{"as_of":"2026-08-11T06:26:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:6c22262adb027a0a1bfa1696e8a7b86850035a9ba4da86ef46127d10ea28f7cf","coverage":[{"denominator":129,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":100,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-10T16:33:20.174351Z","state":"measured"},{"denominator":105,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":105,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-10T06:31:04.303077+00:00","state":"measured"},{"denominator":5,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":5,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-10T10:40:00.398819Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"pith","source_observed_at":"2026-07-10T15:07:19.518197Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2501.13064","last_updated":"2025-03-07T22:36:49Z","snapshot_observed_at":"2026-08-10T16:40:19.014391Z","submitted_at":"2025-01-22T18:18:47Z","title":"Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2501.13064","snapshot_observed_at":"2026-08-07T11:40:36.103140Z","title":"Yu and S","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2506.02115","last_updated":"2025-06-02T18:00:04Z","snapshot_observed_at":"2026-08-09T15:07:34.142230Z","submitted_at":"2025-06-02T18:00:04Z","title":"The error budget of binary neutron star merger simulations for configurations with high spin","version":1},"reference_index":91,"source":"pdf_text","source_observed_at":"2026-08-07T11:40:36.103140Z"},"links":{"cited_paper":"/paper/2501.13064","citing_paper":"/paper/2506.02115"},"observation_digest":"sha256:b10c13fe717fce7baf759449e351b23a5a86f97aa345adff295395d19464b875","observation_id":"2cda26a2-e236-4d7e-9fc6-6c6348aed45a","resolution":{"observed_at":"2026-08-07T11:40:36.103140Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2501.13064","last_updated":"2025-03-07T22:36:49Z","snapshot_observed_at":"2026-08-10T16:40:19.014391Z","submitted_at":"2025-01-22T18:18:47Z","title":"Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides","version":2},"cited_work":{"arxiv_id":"2501.13064","doi":null,"metadata_source":"pith","pith_arxiv_id":"2501.13064","snapshot_observed_at":"2026-07-10T15:07:19.518197Z","title":"Yu and S","venue":"gr-qc","work_id":"7c88362d-a7d3-4fc9-9234-6815e6e0f21b","year":2025},"citing_paper":{"arxiv_id":"2511.19626","last_updated":"2026-05-12T21:40:23Z","snapshot_observed_at":"2026-07-06T22:36:49.325569Z","submitted_at":"2025-11-24T19:01:38Z","title":"Universal Relations with Dynamical Tides","version":2},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-05-17T05:53:11.977211Z"},"links":{"cited_paper":"/paper/2501.13064","citing_paper":"/paper/2511.19626"},"observation_digest":"sha256:7453aa9f3193684d1d1bb3e76e51b3c48a5edac47a77ee53d64f9cfd2a3438c2","observation_id":"3360aef2-96e3-4bfb-8705-c6ecc444519d","resolution":{"observed_at":"2026-05-17T05:54:08.555506Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2501.13064","last_updated":"2025-03-07T22:36:49Z","snapshot_observed_at":"2026-08-10T16:40:19.014391Z","submitted_at":"2025-01-22T18:18:47Z","title":"Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides","version":2},"cited_work":{"arxiv_id":"2501.13064","doi":null,"metadata_source":"pith","pith_arxiv_id":"2501.13064","snapshot_observed_at":"2026-07-10T15:07:19.518197Z","title":"Yu and S","venue":"gr-qc","work_id":"7c88362d-a7d3-4fc9-9234-6815e6e0f21b","year":2025},"citing_paper":{"arxiv_id":"2605.08569","last_updated":"2026-05-09T00:04:35Z","snapshot_observed_at":"2026-08-03T04:55:02.320893Z","submitted_at":"2026-05-09T00:04:35Z","title":"The Good, the Bad, and the Subtle: Relativistic mode sums for neutron-star tidal response","version":1},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-05-12T02:14:04.128117Z"},"links":{"cited_paper":"/paper/2501.13064","citing_paper":"/paper/2605.08569"},"observation_digest":"sha256:4e0b340ad3176f6351f9c904521b484db5bed8812d01ce5e6188f77793fb1a1f","observation_id":"82b13fc7-1b70-43b1-9d95-f2ef4d2f4c64","resolution":{"observed_at":"2026-05-12T02:16:15.961959Z","resolver_source":"arxiv_id","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2501.13064","last_updated":"2025-03-07T22:36:49Z","snapshot_observed_at":"2026-08-10T16:40:19.014391Z","submitted_at":"2025-01-22T18:18:47Z","title":"Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides","version":2},"cited_work":{"arxiv_id":"2501.13064","doi":null,"metadata_source":"pith","pith_arxiv_id":"2501.13064","snapshot_observed_at":"2026-07-10T15:07:19.518197Z","title":"Yu and S","venue":"gr-qc","work_id":"7c88362d-a7d3-4fc9-9234-6815e6e0f21b","year":2025},"citing_paper":{"arxiv_id":"2607.07943","last_updated":"2026-07-08T21:42:21Z","snapshot_observed_at":"2026-08-03T10:13:10.859235Z","submitted_at":"2026-07-08T21:42:21Z","title":"Nonlinear hydrodynamics in spinning neutron stars: Theoretical universal relations and equilibrium solutions","version":1},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-07-10T15:01:14.878332Z"},"links":{"cited_paper":"/paper/2501.13064","citing_paper":"/paper/2607.07943"},"observation_digest":"sha256:85bbdcf40dceaad28de18a8ddab340e0fd0b643aef78f9a769a99507289f4dd5","observation_id":"a1b2840e-5ddf-4efc-8cd5-077228699165","resolution":{"observed_at":"2026-07-10T15:07:19.519482Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2501.13064","last_updated":"2025-03-07T22:36:49Z","snapshot_observed_at":"2026-08-10T16:40:19.014391Z","submitted_at":"2025-01-22T18:18:47Z","title":"Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2501.13064","snapshot_observed_at":"2026-08-10T10:40:00.398819Z","title":"Yu and S","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2608.07311","last_updated":"2026-08-07T15:06:30Z","snapshot_observed_at":"2026-08-11T06:13:56.501440Z","submitted_at":"2026-08-07T15:06:30Z","title":"Oscillations of Dissipative Neutron Stars: The Impact of Hyperonic Reaction Rates","version":1},"reference_index":64,"source":"pdf_text","source_observed_at":"2026-08-10T10:40:00.398819Z"},"links":{"cited_paper":"/paper/2501.13064","citing_paper":"/paper/2608.07311"},"observation_digest":"sha256:a70916aedc882286fd4b9b13f1716d8674d4114964a5be1d13bcb567353ad5e0","observation_id":"bf7db3b6-37a8-4467-b1a4-f3de9b78a13a","resolution":{"observed_at":"2026-08-10T10:40:00.398819Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2501.13064/citation-record","integrity":"/paper/2501.13064/integrity","json":"/paper/2501.13064/citation-record.json","paper":"/paper/2501.13064"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T16:33:19.376520Z","title":"The two approaches are equivalent when only the f-modes are considered, yet our model is more flexible in incorporating other modes (e.g., gravity and pressure modes)","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2501.13064","last_updated":"2025-03-07T22:36:49Z","snapshot_observed_at":"2026-08-10T16:40:19.014391Z","submitted_at":"2025-01-22T18:18:47Z","title":"Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides","version":2},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-10T16:33:19.376520Z"},"links":{"citing_paper":"/paper/2501.13064"},"observation_digest":"sha256:ff1fa18867b60410283f2d98d336eeebc1f4ed434ab64398da1ddc267773d9c9","observation_id":"2e4d8910-8793-47b0-8927-716f31b22d26","resolution":{"observed_at":"2026-08-10T16:33:19.376520Z","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":"2026-08-10T16:33:19.386868Z","title":"For the frame dragging terms [H (eff) fr and H (eff) t,LS], we do not replace Pϕ by µr√u[1 + ...] in order to capture the correct back-reaction torque (as discussed in Sec","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2501.13064","last_updated":"2025-03-07T22:36:49Z","snapshot_observed_at":"2026-08-10T16:40:19.014391Z","submitted_at":"2025-01-22T18:18:47Z","title":"Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides","version":2},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-10T16:33:19.386868Z"},"links":{"citing_paper":"/paper/2501.13064"},"observation_digest":"sha256:af021a3d936373c78ca19b008c15df330675b1fe34a8e0703cccc270243e3805","observation_id":"09bc628d-19d9-448b-a2ed-d5e06997eec6","resolution":{"observed_at":"2026-08-10T16:33:19.386868Z","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":"2026-08-10T16:33:19.396070Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2501.13064","last_updated":"2025-03-07T22:36:49Z","snapshot_observed_at":"2026-08-10T16:40:19.014391Z","submitted_at":"2025-01-22T18:18:47Z","title":"Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides","version":2},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-10T16:33:19.396070Z"},"links":{"citing_paper":"/paper/2501.13064"},"observation_digest":"sha256:36628796e8669f5aaa0da86b9027c85b1416585044a5c9e2f9f9670a1bdfa257","observation_id":"09431f9f-00bd-4d90-955a-1c59362750ea","resolution":{"observed_at":"2026-08-10T16:33:19.396070Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1712.02992","last_updated":"2017-12-08T09:32:11Z","snapshot_observed_at":"2026-07-06T06:13:23.505399Z","submitted_at":"2017-12-08T09:32:11Z","title":"Numerical Relativity Simulations of Precessing Binary Neutron Star Mergers","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1712.02992","snapshot_observed_at":"2026-08-10T16:33:19.468064Z","title":"Dietrich, S","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2501.13064","last_updated":"2025-03-07T22:36:49Z","snapshot_observed_at":"2026-08-10T16:40:19.014391Z","submitted_at":"2025-01-22T18:18:47Z","title":"Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides","version":2},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-10T16:33:19.468064Z"},"links":{"cited_paper":"/paper/1712.02992","citing_paper":"/paper/2501.13064"},"observation_digest":"sha256:bbae935c78b7da7fa770e96ba4f0f0a865b3b5d38d3e89bfe6f24e148e8b3cd5","observation_id":"0c7eeed4-36d8-4851-b7db-6056235488b6","resolution":{"observed_at":"2026-08-10T16:33:19.468064Z","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":"2026-08-10T16:33:19.406443Z","title":"This is achieved by scaling length and time by1/M, frequency byM, energy and linear momentum by1/µ, and angular momentum by1/(µM )","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2501.13064","last_updated":"2025-03-07T22:36:49Z","snapshot_observed_at":"2026-08-10T16:40:19.014391Z","submitted_at":"2025-01-22T18:18:47Z","title":"Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides","version":2},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-10T16:33:19.406443Z"},"links":{"citing_paper":"/paper/2501.13064"},"observation_digest":"sha256:a0260c11a996a90816c216a504f63e22aed1a58da50faba07f9b445586bdc86e","observation_id":"fa1ee42a-1a28-4c4b-80a5-46467ed16c48","resolution":{"observed_at":"2026-08-10T16:33:19.406443Z","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":"2026-08-10T16:33:19.416500Z","title":"(110) The detuning is to be compared with Eqs","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2501.13064","last_updated":"2025-03-07T22:36:49Z","snapshot_observed_at":"2026-08-10T16:40:19.014391Z","submitted_at":"2025-01-22T18:18:47Z","title":"Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides","version":2},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-10T16:33:19.416500Z"},"links":{"citing_paper":"/paper/2501.13064"},"observation_digest":"sha256:3183370c994d825a0c93a1904b98281929f5599935af19d32fac5bcef7123649","observation_id":"70448d52-d6fa-4a42-b233-734bcfb31f1e","resolution":{"observed_at":"2026-08-10T16:33:19.416500Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9307032","last_updated":"1993-07-22T16:42:28Z","snapshot_observed_at":"2026-07-07T01:08:48.539675Z","submitted_at":"1993-07-22T16:42:28Z","title":"Equilibrium, Stability and Orbital Evolution of Close Binary Systems","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9307032","snapshot_observed_at":"2026-08-10T16:33:19.493105Z","title":null,"venue":null,"work_id":null,"year":1994},"citing_paper":{"arxiv_id":"2501.13064","last_updated":"2025-03-07T22:36:49Z","snapshot_observed_at":"2026-08-10T16:40:19.014391Z","submitted_at":"2025-01-22T18:18:47Z","title":"Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides","version":2},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-10T16:33:19.493105Z"},"links":{"cited_paper":"/paper/astro-ph/9307032","citing_paper":"/paper/2501.13064"},"observation_digest":"sha256:aa23bc2af51d378a1e6ac65a9eb887a2971b02d45364e2fd1d9d0e50baeb2d7d","observation_id":"9b0b88b7-34d1-45c4-998f-ca5aeae9705d","resolution":{"observed_at":"2026-08-10T16:33:19.493105Z","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":"2026-08-10T16:33:19.435134Z","title":"2q∗ aqaωa⟨ξa, iˆez × ξa⟩ + X b 2q∗ aqbΩ ⟨ˆez × ξa, ˆez × ξb⟩ # , ≃ +X