{"as_of":"2026-08-14T22:37:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:d92d5bb0e564535864a8678351fc93b395bd5f884cf4a37e5b2fa7b2a88cd215","coverage":[{"denominator":113,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":100,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-14T14:29:00.757995Z","state":"measured"},{"denominator":101,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":101,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-14T06:32:32.682623+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":"2026-08-14T14:29:00.398069Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"cited_works","source_observed_at":null,"state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"1908.03135","last_updated":"2019-08-08T16:01:36Z","snapshot_observed_at":"2026-08-14T14:20:29.928442Z","submitted_at":"2019-08-08T16:01:36Z","title":"Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1908.03135","snapshot_observed_at":"2026-08-14T14:29:00.398069Z","title":null,"venue":null,"work_id":null,"year":1908},"citing_paper":{"arxiv_id":"1908.03135","last_updated":"2019-08-08T16:01:36Z","snapshot_observed_at":"2026-08-14T14:20:29.928442Z","submitted_at":"2019-08-08T16:01:36Z","title":"Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity","version":1},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-14T14:29:00.398069Z"},"links":{"cited_paper":"/paper/1908.03135","citing_paper":"/paper/1908.03135"},"observation_digest":"sha256:78aaec106203ef18266610802554b83e8a73a03528d050be6d8edfdbb09d93a0","observation_id":"12be506c-7fa2-4afe-875c-2ff90405d843","resolution":{"observed_at":"2026-08-14T14:29:00.398069Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/1908.03135/citation-record","integrity":"/paper/1908.03135/integrity","json":"/paper/1908.03135/citation-record.json","paper":"/paper/1908.03135"},"outbound":[{"citation":{"cited_paper":{"arxiv_id":"1908.03135","last_updated":"2019-08-08T16:01:36Z","snapshot_observed_at":"2026-08-14T14:20:29.928442Z","submitted_at":"2019-08-08T16:01:36Z","title":"Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1908.03135","snapshot_observed_at":"2026-08-14T14:29:00.398069Z","title":null,"venue":null,"work_id":null,"year":1908},"citing_paper":{"arxiv_id":"1908.03135","last_updated":"2019-08-08T16:01:36Z","snapshot_observed_at":"2026-08-14T14:20:29.928442Z","submitted_at":"2019-08-08T16:01:36Z","title":"Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity","version":1},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-14T14:29:00.398069Z"},"links":{"cited_paper":"/paper/1908.03135","citing_paper":"/paper/1908.03135"},"observation_digest":"sha256:78aaec106203ef18266610802554b83e8a73a03528d050be6d8edfdbb09d93a0","observation_id":"12be506c-7fa2-4afe-875c-2ff90405d843","resolution":{"observed_at":"2026-08-14T14:29:00.398069Z","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":"2026-08-14T14:29:00.403286Z","title":"tdBag model for strange quark matter tdBag [35] is a bag-like model inspired by the standard MIT bag model [ 36,37]1","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"1908.03135","last_updated":"2019-08-08T16:01:36Z","snapshot_observed_at":"2026-08-14T14:20:29.928442Z","submitted_at":"2019-08-08T16:01:36Z","title":"Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity","version":1},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-14T14:29:00.403286Z"},"links":{"citing_paper":"/paper/1908.03135"},"observation_digest":"sha256:1a81a8baa560c9c9d199b8eee0c454989ebededd4dcb2cb33653af813d2c6857","observation_id":"ce6420f7-245e-4472-9d6a-def0a5effb96","resolution":{"observed_at":"2026-08-14T14:29:00.403286Z","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":"2026-08-14T14:29:00.408076Z","title":"Fraga et al","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"1908.03135","last_updated":"2019-08-08T16:01:36Z","snapshot_observed_at":"2026-08-14T14:20:29.928442Z","submitted_at":"2019-08-08T16:01:36Z","title":"Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity","version":1},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-14T14:29:00.408076Z"},"links":{"citing_paper":"/paper/1908.03135"},"observation_digest":"sha256:7c6cc236ea9b565c98e8b50c78e33dbe7c692fcf6ec51adcab870fb2c98db514","observation_id":"d547355d-3af2-4631-a74a-cb1d22621825","resolution":{"observed_at":"2026-08-14T14:29:00.408076Z","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":"2026-08-14T14:29:00.411898Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"1908.03135","last_updated":"2019-08-08T16:01:36Z","snapshot_observed_at":"2026-08-14T14:20:29.928442Z","submitted_at":"2019-08-08T16:01:36Z","title":"Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity","version":1},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-14T14:29:00.411898Z"},"links":{"citing_paper":"/paper/1908.03135"},"observation_digest":"sha256:3698780e63eb9c15ab7a3a7e4fad10f99b27b8c3390a3616a6eaf222c146861c","observation_id":"2fa0fb00-47cb-432e-bc56-e0604a975584","resolution":{"observed_at":"2026-08-14T14:29:00.411898Z","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":"2026-08-14T14:29:00.415739Z","title":"vacuumless","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"1908.03135","last_updated":"2019-08-08T16:01:36Z","snapshot_observed_at":"2026-08-14T14:20:29.928442Z","submitted_at":"2019-08-08T16:01:36Z","title":"Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity","version":1},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-14T14:29:00.415739Z"},"links":{"citing_paper":"/paper/1908.03135"},"observation_digest":"sha256:e1865b7427e988716d8588100dacc724c9852236d8e815277f3e5ff9b13c843d","observation_id":"2430d00e-50f3-4465-bbb9-4e9bd2843ecd","resolution":{"observed_at":"2026-08-14T14:29:00.415739Z","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":"2026-08-14T14:29:00.419541Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"1908.03135","last_updated":"2019-08-08T16:01:36Z","snapshot_observed_at":"2026-08-14T14:20:29.928442Z","submitted_at":"2019-08-08T16:01:36Z","title":"Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity","version":1},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-14T14:29:00.419541Z"},"links":{"citing_paper":"/paper/1908.03135"},"observation_digest":"sha256:e0ba3077ee536b103bc5ac83c861ea550085e04fff6253130f2605a940b293ea","observation_id":"dbfc6e4c-c95b-4bf0-8042-7b24b036e0a7","resolution":{"observed_at":"2026-08-14T14:29:00.419541Z","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":"2026-08-14T14:29:00.445096Z","title":"Our procedure can be applied to study a variety of parameters and HM EoS choice and enables future studies of NSs binary containing SQM cores","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"1908.03135","last_updated":"2019-08-08T16:01:36Z","snapshot_observed_at":"2026-08-14T14:20:29.928442Z","submitted_at":"2019-08-08T16:01:36Z","title":"Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity","version":1},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-14T14:29:00.445096Z"},"links":{"citing_paper":"/paper/1908.03135"},"observation_digest":"sha256:620b0f95b3b1a8777fbf240248ca0db7e52b2c2b329cf9e652337dcb168f2dd5","observation_id":"2eb793e9-1c09-4700-b16b-b59ad4cebfc5","resolution":{"observed_at":"2026-08-14T14:29:00.445096Z","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":"2026-08-14T14:29:00.428902Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"1908.03135","last_updated":"2019-08-08T16:01:36Z","snapshot_observed_at":"2026-08-14T14:20:29.928442Z","submitted_at":"2019-08-08T16:01:36Z","title":"Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity","version":1},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-14T14:29:00.428902Z"},"links":{"citing_paper":"/paper/1908.03135"},"observation_digest":"sha256:aba55c726a2427e2d05ba398685afdad2d8b00c8a803bb1e55cefba8471a9391","observation_id":"48a53f41-ce09-4410-82f6-1c9d1c4bed65","resolution":{"observed_at":"2026-08-14T14:29:00.428902Z","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":"2026-08-14T14:29:00.432624Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"1908.03135","last_updated":"2019-08-08T16:01:36Z","snapshot_observed_at":"2026-08-14T14:20:29.928442Z","submitted_at":"2019-08-08T16:01:36Z","title":"Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity","version":1},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-14T14:29:00.432624Z"},"links":{"citing_paper":"/paper/1908.03135"},"observation_digest":"sha256:27689e8718d5baa7829de97208367d70834ddfab58f7a61c4fbb2e5ba0db4ac2","observation_id":"8e1b3cab-90c5-4038-982f-dbaa9839bd05","resolution":{"observed_at":"2026-08-14T14:29:00.432624Z","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":"2026-08-14T14:29:00.436413Z","title":"The Inspiral We present the full gravitational waveform obtained from our simulations in Fig","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"1908.03135","last_updated":"2019-08-08T16:01:36Z","snapshot_observed_at":"2026-08-14T14:20:29.928442Z","submitted_at":"2019-08-08T16:01:36Z","title":"Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity","version":1},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-14T14:29:00.436413Z"},"links":{"citing_paper":"/paper/1908.03135"},"observation_digest":"sha256:c7a5c147cc81765ea22713db9a61ee23c16a4731c24c302c2d798732c0946604","observation_id":"c879b4b0-23b6-4fae-a7e8-da67ad95f4ce","resolution":{"observed_at":"2026-08-14T14:29:00.436413Z","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":"2026-08-14T14:29:00.440691Z","title":"45.0 47.5 50.0 52.5 55.0 57.5 60.0 62.5 t[ms] 0.0 0.2 0.4 0.6 0.8 1.0 ρmax [g/cm3] ×1016 ρmax 0.00 0.02 0.04 0.06 M [M⊙] GW170817 Mej 1 2Mdisk Figure 7","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"1908.03135","last_updated":"2019-08-08T16:01:36Z","snapshot_observed_at":"2026-08-14T14:20:29.928442Z","submitted_at":"2019-08-08T16:01:36Z","title":"Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity","version":1},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-14T14:29:00.440691Z"},"links":{"citing_paper":"/paper/1908.03135"},"observation_digest":"sha256:66729fabe74be40da4b9bf9da7a951392e0a87207eb2d7deab4af05cb1cf1f94","observation_id":"49568ec7-5356-45d3-b55f-b14987716465","resolution":{"observed_at":"2026-08-14T14:29:00.440691Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1810.12917","last_updated":"2019-04-10T17:50:33Z","snapshot_observed_at":"2026-08-14T18:06:53.368373Z","submitted_at":"2018-10-30T18:00:01Z","title":"Multimessenger Parameter Estimation of GW170817","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1810.12917","snapshot_observed_at":"2026-08-14T14:29:00.489103Z","title":"Multimessenger Parameter Estimation of GW170817 2018","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"1908.03135","last_updated":"2019-08-08T16:01:36Z","snapshot_observed_at":"2026-08-14T14:20:29.928442Z","submitted_at":"2019-08-08T16:01:36Z","title":"Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity","version":1},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-14T14:29:00.489103Z"},"links":{"cited_paper":"/paper/1810.12917","citing_paper":"/paper/1908.03135"},"observation_digest":"sha256:705c8a6d05afde6267938df1c037c50319fa633c855aaadb4fefe2c7cb2591b0","observation_id":"ad6dfc60-dcca-48e5-81ed-5832cb17fef6","resolution":{"observed_at":"2026-08-14T14:29:00.489103Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1710.05832","last_updated":"2017-10-16T16:57:17Z","snapshot_observed_at":"2026-07-09T17:52:08.260915Z","submitted_at":"2017-10-16T16:57:17Z","title":"GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1710.05832","snapshot_observed_at":"2026-08-14T14:29:00.448644Z","title":"GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"1908.03135","last_updated":"2019-08-08T16:01:36Z","snapshot_observed_at":"2026-08-14T14:20:29.928442Z","submitted_at":"2019-08-08T16:01:36Z","title":"Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity","version":1},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-14T14:29:00.448644Z"},"links":{"cited_paper":"/paper/1710.05832","citing_paper":"/paper/1908.03135"},"observation_digest":"sha256:61716713cd2e08c0338100bb89cfaa86497e9ada84fa63d8ab5bf930c0c7b779","observation_id":"a70ba43f-d25f-4ea8-941e-092ed44966e4","resolution":{"observed_at":"2026-08-14T14:29:00.448644Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1710.05833","last_updated":"2017-10-24T12:03:18Z","snapshot_observed_at":"2026-08-14T20:23:19.773859Z","submitted_at":"2017-10-16T16:57:18Z","title":"Multi-messenger Observations of a Binary Neutron Star Merger","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1710.05833","snapshot_observed_at":"2026-08-14T14:29:00.452593Z","title":"Multi-messenger Observations of a Binary Neutron Star Merger","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"1908.03135","last_updated":"2019-08-08T16:01:36Z","snapshot_observed_at":"2026-08-14T14:20:29.928442Z","submitted_at":"2019-08-08T16:01:36Z","title":"Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity","version":1},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-14T14:29:00.452593Z"},"links":{"cited_paper":"/paper/1710.05833","citing_paper":"/paper/1908.03135"},"observation_digest":"sha256:bd3f3c1f37f9230d2609dabb74cd10a9faa835c9db27f639f149a376846e89bb","observation_id":"8bff7709-b012-4725-a1f5-006eb4989663","resolution":{"observed_at":"2026-08-14T14:29:00.452593Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1710.05834","last_updated":"2017-11-02T11:19:17Z","snapshot_observed_at":"2026-08-14T20:23:20.089633Z","submitted_at":"2017-10-16T16:57:19Z","title":"Gravitational