{"as_of":"2026-08-16T20:30:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:f0a97ce374c023ea61854d10524ea1cdd8e49149c435bf2e5c891545d024adc9","coverage":[{"denominator":69,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":69,"source":"paper_references, paper_reference_links","source_observed_at":"2026-06-29T00:09:37.360084Z","state":"measured"},{"denominator":70,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":70,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-16T06:30:59.297886+00:00","state":"measured"},{"denominator":1,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":1,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-15T15:24:21.722629Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"pith","source_observed_at":"2026-08-15T15:24:22.617313Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2605.30554","last_updated":"2026-05-28T20:36:30Z","snapshot_observed_at":"2026-08-15T18:36:46.400731Z","submitted_at":"2026-05-28T20:36:30Z","title":"Effects of the Symmetry energy slope on the exotic content of the neutron stars","version":1},"cited_work":{"arxiv_id":"2605.30554","doi":null,"metadata_source":"pith","pith_arxiv_id":"2605.30554","snapshot_observed_at":"2026-08-15T15:24:22.617313Z","title":"Effects of the Symmetry energy slope on the exotic content of the neutron stars","venue":"nucl-th","work_id":"8089c498-4f8f-4492-99ba-651e2322eacd","year":2026},"citing_paper":{"arxiv_id":"2608.00439","last_updated":"2026-08-01T04:35:12Z","snapshot_observed_at":"2026-08-15T19:07:00.875902Z","submitted_at":"2026-08-01T04:35:12Z","title":"An Undergraduate Approach to the Quantum Hadrodynamics and the Physics of Neutron Stars Part II: Neutron Stars' Exotic Content","version":1},"reference_index":61,"source":"pdf_text","source_observed_at":"2026-08-15T15:24:21.722629Z"},"links":{"cited_paper":"/paper/2605.30554","citing_paper":"/paper/2608.00439"},"observation_digest":"sha256:4b7471ea8be9df6a9591023b0614d88b5e22ad2d0cbe7c45d09d8212a8d0a99b","observation_id":"90772f3a-daf0-4cc6-aa2f-c4f13420fd3e","resolution":{"observed_at":"2026-08-15T15:24:22.622291Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/2605.30554/citation-record","integrity":"/paper/2605.30554/integrity","json":"/paper/2605.30554/citation-record.json","paper":"/paper/2605.30554"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-06-29T00:09:37.360084Z","title":"This result is exacerbated for the L = 92 MeV in the L3 ωρ , whose onset is pushed to higher densities","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2605.30554","last_updated":"2026-05-28T20:36:30Z","snapshot_observed_at":"2026-08-15T18:36:46.400731Z","submitted_at":"2026-05-28T20:36:30Z","title":"Effects of the Symmetry energy slope on the exotic content of the neutron stars","version":1},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-06-29T00:09:37.360084Z"},"links":{"citing_paper":"/paper/2605.30554"},"observation_digest":"sha256:ba2f6e62a6e5f2dbfa6a9e2eaf347fb929c99085388b25746a32ec137388cdf6","observation_id":"32b1095f-c7c3-4171-8b36-b8456d1ed227","resolution":{"observed_at":"2026-06-29T00:09:37.360084Z","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":"2026-06-29T00:09:37.360084Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2605.30554","last_updated":"2026-05-28T20:36:30Z","snapshot_observed_at":"2026-08-15T18:36:46.400731Z","submitted_at":"2026-05-28T20:36:30Z","title":"Effects of the Symmetry energy slope on the exotic content of the neutron stars","version":1},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-06-29T00:09:37.360084Z"},"links":{"citing_paper":"/paper/2605.30554"},"observation_digest":"sha256:92965723bb4f07761d6abb8d693ea53552e5474c4e6a87331e8f244c0094a6c3","observation_id":"4e04fb8d-4952-4d39-9ff8-e184ae0aed3a","resolution":{"observed_at":"2026-06-29T00:09:37.360084Z","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":"2026-06-29T00:09:37.360084Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2605.30554","last_updated":"2026-05-28T20:36:30Z","snapshot_observed_at":"2026-08-15T18:36:46.400731Z","submitted_at":"2026-05-28T20:36:30Z","title":"Effects of the Symmetry energy slope on the exotic content of the neutron stars","version":1},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-06-29T00:09:37.360084Z"},"links":{"citing_paper":"/paper/2605.30554"},"observation_digest":"sha256:1240b8a61e22ad2f45a85daa77365fe499470f5eeb368c52e8f4ff755d784007","observation_id":"08bfcf53-f3ae-40b7-a685-b66e5ad78b86","resolution":{"observed_at":"2026-06-29T00:09:37.360084Z","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":"2026-06-29T00:09:37.360084Z","title":"01M⊙ star has its radius reduced due to the onset of hyperons","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2605.30554","last_updated":"2026-05-28T20:36:30Z","snapshot_observed_at":"2026-08-15T18:36:46.400731Z","submitted_at":"2026-05-28T20:36:30Z","title":"Effects of the Symmetry energy slope on the exotic content of the neutron stars","version":1},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-06-29T00:09:37.360084Z"},"links":{"citing_paper":"/paper/2605.30554"},"observation_digest":"sha256:43958f27e9291cb4be45087341e563a6f589d95cbea48739e164d9ed73243468","observation_id":"e8f8b297-8b4c-4184-acab-b87bd2e65ec0","resolution":{"observed_at":"2026-06-29T00:09:37.360084Z","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":"2026-06-29T00:09:37.360084Z","title":null,"venue":null,"work_id":null,"year":1994},"citing_paper":{"arxiv_id":"2605.30554","last_updated":"2026-05-28T20:36:30Z","snapshot_observed_at":"2026-08-15T18:36:46.400731Z","submitted_at":"2026-05-28T20:36:30Z","title":"Effects of the Symmetry energy slope on the exotic content of the neutron stars","version":1},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-06-29T00:09:37.360084Z"},"links":{"citing_paper":"/paper/2605.30554"},"observation_digest":"sha256:9afb9b1d8766518fdb1967f3fa516cecfd02d68541d9806ac8058443ed8a0581","observation_id":"8f0de8c9-0b9d-46ee-9d71-68d41ad1a420","resolution":{"observed_at":"2026-06-29T00:09:37.360084Z","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":"2026-06-29T00:09:37.360084Z","title":null,"venue":null,"work_id":null,"year":2000},"citing_paper":{"arxiv_id":"2605.30554","last_updated":"2026-05-28T20:36:30Z","snapshot_observed_at":"2026-08-15T18:36:46.400731Z","submitted_at":"2026-05-28T20:36:30Z","title":"Effects of the Symmetry energy slope on the exotic content of the neutron stars","version":1},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-06-29T00:09:37.360084Z"},"links":{"citing_paper":"/paper/2605.30554"},"observation_digest":"sha256:906ee86ca39853ae920dd49dc56240cf213bc35b997c27c73de0c83fd0f6085c","observation_id":"78637df1-7e27-4662-a580-7cab613833ba","resolution":{"observed_at":"2026-06-29T00:09:37.360084Z","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":"2026-06-29T00:09:37.360084Z","title":"Bethe