a","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2501.13064","last_updated":"2025-03-07T22:36:49Z","snapshot_observed_at":"2026-08-10T16:40:19.014391Z","submitted_at":"2025-01-22T18:18:47Z","title":"Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides","version":2},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-10T16:33:19.435134Z"},"links":{"citing_paper":"/paper/2501.13064"},"observation_digest":"sha256:e2c72ae8d239893c67e2c5a77338d76d33bcab7e59e633ba890588299450d1f3","observation_id":"70f000c9-7909-44a4-8f5a-ecea95427725","resolution":{"observed_at":"2026-08-10T16:33:19.435134Z","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":"2026-08-10T16:33:19.442593Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2501.13064","last_updated":"2025-03-07T22:36:49Z","snapshot_observed_at":"2026-08-10T16:40:19.014391Z","submitted_at":"2025-01-22T18:18:47Z","title":"Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides","version":2},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-10T16:33:19.442593Z"},"links":{"cited_paper":"/paper/1710.05832","citing_paper":"/paper/2501.13064"},"observation_digest":"sha256:b546473e06ee4170712330169d07d1d9fd379916672e911af30cf6579492db9a","observation_id":"09bdb34b-6df5-491e-a242-2e79da002d67","resolution":{"observed_at":"2026-08-10T16:33:19.442593Z","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":"2026-08-07T22:20:24.299342Z","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":"2026-08-10T16:33:19.454647Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2501.13064","last_updated":"2025-03-07T22:36:49Z","snapshot_observed_at":"2026-08-10T16:40:19.014391Z","submitted_at":"2025-01-22T18:18:47Z","title":"Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides","version":2},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-10T16:33:19.454647Z"},"links":{"cited_paper":"/paper/1805.11581","citing_paper":"/paper/2501.13064"},"observation_digest":"sha256:2bf993c92094fec1c6adcbb13b076455481a4aa611a44d39ed1ec88c5c91f940","observation_id":"e982bfb1-7b02-46ca-9bf5-ce552ce0caf0","resolution":{"observed_at":"2026-08-10T16:33:19.454647Z","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":"2026-08-10T16:33:19.460374Z","title":"Hotokezaka, K","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2501.13064","last_updated":"2025-03-07T22:36:49Z","snapshot_observed_at":"2026-08-10T16:40:19.014391Z","submitted_at":"2025-01-22T18:18:47Z","title":"Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides","version":2},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-10T16:33:19.460374Z"},"links":{"cited_paper":"/paper/1502.03457","citing_paper":"/paper/2501.13064"},"observation_digest":"sha256:715ce0f82661241bd42677edc7c14ea1192cd4dd7dd9e7df364108725afd8bb7","observation_id":"76028673-0c08-4d42-bff6-854d28491b59","resolution":{"observed_at":"2026-08-10T16:33:19.460374Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1203.4352","last_updated":"2012-03-20T09:25:36Z","snapshot_observed_at":"2026-07-06T02:44:52.187417Z","submitted_at":"2012-03-20T09:25:36Z","title":"Measurability of the tidal polarizability of neutron stars in late-inspiral gravitational-wave signals","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1203.4352","snapshot_observed_at":"2026-08-10T16:33:19.527083Z","title":"Damour, A","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2501.13064","last_updated":"2025-03-07T22:36:49Z","snapshot_observed_at":"2026-08-10T16:40:19.014391Z","submitted_at":"2025-01-22T18:18:47Z","title":"Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides","version":2},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-10T16:33:19.527083Z"},"links":{"cited_paper":"/paper/1203.4352","citing_paper":"/paper/2501.13064"},"observation_digest":"sha256:d2ce85a6a2b9ad063aa1ffd0ac79b031c778b634d1a535a1db9ec06c41d623e1","observation_id":"99d03b6d-32c6-4375-a6c4-51731610bb2c","resolution":{"observed_at":"2026-08-10T16:33:19.527083Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1812.06988","last_updated":"2018-12-17T19:00:04Z","snapshot_observed_at":"2026-07-06T07:21:45.898421Z","submitted_at":"2018-12-17T19:00:04Z","title":"Gravitational waveforms from SpEC simulations : neutron star-neutron star and low-mass black hole-neutron star binaries","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1812.06988","snapshot_observed_at":"2026-08-10T16:33:19.478493Z","title":"Foucart, M","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2501.13064","last_updated":"2025-03-07T22:36:49Z","snapshot_observed_at":"2026-08-10T16:40:19.014391Z","submitted_at":"2025-01-22T18:18:47Z","title":"Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides","version":2},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-10T16:33:19.478493Z"},"links":{"cited_paper":"/paper/1812.06988","citing_paper":"/paper/2501.13064"},"observation_digest":"sha256:d6d94e802fb2422fa04650da97678c95310e5a8041fd71a25bc376fc8ed7812a","observation_id":"ca77a39c-48a9-4d87-a116-f144ca4f72c8","resolution":{"observed_at":"2026-08-10T16:33:19.478493Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9304027","last_updated":"1993-04-28T18:28:35Z","snapshot_observed_at":"2026-07-07T01:08:42.232149Z","submitted_at":"1993-04-28T18:28:35Z","title":"Hydrodynamic Instability and Coalescence of Binary Neutron Stars","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9304027","snapshot_observed_at":"2026-08-10T16:33:19.484799Z","title":null,"venue":null,"work_id":null,"year":1994},"citing_paper":{"arxiv_id":"2501.13064","last_updated":"2025-03-07T22:36:49Z","snapshot_observed_at":"2026-08-10T16:40:19.014391Z","submitted_at":"2025-01-22T18:18:47Z","title":"Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides","version":2},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-10T16:33:19.484799Z"},"links":{"cited_paper":"/paper/astro-ph/9304027","citing_paper":"/paper/2501.13064"},"observation_digest":"sha256:0f96a367ca29fb7090e95ed8eaf8b51ac7262266262232d8dbced65187fa9550","observation_id":"685dd830-a6fe-46c2-b45b-a4c0758ae5a8","resolution":{"observed_at":"2026-08-10T16:33:19.484799Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1806.01772","last_updated":"2018-10-28T18:57:38Z","snapshot_observed_at":"2026-08-10T07:38:15.562425Z","submitted_at":"2018-06-05T16:10:39Z","title":"Time-domain effective-one-body gravitational waveforms for coalescing compact binaries with nonprecessing spins, tides and self-spin effects","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1806.01772","snapshot_observed_at":"2026-08-10T16:33:19.547644Z","title":"Nagar, S","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2501.13064","last_updated":"2025-03-07T22:36:49Z","snapshot_observed_at":"2026-08-10T16:40:19.014391Z","submitted_at":"2025-01-22T18:18:47Z","title":"Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides","version":2},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-10T16:33:19.547644Z"},"links":{"cited_paper":"/paper/1806.01772","citing_paper":"/paper/2501.13064"},"observation_digest":"sha256:857522135201c9f7c05efb629594fd8395422d0234880f8c9ef3bc2e51175d29","observation_id":"11b7b69a-716b-4650-a178-1d47128edf57","resolution":{"observed_at":"2026-08-10T16:33:19.547644Z","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":"2026-08-10T16:33:19.369127Z","title":"in” replaced by “or","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2501.13064","last_updated":"2025-03-07T22:36:49Z","snapshot_observed_at":"2026-08-10T16:40:19.014391Z","submitted_at":"2025-01-22T18:18:47Z","title":"Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides","version":2},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-10T16:33:19.369127Z"},"links":{"citing_paper":"/paper/2501.13064"},"observation_digest":"sha256:89daefb39ba8a4dbc0cc54c0326b53f5542ead361a048bed8a04768e4f795642","observation_id":"db5380e9-f426-4cde-bdcc-6c28a7aa5ae5","resolution":{"observed_at":"2026-08-10T16:33:19.369127Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0709.1915","last_updated":"2007-12-07T21:22:23Z","snapshot_observed_at":"2026-07-06T01:33:47.610408Z","submitted_at":"2007-09-12T15:46:16Z","title":"Constraining neutron star tidal Love numbers with gravitational wave detectors","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0709.1915","snapshot_observed_at":"2026-08-10T16:33:19.500149Z","title":null,"venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2501.13064","last_updated":"2025-03-07T22:36:49Z","snapshot_observed_at":"2026-08-10T16:40:19.014391Z","submitted_at":"2025-01-22T18:18:47Z","title":"Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides","version":2},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-10T16:33:19.500149Z"},"links":{"cited_paper":"/paper/0709.1915","citing_paper":"/paper/2501.13064"},"observation_digest":"sha256:b2769b828b34889220ae53af9144ba8d5fea69a77636c0e4776705a3061d22e5","observation_id":"3e81aa9d-38d4-4535-a97f-3973462a001b","resolution":{"observed_at":"2026-08-10T16:33:19.500149Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0811.2069","last_updated":"2009-03-11T13:55:12Z","snapshot_observed_at":"2026-07-06T01:50:52.457111Z","submitted_at":"2008-11-13T11:33:11Z","title":"Improved resummation of post-Newtonian multipolar waveforms from circularized compact binaries","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0811.2069","snapshot_observed_at":"2026-08-10T16:33:19.506958Z","title":"Damour, B","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2501.13064","last_updated":"2025-03-07T22:36:49Z","snapshot_observed_at":"2026-08-10T16:40:19.014391Z","submitted_at":"2025-01-22T18:18:47Z","title":"Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides","version":2},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-10T16:33:19.506958Z"},"links":{"cited_paper":"/paper/0811.2069","citing_paper":"/paper/2501.13064"},"observation_digest":"sha256:f39f26025587be152342a0758541788587d9bd12617cd5705a08af1d319ba5fc","observation_id":"537b44d7-ba9c-4412-9a10-ee8efb11c79e","resolution":{"observed_at":"2026-08-10T16:33:19.506958Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0911.3535","last_updated":"2009-11-18T18:09:22Z","snapshot_observed_at":"2026-07-06T02:03:44.584687Z","submitted_at":"2009-11-18T18:09:22Z","title":"Tidal deformability of neutron stars with realistic equations of state and their gravitational wave signatures in binary inspiral","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0911.3535","snapshot_observed_at":"2026-08-10T16:33:19.513484Z","title":"Hinderer, B","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2501.13064","last_updated":"2025-03-07T22:36:49Z","snapshot_observed_at":"2026-08-10T16:40:19.014391Z","submitted_at":"2025-01-22T18:18:47Z","title":"Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides","version":2},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-10T16:33:19.513484Z"},"links":{"cited_paper":"/paper/0911.3535","citing_paper":"/paper/2501.13064"},"observation_digest":"sha256:03eba521ab3faa9a599ef1afc54ef7f327ebf41338a9b75fd4ba6f29a891994a","observation_id":"57582702-75c5-47c8-9e24-71f0ac8606ea","resolution":{"observed_at":"2026-08-10T16:33:19.513484Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1202.3565","last_updated":"2012-06-15T14:04:16Z","snapshot_observed_at":"2026-07-06T02:42:59.643716Z","submitted_at":"2012-02-16T11:07:20Z","title":"Effective action approach to higher-order relativistic tidal interactions in binary systems and their effective one body description","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1202.3565","snapshot_observed_at":"2026-08-10T16:33:19.518966Z","title":null,"venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2501.13064","last_updated":"2025-03-07T22:36:49Z","snapshot_observed_at":"2026-08-10T16:40:19.014391Z","submitted_at":"2025-01-22T18:18:47Z","title":"Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides","version":2},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-10T16:33:19.518966Z"},"links":{"cited_paper":"/paper/1202.3565","citing_paper":"/paper/2501.13064"},"observation_digest":"sha256:e95da3dee460226d32d296a87cbb9b4c8762b2b773503a5c85d46ce077711a07","observation_id":"8e56d808-24fd-410c-bdb6-edef6fad509e","resolution":{"observed_at":"2026-08-10T16:33:19.518966Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1409.6933","last_updated":"2014-09-24T12:46:55Z","snapshot_observed_at":"2026-08-10T10:58:40.344176Z","submitted_at":"2014-09-24T12:46:55Z","title":"Gravitational self-force corrections to two-body tidal interactions and the effective one-body formalism","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1409.6933","snapshot_observed_at":"2026-08-10T16:33:19.533981Z","title":"Bini and T","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2501.13064","last_updated":"2025-03-07T22:36:49Z","snapshot_observed_at":"2026-08-10T16:40:19.014391Z","submitted_at":"2025-01-22T18:18:47Z","title":"Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides","version":2},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-10T16:33:19.533981Z"},"links":{"cited_paper":"/paper/1409.6933","citing_paper":"/paper/2501.13064"},"observation_digest":"sha256:df931fd3cd54af5f329c896f35c455eb64623adeddd379abdd7b8e8ab33f03f5","observation_id":"7e2c9045-01c4-4aaa-992a-a26a457309e3","resolution":{"observed_at":"2026-08-10T16:33:19.533981Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1412.4553","last_updated":"2015-05-13T14:07:20Z","snapshot_observed_at":"2026-08-03T21:35:03.622564Z","submitted_at":"2014-12-15T11:55:06Z","title":"Modeling the dynamics of tidally-interacting binary neutron stars up to