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Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Omnipotent dark energy: A phenomenological answer to the Hubble tension
As of 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 19 inbound Pith citation observations for arXiv:2306.08046.
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 2026-08-10T06:31:04.303077+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-10T19:20:16.716650Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-07-02T15:37:06.377881Z
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Outbound references
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Pith citing papers
Observation 165b5e7f-d8a0-451b-b6ca-ae26479e12ae · 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 Omnipotent dark energy: A phenomenological answer to the Hubble tension
Reference 124
- Resolution
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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 c6ec7e3c-bd57-4c4c-95e5-57b15937d663 · 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 Omnipotent dark energy: A phenomenological answer to the Hubble tension
Reference 64
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Observation 36207ca8-afc7-4d70-8f63-bd476c4eaa9b · inbound
Mapping the $\Lambda_{\rm s}$CDM scenario to $f(T)$ modified gravity: Effects on structure growth rate cites this paper.
Mapping the $\Lambda_{\rm s}$CDM scenario to $f(T)$ modified gravity: Effects on structure growth rate Omnipotent dark energy: A phenomenological answer to the Hubble tension
Reference 51
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Observation 6714754a-7349-4a95-bd44-15a3e80f3564 · inbound
An overview of what current data can (and cannot yet) say about evolving dark energy cites this paper.
An overview of what current data can (and cannot yet) say about evolving dark energy Omnipotent dark energy: A phenomenological answer to the Hubble tension
Reference 191
- Resolution
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Source-reported events for the cited work
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Observation e0bd1a54-6a42-49e1-be2c-9cd7e468d1d6 · inbound
BAO miscalibration cannot rescue late-time solutions to the Hubble tension cites this paper.
BAO miscalibration cannot rescue late-time solutions to the Hubble tension Omnipotent dark energy: A phenomenological answer to the Hubble tension
Reference 284
- Resolution
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Source-reported events for the cited work
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Observation 49907a87-e056-43d8-968e-284c3835b3f8 · 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 Omnipotent dark energy: A phenomenological answer to the Hubble tension
Reference 181
- Resolution
- verified exact
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Source-reported events for the cited work
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Observation d1803a6e-3dcc-4d65-a615-448e8a53c8e7 · 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 Omnipotent dark energy: A phenomenological answer to the Hubble tension
Reference 94
- Resolution
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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 b778f9da-3dd8-43de-b45f-ac2b4e2fb65b · 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 Omnipotent dark energy: A phenomenological answer to the Hubble tension
Reference 103
- Resolution
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Source-reported events for the cited work
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Observation b93e1d9e-fbfa-4418-9754-ed8407edaec1 · inbound
Double the axions, half the tension: multi-field early dark energy eases the Hubble tension cites this paper.
Double the axions, half the tension: multi-field early dark energy eases the Hubble tension Omnipotent dark energy: A phenomenological answer to the Hubble tension
Reference 62
- Resolution
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Observation 354760a9-2b2c-457c-b3e0-bf57dcc23d36 · 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 Omnipotent dark energy: A phenomenological answer to the Hubble tension
Reference 43
- Resolution
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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 3410c7cc-a420-4866-ae31-923985370526 · inbound
Latent-Space Gaussian Processes for Dark-Energy Reconstruction from Observational \(H(z)\) Data cites this paper.
Latent-Space Gaussian Processes for Dark-Energy Reconstruction from Observational \(H(z)\) Data Omnipotent dark energy: A phenomenological answer to the Hubble tension
Reference 53
- Resolution
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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 c6d31f01-6e5c-4ee6-bc65-ac52396071d8 · inbound
Negative neutrino mass or negative dark energy? cites this paper.
Negative neutrino mass or negative dark energy? Omnipotent dark energy: A phenomenological answer to the Hubble tension
Reference 37
- Resolution
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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 8bf1e524-705e-44ed-acf7-b53d82a6d481 · inbound
Early- and Late-Time Modifications to $\Lambda$CDM: Implications for the Hubble Tension cites this paper.
Early- and Late-Time Modifications to $\Lambda$CDM: Implications for the Hubble Tension Omnipotent dark energy: A phenomenological answer to the Hubble tension
Reference 59
- Resolution
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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 f8b7c3dc-f865-4858-8eb2-84ad27265f03 · inbound
Reconstructing dark energy with fewer assumptions cites this paper.
Reconstructing dark energy with fewer assumptions Omnipotent dark energy: A phenomenological answer to the Hubble tension
Reference 112
- Resolution
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Source-reported events for the cited work
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Observation 88284827-ccb9-4ce7-a7a2-2d4802590f81 · 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 Omnipotent dark energy: A phenomenological answer to the Hubble tension
Reference 69
- Resolution
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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 df76679a-2ed8-4a7b-8148-58ab9addc50b · inbound
Running into tension: primordial black holes from ultra-slow-roll inflation, spectral running, and the Hubble tension cites this paper.
Running into tension: primordial black holes from ultra-slow-roll inflation, spectral running, and the Hubble tension Omnipotent dark energy: A phenomenological answer to the Hubble tension
Reference 209
- Resolution
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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 c998bed3-3a19-4767-9b6e-ca7309d1dd34 · 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 Omnipotent dark energy: A phenomenological answer to the Hubble tension
Reference 83
- Resolution
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Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 4765ad8d-3623-42e2-8587-9d769b0eb385 · 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 Omnipotent dark energy: A phenomenological answer to the Hubble tension
Reference 44
- Resolution
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Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 3de4466e-75cd-49bf-bfa7-de6d63651125 · inbound
Hubble tension: the shape wall cites this paper.
Hubble tension: the shape wall Omnipotent dark energy: A phenomenological answer to the Hubble tension
Reference 129
- Resolution
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Source-reported events for the cited work
Unavailable: canonical work link unavailable.