and M","venue":null,"work_id":null,"year":1974},"citing_paper":{"arxiv_id":"2605.30554","last_updated":"2026-05-28T20:36:30Z","snapshot_observed_at":"2026-08-15T18:36:46.400731Z","submitted_at":"2026-05-28T20:36:30Z","title":"Effects of the Symmetry energy slope on the exotic content of the neutron stars","version":1},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-06-29T00:09:37.360084Z"},"links":{"citing_paper":"/paper/2605.30554"},"observation_digest":"sha256:6856f330a1e56c52881648bd86d3d174c23610559abdc5f9f1892c8072433f77","observation_id":"f4b3ca33-9982-4774-893a-3fa1f9b6f0b7","resolution":{"observed_at":"2026-06-29T00:09:37.360084Z","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":"2026-06-29T00:09:37.360084Z","title":null,"venue":null,"work_id":null,"year":1982},"citing_paper":{"arxiv_id":"2605.30554","last_updated":"2026-05-28T20:36:30Z","snapshot_observed_at":"2026-08-15T18:36:46.400731Z","submitted_at":"2026-05-28T20:36:30Z","title":"Effects of the Symmetry energy slope on the exotic content of the neutron stars","version":1},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-06-29T00:09:37.360084Z"},"links":{"citing_paper":"/paper/2605.30554"},"observation_digest":"sha256:eba87a78803bcda765444e49ab69ade45e47c18ac20ddae32f53689741512367","observation_id":"8e3654b4-1c4b-40f4-845b-acbed3f8a406","resolution":{"observed_at":"2026-06-29T00:09:37.360084Z","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":"2026-06-29T00:09:37.360084Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2605.30554","last_updated":"2026-05-28T20:36:30Z","snapshot_observed_at":"2026-08-15T18:36:46.400731Z","submitted_at":"2026-05-28T20:36:30Z","title":"Effects of the Symmetry energy slope on the exotic content of the neutron stars","version":1},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-06-29T00:09:37.360084Z"},"links":{"citing_paper":"/paper/2605.30554"},"observation_digest":"sha256:1e09d553f4f7406933dbb4abc60ff1fe1767996dc02f594c29f327c3b5ad3172","observation_id":"586db116-e985-4777-b523-6e0a09204371","resolution":{"observed_at":"2026-06-29T00:09:37.360084Z","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":"2026-06-29T00:09:37.360084Z","title":"Sedrakian, J.-J","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2605.30554","last_updated":"2026-05-28T20:36:30Z","snapshot_observed_at":"2026-08-15T18:36:46.400731Z","submitted_at":"2026-05-28T20:36:30Z","title":"Effects of the Symmetry energy slope on the exotic content of the neutron stars","version":1},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-06-29T00:09:37.360084Z"},"links":{"citing_paper":"/paper/2605.30554"},"observation_digest":"sha256:a647add59de1753baff8c09fd4c2e55ca77e4977e1233d9df4af665311859d70","observation_id":"0f4b32ab-f090-4922-8fde-996a9f6fa2c4","resolution":{"observed_at":"2026-06-29T00:09:37.360084Z","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":"2026-06-29T00:09:37.360084Z","title":"Chorozidou and T","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2605.30554","last_updated":"2026-05-28T20:36:30Z","snapshot_observed_at":"2026-08-15T18:36:46.400731Z","submitted_at":"2026-05-28T20:36:30Z","title":"Effects of the Symmetry energy slope on the exotic content of the neutron stars","version":1},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-06-29T00:09:37.360084Z"},"links":{"citing_paper":"/paper/2605.30554"},"observation_digest":"sha256:71f5c629651f11d022f479ff6a9e57f56b949f0facd86951e6126cb0292a28b2","observation_id":"bfab8a77-5d06-44d0-a947-15d76199d12f","resolution":{"observed_at":"2026-06-29T00:09:37.360084Z","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":"2026-06-29T00:09:37.360084Z","title":"Dapo, B.-J","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2605.30554","last_updated":"2026-05-28T20:36:30Z","snapshot_observed_at":"2026-08-15T18:36:46.400731Z","submitted_at":"2026-05-28T20:36:30Z","title":"Effects of the Symmetry energy slope on the exotic content of the neutron stars","version":1},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-06-29T00:09:37.360084Z"},"links":{"citing_paper":"/paper/2605.30554"},"observation_digest":"sha256:b06740befe66b41b795f3d5755b1cdc70aac73945548b8c5c50161475d184fbe","observation_id":"74243f0f-9815-46a0-a0c6-bea2f528a8a0","resolution":{"observed_at":"2026-06-29T00:09:37.360084Z","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":"2026-06-29T00:09:37.360084Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2605.30554","last_updated":"2026-05-28T20:36:30Z","snapshot_observed_at":"2026-08-15T18:36:46.400731Z","submitted_at":"2026-05-28T20:36:30Z","title":"Effects of the Symmetry energy slope on the exotic content of the neutron stars","version":1},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-06-29T00:09:37.360084Z"},"links":{"citing_paper":"/paper/2605.30554"},"observation_digest":"sha256:274b50a40fbfffcbcd036cfa2b756ac3b5ebd516bc9de2cd9da04af83e278c18","observation_id":"720931a8-149f-4512-a0ab-b96514dce304","resolution":{"observed_at":"2026-06-29T00:09:37.360084Z","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":"2026-06-29T00:09:37.360084Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2605.30554","last_updated":"2026-05-28T20:36:30Z","snapshot_observed_at":"2026-08-15T18:36:46.400731Z","submitted_at":"2026-05-28T20:36:30Z","title":"Effects of the Symmetry energy slope on the exotic content of the neutron stars","version":1},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-06-29T00:09:37.360084Z"},"links":{"citing_paper":"/paper/2605.30554"},"observation_digest":"sha256:29cdb52474a22f03807690b4dca7126c81787fe7a00cfc393b1cc9be8813925f","observation_id":"6d1748fd-0506-4913-9770-d72a58a45b50","resolution":{"observed_at":"2026-06-29T00:09:37.360084Z","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":"2026-06-29T00:09:37.360084Z","title":"Mohammad Ali Looee, M","venue":null,"work_id":null,"year":2026},"citing_paper":{"arxiv_id":"2605.30554","last_updated":"2026-05-28T20:36:30Z","snapshot_observed_at":"2026-08-15T18:36:46.400731Z","submitted_at":"2026-05-28T20:36:30Z","title":"Effects of the Symmetry energy slope on the exotic content of the neutron stars","version":1},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-06-29T00:09:37.360084Z"},"links":{"citing_paper":"/paper/2605.30554"},"observation_digest":"sha256:8765e49e532e9fd6bd89cee59af50867b2d7027d7189515698a81522d677b0ba","observation_id":"c1cf8530-de29-441c-8fe4-a9b8eec1c450","resolution":{"observed_at":"2026-06-29T00:09:37.360084Z","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":"2026-06-29T00:09:37.360084Z","title":"Bodek and T","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2605.30554","last_updated":"2026-05-28T20:36:30Z","snapshot_observed_at":"2026-08-15T18:36:46.400731Z","submitted_at":"2026-05-28T20:36:30Z","title":"Effects of the Symmetry energy slope on the exotic content