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Paper Citation Record · LEDGER

Coupled dark matter-dark energy in light of near Universe observations

As of 15 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 7 inbound Pith citation observations for arXiv:1006.0877.

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

pith.paper-citation-record.v1
1006.0877 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 7 of 7 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-14T06:32:32.682623+00:00

measured 7 of 7 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-14T14:43:27.509784Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-03T07:57:44.216631Z

Reference resolution

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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 bb9fdb6a-0e81-4a49-a4ee-f318444e3c90 · inbound

Fractional Dark Matter decay: cosmological imprints and observational constraints cites this paper.

Fractional Dark Matter decay: cosmological imprints and observational constraints Coupled dark matter-dark energy in light of near Universe observations

Reference 47

Resolution
unresolved
no resolver link, observed 2026-08-14T14:43:27.509784Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation 1490e190-1f1e-4cbb-87b5-7b396ce75ea8 · inbound

Interacting dark energy in the early 2020s: a promising solution to the $H_0$ and cosmic shear tensions cites this paper.

Interacting dark energy in the early 2020s: a promising solution to the $H_0$ and cosmic shear tensions Coupled dark matter-dark energy in light of near Universe observations

Reference 154

Resolution
unresolved
no resolver link, observed 2026-08-14T13:51:08.805512Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation bf0387f6-2a15-428d-98ea-543b68cf1e92 · inbound

The model-independent degeneracy-breaking point in cosmological models with interacting Dark Energy and Dark Matter cites this paper.

The model-independent degeneracy-breaking point in cosmological models with interacting Dark Energy and Dark Matter Coupled dark matter-dark energy in light of near Universe observations

Reference 35

Resolution
unresolved
no resolver link, observed 2026-08-14T12:59:28.652131Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation f069d9c9-82f0-4bd6-a312-e7db1f1d20e7 · inbound

Interacting phantom dark energy: new accelerating scaling attractors cites this paper.

Interacting phantom dark energy: new accelerating scaling attractors Coupled dark matter-dark energy in light of near Universe observations

Reference 60

Resolution
unresolved
no resolver link, observed 2026-08-12T11:29:07.677957Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation 2363ec20-be5f-4eaf-b4c0-1e7b5c5bae47 · inbound

Solving an Interacting Quintessence Model with a Sound Horizon Initial Condition and its Observational Constraints cites this paper.

Solving an Interacting Quintessence Model with a Sound Horizon Initial Condition and its Observational Constraints Coupled dark matter-dark energy in light of near Universe observations

Reference 38

Resolution
unresolved
no resolver link, observed 2026-08-06T18:14:12.153657Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation 7cbaa9f6-5ac2-4921-a252-6caac5183534 · inbound

Dark Energy Is Not That Into You: Variable Couplings after DESI DR2 BAO cites this paper.

Dark Energy Is Not That Into You: Variable Couplings after DESI DR2 BAO Coupled dark matter-dark energy in light of near Universe observations

Reference 18

Resolution
unresolved
no resolver link, observed 2026-08-05T16:03:01.131503Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation 14928e96-e772-4dbc-921c-34e3cc076cdf · inbound

Non-linear Structure Formation in Planck+DESI Favoured Interacting Dark Energy Cosmologies cites this paper.

Non-linear Structure Formation in Planck+DESI Favoured Interacting Dark Energy Cosmologies Coupled dark matter-dark energy in light of near Universe observations

Reference 81

Resolution
verified exact
local_arxiv, observed 2026-07-03T07:57:44.217918Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

source=pdf_text observed=2026-06-27T11:43:20.857862Z digest=sha256:b30fe434385e9a27ad29906a43b9ac2cce79e742af2289e13c6c9834a6429fb4