Paper Citation Record · LEDGER

Interpreting Binary Neutron Star Mergers: Describing the Binary Neutron Star Dynamics, Modelling Gravitational Waveforms, and Analyzing Detections

As of 18 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 7 inbound Pith citation observations for arXiv:2004.02527.

A citation records a reference. It does not transfer a finding from one paper to another.

pith.paper-citation-record.v1
2004.02527 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 7 of 7 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-18T06:34:40.430872+00:00

measured 7 of 7 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-12T14:17:14.711406Z

measured 0 of 1 external citation measurements

A source-named dated measurement, never combined with another source.

Source: arxiv_reference, observed 2026-07-02T15:27:05.902640Z

Reference resolution

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External citation measurements

No source-named external measurement is stored.

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 3c42fbd7-2841-4af5-825c-9af6ef263a16 · inbound

Null Stream Based Third-generation-ready Glitch Mitigation for Gravitational Wave Measurements cites this paper.

Null Stream Based Third-generation-ready Glitch Mitigation for Gravitational Wave Measurements Interpreting Binary Neutron Star Mergers: Describing the Binary Neutron Star Dynamics, Modelling Gravitational Waveforms, and Analyzing Detections

Reference 50

Resolution: unresolved; no resolver link, observed 2026-08-12T14:17:14.711406Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 1f883f7e-dc24-4405-bfc9-5a14ca2ed5ea · inbound

Applications of machine learning in gravitational wave research with current interferometric detectors cites this paper.

Applications of machine learning in gravitational wave research with current interferometric detectors Interpreting Binary Neutron Star Mergers: Describing the Binary Neutron Star Dynamics, Modelling Gravitational Waveforms, and Analyzing Detections

Reference 152

Resolution: unresolved; no resolver link, observed 2026-08-11T11:42:50.173337Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 1445a76c-c35d-4b21-a5c7-19a29941bd35 · inbound

The error budget of binary neutron star merger simulations for configurations with high spin cites this paper.

The error budget of binary neutron star merger simulations for configurations with high spin Interpreting Binary Neutron Star Mergers: Describing the Binary Neutron Star Dynamics, Modelling Gravitational Waveforms, and Analyzing Detections

Reference 5

Resolution: unresolved; no resolver link, observed 2026-08-07T11:38:32.395591Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation bacfdbf6-8cbc-4450-8887-793b2e1843aa · inbound

Binary black holes in the heat of merger cites this paper.

Binary black holes in the heat of merger Interpreting Binary Neutron Star Mergers: Describing the Binary Neutron Star Dynamics, Modelling Gravitational Waveforms, and Analyzing Detections

Reference 48

Resolution: verified exact; arxiv_id, observed 2026-05-19T07:52:09.587750Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

Observation d648670d-9d1f-4f65-ac99-a970ed4cb23d · inbound

Distinguishing Neutron Star vs. Low-Mass Black Hole Binaries with Late Inspiral & Postmerger Gravitational Waves $-$ Sensitivity to Transmuted Black Holes and Non-Annihilating Dark Matter cites this paper.

Distinguishing Neutron Star vs. Low-Mass Black Hole Binaries with Late Inspiral & Postmerger Gravitational Waves $-$ Sensitivity to Transmuted Black Holes and Non-Annihilating Dark Matter Interpreting Binary Neutron Star Mergers: Describing the Binary Neutron Star Dynamics, Modelling Gravitational Waveforms, and Analyzing Detections

Reference 86

Resolution: verified exact; arxiv_id, observed 2026-05-19T03:47:02.246786Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

Observation 319aff20-6206-471e-b54f-1ac799f7591d · inbound

Remnant properties of binary neutron star mergers undergoing prompt collapse cites this paper.

Remnant properties of binary neutron star mergers undergoing prompt collapse Interpreting Binary Neutron Star Mergers: Describing the Binary Neutron Star Dynamics, Modelling Gravitational Waveforms, and Analyzing Detections

Reference 87

Resolution: unresolved; no resolver link, observed 2026-08-06T14:25:06.070000Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation d1bd87fa-bb9c-4211-b538-6d82daae06ed · inbound

Radial Oscillations of Viscous Stars at Finite Temperature cites this paper.

Radial Oscillations of Viscous Stars at Finite Temperature Interpreting Binary Neutron Star Mergers: Describing the Binary Neutron Star Dynamics, Modelling Gravitational Waveforms, and Analyzing Detections

Reference 10

Resolution: verified exact; arxiv_id, observed 2026-07-02T15:27:05.904027Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.