of the neutron stars","version":1},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-06-29T00:09:37.360084Z"},"links":{"citing_paper":"/paper/2605.30554"},"observation_digest":"sha256:9f4258f3e8b21e483dd24380f1af8c8875f1fabc1f25cf092be3aca539e18b20","observation_id":"5436d2f7-4aad-4e4d-ac53-fa92cc2ea9b6","resolution":{"observed_at":"2026-06-29T00:09:37.360084Z","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":"2026-06-29T00:09:37.360084Z","title":null,"venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2605.30554","last_updated":"2026-05-28T20:36:30Z","snapshot_observed_at":"2026-08-15T18:36:46.400731Z","submitted_at":"2026-05-28T20:36:30Z","title":"Effects of the Symmetry energy slope on the exotic content of the neutron stars","version":1},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-06-29T00:09:37.360084Z"},"links":{"citing_paper":"/paper/2605.30554"},"observation_digest":"sha256:fa339e69159115a3fd7a41a56ad1dca7c056b760730cccd15727db4f7d62e837","observation_id":"f2e5a0cb-1f0b-48b7-8ade-cc8927f62a8c","resolution":{"observed_at":"2026-06-29T00:09:37.360084Z","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":"2026-06-29T00:09:37.360084Z","title":"Kolomeitsev, K","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2605.30554","last_updated":"2026-05-28T20:36:30Z","snapshot_observed_at":"2026-08-15T18:36:46.400731Z","submitted_at":"2026-05-28T20:36:30Z","title":"Effects of the Symmetry energy slope on the exotic content of the neutron stars","version":1},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-06-29T00:09:37.360084Z"},"links":{"citing_paper":"/paper/2605.30554"},"observation_digest":"sha256:f31fde2da621a3cb56acfe41621e346f2da55a762c5e524c1352e870cbff5fe1","observation_id":"a561f97b-0e98-4687-b30f-72d1060afd4d","resolution":{"observed_at":"2026-06-29T00:09:37.360084Z","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":"2026-06-29T00:09:37.360084Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2605.30554","last_updated":"2026-05-28T20:36:30Z","snapshot_observed_at":"2026-08-15T18:36:46.400731Z","submitted_at":"2026-05-28T20:36:30Z","title":"Effects of the Symmetry energy slope on the exotic content of the neutron stars","version":1},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-06-29T00:09:37.360084Z"},"links":{"citing_paper":"/paper/2605.30554"},"observation_digest":"sha256:e48c23c691b189e939c3f190c2a970248ef21b6ee9624a0a53154647d8986214","observation_id":"a42c5447-09af-483a-9887-991d0590cc9c","resolution":{"observed_at":"2026-06-29T00:09:37.360084Z","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":"2026-06-29T00:09:37.360084Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2605.30554","last_updated":"2026-05-28T20:36:30Z","snapshot_observed_at":"2026-08-15T18:36:46.400731Z","submitted_at":"2026-05-28T20:36:30Z","title":"Effects of the Symmetry energy slope on the exotic content of the neutron stars","version":1},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-06-29T00:09:37.360084Z"},"links":{"citing_paper":"/paper/2605.30554"},"observation_digest":"sha256:faf91a4f8bc9d19bfe442ba92f603ab07937bc32a0601c304e3e9496f4e0bd4f","observation_id":"a27bfc77-8bff-4282-93cd-c122110724a9","resolution":{"observed_at":"2026-06-29T00:09:37.360084Z","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":"2026-06-29T00:09:37.360084Z","title":"Dutra, O","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2605.30554","last_updated":"2026-05-28T20:36:30Z","snapshot_observed_at":"2026-08-15T18:36:46.400731Z","submitted_at":"2026-05-28T20:36:30Z","title":"Effects of the Symmetry energy slope on the exotic content of the neutron stars","version":1},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-06-29T00:09:37.360084Z"},"links":{"citing_paper":"/paper/2605.30554"},"observation_digest":"sha256:bf5be04306858311c75511f557a63b29e5356f373cdb9dcbe27cdfda548d02f3","observation_id":"36bb6a89-ff75-41ff-b385-59ccde2e24a5","resolution":{"observed_at":"2026-06-29T00:09:37.360084Z","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":"2026-06-29T00:09:37.360084Z","title":"Oertel, M","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2605.30554","last_updated":"2026-05-28T20:36:30Z","snapshot_observed_at":"2026-08-15T18:36:46.400731Z","submitted_at":"2026-05-28T20:36:30Z","title":"Effects of the Symmetry energy slope on the exotic content of the neutron stars","version":1},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-06-29T00:09:37.360084Z"},"links":{"citing_paper":"/paper/2605.30554"},"observation_digest":"sha256:b08db18029f607fcb78f7f019f722609f5a62f6fd1ac65d907944a0cc7b0d188","observation_id":"34037698-578d-4435-ba63-f2c4fc11bc1f","resolution":{"observed_at":"2026-06-29T00:09:37.360084Z","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":"2026-06-29T00:09:37.360084Z","title":"Paar et al., Neutron star structure and collective exci- tations of ﬁnite nuclei, Phys","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2605.30554","last_updated":"2026-05-28T20:36:30Z","snapshot_observed_at":"2026-08-15T18:36:46.400731Z","submitted_at":"2026-05-28T20:36:30Z","title":"Effects of the Symmetry energy slope on the exotic content of the neutron stars","version":1},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-06-29T00:09:37.360084Z"},"links":{"citing_paper":"/paper/2605.30554"},"observation_digest":"sha256:0aae892a11cdd35abe6d2fe9ff8e451a5c338672f7c8364be23db52ee432fdf5","observation_id":"0e83bf13-17ea-4511-9c41-72660a5db4c6","resolution":{"observed_at":"2026-06-29T00:09:37.360084Z","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":"2026-06-29T00:09:37.360084Z","title":"Lattimer and A","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2605.30554","last_updated":"2026-05-28T20:36:30Z","snapshot_observed_at":"2026-08-15T18:36:46.400731Z","submitted_at":"2026-05-28T20:36:30Z","title":"Effects of the Symmetry energy slope on the exotic content of the neutron stars","version":1},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-06-29T00:09:37.360084Z"},"links":{"citing_paper":"/paper/2605.30554"},"observation_digest":"sha256:47ec8e3262d4fb58091fd7bc1f5d86c3fc1abe511ec3ee1a41f9697e9a325cf6","observation_id":"d7cbacf8-21cf-42ab-b4e5-e28da348b3db","resolution":{"observed_at":"2026-06-29T00:09:37.360084Z","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":"2026-06-29T00:09:37.360084Z","title":"Lattimer and Y","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2605.30554","last_updated":"2026-05-28T20:36:30Z","snapshot_observed_at":"2026-08-15T18:36:46.400731Z","submitted_at":"2026-05-28T20:36:30Z","title":"Effects of the Symmetry energy slope on the exotic content of the neutron