{"as_of":"2026-08-08T02:29:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:29e615db8929176632c24744e1ceb34ece33b24b6875ba18ee583ae7c70cc1c6","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":10,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":10,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-07T06:34:17.273281+00:00","state":"measured"},{"denominator":10,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":10,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-07T12:24:05.615902Z","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":"2026-07-02T10:26:51.893441Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2011.01318","last_updated":"2020-11-02T21:03:39Z","snapshot_observed_at":"2026-08-07T16:52:09.891742Z","submitted_at":"2020-11-02T21:03:39Z","title":"Dark matter admixed neutron star properties in the light of gravitational wave observations: a two fluid approach","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2011.01318","snapshot_observed_at":"2026-08-06T16:35:42.095874Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2507.13227","last_updated":"2025-08-21T13:29:55Z","snapshot_observed_at":"2026-08-07T09:51:34.957047Z","submitted_at":"2025-07-17T15:39:44Z","title":"Effect of Dark matter and $\\sigma$-cut potential on radial and non-radial oscillation modes in neutron stars","version":2},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-08-06T16:35:42.095874Z"},"links":{"cited_paper":"/paper/2011.01318","citing_paper":"/paper/2507.13227"},"observation_digest":"sha256:f26d48984fcf2551ed864f68ef32e5e1a41c6b7af2ba46d1f8a8ffcb403bceca","observation_id":"a7a45fef-4a51-4afb-bd8f-dd8adef6e672","resolution":{"observed_at":"2026-08-06T16:35:42.095874Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2011.01318","last_updated":"2020-11-02T21:03:39Z","snapshot_observed_at":"2026-08-07T16:52:09.891742Z","submitted_at":"2020-11-02T21:03:39Z","title":"Dark matter admixed neutron star properties in the light of gravitational wave observations: a two fluid approach","version":1},"cited_work":{"arxiv_id":"2011.01318","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2011.01318","snapshot_observed_at":"2026-07-02T10:26:51.893441Z","title":"Dark matter admixed neutron star properties in light of gravitational wave observations: A two fluid approach,","venue":null,"work_id":"2378f319-ed07-4c79-a56b-6733cc128ca2","year":2022},"citing_paper":{"arxiv_id":"2511.07567","last_updated":"2026-04-14T18:19:15Z","snapshot_observed_at":"2026-07-06T22:35:27.050353Z","submitted_at":"2025-11-10T19:22:59Z","title":"Dark Matter Heating in Evolving Proto-Neutron Stars: A Two-Fluid Approach","version":2},"reference_index":69,"source":"pdf_text","source_observed_at":"2026-05-17T23:10:30.793407Z"},"links":{"cited_paper":"/paper/2011.01318","citing_paper":"/paper/2511.07567"},"observation_digest":"sha256:9687988ad2f226f8f6c11863855b8c363215633ac7fe28cb8cb8e4faa1c1f9dd","observation_id":"d9c9a093-4b1f-4414-afe3-91a363b27341","resolution":{"observed_at":"2026-05-17T23:12:12.091216Z","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":"2011.01318","last_updated":"2020-11-02T21:03:39Z","snapshot_observed_at":"2026-08-07T16:52:09.891742Z","submitted_at":"2020-11-02T21:03:39Z","title":"Dark matter admixed neutron star properties in the light of gravitational wave observations: a two fluid approach","version":1},"cited_work":{"arxiv_id":"2011.01318","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2011.01318","snapshot_observed_at":"2026-07-02T10:26:51.893441Z","title":"Dark matter admixed neutron star properties in light of gravitational wave observations: A two fluid approach,","venue":null,"work_id":"2378f319-ed07-4c79-a56b-6733cc128ca2","year":2022},"citing_paper":{"arxiv_id":"2604.04560","last_updated":"2026-07-11T01:33:13Z","snapshot_observed_at":"2026-07-16T23:17:50.080024Z","submitted_at":"2026-04-06T09:40:02Z","title":"Neutron star with dark matter using vector portal","version":1},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-05-10T19:33:30.024439Z"},"links":{"cited_paper":"/paper/2011.01318","citing_paper":"/paper/2604.04560"},"observation_digest":"sha256:ca72c8c2b35b07c68e62021ab824d5160725bb01fa99fb5c394c6b61bc595089","observation_id":"8c348f86-894f-4752-8c0c-0490913974a5","resolution":{"observed_at":"2026-05-10T22:50:48.154486Z","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":"2011.01318","last_updated":"2020-11-02T21:03:39Z","snapshot_observed_at":"2026-08-07T16:52:09.891742Z","submitted_at":"2020-11-02T21:03:39Z","title":"Dark matter admixed neutron star properties in the