merger","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1412.4553","snapshot_observed_at":"2026-08-10T16:33:19.541369Z","title":"Bernuzzi, A","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2501.13064","last_updated":"2025-03-07T22:36:49Z","snapshot_observed_at":"2026-08-10T16:40:19.014391Z","submitted_at":"2025-01-22T18:18:47Z","title":"Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides","version":2},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-10T16:33:19.541369Z"},"links":{"cited_paper":"/paper/1412.4553","citing_paper":"/paper/2501.13064"},"observation_digest":"sha256:26b38399f49987ff053c5a120e8f805bc57f3a3a1866e48e25fda35d1c3c99d2","observation_id":"96305710-2644-4efb-845b-437d44242791","resolution":{"observed_at":"2026-08-10T16:33:19.541369Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1910.08370","last_updated":"2020-09-10T10:44:12Z","snapshot_observed_at":"2026-08-11T00:11:35.187330Z","submitted_at":"2019-10-18T12:25:17Z","title":"Fast Rotating Relativistic Stars: Spectra and Stability without Approximation","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1910.08370","snapshot_observed_at":"2026-08-10T16:33:19.627422Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2501.13064","last_updated":"2025-03-07T22:36:49Z","snapshot_observed_at":"2026-08-10T16:40:19.014391Z","submitted_at":"2025-01-22T18:18:47Z","title":"Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides","version":2},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-10T16:33:19.627422Z"},"links":{"cited_paper":"/paper/1910.08370","citing_paper":"/paper/2501.13064"},"observation_digest":"sha256:cffcee1e1b234b45246d5c270f73779214c930b12ff7935597aa87d81a3e343c","observation_id":"5aa0902f-c0d5-48bd-a1f8-a5c069637a16","resolution":{"observed_at":"2026-08-10T16:33:19.627422Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1608.01907","last_updated":"2016-11-15T21:46:53Z","snapshot_observed_at":"2026-08-10T02:12:14.041964Z","submitted_at":"2016-08-05T15:08:55Z","title":"Dynamical Tides in General Relativity: Effective Action and Effective-One-Body Hamiltonian","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1608.01907","snapshot_observed_at":"2026-08-10T16:33:19.555643Z","title":"Steinhoff, T","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2501.13064","last_updated":"2025-03-07T22:36:49Z","snapshot_observed_at":"2026-08-10T16:40:19.014391Z","submitted_at":"2025-01-22T18:18:47Z","title":"Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides","version":2},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-10T16:33:19.555643Z"},"links":{"cited_paper":"/paper/1608.01907","citing_paper":"/paper/2501.13064"},"observation_digest":"sha256:e4394c4a54d50f72877f227ab676f0832c536e560e9dcaf63e1e7c6e0454ef40","observation_id":"9c812c12-fb6e-4f78-aa01-03e945988d22","resolution":{"observed_at":"2026-08-10T16:33:19.555643Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1602.00599","last_updated":"2016-05-09T15:16:37Z","snapshot_observed_at":"2026-07-06T04:44:45.059968Z","submitted_at":"2016-02-01T17:16:14Z","title":"Effects of neutron-star dynamic tides on gravitational waveforms within the effective-one-body approach","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1602.00599","snapshot_observed_at":"2026-08-10T16:33:19.572036Z","title":"Hinderer, A","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2501.13064","last_updated":"2025-03-07T22:36:49Z","snapshot_observed_at":"2026-08-10T16:40:19.014391Z","submitted_at":"2025-01-22T18:18:47Z","title":"Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides","version":2},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-10T16:33:19.572036Z"},"links":{"cited_paper":"/paper/1602.00599","citing_paper":"/paper/2501.13064"},"observation_digest":"sha256:b6879105d1ef5295c9179a1f4b9a660c5edfed4826e2252cc0b5b7476664ce42","observation_id":"40ee9bed-3f6e-4b06-b9c1-33b371bc709d","resolution":{"observed_at":"2026-08-10T16:33:19.572036Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2103.06100","last_updated":"2021-03-26T12:28:13Z","snapshot_observed_at":"2026-08-05T01:21:32.076183Z","submitted_at":"2021-03-10T14:55:27Z","title":"Spin effects on neutron star fundamental-mode dynamical tides: phenomenology and comparison to numerical simulations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2103.06100","snapshot_observed_at":"2026-08-10T16:33:19.581886Z","title":"Steinhoff, T","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2501.13064","last_updated":"2025-03-07T22:36:49Z","snapshot_observed_at":"2026-08-10T16:40:19.014391Z","submitted_at":"2025-01-22T18:18:47Z","title":"Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides","version":2},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-10T16:33:19.581886Z"},"links":{"cited_paper":"/paper/2103.06100","citing_paper":"/paper/2501.13064"},"observation_digest":"sha256:9a5da2fe678fdf756e09884d63da48983f6d4b2dd2cebdd059494438ad6d3a08","observation_id":"f47a6d38-1ec7-43e5-8a7f-6db05710c776","resolution":{"observed_at":"2026-08-10T16:33:19.581886Z","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":"2026-08-10T16:33:19.587879Z","title":"Ranjan Mohanty, U","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2501.13064","last_updated":"2025-03-07T22:36:49Z","snapshot_observed_at":"2026-08-10T16:40:19.014391Z","submitted_at":"2025-01-22T18:18:47Z","title":"Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides","version":2},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-10T16:33:19.587879Z"},"links":{"citing_paper":"/paper/2501.13064"},"observation_digest":"sha256:e6c6ff0bdbb2f3bb96fb9028009013b0b30d8d21565ba05bd6d359bbeb727f7f","observation_id":"d8a23b45-a0b2-435e-bd4b-4b13967f5292","resolution":{"observed_at":"2026-08-10T16:33:19.587879Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1408.3789","last_updated":"2015-01-13T06:24:24Z","snapshot_observed_at":"2026-08-04T20:31:08.098632Z","submitted_at":"2014-08-17T03:22:36Z","title":"Multipolar universal relations between f-mode frequency and tidal deformability of compact stars","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1408.3789","snapshot_observed_at":"2026-08-10T16:33:19.594028Z","title":null,"venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2501.13064","last_updated":"2025-03-07T22:36:49Z","snapshot_observed_at":"2026-08-10T16:40:19.014391Z","submitted_at":"2025-01-22T18:18:47Z","title":"Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides","version":2},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-10T16:33:19.594028Z"},"links":{"cited_paper":"/paper/1408.3789","citing_paper":"/paper/2501.13064"},"observation_digest":"sha256:ba837c909dd88eaeafa9035165199cbed6922649b43c13ca799f6748d27aa572","observation_id":"cbd54773-628c-4729-8aab-ccad70ae8826","resolution":{"observed_at":"2026-08-10T16:33:19.594028Z","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":"2026-08-10T16:33:19.604003Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2501.13064","last_updated":"2025-03-07T22:36:49Z","snapshot_observed_at":"2026-08-10T16:40:19.014391Z","submitted_at":"2025-01-22T18:18:47Z","title":"Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides","version":2},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-10T16:33:19.604003Z"},"links":{"citing_paper":"/paper/2501.13064"},"observation_digest":"sha256:3196e97918e53b32e57093d9d09740ee3b78c897a01d6cd55fb694577ec693a3","observation_id":"85d2d538-444f-47e2-8590-f1152e6b51bf","resolution":{"observed_at":"2026-08-10T16:33:19.604003Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1305.7197","last_updated":"2013-05-30T18:35:18Z","snapshot_observed_at":"2026-07-06T03:14:44.470940Z","submitted_at":"2013-05-30T18:35:18Z","title":"Gravitational wave asteroseismology of fast rotating neutron stars with realistic equations of state","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1305.7197","snapshot_observed_at":"2026-08-10T16:33:19.613606Z","title":null,"venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2501.13064","last_updated":"2025-03-07T22:36:49Z","snapshot_observed_at":"2026-08-10T16:40:19.014391Z","submitted_at":"2025-01-22T18:18:47Z","title":"Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides","version":2},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-10T16:33:19.613606Z"},"links":{"cited_paper":"/paper/1305.7197","citing_paper":"/paper/2501.13064"},"observation_digest":"sha256:4dde1eb6af13e510acc2c90ea46c04286de6b3d14c8a94465ce89d2b97c20750","observation_id":"c708d623-c6d7-4a94-8e74-a44b66f6b6ad","resolution":{"observed_at":"2026-08-10T16:33:19.613606Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2311.07456","last_updated":"2024-07-16T08:23:55Z","snapshot_observed_at":"2026-08-05T15:50:26.974469Z","submitted_at":"2023-11-13T16:41:19Z","title":"New and Robust Gravitational-Waveform Model for High-Mass-Ratio Binary Neutron Star Systems with Dynamical Tidal Effects","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2311.07456","snapshot_observed_at":"2026-08-10T16:33:19.685904Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2501.13064","last_updated":"2025-03-07T22:36:49Z","snapshot_observed_at":"2026-08-10T16:40:19.014391Z","submitted_at":"2025-01-22T18:18:47Z","title":"Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides","version":2},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-08-10T16:33:19.685904Z"},"links":{"cited_paper":"/paper/2311.07456","citing_paper":"/paper/2501.13064"},"observation_digest":"sha256:3ffe57b26ef7046791d3ff78dd7fa29ea876fba9895ee8ace2452253ba87ec6c","observation_id":"e0e778f6-a096-4b87-a7b7-eb6f75620bce","resolution":{"observed_at":"2026-08-10T16:33:19.685904Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2309.05643","last_updated":"2024-01-15T22:33:48Z","snapshot_observed_at":"2026-07-06T16:17:04.004519Z","submitted_at":"2023-09-11T17:33:38Z","title":"Rapidly rotating neutron stars: Universal relations and EOS inference","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2309.05643","snapshot_observed_at":"2026-08-10T16:33:19.637541Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2501.13064","last_updated":"2025-03-07T22:36:49Z","snapshot_observed_at":"2026-08-10T16:40:19.014391Z","submitted_at":"2025-01-22T18:18:47Z","title":"Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides","version":2},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-10T16:33:19.637541Z"},"links":{"cited_paper":"/paper/2309.05643","citing_paper":"/paper/2501.13064"},"observation_digest":"sha256:c4864de8c4db48c877956bba80e1f7d67ecbaf50958644969e48f57188b00509","observation_id":"49bb8e8a-3514-438b-a789-605afb95eadd","resolution":{"observed_at":"2026-08-10T16:33:19.637541Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2211.07002","last_updated":"2023-01-06T23:10:39Z","snapshot_observed_at":"2026-08-08T13:17:02.397044Z","submitted_at":"2022-11-13T19:43:44Z","title":"Beyond the linear tide: impact of the non-linear tidal response of neutron stars on gravitational waveforms from binary inspirals","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2211.07002","snapshot_observed_at":"2026-08-10T16:33:19.644485Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2501.13064","last_updated":"2025-03-07T22:36:49Z","snapshot_observed_at":"2026-08-10T16:40:19.014391Z","submitted_at":"2025-01-22T18:18:47Z","title":"Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides","version":2},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-10T16:33:19.644485Z"},"links":{"cited_paper":"/paper/2211.07002","citing_paper":"/paper/2501.13064"},"observation_digest":"sha256:ec46b7d6affd7157a3fddd7ef110999e8af2a4699caa8b356fca4b03bdbc8bde","observation_id":"5533b227-69b3-4dd6-8191-b5dfb9255fe9","resolution":{"observed_at":"2026-08-10T16:33:19.644485Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2410.03831","last_updated":"2025-03-21T20:51:06Z","snapshot_observed_at":"2026-07-06T19:28:08.374354Z","submitted_at":"2024-10-04T18:01:05Z","title":"Resonance Locking of Anharmonic $g$-Modes in Coalescing Neutron Star Binaries","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2410.03831","snapshot_observed_at":"2026-08-10T16:33:19.652532Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2501.13064","last_updated":"2025-03-07T22:36:49Z","snapshot_observed_at":"2026-08-10T16:40:19.014391Z","submitted_at":"2025-01-22T18:18:47Z","title":"Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides","version":2},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-10T16:33:19.652532Z"},"links":{"cited_paper":"/paper/2410.03831","citing_paper":"/paper/2501.13064"},"observation_digest":"sha256:5b121ae56c186ff09f390ac58d93c0ad9026dcbe5d93fd21791980a58031f399","observation_id":"0b1b0f4e-7c39-440f-804e-b7eceb3a9533","resolution":{"observed_at":"2026-08-10T16:33:19.652532Z","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":"2026-07-06T05:46:13.622041Z","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":"2026-08-10T16:33:19.660242Z","title":"Dietrich, S","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2501.13064","last_updated":"2025-03-07T22:36:49Z","snapshot_observed_at":"2026-08-10T16:40:19.014391Z","submitted_at":"2025-01-22T18:18:47Z","title":"Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides","version":2},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-10T16:33:19.660242Z"},"links":{"cited_paper":"/paper/1706.02969","citing_paper":"/paper/2501.13064"},"observation_digest":"sha256:0b46aaa0d3417b71465a3ed62705255008b5cc1194c60369176bb42d636e608c","observation_id":"755e241e-916e-4972-b095-10fd5da0bf60","resolution":{"observed_at":"2026-08-10T16:33:19.660242Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1802.06518","last_updated":"2018-02-19T05:01:50Z","snapshot_observed_at":"2026-08-01T19:20:23.750149Z","submitted_at":"2018-02-19T05:01:50Z","title":"Frequency-domain