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Paper Citation Record · LEDGER

Evolution of clustering in cosmological models with time-varying dark energy

As of 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:2503.19352.

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

pith.paper-citation-record.v1
2503.19352 v3

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 2026-08-11T06:34:44.6726+00:00

measured 5 of 5 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-07T11:24:24.041422Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-05-13T17:38:03.089749Z

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 8249be73-5a7b-4944-b595-51df397bcb30 · inbound

Constraints on Barrow and Tsallis Holographic Dark Energy from DESI DR2 BAO data cites this paper.

Constraints on Barrow and Tsallis Holographic Dark Energy from DESI DR2 BAO data Evolution of clustering in cosmological models with time-varying dark energy

Reference 81

Resolution
unresolved
no resolver link, observed 2026-08-07T11:24:24.041422Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T11:24:24.041422Z digest=sha256:2ced1b316a06688c568c20b48423f9e19128a55e87a476e01a5a626fa5b2892e

Observation 1703f019-1c67-4989-85f3-d17212342d40 · inbound

Constraint on Symmetric Teleparallel Gravity with Different Dark energy Parametrizations from DESI DR2 BAO Data cites this paper.

Constraint on Symmetric Teleparallel Gravity with Different Dark energy Parametrizations from DESI DR2 BAO Data Evolution of clustering in cosmological models with time-varying dark energy

Reference 58

Resolution
unresolved
no resolver link, observed 2026-08-06T19:22:36.030506Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T19:22:36.030506Z digest=sha256:317e283816ecf297f602d8e83dcf25fa0a7167b7ab9e047ba195fde44b43616c

Observation 79158f8c-c2a7-4142-8f49-a6ec899588a4 · inbound

Updated observational constraints on $\phi$CDM dynamical dark energy cosmological models cites this paper.

Updated observational constraints on $\phi$CDM dynamical dark energy cosmological models Evolution of clustering in cosmological models with time-varying dark energy

Reference 33

Resolution
unresolved
no resolver link, observed 2026-08-04T13:43:12.236432Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-04T13:43:12.236432Z digest=sha256:92572f24494934b32d17c981895200a274c45c3f4abb452e31f49f00ae44c91b

Observation 5c906e85-3699-4657-bd1d-97371df409d4 · inbound

Sound Mode and Scale-Dependent Growth in Two-Fluid Dynamical Dark Energy cites this paper.

Sound Mode and Scale-Dependent Growth in Two-Fluid Dynamical Dark Energy Evolution of clustering in cosmological models with time-varying dark energy

Reference 25

Resolution
unresolved
no resolver link, observed 2026-07-15T14:51:12.413085Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-07-15T14:51:12.413085Z digest=sha256:bdca79451fadb2c2660b201dd4ae35bdca72ce17f7c2169ebc367c58deddd942

Observation 709bce29-f7d0-4656-8644-d123c13a1b0a · inbound

Is the $w_0w_a$CDM cosmological parameterization evidence for dark energy dynamics partially caused by the excess smoothing of Planck PR4 CMB anisotropy data? cites this paper.

Is the $w_0w_a$CDM cosmological parameterization evidence for dark energy dynamics partially caused by the excess smoothing of Planck PR4 CMB anisotropy data? Evolution of clustering in cosmological models with time-varying dark energy

Reference 37

Resolution
verified exact
arxiv_id, observed 2026-05-13T17:38:03.091379Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

source=pdf_text observed=2026-05-13T17:33:08.222231Z digest=sha256:63a53dd39720fbbc7f139baa8fbfd2155cffe81e4c817db0ca3ea0cc6c66b429