba60008","observation_id":"6641382a-92b2-462f-bae1-82cb99596bf9","resolution":{"observed_at":"2026-05-22T12:54:52.482346Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2406.13717","last_updated":"2024-06-19T17:19:10Z","snapshot_observed_at":"2026-08-16T13:41:22.404359Z","submitted_at":"2024-06-19T17:19:10Z","title":"Beyond modified Urca: the nucleon width approximation for flavor-changing processes in dense matter","version":1},"cited_work":{"arxiv_id":"2406.13717","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2406.13717","snapshot_observed_at":"2026-07-04T16:19:57.284731Z","title":null,"venue":null,"work_id":"9d87ef4a-83be-4a80-b8f1-c834af3d32d7","year":2024},"citing_paper":{"arxiv_id":"2605.29187","last_updated":"2026-05-27T23:52:21Z","snapshot_observed_at":"2026-08-07T01:23:31.781933Z","submitted_at":"2026-05-27T23:52:21Z","title":"Assessing the Relative Importance of Neutrino Matter Interaction Channels in Post-Merger Remnant of Binary Neutron Stars","version":1},"reference_index":73,"source":"pdf_text","source_observed_at":"2026-06-29T10:03:39.187375Z"},"links":{"cited_paper":"/paper/2406.13717","citing_paper":"/paper/2605.29187"},"observation_digest":"sha256:f203f4d047311610c703db7b9b8d40158a9b25b6c931cfb87d7acc8fedb2317a","observation_id":"104fdf87-edfd-4b52-bbe1-5bdd6e19f2fd","resolution":{"observed_at":"2026-06-29T10:13:18.007740Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2406.13717","last_updated":"2024-06-19T17:19:10Z","snapshot_observed_at":"2026-08-16T13:41:22.404359Z","submitted_at":"2024-06-19T17:19:10Z","title":"Beyond modified Urca: the nucleon width approximation for flavor-changing processes in dense matter","version":1},"cited_work":{"arxiv_id":"2406.13717","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2406.13717","snapshot_observed_at":"2026-07-04T16:19:57.284731Z","title":null,"venue":null,"work_id":"9d87ef4a-83be-4a80-b8f1-c834af3d32d7","year":2024},"citing_paper":{"arxiv_id":"2606.26326","last_updated":"2026-06-24T19:12:40Z","snapshot_observed_at":"2026-08-15T14:06:50.779231Z","submitted_at":"2026-06-24T19:12:40Z","title":"Studying the QCD Matter produced in Heavy-Ion Collisions using the MUSES Calculation Engine","version":1},"reference_index":157,"source":"pdf_text","source_observed_at":"2026-06-26T00:47:21.247516Z"},"links":{"cited_paper":"/paper/2406.13717","citing_paper":"/paper/2606.26326"},"observation_digest":"sha256:9d951941dce34e72b9ab52ec74c85bd45aeb308521359585012dc9d1c6acbadb","observation_id":"2ed51122-3c41-48e8-8305-3356633b6388","resolution":{"observed_at":"2026-07-04T16:19:57.286169Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2406.13717","last_updated":"2024-06-19T17:19:10Z","snapshot_observed_at":"2026-08-16T13:41:22.404359Z","submitted_at":"2024-06-19T17:19:10Z","title":"Beyond modified Urca: the nucleon width approximation for flavor-changing processes in dense matter","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2406.13717","snapshot_observed_at":"2026-08-16T00:21:42.891574Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2608.12091","last_updated":"2026-08-12T14:14:10Z","snapshot_observed_at":"2026-08-19T10:26:32.818138Z","submitted_at":"2026-08-12T14:14:10Z","title":"Transport properties in binary neutron star mergers: Effect of magnetic field","version":1},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-16T00:21:42.891574Z"},"links":{"cited_paper":"/paper/2406.13717","citing_paper":"/paper/2608.12091"},"observation_digest":"sha256:f472e484e42406ed326aaedd9c912cb0bdd7c2ce17461782974592329b1578ef","observation_id":"eb36e55c-343c-41d0-bc0c-6cd6e93c820f","resolution":{"observed_at":"2026-08-16T00:21:42.891574Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2406.13717/citation-record","integrity":"/paper/2406.13717/integrity","json":"/paper/2406.13717/citation-record.json","paper":"/paper/2406.13717"},"outbound":[],"paper":{"arxiv_id":"2406.13717","last_updated":"2024-06-19T17:19:10Z","latest_version":1,"primary_category":"nucl-th","snapshot_observed_at":"2026-08-16T13:41:22.404359Z","submitted_at":"2024-06-19T17:19:10Z","title":"Beyond modified Urca: the nucleon width approximation for flavor-changing processes in dense matter"},"reference_resolution":{"displayed":0,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":0,"verified_exact":0,"verified_fuzzy":0},"total_outbound_references":0},"refusal":"A citation records a reference. It does not transfer a finding from one paper to another.","schema":"pith.paper-citation-record.v1","standing_sources":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"thesis":"As of 21 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 9 inbound Pith citation observations for arXiv:2406.13717."}