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Paper Citation Record · LEDGER

Improved constrained scheme for the Einstein equations: An approach to the uniqueness issue

As of 22 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:0809.2325.

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

pith.paper-citation-record.v1
0809.2325 v2

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 2026-08-21T06:32:19.484+00:00

measured 5 of 5 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-15T15:05:12.326855Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-08-09T05:33:08.706277Z

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 875b2437-7c4e-417f-98a5-cbbbcece5052 · inbound

Rotating neutron stars with non-barotropic thermal profile cites this paper.

Rotating neutron stars with non-barotropic thermal profile Improved constrained scheme for the Einstein equations: An approach to the uniqueness issue

Reference 50

Resolution
unresolved
no resolver link, observed 2026-08-14T10:30:45.085451Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T10:30:45.085451Z digest=sha256:7ad934ef0392e27554decc4f53c72dbebefe4e5fd0a356df7dd9c297f17a3520

Observation af1ed9e1-92d9-4dd5-a4dc-193d46e54725 · 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 Improved constrained scheme for the Einstein equations: An approach to the uniqueness issue

Reference 168

Resolution
metadata mismatch
local_arxiv, observed 2026-08-09T05:33:08.711674Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

source=pdf_text observed=2026-08-09T05:33:08.568604Z digest=sha256:fcb110207a383228c894acf215fff72f277e2668f22c58e23db5edd6d1c6496d

Observation 70128916-ac1e-4408-b5ec-761bbb5657dc · inbound

Universal relations applied to proto-neutron star generated gravitational waves from three-dimensional core collapse supernova simulations cites this paper.

Universal relations applied to proto-neutron star generated gravitational waves from three-dimensional core collapse supernova simulations Improved constrained scheme for the Einstein equations: An approach to the uniqueness issue

Reference 54

Resolution
unresolved
no resolver link, observed 2026-08-01T04:14:03.261313Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T04:14:03.261313Z digest=sha256:300eaa9d7a66b0cbd25ad49c33fcc2c7e2833c9abe88ebf37aa7574bf0ca7741

Observation 9e48ab64-2383-43d4-b8b0-0d83b8ecbcf4 · inbound

Structural quasi-universality in highly magnetized differentially rotating neutron stars cites this paper.

Structural quasi-universality in highly magnetized differentially rotating neutron stars Improved constrained scheme for the Einstein equations: An approach to the uniqueness issue

Reference 48

Resolution
unresolved
no resolver link, observed 2026-08-15T15:05:12.326855Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-15T15:05:12.326855Z digest=sha256:5c7a31c33e227ba0a10d67076475b5ec693d781b6bca778d9dedaac836456c7e

Observation 73c8fc18-199a-48ca-a3be-65cbc8970c24 · inbound

On the nature of oscillating modes of proto-neutron stars cites this paper.

On the nature of oscillating modes of proto-neutron stars Improved constrained scheme for the Einstein equations: An approach to the uniqueness issue

Reference 65

Resolution
unresolved
no resolver link, observed 2026-08-14T04:16:46.807257Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T04:16:46.807257Z digest=sha256:3052c97f4f853f7650f403000230435ceb1e28d78936ebc62ec537af4f2a9c51