stars","version":1},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-06-29T00:09:37.360084Z"},"links":{"citing_paper":"/paper/2605.30554"},"observation_digest":"sha256:2a951074fb4bb3800e4e722f39931624877b46b87068d40f9b874d4ff8f368d4","observation_id":"09abad2d-8cf3-4ff0-bf0d-8372335084dc","resolution":{"observed_at":"2026-06-29T00:09:37.360084Z","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":"2026-06-29T00:09:37.360084Z","title":"Estee et al., Probing the symmetry energy with the spectral pion ratio, Phys","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2605.30554","last_updated":"2026-05-28T20:36:30Z","snapshot_observed_at":"2026-08-15T18:36:46.400731Z","submitted_at":"2026-05-28T20:36:30Z","title":"Effects of the Symmetry energy slope on the exotic content of the neutron stars","version":1},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-06-29T00:09:37.360084Z"},"links":{"citing_paper":"/paper/2605.30554"},"observation_digest":"sha256:34db58f1beda48e74919ca92c8c70ffbd753d128e650f01aae5db8383ed5f62c","observation_id":"22da33dc-1d1e-4d2a-80ee-83684a92b7ba","resolution":{"observed_at":"2026-06-29T00:09:37.360084Z","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":"2026-06-29T00:09:37.360084Z","title":"Reed et al., Implications of prex-2 on the equation of state of neutron-rich matter, Phys","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2605.30554","last_updated":"2026-05-28T20:36:30Z","snapshot_observed_at":"2026-08-15T18:36:46.400731Z","submitted_at":"2026-05-28T20:36:30Z","title":"Effects of the Symmetry energy slope on the exotic content of the neutron stars","version":1},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-06-29T00:09:37.360084Z"},"links":{"citing_paper":"/paper/2605.30554"},"observation_digest":"sha256:c37bf8549b42d6b5264865070ea9565b6d4f036e1d0984191c5450504f3cf521","observation_id":"fa4728b1-a92e-413d-b873-1b966a077a82","resolution":{"observed_at":"2026-06-29T00:09:37.360084Z","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":"2026-06-29T00:09:37.360084Z","title":"Tagami, T","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2605.30554","last_updated":"2026-05-28T20:36:30Z","snapshot_observed_at":"2026-08-15T18:36:46.400731Z","submitted_at":"2026-05-28T20:36:30Z","title":"Effects of the Symmetry energy slope on the exotic content of the neutron stars","version":1},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-06-29T00:09:37.360084Z"},"links":{"citing_paper":"/paper/2605.30554"},"observation_digest":"sha256:5e0bf28a595ef61330e3fac9e15b62ebc8419eddcaaba6fe71bb36162ec93183","observation_id":"5de09c09-5001-421b-98b5-7fb24bf49de8","resolution":{"observed_at":"2026-06-29T00:09:37.360084Z","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":"2026-06-29T00:09:37.360084Z","title":"Riley et al., A NICER View of the Mas- sive Pulsar PSR J0740+6620 Informed by Ra- dio Timing and XMM-Newton Spectroscopy, Astrophys","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2605.30554","last_updated":"2026-05-28T20:36:30Z","snapshot_observed_at":"2026-08-15T18:36:46.400731Z","submitted_at":"2026-05-28T20:36:30Z","title":"Effects of the Symmetry energy slope on the exotic content of the neutron stars","version":1},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-06-29T00:09:37.360084Z"},"links":{"citing_paper":"/paper/2605.30554"},"observation_digest":"sha256:d4682c2f56b4d5686de8ffd8804cfb2b9167e20d9f973caac72a209bedac00a7","observation_id":"750df80c-dd0e-4681-856a-01d86f3cfb37","resolution":{"observed_at":"2026-06-29T00:09:37.360084Z","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":"2026-06-29T00:09:37.360084Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2605.30554","last_updated":"2026-05-28T20:36:30Z","snapshot_observed_at":"2026-08-15T18:36:46.400731Z","submitted_at":"2026-05-28T20:36:30Z","title":"Effects of the Symmetry energy slope on the exotic content of the neutron stars","version":1},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-06-29T00:09:37.360084Z"},"links":{"citing_paper":"/paper/2605.30554"},"observation_digest":"sha256:2f6c3f3c78067d5bafb3dad96252f70e516095252cf8479394df4ce906eeb0f9","observation_id":"86ce1861-2fb9-4a85-9d93-ca1ee90ba23f","resolution":{"observed_at":"2026-06-29T00:09:37.360084Z","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":"2026-06-29T00:09:37.360084Z","title":"Miller et al., PSR J0030+0451 Mass and Radius from N ICER Data and Implications for the Properties of Neutron Star Matter, Astrophys","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2605.30554","last_updated":"2026-05-28T20:36:30Z","snapshot_observed_at":"2026-08-15T18:36:46.400731Z","submitted_at":"2026-05-28T20:36:30Z","title":"Effects of the Symmetry energy slope on the exotic content of the neutron stars","version":1},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-06-29T00:09:37.360084Z"},"links":{"citing_paper":"/paper/2605.30554"},"observation_digest":"sha256:19a0cd127e8381e68ca35b049c683c8929835f7f1405a26c1127fc339cc62e1d","observation_id":"399704b1-5efc-4426-b1b3-945da1639152","resolution":{"observed_at":"2026-06-29T00:09:37.360084Z","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":"2026-06-29T00:09:37.360084Z","title":"Miller et al., The Radius of PSR J0740+6620 from NICER and XMM-Newton Data, Astrophys","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2605.30554","last_updated":"2026-05-28T20:36:30Z","snapshot_observed_at":"2026-08-15T18:36:46.400731Z","submitted_at":"2026-05-28T20:36:30Z","title":"Effects of the Symmetry energy slope on the exotic content of the neutron stars","version":1},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-06-29T00:09:37.360084Z"},"links":{"citing_paper":"/paper/2605.30554"},"observation_digest":"sha256:647bd542e6b5987cd339b8cbc2e8e8fd3a067c625823471dc93be3ed04e82d4a","observation_id":"bfc027da-08e6-45db-9d32-6f082611f6aa","resolution":{"observed_at":"2026-06-29T00:09:37.360084Z","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":"2026-06-29T00:09:37.360084Z","title":"Annala, T","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2605.30554","last_updated":"2026-05-28T20:36:30Z","snapshot_observed_at":"2026-08-15T18:36:46.400731Z","submitted_at":"2026-05-28T20:36:30Z","title":"Effects of the Symmetry energy slope on the exotic content of the neutron stars","version":1},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-06-29T00:09:37.360084Z"},"links":{"citing_paper":"/paper/2605.30554"},"observation_digest":"sha256:85f42bd6a0da2a563b0a93c5475f30e3f7188cf2d159475ad269e666b937039a","observation_id":"023f002d-534c-488e-b493-844ab7a9d43f","resolution":{"observed_at":"2026-06-29T00:09:37.360084Z","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":"2026-06-29T00:09:37.360084Z","title":"Abbott et al., Gw170817: Observation of grav- itational waves from a binary neutron star inspiral, Phys","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2605.30554","last_updated":"2026-05-28T20:36:30Z","snapshot_observed_at":"2026-08-15T18:36:46.400731Z","submitted_at":"2026-05-28T20:36:30Z","title":"Effects of the Symmetry energy slope on