Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Evolving Dark Energy or Evolving Dark Matter?
As of 7 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 23 inbound Pith citation observations for arXiv:2505.02645.
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 2026-08-07T06:34:17.273281+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-07T10:47:12.068915Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-08-05T02:28:24.338817Z
Reference resolution
0 of 0 outbound references displayed
- verified exact0
- verified fuzzy0
- unresolved0
- parse uncertain0
- malformed identifier0
- metadata mismatch0
External citation measurements
0
arxiv_reference, observed 2026-08-05T02:28:24.338817Z
Outbound references
No outbound reference observations are available for this paper version.
Pith citing papers
Observation 0bd5e5e6-7ef1-418d-ad6c-ba751beb710f · inbound
The Quintom theory of dark energy after DESI DR2 cites this paper.
The Quintom theory of dark energy after DESI DR2 Evolving Dark Energy or Evolving Dark Matter?
Reference 229
- Resolution
- verified exact
- arxiv_id, observed 2026-05-19T13:12:18.364813Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation 7518a012-ca62-4346-a8ad-cbbb853fb563 · inbound
Tsallis-Cirto Hubble parameter: Explaining DESI data and High redshift Supermassive Black Hole cites this paper.
Tsallis-Cirto Hubble parameter: Explaining DESI data and High redshift Supermassive Black Hole Evolving Dark Energy or Evolving Dark Matter?
Reference 34
- Resolution
- metadata mismatch
- arxiv_id, observed 2026-05-19T11:57:16.140378Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation fc7e73d0-3a65-4f10-a689-c99a5b34613d · inbound
Tsallis-Cirto Hubble parameter: Explaining DESI data and High redshift Supermassive Black Hole cites this paper.
Tsallis-Cirto Hubble parameter: Explaining DESI data and High redshift Supermassive Black Hole Evolving Dark Energy or Evolving Dark Matter?
Reference 7
- Resolution
- unresolved
- no resolver link, observed 2026-08-07T10:47:12.068915Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 3ca83fea-574d-4bf7-9dce-b0ca774bccae · inbound
Topological defects as effective dynamical dark energy cites this paper.
Topological defects as effective dynamical dark energy Evolving Dark Energy or Evolving Dark Matter?
Reference 36
- Resolution
- unresolved
- no resolver link, observed 2026-08-07T04:41:33.652949Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation fc21414b-5b27-4a84-ab1c-012e1a73ca8e · inbound
ACT DR6 Leads to Stronger Evidence for Dynamical Dark Matter cites this paper.
ACT DR6 Leads to Stronger Evidence for Dynamical Dark Matter Evolving Dark Energy or Evolving Dark Matter?
Reference 87
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T22:01:23.513743Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation c5a9b4d4-bdb6-4f04-aa88-63eff2e8808a · inbound
Exploring non-cold dark matter in a scenario of dynamical dark energy with DESI DR2 data cites this paper.
Exploring non-cold dark matter in a scenario of dynamical dark energy with DESI DR2 data Evolving Dark Energy or Evolving Dark Matter?
Reference 65
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T18:36:59.634122Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 06994d3c-6ae1-45f2-a297-26509b450fa7 · inbound
New Insights into Dark Energy from DESI DR2 with CMB and SNIa cites this paper.
New Insights into Dark Energy from DESI DR2 with CMB and SNIa Evolving Dark Energy or Evolving Dark Matter?
Reference 13
- Resolution
- verified exact
- arxiv_id, observed 2026-05-19T05:22:05.893912Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation b3ed781b-faaa-4283-9625-83c33bab87e0 · inbound
Cosmological preference for a positive neutrino mass at 2.7$\sigma$: A joint analysis of DESI DR2, DESY5, and DESY1 data cites this paper.
Cosmological preference for a positive neutrino mass at 2.7$\sigma$: A joint analysis of DESI DR2, DESY5, and DESY1 data Evolving Dark Energy or Evolving Dark Matter?
Reference 39
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T15:12:34.613603Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 7f2a3b2c-77ae-45b2-a26a-d9b38b868a08 · inbound
Resolving the Planck-DESI tension by nonminimally coupled quintessence cites this paper.
Resolving the Planck-DESI tension by nonminimally coupled quintessence Evolving Dark Energy or Evolving Dark Matter?
Reference 112
- Resolution
- metadata mismatch
- arxiv_id, observed 2026-05-19T01:36:58.283551Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation 9d673947-49fe-4219-a4f3-2c5fb6ea0b99 · inbound
Comparing Minimal and Non-Minimal Quintessence Models to 2025 DESI Data cites this paper.
Comparing Minimal and Non-Minimal Quintessence Models to 2025 DESI Data Evolving Dark Energy or Evolving Dark Matter?
Reference 47
- Resolution
- verified exact
- arxiv_id, observed 2026-05-18T15:51:35.071306Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation 6c106bf5-01d4-4068-a7f8-0a8e6c1576c2 · inbound
Alleviating the $H_0$ tension through the interacting dark energy model from quantum gravitational field theory in light of DESI DR2 cites this paper.
Alleviating the $H_0$ tension through the interacting dark energy model from quantum gravitational field theory in light of DESI DR2 Evolving Dark Energy or Evolving Dark Matter?
