Paper Citation Record · LEDGER

Omnipotent dark energy: A phenomenological answer to the Hubble tension

As of 14 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 21 inbound Pith citation observations for arXiv:2306.08046.

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pith.paper-citation-record.v1
2306.08046 v2

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Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-12T04:57:06.793851Z

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

Source: arxiv_reference, observed 2026-07-02T15:37:06.377881Z

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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

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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 Omnipotent dark energy: A phenomenological answer to the Hubble tension

Reference 35

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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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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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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

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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

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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

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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

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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

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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

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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

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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

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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

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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

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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

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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

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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

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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

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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

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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: unresolved; no resolver link, observed 2026-08-01T08:08:45.743611Z

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Observation bf14b198-9ee5-43f8-8517-4e6a3f50208b · inbound

Adiabatic Perturbations in GW170817-Compatible Einstein-Gauss-Bonnet Inflation cites this paper.

Adiabatic Perturbations in GW170817-Compatible Einstein-Gauss-Bonnet Inflation Omnipotent dark energy: A phenomenological answer to the Hubble tension

Reference 148

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