Paper Citation Record · LEDGER

A low-redshift preference for an interacting dark energy model

As of 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 11 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 11 of 11 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 11 of 11 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-05T16:03:01.416864Z

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

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

Observation fd1b8ea2-2e96-421f-82ae-9cd127b7f322 · 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 A low-redshift preference for an interacting dark energy model

Reference 109

Resolution: unresolved; no resolver link, observed 2026-08-05T16:03:01.416864Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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

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.

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

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.

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

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

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

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.

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.