gravitational waveform models for inspiraling binary neutron stars","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1802.06518","snapshot_observed_at":"2026-08-10T16:33:19.666617Z","title":"Kawaguchi, K","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2501.13064","last_updated":"2025-03-07T22:36:49Z","snapshot_observed_at":"2026-08-10T16:40:19.014391Z","submitted_at":"2025-01-22T18:18:47Z","title":"Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides","version":2},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-10T16:33:19.666617Z"},"links":{"cited_paper":"/paper/1802.06518","citing_paper":"/paper/2501.13064"},"observation_digest":"sha256:342df5e60b67ac452c16e99c835ac3f9a970b07a7a70ce829553ac4a97560c33","observation_id":"018c2bd8-20f9-4ba6-bc98-ae95ddcfa057","resolution":{"observed_at":"2026-08-10T16:33:19.666617Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1905.06011","last_updated":"2019-07-19T10:05:00Z","snapshot_observed_at":"2026-08-10T08:02:07.993350Z","submitted_at":"2019-05-15T08:05:10Z","title":"Improving the NRTidal model for binary neutron star systems","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1905.06011","snapshot_observed_at":"2026-08-10T16:33:19.673106Z","title":"Dietrich, A","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2501.13064","last_updated":"2025-03-07T22:36:49Z","snapshot_observed_at":"2026-08-10T16:40:19.014391Z","submitted_at":"2025-01-22T18:18:47Z","title":"Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides","version":2},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-10T16:33:19.673106Z"},"links":{"cited_paper":"/paper/1905.06011","citing_paper":"/paper/2501.13064"},"observation_digest":"sha256:77925c163854efde12073ecc238af5353f9e4132ba95510f6846d8c41fc1428f","observation_id":"b8509608-66dd-4528-a239-632e1a532902","resolution":{"observed_at":"2026-08-10T16:33:19.673106Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2307.15125","last_updated":"2023-07-27T18:00:31Z","snapshot_observed_at":"2026-08-08T01:51:25.362825Z","submitted_at":"2023-07-27T18:00:31Z","title":"Analytically improved and numerical-relativity informed effective-one-body model for coalescing binary neutron stars","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2307.15125","snapshot_observed_at":"2026-08-10T16:33:19.679085Z","title":"Gamba, M","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2501.13064","last_updated":"2025-03-07T22:36:49Z","snapshot_observed_at":"2026-08-10T16:40:19.014391Z","submitted_at":"2025-01-22T18:18:47Z","title":"Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides","version":2},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-10T16:33:19.679085Z"},"links":{"cited_paper":"/paper/2307.15125","citing_paper":"/paper/2501.13064"},"observation_digest":"sha256:e464cc69df95f91ff4dc33f7786bdf1b3f193091159c04c93d1f473cf3f02378","observation_id":"751143db-a738-4720-b0dc-764cf750c3e6","resolution":{"observed_at":"2026-08-10T16:33:19.679085Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2205.07577","last_updated":"2024-01-04T16:10:48Z","snapshot_observed_at":"2026-08-07T02:54:02.006407Z","submitted_at":"2022-05-16T11:19:44Z","title":"Rotating Love: The dynamical tides of spinning Newtonian stars","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2205.07577","snapshot_observed_at":"2026-08-10T16:33:19.746630Z","title":"Pnigouras, F","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2501.13064","last_updated":"2025-03-07T22:36:49Z","snapshot_observed_at":"2026-08-10T16:40:19.014391Z","submitted_at":"2025-01-22T18:18:47Z","title":"Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides","version":2},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-08-10T16:33:19.746630Z"},"links":{"cited_paper":"/paper/2205.07577","citing_paper":"/paper/2501.13064"},"observation_digest":"sha256:bb9d1186c6f569dad10b8a009842f15920624573347df74e73f01d179a45c680","observation_id":"ecaf1a6c-f440-46aa-862e-0067bb525e53","resolution":{"observed_at":"2026-08-10T16:33:19.746630Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1905.00818","last_updated":"2019-10-04T08:48:58Z","snapshot_observed_at":"2026-07-06T07:50:00.853773Z","submitted_at":"2019-05-02T15:48:59Z","title":"Frequency domain model of $f$-mode dynamic tides in gravitational waveforms from compact binary inspirals","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1905.00818","snapshot_observed_at":"2026-08-10T16:33:19.692608Z","title":"Schmidt and T","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2501.13064","last_updated":"2025-03-07T22:36:49Z","snapshot_observed_at":"2026-08-10T16:40:19.014391Z","submitted_at":"2025-01-22T18:18:47Z","title":"Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides","version":2},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-08-10T16:33:19.692608Z"},"links":{"cited_paper":"/paper/1905.00818","citing_paper":"/paper/2501.13064"},"observation_digest":"sha256:e67460277d871442bbc0c4286fcf33dc384fe588280aca9a8cb3d1f43928b136","observation_id":"e1345b39-e17e-4c8e-a636-4df1acf7fc81","resolution":{"observed_at":"2026-08-10T16:33:19.692608Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1906.08982","last_updated":"2019-06-21T06:58:14Z","snapshot_observed_at":"2026-08-05T14:12:03.503623Z","submitted_at":"2019-06-21T06:58:14Z","title":"The sum of Love: Exploring the effective tidal deformability of neutron stars","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1906.08982","snapshot_observed_at":"2026-08-10T16:33:19.699926Z","title":"Andersson and P","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2501.13064","last_updated":"2025-03-07T22:36:49Z","snapshot_observed_at":"2026-08-10T16:40:19.014391Z","submitted_at":"2025-01-22T18:18:47Z","title":"Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides","version":2},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-08-10T16:33:19.699926Z"},"links":{"cited_paper":"/paper/1906.08982","citing_paper":"/paper/2501.13064"},"observation_digest":"sha256:dfc15b5ec5e3befafc6b96249c0b41b6a121ff6afabbc3d27fcdc96c14e1d784","observation_id":"6ef0422e-c244-4773-bb14-b02f02895dc9","resolution":{"observed_at":"2026-08-10T16:33:19.699926Z","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":"2026-08-10T16:33:19.706336Z","title":"Andersson and P","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2501.13064","last_updated":"2025-03-07T22:36:49Z","snapshot_observed_at":"2026-08-10T16:40:19.014391Z","submitted_at":"2025-01-22T18:18:47Z","title":"Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides","version":2},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-08-10T16:33:19.706336Z"},"links":{"citing_paper":"/paper/2501.13064"},"observation_digest":"sha256:ec5b37ee76a13f5d6c9333042641c7e39d8cfdf60c9e11664f79add99856762e","observation_id":"c6894710-f6cb-4b5d-aa36-fa861c1ca15c","resolution":{"observed_at":"2026-08-10T16:33:19.706336Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2202.05161","last_updated":"2022-06-19T09:22:41Z","snapshot_observed_at":"2026-07-06T12:36:30.798420Z","submitted_at":"2022-01-31T19:18:54Z","title":"Dynamical tides in superfluid neutron stars","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2202.05161","snapshot_observed_at":"2026-08-10T16:33:19.714349Z","title":"Passamonti, N","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2501.13064","last_updated":"2025-03-07T22:36:49Z","snapshot_observed_at":"2026-08-10T16:40:19.014391Z","submitted_at":"2025-01-22T18:18:47Z","title":"Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides","version":2},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-08-10T16:33:19.714349Z"},"links":{"cited_paper":"/paper/2202.05161","citing_paper":"/paper/2501.13064"},"observation_digest":"sha256:8da45d7c8234e038f2a50e3101aaef53ae0ea44fd0e671d7bcbea1565b3e997a","observation_id":"15a1427b-8814-4387-8ffe-66b95791cdcb","resolution":{"observed_at":"2026-08-10T16:33:19.714349Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2207.13106","last_updated":"2022-07-26T18:00:05Z","snapshot_observed_at":"2026-07-06T13:35:39.787667Z","submitted_at":"2022-07-26T18:00:05Z","title":"Resonant tides in binary neutron star mergers: analytical-numerical relativity study","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2207.13106","snapshot_observed_at":"2026-08-10T16:33:19.725800Z","title":"Gamba and S","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2501.13064","last_updated":"2025-03-07T22:36:49Z","snapshot_observed_at":"2026-08-10T16:40:19.014391Z","submitted_at":"2025-01-22T18:18:47Z","title":"Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides","version":2},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-08-10T16:33:19.725800Z"},"links":{"cited_paper":"/paper/2207.13106","citing_paper":"/paper/2501.13064"},"observation_digest":"sha256:c6df0751262d9fc9088ed561693b9e914239cf1a0baef1b6d751922aa27f7d33","observation_id":"85ccad4f-44e2-4e1f-9867-3f0a6b041b1b","resolution":{"observed_at":"2026-08-10T16:33:19.725800Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2309.04622","last_updated":"2023-09-08T22:22:56Z","snapshot_observed_at":"2026-07-30T16:20:53.887765Z","submitted_at":"2023-09-08T22:22:56Z","title":"The Last Three Seconds: Packed Message delivered by Tides in Binary Neutron Star Mergers","version":1},"cited_work":{"arxiv_id":"2309.04622","doi":null,"metadata_source":"pith","pith_arxiv_id":"2309.04622","snapshot_observed_at":"2026-08-10T16:33:23.432282Z","title":"The Last Three Seconds: Packed Message delivered by Tides in Binary Neutron Star Mergers","venue":"gr-qc","work_id":"beba5dce-a57c-4729-b54b-2910eef5cc8c","year":2023},"citing_paper":{"arxiv_id":"2501.13064","last_updated":"2025-03-07T22:36:49Z","snapshot_observed_at":"2026-08-10T16:40:19.014391Z","submitted_at":"2025-01-22T18:18:47Z","title":"Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides","version":2},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-08-10T16:33:19.734444Z"},"links":{"cited_paper":"/paper/2309.04622","citing_paper":"/paper/2501.13064"},"observation_digest":"sha256:1e013a56c4d142b78d5758f20395612e7690f5cc73db21586a35786a7def447b","observation_id":"14d488e4-f325-41ff-b6fe-a7e4f59694ca","resolution":{"observed_at":"2026-08-10T16:33:23.453271Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2304.02030","last_updated":"2024-02-27T08:27:50Z","snapshot_observed_at":"2026-08-06T01:15:47.948669Z","submitted_at":"2023-04-04T18:00:00Z","title":"Gravitoelectric dynamical tides at second post-Newtonian order","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2304.02030","snapshot_observed_at":"2026-08-10T16:33:19.740424Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2501.13064","last_updated":"2025-03-07T22:36:49Z","snapshot_observed_at":"2026-08-10T16:40:19.014391Z","submitted_at":"2025-01-22T18:18:47Z","title":"Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides","version":2},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-08-10T16:33:19.740424Z"},"links":{"cited_paper":"/paper/2304.02030","citing_paper":"/paper/2501.13064"},"observation_digest":"sha256:f2bbb6efe608c7d54888136cc84dfeb0c832b677f12c2411da4470c3c436f503","observation_id":"41aadd8a-f226-4e47-bb23-f695f33f324c","resolution":{"observed_at":"2026-08-10T16:33:19.740424Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1302.2292","last_updated":"2015-09-25T21:11:08Z","snapshot_observed_at":"2026-07-06T03:06:05.619370Z","submitted_at":"2013-02-10T02:42:37Z","title":"An instability due to the nonlinear coupling of p-modes to g-modes: Implications for coalescing neutron star binaries","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1302.2292","snapshot_observed_at":"2026-08-10T16:33:19.820698Z","title":null,"venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2501.13064","last_updated":"2025-03-07T22:36:49Z","snapshot_observed_at":"2026-08-10T16:40:19.014391Z","submitted_at":"2025-01-22T18:18:47Z","title":"Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides","version":2},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-08-10T16:33:19.820698Z"},"links":{"cited_paper":"/paper/1302.2292","citing_paper":"/paper/2501.13064"},"observation_digest":"sha256:3b3097def7da0be5fa5f77c4d1018eed9f6fcd5b19ae636da8193404fdc00438","observation_id":"56e8a4f9-374e-45d6-bca2-7aba2dddd674","resolution":{"observed_at":"2026-08-10T16:33:19.820698Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2311.04075","last_updated":"2024-03-06T12:38:30Z","snapshot_observed_at":"2026-08-07T00:25:28.575260Z","submitted_at":"2023-11-07T15:40:36Z","title":"General relativistic dynamical tides in binary inspirals, without modes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2311.04075","snapshot_observed_at":"2026-08-10T16:33:19.752772Z","title":"Pitre and E","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2501.13064","last_updated":"2025-03-07T22:36:49Z","snapshot_observed_at":"2026-08-10T16:40:19.014391Z","submitted_at":"2025-01-22T18:18:47Z","title":"Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides","version":2},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-08-10T16:33:19.752772Z"},"links":{"cited_paper":"/paper/2311.04075","citing_paper":"/paper/2501.13064"},"observation_digest":"sha256:dbfbe1065207305bd5eaea4383ee8b3233fcae37808ea48c836ce9658e4f3014","observation_id":"ede7d709-d887-42a7-b169-6b17758b4ef4","resolution":{"observed_at":"2026-08-10T16:33:19.752772Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2311.16561","last_updated":"2024-04-27T16:23:28Z","snapshot_observed_at":"2026-07-06T16:53:39.713988Z","submitted_at":"2023-11-28T07:02:53Z","title":"Cost