Paper Citation Record · LEDGER

Dynamical dark energy with AdS-dS transitions vs. Baryon Acoustic Oscillations at $z =$ 2.3-2.4

As of 22 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 11 inbound Pith citation observations for arXiv:2504.07299.

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

pith.paper-citation-record.v1
2504.07299 v2

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 2026-08-22T06:32:14.747728+00:00

measured 11 of 11 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-07T12:22:19.023796Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-03T07:07:44.869956Z

Reference resolution

0 of 0 outbound references displayed

verified exact0
verified fuzzy0
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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 358f6a88-fad2-4512-b32a-542be7115b29 · inbound

What solves the Hubble tension in phenomenological dark energy models at background level? cites this paper.

What solves the Hubble tension in phenomenological dark energy models at background level? Dynamical dark energy with AdS-dS transitions vs. Baryon Acoustic Oscillations at $z =$ 2.3-2.4

Reference 55

Resolution: unresolved; no resolver link, observed 2026-08-07T12:22:19.023796Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation dec26bcf-2716-48cb-ab77-9824ecd4448d · inbound

Nonlinear Matter Power Spectrum from relativistic $N$-body Simulations: $\Lambda_{\rm s}$CDM versus $\Lambda$CDM cites this paper.

Nonlinear Matter Power Spectrum from relativistic $N$-body Simulations: $\Lambda_{\rm s}$CDM versus $\Lambda$CDM Dynamical dark energy with AdS-dS transitions vs. Baryon Acoustic Oscillations at $z =$ 2.3-2.4

Reference 245

Resolution: verified exact; arxiv_id, observed 2026-05-18T04:50:55.388821Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

Observation af568d1a-4383-4984-99c0-c1e3f8dd8810 · inbound

Probing dynamical dark energy with late-time data: Evidence, tensions, and the limits of the $w_0w_a$CDM framework cites this paper.

Probing dynamical dark energy with late-time data: Evidence, tensions, and the limits of the $w_0w_a$CDM framework Dynamical dark energy with AdS-dS transitions vs. Baryon Acoustic Oscillations at $z =$ 2.3-2.4

Reference 85

Resolution: verified exact; arxiv_id, observed 2026-05-21T13:30:12.240867Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

Observation 95e573b5-6e29-4a69-8b86-a5584edddcbd · inbound

Sign-Switching Dark Energy: Smooth Transitions with Recent DESI DR2 Observations cites this paper.

Sign-Switching Dark Energy: Smooth Transitions with Recent DESI DR2 Observations Dynamical dark energy with AdS-dS transitions vs. Baryon Acoustic Oscillations at $z =$ 2.3-2.4

Reference 82

Resolution: verified exact; arxiv_id, observed 2026-05-16T05:20:39.554902Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

Observation 04df336a-d802-4623-8a8b-ab0b40ca55c8 · inbound

Background-level reconstruction of scalar-field potentials from dark-energy histories and comparison with analytic potential families cites this paper.

Background-level reconstruction of scalar-field potentials from dark-energy histories and comparison with analytic potential families Dynamical dark energy with AdS-dS transitions vs. Baryon Acoustic Oscillations at $z =$ 2.3-2.4

Reference 94

Resolution: unresolved; no resolver link, observed 2026-07-15T12:01:04.317365Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 1ffa85dc-8ae8-4450-bf4c-dee5289da3eb · inbound

On the origin of the BAOtr-DESI tension cites this paper.

On the origin of the BAOtr-DESI tension Dynamical dark energy with AdS-dS transitions vs. Baryon Acoustic Oscillations at $z =$ 2.3-2.4

Reference 76

Resolution: verified exact; arxiv_id, observed 2026-05-11T09:41:00.896177Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

Observation 7b04e071-1081-433b-a5b7-de00d6fc22f0 · inbound

Do equation of state parametrizations of dark energy faithfully capture the dynamics of the late universe? cites this paper.

Do equation of state parametrizations of dark energy faithfully capture the dynamics of the late universe? Dynamical dark energy with AdS-dS transitions vs. Baryon Acoustic Oscillations at $z =$ 2.3-2.4

Reference 59

Resolution: verified exact; arxiv_id, observed 2026-05-11T11:36:02.024024Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

Observation f66fb97c-bf09-4db3-9a06-c465f15291b8 · inbound

Negative neutrino mass or negative dark energy? cites this paper.

Negative neutrino mass or negative dark energy? Dynamical dark energy with AdS-dS transitions vs. Baryon Acoustic Oscillations at $z =$ 2.3-2.4

Reference 94

Resolution: verified exact; arxiv_id, observed 2026-05-21T03:03:55.328943Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

Observation 68539cee-142d-4aeb-bee2-be9fae0f736b · inbound

Endpoint Logarithms in the NLO Mueller-Navelet Jet Vertex: Threshold Matching and BLM/MOM Prescription Sensitivity cites this paper.

Endpoint Logarithms in the NLO Mueller-Navelet Jet Vertex: Threshold Matching and BLM/MOM Prescription Sensitivity Dynamical dark energy with AdS-dS transitions vs. Baryon Acoustic Oscillations at $z =$ 2.3-2.4

Reference 33

Resolution: unresolved; no resolver link, observed 2026-07-12T14:25:03.782538Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 7f5ef45a-aa9a-4c8d-9f40-3828a7a94d2e · inbound

A Friendly Phantom: Late-time AdS-to-dS transition and cosmological tensions cites this paper.

A Friendly Phantom: Late-time AdS-to-dS transition and cosmological tensions Dynamical dark energy with AdS-dS transitions vs. Baryon Acoustic Oscillations at $z =$ 2.3-2.4

Reference 33

Resolution: verified exact; arxiv_id, observed 2026-07-03T07:07:44.872524Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

Observation e3c469d5-4e50-4853-831f-33546d211efd · inbound

Defocusing dark energy: Raychaudhuri diagnostics beyond $w<-1/3$ and the phantom divide cites this paper.

Defocusing dark energy: Raychaudhuri diagnostics beyond $w<-1/3$ and the phantom divide Dynamical dark energy with AdS-dS transitions vs. Baryon Acoustic Oscillations at $z =$ 2.3-2.4

Reference 99

Resolution: unresolved; no resolver link, observed 2026-08-01T16:30:05.259299Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.