the exotic content of the neutron stars","version":1},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-06-29T00:09:37.360084Z"},"links":{"citing_paper":"/paper/2605.30554"},"observation_digest":"sha256:c5fa152e4f08defa7c446cfb3913f12f341f912efd2986f3fe2e0f7bbeac6c1a","observation_id":"ded3b9ad-e715-4bb3-b020-2558dc1ae81d","resolution":{"observed_at":"2026-06-29T00:09:37.360084Z","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":"2026-06-29T00:09:37.360084Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2605.30554","last_updated":"2026-05-28T20:36:30Z","snapshot_observed_at":"2026-08-15T18:36:46.400731Z","submitted_at":"2026-05-28T20:36:30Z","title":"Effects of the Symmetry energy slope on the exotic content of the neutron stars","version":1},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-06-29T00:09:37.360084Z"},"links":{"citing_paper":"/paper/2605.30554"},"observation_digest":"sha256:9f7c63e737550dc6123a254879d9774023e1abd3b2aa706071264939a8c6016a","observation_id":"23a1d7b1-10f7-4d49-8754-67167caa7487","resolution":{"observed_at":"2026-06-29T00:09:37.360084Z","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":"2026-06-29T00:09:37.360084Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2605.30554","last_updated":"2026-05-28T20:36:30Z","snapshot_observed_at":"2026-08-15T18:36:46.400731Z","submitted_at":"2026-05-28T20:36:30Z","title":"Effects of the Symmetry energy slope on the exotic content of the neutron stars","version":1},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-06-29T00:09:37.360084Z"},"links":{"citing_paper":"/paper/2605.30554"},"observation_digest":"sha256:4f545cfaa7c705fffc8f4a3b3691f68bcaeba64ec98c11d3d13ef498e64a5a95","observation_id":"7725fdd5-4485-4469-a0ce-ded7fcbdbf1c","resolution":{"observed_at":"2026-06-29T00:09:37.360084Z","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":"2026-06-29T00:09:37.360084Z","title":"Fattoyev et al., Relativistic eﬀective interaction for nuclei, giant resonances, and neutron stars, Phys","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2605.30554","last_updated":"2026-05-28T20:36:30Z","snapshot_observed_at":"2026-08-15T18:36:46.400731Z","submitted_at":"2026-05-28T20:36:30Z","title":"Effects of the Symmetry energy slope on the exotic content of the neutron stars","version":1},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-06-29T00:09:37.360084Z"},"links":{"citing_paper":"/paper/2605.30554"},"observation_digest":"sha256:1e2ddca665a79b20dcd4748ed2b13c8a964bb4e4191a5e7a76adc7078889b797","observation_id":"ad3feaef-7588-4b75-b52c-60d66f5cd0f7","resolution":{"observed_at":"2026-06-29T00:09:37.360084Z","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":"2026-06-29T00:09:37.360084Z","title":"Cavagnoli, D","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2605.30554","last_updated":"2026-05-28T20:36:30Z","snapshot_observed_at":"2026-08-15T18:36:46.400731Z","submitted_at":"2026-05-28T20:36:30Z","title":"Effects of the Symmetry energy slope on the exotic content of the neutron stars","version":1},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-06-29T00:09:37.360084Z"},"links":{"citing_paper":"/paper/2605.30554"},"observation_digest":"sha256:c0aa5fc020e287f070ef9f4a13cba8519097d94057186d6eacb026fee1980d0e","observation_id":"afe825ed-6233-4a88-a0a0-81073a9df6b8","resolution":{"observed_at":"2026-06-29T00:09:37.360084Z","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":"2026-06-29T00:09:37.360084Z","title":"Dexheimer et al., What do we learn about vector inter- actions from gw170817?, J","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2605.30554","last_updated":"2026-05-28T20:36:30Z","snapshot_observed_at":"2026-08-15T18:36:46.400731Z","submitted_at":"2026-05-28T20:36:30Z","title":"Effects of the Symmetry energy slope on the exotic content of the neutron stars","version":1},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-06-29T00:09:37.360084Z"},"links":{"citing_paper":"/paper/2605.30554"},"observation_digest":"sha256:d536f8e5feab30743354a5846a9d36f06bf7d8b6d94249bbf989975f318f96fd","observation_id":"3de242df-03f9-451b-af73-3171ea012287","resolution":{"observed_at":"2026-06-29T00:09:37.360084Z","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":"2026-06-29T00:09:37.360084Z","title":"Kubis and M","venue":null,"work_id":null,"year":1997},"citing_paper":{"arxiv_id":"2605.30554","last_updated":"2026-05-28T20:36:30Z","snapshot_observed_at":"2026-08-15T18:36:46.400731Z","submitted_at":"2026-05-28T20:36:30Z","title":"Effects of the Symmetry energy slope on the exotic content of the neutron stars","version":1},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-06-29T00:09:37.360084Z"},"links":{"citing_paper":"/paper/2605.30554"},"observation_digest":"sha256:b4343cf9c9b76990bd244a562e1812d1aad52d8ffb5bd2b725fddc61308c0ee3","observation_id":"cd722c9d-bae7-4df8-8100-956ad8d8ab8b","resolution":{"observed_at":"2026-06-29T00:09:37.360084Z","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":"2026-06-29T00:09:37.360084Z","title":null,"venue":null,"work_id":null,"year":2002},"citing_paper":{"arxiv_id":"2605.30554","last_updated":"2026-05-28T20:36:30Z","snapshot_observed_at":"2026-08-15T18:36:46.400731Z","submitted_at":"2026-05-28T20:36:30Z","title":"Effects of the Symmetry energy slope on the exotic content of the neutron stars","version":1},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-06-29T00:09:37.360084Z"},"links":{"citing_paper":"/paper/2605.30554"},"observation_digest":"sha256:dc864f448092c8297fae4690634984bbfc5657498a54446ff6f99a072fc2d693","observation_id":"16122312-1ab2-4e7f-bb0f-a68d52f6e2c4","resolution":{"observed_at":"2026-06-29T00:09:37.360084Z","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":"2026-06-29T00:09:37.360084Z","title":"Lopes and D","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2605.30554","last_updated":"2026-05-28T20:36:30Z","snapshot_observed_at":"2026-08-15T18:36:46.400731Z","submitted_at":"2026-05-28T20:36:30Z","title":"Effects of the Symmetry energy slope on the exotic content of the neutron stars","version":1},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-06-29T00:09:37.360084Z"},"links":{"citing_paper":"/paper/2605.30554"},"observation_digest":"sha256:dfc4521870d88f6720f3ce587afeba09b22730b8beda3ead94258554b8074a68","observation_id":"3a3c5be2-5276-4de3-a3b0-cd77ecfaa275","resolution":{"observed_at":"2026-06-29T00:09:37.360084Z","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":"2026-06-29T00:09:37.360084Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2605.30554","last_updated":"2026-05-28T20:36:30Z","snapshot_observed_at":"2026-08-15T18:36:46.400731Z","submitted_at":"2026-05-28T20:36:30Z","title":"Effects of the Symmetry energy slope on the exotic content of the neutron