of inferred nuclear parameters towards the f-mode dynamical tide in binary neutron stars","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2311.16561","snapshot_observed_at":"2026-08-10T16:33:19.758427Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2501.13064","last_updated":"2025-03-07T22:36:49Z","snapshot_observed_at":"2026-08-10T16:40:19.014391Z","submitted_at":"2025-01-22T18:18:47Z","title":"Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides","version":2},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-08-10T16:33:19.758427Z"},"links":{"cited_paper":"/paper/2311.16561","citing_paper":"/paper/2501.13064"},"observation_digest":"sha256:66044e57c41900081137f08267535e9e0725fa0c293dec326ddb657d96bb1a9c","observation_id":"3f3ed5ce-90ba-43be-bfc2-acf3cd106085","resolution":{"observed_at":"2026-08-10T16:33:19.758427Z","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":"2026-08-10T16:33:19.764418Z","title":null,"venue":null,"work_id":null,"year":1978},"citing_paper":{"arxiv_id":"2501.13064","last_updated":"2025-03-07T22:36:49Z","snapshot_observed_at":"2026-08-10T16:40:19.014391Z","submitted_at":"2025-01-22T18:18:47Z","title":"Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides","version":2},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-08-10T16:33:19.764418Z"},"links":{"citing_paper":"/paper/2501.13064"},"observation_digest":"sha256:18f414cdc54b76bbb404d3f2f84781f7bd4b1dd671c71a293db17dab069117e9","observation_id":"10b323d5-661b-4be1-8059-8b4c31547430","resolution":{"observed_at":"2026-08-10T16:33:19.764418Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9404062","last_updated":"1994-04-25T01:31:08Z","snapshot_observed_at":"2026-08-03T14:07:42.352683Z","submitted_at":"1994-04-25T01:31:08Z","title":"Resonant Oscillations and Tidal Heating in Coalescing Binary Neutron Stars","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9404062","snapshot_observed_at":"2026-08-10T16:33:19.770787Z","title":"Lai, Resonant Oscillations and Tidal Heating in Coalescing Binary Neutron Stars, MNRAS 270, 611 (1994), arXiv:astro-ph/9404062 [astro-ph]","venue":null,"work_id":null,"year":1994},"citing_paper":{"arxiv_id":"2501.13064","last_updated":"2025-03-07T22:36:49Z","snapshot_observed_at":"2026-08-10T16:40:19.014391Z","submitted_at":"2025-01-22T18:18:47Z","title":"Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides","version":2},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-08-10T16:33:19.770787Z"},"links":{"cited_paper":"/paper/astro-ph/9404062","citing_paper":"/paper/2501.13064"},"observation_digest":"sha256:ced3a27b4013f1d2d398f0a831fe3efb619db7ee2d7c9bcc68e910b540c028fc","observation_id":"901118d1-3913-42cd-b70a-d811cbdcf6fe","resolution":{"observed_at":"2026-08-10T16:33:19.770787Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/0101092","last_updated":"2001-07-11T21:01:54Z","snapshot_observed_at":"2026-08-10T06:38:01.648898Z","submitted_at":"2001-01-23T23:57:44Z","title":"Nonlinear mode coupling in rotating stars and the r-mode instability in neutron stars","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"gr-qc/0101092","snapshot_observed_at":"2026-08-10T16:33:19.791100Z","title":null,"venue":null,"work_id":null,"year":2002},"citing_paper":{"arxiv_id":"2501.13064","last_updated":"2025-03-07T22:36:49Z","snapshot_observed_at":"2026-08-10T16:40:19.014391Z","submitted_at":"2025-01-22T18:18:47Z","title":"Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides","version":2},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-08-10T16:33:19.791100Z"},"links":{"cited_paper":"/paper/gr-qc/0101092","citing_paper":"/paper/2501.13064"},"observation_digest":"sha256:fa0449cc50c2c3a635a6e519efef5ec87aca980eb6c4446e93d6bc607bf6a487","observation_id":"a3495fd9-30b1-42d5-827a-7fcb81ae4bb3","resolution":{"observed_at":"2026-08-10T16:33:19.791100Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2003.02373","last_updated":"2020-06-04T03:41:46Z","snapshot_observed_at":"2026-08-10T00:44:21.733574Z","submitted_at":"2020-03-04T23:55:04Z","title":"Excitation of f-modes during mergers of spinning binary neutron star","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2003.02373","snapshot_observed_at":"2026-08-10T16:33:19.799899Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2501.13064","last_updated":"2025-03-07T22:36:49Z","snapshot_observed_at":"2026-08-10T16:40:19.014391Z","submitted_at":"2025-01-22T18:18:47Z","title":"Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides","version":2},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-08-10T16:33:19.799899Z"},"links":{"cited_paper":"/paper/2003.02373","citing_paper":"/paper/2501.13064"},"observation_digest":"sha256:38eeedef37c519098ee42384fb7a2f4212d69ab4beb518722b823af2af38f99e","observation_id":"9e44c177-e4b5-4be8-b4c2-535e28e73679","resolution":{"observed_at":"2026-08-10T16:33:19.799899Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2404.00147","last_updated":"2024-07-17T23:48:02Z","snapshot_observed_at":"2026-08-08T10:14:14.519343Z","submitted_at":"2024-03-29T20:41:15Z","title":"Dynamical tides during the inspiral of rapidly spinning neutron stars: Solutions beyond mode resonance","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.00147","snapshot_observed_at":"2026-08-10T16:33:19.809291Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2501.13064","last_updated":"2025-03-07T22:36:49Z","snapshot_observed_at":"2026-08-10T16:40:19.014391Z","submitted_at":"2025-01-22T18:18:47Z","title":"Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides","version":2},"reference_index":54,"source":"pdf_text","source_observed_at":"2026-08-10T16:33:19.809291Z"},"links":{"cited_paper":"/paper/2404.00147","citing_paper":"/paper/2501.13064"},"observation_digest":"sha256:8671ccf6b9eeff054256022db44a8f1e36e65e4d9c3d9c836ad0bca13a310341","observation_id":"0c0c891f-2160-4aba-b271-63c09f8c7da3","resolution":{"observed_at":"2026-08-10T16:33:19.809291Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/9811091","last_updated":"1998-11-26T20:44:21Z","snapshot_observed_at":"2026-07-07T03:29:43.892120Z","submitted_at":"1998-11-26T20:44:21Z","title":"Effective one-body approach to general relativistic two-body dynamics","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"gr-qc/9811091","snapshot_observed_at":"2026-08-10T16:33:19.891211Z","title":"Buonanno and T","venue":null,"work_id":null,"year":1999},"citing_paper":{"arxiv_id":"2501.13064","last_updated":"2025-03-07T22:36:49Z","snapshot_observed_at":"2026-08-10T16:40:19.014391Z","submitted_at":"2025-01-22T18:18:47Z","title":"Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides","version":2},"reference_index":55,"source":"pdf_text","source_observed_at":"2026-08-10T16:33:19.891211Z"},"links":{"cited_paper":"/paper/gr-qc/9811091","citing_paper":"/paper/2501.13064"},"observation_digest":"sha256:825425f2e30451c5c6c9e6edd66d7f1c51eb57a2fb748f52381d163e3bc56d77","observation_id":"90f28da3-4874-42ec-8ec5-58f0d61f1b70","resolution":{"observed_at":"2026-08-10T16:33:19.891211Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1307.2890","last_updated":"2014-01-22T23:29:47Z","snapshot_observed_at":"2026-08-05T23:51:33.403329Z","submitted_at":"2013-07-10T19:51:39Z","title":"The stability of tidally deformed neutron stars to three- and four-mode coupling","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1307.2890","snapshot_observed_at":"2026-08-10T16:33:19.832270Z","title":"Venumadhav, A","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2501.13064","last_updated":"2025-03-07T22:36:49Z","snapshot_observed_at":"2026-08-10T16:40:19.014391Z","submitted_at":"2025-01-22T18:18:47Z","title":"Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides","version":2},"reference_index":56,"source":"pdf_text","source_observed_at":"2026-08-10T16:33:19.832270Z"},"links":{"cited_paper":"/paper/1307.2890","citing_paper":"/paper/2501.13064"},"observation_digest":"sha256:eb51e4e4ca1e9da9a5cc6445b9d0af4b0cf44dc9b2a65849b96af84dfd292790","observation_id":"e463da04-b041-4fae-968b-43e8e5a64169","resolution":{"observed_at":"2026-08-10T16:33:19.832270Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1509.06975","last_updated":"2016-03-07T17:25:41Z","snapshot_observed_at":"2026-08-07T19:20:24.004295Z","submitted_at":"2015-09-22T00:50:45Z","title":"Growth rate of the tidal p-mode g-mode instability in coalescing binary neutron stars","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1509.06975","snapshot_observed_at":"2026-08-10T16:33:19.844614Z","title":null,"venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2501.13064","last_updated":"2025-03-07T22:36:49Z","snapshot_observed_at":"2026-08-10T16:40:19.014391Z","submitted_at":"2025-01-22T18:18:47Z","title":"Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides","version":2},"reference_index":57,"source":"pdf_text","source_observed_at":"2026-08-10T16:33:19.844614Z"},"links":{"cited_paper":"/paper/1509.06975","citing_paper":"/paper/2501.13064"},"observation_digest":"sha256:2e472cb34aee948fd666bd24d177fa49572a5b8f2dcfb2232b09c0c6d4c5a543","observation_id":"2565f0e0-2f87-4eb6-b47d-3b2108097e8b","resolution":{"observed_at":"2026-08-10T16:33:19.844614Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1609.06362","last_updated":"2016-12-02T21:40:59Z","snapshot_observed_at":"2026-08-07T06:19:12.122735Z","submitted_at":"2016-09-20T21:12:44Z","title":"Impact of the tidal p-g instability on the gravitational wave signal from coalescing binary neutron stars","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1609.06362","snapshot_observed_at":"2026-08-10T16:33:19.856662Z","title":"Essick, S","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2501.13064","last_updated":"2025-03-07T22:36:49Z","snapshot_observed_at":"2026-08-10T16:40:19.014391Z","submitted_at":"2025-01-22T18:18:47Z","title":"Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides","version":2},"reference_index":58,"source":"pdf_text","source_observed_at":"2026-08-10T16:33:19.856662Z"},"links":{"cited_paper":"/paper/1609.06362","citing_paper":"/paper/2501.13064"},"observation_digest":"sha256:e0391ec365399282bf4c10f5ae3b0690fd4653ee84d737bab6f8faf4f5af9a89","observation_id":"5bd20257-7f23-4757-9e89-8411c0b06dd4","resolution":{"observed_at":"2026-08-10T16:33:19.856662Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1808.08676","last_updated":"2018-09-19T14:05:01Z","snapshot_observed_at":"2026-07-06T06:57:33.984469Z","submitted_at":"2018-08-27T03:17:05Z","title":"Constraining the p-mode--g-mode tidal instability with GW170817","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1808.08676","snapshot_observed_at":"2026-08-10T16:33:19.864469Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2501.13064","last_updated":"2025-03-07T22:36:49Z","snapshot_observed_at":"2026-08-10T16:40:19.014391Z","submitted_at":"2025-01-22T18:18:47Z","title":"Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides","version":2},"reference_index":59,"source":"pdf_text","source_observed_at":"2026-08-10T16:33:19.864469Z"},"links":{"cited_paper":"/paper/1808.08676","citing_paper":"/paper/2501.13064"},"observation_digest":"sha256:9d58aae25279f9da12cb7ef90881b954e7dda59dcccfcf721324f9cc666d9320","observation_id":"c5c80eee-9c00-4aa7-9706-bd5a651c3aea","resolution":{"observed_at":"2026-08-10T16:33:19.864469Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1806.04163","last_updated":"2018-06-11T18:07:17Z","snapshot_observed_at":"2026-07-06T06:44:13.430115Z","submitted_at":"2018-06-11T18:07:17Z","title":"Urca reactions during neutron star inspiral","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1806.04163","snapshot_observed_at":"2026-08-10T16:33:19.870110Z","title":"Arras and N","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2501.13064","last_updated":"2025-03-07T22:36:49Z","snapshot_observed_at":"2026-08-10T16:40:19.014391Z","submitted_at":"2025-01-22T18:18:47Z","title":"Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides","version":2},"reference_index":60,"source":"pdf_text","source_observed_at":"2026-08-10T16:33:19.870110Z"},"links":{"cited_paper":"/paper/1806.04163","citing_paper":"/paper/2501.13064"},"observation_digest":"sha256:57f48fa8a72aa61096ea5585d25bd9345630092053eb37b26454d15b11030571","observation_id":"9629db00-d14d-4e9f-ac3a-8be7b0aad2ca","resolution":{"observed_at":"2026-08-10T16:33:19.870110Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2407.02584","last_updated":"2025-01-14T10:20:38Z","snapshot_observed_at":"2026-08-09T00:25:29.316269Z","submitted_at":"2024-07-02T18:07:57Z","title":"Dissipative tidal effects to next-to-leading order and constraints on the dissipative tidal deformability using gravitational wave data","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2407.02584","snapshot_observed_at":"2026-08-10T16:33:19.876382Z","title":"Abhishek Hegade