Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Remedy of some cosmological tensions via effective phantom-like behavior of interacting vacuum energy
As of 19 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 7 inbound Pith citation observations for arXiv:2102.12902.
A citation records a reference. It does not transfer a finding from one paper to another.
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One-hop event checks from named stored sources.
Source: scholarly_work_events, retraction_status_cache, observed 2026-08-19T06:32:44.657259+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-10T19:20:16.860847Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-07-03T07:47:45.299592Z
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0 of 0 outbound references displayed
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Outbound references
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Pith citing papers
Observation c7d0424b-4015-4d20-b6b0-ddcd747f1ab4 · 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 Remedy of some cosmological tensions via effective phantom-like behavior of interacting vacuum energy
Reference 134
- Resolution
- verified exact
- arxiv_id, observed 2026-05-24T03:53:54.708772Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.
Observation 85787442-bcfe-450e-9513-e65b38113d79 · inbound
Sign Switching in Dark Sector Coupling Interactions as a Candidate for Resolving Cosmological Tensions cites this paper.
Sign Switching in Dark Sector Coupling Interactions as a Candidate for Resolving Cosmological Tensions Remedy of some cosmological tensions via effective phantom-like behavior of interacting vacuum energy
Reference 88
- Resolution
- unresolved
- no resolver link, observed 2026-08-10T19:20:16.860847Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 967dc137-7f5b-4ad1-994d-61e99f6e1596 · inbound
Revisiting the Matter Creation Process: Observational Constraints on Gravitationally Induced Dark Energy and the Hubble Tension cites this paper.
Revisiting the Matter Creation Process: Observational Constraints on Gravitationally Induced Dark Energy and the Hubble Tension Remedy of some cosmological tensions via effective phantom-like behavior of interacting vacuum energy
Reference 83
- Resolution
- verified exact
- arxiv_id, observed 2026-05-16T12:17:52.607149Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.
Observation e780ec1e-ef30-4770-9a0c-1b1395ca57db · 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 Remedy of some cosmological tensions via effective phantom-like behavior of interacting vacuum energy
Reference 61
- Resolution
- verified exact
- arxiv_id, observed 2026-05-21T13:30:11.890850Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.
Observation 5491f2e1-115b-4b75-a967-1ef477b00b2f · 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 Remedy of some cosmological tensions via effective phantom-like behavior of interacting vacuum energy
Reference 70
- 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 7d1a57d7-c270-455d-9706-227c5cdae240 · 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 Remedy of some cosmological tensions via effective phantom-like behavior of interacting vacuum energy
Reference 42
- Resolution
- verified exact
- arxiv_id, observed 2026-07-02T15:37:06.596524Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.
Observation ef14786c-a8f7-446e-98f9-1851b5a7c1a5 · inbound
Non-linear Structure Formation in Planck+DESI Favoured Interacting Dark Energy Cosmologies cites this paper.
Non-linear Structure Formation in Planck+DESI Favoured Interacting Dark Energy Cosmologies Remedy of some cosmological tensions via effective phantom-like behavior of interacting vacuum energy
Reference 38
- Resolution
- verified exact
- arxiv_id, observed 2026-07-03T07:47:45.300765Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.