stars","version":1},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-06-29T00:09:37.360084Z"},"links":{"citing_paper":"/paper/2605.30554"},"observation_digest":"sha256:29fcaaad7975912562f4b5baea30198ca0904edf44ebb25cc64daba62bd19b2c","observation_id":"15977b96-3d1c-4db3-925a-35ce77fa27aa","resolution":{"observed_at":"2026-06-29T00:09:37.360084Z","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":"2026-06-29T00:09:37.360084Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2605.30554","last_updated":"2026-05-28T20:36:30Z","snapshot_observed_at":"2026-08-15T18:36:46.400731Z","submitted_at":"2026-05-28T20:36:30Z","title":"Effects of the Symmetry energy slope on the exotic content of the neutron stars","version":1},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-06-29T00:09:37.360084Z"},"links":{"citing_paper":"/paper/2605.30554"},"observation_digest":"sha256:c18e30ebbd009c2efbc68059370120b693383f4f421cbbcfd1edcd620d9d2934","observation_id":"663122c1-b721-4550-8bf1-387727ef3df8","resolution":{"observed_at":"2026-06-29T00:09:37.360084Z","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":"2026-06-29T00:09:37.360084Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2605.30554","last_updated":"2026-05-28T20:36:30Z","snapshot_observed_at":"2026-08-15T18:36:46.400731Z","submitted_at":"2026-05-28T20:36:30Z","title":"Effects of the Symmetry energy slope on the exotic content of the neutron stars","version":1},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-06-29T00:09:37.360084Z"},"links":{"citing_paper":"/paper/2605.30554"},"observation_digest":"sha256:538885372c015797858b84369894974701c49b5d62124d6e1af5bb203e4a0d27","observation_id":"489940f1-efec-4769-9317-7ce186e13e56","resolution":{"observed_at":"2026-06-29T00:09:37.360084Z","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":"2026-06-29T00:09:37.360084Z","title":"Kl¨ ahn et al., Constraints on the high-density nuclear equation of state from the phenomenol- ogy of compact stars and heavy-ion collisions, Phys","venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"2605.30554","last_updated":"2026-05-28T20:36:30Z","snapshot_observed_at":"2026-08-15T18:36:46.400731Z","submitted_at":"2026-05-28T20:36:30Z","title":"Effects of the Symmetry energy slope on the exotic content of the neutron stars","version":1},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-06-29T00:09:37.360084Z"},"links":{"citing_paper":"/paper/2605.30554"},"observation_digest":"sha256:7d8aadaf7112e03b8434cb38dd1e489dcc5832b78c9abd126feafe12b48a69e8","observation_id":"7244d171-8b83-4ac4-b687-8cc43abfb36c","resolution":{"observed_at":"2026-06-29T00:09:37.360084Z","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":"2026-06-29T00:09:37.360084Z","title":null,"venue":null,"work_id":null,"year":1992},"citing_paper":{"arxiv_id":"2605.30554","last_updated":"2026-05-28T20:36:30Z","snapshot_observed_at":"2026-08-15T18:36:46.400731Z","submitted_at":"2026-05-28T20:36:30Z","title":"Effects of the Symmetry energy slope on the exotic content of the neutron stars","version":1},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-06-29T00:09:37.360084Z"},"links":{"citing_paper":"/paper/2605.30554"},"observation_digest":"sha256:c865fd8e4548bb7338fae21ef1da84230f7bc7e10f9114b721a063e16dc62c53","observation_id":"e9fc3957-fc85-4f2d-90c9-ec47e18f663b","resolution":{"observed_at":"2026-06-29T00:09:37.360084Z","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":"2026-06-29T00:09:37.360084Z","title":"Miyatsu, M.-K","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2605.30554","last_updated":"2026-05-28T20:36:30Z","snapshot_observed_at":"2026-08-15T18:36:46.400731Z","submitted_at":"2026-05-28T20:36:30Z","title":"Effects of the Symmetry energy slope on the exotic content of the neutron stars","version":1},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-06-29T00:09:37.360084Z"},"links":{"citing_paper":"/paper/2605.30554"},"observation_digest":"sha256:82859e916dc0959adfc0004f9538d0daf45310a38e3dc035218971ae524915ff","observation_id":"abfd6305-afc8-45d2-a39f-7a590da929a5","resolution":{"observed_at":"2026-06-29T00:09:37.360084Z","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":"2026-06-29T00:09:37.360084Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2605.30554","last_updated":"2026-05-28T20:36:30Z","snapshot_observed_at":"2026-08-15T18:36:46.400731Z","submitted_at":"2026-05-28T20:36:30Z","title":"Effects of the Symmetry energy slope on the exotic content of the neutron stars","version":1},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-06-29T00:09:37.360084Z"},"links":{"citing_paper":"/paper/2605.30554"},"observation_digest":"sha256:a6232349910a08e5fbca781607cfd1055938815d7bb266a43b0e5e067dc2f275","observation_id":"695ca39f-36c4-42b6-9022-0dd8c3534543","resolution":{"observed_at":"2026-06-29T00:09:37.360084Z","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":"2026-06-29T00:09:37.360084Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2605.30554","last_updated":"2026-05-28T20:36:30Z","snapshot_observed_at":"2026-08-15T18:36:46.400731Z","submitted_at":"2026-05-28T20:36:30Z","title":"Effects of the Symmetry energy slope on the exotic content of the neutron stars","version":1},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-06-29T00:09:37.360084Z"},"links":{"citing_paper":"/paper/2605.30554"},"observation_digest":"sha256:58d326081e08aa4d4481bcada6676d8acfcf7b015ec05d7a49c5c68a1635ef55","observation_id":"573dfa5a-279d-43a3-b17a-4bb6a88e6b89","resolution":{"observed_at":"2026-06-29T00:09:37.360084Z","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":"2026-06-29T00:09:37.360084Z","title":"Boguta and A","venue":null,"work_id":null,"year":1977},"citing_paper":{"arxiv_id":"2605.30554","last_updated":"2026-05-28T20:36:30Z","snapshot_observed_at":"2026-08-15T18:36:46.400731Z","submitted_at":"2026-05-28T20:36:30Z","title":"Effects of the Symmetry energy slope on the exotic content of the neutron stars","version":1},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-06-29T00:09:37.360084Z"},"links":{"citing_paper":"/paper/2605.30554"},"observation_digest":"sha256:ae3ffcf6ce216994b5fe06004c7e73cfd27b57f0f7e10ab85aad5299252eb7bd","observation_id":"eebaa69d-ee8e-4515-b3b1-ff56242bc2bf","resolution":{"observed_at":"2026-06-29T00:09:37.360084Z","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":"2026-06-29T00:09:37.360084Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2605.30554","last_updated":"2026-05-28T20:36:30Z","snapshot_observed_at":"2026-08-15T18:36:46.400731Z","submitted_at":"2026-05-28T20:36:30Z","title":"Effects of the Symmetry energy slope on the exotic content of the neutron stars","version":1},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-06-29T00:09:37.360084Z"},"links":{"citing_paper":"/paper/2605.30554"},"observation_digest":"sha256:88b8a74f663c92f5995ee9675281867674a3aef191062581c6a2d7dd854b7aed","observation_id":"5b4ac16b-a96b-4f4f-9443-bb4af405f438","resolution":{"observed_at":"2026-06-29T00:09:37.360084Z","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":"2026-06-29T00:09:37.360084Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2605.30554","last_updated":"2026-05-28T20:36:30Z","snapshot_observed_at":"2026-08-15T18:36:46.400731Z","submitted_at":"2026-05-28T20:36:30Z","title":"Effects