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Paper Citation Record · LEDGER

An inhomogeneous alternative to dark energy?

As of 24 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 6 inbound Pith citation observations for arXiv:astro-ph/0512006.

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

pith.paper-citation-record.v1
astro-ph/0512006 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 2026-08-23T06:30:58.430688+00:00

measured 6 of 6 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-16T12:17:22.587089Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-06-26T23:00:12.457733Z

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 5ab752bf-6994-4df1-8955-e259dd0578bf · inbound

CMB dipoles and other low-order multipoles in the quasispherical Szekeres model cites this paper.

CMB dipoles and other low-order multipoles in the quasispherical Szekeres model An inhomogeneous alternative to dark energy?

Reference 13

Resolution
verified exact
local_arxiv, observed 2026-05-24T18:54:50.876194Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

source=pdf_text observed=2026-05-24T18:53:10.493042Z digest=sha256:98405e10268bd789494c37b7fa65b2335fd5988f43635363524cb197d7a6d427

Observation 01502511-034a-4490-bde7-7be6c466578d · inbound

Physical geometry of the quasispherical Szekeres models cites this paper.

Physical geometry of the quasispherical Szekeres models An inhomogeneous alternative to dark energy?

Reference 17

Resolution
unresolved
no resolver link, observed 2026-08-14T14:55:57.904394Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T14:55:57.904394Z digest=sha256:ad03293f537abe6fa3e933d5e527fee3930be2f61f79239d43a72c1aa54bbf98

Observation 60c59ac3-b322-4b21-939d-e9b175f5a6d0 · inbound

CMB sky for an off-center observer in a local void I: framework for forecasts cites this paper.

CMB sky for an off-center observer in a local void I: framework for forecasts An inhomogeneous alternative to dark energy?

Reference 8

Resolution
unresolved
no resolver link, observed 2026-08-14T13:23:31.847128Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T13:23:31.847128Z digest=sha256:0d1f55e8cd6785fda555585cabd1f67a63e51bb087392e941ba5fe115681d99f

Observation 851e7cba-256e-4fbe-8605-ed4427f2c37c · inbound

Little ado about everything II: an `emergent' dark energy from structure formation to rule cosmic tensions cites this paper.

Little ado about everything II: an `emergent' dark energy from structure formation to rule cosmic tensions An inhomogeneous alternative to dark energy?

Reference 64

Resolution
unresolved
no resolver link, observed 2026-08-08T17:56:52.131424Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-08T17:56:52.131424Z digest=sha256:944f5fb4a6c09b851c4ef7a214377c529ded04d618aa50f284dc6dafdf26c69d

Observation 62f7a9e0-dffb-4982-bd69-9f5705f01b2f · inbound

Alleviating the Hubble Tension with a Local Void and Transitions of the Absolute Magnitude cites this paper.

Alleviating the Hubble Tension with a Local Void and Transitions of the Absolute Magnitude An inhomogeneous alternative to dark energy?

Reference 32

Resolution
unresolved
no resolver link, observed 2026-08-16T12:17:22.587089Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-16T12:17:22.587089Z digest=sha256:abb3edbf47b64d8bc195474af1aef5e778612543ee0e8ab31fec69900a23cdd5

Observation bed6db92-d214-46b2-a73e-7decaa74b9c6 · inbound

Impact of inhomogeneous curvature on growth rate measurements from magnitude fluctuations cites this paper.

Impact of inhomogeneous curvature on growth rate measurements from magnitude fluctuations An inhomogeneous alternative to dark energy?

Reference 171

Resolution
verified exact
local_arxiv, observed 2026-06-26T23:00:12.459470Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:20cbf29229118962cd808537a4e52189041e056f8ce9aca2b208914a16ca0b49