Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links, observed 2026-05-15T12:28:25.709680Z
Paper Citation Record · LEDGER
A class of decelerating inhomogeneous cosmological models giving rise to accelerating FLRW universes at large scales
As of 6 August 2026, this Paper Citation Record lists 67 of 67 outbound references and 1 inbound Pith citation observation for arXiv:2603.11377.
A citation records a reference. It does not transfer a finding from one paper to another.
Coverage vector
One-hop event checks from named stored sources.
Source: scholarly_work_events, retraction_status_cache, observed 2026-08-06T06:34:29.942622+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-06-29T19:25:54.897253Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-06-29T19:33:54.231812Z
Reference resolution
67 of 67 outbound references displayed
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External citation measurements
No source-named external measurement is stored.
Outbound references
Observation a2f23cb4-ade0-4cc3-b732-2694391f72a2 · outbound
This paper cites an unresolved cited work.
A class of decelerating inhomogeneous cosmological models giving rise to accelerating FLRW universes at large scales Unresolved cited work
Reference 1
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Observation bc96c94a-ed4b-45b2-8ae4-d10e06c47d5e · outbound
This paper cites free-falling.
A class of decelerating inhomogeneous cosmological models giving rise to accelerating FLRW universes at large scales free-falling
Reference 2
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A class of decelerating inhomogeneous cosmological models giving rise to accelerating FLRW universes at large scales Unresolved cited work
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A class of decelerating inhomogeneous cosmological models giving rise to accelerating FLRW universes at large scales Unresolved cited work
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Observation 3fcedf08-b26b-499e-afda-a1fabfd4a526 · outbound
This paper cites The complete set of equations Our model has 6 independent spacetime functions, namely, H, ε, nµ, and 2 viscosity parameters,ζ A andζ B.
A class of decelerating inhomogeneous cosmological models giving rise to accelerating FLRW universes at large scales The complete set of equations Our model has 6 independent spacetime functions, namely, H, ε, nµ, and 2 viscosity parameters,ζ A andζ B
Reference 5
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A class of decelerating inhomogeneous cosmological models giving rise to accelerating FLRW universes at large scales Unresolved cited work
Reference 6
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Observation 5eb7b2de-0692-4e8e-9cf2-ffae5084a06c · outbound
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A class of decelerating inhomogeneous cosmological models giving rise to accelerating FLRW universes at large scales critical density
Reference 7
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This paper cites We have focused on novelties for the late time regimen, while we kept the earlier epochs as homogeneous and isotropic as in the standard picture of Cosmology.
A class of decelerating inhomogeneous cosmological models giving rise to accelerating FLRW universes at large scales We have focused on novelties for the late time regimen, while we kept the earlier epochs as homogeneous and isotropic as in the standard picture of Cosmology
Reference 8
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A class of decelerating inhomogeneous cosmological models giving rise to accelerating FLRW universes at large scales Unresolved cited work
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A class of decelerating inhomogeneous cosmological models giving rise to accelerating FLRW universes at large scales Unresolved cited work
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A class of decelerating inhomogeneous cosmological models giving rise to accelerating FLRW universes at large scales Unresolved cited work
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A class of decelerating inhomogeneous cosmological models giving rise to accelerating FLRW universes at large scales Unresolved cited work
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A class of decelerating inhomogeneous cosmological models giving rise to accelerating FLRW universes at large scales Unresolved cited work
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Observation 5ebb2dde-2dcb-43af-b12d-b58d9f627f6d · outbound
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A class of decelerating inhomogeneous cosmological models giving rise to accelerating FLRW universes at large scales Is the Observable Universe Consistent with the Cosmological Principle?
