{"as_of":"2026-08-17T21:32:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:3c46e62f27ec5f139452e2aac777018104e79768f2c542b4a9f7adec639177d0","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":12,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":12,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-17T06:30:58.91139+00:00","state":"measured"},{"denominator":12,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":12,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-16T05:25:17.566316Z","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":"2026-08-17T20:01:22.243481Z","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":"2026-08-11T05:14:02.716003Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2412.17946","last_updated":"2025-03-06T17:03:55Z","snapshot_observed_at":"2026-08-17T12:53:33.780776Z","submitted_at":"2024-12-23T19:57:10Z","title":"Supernova Remnants with Mirror Dark Matter and Hyperons","version":2},"reference_index":89,"source":"pdf_text","source_observed_at":"2026-08-11T05:14:02.716003Z"},"links":{"cited_paper":"/paper/2011.01318","citing_paper":"/paper/2412.17946"},"observation_digest":"sha256:329ae154af26f0f2f477a62e778072a4cdf8e5913a7506411d550d6df7839b2c","observation_id":"d5badac3-3931-4d3c-b9b8-09945317cc83","resolution":{"observed_at":"2026-08-11T05:14:02.716003Z","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":"2026-08-17T20:01:22.243481Z","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":"2026-08-16T05:25:17.566316Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2504.20825","last_updated":"2025-09-07T19:39:37Z","snapshot_observed_at":"2026-08-16T17:27:28.635325Z","submitted_at":"2025-04-29T14:46:04Z","title":"Numerical Relativity Simulations of Dark Matter Admixed Binary Neutron Stars","version":2},"reference_index":98,"source":"pdf_text","source_observed_at":"2026-08-16T05:25:17.566316Z"},"links":{"cited_paper":"/paper/2011.01318","citing_paper":"/paper/2504.20825"},"observation_digest":"sha256:d0f26fd683615d58cc314520838c94a9e61abb93089b3c1c6937e70a14b565d9","observation_id":"5f951c0a-4003-4a3a-9d7e-8d1addb508c0","resolution":{"observed_at":"2026-08-16T05:25:17.566316Z","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":"2026-08-17T20:01:22.243481Z","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":"2026-08-10T22:01:48.115042Z","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:e5fccdaf31085a1ca15f8ee9e1d7caa8f385e49dd5db0e82481afecffbda6147","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":"2026-08-17T20:01:22.243481Z","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":"2026-08-11T06:28:42.870500Z","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":"sha256:23fd99292adf91c07bf62ae010471a9dc3844a11b104f9dfbaafada561d6b6bb","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 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2011.01318","last_updated":"2020-11-02T21:03:39Z","snapshot_observed_at":"2026-08-17T20:01:22.243481Z","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":"sha256:242d34d8fefc59f7e8746bbdccc23e4ae738c731f6d6858bea63b14f56253d83","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 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2011.01318","last_updated":"2020-11-02T21:03:39Z","snapshot_observed_at":"2026-08-17T20:01:22.243481Z","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":"2026-08-16T22:40:52.127900Z","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:ade383d0ae2126efe984d6c92bcb587767c287faedd17c73dfa31167a6b56e95","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 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2011.01318","last_updated":"2020-11-02T21:03:39Z","snapshot_observed_at":"2026-08-17T20:01:22.243481Z","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":"2026-08-12T17:55:34.651355Z","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":"sha256:900d333aa1248892ad5a6bfb0d9b9e93a287891eb65780a4d7faf9a78c017ada","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 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2011.01318","last_updated":"2020-11-02T21:03:39Z","snapshot_observed_at":"2026-08-17T20:01:22.243481Z","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":"2026-08-14T04:28:30.350261Z","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":"sha256:12792ef00c4f28fcd62ebc37d66e31e47d35646bd9f4cdc0ce256756e4ba0c96","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 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2011.01318","last_updated":"2020-11-02T21:03:39Z","snapshot_observed_at":"2026-08-17T20:01:22.243481Z","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":"sha256:1b397e6e474f8e29e9435e747753b218f71796dfcb735850f29ad86a1dfe6587","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 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2011.01318","last_updated":"2020-11-02T21:03:39Z","snapshot_observed_at":"2026-08-17T20:01:22.243481Z","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":"2026-08-14T16:03:27.568683Z","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":"sha256:1cc0fc590767ff490ed6133b0456c6d039a1d1a0cb2fc2ef9d323322ac063352","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":"2026-08-17T20:01:22.243481Z","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":"2026-08-17T03:26:04.600930Z","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:eb46cdebd71c1635ee2265532235eff56db644100d9f458f7ab941eb7f101c63","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":"2026-08-17T20:01:22.243481Z","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":"2026-08-13T18:24:07.514776Z","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":"sha256:70bed9c12f997192425aece08b25ae2d6a74a27ebc5728db39b1756bb0d31446","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":"2026-08-17T20:01:22.243481Z","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":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"thesis":"As of 17 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 12 inbound Pith citation observations for arXiv:2011.01318."}