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Paper Citation Record · LEDGER

High-resolution numerical relativity simulations of spinning binary neutron star mergers

As of 15 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:1803.07965.

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

pith.paper-citation-record.v1
1803.07965 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 4 of 4 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-14T06:32:32.682623+00:00

measured 4 of 4 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-14T14:29:00.681307Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-08-07T11:41:21.018654Z

Reference resolution

0 of 0 outbound references displayed

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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 f8b90ebc-f798-4afa-bf47-78a0daee5a1a · inbound

Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity cites this paper.

Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity High-resolution numerical relativity simulations of spinning binary neutron star mergers

Reference 79

Resolution
unresolved
no resolver link, observed 2026-08-14T14:29:00.681307Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T14:29:00.681307Z digest=sha256:78f359f60a1ab0b2b49883120316e4830a82143d7b2056a0c5a2b769e23dfee4

Observation b88f1592-33d3-4ae9-83c3-c9a3c7a31c36 · inbound

Rotating neutron stars with non-barotropic thermal profile cites this paper.

Rotating neutron stars with non-barotropic thermal profile High-resolution numerical relativity simulations of spinning binary neutron star mergers

Reference 65

Resolution
unresolved
no resolver link, observed 2026-08-14T10:30:45.141690Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T10:30:45.141690Z digest=sha256:6f7f71b325746bf076a26aa713807a1baade84de3fbbe6883dddf242724d0139

Observation b398260b-0266-43b5-8b0b-916024d975c8 · inbound

Cooling binary neutron star remnants via nucleon-nucleon-axion bremsstrahlung cites this paper.

Cooling binary neutron star remnants via nucleon-nucleon-axion bremsstrahlung High-resolution numerical relativity simulations of spinning binary neutron star mergers

Reference 80

Resolution
unresolved
no resolver link, observed 2026-08-14T05:28:09.113603Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T05:28:09.113603Z digest=sha256:0279966e38dd55243e3154682b3d50cbb75e61cddc5fcfb3e4d3b1db34f7fc12

Observation 86d96897-d2ba-4472-b053-2a164f8482f5 · 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 High-resolution numerical relativity simulations of spinning binary neutron star mergers

Reference 114

Resolution
verified exact
local_arxiv, observed 2026-08-07T11:41:21.025043Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

source=pdf_text observed=2026-08-07T11:40:58.217117Z digest=sha256:ac111a0e1acc8f8b87d679f03fc2ff50b8450e31e6031525758770c42c498a31