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Paper Citation Record · LEDGER

On the Maximum Mass of Differentially Rotating Neutron Stars

As of 14 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 6 inbound Pith citation observations for arXiv:astro-ph/9910565.

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

pith.paper-citation-record.v1
astro-ph/9910565 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 6 of 6 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 6 of 6 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-14T13:18:07.098465Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-12T05:18:35.618520Z

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 b27c67da-3d3a-46de-bf79-b26fc94a1a4d · 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 On the Maximum Mass of Differentially Rotating Neutron Stars

Reference 63

Resolution
unresolved
no resolver link, observed 2026-08-14T13:18:07.098465Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation 8e874713-aac3-442a-8422-eaeffb836062 · inbound

Connecting GRBs from Binary Neutron Star Mergers to Nuclear Properties of Neutron Stars cites this paper.

Connecting GRBs from Binary Neutron Star Mergers to Nuclear Properties of Neutron Stars On the Maximum Mass of Differentially Rotating Neutron Stars

Reference 72

Resolution
unresolved
no resolver link, observed 2026-08-11T18:36:01.041687Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation b5295c13-f461-48e3-bcd8-18b416b9bee1 · inbound

Neutrinos from explosive transients at the dawn of multi-messenger astronomy cites this paper.

Neutrinos from explosive transients at the dawn of multi-messenger astronomy On the Maximum Mass of Differentially Rotating Neutron Stars

Reference 136

Resolution
unresolved
no resolver link, observed 2026-08-11T16:53:00.982583Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation bccc1e86-587a-40ab-b5a5-f2d56147af98 · 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 On the Maximum Mass of Differentially Rotating Neutron Stars

Reference 91

Resolution
unresolved
no resolver link, observed 2026-08-04T18:11:12.827883Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-04T18:11:12.827883Z digest=sha256:9d76fdd5950ac367100a649c7da58ac2f8439c63d1787cdef3524275524024bd

Observation 1b0f3218-4c8c-4112-bb4e-8595fa1d510f · inbound

nmma: An extended Bayesian framework for Nuclear Multimessenger Astronomy in the Era of Next-Generation Detectors cites this paper.

nmma: An extended Bayesian framework for Nuclear Multimessenger Astronomy in the Era of Next-Generation Detectors On the Maximum Mass of Differentially Rotating Neutron Stars

Reference 27

Resolution
verified exact
local_arxiv, observed 2026-07-12T05:18:35.620131Z

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=arxiv_source observed=2026-07-12T05:14:58.841553Z digest=sha256:64218c761a781f8de06f2ca3773947488dddf72333a38de8318982fca700f86e

Observation 26a62928-0ff7-458d-a4e9-a4aee956a7e6 · inbound

GRACE: An Open-Source Framework for GPU-Accelerated Numerical Relativity cites this paper.

GRACE: An Open-Source Framework for GPU-Accelerated Numerical Relativity On the Maximum Mass of Differentially Rotating Neutron Stars

Reference 129

Resolution
unresolved
no resolver link, observed 2026-07-14T15:02:35.854356Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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