light of gravitational wave observations: a two fluid approach","version":1},"cited_work":{"arxiv_id":"2011.01318","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2011.01318","snapshot_observed_at":"2026-07-02T10:26:51.893441Z","title":"Dark matter admixed neutron star properties in light of gravitational wave observations: A two fluid approach,","venue":null,"work_id":"2378f319-ed07-4c79-a56b-6733cc128ca2","year":2022},"citing_paper":{"arxiv_id":"2605.10467","last_updated":"2026-05-11T12:33:25Z","snapshot_observed_at":"2026-07-06T23:22:28.318343Z","submitted_at":"2026-05-11T12:33:25Z","title":"Axial Quasi-normal Modes of Admixed Neutron Stars","version":1},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-05-12T04:37:29.457932Z"},"links":{"cited_paper":"/paper/2011.01318","citing_paper":"/paper/2605.10467"},"observation_digest":"sha256:3e650b8c18a13a664d00aacd42128033bdc77984da11558142da1042a7569c2f","observation_id":"e07739ac-1826-4921-8c50-aa3889e793bc","resolution":{"observed_at":"2026-05-12T06:06:24.892695Z","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":"2011.01318","last_updated":"2020-11-02T21:03:39Z","snapshot_observed_at":"2026-08-07T16:52:09.891742Z","submitted_at":"2020-11-02T21:03:39Z","title":"Dark matter admixed neutron star properties in the light of gravitational wave observations: a two fluid approach","version":1},"cited_work":{"arxiv_id":"2011.01318","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2011.01318","snapshot_observed_at":"2026-07-02T10:26:51.893441Z","title":"Dark matter admixed neutron star properties in light of gravitational wave observations: A two fluid approach,","venue":null,"work_id":"2378f319-ed07-4c79-a56b-6733cc128ca2","year":2022},"citing_paper":{"arxiv_id":"2606.05082","last_updated":"2026-06-03T16:39:40Z","snapshot_observed_at":"2026-08-05T23:50:48.694506Z","submitted_at":"2026-06-03T16:39:40Z","title":"First Constraints on the Ellipticities of Self-Interacting Fermionic Dark Matter Admixed Neutron Stars from Continuous Gravitational-Wave Searches","version":1},"reference_index":63,"source":"pdf_text","source_observed_at":"2026-06-28T05:03:42.639549Z"},"links":{"cited_paper":"/paper/2011.01318","citing_paper":"/paper/2606.05082"},"observation_digest":"sha256:f0eaac8624b7427b5f0403eaa598d4444d7797dea0d508584fdff1408b58525b","observation_id":"2c225b22-4b63-4e01-a702-813e2d276699","resolution":{"observed_at":"2026-07-02T10:26:51.894916Z","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":"2011.01318","last_updated":"2020-11-02T21:03:39Z","snapshot_observed_at":"2026-08-07T16:52:09.891742Z","submitted_at":"2020-11-02T21:03:39Z","title":"Dark matter admixed neutron star properties in the light of gravitational wave observations: a two fluid approach","version":1},"cited_work":{"arxiv_id":"2011.01318","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2011.01318","snapshot_observed_at":"2026-07-02T10:26:51.893441Z","title":"Dark matter admixed neutron star properties in light of gravitational wave observations: A two fluid approach,","venue":null,"work_id":"2378f319-ed07-4c79-a56b-6733cc128ca2","year":2022},"citing_paper":{"arxiv_id":"2606.27456","last_updated":"2026-06-25T18:27:56Z","snapshot_observed_at":"2026-07-07T00:01:39.205208Z","submitted_at":"2026-06-25T18:27:56Z","title":"The crust of dark-matter admixed neutron stars: bulk properties and torsional oscillations","version":1},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-06-29T01:38:22.585392Z"},"links":{"cited_paper":"/paper/2011.01318","citing_paper":"/paper/2606.27456"},"observation_digest":"sha256:99813fa20c959f182ce02d63b7d60d42450615457577c9b17b59fbdb6029aa4b","observation_id":"5ec95770-1701-4597-afc2-663ecdcda518","resolution":{"observed_at":"2026-07-01T18:45:59.139942Z","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":"2011.01318","last_updated":"2020-11-02T21:03:39Z","snapshot_observed_at":"2026-08-07T16:52:09.891742Z","submitted_at":"2020-11-02T21:03:39Z","title":"Dark matter admixed neutron star properties in the light of gravitational wave observations: a two fluid approach","version":1},"cited_work":{"arxiv_id":"2011.01318","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2011.01318","snapshot_observed_at":"2026-07-02T10:26:51.893441Z","title":"Dark matter admixed neutron star properties in light of gravitational wave observations: A two fluid approach,","venue":null,"work_id":"2378f319-ed07-4c79-a56b-6733cc128ca2","year":2022},"citing_paper":{"arxiv_id":"2607.00888","last_updated":"2026-07-01T12:54:11Z","snapshot_observed_at":"2026-08-02T11:37:51.086281Z","submitted_at":"2026-07-01T12:54:11Z","title":"A