Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Simulation of merging binary neutron stars in full general relativity: $\Gamma=2$ case
As of 21 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 8 inbound Pith citation observations for arXiv:gr-qc/9911058.
A citation records a reference. It does not transfer a finding from one paper to another.
Coverage vector
One-hop event checks from named stored sources.
Source: scholarly_work_events, retraction_status_cache, observed 2026-08-21T06:32:19.484+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-16T00:30:58.673512Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-07-08T20:35:34.287367Z
Reference resolution
0 of 0 outbound references displayed
- verified exact0
- verified fuzzy0
- unresolved0
- parse uncertain0
- malformed identifier0
- metadata mismatch0
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 16617f2d-e617-4292-b21d-035a5a002a66 · inbound
Quasinormal modes of black holes and black branes cites this paper.
Quasinormal modes of black holes and black branes Simulation of merging binary neutron stars in full general relativity: $\Gamma=2$ case
Reference 94
- Resolution
- verified exact
- arxiv_id, observed 2026-05-12T00:59:53.195437Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.
Observation 79a211fb-d473-47ad-964c-ebaa9ce806a0 · inbound
Phase transitions in neutron stars and their links to gravitational waves cites this paper.
Phase transitions in neutron stars and their links to gravitational waves Simulation of merging binary neutron stars in full general relativity: $\Gamma=2$ case
Reference 204
- Resolution
- verified exact
- local_arxiv, observed 2026-05-25T01:55:12.811915Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.
Observation 6844494d-7126-4c65-a174-09b0c4829640 · inbound
Inferring prompt black-hole formation in neutron star mergers from gravitational-wave data cites this paper.
Inferring prompt black-hole formation in neutron star mergers from gravitational-wave data Simulation of merging binary neutron stars in full general relativity: $\Gamma=2$ case
Reference 23
- Resolution
- unresolved
- no resolver link, observed 2026-08-14T13:18:06.986809Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation a80180d8-18cd-4248-a888-ee1343988a00 · inbound
kiloHertz gravitational waves from binary neutron star remnants: time-domain model and constraints on extreme matter cites this paper.
kiloHertz gravitational waves from binary neutron star remnants: time-domain model and constraints on extreme matter Simulation of merging binary neutron stars in full general relativity: $\Gamma=2$ case
Reference 17
- Resolution
- unresolved
- no resolver link, observed 2026-08-14T10:20:11.466819Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 8f0bf705-ed26-4b0e-9b09-0495394c2594 · inbound
Solving Hamiltonian Constraint Equation with Physics-Informed Neural Networks cites this paper.
Solving Hamiltonian Constraint Equation with Physics-Informed Neural Networks Simulation of merging binary neutron stars in full general relativity: $\Gamma=2$ case
Reference 38
- Resolution
- verified exact
- local_arxiv, observed 2026-07-08T20:35:34.288869Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.
Observation b179ec8d-49d6-4b78-bc8d-324499432126 · inbound
GRACE: An Open-Source Framework for GPU-Accelerated Numerical Relativity cites this paper.
GRACE: An Open-Source Framework for GPU-Accelerated Numerical Relativity Simulation of merging binary neutron stars in full general relativity: $\Gamma=2$ case
Reference 5
- Resolution
- unresolved
- no resolver link, observed 2026-07-14T15:02:35.854356Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation d22d3368-c2dd-404c-81d6-a1b883026486 · inbound
Transport Properties of the MRI in Differentially Rotating Neutron Stars cites this paper.
Transport Properties of the MRI in Differentially Rotating Neutron Stars Simulation of merging binary neutron stars in full general relativity: $\Gamma=2$ case
Reference 8
- Resolution
- unresolved
- no resolver link, observed 2026-07-31T14:28:12.534458Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation b57d55a4-ffaa-40eb-8ae4-d24a4aa0538a · inbound
Taiji Resolving Power for the Transverse Scalar Mode of Gravitational Waves cites this paper.
Taiji Resolving Power for the Transverse Scalar Mode of Gravitational Waves Simulation of merging binary neutron stars in full general relativity: $\Gamma=2$ case
Reference 6
- Resolution
- unresolved
- no resolver link, observed 2026-08-16T00:30:58.673512Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.