Reference 136
- Resolution
- unresolved
- no resolver link, observed 2026-08-04T09:59:24.263428Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 3d8ebcab-fda3-4fb3-921b-dc538c70b840 · inbound
Model-independent late-universe measurements of $H_0$ and $\Omega_K$ with the parametrization based on cosmic age-improved inverse distance ladder cites this paper.
Model-independent late-universe measurements of $H_0$ and $\Omega_K$ with the parametrization based on cosmic age-improved inverse distance ladder Evolving Dark Energy or Evolving Dark Matter?
Reference 107
- Resolution
- unresolved
- no resolver link, observed 2026-08-04T07:19:40.353395Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 9b40c355-faad-4d75-bfd9-a798511c4768 · inbound
Hermitian formulation for mass dimension one fermions: Flat and curved space-times cites this paper.
Hermitian formulation for mass dimension one fermions: Flat and curved space-times Evolving Dark Energy or Evolving Dark Matter?
Reference 5
- Resolution
- unresolved
- no resolver link, observed 2026-08-04T06:58:56.212347Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 8739eecd-ef85-4796-9996-501c2ec9218c · inbound
Exploring the interplay of late-time dynamical dark energy and new physics before recombination cites this paper.
Exploring the interplay of late-time dynamical dark energy and new physics before recombination Evolving Dark Energy or Evolving Dark Matter?
Reference 47
- Resolution
- verified exact
- arxiv_id, observed 2026-05-14T23:13:15.801364Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation b6b6e23a-6ef2-438e-9df7-81bc844facfa · inbound
Friedmann cosmology with fluids and hyperfluids cites this paper.
Friedmann cosmology with fluids and hyperfluids Evolving Dark Energy or Evolving Dark Matter?
Reference 10
- Resolution
- verified exact
- arxiv_id, observed 2026-05-13T18:33:06.593086Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation f409a07d-f78a-4a5d-abe2-8e5eeb0c4924 · inbound
Accelerating scaling solutions from dark matter particle creation cites this paper.
Accelerating scaling solutions from dark matter particle creation Evolving Dark Energy or Evolving Dark Matter?
Reference 129
- 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 a59c6aa5-865e-4477-967a-f4e37581842a · inbound
The open-Universe signal: A model artifact rather than genuine curvature cites this paper.
The open-Universe signal: A model artifact rather than genuine curvature Evolving Dark Energy or Evolving Dark Matter?
Reference 35
- Resolution
- metadata mismatch
- arxiv_id, observed 2026-05-11T21:26:15.902774Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation 86a20e66-8b6f-4abd-9837-7cdf1484ed83 · inbound
Kinematic Lensing Ratio: Reviving Weak Lensing Cosmography as a Geometric Dark Energy Probe cites this paper.
Kinematic Lensing Ratio: Reviving Weak Lensing Cosmography as a Geometric Dark Energy Probe Evolving Dark Energy or Evolving Dark Matter?
Reference 11
- Resolution
- verified exact
- arxiv_id, observed 2026-05-12T00:36:14.708951Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation 587536ea-0088-4dcb-8e2d-0fb57e80975c · inbound
Signatures of Modified Gravity on Linear Scales in a Dynamical Dark Energy Background cites this paper.
Signatures of Modified Gravity on Linear Scales in a Dynamical Dark Energy Background Evolving Dark Energy or Evolving Dark Matter?
Reference 41
- Resolution
- verified exact
- arxiv_id, observed 2026-05-22T05:41:08.670330Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation c1d54601-2c2e-4795-bddb-b77458c7d4b7 · inbound
Signatures of Modified Gravity on Linear Scales in a Dynamical Dark Energy Background cites this paper.
Signatures of Modified Gravity on Linear Scales in a Dynamical Dark Energy Background Evolving Dark Energy or Evolving Dark Matter?
Reference 41
- Resolution
- unresolved
- no resolver link, observed 2026-08-02T13:29:56.091307Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation eb122343-2b1e-4599-8a70-4c7a6cbacf4e · inbound
Late-time Quantum Vacuum Decay and its Cosmological Implications cites this paper.
Late-time Quantum Vacuum Decay and its Cosmological Implications Evolving Dark Energy or Evolving Dark Matter?
Reference 62
- Resolution
- verified exact
- arxiv_id, observed 2026-06-29T05:43:08.158561Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation c47195c8-b2a6-4dee-8ec1-4eafc3e97849 · inbound
Neutrino mass constraints in the Schwarzschild-de Sitter black-hole dark energy model with ACT DR6 and DESI DR2 data cites this paper.
Neutrino mass constraints in the Schwarzschild-de Sitter black-hole dark energy model with ACT DR6 and DESI DR2 data Evolving Dark Energy or Evolving Dark Matter?
Reference 115
- Resolution
- unresolved
- no resolver link, observed 2026-07-12T04:18:55.037825Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation f9e6e53e-fc6f-4f61-a706-cf5b25aed50a · inbound
General Relativistic Entropic Acceleration at the perturbation level: a CLASS implementation and first Boltzmann-code constraints cites this paper.
General Relativistic Entropic Acceleration at the perturbation level: a CLASS implementation and first Boltzmann-code constraints Evolving Dark Energy or Evolving Dark Matter?
Reference 111
- Resolution
- unresolved
- no resolver link, observed 2026-08-01T01:25:44.286844Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.