of the Symmetry energy slope on the exotic content of the neutron stars","version":1},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-06-29T00:09:37.360084Z"},"links":{"citing_paper":"/paper/2605.30554"},"observation_digest":"sha256:8115133b713176161ff79a28e50988a9eb575f88b47544310893e852d07000ba","observation_id":"e2a14d96-24a6-4b4f-b8d5-acf738712a8a","resolution":{"observed_at":"2026-06-29T00:09:37.360084Z","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":"2026-06-29T00:09:37.360084Z","title":"Schaﬀner-Bielich and A","venue":null,"work_id":null,"year":2000},"citing_paper":{"arxiv_id":"2605.30554","last_updated":"2026-05-28T20:36:30Z","snapshot_observed_at":"2026-08-15T18:36:46.400731Z","submitted_at":"2026-05-28T20:36:30Z","title":"Effects of the Symmetry energy slope on the exotic content of the neutron stars","version":1},"reference_index":54,"source":"pdf_text","source_observed_at":"2026-06-29T00:09:37.360084Z"},"links":{"citing_paper":"/paper/2605.30554"},"observation_digest":"sha256:166ce78ceefae6476e2a0f21e8efaf17ff41456f578fd19ba1f0f4f15d26be8a","observation_id":"d86fecbc-5b7a-40a7-a91e-2fe6eaeed8bc","resolution":{"observed_at":"2026-06-29T00:09:37.360084Z","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":"2026-06-29T00:09:37.360084Z","title":"Inoue, Hyperon forces from qcd and their applications, JPS Conf","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2605.30554","last_updated":"2026-05-28T20:36:30Z","snapshot_observed_at":"2026-08-15T18:36:46.400731Z","submitted_at":"2026-05-28T20:36:30Z","title":"Effects of the Symmetry energy slope on the exotic content of the neutron stars","version":1},"reference_index":55,"source":"pdf_text","source_observed_at":"2026-06-29T00:09:37.360084Z"},"links":{"citing_paper":"/paper/2605.30554"},"observation_digest":"sha256:9b76ac3a554ecdf5162ae39b50bb8975154c45404f42abf6899cc79b4d62d069","observation_id":"a115a36f-4b3e-4d27-8834-dfb481635434","resolution":{"observed_at":"2026-06-29T00:09:37.360084Z","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":"2026-06-29T00:09:37.360084Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2605.30554","last_updated":"2026-05-28T20:36:30Z","snapshot_observed_at":"2026-08-15T18:36:46.400731Z","submitted_at":"2026-05-28T20:36:30Z","title":"Effects of the Symmetry energy slope on the exotic content of the neutron stars","version":1},"reference_index":56,"source":"pdf_text","source_observed_at":"2026-06-29T00:09:37.360084Z"},"links":{"citing_paper":"/paper/2605.30554"},"observation_digest":"sha256:e71f5f769acd4c28e55ec2bc4a31b48f69b1f671333610a5d445a88b49fc6809","observation_id":"f4ff76fb-a542-4653-b840-99cc8300f1f4","resolution":{"observed_at":"2026-06-29T00:09:37.360084Z","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":"2026-06-29T00:09:37.360084Z","title":"271, 03002 (2022)","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2605.30554","last_updated":"2026-05-28T20:36:30Z","snapshot_observed_at":"2026-08-15T18:36:46.400731Z","submitted_at":"2026-05-28T20:36:30Z","title":"Effects of the Symmetry energy slope on the exotic content of the neutron stars","version":1},"reference_index":57,"source":"pdf_text","source_observed_at":"2026-06-29T00:09:37.360084Z"},"links":{"citing_paper":"/paper/2605.30554"},"observation_digest":"sha256:7610101be3af098fed69c5a4cc46b8690896e56d1799dbb08c7754d8fae9fd46","observation_id":"99ad2930-aead-4cc4-b056-d65c7646e463","resolution":{"observed_at":"2026-06-29T00:09:37.360084Z","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":"2026-06-29T00:09:37.360084Z","title":"Friedman and A","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2605.30554","last_updated":"2026-05-28T20:36:30Z","snapshot_observed_at":"2026-08-15T18:36:46.400731Z","submitted_at":"2026-05-28T20:36:30Z","title":"Effects of the Symmetry energy slope on the exotic content of the neutron stars","version":1},"reference_index":58,"source":"pdf_text","source_observed_at":"2026-06-29T00:09:37.360084Z"},"links":{"citing_paper":"/paper/2605.30554"},"observation_digest":"sha256:0a657b0ff46fe29b5ebf74cf4e9126cdd9ba1c5dc7cccd458ec63f763a4c57b1","observation_id":"0326e96f-cf0a-40c4-9195-ddef7d3099c7","resolution":{"observed_at":"2026-06-29T00:09:37.360084Z","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":"2026-06-29T00:09:37.360084Z","title":null,"venue":null,"work_id":null,"year":1939},"citing_paper":{"arxiv_id":"2605.30554","last_updated":"2026-05-28T20:36:30Z","snapshot_observed_at":"2026-08-15T18:36:46.400731Z","submitted_at":"2026-05-28T20:36:30Z","title":"Effects of the Symmetry energy slope on the exotic content of the neutron stars","version":1},"reference_index":59,"source":"pdf_text","source_observed_at":"2026-06-29T00:09:37.360084Z"},"links":{"citing_paper":"/paper/2605.30554"},"observation_digest":"sha256:bcea4b1e0236fa8b63f372b5e04d90a0a5523a1d5fb12cda48786e6962d96ae0","observation_id":"36ca02af-0d78-44ff-924a-76ae6fdb0740","resolution":{"observed_at":"2026-06-29T00:09:37.360084Z","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":"2026-06-29T00:09:37.360084Z","title":null,"venue":null,"work_id":null,"year":1971},"citing_paper":{"arxiv_id":"2605.30554","last_updated":"2026-05-28T20:36:30Z","snapshot_observed_at":"2026-08-15T18:36:46.400731Z","submitted_at":"2026-05-28T20:36:30Z","title":"Effects of the Symmetry energy slope on the exotic content of the neutron stars","version":1},"reference_index":60,"source":"pdf_text","source_observed_at":"2026-06-29T00:09:37.360084Z"},"links":{"citing_paper":"/paper/2605.30554"},"observation_digest":"sha256:f2aca92369c17211c8cb03775f53a8074fb2b99d1919c3cf05a5e3e02b60e292","observation_id":"23b33f98-5230-4656-a533-3ff72d62dbdc","resolution":{"observed_at":"2026-06-29T00:09:37.360084Z","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":"2026-06-29T00:09:37.360084Z","title":null,"venue":null,"work_id":null,"year":1971},"citing_paper":{"arxiv_id":"2605.30554","last_updated":"2026-05-28T20:36:30Z","snapshot_observed_at":"2026-08-15T18:36:46.400731Z","submitted_at":"2026-05-28T20:36:30Z","title":"Effects of the Symmetry energy slope on the exotic content of the neutron stars","version":1},"reference_index":61,"source":"pdf_text","source_observed_at":"2026-06-29T00:09:37.360084Z"},"links":{"citing_paper":"/paper/2605.30554"},"observation_digest":"sha256:fa69ab708af4bf9ef44215feb45e389ca966c2563e64aab0d52df4e334e87611","observation_id":"3ece1d8e-4b2f-4283-bd6a-ba4b133acda4","resolution":{"observed_at":"2026-06-29T00:09:37.360084Z","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":"2026-06-29T00:09:37.360084Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2605.30554","last_updated":"2026-05-28T20:36:30Z","snapshot_observed_at":"2026-08-15T18:36:46.400731Z","submitted_at":"2026-05-28T20:36:30Z","title":"Effects