Reference 43
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Observation 6ea89654-d13b-4519-a845-1d7975a7172e · outbound
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A class of decelerating inhomogeneous cosmological models giving rise to accelerating FLRW universes at large scales The Best Inflationary Models After Planck
Reference 44
- Resolution
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Reference 46
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Source-reported events for the cited work
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Observation 881db880-2b6e-46b6-9425-1fd35f6d97d4 · outbound
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A class of decelerating inhomogeneous cosmological models giving rise to accelerating FLRW universes at large scales Unresolved cited work
Reference 47
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Source-reported events for the cited work
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Observation ff5c84c9-038f-4518-b6c9-0bf3363b29e8 · outbound
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A class of decelerating inhomogeneous cosmological models giving rise to accelerating FLRW universes at large scales Unresolved cited work
Reference 48
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Source-reported events for the cited work
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Observation 8942ed53-9e78-4cbf-ab0d-b619adfd9001 · outbound
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A class of decelerating inhomogeneous cosmological models giving rise to accelerating FLRW universes at large scales Unresolved cited work
Reference 49
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Source-reported events for the cited work
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Observation 1a5f5ad4-8a18-45c7-9424-25f0092283f6 · outbound
This paper cites Consequences of dark matter-dark energy interaction on cosmological parameters derived from SNIa data.
A class of decelerating inhomogeneous cosmological models giving rise to accelerating FLRW universes at large scales Consequences of dark matter-dark energy interaction on cosmological parameters derived from SNIa data
Reference 50
- Resolution
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Source-reported events for the cited work
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Observation de2b6efb-3f82-49cd-a553-fee8dfe84f41 · outbound
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A class of decelerating inhomogeneous cosmological models giving rise to accelerating FLRW universes at large scales Unresolved cited work
Reference 51
- Resolution
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Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.
Observation e5446461-ffce-4caf-9f8a-f9e71ec69806 · outbound
This paper cites Dark Matter and Dark Energy Interactions: Theoretical Challenges, Cosmological Implications and Observational Signatures.
A class of decelerating inhomogeneous cosmological models giving rise to accelerating FLRW universes at large scales Dark Matter and Dark Energy Interactions: Theoretical Challenges, Cosmological Implications and Observational Signatures
Reference 52
- Resolution
- verified exact
- local_arxiv, observed 2026-05-15T12:30:00.341172Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.
Observation 93602277-9844-4b27-a6ae-f57141cb1afe · outbound
This paper cites an unresolved cited work.
A class of decelerating inhomogeneous cosmological models giving rise to accelerating FLRW universes at large scales Unresolved cited work
Reference 53
- Resolution
- unresolved
- raw_fallback, observed 2026-05-15T12:30:01.053082Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.
Observation 920b07b3-e519-41dc-98e5-6c00dcaa22d0 · outbound
This paper cites an unresolved cited work.
A class of decelerating inhomogeneous cosmological models giving rise to accelerating FLRW universes at large scales Unresolved cited work
Reference 54
- Resolution
- unresolved
- raw_fallback, observed 2026-05-15T12:30:01.087637Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.
Observation b8dfd0f9-bbcd-4acb-88bd-f4786d638fd0 · outbound
This paper cites an unresolved cited work.
A class of decelerating inhomogeneous cosmological models giving rise to accelerating FLRW universes at large scales Unresolved cited work
Reference 55
- Resolution
- unresolved
- raw_fallback, observed 2026-05-15T12:30:01.124147Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.
Observation 69da729c-2143-4cba-bfc4-8a7c275745a4 · outbound
This paper cites To CPL, or not to CPL? What we have not learned about the dark energy equation of state.
A class of decelerating inhomogeneous cosmological models giving rise to accelerating FLRW universes at large scales To CPL, or not to CPL? What we have not learned about the dark energy equation of state
Reference 56
- Resolution
- verified exact
- arxiv_id, observed 2026-06-09T02:06:02.692145Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.
Observation c4c4654f-348f-4dfa-9810-7d47c48005b1 · outbound
This paper cites an unresolved cited work.
A class of decelerating inhomogeneous cosmological models giving rise to accelerating FLRW universes at large scales Unresolved cited work
Reference 57
- Resolution
- unresolved
- raw_fallback, observed 2026-05-15T12:30:01.105516Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.
Observation 39d3388a-8306-497c-808e-1dfa656ba437 · outbound
This paper cites an unresolved cited work.
A class of decelerating inhomogeneous cosmological models giving rise to accelerating FLRW universes at large scales Unresolved cited work
Reference 58
- Resolution
- unresolved
- raw_fallback, observed 2026-05-15T12:30:01.082527Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.
