Paper Citation Record · LEDGER

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

As of 21 August 2026, this Paper Citation Record lists 100 of 300 outbound references and 43 inbound Pith citation observations for arXiv:1908.04281.

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1908.04281 v2

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measured 100 of 300 reference resolution

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Observation 8ac032b0-59f5-4c69-8039-0d5432eca178 · outbound

This paper cites Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant.

Interacting dark energy in the early 2020s: a promising solution to the $H_0$ and cosmic shear tensions Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant

Reference 1

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Observation 79d51aa1-bf5f-475f-9161-52608be0f5c9 · outbound

This paper cites Measurements of Omega and Lambda from 42 High-Redshift Supernovae.

Interacting dark energy in the early 2020s: a promising solution to the $H_0$ and cosmic shear tensions Measurements of Omega and Lambda from 42 High-Redshift Supernovae

Reference 2

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Observation 1087159b-36c1-4cca-81cc-f92f16abbded · outbound

This paper cites Planck 2015 results. XIII. Cosmological parameters.

Interacting dark energy in the early 2020s: a promising solution to the $H_0$ and cosmic shear tensions Planck 2015 results. XIII. Cosmological parameters

Reference 3

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Observation de9acdaa-3df8-47d3-a435-49cf3b619c75 · outbound

This paper cites The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological analysis of the DR12 galaxy sample.

Interacting dark energy in the early 2020s: a promising solution to the $H_0$ and cosmic shear tensions The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological analysis of the DR12 galaxy sample

Reference 4

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Observation 659f0055-25f2-4edb-84b2-0ebb93042a21 · outbound

This paper cites Dark Energy Survey Year 1 Results: Cosmological Constraints from Cosmic Shear.

Interacting dark energy in the early 2020s: a promising solution to the $H_0$ and cosmic shear tensions Dark Energy Survey Year 1 Results: Cosmological Constraints from Cosmic Shear

Reference 5

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Observation 1c800e3d-9c8a-4b5c-b389-5668f1998db2 · outbound

This paper cites Cosmology at at Crossroads: Tension with the Hubble Constant.

Interacting dark energy in the early 2020s: a promising solution to the $H_0$ and cosmic shear tensions Cosmology at at Crossroads: Tension with the Hubble Constant

Reference 6

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Observation 07ed142c-3cc6-41ef-b98e-cc3d52de5f46 · outbound

This paper cites Crack in the cosmological paradigm.

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

Reference 7

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Observation 76a9d7ae-ebc8-4a4b-b6ef-83e176612a26 · outbound

This paper cites Planck 2018 results. VI. Cosmological parameters.

Interacting dark energy in the early 2020s: a promising solution to the $H_0$ and cosmic shear tensions Planck 2018 results. VI. Cosmological parameters

Reference 8

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Observation c30f7ba7-2d89-4339-b951-7d5ec98b6212 · outbound

This paper cites Large Magellanic Cloud Cepheid Standards Provide a 1% Foundation for the Determination of the Hubble Constant and Stronger Evidence for Physics Beyond LambdaCDM.

Interacting dark energy in the early 2020s: a promising solution to the $H_0$ and cosmic shear tensions Large Magellanic Cloud Cepheid Standards Provide a 1% Foundation for the Determination of the Hubble Constant and Stronger Evidence for Physics Beyond LambdaCDM

Reference 9

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Observation e06f4e8f-18eb-43e7-9dac-85c4441bd6e7 · outbound

This paper cites Constraining the Cosmology of the Phantom Brane using Distance Measures.

Interacting dark energy in the early 2020s: a promising solution to the $H_0$ and cosmic shear tensions Constraining the Cosmology of the Phantom Brane using Distance Measures

Reference 10

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Observation de7ee068-46c6-40ca-9f8e-792aa3929353 · outbound

This paper cites Reconciling Planck with the local value of $H_0$ in extended parameter space.

Interacting dark energy in the early 2020s: a promising solution to the $H_0$ and cosmic shear tensions Reconciling Planck with the local value of $H_0$ in extended parameter space

Reference 11

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Observation abb33c6d-3b2b-4817-9a5f-44cd28e15357 · outbound

This paper cites How the Dark Energy Can Reconcile \textit{Planck} with Local Determination of the Hubble Constant.

Interacting dark energy in the early 2020s: a promising solution to the $H_0$ and cosmic shear tensions How the Dark Energy Can Reconcile \textit{Planck} with Local Determination of the Hubble Constant

Reference 12

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Observation 79215033-f76e-4ac1-9faf-775578b5dc04 · outbound

This paper cites The trouble with $H_0$.

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

Reference 13

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Observation 4af1a396-2821-44ce-b255-ad28443e812d · outbound

This paper cites Light dark photon and fermionic dark radiation for the Hubble constant and the structure formation.