Waves and Gamma-rays from a Binary Neutron Star Merger: GW170817 and GRB 170817A","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1710.05834","snapshot_observed_at":"2026-08-14T14:29:00.456415Z","title":"Gravitational Waves and Gamma-rays from a Binary Neutron Star Merger: GW170817 and GRB 170817A","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"1908.03135","last_updated":"2019-08-08T16:01:36Z","snapshot_observed_at":"2026-08-14T14:20:29.928442Z","submitted_at":"2019-08-08T16:01:36Z","title":"Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity","version":1},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-14T14:29:00.456415Z"},"links":{"cited_paper":"/paper/1710.05834","citing_paper":"/paper/1908.03135"},"observation_digest":"sha256:f63306d5a4dc9fe275f5eeb47a7a3c817f49af55442017ec0034b56b77b269af","observation_id":"3e106721-6e1e-4347-a824-cccaeafa9e09","resolution":{"observed_at":"2026-08-14T14:29:00.456415Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1806.08793","last_updated":"2018-08-02T14:11:06Z","snapshot_observed_at":"2026-08-14T19:00:25.354471Z","submitted_at":"2018-06-22T18:00:00Z","title":"Parameter Estimation for GW170817 using Relative Binning","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1806.08793","snapshot_observed_at":"2026-08-14T14:29:00.460524Z","title":"Parameter Estimation for GW170817 using Relative Binning 2018","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"1908.03135","last_updated":"2019-08-08T16:01:36Z","snapshot_observed_at":"2026-08-14T14:20:29.928442Z","submitted_at":"2019-08-08T16:01:36Z","title":"Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity","version":1},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-14T14:29:00.460524Z"},"links":{"cited_paper":"/paper/1806.08793","citing_paper":"/paper/1908.03135"},"observation_digest":"sha256:7af29a6429227cef164730c76ec1daa7a58d5c9ffc3aace4f7df14a689f04a30","observation_id":"54e73f3a-0900-4f24-ad31-9b08f38200ff","resolution":{"observed_at":"2026-08-14T14:29:00.460524Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1804.08583","last_updated":"2018-10-30T18:34:14Z","snapshot_observed_at":"2026-08-14T19:22:56.378643Z","submitted_at":"2018-04-23T17:22:22Z","title":"Tidal Deformabilities and Radii of Neutron Stars from the Observation of GW170817","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1804.08583","snapshot_observed_at":"2026-08-14T14:29:00.464302Z","title":"Tidal Deformabilities and Radii of Neutron Stars from the Observation of GW170817","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"1908.03135","last_updated":"2019-08-08T16:01:36Z","snapshot_observed_at":"2026-08-14T14:20:29.928442Z","submitted_at":"2019-08-08T16:01:36Z","title":"Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity","version":1},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-14T14:29:00.464302Z"},"links":{"cited_paper":"/paper/1804.08583","citing_paper":"/paper/1908.03135"},"observation_digest":"sha256:c2dc5fe391f42a3a3ee0986f0f527794160338a1092475edf396896f8b7a7016","observation_id":"e13b942a-faea-44e2-bfa0-586d06711774","resolution":{"observed_at":"2026-08-14T14:29:00.464302Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1805.11579","last_updated":"2019-01-22T19:56:03Z","snapshot_observed_at":"2026-08-14T19:09:50.234456Z","submitted_at":"2018-05-29T16:55:48Z","title":"Properties of the binary neutron star merger GW170817","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1805.11579","snapshot_observed_at":"2026-08-14T14:29:00.468409Z","title":"Properties of the binary neutron star merger GW170817","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"1908.03135","last_updated":"2019-08-08T16:01:36Z","snapshot_observed_at":"2026-08-14T14:20:29.928442Z","submitted_at":"2019-08-08T16:01:36Z","title":"Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity","version":1},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-14T14:29:00.468409Z"},"links":{"cited_paper":"/paper/1805.11579","citing_paper":"/paper/1908.03135"},"observation_digest":"sha256:030e00a1b9a00f43aeec43840bf1ba206714e49235d20bf39698112a9d4f8b26","observation_id":"8017ad51-bfec-4cbc-8d10-2aa1d45ad09a","resolution":{"observed_at":"2026-08-14T14:29:00.468409Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1805.11581","last_updated":"2018-10-15T17:59:04Z","snapshot_observed_at":"2026-08-14T19:09:49.769515Z","submitted_at":"2018-05-29T16:56:13Z","title":"GW170817: Measurements of Neutron Star Radii and Equation of State","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1805.11581","snapshot_observed_at":"2026-08-14T14:29:00.472005Z","title":"GW170817: Measurements of neutron star radii and equation of state","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"1908.03135","last_updated":"2019-08-08T16:01:36Z","snapshot_observed_at":"2026-08-14T14:20:29.928442Z","submitted_at":"2019-08-08T16:01:36Z","title":"Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity","version":1},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-14T14:29:00.472005Z"},"links":{"cited_paper":"/paper/1805.11581","citing_paper":"/paper/1908.03135"},"observation_digest":"sha256:1a73629f7c1a5a21477589ca173d0fe184367d253c7ce99aac571073fd39384a","observation_id":"ed687f9e-a831-4cd4-8105-13a6d318d92b","resolution":{"observed_at":"2026-08-14T14:29:00.472005Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1811.12907","last_updated":"2019-10-04T08:10:25Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2018-11-30T17:34:09Z","title":"GWTC-1: A Gravitational-Wave Transient Catalog of Compact Binary Mergers Observed by LIGO and Virgo during the First and Second Observing Runs","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1811.12907","snapshot_observed_at":"2026-08-14T14:29:00.475534Z","title":"GWTC-1: A Gravitational-Wave Transient Catalog of Compact Binary Mergers Observed by LIGO and Virgo during the First and Second Observing Runs 2018","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"1908.03135","last_updated":"2019-08-08T16:01:36Z","snapshot_observed_at":"2026-08-14T14:20:29.928442Z","submitted_at":"2019-08-08T16:01:36Z","title":"Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity","version":1},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-14T14:29:00.475534Z"},"links":{"cited_paper":"/paper/1811.12907","citing_paper":"/paper/1908.03135"},"observation_digest":"sha256:4ef03ae3e96a4cfcc9d8953f5d68caf0be7d74605791cf40d94356f06c95f182","observation_id":"d95edacd-148c-4ec2-ab2d-f83b15ad3400","resolution":{"observed_at":"2026-08-14T14:29:00.475534Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1711.03647","last_updated":"2017-12-24T17:36:18Z","snapshot_observed_at":"2026-08-14T20:15:06.207450Z","submitted_at":"2017-11-09T23:34:10Z","title":"GW170817: Joint Constraint on the Neutron Star Equation of State from Multimessenger Observations","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1711.03647","snapshot_observed_at":"2026-08-14T14:29:00.478943Z","title":"GW170817: Joint Constraint on the Neutron Star Equation of State from Multimessenger Observations","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"1908.03135","last_updated":"2019-08-08T16:01:36Z","snapshot_observed_at":"2026-08-14T14:20:29.928442Z","submitted_at":"2019-08-08T16:01:36Z","title":"Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity","version":1},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-14T14:29:00.478943Z"},"links":{"cited_paper":"/paper/1711.03647","citing_paper":"/paper/1908.03135"},"observation_digest":"sha256:af8d0ce040beb3b3e06f7f2cfde6915867b22180819f527e3349d7ba4424bb6d","observation_id":"10620419-ccd5-437a-9e95-81c1bc224beb","resolution":{"observed_at":"2026-08-14T14:29:00.478943Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1710.06843","last_updated":"2017-11-09T13:25:18Z","snapshot_observed_at":"2026-08-14T20:22:27.672123Z","submitted_at":"2017-10-18T17:49:44Z","title":"Neutron-star radius constraints from GW170817 and future detections","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1710.06843","snapshot_observed_at":"2026-08-14T14:29:00.482250Z","title":"Neutron-star radius constraints from GW170817 and future detections","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"1908.03135","last_updated":"2019-08-08T16:01:36Z","snapshot_observed_at":"2026-08-14T14:20:29.928442Z","submitted_at":"2019-08-08T16:01:36Z","title":"Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity","version":1},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-14T14:29:00.482250Z"},"links":{"cited_paper":"/paper/1710.06843","citing_paper":"/paper/1908.03135"},"observation_digest":"sha256:8dd8f9673a08a5e484d938d4546e9bf8b29c990c0840e387dc4c910e0489cebb","observation_id":"5f443b4d-d302-4014-9a8e-5185dcf287d7","resolution":{"observed_at":"2026-08-14T14:29:00.482250Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1805.09371","last_updated":"2018-10-17T18:23:38Z","snapshot_observed_at":"2026-08-14T19:11:51.800026Z","submitted_at":"2018-05-23T18:31:07Z","title":"Constraints on the neutron star equation of state from AT2017gfo using radiative transfer simulations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1805.09371","snapshot_observed_at":"2026-08-14T14:29:00.485976Z","title":"Constraints on the neutron star equation of state from AT2017gfo using radiative transfer simulations 2018","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"1908.03135","last_updated":"2019-08-08T16:01:36Z","snapshot_observed_at":"2026-08-14T14:20:29.928442Z","submitted_at":"2019-08-08T16:01:36Z","title":"Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity","version":1},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-14T14:29:00.485976Z"},"links":{"cited_paper":"/paper/1805.09371","citing_paper":"/paper/1908.03135"},"observation_digest":"sha256:420214cb3f77b6eab1407e9e3359f5f6a318b15bced83fe021ca6d01ed7fb91c","observation_id":"06315c03-782d-4efb-be67-d8a3ae5ea1d4","resolution":{"observed_at":"2026-08-14T14:29:00.485976Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1101.4298","last_updated":"2011-03-30T13:57:32Z","snapshot_observed_at":"2026-07-06T02:22:23.572887Z","submitted_at":"2011-01-22T15:51:37Z","title":"The missing link: Merging neutron stars naturally produce jet-like structures and can power short Gamma-Ray Bursts","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1101.4298","snapshot_observed_at":"2026-08-14T14:29:00.531276Z","title":"The missing link: Merging neutron stars naturally produce jet-like structures and can power short Gamma-Ray Bursts","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"1908.03135","last_updated":"2019-08-08T16:01:36Z","snapshot_observed_at":"2026-08-14T14:20:29.928442Z","submitted_at":"2019-08-08T16:01:36Z","title":"Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity","version":1},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-14T14:29:00.531276Z"},"links":{"cited_paper":"/paper/1101.4298","citing_paper":"/paper/1908.03135"},"observation_digest":"sha256:abfdb922b2cc2dcef5181135d59392c1e077687823ba6eed229008cfa09f17e5","observation_id":"918b7c48-8ba8-4201-844d-900979e7aef5","resolution":{"observed_at":"2026-08-14T14:29:00.531276Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1812.04803","last_updated":"2021-02-04T16:55:12Z","snapshot_observed_at":"2026-08-14T17:44:55.944887Z","submitted_at":"2018-12-12T04:23:11Z","title":"Multi-messenger Bayesian parameter inference of a binary neutron-star merger","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1812.04803","snapshot_observed_at":"2026-08-14T14:29:00.492227Z","title":"Multi-messenger Bayesian parameter inference of a binary neutron-star merger 2018","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"1908.03135","last_updated":"2019-08-08T16:01:36Z","snapshot_observed_at":"2026-08-14T14:20:29.928442Z","submitted_at":"2019-08-08T16:01:36Z","title":"Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity","version":1},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-14T14:29:00.492227Z"},"links":{"cited_paper":"/paper/1812.04803","citing_paper":"/paper/1908.03135"},"observation_digest":"sha256:4db39cad1f7e8bcd023c4413888dc94dc9e06c2ae33546901859e99270f5d16b","observation_id":"158c3ea7-a2b2-46e7-960b-6d934ef3f826","resolution":{"observed_at":"2026-08-14T14:29:00.492227Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1711.02644","last_updated":"2018-03-22T14:25:12Z","snapshot_observed_at":"2026-08-14T20:15:59.729401Z","submitted_at":"2017-11-07T18:06:28Z","title":"Gravitational-wave constraints on the neutron-star-matter Equation of State","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1711.02644","snapshot_observed_at":"2026-08-14T14:29:00.495279Z","title":"Gravitational-wave constraints on the neutron-star-matter Equation of State","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"1908.03135","last_updated":"2019-08-08T16:01:36Z","snapshot_observed_at":"2026-08-14T14:20:29.928442Z","submitted_at":"2019-08-08T16:01:36Z","title":"Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity","version":1},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-14T14:29:00.495279Z"},"links":{"cited_paper":"/paper/1711.02644","citing_paper":"/paper/1908.03135"},"observation_digest":"sha256:01f7b6203666ce6fadbd9cd009d4224bc36526bd166794605b4002efe6af0143","observation_id":"46a99fca-c0f1-4eb4-b5e6-3a2d733b530f","resolution":{"observed_at":"2026-08-14T14:29:00.495279Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1803.00549","last_updated":"2018-05-31T11:15:49Z","snapshot_observed_at":"2026-08-14T19:40:33.450471Z","submitted_at":"2018-03-01T18:36:24Z","title":"New