K., J","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2501.13064","last_updated":"2025-03-07T22:36:49Z","snapshot_observed_at":"2026-08-10T16:40:19.014391Z","submitted_at":"2025-01-22T18:18:47Z","title":"Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides","version":2},"reference_index":61,"source":"pdf_text","source_observed_at":"2026-08-10T16:33:19.876382Z"},"links":{"cited_paper":"/paper/2407.02584","citing_paper":"/paper/2501.13064"},"observation_digest":"sha256:b3432b708957c45c0bd2786b23b2e32c7f15c27b5546b83cde8be8e58517fab8","observation_id":"2c975ef9-996d-4154-953d-117c7aed0047","resolution":{"observed_at":"2026-08-10T16:33:19.876382Z","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":"2026-08-10T16:33:19.884410Z","title":"Campanelli, C","venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"2501.13064","last_updated":"2025-03-07T22:36:49Z","snapshot_observed_at":"2026-08-10T16:40:19.014391Z","submitted_at":"2025-01-22T18:18:47Z","title":"Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides","version":2},"reference_index":62,"source":"pdf_text","source_observed_at":"2026-08-10T16:33:19.884410Z"},"links":{"citing_paper":"/paper/2501.13064"},"observation_digest":"sha256:ea435cfc76d654140da7d55af9b1190e61b3f5ba3bbc4362f4d01b87df77aa79","observation_id":"1d945dfb-1dd2-4101-b75b-2182a3503262","resolution":{"observed_at":"2026-08-10T16:33:19.884410Z","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":"2026-07-06T06:41:51.126097Z","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":"2026-08-10T16:33:19.956040Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2501.13064","last_updated":"2025-03-07T22:36:49Z","snapshot_observed_at":"2026-08-10T16:40:19.014391Z","submitted_at":"2025-01-22T18:18:47Z","title":"Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides","version":2},"reference_index":63,"source":"pdf_text","source_observed_at":"2026-08-10T16:33:19.956040Z"},"links":{"cited_paper":"/paper/1805.11579","citing_paper":"/paper/2501.13064"},"observation_digest":"sha256:7168074142642774c85b8510742fbb6c17ddf903468496e78af5e845633a01db","observation_id":"1a9a8777-af86-4e22-bb3e-456155035d8b","resolution":{"observed_at":"2026-08-10T16:33:19.956040Z","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":"2026-08-10T16:33:19.897586Z","title":"Douchin and P","venue":null,"work_id":null,"year":2001},"citing_paper":{"arxiv_id":"2501.13064","last_updated":"2025-03-07T22:36:49Z","snapshot_observed_at":"2026-08-10T16:40:19.014391Z","submitted_at":"2025-01-22T18:18:47Z","title":"Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides","version":2},"reference_index":64,"source":"pdf_text","source_observed_at":"2026-08-10T16:33:19.897586Z"},"links":{"cited_paper":"/paper/astro-ph/0111092","citing_paper":"/paper/2501.13064"},"observation_digest":"sha256:f4d1fb284f4aee080fbb3dfb2750bdc7e9b83ce3a755f96494d132391e18d10e","observation_id":"28225e48-fb4d-4ec2-97f0-261510050085","resolution":{"observed_at":"2026-08-10T16:33:19.897586Z","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":"2026-08-10T16:33:19.906876Z","title":"Christensen-Dalsgaard, Lecture Notes on Stellar Oscillations(Institut for Fysik og Astronomi, Aarhus Universitet, 1998)","venue":null,"work_id":null,"year":1998},"citing_paper":{"arxiv_id":"2501.13064","last_updated":"2025-03-07T22:36:49Z","snapshot_observed_at":"2026-08-10T16:40:19.014391Z","submitted_at":"2025-01-22T18:18:47Z","title":"Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides","version":2},"reference_index":65,"source":"pdf_text","source_observed_at":"2026-08-10T16:33:19.906876Z"},"links":{"citing_paper":"/paper/2501.13064"},"observation_digest":"sha256:64cdaa62b92ef22bd20542d063b7b4b6486d692a0ff763db0cab789240aeb7a5","observation_id":"67c3ac72-cbae-4ae5-bc66-b04874dc4aa1","resolution":{"observed_at":"2026-08-10T16:33:19.906876Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/0601029","last_updated":"2007-02-02T21:47:18Z","snapshot_observed_at":"2026-07-07T03:21:58.774337Z","submitted_at":"2006-01-07T23:58:01Z","title":"Gravitomagnetic resonant excitation of Rossby modes in coalescing neutron star binaries","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"gr-qc/0601029","snapshot_observed_at":"2026-08-10T16:33:19.915724Z","title":null,"venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2501.13064","last_updated":"2025-03-07T22:36:49Z","snapshot_observed_at":"2026-08-10T16:40:19.014391Z","submitted_at":"2025-01-22T18:18:47Z","title":"Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides","version":2},"reference_index":66,"source":"pdf_text","source_observed_at":"2026-08-10T16:33:19.915724Z"},"links":{"cited_paper":"/paper/gr-qc/0601029","citing_paper":"/paper/2501.13064"},"observation_digest":"sha256:0465f2c0016edb4c4a49f5b5c60be55cb21f72245b3e2829a006adf90fe4c0d9","observation_id":"4b351916-6519-4170-aebf-1548a91ecd86","resolution":{"observed_at":"2026-08-10T16:33:19.915724Z","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":"2026-08-10T16:33:19.924648Z","title":"Goldstein, C","venue":null,"work_id":null,"year":2002},"citing_paper":{"arxiv_id":"2501.13064","last_updated":"2025-03-07T22:36:49Z","snapshot_observed_at":"2026-08-10T16:40:19.014391Z","submitted_at":"2025-01-22T18:18:47Z","title":"Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides","version":2},"reference_index":67,"source":"pdf_text","source_observed_at":"2026-08-10T16:33:19.924648Z"},"links":{"citing_paper":"/paper/2501.13064"},"observation_digest":"sha256:88f8b3f0359f4728fb829e5f7c86413c32d5573627345fe3c93f78b2228e0386","observation_id":"3b59b1ba-318e-453b-8828-96eb0dcc8d9d","resolution":{"observed_at":"2026-08-10T16:33:19.924648Z","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":"2026-08-10T16:33:19.934875Z","title":"Poisson and C","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2501.13064","last_updated":"2025-03-07T22:36:49Z","snapshot_observed_at":"2026-08-10T16:40:19.014391Z","submitted_at":"2025-01-22T18:18:47Z","title":"Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides","version":2},"reference_index":68,"source":"pdf_text","source_observed_at":"2026-08-10T16:33:19.934875Z"},"links":{"citing_paper":"/paper/2501.13064"},"observation_digest":"sha256:64aa1e003096c750cd450c0398efc930f40530e0939af47d6c410d693347cc48","observation_id":"848db00a-481a-4656-8b5f-0b42ca00e6bb","resolution":{"observed_at":"2026-08-10T16:33:19.934875Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1101.1673","last_updated":"2011-01-09T20:36:19Z","snapshot_observed_at":"2026-07-06T02:21:47.279050Z","submitted_at":"2011-01-09T20:36:19Z","title":"Post-1-Newtonian tidal effects in the gravitational waveform from binary inspirals","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1101.1673","snapshot_observed_at":"2026-08-10T16:33:19.941949Z","title":"Vines, É","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2501.13064","last_updated":"2025-03-07T22:36:49Z","snapshot_observed_at":"2026-08-10T16:40:19.014391Z","submitted_at":"2025-01-22T18:18:47Z","title":"Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides","version":2},"reference_index":69,"source":"pdf_text","source_observed_at":"2026-08-10T16:33:19.941949Z"},"links":{"cited_paper":"/paper/1101.1673","citing_paper":"/paper/2501.13064"},"observation_digest":"sha256:805030180244bd5befc698f288d2fdad0ba92c1a17802b38399969b1a1b4b767","observation_id":"7545718b-2bed-4cb9-9236-4c21c514f4ec","resolution":{"observed_at":"2026-08-10T16:33:19.941949Z","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":"2026-08-10T16:33:19.948963Z","title":null,"venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2501.13064","last_updated":"2025-03-07T22:36:49Z","snapshot_observed_at":"2026-08-10T16:40:19.014391Z","submitted_at":"2025-01-22T18:18:47Z","title":"Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides","version":2},"reference_index":70,"source":"pdf_text","source_observed_at":"2026-08-10T16:33:19.948963Z"},"links":{"cited_paper":"/paper/0812.2163","citing_paper":"/paper/2501.13064"},"observation_digest":"sha256:d2856d432afd198eb1693a3340742ea5c0cb26e4f76bba0715b1d30ea36fce1e","observation_id":"82a1c4f8-1125-4c71-9693-9b8957564c8d","resolution":{"observed_at":"2026-08-10T16:33:19.948963Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1111.5610","last_updated":"2012-02-29T21:58:04Z","snapshot_observed_at":"2026-08-04T20:01:09.060900Z","submitted_at":"2011-11-23T20:58:32Z","title":"The complete non-spinning effective-one-body metric at linear order in the mass ratio","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1111.5610","snapshot_observed_at":"2026-08-10T16:33:20.020976Z","title":"Barausse, A","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2501.13064","last_updated":"2025-03-07T22:36:49Z","snapshot_observed_at":"2026-08-10T16:40:19.014391Z","submitted_at":"2025-01-22T18:18:47Z","title":"Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides","version":2},"reference_index":71,"source":"pdf_text","source_observed_at":"2026-08-10T16:33:20.020976Z"},"links":{"cited_paper":"/paper/1111.5610","citing_paper":"/paper/2501.13064"},"observation_digest":"sha256:2a87d57e7386daf4f7dce72565757f8e1c119ad5406af26fc7b2dd1e510000dc","observation_id":"2d714958-7c72-4c29-b10e-7ccd52a3aa0f","resolution":{"observed_at":"2026-08-10T16:33:20.020976Z","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":"2026-08-10T16:33:19.964070Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2501.13064","last_updated":"2025-03-07T22:36:49Z","snapshot_observed_at":"2026-08-10T16:40:19.014391Z","submitted_at":"2025-01-22T18:18:47Z","title":"Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides","version":2},"reference_index":72,"source":"pdf_text","source_observed_at":"2026-08-10T16:33:19.964070Z"},"links":{"citing_paper":"/paper/2501.13064"},"observation_digest":"sha256:a7dab140d9174c6b2f62c9b9d875719661ef6bb9f51a7938855cbe8497e9caf8","observation_id":"10e12fe8-6760-426c-8662-8d19290148dc","resolution":{"observed_at":"2026-08-10T16:33:19.964070Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1406.2207","last_updated":"2014-06-09T15:00:03Z","snapshot_observed_at":"2026-08-04T08:41:52.718096Z","submitted_at":"2014-06-09T15:00:03Z","title":"Tidal dissipation in stars and giant planets","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1406.2207","snapshot_observed_at":"2026-08-10T16:33:19.970382Z","title":null,"venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2501.13064","last_updated":"2025-03-07T22:36:49Z","snapshot_observed_at":"2026-08-10T16:40:19.014391Z","submitted_at":"2025-01-22T18:18:47Z","title":"Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides","version":2},"reference_index":73,"source":"pdf_text","source_observed_at":"2026-08-10T16:33:19.970382Z"},"links":{"cited_paper":"/paper/1406.2207","citing_paper":"/paper/2501.13064"},"observation_digest":"sha256:46a328b009d3e28e9166e0713e279a6b4874dddebb33594546384ecd67672055","observation_id":"02bfe71d-9db4-4d97-8733-13cfb26249a1","resolution":{"observed_at":"2026-08-10T16:33:19.970382Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2003.04469","last_updated":"2020-05-19T15:37:42Z","snapshot_observed_at":"2026-08-05T22:53:06.171453Z","submitted_at":"2020-03-10T00:06:11Z","title":"Fourth post-Newtonian effective-one-body Hamiltonians with generic spins","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2003.04469","snapshot_observed_at":"2026-08-10T16:33:19.977259Z","title":"Khalil, J","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2501.13064","last_updated":"2025-03-07T22:36:49Z","snapshot_observed_at":"2026-08-10T16:40:19.014391Z","submitted_at":"2025-01-22T18:18:47Z","title":"Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides","version":2},"reference_index":74,"source":"pdf_text","source_observed_at":"2026-08-10T16:33:19.977259Z"},"links":{"cited_paper":"/paper/2003.04469","citing_paper":"/paper/2501.13064"},"observation_digest":"sha256:b8ff4fa77c480ffeff3fc62e43c965243b7d4644bae1a1b47710c5e74c56fd6e","observation_id":"3241e47e-bfa8-4180-b95b-aa782d7534f4","resolution":{"observed_at":"2026-08-10T16:33:19.977259Z","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":"2026-08-10T16:33:19.428239Z","title":"56 and 60) to 1 PN order","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2501.13064","last_updated":"2025-03-07T22:36:49Z","snapshot_observed_at":"2026-08-10T16:40:19.014391Z","submitted_at":"2025-01-22T18:18:47Z","title":"Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides","version":2},"reference_index":75,"source":"pdf_text","source_observed_at":"2026-08-10T16:33:19.428239Z"},"links":{"citing_paper":"/paper/2501.13064"},"observation_digest":"sha256:85e0170ef3dff0d5431e417afa8ae800b4de0fdb44975d28b117095d2be536d2","observation_id":"4940acd1-0e94-4a5a-963d-de40af1c7131","resolution":{"observed_at":"2026-08-10T16:33:19.428239Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1211.1060","last_updated":"2013-01-23T23:47:00Z","snapshot_observed_at":"2026-08-05T10:33:58.996735Z","submitted_at":"2012-11-05T22:28:04Z","title":"First Law of Mechanics for Black Hole Binaries with