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Paper Citation Record · LEDGER

A low-redshift preference for an interacting dark energy model

As of 4 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 10 inbound Pith citation observations for arXiv:2503.15659.

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

pith.paper-citation-record.v1
2503.15659 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 10 of 10 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-04T06:34:03.388597+00:00

measured 10 of 10 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-04T18:21:13.045173Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-04T22:30:10.459571Z

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 b7ba1c13-066a-4a8c-98eb-86f538c6d08e · inbound

Resolving the Planck-DESI tension by nonminimally coupled quintessence cites this paper.

Resolving the Planck-DESI tension by nonminimally coupled quintessence A low-redshift preference for an interacting dark energy model

Reference 52

Resolution
verified exact
arxiv_id, observed 2026-05-19T01:36:58.232543Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

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Observation 070e6bac-6c55-434e-91e9-ba8a92a96717 · inbound

Revisiting the Hubble tension problem in the framework of holographic dark energy cites this paper.

Revisiting the Hubble tension problem in the framework of holographic dark energy A low-redshift preference for an interacting dark energy model

Reference 37

Resolution
verified exact
arxiv_id, observed 2026-05-17T22:20:23.400034Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

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Observation e05c6169-ae89-4065-bbde-d34d5a7c6b8c · inbound

Lorentz Violation in Emergent Gravity and Its Cosmological Consequences cites this paper.

Lorentz Violation in Emergent Gravity and Its Cosmological Consequences A low-redshift preference for an interacting dark energy model

Reference 43

Resolution
unresolved
no resolver link, observed 2026-08-03T19:55:31.250507Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation 8a2753cd-fb78-49e1-a486-9bcdf82e010f · inbound

On the Metric $f(R)$ gravity Viability in Accounting for the Binned Supernovae Data cites this paper.

On the Metric $f(R)$ gravity Viability in Accounting for the Binned Supernovae Data A low-redshift preference for an interacting dark energy model

Reference 5

Resolution
metadata mismatch
arxiv_id, observed 2026-05-16T20:33:24.362491Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

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Observation c3f17885-91ab-4ad8-9df4-94a54352769f · 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 A low-redshift preference for an interacting dark energy model

Reference 29

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:ab9b1de624ad085e159febdb81fafca265599def2165b645a9310d5d799a4054

Observation 94344bea-a3ac-4639-ba96-bc7a5a5ef56f · inbound

Model-Independent Reconstruction of Quintessence Potential and Kinetic Energy from DESI DR2 and Pantheon+ Supernovae cites this paper.

Model-Independent Reconstruction of Quintessence Potential and Kinetic Energy from DESI DR2 and Pantheon+ Supernovae A low-redshift preference for an interacting dark energy model

Reference 41

Resolution
verified exact
arxiv_id, observed 2026-05-15T01:33:27.416232Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

source=pdf_text observed=2026-05-15T01:30:47.614992Z digest=sha256:641c37786849e90564f016dc9a23da772a75eea78311655f87bb75baeb2d0e3d

Observation deef2d1b-0e0e-4074-a1ce-0895adc4251e · inbound

Effective field theory interpretation of ATLAS measurements involving the Higgs boson, electroweak bosons and the top quark cites this paper.

Effective field theory interpretation of ATLAS measurements involving the Higgs boson, electroweak bosons and the top quark A low-redshift preference for an interacting dark energy model

Reference 71

Resolution
verified exact
arxiv_id, observed 2026-07-04T22:30:10.460985Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

source=pdf_text observed=2026-07-04T22:27:16.736476Z digest=sha256:2548089ad1d877dada99f89d71b182fb2c42e0f4f2b9ab4e2b671379521361e9

Observation 70e6c5b4-56e7-41cc-b31d-42ce2e4f8212 · inbound

Saturation Mechanisms in the Interacting Dark Sector cites this paper.

Saturation Mechanisms in the Interacting Dark Sector A low-redshift preference for an interacting dark energy model

Reference 72

Resolution
verified exact
arxiv_id, observed 2026-05-11T18:41:13.118395Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

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Observation 6ac33d3a-8dcc-4901-add9-f17cc58a5e8a · inbound

Accelerating scaling solutions from dark matter particle creation cites this paper.

Accelerating scaling solutions from dark matter particle creation A low-redshift preference for an interacting dark energy model

Reference 63

Resolution
unresolved
no resolver link, observed 2026-07-12T18:37:05.978670Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation 6883d311-781a-443c-9a5d-8d1a2cc70e94 · inbound

Boosting the optical depth to Thomson scattering with primordial black hole evaporation at high redshift cites this paper.

Boosting the optical depth to Thomson scattering with primordial black hole evaporation at high redshift A low-redshift preference for an interacting dark energy model

Reference 94

Resolution
unresolved
no resolver link, observed 2026-08-04T18:21:13.045173Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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