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Paper Citation Record · LEDGER

Interacting dark energy in the early 2020s: a promising solution to the $H_0$ and cosmic shear tensions

As of 9 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 36 inbound Pith citation observations for arXiv:1908.04281.

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pith.paper-citation-record.v1
1908.04281 v2

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Pith citing papers itemized under the disclosed page cap.

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Pith citing papers

Observation 272bc0ef-b06f-4082-9cf5-473cac880da6 · 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 Interacting dark energy in the early 2020s: a promising solution to the $H_0$ and cosmic shear tensions

Reference 131

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Observation 28ca14df-e58e-4b0b-a008-7dde6451c7b5 · inbound

Little ado about everything II: an `emergent' dark energy from structure formation to rule cosmic tensions cites this paper.

Little ado about everything II: an `emergent' dark energy from structure formation to rule cosmic tensions Interacting dark energy in the early 2020s: a promising solution to the $H_0$ and cosmic shear tensions

Reference 96

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Observation c0a76884-7d56-460e-b097-f2ffc0ecc208 · 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 Interacting dark energy in the early 2020s: a promising solution to the $H_0$ and cosmic shear tensions

Reference 104

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Observation 9e83fd46-87f6-486f-a968-fc7c81b5020d · inbound

The Quintom theory of dark energy after DESI DR2 cites this paper.

The Quintom theory of dark energy after DESI DR2 Interacting dark energy in the early 2020s: a promising solution to the $H_0$ and cosmic shear tensions

Reference 213

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Solving an Interacting Quintessence Model with a Sound Horizon Initial Condition and its Observational Constraints cites this paper.

Solving an Interacting Quintessence Model with a Sound Horizon Initial Condition and its Observational Constraints Interacting dark energy in the early 2020s: a promising solution to the $H_0$ and cosmic shear tensions

Reference 67

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Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime cites this paper.

Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime Interacting dark energy in the early 2020s: a promising solution to the $H_0$ and cosmic shear tensions

Reference 59

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Hubble Tension and the G-step Model: Re-examination of Recent Constraints on Modified Local Physics cites this paper.

Hubble Tension and the G-step Model: Re-examination of Recent Constraints on Modified Local Physics Interacting dark energy in the early 2020s: a promising solution to the $H_0$ and cosmic shear tensions

Reference 50

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Dark Energy Is Not That Into You: Variable Couplings after DESI DR2 BAO cites this paper.

Dark Energy Is Not That Into You: Variable Couplings after DESI DR2 BAO Interacting dark energy in the early 2020s: a promising solution to the $H_0$ and cosmic shear tensions

Reference 64

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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 Interacting dark energy in the early 2020s: a promising solution to the $H_0$ and cosmic shear tensions

Reference 214

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Observation 84c2c7b6-9487-48cf-b717-0f3f01ea601a · inbound

Alleviating the $H_0$ tension through the interacting dark energy model from quantum gravitational field theory in light of DESI DR2 cites this paper.

Alleviating the $H_0$ tension through the interacting dark energy model from quantum gravitational field theory in light of DESI DR2 Interacting dark energy in the early 2020s: a promising solution to the $H_0$ and cosmic shear tensions

Reference 88

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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 Interacting dark energy in the early 2020s: a promising solution to the $H_0$ and cosmic shear tensions

Reference 83

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Dark sector interactions in the $w \rightarrow -1$ limit: velocity locking in pure momentum exchange models cites this paper.

Dark sector interactions in the $w \rightarrow -1$ limit: velocity locking in pure momentum exchange models Interacting dark energy in the early 2020s: a promising solution to the $H_0$ and cosmic shear tensions

Reference 25

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A microphysically inspired approach to dark matter-dark energy interactions: first bounds on dark-sector scattering cross sections cites this paper.

A microphysically inspired approach to dark matter-dark energy interactions: first bounds on dark-sector scattering cross sections Interacting dark energy in the early 2020s: a promising solution to the $H_0$ and cosmic shear tensions

Reference 21

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Robust Preference for Dark Sector Interactions cites this paper.

Robust Preference for Dark Sector Interactions Interacting dark energy in the early 2020s: a promising solution to the $H_0$ and cosmic shear tensions

Reference 83

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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 Interacting dark energy in the early 2020s: a promising solution to the $H_0$ and cosmic shear tensions

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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 Interacting dark energy in the early 2020s: a promising solution to the $H_0$ and cosmic shear tensions

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Disentangling Similarity and Relatedness in Topic Models cites this paper.

Disentangling Similarity and Relatedness in Topic Models Interacting dark energy in the early 2020s: a promising solution to the $H_0$ and cosmic shear tensions

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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 Interacting dark energy in the early 2020s: a promising solution to the $H_0$ and cosmic shear tensions

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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 Interacting dark energy in the early 2020s: a promising solution to the $H_0$ and cosmic shear tensions

Reference 35

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Effective field theory interpretation of ATLAS measurements involving the Higgs boson, electroweak bosons and the top quark cites this paper.

Effective field theory interpretation of ATLAS measurements involving the Higgs boson, electroweak bosons and the top quark Interacting dark energy in the early 2020s: a promising solution to the $H_0$ and cosmic shear tensions

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Saturation Mechanisms in the Interacting Dark Sector cites this paper.

