Paper Citation Record · LEDGER

Dynamical dark energy with AdS-to-dS and dS-to-dS transitions: Implications for the $H_0$ tension

As of 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 14 inbound Pith citation observations for arXiv:2502.14667.

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

pith.paper-citation-record.v1
2502.14667 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 14 of 14 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-10T06:31:04.303077+00:00

measured 14 of 14 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-07T10:52:56.770713Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-03T07:07:44.865277Z

Reference resolution

0 of 0 outbound references displayed

verified exact0
verified fuzzy0
unresolved0
parse uncertain0
malformed identifier0
metadata mismatch0

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 7fb752fa-cdbe-4534-8938-ce9eb3015e5f · inbound

Can the universe experience an AdS landscape since matter-radiation equality? cites this paper.

Can the universe experience an AdS landscape since matter-radiation equality? Dynamical dark energy with AdS-to-dS and dS-to-dS transitions: Implications for the $H_0$ tension

Reference 143

Resolution: unresolved; no resolver link, observed 2026-08-07T10:52:56.770713Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 0acc7184-2904-4d45-a606-bb0bb90f66cd · 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-to-dS and dS-to-dS transitions: Implications for the $H_0$ tension

Reference 211

Resolution: verified exact; arxiv_id, observed 2026-05-18T04:50:55.470328Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

Observation 3a9b97f5-e3b7-4db2-907c-e42655db2bec · 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-to-dS and dS-to-dS transitions: Implications for the $H_0$ tension

Reference 84

Resolution: verified exact; arxiv_id, observed 2026-05-21T13:30:12.103790Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

Observation 4c4c3af4-a962-43d1-8c6f-dcdece196f35 · 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-to-dS and dS-to-dS transitions: Implications for the $H_0$ tension

Reference 79

Resolution: verified exact; arxiv_id, observed 2026-05-16T05:20:39.715453Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

Observation 733d05f6-8b79-468e-9ae2-a36058957c33 · inbound

Statistical consistency of sign-switching vacuum energy with cosmological observations cites this paper.

Statistical consistency of sign-switching vacuum energy with cosmological observations Dynamical dark energy with AdS-to-dS and dS-to-dS transitions: Implications for the $H_0$ tension

Reference 61

Resolution: unresolved; no resolver link, observed 2026-08-02T18:35:52.977343Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation fc703ae5-1633-49d2-970f-c32c31ed0d85 · 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-to-dS and dS-to-dS transitions: Implications for the $H_0$ tension

Reference 93

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 87d19040-4927-493a-b10c-fa301efbd8fb · 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-to-dS and dS-to-dS transitions: Implications for the $H_0$ tension

Reference 44

Resolution: verified exact; arxiv_id, observed 2026-05-10T14:15:30.105612Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

Observation 77434247-2a2f-4daa-9d1a-f686687b5098 · inbound

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

Negative neutrino mass or negative dark energy? Dynamical dark energy with AdS-to-dS and dS-to-dS transitions: Implications for the $H_0$ tension

Reference 63

Resolution: verified exact; arxiv_id, observed 2026-05-21T03:03:55.598272Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

Observation d445d2d1-4a4a-4b13-8b2d-9c9e83e83d8c · inbound

What it takes to solve the Hubble tension through Modifications of Cosmological Recombination II: in light of ACT DR6 and DESI DR2 cites this paper.

What it takes to solve the Hubble tension through Modifications of Cosmological Recombination II: in light of ACT DR6 and DESI DR2 Dynamical dark energy with AdS-to-dS and dS-to-dS transitions: Implications for the $H_0$ tension

Reference 124

Resolution: verified exact; arxiv_id, observed 2026-07-02T15:37:06.540402Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

Observation a46ebf2d-c9aa-4007-aa1e-2720e1beab83 · 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-to-dS and dS-to-dS transitions: Implications for the $H_0$ tension

Reference 32

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 3b58f4d9-2822-498c-868b-b8ad3c72ef99 · 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-to-dS and dS-to-dS transitions: Implications for the $H_0$ tension

Reference 32

Resolution: verified exact; arxiv_id, observed 2026-07-03T07:07:44.866654Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

Observation 678f8c92-615b-42f4-83e4-1e9ff985f056 · inbound

Cosmological Viability of Exponential Infrared $f(T)$ Gravity cites this paper.

Cosmological Viability of Exponential Infrared $f(T)$ Gravity Dynamical dark energy with AdS-to-dS and dS-to-dS transitions: Implications for the $H_0$ tension

Reference 193

Resolution: verified exact; arxiv_id, observed 2026-07-01T11:15:42.203797Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

Observation 1793422d-2377-40aa-bec3-87ef896a007c · 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-to-dS and dS-to-dS transitions: Implications for the $H_0$ tension

Reference 92

Resolution: unresolved; no resolver link, observed 2026-08-01T16:30:04.343637Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 217f52e3-5fad-47c7-ac47-fba20eb58718 · inbound

Hubble tension: the shape wall cites this paper.

Hubble tension: the shape wall Dynamical dark energy with AdS-to-dS and dS-to-dS transitions: Implications for the $H_0$ tension

Reference 157

Resolution: unresolved; no resolver link, observed 2026-08-01T08:08:48.905165Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.