constraints on radii and tidal deformabilities of neutron stars from GW170817","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1803.00549","snapshot_observed_at":"2026-08-14T14:29:00.498343Z","title":"New constraints on radii and tidal deformabilities of neutron stars from GW170817","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"1908.03135","last_updated":"2019-08-08T16:01:36Z","snapshot_observed_at":"2026-08-14T14:20:29.928442Z","submitted_at":"2019-08-08T16:01:36Z","title":"Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity","version":1},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-14T14:29:00.498343Z"},"links":{"cited_paper":"/paper/1803.00549","citing_paper":"/paper/1908.03135"},"observation_digest":"sha256:359e0b40090fad3566df0fa0cea1ed8240a7b3194795947ea82cbd65f41267bb","observation_id":"7f442483-dab2-4d13-b030-b0259a70dfb0","resolution":{"observed_at":"2026-08-14T14:29:00.498343Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1903.09121","last_updated":"2021-07-27T11:45:07Z","snapshot_observed_at":"2026-08-14T16:58:41.975167Z","submitted_at":"2019-03-21T17:30:37Z","title":"Evidence for quark-matter cores in massive neutron stars","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1903.09121","snapshot_observed_at":"2026-08-14T14:29:00.501712Z","title":"Quark-matter cores in neutron stars 2019","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"1908.03135","last_updated":"2019-08-08T16:01:36Z","snapshot_observed_at":"2026-08-14T14:20:29.928442Z","submitted_at":"2019-08-08T16:01:36Z","title":"Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity","version":1},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-14T14:29:00.501712Z"},"links":{"cited_paper":"/paper/1903.09121","citing_paper":"/paper/1908.03135"},"observation_digest":"sha256:06b2ea5b75ad597b94163995053e821697da9a2072119c1b42c398964ede25f1","observation_id":"c3752739-1d5b-4d87-9b62-a2e346899b0d","resolution":{"observed_at":"2026-08-14T14:29:00.501712Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1807.03684","last_updated":"2019-02-19T05:54:45Z","snapshot_observed_at":"2026-08-14T18:53:43.234542Z","submitted_at":"2018-07-10T14:46:27Z","title":"Signatures of quark-hadron phase transitions in general-relativistic neutron-star mergers","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1807.03684","snapshot_observed_at":"2026-08-14T14:29:00.504928Z","title":"Signatures of quark-hadron phase transitions in general-relativistic neutron-star mergers","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"1908.03135","last_updated":"2019-08-08T16:01:36Z","snapshot_observed_at":"2026-08-14T14:20:29.928442Z","submitted_at":"2019-08-08T16:01:36Z","title":"Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity","version":1},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-14T14:29:00.504928Z"},"links":{"cited_paper":"/paper/1807.03684","citing_paper":"/paper/1908.03135"},"observation_digest":"sha256:c822bfed78b50e764e364976d608dc99161b31714ce4b1a2d8d6b1a647bbcf78","observation_id":"b0c36628-9d91-49ff-bc1f-f0c327f3e12d","resolution":{"observed_at":"2026-08-14T14:29:00.504928Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1809.01116","last_updated":"2019-01-16T16:28:44Z","snapshot_observed_at":"2026-08-14T18:33:08.609692Z","submitted_at":"2018-09-04T17:42:08Z","title":"Identifying a first-order phase transition in neutron star mergers through gravitational waves","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1809.01116","snapshot_observed_at":"2026-08-14T14:29:00.508510Z","title":"Identifying a first-order phase transition in neutron star mergers through gravitational waves","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"1908.03135","last_updated":"2019-08-08T16:01:36Z","snapshot_observed_at":"2026-08-14T14:20:29.928442Z","submitted_at":"2019-08-08T16:01:36Z","title":"Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity","version":1},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-14T14:29:00.508510Z"},"links":{"cited_paper":"/paper/1809.01116","citing_paper":"/paper/1908.03135"},"observation_digest":"sha256:1dcdeb9285d876ebcf292486da3a95fabb853653b0458d5aaca49b0216d389a2","observation_id":"78ef91d4-e46c-4101-bada-8ad0a34dbd08","resolution":{"observed_at":"2026-08-14T14:29:00.508510Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1306.6052","last_updated":"2013-10-23T22:40:02Z","snapshot_observed_at":"2026-07-06T03:16:45.088192Z","submitted_at":"2013-06-25T18:12:14Z","title":"Beyond second-order convergence in simulations of binary neutron stars in full general-relativity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1306.6052","snapshot_observed_at":"2026-08-14T14:29:00.512401Z","title":"Beyond second-order convergence in simulations of binary neutron stars in full general-relativity","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"1908.03135","last_updated":"2019-08-08T16:01:36Z","snapshot_observed_at":"2026-08-14T14:20:29.928442Z","submitted_at":"2019-08-08T16:01:36Z","title":"Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity","version":1},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-08-14T14:29:00.512401Z"},"links":{"cited_paper":"/paper/1306.6052","citing_paper":"/paper/1908.03135"},"observation_digest":"sha256:56691f44997cb8e267b33ac19677541372864da4b369322a283c2f64d6476c3a","observation_id":"b7850eb9-7f6f-4e92-be18-c8fe493fc6f2","resolution":{"observed_at":"2026-08-14T14:29:00.512401Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1502.03457","last_updated":"2015-02-11T21:14:03Z","snapshot_observed_at":"2026-07-06T04:08:59.584218Z","submitted_at":"2015-02-11T21:14:03Z","title":"Exploring tidal effects of coalescing binary neutron stars in numerical relativity II: Longterm simulations","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1502.03457","snapshot_observed_at":"2026-08-14T14:29:00.516067Z","title":"Exploring tidal effects of coalescing binary neutron stars in numerical relativity","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"1908.03135","last_updated":"2019-08-08T16:01:36Z","snapshot_observed_at":"2026-08-14T14:20:29.928442Z","submitted_at":"2019-08-08T16:01:36Z","title":"Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity","version":1},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-14T14:29:00.516067Z"},"links":{"cited_paper":"/paper/1502.03457","citing_paper":"/paper/1908.03135"},"observation_digest":"sha256:a31d3d01826fa5e1c6088011563d75dbc2388d97ca551dc92a4026653d9558de","observation_id":"938b5e79-fb77-4da6-86f4-8b9904954cf1","resolution":{"observed_at":"2026-08-14T14:29:00.516067Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1706.02969","last_updated":"2018-07-05T08:27:25Z","snapshot_observed_at":"2026-08-14T20:55:03.305843Z","submitted_at":"2017-06-09T14:23:36Z","title":"Closed-form tidal approximants for binary neutron star gravitational waveforms constructed from high-resolution numerical relativity simulations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1706.02969","snapshot_observed_at":"2026-08-14T14:29:00.519929Z","title":"Closed-form tidal approximants for binary neutron star gravitational waveforms constructed from high-resolution numerical relativity simulations","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"1908.03135","last_updated":"2019-08-08T16:01:36Z","snapshot_observed_at":"2026-08-14T14:20:29.928442Z","submitted_at":"2019-08-08T16:01:36Z","title":"Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity","version":1},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-14T14:29:00.519929Z"},"links":{"cited_paper":"/paper/1706.02969","citing_paper":"/paper/1908.03135"},"observation_digest":"sha256:6b1841909e5dd501d552ed6cf3b250021e88a771f77146d053b5dfd12692ef7a","observation_id":"96699d41-5945-4471-a0d4-42d2ff3547e5","resolution":{"observed_at":"2026-08-14T14:29:00.519929Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1708.08926","last_updated":"2017-08-29T18:00:01Z","snapshot_observed_at":"2026-08-14T20:38:01.730806Z","submitted_at":"2017-08-29T18:00:01Z","title":"Sub-radian-accuracy gravitational waveforms of coalescing binary neutron stars in numerical relativity","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1708.08926","snapshot_observed_at":"2026-08-14T14:29:00.523739Z","title":"Sub-radian-accuracy gravitational waveforms of coalescing binary neutron stars in numerical relativity","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"1908.03135","last_updated":"2019-08-08T16:01:36Z","snapshot_observed_at":"2026-08-14T14:20:29.928442Z","submitted_at":"2019-08-08T16:01:36Z","title":"Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity","version":1},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-14T14:29:00.523739Z"},"links":{"cited_paper":"/paper/1708.08926","citing_paper":"/paper/1908.03135"},"observation_digest":"sha256:3ed507bc265549ba8f85451a0051759eaa7b357c8aefc67452864fcba074cd32","observation_id":"3e05ff32-7409-45ea-9955-01c1cc4e4fb1","resolution":{"observed_at":"2026-08-14T14:29:00.523739Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1806.01625","last_updated":"2018-06-05T12:14:30Z","snapshot_observed_at":"2026-08-14T19:07:22.865818Z","submitted_at":"2018-06-05T12:14:30Z","title":"CoRe database of binary neutron star merger waveforms and its application in waveform development","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1806.01625","snapshot_observed_at":"2026-08-14T14:29:00.527475Z","title":"CoRe database of binary neutron star merger waveforms","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"1908.03135","last_updated":"2019-08-08T16:01:36Z","snapshot_observed_at":"2026-08-14T14:20:29.928442Z","submitted_at":"2019-08-08T16:01:36Z","title":"Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity","version":1},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-14T14:29:00.527475Z"},"links":{"cited_paper":"/paper/1806.01625","citing_paper":"/paper/1908.03135"},"observation_digest":"sha256:fb884d715c0b3b505fa066879592b7343c818ccd0fe85e271072b47c5acd0d1d","observation_id":"d2555a13-ee79-49d6-bcd9-6212732d780c","resolution":{"observed_at":"2026-08-14T14:29:00.527475Z","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":"2026-08-14T14:29:00.574549Z","title":"A New Extended Model of Hadrons.Phys","venue":null,"work_id":null,"year":1974},"citing_paper":{"arxiv_id":"1908.03135","last_updated":"2019-08-08T16:01:36Z","snapshot_observed_at":"2026-08-14T14:20:29.928442Z","submitted_at":"2019-08-08T16:01:36Z","title":"Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity","version":1},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-14T14:29:00.574549Z"},"links":{"citing_paper":"/paper/1908.03135"},"observation_digest":"sha256:69180126880045f328a4f07df6d9384ddf5756c4b0947d4ab737d00d5b885611","observation_id":"732fef48-4627-48a4-902c-aa4bd0590e8b","resolution":{"observed_at":"2026-08-14T14:29:00.574549Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1403.3680","last_updated":"2014-05-09T15:36:29Z","snapshot_observed_at":"2026-08-04T04:31:19.774761Z","submitted_at":"2014-03-14T19:41:42Z","title":"Magnetized Neutron Stars With Realistic Equations of State and Neutrino Cooling","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1403.3680","snapshot_observed_at":"2026-08-14T14:29:00.535005Z","title":"Magnetized Neutron Stars With Realistic Equations of State and Neutrino Cooling","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"1908.03135","last_updated":"2019-08-08T16:01:36Z","snapshot_observed_at":"2026-08-14T14:20:29.928442Z","submitted_at":"2019-08-08T16:01:36Z","title":"Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity","version":1},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-14T14:29:00.535005Z"},"links":{"cited_paper":"/paper/1403.3680","citing_paper":"/paper/1908.03135"},"observation_digest":"sha256:d79574fc171e8ad8573c08b3a924f3918b76e2ffb7fd0dd72cb643fb53b81eff","observation_id":"a0da15cf-f658-4c54-aa60-318a5544fc4f","resolution":{"observed_at":"2026-08-14T14:29:00.535005Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1502.06660","last_updated":"2015-03-03T10:58:05Z","snapshot_observed_at":"2026-07-06T04:10:04.095779Z","submitted_at":"2015-02-24T00:30:22Z","title":"The dynamical mass ejection from binary neutron star mergers: Radiation-hydrodynamics study in general relativity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1502.06660","snapshot_observed_at":"2026-08-14T14:29:00.538516Z","title":"Dynamical mass ejection from binary neutron star mergers: Radiation-hydrodynamics study in general relativity","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"1908.03135","last_updated":"2019-08-08T16:01:36Z","snapshot_observed_at":"2026-08-14T14:20:29.928442Z","submitted_at":"2019-08-08T16:01:36Z","title":"Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity","version":1},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-14T14:29:00.538516Z"},"links":{"cited_paper":"/paper/1502.06660","citing_paper":"/paper/1908.03135"},"observation_digest":"sha256:ef2275ab588f4bf62548d7b05a45931af009dd0b6153ceae56c0c5acc503b1d0","observation_id":"9c816f03-bf0e-498d-9e8f-f8c42b2783b8","resolution":{"observed_at":"2026-08-14T14:29:00.538516Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1505.01607","last_updated":"2015-05-07T07:35:19Z","snapshot_observed_at":"2026-08-10T03:31:43.290630Z","submitted_at":"2015-05-07T07:35:19Z","title":"Effects of the microphysical Equation of State in the mergers of magnetized Neutron Stars With Neutrino