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Paper Citation Record · LEDGER

How to move a black hole without excision: gauge conditions for the numerical evolution of a moving puncture

As of 15 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 6 inbound Pith citation observations for arXiv:gr-qc/0605030.

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

pith.paper-citation-record.v1
gr-qc/0605030 v2

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 2026-08-15T06:32:42.880941+00:00

measured 6 of 6 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-14T05:28:09.099772Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-05-18T05:50:56.814084Z

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 0449ba19-6914-4519-b157-57028b22fb41 · inbound

Cooling binary neutron star remnants via nucleon-nucleon-axion bremsstrahlung cites this paper.

Cooling binary neutron star remnants via nucleon-nucleon-axion bremsstrahlung How to move a black hole without excision: gauge conditions for the numerical evolution of a moving puncture

Reference 77

Resolution
unresolved
no resolver link, observed 2026-08-14T05:28:09.099772Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T05:28:09.099772Z digest=sha256:4e5f9f8c761da749df4dcd270a6e56fa3b45e862dc24a15dc164141d143496c5

Observation 7f33bec3-c100-4f9e-b8b6-6fe2ad53d100 · inbound

Inflaton Dynamics in Higher-Derivative Scalar-Tensor Theories of Gravity cites this paper.

Inflaton Dynamics in Higher-Derivative Scalar-Tensor Theories of Gravity How to move a black hole without excision: gauge conditions for the numerical evolution of a moving puncture

Reference 81

Resolution
unresolved
no resolver link, observed 2026-08-07T14:44:16.829125Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T14:44:16.829125Z digest=sha256:20a04cd0d00c21434e814c9cc286816a563bbcd08874e1eddf09c25d7e468cc0

Observation 819a7852-6989-4115-b56a-e5f688d72bc8 · inbound

AthenaK simulations of the binary black hole merger GW150914 cites this paper.

AthenaK simulations of the binary black hole merger GW150914 How to move a black hole without excision: gauge conditions for the numerical evolution of a moving puncture

Reference 86

Resolution
unresolved
no resolver link, observed 2026-08-07T05:57:54.377569Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T05:57:54.377569Z digest=sha256:07871e1a2f34c19d83c0c89def6169af47f8223c8ecc98a8e2415a2461cbec87

Observation 96afd846-32bd-4134-ab9c-11760e0125cb · inbound

Scalar fields around black hole binaries in LIGO-Virgo-KAGRA cites this paper.

Scalar fields around black hole binaries in LIGO-Virgo-KAGRA How to move a black hole without excision: gauge conditions for the numerical evolution of a moving puncture

Reference 107

Resolution
verified exact
local_arxiv, observed 2026-05-18T05:50:56.816448Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

source=pdf_text observed=2026-05-18T05:48:25.646347Z digest=sha256:e585ab59f2b8c1e1f8715942c3ace49f27c4e88d14719815b73de1086c686746

Observation 43a821cc-5178-4cfd-89ff-8e4a7be1f276 · inbound

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

GRACE: An Open-Source Framework for GPU-Accelerated Numerical Relativity How to move a black hole without excision: gauge conditions for the numerical evolution of a moving puncture

Reference 67

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

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-07-14T15:02:35.854356Z digest=sha256:90f3593f96b0b0e3a34c658d0704dfc8f7bc35e3191952b07eb065235ba79c20

Observation 2f5df4bf-082e-4315-a156-276faebb10f1 · inbound

Nonlinear Dynamics near the Threshold of Gravitational Collapse cites this paper.

Nonlinear Dynamics near the Threshold of Gravitational Collapse How to move a black hole without excision: gauge conditions for the numerical evolution of a moving puncture

Reference 67

Resolution
unresolved
no resolver link, observed 2026-08-01T09:07:05.144171Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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