Spins","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1211.1060","snapshot_observed_at":"2026-08-10T16:33:19.983654Z","title":"Blanchet, A","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2501.13064","last_updated":"2025-03-07T22:36:49Z","snapshot_observed_at":"2026-08-10T16:40:19.014391Z","submitted_at":"2025-01-22T18:18:47Z","title":"Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides","version":2},"reference_index":76,"source":"pdf_text","source_observed_at":"2026-08-10T16:33:19.983654Z"},"links":{"cited_paper":"/paper/1211.1060","citing_paper":"/paper/2501.13064"},"observation_digest":"sha256:1a5f772f5ff1725cb2bdb508dd71cf1c4d4d82b6c70c1972b18cd73011230ed0","observation_id":"24dca6aa-1f9b-44a9-b2b7-353e37c7e1ab","resolution":{"observed_at":"2026-08-10T16:33:19.983654Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/0103018","last_updated":"2001-10-01T14:35:29Z","snapshot_observed_at":"2026-07-07T03:13:50.798072Z","submitted_at":"2001-03-07T08:39:09Z","title":"Coalescence of Two Spinning Black Holes: An Effective One-Body Approach","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"gr-qc/0103018","snapshot_observed_at":"2026-08-10T16:33:19.990616Z","title":"Damour, Coalescence of two spinning black holes: An effective one-body approach, Phys","venue":null,"work_id":null,"year":2001},"citing_paper":{"arxiv_id":"2501.13064","last_updated":"2025-03-07T22:36:49Z","snapshot_observed_at":"2026-08-10T16:40:19.014391Z","submitted_at":"2025-01-22T18:18:47Z","title":"Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides","version":2},"reference_index":77,"source":"pdf_text","source_observed_at":"2026-08-10T16:33:19.990616Z"},"links":{"cited_paper":"/paper/gr-qc/0103018","citing_paper":"/paper/2501.13064"},"observation_digest":"sha256:20618eea1dfd7be3ff171c24f77b97c084d0a6374cab7fa0e0ac2258faf1eb2e","observation_id":"d64f3cc9-8212-4bec-a020-b80bce99dd68","resolution":{"observed_at":"2026-08-10T16:33:19.990616Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/0508067","last_updated":"2005-08-16T21:49:04Z","snapshot_observed_at":"2026-07-07T03:21:23.538211Z","submitted_at":"2005-08-16T21:49:04Z","title":"Transition from inspiral to plunge in precessing binaries of spinning black holes","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"gr-qc/0508067","snapshot_observed_at":"2026-08-10T16:33:19.998462Z","title":"Buonanno, Y","venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"2501.13064","last_updated":"2025-03-07T22:36:49Z","snapshot_observed_at":"2026-08-10T16:40:19.014391Z","submitted_at":"2025-01-22T18:18:47Z","title":"Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides","version":2},"reference_index":78,"source":"pdf_text","source_observed_at":"2026-08-10T16:33:19.998462Z"},"links":{"cited_paper":"/paper/gr-qc/0508067","citing_paper":"/paper/2501.13064"},"observation_digest":"sha256:77827f658c1a6430f1252728718483a05a7701c89111eccb97ef670aecb17b23","observation_id":"7c031143-6935-452c-93f7-b938c81cafe3","resolution":{"observed_at":"2026-08-10T16:33:19.998462Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0704.3550","last_updated":"2007-07-26T15:30:22Z","snapshot_observed_at":"2026-07-06T01:26:42.258173Z","submitted_at":"2007-04-26T14:22:01Z","title":"Final spin of a coalescing black-hole binary: an Effective-One-Body approach","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0704.3550","snapshot_observed_at":"2026-08-10T16:33:20.006977Z","title":"Damour and A","venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2501.13064","last_updated":"2025-03-07T22:36:49Z","snapshot_observed_at":"2026-08-10T16:40:19.014391Z","submitted_at":"2025-01-22T18:18:47Z","title":"Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides","version":2},"reference_index":79,"source":"pdf_text","source_observed_at":"2026-08-10T16:33:20.006977Z"},"links":{"cited_paper":"/paper/0704.3550","citing_paper":"/paper/2501.13064"},"observation_digest":"sha256:cf44dbd09717fba65750f1485b94f8ddca5b26ef023fdd047280d22c644bf2e5","observation_id":"5f1ffd4a-c0b3-4bd4-8047-34a1586cc32e","resolution":{"observed_at":"2026-08-10T16:33:20.006977Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0803.0915","last_updated":"2008-03-06T17:20:27Z","snapshot_observed_at":"2026-07-06T01:35:42.184502Z","submitted_at":"2008-03-06T17:20:27Z","title":"Effective one body approach to the dynamics of two spinning black holes with next-to-leading order spin-orbit coupling","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0803.0915","snapshot_observed_at":"2026-08-10T16:33:20.028150Z","title":"Damour, P","venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2501.13064","last_updated":"2025-03-07T22:36:49Z","snapshot_observed_at":"2026-08-10T16:40:19.014391Z","submitted_at":"2025-01-22T18:18:47Z","title":"Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides","version":2},"reference_index":80,"source":"pdf_text","source_observed_at":"2026-08-10T16:33:20.028150Z"},"links":{"cited_paper":"/paper/0803.0915","citing_paper":"/paper/2501.13064"},"observation_digest":"sha256:e85912366c603ea45c1db27eb7808afeef6b7fae345b1a09b8fe2a4fb27eaddf","observation_id":"59d703cb-cbe7-42df-bdcf-e6ee5563588f","resolution":{"observed_at":"2026-08-10T16:33:20.028150Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1106.1021","last_updated":"2012-03-09T23:33:06Z","snapshot_observed_at":"2026-08-10T07:42:35.528793Z","submitted_at":"2011-06-06T11:19:50Z","title":"Inspiral-merger-ringdown multipolar waveforms of nonspinning black-hole binaries using the effective-one-body formalism","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1106.1021","snapshot_observed_at":"2026-08-10T16:33:20.035647Z","title":null,"venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2501.13064","last_updated":"2025-03-07T22:36:49Z","snapshot_observed_at":"2026-08-10T16:40:19.014391Z","submitted_at":"2025-01-22T18:18:47Z","title":"Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides","version":2},"reference_index":81,"source":"pdf_text","source_observed_at":"2026-08-10T16:33:20.035647Z"},"links":{"cited_paper":"/paper/1106.1021","citing_paper":"/paper/2501.13064"},"observation_digest":"sha256:4be36e13de69b04b040b98dec210fedb02682368c3efab92fe216e974c84b7d7","observation_id":"912f6b0a-77a9-47c8-9d4c-64c01d6ed21e","resolution":{"observed_at":"2026-08-10T16:33:20.035647Z","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":"2026-08-10T16:33:20.043141Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2501.13064","last_updated":"2025-03-07T22:36:49Z","snapshot_observed_at":"2026-08-10T16:40:19.014391Z","submitted_at":"2025-01-22T18:18:47Z","title":"Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides","version":2},"reference_index":82,"source":"pdf_text","source_observed_at":"2026-08-10T16:33:20.043141Z"},"links":{"citing_paper":"/paper/2501.13064"},"observation_digest":"sha256:9c30767c7d3cfd423bf6596d3424aa471dbf3cec636c08a15dad93693a709b26","observation_id":"930bebef-6ea5-4cc3-9886-329af3e19779","resolution":{"observed_at":"2026-08-10T16:33:20.043141Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1009.4919","last_updated":"2014-10-09T02:27:05Z","snapshot_observed_at":"2026-07-06T02:15:53.345163Z","submitted_at":"2010-09-24T19:44:02Z","title":"First-post-Newtonian quadrupole tidal interactions in binary systems","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1009.4919","snapshot_observed_at":"2026-08-10T16:33:20.055218Z","title":null,"venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2501.13064","last_updated":"2025-03-07T22:36:49Z","snapshot_observed_at":"2026-08-10T16:40:19.014391Z","submitted_at":"2025-01-22T18:18:47Z","title":"Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides","version":2},"reference_index":83,"source":"pdf_text","source_observed_at":"2026-08-10T16:33:20.055218Z"},"links":{"cited_paper":"/paper/1009.4919","citing_paper":"/paper/2501.13064"},"observation_digest":"sha256:1b195dd55ffde8e5cdd587883a8012381d83a23ddb23bb6b5f8221c1a9b23c7b","observation_id":"17f6e576-9c7d-4162-8930-9cd4d91d23f8","resolution":{"observed_at":"2026-08-10T16:33:20.055218Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2308.01865","last_updated":"2024-02-27T08:39:22Z","snapshot_observed_at":"2026-08-10T12:44:42.399322Z","submitted_at":"2023-08-03T16:40:41Z","title":"Renormalizing Love: tidal effects at the third post-Newtonian order","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2308.01865","snapshot_observed_at":"2026-08-10T16:33:20.060200Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2501.13064","last_updated":"2025-03-07T22:36:49Z","snapshot_observed_at":"2026-08-10T16:40:19.014391Z","submitted_at":"2025-01-22T18:18:47Z","title":"Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides","version":2},"reference_index":84,"source":"pdf_text","source_observed_at":"2026-08-10T16:33:20.060200Z"},"links":{"cited_paper":"/paper/2308.01865","citing_paper":"/paper/2501.13064"},"observation_digest":"sha256:b60b6e3e14318dc0e4d5c91c22bd4c0d7ac199002882206086c2e12ae254f7b6","observation_id":"986dbb85-703f-4b5f-9652-1456265776df","resolution":{"observed_at":"2026-08-10T16:33:20.060200Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1310.1528","last_updated":"2024-07-12T19:24:23Z","snapshot_observed_at":"2026-07-06T03:24:52.562608Z","submitted_at":"2013-10-06T02:23:37Z","title":"Post-Newtonian Theory for Gravitational Waves","version":6},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1310.1528","snapshot_observed_at":"2026-08-10T16:33:20.068306Z","title":"Blanchet, Gravitational Radiation from Post-Newtonian Sources and Inspiralling Compact Binaries, Living Reviews in Relativity 17, 2 (2014), arXiv:1310.1528 [gr-qc]","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2501.13064","last_updated":"2025-03-07T22:36:49Z","snapshot_observed_at":"2026-08-10T16:40:19.014391Z","submitted_at":"2025-01-22T18:18:47Z","title":"Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides","version":2},"reference_index":85,"source":"pdf_text","source_observed_at":"2026-08-10T16:33:20.068306Z"},"links":{"cited_paper":"/paper/1310.1528","citing_paper":"/paper/2501.13064"},"observation_digest":"sha256:db08b9a3bbe6601fb76da3f03313b5d17478bd38adca90007ad6fa995f78d6de","observation_id":"7471fd88-cae9-4bcb-92a7-719e37c104f4","resolution":{"observed_at":"2026-08-10T16:33:20.068306Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/0602117","last_updated":"2006-05-18T12:30:20Z","snapshot_observed_at":"2026-07-07T03:22:13.853273Z","submitted_at":"2006-02-28T14:36:50Z","title":"Gravitational Recoil during Binary Black Hole Coalescence using the Effective One Body Approach","version":2},"cited_work":{"arxiv_id":"gr-qc/0602117","doi":null,"metadata_source":"pith","pith_arxiv_id":"gr-qc/0602117","snapshot_observed_at":"2026-08-10T16:33:21.997428Z","title":"Gravitational Recoil during Binary Black Hole Coalescence using the Effective One Body Approach","venue":"gr-qc","work_id":"ced4de93-9d2d-4d9e-92a5-3bda9b5afb41","year":2006},"citing_paper":{"arxiv_id":"2501.13064","last_updated":"2025-03-07T22:36:49Z","snapshot_observed_at":"2026-08-10T16:40:19.014391Z","submitted_at":"2025-01-22T18:18:47Z","title":"Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides","version":2},"reference_index":86,"source":"pdf_text","source_observed_at":"2026-08-10T16:33:20.075592Z"},"links":{"cited_paper":"/paper/gr-qc/0602117","citing_paper":"/paper/2501.13064"},"observation_digest":"sha256:a4c6ecde14eac8daa1071226e285bc9173c634c638c6fa3a945dbedd51a18d4f","observation_id":"d3e6a18e-6cc6-40b9-9d08-71e7b010ca4d","resolution":{"observed_at":"2026-08-10T16:33:22.005843Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/9211025","last_updated":"1992-11-19T17:25:06Z","snapshot_observed_at":"2026-07-07T03:24:06.897199Z","submitted_at":"1992-11-19T17:25:06Z","title":"Spin effects in the inspiral of coalescing compact binaries","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"gr-qc/9211025","snapshot_observed_at":"2026-08-10T16:33:20.081659Z","title":null,"venue":null,"work_id":null,"year":1993},"citing_paper":{"arxiv_id":"2501.13064","last_updated":"2025-03-07T22:36:49Z","snapshot_observed_at":"2026-08-10T16:40:19.014391Z","submitted_at":"2025-01-22T18:18:47Z","title":"Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides","version":2},"reference_index":87,"source":"pdf_text","source_observed_at":"2026-08-10T16:33:20.081659Z"},"links":{"cited_paper":"/paper/gr-qc/9211025","citing_paper":"/paper/2501.13064"},"observation_digest":"sha256:9fbc22d93e291aae57320d9ebbc03bf395659c96a1347e89b694206e37aa7c33","observation_id":"8574904f-59c7-4b36-ab51-542756965250","resolution":{"observed_at":"2026-08-10T16:33:20.081659Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0912.3517","last_updated":"2010-02-26T20:25:08Z","snapshot_observed_at":"2026-08-03T18:04:35.184507Z","submitted_at":"2009-12-17T20:56:28Z","title":"An improved effective-one-body Hamiltonian for spinning black-hole binaries","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0912.3517","snapshot_observed_at":"2026-08-10T16:33:20.089980Z","title":"Barausse and A","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2501.13064","last_updated":"2025-03-07T22:36:49Z","snapshot_observed_at":"2026-08-10T16:40:19.014391Z","submitted_at":"2025-01-22T18:18:47Z","title":"Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides","version":2},"reference_index":88,"source":"pdf_text","source_observed_at":"2026-08-10T16:33:20.089980Z"},"links":{"cited_paper":"/paper/0912.3517","citing_paper":"/paper/2501.13064"},"observation_digest":"sha256:9e6fa6dda9e73a96f1d3f38645aa710d659f97c6dcefed2ee22d647949ae9cdf","observation_id":"c2ef7411-f986-436e-8680-d1dc2ad50ad7","resolution":{"observed_at":"2026-08-10T16:33:20.089980Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1107.2904","last_updated":"2011-11-04T16:48:59Z","snapshot_observed_at":"2026-07-06T02:30:54.440299Z","submitted_at":"2011-07-14T19:35:30Z","title":"Extending