Cooling","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1505.01607","snapshot_observed_at":"2026-08-14T14:29:00.542335Z","title":"Effects of the microphysical Equation of State in the mergers of magnetized Neutron Stars With Neutrino Cooling","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"1908.03135","last_updated":"2019-08-08T16:01:36Z","snapshot_observed_at":"2026-08-14T14:20:29.928442Z","submitted_at":"2019-08-08T16:01:36Z","title":"Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity","version":1},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-08-14T14:29:00.542335Z"},"links":{"cited_paper":"/paper/1505.01607","citing_paper":"/paper/1908.03135"},"observation_digest":"sha256:fcde894b61d9b0e66f9398450832a3d2db98cdae79d748886e6b2ab9336664f8","observation_id":"3f04f5a8-d9d3-4adc-ab99-088dce373924","resolution":{"observed_at":"2026-08-14T14:29:00.542335Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1708.08452","last_updated":"2018-01-10T20:43:41Z","snapshot_observed_at":"2026-08-14T20:38:27.399219Z","submitted_at":"2017-08-28T18:00:01Z","title":"Monte-Carlo closure for moment-based transport schemes in general relativistic radiation hydrodynamics simulations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1708.08452","snapshot_observed_at":"2026-08-14T14:29:00.545820Z","title":"Monte Carlo closure for moment-based transport schemes in general relativistic radiation hydrodynamic simulations","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"1908.03135","last_updated":"2019-08-08T16:01:36Z","snapshot_observed_at":"2026-08-14T14:20:29.928442Z","submitted_at":"2019-08-08T16:01:36Z","title":"Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity","version":1},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-08-14T14:29:00.545820Z"},"links":{"cited_paper":"/paper/1708.08452","citing_paper":"/paper/1908.03135"},"observation_digest":"sha256:4343b57b715e8d7d7ffae81745c3b5ae512c656d89941ae85433fb90e0c45221","observation_id":"3bd3d795-1653-4c66-9d10-7942e433cae7","resolution":{"observed_at":"2026-08-14T14:29:00.545820Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1711.00473","last_updated":"2018-05-04T18:16:43Z","snapshot_observed_at":"2026-08-14T20:17:54.344578Z","submitted_at":"2017-11-01T18:00:02Z","title":"GW170817, General Relativistic Magnetohydrodynamic Simulations, and the Neutron Star Maximum Mass","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1711.00473","snapshot_observed_at":"2026-08-14T14:29:00.549490Z","title":"GW170817, General Relativistic Magnetohydrodynamic Simulations, and the Neutron Star Maximum Mass","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"1908.03135","last_updated":"2019-08-08T16:01:36Z","snapshot_observed_at":"2026-08-14T14:20:29.928442Z","submitted_at":"2019-08-08T16:01:36Z","title":"Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity","version":1},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-08-14T14:29:00.549490Z"},"links":{"cited_paper":"/paper/1711.00473","citing_paper":"/paper/1908.03135"},"observation_digest":"sha256:f6c330759a0e01b82e5e45c3ae69168bbb1249b33b3436cf7d1f04f3aa758e78","observation_id":"f8e24310-f8b5-4d68-80be-50909b290bf3","resolution":{"observed_at":"2026-08-14T14:29:00.549490Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1701.08738","last_updated":"2017-05-01T08:14:45Z","snapshot_observed_at":"2026-08-14T21:18:51.623921Z","submitted_at":"2017-01-30T18:15:16Z","title":"General relativistic magnetohydrodynamic simulations of binary neutron star mergers forming a long-lived neutron star","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1701.08738","snapshot_observed_at":"2026-08-14T14:29:00.553272Z","title":"General relativistic magnetohydrodynamic simulations of binary neutron star mergers forming a long-lived neutron star","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"1908.03135","last_updated":"2019-08-08T16:01:36Z","snapshot_observed_at":"2026-08-14T14:20:29.928442Z","submitted_at":"2019-08-08T16:01:36Z","title":"Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity","version":1},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-08-14T14:29:00.553272Z"},"links":{"cited_paper":"/paper/1701.08738","citing_paper":"/paper/1908.03135"},"observation_digest":"sha256:dbe7f43a5901b93d6d767db9a2a7d07a635c6a348a167f07ac46bca24dff7028","observation_id":"cc4614eb-06f1-4695-8afb-ccc958807dfb","resolution":{"observed_at":"2026-08-14T14:29:00.553272Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1710.01311","last_updated":"2018-05-09T13:13:15Z","snapshot_observed_at":"2026-08-14T20:27:11.162162Z","submitted_at":"2017-10-03T18:00:05Z","title":"Global simulations of strongly magnetized remnant massive neutron stars formed in binary neutron star mergers","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1710.01311","snapshot_observed_at":"2026-08-14T14:29:00.556836Z","title":"Global simulations of strongly magnetized remnant massive neutron stars formed in binary neutron star mergers","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"1908.03135","last_updated":"2019-08-08T16:01:36Z","snapshot_observed_at":"2026-08-14T14:20:29.928442Z","submitted_at":"2019-08-08T16:01:36Z","title":"Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity","version":1},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-08-14T14:29:00.556836Z"},"links":{"cited_paper":"/paper/1710.01311","citing_paper":"/paper/1908.03135"},"observation_digest":"sha256:4ce55c4164eac22fbb56d50c4d4d5df1973369d41b9ee907d6c52ddf3a02f22d","observation_id":"3dcb2221-cb8e-42f3-a05e-83ce5534946e","resolution":{"observed_at":"2026-08-14T14:29:00.556836Z","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":"2026-08-14T14:29:00.424365Z","title":"They consider the ground state of matter to be three Fermi seas of deconfined quarks in equal proportions of up, down and strange flavors","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"1908.03135","last_updated":"2019-08-08T16:01:36Z","snapshot_observed_at":"2026-08-14T14:20:29.928442Z","submitted_at":"2019-08-08T16:01:36Z","title":"Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity","version":1},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-08-14T14:29:00.424365Z"},"links":{"citing_paper":"/paper/1908.03135"},"observation_digest":"sha256:0ec946dd5f3a21cb8e52992cbccff7813deec824ace27d820c10e7a02e469332","observation_id":"b3cc82d8-06b2-44d5-a6c2-dc3a413f4312","resolution":{"observed_at":"2026-08-14T14:29:00.424365Z","resolver_source":null,"status":"malformed_identifier"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1703.02046","last_updated":"2017-03-06T19:00:01Z","snapshot_observed_at":"2026-08-14T21:13:16.649302Z","submitted_at":"2017-03-06T19:00:01Z","title":"General-Relativistic Large-Eddy Simulations of Binary Neutron Star Mergers","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1703.02046","snapshot_observed_at":"2026-08-14T14:29:00.560770Z","title":"General-Relativistic Large-Eddy Simulations of Binary Neutron Star Mergers","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"1908.03135","last_updated":"2019-08-08T16:01:36Z","snapshot_observed_at":"2026-08-14T14:20:29.928442Z","submitted_at":"2019-08-08T16:01:36Z","title":"Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity","version":1},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-08-14T14:29:00.560770Z"},"links":{"cited_paper":"/paper/1703.02046","citing_paper":"/paper/1908.03135"},"observation_digest":"sha256:0b9f187d94977d8acb3322a288547a74c434ee43b4a31ccecccfa18f4dcaa38c","observation_id":"7f8ffd84-2bf0-4802-af1a-bf068be4eb1b","resolution":{"observed_at":"2026-08-14T14:29:00.560770Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1703.10303","last_updated":"2017-03-30T03:53:11Z","snapshot_observed_at":"2026-08-14T21:09:17.007386Z","submitted_at":"2017-03-30T03:53:11Z","title":"General relativistic viscous hydrodynamics of differentially rotating neutron stars","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1703.10303","snapshot_observed_at":"2026-08-14T14:29:00.564783Z","title":"General relativistic viscous hydrodynamics of differentially rotating neutron stars","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"1908.03135","last_updated":"2019-08-08T16:01:36Z","snapshot_observed_at":"2026-08-14T14:20:29.928442Z","submitted_at":"2019-08-08T16:01:36Z","title":"Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity","version":1},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-08-14T14:29:00.564783Z"},"links":{"cited_paper":"/paper/1703.10303","citing_paper":"/paper/1908.03135"},"observation_digest":"sha256:821a180e51e1db717b0befa8855ab0d24eedc6c46ba8c48bd4e20257859102fd","observation_id":"1abeb706-30a9-41f4-bfa0-08e5d83eb5bc","resolution":{"observed_at":"2026-08-14T14:29:00.564783Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1904.01545","last_updated":"2019-04-02T16:59:54Z","snapshot_observed_at":"2026-08-14T16:52:51.320166Z","submitted_at":"2019-04-02T16:59:54Z","title":"Merger of compact stars in the two-families scenario","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1904.01545","snapshot_observed_at":"2026-08-14T14:29:00.568262Z","title":"Merger of Compact Stars in the Two-Families Scenario 2019","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"1908.03135","last_updated":"2019-08-08T16:01:36Z","snapshot_observed_at":"2026-08-14T14:20:29.928442Z","submitted_at":"2019-08-08T16:01:36Z","title":"Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity","version":1},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-08-14T14:29:00.568262Z"},"links":{"cited_paper":"/paper/1904.01545","citing_paper":"/paper/1908.03135"},"observation_digest":"sha256:8a24a8f7b9e07c5b860d88da3fe6af2315b4a5860b75c619876aa688d1c98634","observation_id":"4f696ca0-b121-497c-8e31-ba18b0ef6b41","resolution":{"observed_at":"2026-08-14T14:29:00.568262Z","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":"2026-08-14T14:29:00.571587Z","title":"Strange Matter","venue":null,"work_id":null,"year":1984},"citing_paper":{"arxiv_id":"1908.03135","last_updated":"2019-08-08T16:01:36Z","snapshot_observed_at":"2026-08-14T14:20:29.928442Z","submitted_at":"2019-08-08T16:01:36Z","title":"Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity","version":1},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-08-14T14:29:00.571587Z"},"links":{"citing_paper":"/paper/1908.03135"},"observation_digest":"sha256:9ce4d67b3741be514877d87362eeb603566143a165056cdab6158c2551a42a95","observation_id":"1fc70d1a-53ff-4e31-bc1c-173072dd244d","resolution":{"observed_at":"2026-08-14T14:29:00.571587Z","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":"2026-08-14T14:29:00.577484Z","title":"THE MIT BAG MODEL","venue":null,"work_id":null,"year":1979},"citing_paper":{"arxiv_id":"1908.03135","last_updated":"2019-08-08T16:01:36Z","snapshot_observed_at":"2026-08-14T14:20:29.928442Z","submitted_at":"2019-08-08T16:01:36Z","title":"Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity","version":1},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-08-14T14:29:00.577484Z"},"links":{"citing_paper":"/paper/1908.03135"},"observation_digest":"sha256:e711edb6bee010ec6b2c0e290d9f960814de46b20418a1870cc3a8e398fcef0a","observation_id":"527c7d77-1679-4a1a-b1e3-8b261fd3442e","resolution":{"observed_at":"2026-08-14T14:29:00.577484Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"nucl-th/0411016","last_updated":"2005-04-25T16:46:39Z","snapshot_observed_at":"2026-08-11T14:28:40.862173Z","submitted_at":"2004-11-04T00:26:21Z","title":"Hybrid stars that masquerade as neutron stars","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"nucl-th/0411016","snapshot_observed_at":"2026-08-14T14:29:00.580130Z","title":"Hybrid stars that masquerade as neutron stars","venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"1908.03135","last_updated":"2019-08-08T16:01:36Z","snapshot_observed_at":"2026-08-14T14:20:29.928442Z","submitted_at":"2019-08-08T16:01:36Z","title":"Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity","version":1},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-08-14T14:29:00.580130Z"},"links":{"cited_paper":"/paper/nucl-th/0411016","citing_paper":"/paper/1908.03135"},"observation_digest":"sha256:f49c238d12bb1d60406aa231ba2640d87437768887471d1cd57bd04a3dbbc08b","observation_id":"426669f8-d535-4aff-9526-dc1ff966b00a","resolution":{"observed_at":"2026-08-14T14:29:00.580130Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0709.4635","last_updated":"2008-01-21T08:57:17Z","snapshot_observed_at":"2026-07-06T01:34:39.570334Z","submitted_at":"2007-09-28T18:31:24Z","title":"Color superconductivity in dense quark matter","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0709.4635","snapshot_observed_at":"2026-08-14T14:29:00.583170Z","title":"Color superconductivity in dense quark matter","venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"1908.03135","last_updated":"2019-08-08T16:01:36Z","snapshot_observed_at":"2026-08-14T14:20:29.928442Z","submitted_at":"2019-08-08T16:01:36Z","title":"Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity","version":1},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-08-14T14:29:00.583170Z"},"links":{"cited_paper":"/paper/0709.4635","citing_paper":"/paper/1908.03135"},"observation_digest":"sha256:b57e542eed9ca6c76d7f50f3530a846cd09edb464c9158f90956267084b63141","observation_id":"79708474-f800-4e9e-a665-efcb364df4d5","resolution":{"observed_at":"2026-08-14T14:29:00.583170Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"hep-ph/0211070","last_updated":"2002-11-05T22:48:40Z","snapshot_observed_at":"2026-07-07T03:57:59.961222Z","submitted_at":"2002-11-05T22:48:40Z","title":"Color-flavor