of the Symmetry energy slope on the exotic content of the neutron stars","version":1},"reference_index":62,"source":"pdf_text","source_observed_at":"2026-06-29T00:09:37.360084Z"},"links":{"citing_paper":"/paper/2605.30554"},"observation_digest":"sha256:d4064334dfd5710ff07dc34f01d8d3c7731dfd397e540ee84034a219159ca148","observation_id":"d11f03c7-7635-4aa1-bacd-cb093c100b3c","resolution":{"observed_at":"2026-06-29T00:09:37.360084Z","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":"2026-06-29T00:09:37.360084Z","title":"Mauviard et al., A nicer view of the 1.4 m0 edge-on pulsar psr j0614-3329, Astrophys","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2605.30554","last_updated":"2026-05-28T20:36:30Z","snapshot_observed_at":"2026-08-15T18:36:46.400731Z","submitted_at":"2026-05-28T20:36:30Z","title":"Effects of the Symmetry energy slope on the exotic content of the neutron stars","version":1},"reference_index":63,"source":"pdf_text","source_observed_at":"2026-06-29T00:09:37.360084Z"},"links":{"citing_paper":"/paper/2605.30554"},"observation_digest":"sha256:b2bad6e6c88ce729874a5b433d7fa9ba2d4ffe31660f070e60d3a6b0696f6a2f","observation_id":"b811a6c5-001e-41fb-917f-3b625537585d","resolution":{"observed_at":"2026-06-29T00:09:37.360084Z","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":"2026-06-29T00:09:37.360084Z","title":"Choudhury et al., A nicer view of the near- est and brightest millisecond pulsar: Psr j0437-4715, Astrophys","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2605.30554","last_updated":"2026-05-28T20:36:30Z","snapshot_observed_at":"2026-08-15T18:36:46.400731Z","submitted_at":"2026-05-28T20:36:30Z","title":"Effects of the Symmetry energy slope on the exotic content of the neutron stars","version":1},"reference_index":64,"source":"pdf_text","source_observed_at":"2026-06-29T00:09:37.360084Z"},"links":{"citing_paper":"/paper/2605.30554"},"observation_digest":"sha256:17054774a2bd17ee9962d1b83f37768e3f025ac548029a73d2d7522b6cea1e4e","observation_id":"91549534-2aa6-49dd-8fe4-583458c45449","resolution":{"observed_at":"2026-06-29T00:09:37.360084Z","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":"2026-06-29T00:09:37.360084Z","title":"Hinderer, Tidal love numbers of neutron stars, Astrophys","venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2605.30554","last_updated":"2026-05-28T20:36:30Z","snapshot_observed_at":"2026-08-15T18:36:46.400731Z","submitted_at":"2026-05-28T20:36:30Z","title":"Effects of the Symmetry energy slope on the exotic content of the neutron stars","version":1},"reference_index":65,"source":"pdf_text","source_observed_at":"2026-06-29T00:09:37.360084Z"},"links":{"citing_paper":"/paper/2605.30554"},"observation_digest":"sha256:f0d6ddafb14437939256d61302d7a5eeb8d71af2850d7ca5e76c7032eae7df01","observation_id":"ec8d8cec-6bcd-4cd0-8fec-23814217a482","resolution":{"observed_at":"2026-06-29T00:09:37.360084Z","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":"2026-06-29T00:09:37.360084Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2605.30554","last_updated":"2026-05-28T20:36:30Z","snapshot_observed_at":"2026-08-15T18:36:46.400731Z","submitted_at":"2026-05-28T20:36:30Z","title":"Effects of the Symmetry energy slope on the exotic content of the neutron stars","version":1},"reference_index":66,"source":"pdf_text","source_observed_at":"2026-06-29T00:09:37.360084Z"},"links":{"citing_paper":"/paper/2605.30554"},"observation_digest":"sha256:c4ba0c481f5c711527653106d73087ea0e706401983de85500de9d20bc1bd653","observation_id":"cbd47724-2229-448c-90c9-265597e07467","resolution":{"observed_at":"2026-06-29T00:09:37.360084Z","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":"2026-06-29T00:09:37.360084Z","title":"Tang, Y.-J","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2605.30554","last_updated":"2026-05-28T20:36:30Z","snapshot_observed_at":"2026-08-15T18:36:46.400731Z","submitted_at":"2026-05-28T20:36:30Z","title":"Effects of the Symmetry energy slope on the exotic content of the neutron stars","version":1},"reference_index":67,"source":"pdf_text","source_observed_at":"2026-06-29T00:09:37.360084Z"},"links":{"citing_paper":"/paper/2605.30554"},"observation_digest":"sha256:9f140dff6c0e43079788d8123b866c12335f99f4aa773f6b0f7cb42ecb2d2659","observation_id":"85e988c5-d1fb-44da-a3c7-f67582ce82b7","resolution":{"observed_at":"2026-06-29T00:09:37.360084Z","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":"2026-06-29T00:09:37.360084Z","title":"Ferreira and C","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2605.30554","last_updated":"2026-05-28T20:36:30Z","snapshot_observed_at":"2026-08-15T18:36:46.400731Z","submitted_at":"2026-05-28T20:36:30Z","title":"Effects of the Symmetry energy slope on the exotic content of the neutron stars","version":1},"reference_index":68,"source":"pdf_text","source_observed_at":"2026-06-29T00:09:37.360084Z"},"links":{"citing_paper":"/paper/2605.30554"},"observation_digest":"sha256:292fa5ccdc9f269226e24e7b258c9237e8accffd8283b7e828075326359631ca","observation_id":"0d594790-bddb-47c8-99c7-099553882534","resolution":{"observed_at":"2026-06-29T00:09:37.360084Z","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":"2026-06-29T00:09:37.360084Z","title":"Bauswein, A","venue":null,"work_id":null,"year":2026},"citing_paper":{"arxiv_id":"2605.30554","last_updated":"2026-05-28T20:36:30Z","snapshot_observed_at":"2026-08-15T18:36:46.400731Z","submitted_at":"2026-05-28T20:36:30Z","title":"Effects of the Symmetry energy slope on the exotic content of the neutron stars","version":1},"reference_index":69,"source":"pdf_text","source_observed_at":"2026-06-29T00:09:37.360084Z"},"links":{"citing_paper":"/paper/2605.30554"},"observation_digest":"sha256:2461dbc1c41fa623a8411c56f033fca24572da63a55130c3860b283c10d08b99","observation_id":"83b5e557-406c-4bb3-af17-85bbb8741e36","resolution":{"observed_at":"2026-06-29T00:09:37.360084Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"2605.30554","last_updated":"2026-05-28T20:36:30Z","latest_version":1,"primary_category":"nucl-th","snapshot_observed_at":"2026-08-15T18:36:46.400731Z","submitted_at":"2026-05-28T20:36:30Z","title":"Effects of the Symmetry energy slope on the exotic content of the neutron stars"},"reference_resolution":{"displayed":69,"state_counts":{"malformed_identifier":1,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":68,"verified_exact":0,"verified_fuzzy":0},"total_outbound_references":69},"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":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"thesis":"As of 16 August 2026, this Paper Citation Record lists 69 of 69 outbound references and 1 inbound Pith citation observation for arXiv:2605.30554."}