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Paper Citation Record · LEDGER

Equilibrium sequences of differentially rotating stars with post-merger-like rotational profiles

As of 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2011.10612.

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

pith.paper-citation-record.v1
2011.10612 v3

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 3 of 3 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 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-09T00:07:29.672082Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-03T22:08:58.790454Z

Reference resolution

0 of 0 outbound references displayed

  • verified exact0
  • verified fuzzy0
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  • 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 961f1c6c-8201-49ec-8e08-f362b67658d9 · inbound

General-relativistic resistive-magnetohydrodynamics simulations of self-consistent magnetized rotating neutron stars cites this paper.

General-relativistic resistive-magnetohydrodynamics simulations of self-consistent magnetized rotating neutron stars Equilibrium sequences of differentially rotating stars with post-merger-like rotational profiles

Reference 68

Resolution
verified exact
arxiv_id, observed 2026-05-09T04:41:37.832939Z

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=2026-05-23T20:56:06.983493Z digest=sha256:ded3cdf3a63d7267bb5a87215276434e40b2856f5b29d04991c664d649eec2b3

Observation c7048adf-e343-4b19-a330-a175e56f4908 · 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 Equilibrium sequences of differentially rotating stars with post-merger-like rotational profiles

Reference 64

Resolution
unresolved
no resolver link, observed 2026-08-09T00:07:29.672082Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-09T00:07:29.672082Z digest=sha256:948ef467b641ca75b56ae23b80165678864112436aac38030a5663f8f2c06fc5

Observation b7f0ad07-787e-4d64-a11b-9b2d34bc7705 · inbound

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

Hybrid Stars with Post-Merger Rotation Profiles Equilibrium sequences of differentially rotating stars with post-merger-like rotational profiles

Reference 18

Resolution
verified exact
arxiv_id, observed 2026-07-03T22:08:58.792269Z

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=sha256:3c274ba9ee18a4bfcd1e391675d317d67c8c61ba47f03666eaa8c4f05966ed48