locked strange matter","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-ph/0211070","snapshot_observed_at":"2026-08-14T14:29:00.586141Z","title":"Color flavor locked strange matter","venue":null,"work_id":null,"year":2002},"citing_paper":{"arxiv_id":"1908.03135","last_updated":"2019-08-08T16:01:36Z","snapshot_observed_at":"2026-08-14T14:20:29.928442Z","submitted_at":"2019-08-08T16:01:36Z","title":"Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity","version":1},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-08-14T14:29:00.586141Z"},"links":{"cited_paper":"/paper/hep-ph/0211070","citing_paper":"/paper/1908.03135"},"observation_digest":"sha256:32f9a1a8a4b644e26af8643a48dcfde2dab8dabda4d1520c8035fecf57ddb23f","observation_id":"2f457fcf-e166-4712-9d11-6af92e94a16b","resolution":{"observed_at":"2026-08-14T14:29:00.586141Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"hep-ph/0101143","last_updated":"2001-01-14T19:19:21Z","snapshot_observed_at":"2026-08-14T07:29:35.250353Z","submitted_at":"2001-01-14T19:19:21Z","title":"Small, Dense Quark Stars from Perturbative QCD","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-ph/0101143","snapshot_observed_at":"2026-08-14T14:29:00.589505Z","title":"Small, dense quark stars from perturbative QCD","venue":null,"work_id":null,"year":2001},"citing_paper":{"arxiv_id":"1908.03135","last_updated":"2019-08-08T16:01:36Z","snapshot_observed_at":"2026-08-14T14:20:29.928442Z","submitted_at":"2019-08-08T16:01:36Z","title":"Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity","version":1},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-08-14T14:29:00.589505Z"},"links":{"cited_paper":"/paper/hep-ph/0101143","citing_paper":"/paper/1908.03135"},"observation_digest":"sha256:a023ef3d5eaba4727ba38dee9701fe86a7cff507066f160c684b85a7a7f5c76d","observation_id":"47686bc2-cd28-4364-b5b6-c19c06d6963b","resolution":{"observed_at":"2026-08-14T14:29:00.589505Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1503.07442","last_updated":"2015-03-25T16:14:16Z","snapshot_observed_at":"2026-08-06T23:30:11.638614Z","submitted_at":"2015-03-25T16:14:16Z","title":"Vector interaction enhanced bag model for astrophysical applications","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1503.07442","snapshot_observed_at":"2026-08-14T14:29:00.593057Z","title":"Vector interaction enhanced bag model for astrophysical applications","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"1908.03135","last_updated":"2019-08-08T16:01:36Z","snapshot_observed_at":"2026-08-14T14:20:29.928442Z","submitted_at":"2019-08-08T16:01:36Z","title":"Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity","version":1},"reference_index":54,"source":"pdf_text","source_observed_at":"2026-08-14T14:29:00.593057Z"},"links":{"cited_paper":"/paper/1503.07442","citing_paper":"/paper/1908.03135"},"observation_digest":"sha256:8fed49b2b1986188100382db6f253c6a7339964c592c707ea4c4e17e51eb9a5f","observation_id":"ca8d9c8e-2eb7-4440-9a3a-37bfed7ef14f","resolution":{"observed_at":"2026-08-14T14:29:00.593057Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1706.09371","last_updated":"2018-04-24T17:10:00Z","snapshot_observed_at":"2026-08-14T20:51:01.013404Z","submitted_at":"2017-06-28T17:21:15Z","title":"Phase transition effects on the dynamical stability of hybrid neutron stars","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1706.09371","snapshot_observed_at":"2026-08-14T14:29:00.596995Z","title":"Phase transition effects on the dynamical stability of hybrid neutron stars","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"1908.03135","last_updated":"2019-08-08T16:01:36Z","snapshot_observed_at":"2026-08-14T14:20:29.928442Z","submitted_at":"2019-08-08T16:01:36Z","title":"Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity","version":1},"reference_index":55,"source":"pdf_text","source_observed_at":"2026-08-14T14:29:00.596995Z"},"links":{"cited_paper":"/paper/1706.09371","citing_paper":"/paper/1908.03135"},"observation_digest":"sha256:86c9d0a31252933281ef6eb8b343100154083dfebeba0602eae968224f062924","observation_id":"212b9156-c50c-43bd-9da0-aa92afe666f5","resolution":{"observed_at":"2026-08-14T14:29:00.596995Z","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":"2026-08-14T14:29:00.600639Z","title":"Collapsed nuclei","venue":null,"work_id":null,"year":1971},"citing_paper":{"arxiv_id":"1908.03135","last_updated":"2019-08-08T16:01:36Z","snapshot_observed_at":"2026-08-14T14:20:29.928442Z","submitted_at":"2019-08-08T16:01:36Z","title":"Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity","version":1},"reference_index":56,"source":"pdf_text","source_observed_at":"2026-08-14T14:29:00.600639Z"},"links":{"citing_paper":"/paper/1908.03135"},"observation_digest":"sha256:d7fe51dc135655af4843c34b53b2a71450f748a353b27815b43df391787fec26","observation_id":"d99344e6-5cac-46dd-baab-c983c6ba66cd","resolution":{"observed_at":"2026-08-14T14:29:00.600639Z","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":"2026-08-14T14:29:00.604031Z","title":"Cosmic Separation of Phases","venue":null,"work_id":null,"year":1984},"citing_paper":{"arxiv_id":"1908.03135","last_updated":"2019-08-08T16:01:36Z","snapshot_observed_at":"2026-08-14T14:20:29.928442Z","submitted_at":"2019-08-08T16:01:36Z","title":"Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity","version":1},"reference_index":57,"source":"pdf_text","source_observed_at":"2026-08-14T14:29:00.604031Z"},"links":{"citing_paper":"/paper/1908.03135"},"observation_digest":"sha256:ffd54409c6b6d5268707df813f55c868043886a52b8bbecb46d85d784dbe4402","observation_id":"a38e1a00-34d1-4781-a077-5a9e1322dea7","resolution":{"observed_at":"2026-08-14T14:29:00.604031Z","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":"2026-08-14T14:29:00.607280Z","title":"Compact Stars: Nuclear Physics, Particle Physics, and General Relativity, 2 ed.; Springer: The address, 2000","venue":null,"work_id":null,"year":2000},"citing_paper":{"arxiv_id":"1908.03135","last_updated":"2019-08-08T16:01:36Z","snapshot_observed_at":"2026-08-14T14:20:29.928442Z","submitted_at":"2019-08-08T16:01:36Z","title":"Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity","version":1},"reference_index":58,"source":"pdf_text","source_observed_at":"2026-08-14T14:29:00.607280Z"},"links":{"citing_paper":"/paper/1908.03135"},"observation_digest":"sha256:6bce03706cb5ceda9aeb97277d9f468af8baaaa6884e58fc65f65d20d0d70a82","observation_id":"a1ad622e-3624-409f-a323-edd756a7ea15","resolution":{"observed_at":"2026-08-14T14:29:00.607280Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1308.1452","last_updated":"2013-10-14T17:35:36Z","snapshot_observed_at":"2026-07-06T03:20:09.687356Z","submitted_at":"2013-08-07T00:37:24Z","title":"Surface tension and curvature energy of quark matter in the NJL model","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1308.1452","snapshot_observed_at":"2026-08-14T14:29:00.610565Z","title":"Surface tension and curvature energy of quark matter in the Nambu-Jona-Lasinio model","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"1908.03135","last_updated":"2019-08-08T16:01:36Z","snapshot_observed_at":"2026-08-14T14:20:29.928442Z","submitted_at":"2019-08-08T16:01:36Z","title":"Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity","version":1},"reference_index":59,"source":"pdf_text","source_observed_at":"2026-08-14T14:29:00.610565Z"},"links":{"cited_paper":"/paper/1308.1452","citing_paper":"/paper/1908.03135"},"observation_digest":"sha256:9a3788cfff4f70e94a8b3f9835f79dfba1199c3b582b45082f4f61374e4a971f","observation_id":"46e8a920-112a-4f0b-b6bc-923689a01104","resolution":{"observed_at":"2026-08-14T14:29:00.610565Z","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":"2026-08-14T14:29:00.614229Z","title":"Dynamical Model of Elementary Particles Based on an Analogy with Superconductivity","venue":null,"work_id":null,"year":1961},"citing_paper":{"arxiv_id":"1908.03135","last_updated":"2019-08-08T16:01:36Z","snapshot_observed_at":"2026-08-14T14:20:29.928442Z","submitted_at":"2019-08-08T16:01:36Z","title":"Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity","version":1},"reference_index":60,"source":"pdf_text","source_observed_at":"2026-08-14T14:29:00.614229Z"},"links":{"citing_paper":"/paper/1908.03135"},"observation_digest":"sha256:6a22bbf3ae906412161747e2a93a39ae26efd818646f5bf0960a9a19c38fec6d","observation_id":"db1ef07b-80f7-4b05-8d23-8ecb3a5f6c8f","resolution":{"observed_at":"2026-08-14T14:29:00.614229Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0111092","last_updated":"2001-11-12T11:28:05Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2001-11-05T17:05:33Z","title":"A unified equation of state of dense matter and neutron star structure","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0111092","snapshot_observed_at":"2026-08-14T14:29:00.617794Z","title":"A unified equation of state of dense matter and neutron star structure","venue":null,"work_id":null,"year":2001},"citing_paper":{"arxiv_id":"1908.03135","last_updated":"2019-08-08T16:01:36Z","snapshot_observed_at":"2026-08-14T14:20:29.928442Z","submitted_at":"2019-08-08T16:01:36Z","title":"Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity","version":1},"reference_index":61,"source":"pdf_text","source_observed_at":"2026-08-14T14:29:00.617794Z"},"links":{"cited_paper":"/paper/astro-ph/0111092","citing_paper":"/paper/1908.03135"},"observation_digest":"sha256:8c40fdb77e3b94257f506a6a73dc280503d67b474d428f9c2fb7312acad16878","observation_id":"63c07bd6-5511-4ec7-97f9-c0dd3eb6c87f","resolution":{"observed_at":"2026-08-14T14:29:00.617794Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/0610128","last_updated":"2006-10-26T17:23:13Z","snapshot_observed_at":"2026-07-07T03:23:14.583543Z","submitted_at":"2006-10-26T17:23:13Z","title":"Calibration of Moving Puncture Simulations","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"gr-qc/0610128","snapshot_observed_at":"2026-08-14T14:29:00.621281Z","title":"Calibration of Moving Puncture Simulations","venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"1908.03135","last_updated":"2019-08-08T16:01:36Z","snapshot_observed_at":"2026-08-14T14:20:29.928442Z","submitted_at":"2019-08-08T16:01:36Z","title":"Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity","version":1},"reference_index":62,"source":"pdf_text","source_observed_at":"2026-08-14T14:29:00.621281Z"},"links":{"cited_paper":"/paper/gr-qc/0610128","citing_paper":"/paper/1908.03135"},"observation_digest":"sha256:16d25a63a9a54ce942bdcc9c648fe4a326be74fd325adbc2ce28bbdc59628713","observation_id":"ee98d37e-0c58-4763-9ed9-9b3039bbffc0","resolution":{"observed_at":"2026-08-14T14:29:00.621281Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1104.4751","last_updated":"2011-08-11T09:46:12Z","snapshot_observed_at":"2026-08-10T14:54:20.028364Z","submitted_at":"2011-04-25T16:51:36Z","title":"Numerical relativity simulations of binary neutron stars","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1104.4751","snapshot_observed_at":"2026-08-14T14:29:00.625103Z","title":"Numerical relativity simulations of binary neutron stars","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"1908.03135","last_updated":"2019-08-08T16:01:36Z","snapshot_observed_at":"2026-08-14T14:20:29.928442Z","submitted_at":"2019-08-08T16:01:36Z","title":"Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity","version":1},"reference_index":63,"source":"pdf_text","source_observed_at":"2026-08-14T14:29:00.625103Z"},"links":{"cited_paper":"/paper/1104.4751","citing_paper":"/paper/1908.03135"},"observation_digest":"sha256:2a18b86b3a2986993a61be212ab3b83f832d1982813e327c728c5d5d6d97d94e","observation_id":"b4909ae5-51e7-4c33-89c5-557fc8174454","resolution":{"observed_at":"2026-08-14T14:29:00.625103Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1504.01266","last_updated":"2015-04-06T11:34:31Z","snapshot_observed_at":"2026-08-10T08:49:28.194106Z","submitted_at":"2015-04-06T11:34:31Z","title":"Numerical relativity simulations of neutron star merger remnants using conservative mesh refinement","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1504.01266","snapshot_observed_at":"2026-08-14T14:29:00.629131Z","title":"Numerical relativity simulations of neutron star merger remnants using conservative mesh refinement","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"1908.03135","last_updated":"2019-08-08T16:01:36Z","snapshot_observed_at":"2026-08-14T14:20:29.928442Z","submitted_at":"2019-08-08T16:01:36Z","title":"Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity","version":1},"reference_index":64,"source":"pdf_text","source_observed_at":"2026-08-14T14:29:00.629131Z"},"links":{"cited_paper":"/paper/1504.01266","citing_paper":"/paper/1908.03135"},"observation_digest":"sha256:7d3f08407ce9b85547f7cd7b08f51725a4ce2c4d80b9623de0501f5dd2481543","observation_id":"5189230f-4b48-4937-ab44-79bc23b5a12d","resolution":{"observed_at":"2026-08-14T14:29:00.629131Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1604.07999","last_updated":"2016-09-19T08:43:56Z","snapshot_observed_at":"2026-08-14T21:59:54.444643Z","submitted_at":"2016-04-27T09:48:15Z","title":"Gravitational waveforms from binary neutron star mergers with high-order WENO schemes in numerical relativity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1604.07999","snapshot_observed_at":"2026-08-14T14:29:00.632873Z","title":"Gravitational waveforms from binary neutron star mergers with high-order weighted-essentially-nonoscillatory schemes in numerical