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Paper Citation Record · LEDGER

Long-term evolution of a merger-remnant neutron star in general relativistic magnetohydrodynamics I: Effect of magnetic winding

As of 9 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:2102.01346.

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

pith.paper-citation-record.v1
2102.01346 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 5 of 5 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-09T06:31:02.800959+00:00

measured 5 of 5 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-09T05:33:08.101891Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-03T13:08:08.605758Z

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 7e80ca59-6421-473c-91f1-a874c19bdfc8 · 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 Long-term evolution of a merger-remnant neutron star in general relativistic magnetohydrodynamics I: Effect of magnetic winding

Reference 58

Resolution
verified exact
arxiv_id, observed 2026-05-09T04:41:38.306229Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

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Observation 977cf1b2-871d-40a9-ba20-b7a8d1b73a52 · inbound

SACRA-2D: New axisymmetric general relativistic hydrodynamics code with fixed mesh refinement cites this paper.

SACRA-2D: New axisymmetric general relativistic hydrodynamics code with fixed mesh refinement Long-term evolution of a merger-remnant neutron star in general relativistic magnetohydrodynamics I: Effect of magnetic winding

Reference 75

Resolution
unresolved
no resolver link, observed 2026-08-09T05:33:08.101891Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-09T05:33:08.101891Z digest=sha256:6a506b52f7fb825b894fa7f82dd55af7530f37c3edf3cc66e12e899aeb6b4edc

Observation 9c0b8b16-5935-4310-99b8-d25cc9bc7869 · inbound

Neutrino pair annihilation driven jets from black-hole torus systems cites this paper.

Neutrino pair annihilation driven jets from black-hole torus systems Long-term evolution of a merger-remnant neutron star in general relativistic magnetohydrodynamics I: Effect of magnetic winding

Reference 43

Resolution
unresolved
no resolver link, observed 2026-08-07T11:41:25.639967Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T11:41:25.639967Z digest=sha256:03cb65638638658dc1c102f1bea84b9d66054c1f8cfc25daedef45491e43b6e8

Observation a2a8eaa0-3449-4e0b-ab06-10a9a17a9822 · inbound

A magnetar formation in binary neutron star merger cites this paper.

A magnetar formation in binary neutron star merger Long-term evolution of a merger-remnant neutron star in general relativistic magnetohydrodynamics I: Effect of magnetic winding

Reference 119

Resolution
verified exact
arxiv_id, observed 2026-07-03T07:37:44.749074Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

source=pdf_text observed=2026-06-27T12:03:16.536504Z digest=sha256:530890b99d5623bb68e0cf82fd898f091c7f6cb515fe87fa17db5a2961c40aa5

Observation 91fb7fbc-91c6-474c-9f78-387ce0f92785 · inbound

Implementation of multi-grid Poisson solver in numerical relativity and its application to gravitational collapse of massive star cites this paper.

Implementation of multi-grid Poisson solver in numerical relativity and its application to gravitational collapse of massive star Long-term evolution of a merger-remnant neutron star in general relativistic magnetohydrodynamics I: Effect of magnetic winding

Reference 19

Resolution
verified exact
arxiv_id, observed 2026-07-03T13:08:08.607190Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

source=pdf_text observed=2026-06-27T08:29:21.873428Z digest=sha256:4ba2b0156211c841091c581b839ca33b8cefdd150ff4e2654e3c9afbb9f90b55