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Paper Citation Record · LEDGER

On the stability and maximum mass of differentially rotating relativistic stars

As of 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1709.06058.

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

pith.paper-citation-record.v1
1709.06058 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 2 of 2 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-10T06:31:04.303077+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-09T00:07:29.627697Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-03T21:58:59.630644Z

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 645953d0-397a-4811-b124-82913428ab3a · inbound

Axisymmetric stability of neutron stars as extreme rotators in massive scalar-tensor theory cites this paper.

Axisymmetric stability of neutron stars as extreme rotators in massive scalar-tensor theory On the stability and maximum mass of differentially rotating relativistic stars

Reference 48

Resolution
unresolved
no resolver link, observed 2026-08-09T00:07:29.627697Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-09T00:07:29.627697Z digest=sha256:fd56c3de7786cadf6e3f3f628938543cffbfc62321eb9416f49c018f890b47b2

Observation 1a74b729-5214-4315-9b9e-0b5e822933eb · inbound

Hybrid Stars with Post-Merger Rotation Profiles cites this paper.

Hybrid Stars with Post-Merger Rotation Profiles On the stability and maximum mass of differentially rotating relativistic stars

Reference 21

Resolution
verified exact
local_arxiv, observed 2026-07-03T21:58:59.631854Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

source=pdf_text observed=2026-06-26T23:50:12.361235Z digest=sha256:fdd1b7ef0b495d5509ae97fd5d7a799bbc1a1b456d957834235108cd519067f2