relativity","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"1908.03135","last_updated":"2019-08-08T16:01:36Z","snapshot_observed_at":"2026-08-14T14:20:29.928442Z","submitted_at":"2019-08-08T16:01:36Z","title":"Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity","version":1},"reference_index":65,"source":"pdf_text","source_observed_at":"2026-08-14T14:29:00.632873Z"},"links":{"cited_paper":"/paper/1604.07999","citing_paper":"/paper/1908.03135"},"observation_digest":"sha256:03fecff3681129d55036ed7c0dca8013c23aa63ef721d5baf46dc7b5d0354212","observation_id":"cc7b9e0d-5153-42de-86a1-31bd5e4a738f","resolution":{"observed_at":"2026-08-14T14:29:00.632873Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0908.0620","last_updated":"2009-08-05T08:53:41Z","snapshot_observed_at":"2026-08-12T09:44:33.645961Z","submitted_at":"2009-08-05T08:53:41Z","title":"A new numerical method to construct binary neutron star initial data","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0908.0620","snapshot_observed_at":"2026-08-14T14:29:00.636564Z","title":"A New numerical method to construct binary neutron star initial data","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"1908.03135","last_updated":"2019-08-08T16:01:36Z","snapshot_observed_at":"2026-08-14T14:20:29.928442Z","submitted_at":"2019-08-08T16:01:36Z","title":"Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity","version":1},"reference_index":66,"source":"pdf_text","source_observed_at":"2026-08-14T14:29:00.636564Z"},"links":{"cited_paper":"/paper/0908.0620","citing_paper":"/paper/1908.03135"},"observation_digest":"sha256:5264f978e708adc29358831fecc8279bb4620731df03596a7448914c27f1f8ad","observation_id":"70cc7c76-be20-4ce0-abb7-b586a0968d31","resolution":{"observed_at":"2026-08-14T14:29:00.636564Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0812.2163","last_updated":"2008-12-11T14:59:23Z","snapshot_observed_at":"2026-07-06T01:47:44.956336Z","submitted_at":"2008-12-11T14:59:23Z","title":"Constraints on a phenomenologically parameterized neutron-star equation of state","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0812.2163","snapshot_observed_at":"2026-08-14T14:29:00.640184Z","title":"Constraints on a phenomenologically parameterized neutron-star equation of state","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"1908.03135","last_updated":"2019-08-08T16:01:36Z","snapshot_observed_at":"2026-08-14T14:20:29.928442Z","submitted_at":"2019-08-08T16:01:36Z","title":"Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity","version":1},"reference_index":67,"source":"pdf_text","source_observed_at":"2026-08-14T14:29:00.640184Z"},"links":{"cited_paper":"/paper/0812.2163","citing_paper":"/paper/1908.03135"},"observation_digest":"sha256:004d6119e48d4302e5addc69a56c153e8b8013e98a1d11d6dde7bf9662409e4b","observation_id":"9803830c-389b-402c-ba28-ce424dff83d6","resolution":{"observed_at":"2026-08-14T14:29:00.640184Z","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":"2026-08-14T14:29:00.643875Z","title":"Instabilities in Close Neutron Star Binaries","venue":null,"work_id":null,"year":1995},"citing_paper":{"arxiv_id":"1908.03135","last_updated":"2019-08-08T16:01:36Z","snapshot_observed_at":"2026-08-14T14:20:29.928442Z","submitted_at":"2019-08-08T16:01:36Z","title":"Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity","version":1},"reference_index":68,"source":"pdf_text","source_observed_at":"2026-08-14T14:29:00.643875Z"},"links":{"citing_paper":"/paper/1908.03135"},"observation_digest":"sha256:90cfdb30e2ee44148e71d574c6a348ac7707efca91937c58f309434c30f6bd2d","observation_id":"79c32faa-966a-4d3e-957a-53301899d8eb","resolution":{"observed_at":"2026-08-14T14:29:00.643875Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/9601017","last_updated":"1996-03-04T22:51:17Z","snapshot_observed_at":"2026-08-07T21:25:58.817733Z","submitted_at":"1996-01-10T23:28:20Z","title":"Relativistic Numerical Method for Close Neutron Star Binaries","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"gr-qc/9601017","snapshot_observed_at":"2026-08-14T14:29:00.647422Z","title":"Relativistic numerical model for close neutron star binaries.Phys","venue":null,"work_id":null,"year":1996},"citing_paper":{"arxiv_id":"1908.03135","last_updated":"2019-08-08T16:01:36Z","snapshot_observed_at":"2026-08-14T14:20:29.928442Z","submitted_at":"2019-08-08T16:01:36Z","title":"Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity","version":1},"reference_index":69,"source":"pdf_text","source_observed_at":"2026-08-14T14:29:00.647422Z"},"links":{"cited_paper":"/paper/gr-qc/9601017","citing_paper":"/paper/1908.03135"},"observation_digest":"sha256:870951f297c886a275d7f387e5be7378499ac03983e72a088c1f07dd3107c1f3","observation_id":"a8974c3c-767f-4130-842a-8328794939f5","resolution":{"observed_at":"2026-08-14T14:29:00.647422Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/9810051","last_updated":"1998-12-23T16:22:06Z","snapshot_observed_at":"2026-07-07T03:29:36.497216Z","submitted_at":"1998-10-15T18:36:24Z","title":"Conformal ``thin sandwich'' data for the initial-value problem of general relativity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"gr-qc/9810051","snapshot_observed_at":"2026-08-14T14:29:00.651039Z","title":"Conformal ’thin sandwich’ data for the initial-value problem.Phys","venue":null,"work_id":null,"year":1999},"citing_paper":{"arxiv_id":"1908.03135","last_updated":"2019-08-08T16:01:36Z","snapshot_observed_at":"2026-08-14T14:20:29.928442Z","submitted_at":"2019-08-08T16:01:36Z","title":"Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity","version":1},"reference_index":70,"source":"pdf_text","source_observed_at":"2026-08-14T14:29:00.651039Z"},"links":{"cited_paper":"/paper/gr-qc/9810051","citing_paper":"/paper/1908.03135"},"observation_digest":"sha256:bc112daedb733f44039fc13e51d4cb9c2b1ebab25ce752dca63a463183415c0f","observation_id":"434c7d95-50e9-45f2-9c15-81fb64154a89","resolution":{"observed_at":"2026-08-14T14:29:00.651039Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1209.5336","last_updated":"2014-11-04T18:16:11Z","snapshot_observed_at":"2026-07-06T02:56:12.187611Z","submitted_at":"2012-09-24T17:00:50Z","title":"Constructing quasi-equilibrium initial data for binary neutron stars with arbitrary spins","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1209.5336","snapshot_observed_at":"2026-08-14T14:29:00.654372Z","title":"Constructing quasi-equilibrium initial data for binary neutron stars with arbitrary spins","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"1908.03135","last_updated":"2019-08-08T16:01:36Z","snapshot_observed_at":"2026-08-14T14:20:29.928442Z","submitted_at":"2019-08-08T16:01:36Z","title":"Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity","version":1},"reference_index":71,"source":"pdf_text","source_observed_at":"2026-08-14T14:29:00.654372Z"},"links":{"cited_paper":"/paper/1209.5336","citing_paper":"/paper/1908.03135"},"observation_digest":"sha256:37d9fc03a2980a3493cb3fbc712ec47aa4dc252e1b61483e8cb6d74ab3b7100d","observation_id":"8c0cd0c8-a024-4988-a9d7-3d98d4c3f99d","resolution":{"observed_at":"2026-08-14T14:29:00.654372Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1507.07100","last_updated":"2015-07-25T13:24:10Z","snapshot_observed_at":"2026-07-06T04:24:52.856912Z","submitted_at":"2015-07-25T13:24:10Z","title":"Binary Neutron Stars with Generic Spin, Eccentricity, Mass ratio, and Compactness - Quasi-equilibrium Sequences and First Evolutions","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1507.07100","snapshot_observed_at":"2026-08-14T14:29:00.657377Z","title":"Binary Neutron Stars with Generic Spin, Eccentricity, Mass ratio, and Compactness - Quasi-equilibrium Sequences and First Evolutions","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"1908.03135","last_updated":"2019-08-08T16:01:36Z","snapshot_observed_at":"2026-08-14T14:20:29.928442Z","submitted_at":"2019-08-08T16:01:36Z","title":"Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity","version":1},"reference_index":72,"source":"pdf_text","source_observed_at":"2026-08-14T14:29:00.657377Z"},"links":{"cited_paper":"/paper/1507.07100","citing_paper":"/paper/1908.03135"},"observation_digest":"sha256:f0091bccb49798dc9dcb8ad7308f81e4a04ffdb0dbfe6cf0c1db82747cf26e78","observation_id":"450d40d3-9e32-476f-8c42-266d984df0fd","resolution":{"observed_at":"2026-08-14T14:29:00.657377Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1408.4136","last_updated":"2014-10-30T10:18:19Z","snapshot_observed_at":"2026-07-06T03:52:00.062001Z","submitted_at":"2014-08-18T20:01:19Z","title":"Initial data for binary neutron stars with adjustable eccentricity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1408.4136","snapshot_observed_at":"2026-08-14T14:29:00.660614Z","title":"Initial data for binary neutron stars with adjustable eccentricity","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"1908.03135","last_updated":"2019-08-08T16:01:36Z","snapshot_observed_at":"2026-08-14T14:20:29.928442Z","submitted_at":"2019-08-08T16:01:36Z","title":"Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity","version":1},"reference_index":73,"source":"pdf_text","source_observed_at":"2026-08-14T14:29:00.660614Z"},"links":{"cited_paper":"/paper/1408.4136","citing_paper":"/paper/1908.03135"},"observation_digest":"sha256:62a06a4ca217f1720b2fbec11fa9d7b1cd016abf5a6a5f47f990b0ed1b500dc4","observation_id":"448e2a16-6501-4389-92bb-a3e8689e05b6","resolution":{"observed_at":"2026-08-14T14:29:00.660614Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1405.6207","last_updated":"2014-09-03T19:35:37Z","snapshot_observed_at":"2026-08-05T11:56:50.383128Z","submitted_at":"2014-05-23T20:00:11Z","title":"Reducing orbital eccentricity in initial data of binary neutron stars","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1405.6207","snapshot_observed_at":"2026-08-14T14:29:00.664072Z","title":"Reducing orbital eccentricity in initial data of binary neutron stars","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"1908.03135","last_updated":"2019-08-08T16:01:36Z","snapshot_observed_at":"2026-08-14T14:20:29.928442Z","submitted_at":"2019-08-08T16:01:36Z","title":"Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity","version":1},"reference_index":74,"source":"pdf_text","source_observed_at":"2026-08-14T14:29:00.664072Z"},"links":{"cited_paper":"/paper/1405.6207","citing_paper":"/paper/1908.03135"},"observation_digest":"sha256:07c4a2d7b0a0e40f9f124e84c9ac157fa08f6b3ae1793a3edf4c1c0e5f4f288c","observation_id":"6deae75e-58b1-4f60-a1c1-65646068e897","resolution":{"observed_at":"2026-08-14T14:29:00.664072Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0912.2920","last_updated":"2010-04-27T16:38:50Z","snapshot_observed_at":"2026-07-06T02:04:43.515736Z","submitted_at":"2009-12-15T15:12:17Z","title":"Constraint violation in free evolution schemes: comparing BSSNOK with a conformal decomposition of Z4","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0912.2920","snapshot_observed_at":"2026-08-14T14:29:00.667625Z","title":"Constraint violation in free evolution schemes: Comparing BSSNOK with a conformal decomposition of Z4","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"1908.03135","last_updated":"2019-08-08T16:01:36Z","snapshot_observed_at":"2026-08-14T14:20:29.928442Z","submitted_at":"2019-08-08T16:01:36Z","title":"Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity","version":1},"reference_index":75,"source":"pdf_text","source_observed_at":"2026-08-14T14:29:00.667625Z"},"links":{"cited_paper":"/paper/0912.2920","citing_paper":"/paper/1908.03135"},"observation_digest":"sha256:90c4fe729ea77d198d263950b509733ae4de34fa8297c4b4da6a96a4d2af727e","observation_id":"f91efdd9-c18a-4596-b6bf-f6b7298bd7ef","resolution":{"observed_at":"2026-08-14T14:29:00.667625Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1107.5539","last_updated":"2012-02-20T10:28:35Z","snapshot_observed_at":"2026-08-08T19:46:08.712096Z","submitted_at":"2011-07-27T17:04:03Z","title":"Constraint damping for the Z4c formulation of general relativity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1107.5539","snapshot_observed_at":"2026-08-14T14:29:00.671104Z","title":"Constraint damping for the Z4c formulation of general relativity","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"1908.03135","last_updated":"2019-08-08T16:01:36Z","snapshot_observed_at":"2026-08-14T14:20:29.928442Z","submitted_at":"2019-08-08T16:01:36Z","title":"Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity","version":1},"reference_index":76,"source":"pdf_text","source_observed_at":"2026-08-14T14:29:00.671104Z"},"links":{"cited_paper":"/paper/1107.5539","citing_paper":"/paper/1908.03135"},"observation_digest":"sha256:76de36d3f06b516289155a358d2922db33547cd30a7ac539902fe89dde372d3b","observation_id":"ca1d5a7e-ef81-48ba-abca-4d416080b144","resolution":{"observed_at":"2026-08-14T14:29:00.671104Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1212.2901","last_updated":"2012-12-12T17:44:15Z","snapshot_observed_at":"2026-07-06T03:01:52.564460Z","submitted_at":"2012-12-12T17:44:15Z","title":"Compact binary evolutions with the Z4c formulation","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1212.2901","snapshot_observed_at":"2026-08-14T14:29:00.674397Z","title":"Compact binary evolutions with the Z4c