Saturation Mechanisms in the Interacting Dark Sector Interacting dark energy in the early 2020s: a promising solution to the $H_0$ and cosmic shear tensions

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Accelerating scaling solutions from dark matter particle creation cites this paper.

Accelerating scaling solutions from dark matter particle creation Interacting dark energy in the early 2020s: a promising solution to the $H_0$ and cosmic shear tensions

Reference 49

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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 Interacting dark energy in the early 2020s: a promising solution to the $H_0$ and cosmic shear tensions

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Alleviating the Hubble Tension Using $\Lambda$sCDM Model: A Coupled Dark Energy - Dark Matter Interaction cites this paper.

Alleviating the Hubble Tension Using $\Lambda$sCDM Model: A Coupled Dark Energy - Dark Matter Interaction Interacting dark energy in the early 2020s: a promising solution to the $H_0$ and cosmic shear tensions

Reference 26

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Alleviating the Hubble Tension Using $\Lambda$sCDM Model: A Coupled Dark Energy - Dark Matter Interaction cites this paper.

Alleviating the Hubble Tension Using $\Lambda$sCDM Model: A Coupled Dark Energy - Dark Matter Interaction Interacting dark energy in the early 2020s: a promising solution to the $H_0$ and cosmic shear tensions

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Unifying Early and Late Dark Energy: Dynamical Requirements and Obstructions cites this paper.

Unifying Early and Late Dark Energy: Dynamical Requirements and Obstructions Interacting dark energy in the early 2020s: a promising solution to the $H_0$ and cosmic shear tensions

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Neutrino mass constraints in interacting dark energy models after DESI DR2 cites this paper.

Neutrino mass constraints in interacting dark energy models after DESI DR2 Interacting dark energy in the early 2020s: a promising solution to the $H_0$ and cosmic shear tensions

Reference 147

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Dissipative Cosmology and the Nature of Dark Energy: Insights from Bulk Viscosity with DESI DR2 observations cites this paper.

Dissipative Cosmology and the Nature of Dark Energy: Insights from Bulk Viscosity with DESI DR2 observations Interacting dark energy in the early 2020s: a promising solution to the $H_0$ and cosmic shear tensions

Reference 111

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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 Interacting dark energy in the early 2020s: a promising solution to the $H_0$ and cosmic shear tensions

Reference 22

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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 Interacting dark energy in the early 2020s: a promising solution to the $H_0$ and cosmic shear tensions

Reference 65

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Cosmological Viability of Exponential Infrared $f(T)$ Gravity cites this paper.

Cosmological Viability of Exponential Infrared $f(T)$ Gravity Interacting dark energy in the early 2020s: a promising solution to the $H_0$ and cosmic shear tensions

Reference 164

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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 Interacting dark energy in the early 2020s: a promising solution to the $H_0$ and cosmic shear tensions

Reference 177

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Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

source=pdf_text observed=2026-07-01T04:31:47.886338Z digest=sha256:fca0b7cd8e42dd82a0a3b53e7b7ad358c5cd19b7982b40f66f6c7d366d7cf388

Observation 681ee92d-f6cd-4c72-b1d7-50a8d5f29c47 · inbound

Neutrino mass constraints in the Schwarzschild-de Sitter black-hole dark energy model with ACT DR6 and DESI DR2 data cites this paper.

Neutrino mass constraints in the Schwarzschild-de Sitter black-hole dark energy model with ACT DR6 and DESI DR2 data Interacting dark energy in the early 2020s: a promising solution to the $H_0$ and cosmic shear tensions

Reference 27

Resolution
unresolved
no resolver link, observed 2026-07-12T04:18:55.037825Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-07-12T04:18:55.037825Z digest=sha256:4e53929c643dedeefaf54003b45a7def6f14dcf5265ac8c1ec6b5e975b6eb1f3

Observation 564ada54-2cef-4891-83be-704415d171c7 · inbound

The $H_0$ World Cup. I. Summary of the baseline group stage results cites this paper.

The $H_0$ World Cup. I. Summary of the baseline group stage results Interacting dark energy in the early 2020s: a promising solution to the $H_0$ and cosmic shear tensions

Reference 87

Resolution
unresolved
no resolver link, observed 2026-08-02T05:41:40.493993Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-02T05:41:40.493993Z digest=sha256:7784946c6ae827f0ddcf2d6f44d4ac31e21a05444fff7048fb4a4dfbb2abfb1a

Observation 1e0892a2-43a1-4685-b83a-36457fb87b65 · inbound

The $H_0$ world cup. II. A comprehensive competition between proposed Hubble tension solutions cites this paper.

The $H_0$ world cup. II. A comprehensive competition between proposed Hubble tension solutions Interacting dark energy in the early 2020s: a promising solution to the $H_0$ and cosmic shear tensions

Reference 178

Resolution
unresolved
no resolver link, observed 2026-08-02T05:48:21.596561Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-02T05:48:21.596561Z digest=sha256:fc2ff0bf1ddb313f0e4e21f1ba0387cfb6396a1242fb1d2a4c652ebbf9cc1dd0

Observation 8534522e-bdfe-4e63-ab65-57ddee2a5516 · inbound

Hubble tension: the shape wall cites this paper.

Hubble tension: the shape wall Interacting dark energy in the early 2020s: a promising solution to the $H_0$ and cosmic shear tensions

Reference 56

Resolution
unresolved
no resolver link, observed 2026-08-01T08:08:36.493547Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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