Interacting dark energy in the early 2020s: a promising solution to the $H_0$ and cosmic shear tensions Light dark photon and fermionic dark radiation for the Hubble constant and the structure formation

Reference 14

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Observation b3b65b6d-7175-4971-8106-042312da5a80 · outbound

This paper cites Early dark energy, the Hubble-parameter tension, and the string axiverse.

Interacting dark energy in the early 2020s: a promising solution to the $H_0$ and cosmic shear tensions Early dark energy, the Hubble-parameter tension, and the string axiverse

Reference 15

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Observation 6afd31fe-27f2-4841-b216-5a92ecf197b1 · outbound

This paper cites Partially Acoustic Dark Matter, Interacting Dark Radiation, and Large Scale Structure.

Interacting dark energy in the early 2020s: a promising solution to the $H_0$ and cosmic shear tensions Partially Acoustic Dark Matter, Interacting Dark Radiation, and Large Scale Structure

Reference 16

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Observation be3f0589-8cfe-4285-8b7d-f6d792789e64 · outbound

This paper cites Dynamical dark energy in light of the latest observations.

Interacting dark energy in the early 2020s: a promising solution to the $H_0$ and cosmic shear tensions Dynamical dark energy in light of the latest observations

Reference 17

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Observation 8b5f2f0c-3322-46b3-8750-3a44b0597011 · outbound

This paper cites Unveiling $\nu$ secrets with cosmological data: neutrino masses and mass hierarchy.

Interacting dark energy in the early 2020s: a promising solution to the $H_0$ and cosmic shear tensions Unveiling $\nu$ secrets with cosmological data: neutrino masses and mass hierarchy

Reference 18

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Observation 279aac6f-9f3f-4e3a-972c-50646d6b94e2 · outbound

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

Reference 19

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This paper cites Do joint CMB and HST data support a scale invariant spectrum?.

Interacting dark energy in the early 2020s: a promising solution to the $H_0$ and cosmic shear tensions Do joint CMB and HST data support a scale invariant spectrum?

Reference 20

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Interacting dark energy in the early 2020s: a promising solution to the $H_0$ and cosmic shear tensions A search for sterile neutrinos with the latest cosmological observations

Reference 21

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Observation 92f3d01f-11d6-40a8-b98e-9876876cb6bd · outbound

This paper cites Search for sterile neutrinos in holographic dark energy cosmology: Reconciling Planck observation with the local measurement of the Hubble constant.

Interacting dark energy in the early 2020s: a promising solution to the $H_0$ and cosmic shear tensions Search for sterile neutrinos in holographic dark energy cosmology: Reconciling Planck observation with the local measurement of the Hubble constant

Reference 22

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This paper cites Constraining Dark Energy Dynamics in Extended Parameter Space.

Interacting dark energy in the early 2020s: a promising solution to the $H_0$ and cosmic shear tensions Constraining Dark Energy Dynamics in Extended Parameter Space

Reference 23

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Interacting dark energy in the early 2020s: a promising solution to the $H_0$ and cosmic shear tensions Cosmological searches for a non-cold dark matter component

Reference 24

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Interacting dark energy in the early 2020s: a promising solution to the $H_0$ and cosmic shear tensions Changing the prior: absolute neutrino mass constraints in nonlocal gravity

Reference 25

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Observation bb0fb8e5-a7da-4417-9c6e-a3e05fa51c7c · outbound

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Interacting dark energy in the early 2020s: a promising solution to the $H_0$ and cosmic shear tensions The $H_0$ tension in light of vacuum dynamics in the Universe

Reference 26

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Interacting dark energy in the early 2020s: a promising solution to the $H_0$ and cosmic shear tensions Searching for sterile neutrinos in dynamical dark energy cosmologies

Reference 27

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This paper cites Galileon Gravity in Light of ISW, CMB, BAO and $H_0$ data.

Interacting dark energy in the early 2020s: a promising solution to the $H_0$ and cosmic shear tensions Galileon Gravity in Light of ISW, CMB, BAO and $H_0$ data

Reference 28

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Observation 6916f1e8-5dfc-4daf-b00b-4821cea28259 · outbound

This paper cites Latest astronomical constraints on some nonlinear parametric dark energy models.

Interacting dark energy in the early 2020s: a promising solution to the $H_0$ and cosmic shear tensions Latest astronomical constraints on some nonlinear parametric dark energy models

Reference 29

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Observation 86e2b2e2-6bc3-4968-b8ea-ec6e1cddb26f · outbound

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

Reference 30

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This paper cites Partially Acoustic Dark Matter Cosmology and Cosmological Constraints.

Interacting dark energy in the early 2020s: a promising solution to the $H_0$ and cosmic shear tensions Partially Acoustic Dark Matter Cosmology and Cosmological Constraints

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This paper cites A Vacuum Phase Transition Solves $H_0$ Tension.