formulation","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"1908.03135","last_updated":"2019-08-08T16:01:36Z","snapshot_observed_at":"2026-08-14T14:20:29.928442Z","submitted_at":"2019-08-08T16:01:36Z","title":"Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity","version":1},"reference_index":77,"source":"pdf_text","source_observed_at":"2026-08-14T14:29:00.674397Z"},"links":{"cited_paper":"/paper/1212.2901","citing_paper":"/paper/1908.03135"},"observation_digest":"sha256:8764c5168ed779825e6b1733b41845f8612ecd6025b145606b65f93ee8f91893","observation_id":"dc5cb1c0-718e-4f17-a279-20ad711dcc86","resolution":{"observed_at":"2026-08-14T14:29:00.674397Z","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":"2026-08-14T14:29:00.677766Z","title":"An improved weighted essentially non-oscillatory scheme for hyperbolic conservation laws","venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"1908.03135","last_updated":"2019-08-08T16:01:36Z","snapshot_observed_at":"2026-08-14T14:20:29.928442Z","submitted_at":"2019-08-08T16:01:36Z","title":"Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity","version":1},"reference_index":78,"source":"pdf_text","source_observed_at":"2026-08-14T14:29:00.677766Z"},"links":{"citing_paper":"/paper/1908.03135"},"observation_digest":"sha256:8d05ca2d797e57b317744aa24e31a0644641f2bf09aef0f98f0a9dfd73d44cec","observation_id":"94eec824-d38a-4fcf-b9ba-782729f651c9","resolution":{"observed_at":"2026-08-14T14:29:00.677766Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1803.07965","last_updated":"2018-03-21T15:28:55Z","snapshot_observed_at":"2026-08-14T19:33:56.034244Z","submitted_at":"2018-03-21T15:28:55Z","title":"High-resolution numerical relativity simulations of spinning binary neutron star mergers","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1803.07965","snapshot_observed_at":"2026-08-14T14:29:00.681307Z","title":"High-resolution numerical relativity simulations of spinning binary neutron star mergers","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"1908.03135","last_updated":"2019-08-08T16:01:36Z","snapshot_observed_at":"2026-08-14T14:20:29.928442Z","submitted_at":"2019-08-08T16:01:36Z","title":"Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity","version":1},"reference_index":79,"source":"pdf_text","source_observed_at":"2026-08-14T14:29:00.681307Z"},"links":{"cited_paper":"/paper/1803.07965","citing_paper":"/paper/1908.03135"},"observation_digest":"sha256:aef1232a997bb70adf5900147d70ab4ddeaa72c19c0194e4f50aee947c0e4fd8","observation_id":"f8b90ebc-f798-4afa-bf47-78a0daee5a1a","resolution":{"observed_at":"2026-08-14T14:29:00.681307Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1204.3858","last_updated":"2012-04-17T17:54:35Z","snapshot_observed_at":"2026-08-06T22:36:26.327514Z","submitted_at":"2012-04-17T17:54:35Z","title":"Binary Neutron Star Mergers","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1204.3858","snapshot_observed_at":"2026-08-14T14:29:00.684905Z","title":"Binary Neutron Star Mergers","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"1908.03135","last_updated":"2019-08-08T16:01:36Z","snapshot_observed_at":"2026-08-14T14:20:29.928442Z","submitted_at":"2019-08-08T16:01:36Z","title":"Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity","version":1},"reference_index":80,"source":"pdf_text","source_observed_at":"2026-08-14T14:29:00.684905Z"},"links":{"cited_paper":"/paper/1204.3858","citing_paper":"/paper/1908.03135"},"observation_digest":"sha256:1c60660bb6048759e490e8c841fd9f6685b56fb26a0e9fa32bd2ecf14b3f92ff","observation_id":"68217d01-c142-476a-b132-8d25232dbaff","resolution":{"observed_at":"2026-08-14T14:29:00.684905Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1804.02235","last_updated":"2018-04-06T12:37:24Z","snapshot_observed_at":"2026-08-14T19:28:35.939152Z","submitted_at":"2018-04-06T12:37:24Z","title":"Matter imprints in waveform models for neutron star binaries: tidal and self-spin effects","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1804.02235","snapshot_observed_at":"2026-08-14T14:29:00.688693Z","title":"Matter imprints in waveform models for neutron star binaries: Tidal and self-spin effects","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"1908.03135","last_updated":"2019-08-08T16:01:36Z","snapshot_observed_at":"2026-08-14T14:20:29.928442Z","submitted_at":"2019-08-08T16:01:36Z","title":"Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity","version":1},"reference_index":81,"source":"pdf_text","source_observed_at":"2026-08-14T14:29:00.688693Z"},"links":{"cited_paper":"/paper/1804.02235","citing_paper":"/paper/1908.03135"},"observation_digest":"sha256:ecf3798bd3b0f77ad7b36d8a50af7ff223d797cd85a53bf0ac12a9ea83675767","observation_id":"69328b24-54e3-4d40-8558-8f5f9ea5fdec","resolution":{"observed_at":"2026-08-14T14:29:00.688693Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1607.06636","last_updated":"2016-07-22T11:26:39Z","snapshot_observed_at":"2026-08-14T21:47:16.679371Z","submitted_at":"2016-07-22T11:26:39Z","title":"Gravitational waves and mass ejecta from binary neutron star mergers: Effect of the mass-ratio","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1607.06636","snapshot_observed_at":"2026-08-14T14:29:00.692652Z","title":"Gravitational waves and mass ejecta from binary neutron star mergers: Effect of the mass-ratio","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"1908.03135","last_updated":"2019-08-08T16:01:36Z","snapshot_observed_at":"2026-08-14T14:20:29.928442Z","submitted_at":"2019-08-08T16:01:36Z","title":"Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity","version":1},"reference_index":82,"source":"pdf_text","source_observed_at":"2026-08-14T14:29:00.692652Z"},"links":{"cited_paper":"/paper/1607.06636","citing_paper":"/paper/1908.03135"},"observation_digest":"sha256:d70ad60d9fa65042b5d7a9d0b18bae38a2ba3db899a9cd81e2edfb123aad9459","observation_id":"4ce158b7-af08-4a35-9f23-b02c0b8c6aba","resolution":{"observed_at":"2026-08-14T14:29:00.692652Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1611.07367","last_updated":"2016-11-22T15:36:46Z","snapshot_observed_at":"2026-08-14T21:29:10.718696Z","submitted_at":"2016-11-22T15:36:46Z","title":"Gravitational waves and mass ejecta from binary neutron star mergers: Effect of the stars' rotation","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1611.07367","snapshot_observed_at":"2026-08-14T14:29:00.696434Z","title":"Gravitational waves and mass ejecta from binary neutron star mergers: Effect of the stars’ rotation","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"1908.03135","last_updated":"2019-08-08T16:01:36Z","snapshot_observed_at":"2026-08-14T14:20:29.928442Z","submitted_at":"2019-08-08T16:01:36Z","title":"Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity","version":1},"reference_index":83,"source":"pdf_text","source_observed_at":"2026-08-14T14:29:00.696434Z"},"links":{"cited_paper":"/paper/1611.07367","citing_paper":"/paper/1908.03135"},"observation_digest":"sha256:39615eb599def9411ff51510bf7fe2d6e763b20d7159bb85d53190f883044b00","observation_id":"8c17c92c-73e6-49ed-8a86-e2fdb1e957ff","resolution":{"observed_at":"2026-08-14T14:29:00.696434Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1308.3271","last_updated":"2014-09-19T12:19:21Z","snapshot_observed_at":"2026-07-31T09:27:13.454528Z","submitted_at":"2013-08-14T22:45:26Z","title":"A simple model of complete precessing black-hole-binary gravitational waveforms","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1308.3271","snapshot_observed_at":"2026-08-14T14:29:00.700319Z","title":"Simple Model of Complete Precessing Black-Hole-Binary Gravitational Waveforms","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"1908.03135","last_updated":"2019-08-08T16:01:36Z","snapshot_observed_at":"2026-08-14T14:20:29.928442Z","submitted_at":"2019-08-08T16:01:36Z","title":"Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity","version":1},"reference_index":84,"source":"pdf_text","source_observed_at":"2026-08-14T14:29:00.700319Z"},"links":{"cited_paper":"/paper/1308.3271","citing_paper":"/paper/1908.03135"},"observation_digest":"sha256:f78f3c3b90d014b4b901c009d496c9024e9c1e71e7daed1a78f8ac13e166484e","observation_id":"b3fe394d-bd46-4b1d-b837-a981f22bc360","resolution":{"observed_at":"2026-08-14T14:29:00.700319Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1811.00364","last_updated":"2019-07-29T15:54:28Z","snapshot_observed_at":"2026-08-14T18:05:45.935830Z","submitted_at":"2018-11-01T13:23:52Z","title":"Tests of General Relativity with GW170817","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1811.00364","snapshot_observed_at":"2026-08-14T14:29:00.704071Z","title":"Tests of General Relativity with GW170817 2018","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"1908.03135","last_updated":"2019-08-08T16:01:36Z","snapshot_observed_at":"2026-08-14T14:20:29.928442Z","submitted_at":"2019-08-08T16:01:36Z","title":"Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity","version":1},"reference_index":85,"source":"pdf_text","source_observed_at":"2026-08-14T14:29:00.704071Z"},"links":{"cited_paper":"/paper/1811.00364","citing_paper":"/paper/1908.03135"},"observation_digest":"sha256:a55a7acccf0f2f35f417e43a9571d7bb5fc9c5d39f54e87e35e23078b0093ef8","observation_id":"f4d7507e-bc05-4efe-b3aa-85a6e48fa51f","resolution":{"observed_at":"2026-08-14T14:29:00.704071Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1403.5672","last_updated":"2014-08-21T11:59:24Z","snapshot_observed_at":"2026-07-06T03:39:10.785048Z","submitted_at":"2014-03-22T15:13:32Z","title":"Constraining the Equation of State of Neutron Stars from Binary Mergers","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1403.5672","snapshot_observed_at":"2026-08-14T14:29:00.707369Z","title":"Constraining the Equation of State of Neutron Stars from Binary Mergers","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"1908.03135","last_updated":"2019-08-08T16:01:36Z","snapshot_observed_at":"2026-08-14T14:20:29.928442Z","submitted_at":"2019-08-08T16:01:36Z","title":"Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity","version":1},"reference_index":86,"source":"pdf_text","source_observed_at":"2026-08-14T14:29:00.707369Z"},"links":{"cited_paper":"/paper/1403.5672","citing_paper":"/paper/1908.03135"},"observation_digest":"sha256:0a397fca186f36318d556f999a433a2b09b0765086e997eb537eb12a9610509a","observation_id":"d0de0b5d-d400-4081-86ef-0abc49111522","resolution":{"observed_at":"2026-08-14T14:29:00.707369Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1412.3240","last_updated":"2015-03-06T16:30:59Z","snapshot_observed_at":"2026-08-03T23:03:20.003241Z","submitted_at":"2014-12-10T09:54:23Z","title":"Spectral properties of the post-merger gravitational-wave signal from binary neutron stars","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1412.3240","snapshot_observed_at":"2026-08-14T14:29:00.711795Z","title":"Spectral properties of the post-merger gravitational-wave signal from binary neutron stars","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"1908.03135","last_updated":"2019-08-08T16:01:36Z","snapshot_observed_at":"2026-08-14T14:20:29.928442Z","submitted_at":"2019-08-08T16:01:36Z","title":"Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity","version":1},"reference_index":87,"source":"pdf_text","source_observed_at":"2026-08-14T14:29:00.711795Z"},"links":{"cited_paper":"/paper/1412.3240","citing_paper":"/paper/1908.03135"},"observation_digest":"sha256:98a68080ccd1d163a74a538cb65124668103d1030726e42d57e34e44950ea5d5","observation_id":"1d11bb47-d7ce-4df9-8e7f-3f303a8b7799","resolution":{"observed_at":"2026-08-14T14:29:00.711795Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1604.00246","last_updated":"2016-06-01T08:27:21Z","snapshot_observed_at":"2026-08-14T22:03:28.880188Z","submitted_at":"2016-04-01T13:55:19Z","title":"Gravitational-wave signal from binary neutron stars: a systematic analysis of the spectral properties","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1604.00246","snapshot_observed_at":"2026-08-14T14:29:00.715538Z","title":"Gravitational-wave signal from binary neutron stars: a systematic analysis of the spectral properties","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"1908.03135","last_updated":"2019-08-08T16:01:36Z","snapshot_observed_at":"2026-08-14T14:20:29.928442Z","submitted_at":"2019-08-08T16:01:36Z","title":"Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity","version":1},"reference_index":88,"source":"pdf_text","source_observed_at":"2026-08-14T14:29:00.715538Z"},"links":{"cited_paper":"/paper/1604.00246","citing_paper":"/paper/1908.03135"},"observation_digest":"sha256:e1910bfba3fa10b2d0684b546c3bbf46891fa20a223cc4c8af4c82275d05d301","observation_id":"ab513a6b-01e4-4b25-858b-5d99fb613ab5","resolution":{"observed_at":"2026-08-14T14:29:00.715538Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1106.1616","last_updated":"2011-11-23T09:18:38Z","snapshot_observed_at":"2026-07-06T02:29:00.735517Z","submitted_at":"2011-06-08T18:30:14Z","title":"Measuring neutron-star properties via gravitational waves from binary mergers","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1106.1616","snapshot_observed_at":"2026-08-14T14:29:00.718676Z","title":"Measuring neutron-star properties via gravitational waves from binary mergers","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"1908.03135","last_updated":"2019-08-08T16:01:36Z","snapshot_observed_at":"2026-08-14T14:20:29.928442Z","submitted_at":"2019-08-08T16:01:36Z","title":"Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity","version":1},"reference_index":89,"source":"pdf_text","source_observed_at":"2026-08-14T14:29:00.718676Z"},"links":{"cited_paper":"/paper/1106.1616","citing_paper":"/paper/1908.03135"},"observation_digest":"sha256:682e142a243b29d0f4dccbd0a714db6aa0335d0d3d2c6abffba62eeb440acfb6","observation_id":"b1e06f7f-6b7b-4353-8d43-96c010daf295","resolution":{"observed_at":"2026-08-14T14:29:00.718676Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1105.0368","last_updated":"2011-05-02T15:54:35Z","snapshot_observed_at":"2026-07-06T02:27:06.972090Z","submitted_at":"2011-05-02T15:54:35Z","title":"Gravitational