the effective-one-body Hamiltonian of black-hole binaries to include next-to-next-to-leading spin-orbit couplings","version":2},"cited_work":{"arxiv_id":"1107.2904","doi":null,"metadata_source":"pith","pith_arxiv_id":"1107.2904","snapshot_observed_at":"2026-08-10T16:33:21.860821Z","title":"Extending the effective-one-body Hamiltonian of black-hole binaries to include next-to-next-to-leading spin-orbit couplings","venue":"gr-qc","work_id":"95067ba1-afb4-4df7-8c06-340d62102873","year":2011},"citing_paper":{"arxiv_id":"2501.13064","last_updated":"2025-03-07T22:36:49Z","snapshot_observed_at":"2026-08-10T16:40:19.014391Z","submitted_at":"2025-01-22T18:18:47Z","title":"Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides","version":2},"reference_index":89,"source":"pdf_text","source_observed_at":"2026-08-10T16:33:20.096319Z"},"links":{"cited_paper":"/paper/1107.2904","citing_paper":"/paper/2501.13064"},"observation_digest":"sha256:c463ac9aff44332d592d840bb9f9bab3877e7966b3b9dc52ae645a71b3979f1f","observation_id":"4b7a601b-6047-4b86-be1f-802b8ead30a0","resolution":{"observed_at":"2026-08-10T16:33:21.873000Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1202.0790","last_updated":"2012-08-21T17:39:43Z","snapshot_observed_at":"2026-08-06T06:13:16.638643Z","submitted_at":"2012-02-03T18:06:36Z","title":"Prototype effective-one-body model for nonprecessing spinning inspiral-merger-ringdown waveforms","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1202.0790","snapshot_observed_at":"2026-08-10T16:33:20.102609Z","title":"Taracchini, Y","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2501.13064","last_updated":"2025-03-07T22:36:49Z","snapshot_observed_at":"2026-08-10T16:40:19.014391Z","submitted_at":"2025-01-22T18:18:47Z","title":"Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides","version":2},"reference_index":90,"source":"pdf_text","source_observed_at":"2026-08-10T16:33:20.102609Z"},"links":{"cited_paper":"/paper/1202.0790","citing_paper":"/paper/2501.13064"},"observation_digest":"sha256:8d4278748e7233c79c3c713239d7005561ad7b3eaf3ce919ec99a81f06f8fcac","observation_id":"174a52c2-888f-4097-861e-9950cb465734","resolution":{"observed_at":"2026-08-10T16:33:20.102609Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/9709032","last_updated":"1997-09-12T20:33:28Z","snapshot_observed_at":"2026-08-10T06:43:10.689711Z","submitted_at":"1997-09-12T20:33:28Z","title":"Gravitational waves from inspiraling compact binaries: The quadrupole-moment term","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"gr-qc/9709032","snapshot_observed_at":"2026-08-10T16:33:20.108504Z","title":"Poisson, Gravitational waves from inspiraling compact binaries: The quadrupole-moment term, Phys","venue":null,"work_id":null,"year":1998},"citing_paper":{"arxiv_id":"2501.13064","last_updated":"2025-03-07T22:36:49Z","snapshot_observed_at":"2026-08-10T16:40:19.014391Z","submitted_at":"2025-01-22T18:18:47Z","title":"Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides","version":2},"reference_index":91,"source":"pdf_text","source_observed_at":"2026-08-10T16:33:20.108504Z"},"links":{"cited_paper":"/paper/gr-qc/9709032","citing_paper":"/paper/2501.13064"},"observation_digest":"sha256:94a2d9fd3dfce169908a796b33ba3fbb5b5cd57b8a9e2d79bb2444e07f93d71a","observation_id":"e8cde60f-9cb3-41da-9728-252c414964da","resolution":{"observed_at":"2026-08-10T16:33:20.108504Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1701.06318","last_updated":"2017-09-06T06:10:44Z","snapshot_observed_at":"2026-08-08T10:02:53.920575Z","submitted_at":"2017-01-23T10:20:30Z","title":"Testing the binary black hole nature of a compact binary coalescence","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1701.06318","snapshot_observed_at":"2026-08-10T16:33:20.115996Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2501.13064","last_updated":"2025-03-07T22:36:49Z","snapshot_observed_at":"2026-08-10T16:40:19.014391Z","submitted_at":"2025-01-22T18:18:47Z","title":"Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides","version":2},"reference_index":92,"source":"pdf_text","source_observed_at":"2026-08-10T16:33:20.115996Z"},"links":{"cited_paper":"/paper/1701.06318","citing_paper":"/paper/2501.13064"},"observation_digest":"sha256:90bf08ad0518009897b4566ac92b0b3b40748ad409ee4886d33313e871bbafa8","observation_id":"d63f4c1f-5a07-4592-9cca-5fd619c44b35","resolution":{"observed_at":"2026-08-10T16:33:20.115996Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2407.17560","last_updated":"2025-02-06T09:32:22Z","snapshot_observed_at":"2026-07-06T18:51:32.567284Z","submitted_at":"2024-07-24T18:00:03Z","title":"Observability of dynamical tides in merging eccentric neutron star binaries","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2407.17560","snapshot_observed_at":"2026-08-10T16:33:20.122857Z","title":"Takátsy, B","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2501.13064","last_updated":"2025-03-07T22:36:49Z","snapshot_observed_at":"2026-08-10T16:40:19.014391Z","submitted_at":"2025-01-22T18:18:47Z","title":"Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides","version":2},"reference_index":93,"source":"pdf_text","source_observed_at":"2026-08-10T16:33:20.122857Z"},"links":{"cited_paper":"/paper/2407.17560","citing_paper":"/paper/2501.13064"},"observation_digest":"sha256:5ee0ca372952be3d6f25824fbdf2271ee2ccf573cfa3af6d85b052b57503c24b","observation_id":"877dd6b8-3fa7-4804-bbea-7f525793aecb","resolution":{"observed_at":"2026-08-10T16:33:20.122857Z","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":"2026-08-10T16:33:20.130335Z","title":"Haberland, J","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2501.13064","last_updated":"2025-03-07T22:36:49Z","snapshot_observed_at":"2026-08-10T16:40:19.014391Z","submitted_at":"2025-01-22T18:18:47Z","title":"Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides","version":2},"reference_index":94,"source":"pdf_text","source_observed_at":"2026-08-10T16:33:20.130335Z"},"links":{"citing_paper":"/paper/2501.13064"},"observation_digest":"sha256:4159d37c9cbd18c94b495b4abe2e6c9d1d2d89fe6730e0d57420be63563540e7","observation_id":"6e28d92d-6fff-4bcb-9812-61db95cd36cc","resolution":{"observed_at":"2026-08-10T16:33:20.130335Z","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":"2026-08-10T16:33:20.137921Z","title":"Reisenegger and P","venue":null,"work_id":null,"year":1994},"citing_paper":{"arxiv_id":"2501.13064","last_updated":"2025-03-07T22:36:49Z","snapshot_observed_at":"2026-08-10T16:40:19.014391Z","submitted_at":"2025-01-22T18:18:47Z","title":"Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides","version":2},"reference_index":95,"source":"pdf_text","source_observed_at":"2026-08-10T16:33:20.137921Z"},"links":{"citing_paper":"/paper/2501.13064"},"observation_digest":"sha256:4490de56c8e70395b2cc68e5ae8b42457eacf8ee7062a53014870f25caeb6713","observation_id":"cf02d283-fcea-418d-b3b0-35360965e84e","resolution":{"observed_at":"2026-08-10T16:33:20.137921Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1610.00745","last_updated":"2016-12-04T19:59:19Z","snapshot_observed_at":"2026-07-06T05:13:10.794189Z","submitted_at":"2016-10-03T20:51:10Z","title":"Resonant tidal excitation of superfluid neutron stars in coalescing binaries","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1610.00745","snapshot_observed_at":"2026-08-10T16:33:20.145963Z","title":"Yu and N","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2501.13064","last_updated":"2025-03-07T22:36:49Z","snapshot_observed_at":"2026-08-10T16:40:19.014391Z","submitted_at":"2025-01-22T18:18:47Z","title":"Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides","version":2},"reference_index":96,"source":"pdf_text","source_observed_at":"2026-08-10T16:33:20.145963Z"},"links":{"cited_paper":"/paper/1610.00745","citing_paper":"/paper/2501.13064"},"observation_digest":"sha256:cb1777586e3938918f62c119008bd3eaff6a103ea509b09ea449e0c4e578d5d5","observation_id":"75955737-e8cd-4bd2-9e09-ff4b8cf83b6b","resolution":{"observed_at":"2026-08-10T16:33:20.145963Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1705.04700","last_updated":"2017-06-28T18:00:06Z","snapshot_observed_at":"2026-07-06T05:42:27.622788Z","submitted_at":"2017-05-12T18:01:55Z","title":"Dynamical tides in coalescing superfluid neutron star binaries with hyperon cores and their detectability with third generation gravitational-wave detectors","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1705.04700","snapshot_observed_at":"2026-08-10T16:33:20.154011Z","title":"Yu and N","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2501.13064","last_updated":"2025-03-07T22:36:49Z","snapshot_observed_at":"2026-08-10T16:40:19.014391Z","submitted_at":"2025-01-22T18:18:47Z","title":"Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides","version":2},"reference_index":97,"source":"pdf_text","source_observed_at":"2026-08-10T16:33:20.154011Z"},"links":{"cited_paper":"/paper/1705.04700","citing_paper":"/paper/2501.13064"},"observation_digest":"sha256:fe7a682212b563a8742773d923dd5b7132ce63e72aecdafcb6fc330920832a0a","observation_id":"c0db9493-7b6c-4f5b-a717-0ecc836b99a7","resolution":{"observed_at":"2026-08-10T16:33:20.154011Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2106.16123","last_updated":"2021-06-30T15:20:39Z","snapshot_observed_at":"2026-08-10T07:12:31.833686Z","submitted_at":"2021-06-30T15:20:39Z","title":"General-relativistic treatment of tidal $g$-mode resonances in coalescing binaries of neutron stars. I. Theoretical framework and crust breaking","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2106.16123","snapshot_observed_at":"2026-08-10T16:33:20.161162Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2501.13064","last_updated":"2025-03-07T22:36:49Z","snapshot_observed_at":"2026-08-10T16:40:19.014391Z","submitted_at":"2025-01-22T18:18:47Z","title":"Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides","version":2},"reference_index":98,"source":"pdf_text","source_observed_at":"2026-08-10T16:33:20.161162Z"},"links":{"cited_paper":"/paper/2106.16123","citing_paper":"/paper/2501.13064"},"observation_digest":"sha256:8e126b9e1bc77b1c80dee2eb02a577826f5d71665af868dcf086ef48a7774b40","observation_id":"90161a59-6e8c-49a1-86ce-1d73506063ed","resolution":{"observed_at":"2026-08-10T16:33:20.161162Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2107.00533","last_updated":"2021-09-14T11:48:52Z","snapshot_observed_at":"2026-08-05T00:07:22.921283Z","submitted_at":"2021-07-01T15:24:49Z","title":"General-relativistic treatment of tidal $g$-mode resonances in coalescing binaries of neutron stars. II. As triggers for precursor flares of short gamma-ray bursts","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2107.00533","snapshot_observed_at":"2026-08-10T16:33:20.168234Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2501.13064","last_updated":"2025-03-07T22:36:49Z","snapshot_observed_at":"2026-08-10T16:40:19.014391Z","submitted_at":"2025-01-22T18:18:47Z","title":"Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides","version":2},"reference_index":99,"source":"pdf_text","source_observed_at":"2026-08-10T16:33:20.168234Z"},"links":{"cited_paper":"/paper/2107.00533","citing_paper":"/paper/2501.13064"},"observation_digest":"sha256:fbe6a694f2e4e5c1ba19653e80a5715278bef9abc7cfc590a581a75a25390c53","observation_id":"aaba65bb-109c-43a7-914d-950596493d36","resolution":{"observed_at":"2026-08-10T16:33:20.168234Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2409.20178","last_updated":"2024-09-30T10:42:04Z","snapshot_observed_at":"2026-08-08T13:30:17.498530Z","submitted_at":"2024-09-30T10:42:04Z","title":"Neutron star g-modes in the relativistic Cowling approximation","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2409.20178","snapshot_observed_at":"2026-08-10T16:33:20.174351Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2501.13064","last_updated":"2025-03-07T22:36:49Z","snapshot_observed_at":"2026-08-10T16:40:19.014391Z","submitted_at":"2025-01-22T18:18:47Z","title":"Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides","version":2},"reference_index":100,"source":"pdf_text","source_observed_at":"2026-08-10T16:33:20.174351Z"},"links":{"cited_paper":"/paper/2409.20178","citing_paper":"/paper/2501.13064"},"observation_digest":"sha256:d281d3a7b90745ffa832cb7dcf84284303d18591efc41681609aa39acc61b3ee","observation_id":"2f704d18-e740-401d-9eb9-c52b232b2b9a","resolution":{"observed_at":"2026-08-10T16:33:20.174351Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"2501.13064","last_updated":"2025-03-07T22:36:49Z","latest_version":2,"primary_category":"gr-qc","snapshot_observed_at":"2026-08-10T16:40:19.014391Z","submitted_at":"2025-01-22T18:18:47Z","title":"Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides"},"reference_resolution":{"displayed":100,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":97,"verified_exact":3,"verified_fuzzy":0},"total_outbound_references":129},"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":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"thesis":"As of 11 August 2026, this Paper Citation Record lists 100 of 129 outbound references and 5 inbound Pith citation observations for arXiv:2501.13064."}