{"as_of":"2026-08-08T04:45:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:a7774187afbf30cf56f58cd57ce0880950189542b76b41447509d941a0decbcd","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":5,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":5,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-07T06:34:17.273281+00:00","state":"measured"},{"denominator":5,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":5,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-06T19:44:32.364106Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"arxiv_reference","source_observed_at":"2026-05-11T19:41:09.644773Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"1411.6681","last_updated":"2015-10-10T19:29:16Z","snapshot_observed_at":"2026-07-06T04:01:34.274140Z","submitted_at":"2014-11-24T23:05:05Z","title":"Chiral symmetry and effective field theories for hadronic, nuclear and stellar matter","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1411.6681","snapshot_observed_at":"2026-08-06T19:44:32.364106Z","title":"Chiral symmetry and effective field theories for hadronic, nuclear and stellar matter,","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2507.04939","last_updated":"2025-08-05T17:03:39Z","snapshot_observed_at":"2026-08-06T19:33:22.239679Z","submitted_at":"2025-07-07T12:36:55Z","title":"From Nuclear Matter with Quenched $g_A$ to Compact-Star Matter with a Signal for Emergent Hidden Scale Symmetry","version":4},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-06T19:44:32.364106Z"},"links":{"cited_paper":"/paper/1411.6681","citing_paper":"/paper/2507.04939"},"observation_digest":"sha256:a9d961b50a3bae6cb73fe519eadf1d2a5ac9d1c72a5127f7010b4c5bd1638dfc","observation_id":"65fa6ef5-74c5-4949-aced-fa308dfe6db5","resolution":{"observed_at":"2026-08-06T19:44:32.364106Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1411.6681","last_updated":"2015-10-10T19:29:16Z","snapshot_observed_at":"2026-07-06T04:01:34.274140Z","submitted_at":"2014-11-24T23:05:05Z","title":"Chiral symmetry and effective field theories for hadronic, nuclear and stellar matter","version":2},"cited_work":{"arxiv_id":"1411.6681","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"1411.6681","snapshot_observed_at":"2026-07-04T20:36:53.442999Z","title":null,"venue":null,"work_id":"b144a0af-0b62-4b80-b435-824c007b8364","year":2016},"citing_paper":{"arxiv_id":"2604.09154","last_updated":"2026-04-20T10:05:19Z","snapshot_observed_at":"2026-07-06T22:58:04.106299Z","submitted_at":"2026-04-10T09:40:42Z","title":"From binding and saturation to criticality in nuclear matter with lattice effective field theory","version":2},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-05-10T17:28:56.147494Z"},"links":{"cited_paper":"/paper/1411.6681","citing_paper":"/paper/2604.09154"},"observation_digest":"sha256:fc920d16cf13f51767431640b0ea8685ce7f4bbafb9d116cd58c39735427a0a4","observation_id":"5e840370-c451-4fd0-af69-8a8cac50b62a","resolution":{"observed_at":"2026-07-04T20:36:53.442999Z","resolver_source":"arxiv_id","status":"malformed_identifier"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1411.6681","last_updated":"2015-10-10T19:29:16Z","snapshot_observed_at":"2026-07-06T04:01:34.274140Z","submitted_at":"2014-11-24T23:05:05Z","title":"Chiral symmetry and effective field theories for hadronic, nuclear and stellar matter","version":2},"cited_work":{"arxiv_id":"1411.6681","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"1411.6681","snapshot_observed_at":"2026-07-04T20:36:53.442999Z","title":null,"venue":null,"work_id":"b144a0af-0b62-4b80-b435-824c007b8364","year":2016},"citing_paper":{"arxiv_id":"2604.22382","last_updated":"2026-04-24T09:21:10Z","snapshot_observed_at":"2026-07-06T23:08:47.078992Z","submitted_at":"2026-04-24T09:21:10Z","title":"QCD vacuum pressure and its influence on the equation of state of non-strange quark stars","version":1},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-05-08T11:15:42.182424Z"},"links":{"cited_paper":"/paper/1411.6681","citing_paper":"/paper/2604.22382"},"observation_digest":"sha256:bfeef7252fc7a1f88abadb8a47bacc3efc20b54dec086e7143aa9e839eae23b5","observation_id":"c9de26fa-8967-4f4a-8910-7988443091fe","resolution":{"observed_at":"2026-07-04T20:36:53.442999Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1411.6681","last_updated":"2015-10-10T19:29:16Z","snapshot_observed_at":"2026-07-06T04:01:34.274140Z","submitted_at":"2014-11-24T23:05:05Z","title":"Chiral symmetry and effective field theories for hadronic, nuclear and stellar matter","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1411.6681","snapshot_observed_at":"2026-08-02T03:23:32.042731Z","title":null,"venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2607.13930","last_updated":"2026-07-15T15:12:43Z","snapshot_observed_at":"2026-08-03T13:21:18.717784Z","submitted_at":"2026-07-15T15:12:43Z","title":"NNStar: An end-to-end AI agent for nuclear matter and neutron star physics","version":1},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-02T03:23:32.042731Z"},"links":{"cited_paper":"/paper/1411.6681","citing_paper":"/paper/2607.13930"},"observation_digest":"sha256:413c1949f985f50bb151da1478a7d62a1e9234ddd32f15e9eb9e5ee5567e8ce8","observation_id":"6ca25f5c-eb89-4af5-82ad-d3adca4f5f8c","resolution":{"observed_at":"2026-08-02T03:23:32.042731Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1411.6681","last_updated":"2015-10-10T19:29:16Z","snapshot_observed_at":"2026-07-06T04:01:34.274140Z","submitted_at":"2014-11-24T23:05:05Z","title":"Chiral symmetry and effective field theories for hadronic, nuclear and stellar matter","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1411.6681","snapshot_observed_at":"2026-08-02T03:00:54.016077Z","title":"Holt, Mannque Rho, and Wolfram Weise","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2607.14058","last_updated":"2026-07-15T17:29:11Z","snapshot_observed_at":"2026-08-06T22:54:05.833536Z","submitted_at":"2026-07-15T17:29:11Z","title":"Towards compressed baryonic matter densities: D meson diffusion","version":1},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-08-02T03:00:54.016077Z"},"links":{"cited_paper":"/paper/1411.6681","citing_paper":"/paper/2607.14058"},"observation_digest":"sha256:84a031fe81cbcd3f47039d2dd05d47886d2e028f8af95a2f9d50911bb789f4ea","observation_id":"6f28daeb-58e5-4265-83cf-4204c93fb042","resolution":{"observed_at":"2026-08-02T03:00:54.016077Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/1411.6681/citation-record","integrity":"/paper/1411.6681/integrity","json":"/paper/1411.6681/citation-record.json","paper":"/paper/1411.6681"},"outbound":[],"paper":{"arxiv_id":"1411.6681","last_updated":"2015-10-10T19:29:16Z","latest_version":2,"primary_category":"nucl-th","snapshot_observed_at":"2026-07-06T04:01:34.274140Z","submitted_at":"2014-11-24T23:05:05Z","title":"Chiral symmetry and effective field theories for hadronic, nuclear and stellar 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":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"thesis":"As of 8 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:1411.6681."}