self-consistent single-fluid framework for neutron stars admixed with mirror dark matter","version":1},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-07-02T08:36:45.802728Z"},"links":{"cited_paper":"/paper/2011.01318","citing_paper":"/paper/2607.00888"},"observation_digest":"sha256:e5bb017b3a1bd03de3825a75f6e5c7be04d79c8f3eceaa809a2f8a8f6699f181","observation_id":"ac3634b5-3e68-440c-b093-7fe88878f2c3","resolution":{"observed_at":"2026-07-02T08:46:48.789772Z","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":"2011.01318","last_updated":"2020-11-02T21:03:39Z","snapshot_observed_at":"2026-08-07T16:52:09.891742Z","submitted_at":"2020-11-02T21:03:39Z","title":"Dark matter admixed neutron star properties in the light of gravitational wave observations: a two fluid approach","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2011.01318","snapshot_observed_at":"2026-07-11T14:13:15.858928Z","title":null,"venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2607.04744","last_updated":"2026-07-06T07:31:20Z","snapshot_observed_at":"2026-08-05T16:40:20.918198Z","submitted_at":"2026-07-06T07:31:20Z","title":"Rotating Fermion-Boson Stars in $R$-squared Gravity","version":1},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-07-11T14:13:15.858928Z"},"links":{"cited_paper":"/paper/2011.01318","citing_paper":"/paper/2607.04744"},"observation_digest":"sha256:48be16305fe67273cc320ec1d71651fee9f834db8a119680961d35ec876ad141","observation_id":"8bf2412e-4f39-4665-bb88-6b7889774dbf","resolution":{"observed_at":"2026-07-11T14:13:15.858928Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2011.01318","last_updated":"2020-11-02T21:03:39Z","snapshot_observed_at":"2026-08-07T16:52:09.891742Z","submitted_at":"2020-11-02T21:03:39Z","title":"Dark matter admixed neutron star properties in the light of gravitational wave observations: a two fluid approach","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2011.01318","snapshot_observed_at":"2026-07-13T05:17:12.889672Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2607.09119","last_updated":"2026-07-10T06:16:49Z","snapshot_observed_at":"2026-08-08T02:18:59.676855Z","submitted_at":"2026-07-10T06:16:49Z","title":"Effects of dark matter and magnetic field on neutron star properties in relativistic mean-field theory: A single-fluid approach","version":1},"reference_index":69,"source":"pdf_text","source_observed_at":"2026-07-13T05:17:12.889672Z"},"links":{"cited_paper":"/paper/2011.01318","citing_paper":"/paper/2607.09119"},"observation_digest":"sha256:8dd0b3b5b998cd8790f6b4b04ee049211daabb655b4988caaee7097bc4b85cf8","observation_id":"a4518545-3ed5-4f41-8df6-fb17826b1379","resolution":{"observed_at":"2026-07-13T05:17:12.889672Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2011.01318","last_updated":"2020-11-02T21:03:39Z","snapshot_observed_at":"2026-08-07T16:52:09.891742Z","submitted_at":"2020-11-02T21:03:39Z","title":"Dark matter admixed neutron star properties in the light of gravitational wave observations: a two fluid approach","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2011.01318","snapshot_observed_at":"2026-08-07T12:24:05.615902Z","title":"Dark matter ad- mixed neutron star properties in light of gravitational wave observations: A two fluid approach,","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2608.06224","last_updated":"2026-08-06T16:13:49Z","snapshot_observed_at":"2026-08-08T02:17:43.887635Z","submitted_at":"2026-08-06T16:13:49Z","title":"A Neutron Star Hidden Inside a Black Hole","version":1},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-07T12:24:05.615902Z"},"links":{"cited_paper":"/paper/2011.01318","citing_paper":"/paper/2608.06224"},"observation_digest":"sha256:58a3fddf8266c042d1317c6d9f78d9bda550786c01adf5ce6bdf4c51dfa4c5c3","observation_id":"13f00c2e-9b5f-40c6-a632-8ea40ed4b169","resolution":{"observed_at":"2026-08-07T12:24:05.615902Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2011.01318/citation-record","integrity":"/paper/2011.01318/integrity","json":"/paper/2011.01318/citation-record.json","paper":"/paper/2011.01318"},"outbound":[],"paper":{"arxiv_id":"2011.01318","last_updated":"2020-11-02T21:03:39Z","latest_version":1,"primary_category":"nucl-th","snapshot_observed_at":"2026-08-07T16:52:09.891742Z","submitted_at":"2020-11-02T21:03:39Z","title":"Dark matter admixed neutron star properties in the light of gravitational wave observations: a two fluid approach"},"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 10 inbound Pith citation observations for arXiv:2011.01318."}