Paper Citation Record · LEDGER

Exploring new physics in the late Universe's expansion through non-parametric inference

As of 8 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 12 inbound Pith citation observations for arXiv:2407.04223.

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

pith.paper-citation-record.v1
2407.04223 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

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measured 12 of 12 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-08T06:32:00.761636+00:00

measured 12 of 12 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-07T12:25:52.140348Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-05-24T03:53:54.518945Z

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 d4d076ec-612a-4671-a0cc-fe5368b87ac5 · inbound

$\Lambda_{\rm s}$CDM cosmology from a type-II minimally modified gravity cites this paper.

$\Lambda_{\rm s}$CDM cosmology from a type-II minimally modified gravity Exploring new physics in the late Universe's expansion through non-parametric inference

Reference 143

Resolution: verified exact; arxiv_id, observed 2026-05-24T03:53:54.522629Z

Source-reported events for the cited work

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Observation 60413145-fb44-4a71-b967-ac77087a4ea7 · inbound

Revisiting the temperature evolution law of the CMB with gaussian processes cites this paper.

Revisiting the temperature evolution law of the CMB with gaussian processes Exploring new physics in the late Universe's expansion through non-parametric inference

Reference 54

Resolution: unresolved; no resolver link, observed 2026-08-07T12:25:52.140348Z

Source-reported events for the cited work

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Observation f8cd5f60-ed28-480a-9f3a-9a7aee401990 · inbound

Is $\omega_0 \omega_a$CDM a good model for the clumpy Universe? cites this paper.

Is $\omega_0 \omega_a$CDM a good model for the clumpy Universe? Exploring new physics in the late Universe's expansion through non-parametric inference

Reference 60

Resolution: unresolved; no resolver link, observed 2026-08-06T21:15:10.137016Z

Source-reported events for the cited work

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Observation 638be0f4-df40-4646-a8b8-7cf01577f3be · 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 Exploring new physics in the late Universe's expansion through non-parametric inference

Reference 200

Resolution: verified exact; arxiv_id, observed 2026-05-18T04:50:55.203284Z

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Observation a7500c11-ccd9-48ee-a634-58cf358567ac · 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 Exploring new physics in the late Universe's expansion through non-parametric inference

Reference 147

Resolution: verified exact; arxiv_id, observed 2026-05-21T13:30:12.405790Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

Observation 43e9adc5-1767-4ab3-a2bb-c65c3a7e52c5 · 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 Exploring new physics in the late Universe's expansion through non-parametric inference

Reference 158

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 0b3481c5-f28b-47a3-ab63-4ebdb1ca6977 · 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? Exploring new physics in the late Universe's expansion through non-parametric inference

Reference 106

Resolution: verified exact; arxiv_id, observed 2026-05-10T14:20:31.193470Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

Observation 360defe8-0edd-48e1-a912-bc7bfe94dc88 · inbound

Geometric Constraints on the Pre-Recombination Expansion History from the Hubble Tension cites this paper.

Geometric Constraints on the Pre-Recombination Expansion History from the Hubble Tension Exploring new physics in the late Universe's expansion through non-parametric inference

Reference 110

Resolution: verified exact; arxiv_id, observed 2026-05-12T00:36:16.233348Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

Observation c1dce4cf-0922-4bb3-a0a6-16443586a0e6 · inbound

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

Negative neutrino mass or negative dark energy? Exploring new physics in the late Universe's expansion through non-parametric inference

Reference 60

Resolution: verified exact; arxiv_id, observed 2026-05-21T03:03:55.538979Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

Observation 50a24fc0-3709-4f98-84e3-f40b24088668 · inbound

Alleviating the Hubble Tension with Smooth Sign-Switching Dark Energy: Full CMB Constraints with DESI and PantheonPlus cites this paper.

Alleviating the Hubble Tension with Smooth Sign-Switching Dark Energy: Full CMB Constraints with DESI and PantheonPlus Exploring new physics in the late Universe's expansion through non-parametric inference

Reference 135

Resolution: unresolved; no resolver link, observed 2026-07-11T09:40:49.196932Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation eea9ecb5-60f8-438b-95b4-1d5f88512419 · 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 Exploring new physics in the late Universe's expansion through non-parametric inference

Reference 51

Resolution: unresolved; no resolver link, observed 2026-08-01T16:30:00.139235Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 46f03398-aaa6-4fb8-b548-0e70896245d7 · inbound

Hubble tension: the shape wall cites this paper.

Hubble tension: the shape wall Exploring new physics in the late Universe's expansion through non-parametric inference

Reference 256

Resolution: unresolved; no resolver link, observed 2026-08-01T08:08:58.667903Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.