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Paper Citation Record · LEDGER

Inevitable manifestation of wiggles in the expansion of the late Universe

As of 15 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 8 inbound Pith citation observations for arXiv:2207.10609.

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

pith.paper-citation-record.v1
2207.10609 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 8 of 8 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-15T06:32:42.880941+00:00

measured 8 of 8 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-12T04:57:06.726709Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-05-24T03:53:54.335151Z

Reference resolution

0 of 0 outbound references displayed

  • verified exact0
  • verified fuzzy0
  • unresolved0
  • parse uncertain0
  • malformed identifier0
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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 5d640cf6-dd55-4540-889b-0cf80df7222d · 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 Inevitable manifestation of wiggles in the expansion of the late Universe

Reference 111

Resolution
verified exact
arxiv_id, observed 2026-05-24T03:53:54.338083Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

source=pdf_text observed=2026-05-24T03:50:50.435997Z digest=sha256:66696537fb857e12aafc72a07052955c28972f316d598382d10b168ec9822031

Observation 4835f69a-dc2a-4eef-8dca-b8e9943970a5 · inbound

Exploring cosmological imprints of phantom crossing with dynamical dark energy in Horndeski gravity cites this paper.

Exploring cosmological imprints of phantom crossing with dynamical dark energy in Horndeski gravity Inevitable manifestation of wiggles in the expansion of the late Universe

Reference 23

Resolution
unresolved
no resolver link, observed 2026-08-12T04:57:06.726709Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-12T04:57:06.726709Z digest=sha256:19687686bfae68a00d9c064a371fd141e6ab3d048c587c1c6554298d55c329bc

Observation f0d05384-929b-4307-9270-42a1cf35c379 · inbound

DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics? cites this paper.

DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics? Inevitable manifestation of wiggles in the expansion of the late Universe

Reference 112

Resolution
unresolved
no resolver link, observed 2026-08-11T13:41:23.978168Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-11T13:41:23.978168Z digest=sha256:e12e0ee3b1ff1231a75fe97cb16825d6c301e8b2629c028b973cada6b53b08a4

Observation 3818663d-964c-4c31-b161-0a2516448412 · 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 Inevitable manifestation of wiggles in the expansion of the late Universe

Reference 173

Resolution
verified exact
arxiv_id, observed 2026-05-18T04:50:55.128356Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

source=pdf_text observed=2026-05-18T04:46:14.832965Z digest=sha256:f81ce16ddcf26e801a71c300f8361471706ba88ee40f14ec8a0c4a176fd9822a

Observation 28ec00f9-39e3-4bb9-83b4-c1d5eb761c56 · 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 Inevitable manifestation of wiggles in the expansion of the late Universe

Reference 125

Resolution
verified exact
arxiv_id, observed 2026-05-21T13:30:11.851360Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

source=pdf_text observed=2026-05-21T13:29:05.147292Z digest=sha256:fb066489c989770f0cf328bac0127891249e21f23c2c05a9f1040d94cbd0c543

Observation c2e767df-23be-4d62-a348-a8fba133de99 · 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 Inevitable manifestation of wiggles in the expansion of the late Universe

Reference 136

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

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-07-15T12:01:04.317365Z digest=sha256:7c07ab47de13bce00df35888af9697ec5532982a5bd35465c622c85a5e49a68b

Observation c94cf6a5-bded-4127-b990-489c07235194 · 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? Inevitable manifestation of wiggles in the expansion of the late Universe

Reference 66

Resolution
verified exact
arxiv_id, observed 2026-05-10T14:20:30.975749Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

source=pdf_text observed=2026-05-10T14:10:57.749079Z digest=sha256:d385c6653408e81f2892d0733b7b45189749d3c459bb36905ee775b656fecb8f

Observation c1569f77-321c-4ef1-8480-4c9aa381281f · 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 Inevitable manifestation of wiggles in the expansion of the late Universe

Reference 114

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

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-07-11T09:40:49.196932Z digest=sha256:5c65457d176cb1e996274a232b3f5ed0d4ec391914f205d6e076f281ca27631e