Paper Citation Record · LEDGER

Fast Rotating Relativistic Stars: Spectra and Stability without Approximation

As of 13 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:1910.08370.

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

pith.paper-citation-record.v1
1910.08370 v3

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 2026-08-13T06:32:02.005865+00:00

measured 4 of 4 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-10T16:33:19.627422Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-10T15:07:19.451894Z

Reference resolution

0 of 0 outbound references displayed

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verified fuzzy0
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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 5aa0902f-c0d5-48bd-a1f8-a5c069637a16 · inbound

Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides cites this paper.

Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides Fast Rotating Relativistic Stars: Spectra and Stability without Approximation

Reference 23

Resolution: unresolved; no resolver link, observed 2026-08-10T16:33:19.627422Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 279ac13b-0de8-4ab2-9c8b-40ef5ce5df54 · 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 Fast Rotating Relativistic Stars: Spectra and Stability without Approximation

Reference 87

Resolution: unresolved; no resolver link, observed 2026-08-07T11:40:35.696738Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 64bedb7e-b533-4815-83ac-c865c9566ef2 · inbound

Magnetic effects on fundamental modes in rotating neutron stars with a purely toroidal magnetic field cites this paper.

Magnetic effects on fundamental modes in rotating neutron stars with a purely toroidal magnetic field Fast Rotating Relativistic Stars: Spectra and Stability without Approximation

Reference 53

Resolution: unresolved; no resolver link, observed 2026-08-04T18:11:08.850822Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation df7b6cfb-a6e2-49e1-a23f-ab59b5c46e45 · inbound

Nonlinear hydrodynamics in spinning neutron stars: Theoretical universal relations and equilibrium solutions cites this paper.

Nonlinear hydrodynamics in spinning neutron stars: Theoretical universal relations and equilibrium solutions Fast Rotating Relativistic Stars: Spectra and Stability without Approximation

Reference 86

Resolution: verified exact; local_arxiv, observed 2026-07-10T15:07:19.453116Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.