Observation 0874c47a-0428-41d4-a2d1-043cab4ebb2c · outbound
This paper cites an unresolved cited work.
A class of decelerating inhomogeneous cosmological models giving rise to accelerating FLRW universes at large scales Unresolved cited work
Reference 59
- Resolution
- unresolved
- raw_fallback, observed 2026-05-15T12:30:01.079732Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.
Observation 4cca2b0b-0ee5-40bf-b7a1-85ad0c4f7c24 · outbound
This paper cites Everything You Always Wanted To Know About The Cosmological Constant Problem (But Were Afraid To Ask).
A class of decelerating inhomogeneous cosmological models giving rise to accelerating FLRW universes at large scales Everything You Always Wanted To Know About The Cosmological Constant Problem (But Were Afraid To Ask)
Reference 60
- Resolution
- verified exact
- local_arxiv, observed 2026-05-15T12:30:00.310558Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.
Observation a936bc72-c618-415a-ac82-557431903bf5 · outbound
This paper cites an unresolved cited work.
A class of decelerating inhomogeneous cosmological models giving rise to accelerating FLRW universes at large scales Unresolved cited work
Reference 61
- Resolution
- unresolved
- raw_fallback, observed 2026-05-15T12:30:01.085087Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.
Observation 4e654217-6f86-4c0e-9c92-ba396c0decc6 · outbound
This paper cites an unresolved cited work.
A class of decelerating inhomogeneous cosmological models giving rise to accelerating FLRW universes at large scales Unresolved cited work
Reference 62
- Resolution
- unresolved
- raw_fallback, observed 2026-05-15T12:30:01.075994Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.
Observation 18580f5c-2b42-420f-ba1f-ae94ee2115d9 · outbound
This paper cites an unresolved cited work.
A class of decelerating inhomogeneous cosmological models giving rise to accelerating FLRW universes at large scales Unresolved cited work
Reference 63
- Resolution
- verified exact
- doi, observed 2026-05-15T12:29:59.962844Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.
Observation 0f09ed31-04bd-42f1-93b9-bf0c7d58b4e4 · outbound
This paper cites Light propagation in statistically homogeneous and isotropic dust universes.
A class of decelerating inhomogeneous cosmological models giving rise to accelerating FLRW universes at large scales Light propagation in statistically homogeneous and isotropic dust universes
Reference 64
- Resolution
- verified exact
- local_arxiv, observed 2026-05-15T12:30:00.325151Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.
Observation 42e250cd-aa82-49c8-b006-ae39eb4ce62b · outbound
This paper cites an unresolved cited work.
A class of decelerating inhomogeneous cosmological models giving rise to accelerating FLRW universes at large scales Unresolved cited work
Reference 65
- Resolution
- unresolved
- raw_fallback, observed 2026-05-15T12:30:01.157948Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.
Observation 2f7e62ef-b52c-4de3-a242-6bc3cd4aadcf · outbound
This paper cites an unresolved cited work.
A class of decelerating inhomogeneous cosmological models giving rise to accelerating FLRW universes at large scales Unresolved cited work
Reference 66
- Resolution
- unresolved
- raw_fallback, observed 2026-05-15T12:30:01.036760Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.
Observation 34739fef-65fb-4455-8e98-663a9c2112c5 · outbound
This paper cites an unresolved cited work.
A class of decelerating inhomogeneous cosmological models giving rise to accelerating FLRW universes at large scales Unresolved cited work
Reference 67
- Resolution
- unresolved
- raw_fallback, observed 2026-05-15T12:30:01.002978Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.
Pith citing papers
Observation 8143b72e-73dd-4df5-a0a5-e91e55061a71 · inbound
Pseudosymmetry, Ricci soliton and Curvature Inheritance symmetries of Friedmann Lema\^itre Robertson Walker spacetime cites this paper.
Pseudosymmetry, Ricci soliton and Curvature Inheritance symmetries of Friedmann Lema\^itre Robertson Walker spacetime A class of decelerating inhomogeneous cosmological models giving rise to accelerating FLRW universes at large scales
Reference 59
- Resolution
- verified exact
- local_arxiv, observed 2026-06-29T19:33:54.233198Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.