waves and nonaxisymmetric oscillation modes in mergers of compact object binaries","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1105.0368","snapshot_observed_at":"2026-08-14T14:29:00.721742Z","title":"Gravitational waves and nonaxisymmetric oscillation modes in mergers of compact object binaries.Mon","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"1908.03135","last_updated":"2019-08-08T16:01:36Z","snapshot_observed_at":"2026-08-14T14:20:29.928442Z","submitted_at":"2019-08-08T16:01:36Z","title":"Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity","version":1},"reference_index":90,"source":"pdf_text","source_observed_at":"2026-08-14T14:29:00.721742Z"},"links":{"cited_paper":"/paper/1105.0368","citing_paper":"/paper/1908.03135"},"observation_digest":"sha256:ff159deeb4cac7b080e2cb7cdba22588de8bd64f4e893768904ce4eb45b7a7dc","observation_id":"191e3292-61bf-4258-b3b3-e8c941688160","resolution":{"observed_at":"2026-08-14T14:29:00.721742Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1204.1888","last_updated":"2012-07-18T06:26:33Z","snapshot_observed_at":"2026-07-06T02:46:00.739446Z","submitted_at":"2012-04-09T14:26:49Z","title":"Equation-of-state dependence of the gravitational-wave signal from the ring-down phase of neutron-star mergers","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1204.1888","snapshot_observed_at":"2026-08-14T14:29:00.724961Z","title":"Equation-of-state dependence of the gravitational-wave signal from the ring-down phase of neutron-star mergers","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"1908.03135","last_updated":"2019-08-08T16:01:36Z","snapshot_observed_at":"2026-08-14T14:20:29.928442Z","submitted_at":"2019-08-08T16:01:36Z","title":"Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity","version":1},"reference_index":91,"source":"pdf_text","source_observed_at":"2026-08-14T14:29:00.724961Z"},"links":{"cited_paper":"/paper/1204.1888","citing_paper":"/paper/1908.03135"},"observation_digest":"sha256:79fe1c837ce435e127265153189fb40bdbad0338947fec4c8a7303779860e6ed","observation_id":"4c368f6b-dab0-44cd-9f7c-375770641918","resolution":{"observed_at":"2026-08-14T14:29:00.724961Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1403.5301","last_updated":"2014-06-19T09:51:25Z","snapshot_observed_at":"2026-07-06T03:39:03.568519Z","submitted_at":"2014-03-20T21:24:51Z","title":"Revealing the high-density equation of state through binary neutron star mergers","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1403.5301","snapshot_observed_at":"2026-08-14T14:29:00.728049Z","title":"Revealing the high-density equation of state through binary neutron star mergers","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"1908.03135","last_updated":"2019-08-08T16:01:36Z","snapshot_observed_at":"2026-08-14T14:20:29.928442Z","submitted_at":"2019-08-08T16:01:36Z","title":"Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity","version":1},"reference_index":92,"source":"pdf_text","source_observed_at":"2026-08-14T14:29:00.728049Z"},"links":{"cited_paper":"/paper/1403.5301","citing_paper":"/paper/1908.03135"},"observation_digest":"sha256:87903a2e9b1fab2821e97d9368724558ea24b313e9d69af373bff6c66a62aecb","observation_id":"6e31b725-10b2-44d0-8b2a-8aaadf4e8421","resolution":{"observed_at":"2026-08-14T14:29:00.728049Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1509.08522","last_updated":"2015-09-28T22:07:01Z","snapshot_observed_at":"2026-08-14T22:30:27.935355Z","submitted_at":"2015-09-28T22:07:01Z","title":"Observing Gravitational Waves From The Post-Merger Phase Of Binary Neutron Star Coalescence","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1509.08522","snapshot_observed_at":"2026-08-14T14:29:00.731450Z","title":"Observing Gravitational Waves From The Post-Merger Phase Of Binary Neutron Star Coalescence","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"1908.03135","last_updated":"2019-08-08T16:01:36Z","snapshot_observed_at":"2026-08-14T14:20:29.928442Z","submitted_at":"2019-08-08T16:01:36Z","title":"Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity","version":1},"reference_index":93,"source":"pdf_text","source_observed_at":"2026-08-14T14:29:00.731450Z"},"links":{"cited_paper":"/paper/1509.08522","citing_paper":"/paper/1908.03135"},"observation_digest":"sha256:0ff2722fd1c54d807dd015cabe7dd0578df7f8b4365eceaa5f9341cfb7532b9d","observation_id":"5459dbe1-3f2b-4f1f-86aa-4f8db63ad53f","resolution":{"observed_at":"2026-08-14T14:29:00.731450Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1502.03176","last_updated":"2015-06-02T18:04:27Z","snapshot_observed_at":"2026-08-14T18:30:39.005896Z","submitted_at":"2015-02-11T02:27:43Z","title":"A unified picture of the post-merger dynamics and gravitational wave emission in neutron-star mergers","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1502.03176","snapshot_observed_at":"2026-08-14T14:29:00.734946Z","title":"Unified picture of the post-merger dynamics and gravitational wave emission in neutron star mergers","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"1908.03135","last_updated":"2019-08-08T16:01:36Z","snapshot_observed_at":"2026-08-14T14:20:29.928442Z","submitted_at":"2019-08-08T16:01:36Z","title":"Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity","version":1},"reference_index":94,"source":"pdf_text","source_observed_at":"2026-08-14T14:29:00.734946Z"},"links":{"cited_paper":"/paper/1502.03176","citing_paper":"/paper/1908.03135"},"observation_digest":"sha256:3cbabf20dad69f8f4c547e6695d56343702d55c30a315917dcebacc9551d7c7f","observation_id":"4a402242-db0c-4da9-872e-ee540f81483f","resolution":{"observed_at":"2026-08-14T14:29:00.734946Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1504.01764","last_updated":"2015-08-17T20:40:58Z","snapshot_observed_at":"2026-08-06T17:41:19.163105Z","submitted_at":"2015-04-07T21:51:13Z","title":"Modeling the complete gravitational wave spectrum of neutron star mergers","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1504.01764","snapshot_observed_at":"2026-08-14T14:29:00.738639Z","title":"Modeling the complete gravitational wave spectrum of neutron star mergers","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"1908.03135","last_updated":"2019-08-08T16:01:36Z","snapshot_observed_at":"2026-08-14T14:20:29.928442Z","submitted_at":"2019-08-08T16:01:36Z","title":"Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity","version":1},"reference_index":95,"source":"pdf_text","source_observed_at":"2026-08-14T14:29:00.738639Z"},"links":{"cited_paper":"/paper/1504.01764","citing_paper":"/paper/1908.03135"},"observation_digest":"sha256:77c4beeed713958ac713085c41858405c6c1b73d594bdc0a7671b91192803840","observation_id":"cbe44726-2916-44c8-864e-826e12c3ab9c","resolution":{"observed_at":"2026-08-14T14:29:00.738639Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1807.06857","last_updated":"2018-11-12T10:19:58Z","snapshot_observed_at":"2026-08-14T18:50:34.525078Z","submitted_at":"2018-07-18T10:49:29Z","title":"Gravitational waves and mass ejecta from binary neutron star mergers: Effect of large eccentricities","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1807.06857","snapshot_observed_at":"2026-08-14T14:29:00.742787Z","title":"Gravitational waves and mass ejecta from binary neutron star mergers: Effect of large eccentricities","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"1908.03135","last_updated":"2019-08-08T16:01:36Z","snapshot_observed_at":"2026-08-14T14:20:29.928442Z","submitted_at":"2019-08-08T16:01:36Z","title":"Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity","version":1},"reference_index":96,"source":"pdf_text","source_observed_at":"2026-08-14T14:29:00.742787Z"},"links":{"cited_paper":"/paper/1807.06857","citing_paper":"/paper/1908.03135"},"observation_digest":"sha256:cb9741d4e1b4786e545b394b3418541fc7853c96c21ed7ac6710d5ecbd9327d6","observation_id":"9987e94c-d231-4738-8b7d-31032b8a8219","resolution":{"observed_at":"2026-08-14T14:29:00.742787Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1610.09381","last_updated":"2017-07-18T00:31:50Z","snapshot_observed_at":"2026-08-14T21:32:58.641366Z","submitted_at":"2016-10-28T20:00:05Z","title":"Kilonovae","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1610.09381","snapshot_observed_at":"2026-08-14T14:29:00.746338Z","title":"Kilonovae","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"1908.03135","last_updated":"2019-08-08T16:01:36Z","snapshot_observed_at":"2026-08-14T14:20:29.928442Z","submitted_at":"2019-08-08T16:01:36Z","title":"Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity","version":1},"reference_index":97,"source":"pdf_text","source_observed_at":"2026-08-14T14:29:00.746338Z"},"links":{"cited_paper":"/paper/1610.09381","citing_paper":"/paper/1908.03135"},"observation_digest":"sha256:eeee39836f01226bf4b8a1173f8a89f4bf936538f022b61895a762f9b9633475","observation_id":"21256722-3157-4a38-a052-8eb14e18f75a","resolution":{"observed_at":"2026-08-14T14:29:00.746338Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1612.03665","last_updated":"2016-12-12T13:24:28Z","snapshot_observed_at":"2026-08-14T21:26:00.313156Z","submitted_at":"2016-12-12T13:24:28Z","title":"Modeling dynamical ejecta from binary neutron star mergers and implications for electromagnetic counterparts","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1612.03665","snapshot_observed_at":"2026-08-14T14:29:00.750629Z","title":"Modeling dynamical ejecta from binary neutron star mergers and implications for electromagnetic counterparts","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"1908.03135","last_updated":"2019-08-08T16:01:36Z","snapshot_observed_at":"2026-08-14T14:20:29.928442Z","submitted_at":"2019-08-08T16:01:36Z","title":"Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity","version":1},"reference_index":98,"source":"pdf_text","source_observed_at":"2026-08-14T14:29:00.750629Z"},"links":{"cited_paper":"/paper/1612.03665","citing_paper":"/paper/1908.03135"},"observation_digest":"sha256:ec90a41e1bbc1e6bdbdbf660b8f49579d51c06381ec984b74048c87318de67f3","observation_id":"f822b7eb-63ec-4be4-bd22-7af0b0a6ee5a","resolution":{"observed_at":"2026-08-14T14:29:00.750629Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0502470","last_updated":"2005-04-25T17:24:15Z","snapshot_observed_at":"2026-07-07T00:48:17.559513Z","submitted_at":"2005-02-22T23:31:24Z","title":"Neutrino-Dominated Accretion and Supernovae","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0502470","snapshot_observed_at":"2026-08-14T14:29:00.754374Z","title":"Neutrino-dominated accretion and supernovae.Astrophys","venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"1908.03135","last_updated":"2019-08-08T16:01:36Z","snapshot_observed_at":"2026-08-14T14:20:29.928442Z","submitted_at":"2019-08-08T16:01:36Z","title":"Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity","version":1},"reference_index":99,"source":"pdf_text","source_observed_at":"2026-08-14T14:29:00.754374Z"},"links":{"cited_paper":"/paper/astro-ph/0502470","citing_paper":"/paper/1908.03135"},"observation_digest":"sha256:892e2826c3cea5390dcbb82bab932bcdfbd376fcb3da9935c7e2bac0b66d6aa8","observation_id":"07f103c9-c38e-4646-a71e-a834e2757a45","resolution":{"observed_at":"2026-08-14T14:29:00.754374Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0509365","last_updated":"2005-09-13T21:24:22Z","snapshot_observed_at":"2026-07-07T00:53:53.176708Z","submitted_at":"2005-09-13T21:24:22Z","title":"Nucleosynthesis in the Outflow from Gamma Ray Burst Accretion Disks","version":1},"cited_work":{"arxiv_id":"astro-ph/0509365","doi":null,"metadata_source":"pith","pith_arxiv_id":"astro-ph/0509365","snapshot_observed_at":"2026-08-14T14:29:01.026426Z","title":"Nucleosynthesis in the Outflow from Gamma Ray Burst Accretion Disks","venue":"astro-ph","work_id":"59058b41-e54f-43bc-a6cd-6e16813702a3","year":2005},"citing_paper":{"arxiv_id":"1908.03135","last_updated":"2019-08-08T16:01:36Z","snapshot_observed_at":"2026-08-14T14:20:29.928442Z","submitted_at":"2019-08-08T16:01:36Z","title":"Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity","version":1},"reference_index":100,"source":"pdf_text","source_observed_at":"2026-08-14T14:29:00.757995Z"},"links":{"cited_paper":"/paper/astro-ph/0509365","citing_paper":"/paper/1908.03135"},"observation_digest":"sha256:4ca7ba0780b92f540389061583bc422d1ddcab9ed8f02f5b5f58df1e6ad7327c","observation_id":"4d5e1107-8dd1-4a62-8c6c-4f3e6be70477","resolution":{"observed_at":"2026-08-14T14:29:01.030478Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}}],"paper":{"arxiv_id":"1908.03135","last_updated":"2019-08-08T16:01:36Z","latest_version":1,"primary_category":"gr-qc","snapshot_observed_at":"2026-08-14T14:20:29.928442Z","submitted_at":"2019-08-08T16:01:36Z","title":"Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity"},"reference_resolution":{"displayed":100,"state_counts":{"malformed_identifier":2,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":97,"verified_exact":1,"verified_fuzzy":0},"total_outbound_references":113},"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":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"thesis":"As of 14 August 2026, this Paper Citation Record lists 100 of 113 outbound references and 1 inbound Pith citation observation for arXiv:1908.03135."}