Interacting dark energy in the early 2020s: a promising solution to the $H_0$ and cosmic shear tensions A Vacuum Phase Transition Solves $H_0$ Tension

Reference 32

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Interacting dark energy in the early 2020s: a promising solution to the $H_0$ and cosmic shear tensions Reducing the $H_0$ and $\sigma_8$ tensions with Dark Matter-neutrino interactions

Reference 33

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Interacting dark energy in the early 2020s: a promising solution to the $H_0$ and cosmic shear tensions $H_0$ tension as a hint for a transition in gravitational theory

Reference 34

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Interacting dark energy in the early 2020s: a promising solution to the $H_0$ and cosmic shear tensions Do current cosmological observations rule out all Covariant Galileons?

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Interacting dark energy in the early 2020s: a promising solution to the $H_0$ and cosmic shear tensions The $H_0$ and $\sigma_8$ tensions and the scale invariant spectrum

Reference 36

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Interacting dark energy in the early 2020s: a promising solution to the $H_0$ and cosmic shear tensions Does the Hubble constant tension call for new physics?

Reference 37

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Interacting dark energy in the early 2020s: a promising solution to the $H_0$ and cosmic shear tensions Density perturbations for running vacuum: a successful approach to structure formation and to the $\sigma_8$-tension

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Interacting dark energy in the early 2020s: a promising solution to the $H_0$ and cosmic shear tensions Constraints on the sum of the neutrino masses in dynamical dark energy models with $w(z) \geq -1$ are tighter than those obtained in $\Lambda$CDM

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Interacting dark energy in the early 2020s: a promising solution to the $H_0$ and cosmic shear tensions Structure formation in $f(T)$ gravity and a solution for $H_0$ tension

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Interacting dark energy in the early 2020s: a promising solution to the $H_0$ and cosmic shear tensions The implications of an extended dark energy cosmology with massive neutrinos for cosmological tensions

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Interacting dark energy in the early 2020s: a promising solution to the $H_0$ and cosmic shear tensions Cosmological bounds on dark matter-photon coupling

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Interacting dark energy in the early 2020s: a promising solution to the $H_0$ and cosmic shear tensions Ups and Downs in Dark Energy: phase transition in dark sector as a proposal to lessen cosmological tensions

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

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Interacting dark energy in the early 2020s: a promising solution to the $H_0$ and cosmic shear tensions Can the $H_0$ tension be resolved in extensions to $\Lambda$CDM cosmology?

Reference 45

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Interacting dark energy in the early 2020s: a promising solution to the $H_0$ and cosmic shear tensions Primordial gravitational waves and the H0-tension problem

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Interacting dark energy in the early 2020s: a promising solution to the $H_0$ and cosmic shear tensions Observational constraints on one-parameter dynamical dark-energy parametrizations and the $H_0$ tension

Reference 47

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This paper cites Ginzburg-Landau Theory of Dark Energy: A Framework to Study Both Temporal and Spatial Cosmological Tensions Simultaneously.

Interacting dark energy in the early 2020s: a promising solution to the $H_0$ and cosmic shear tensions Ginzburg-Landau Theory of Dark Energy: A Framework to Study Both Temporal and Spatial Cosmological Tensions Simultaneously

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Interacting dark energy in the early 2020s: a promising solution to the $H_0$ and cosmic shear tensions Sounds Discordant: Classical Distance Ladder & $\Lambda$CDM -based Determinations of the Cosmological Sound Horizon

Reference 49

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Interacting dark energy in the early 2020s: a promising solution to the $H_0$ and cosmic shear tensions Early Dark Energy Can Resolve The Hubble Tension

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Interacting dark energy in the early 2020s: a promising solution to the $H_0$ and cosmic shear tensions The Neutrino Puzzle: Anomalies, Interactions, and Cosmological Tensions

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Interacting dark energy in the early 2020s: a promising solution to the $H_0$ and cosmic shear tensions Alleviating the $H_0$ and $\sigma_8$ anomalies with a decaying dark matter model

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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

Resolution: unresolved; no resolver link, observed 2026-08-08T17:56:52.300787Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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

Resolution: unresolved; no resolver link, observed 2026-08-07T18:51:43.640491Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 1ac2602b-b2bd-4fd8-bd78-462202917bfe · inbound

Evidence for non-cold dark matter from DESI DR2 measurements cites this paper.

Evidence for non-cold dark matter from DESI DR2 measurements Interacting dark energy in the early 2020s: a promising solution to the $H_0$ and cosmic shear tensions

Reference 67

Resolution: unresolved; no resolver link, observed 2026-08-16T11:53:55.949431Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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

Resolution: verified exact; arxiv_id, observed 2026-05-19T13:12:18.567787Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

Observation e2ff1651-ac28-4b42-a059-54a5669f0368 · inbound

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

Resolution: unresolved; no resolver link, observed 2026-08-06T18:14:14.345917Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation e55833c5-6aa5-474b-b9de-c8428cad290c · inbound

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

Resolution: unresolved; no resolver link, observed 2026-08-06T05:28:59.809102Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation d0027b22-1158-407b-b1d5-1842bb2499e0 · inbound

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

Resolution: unresolved; no resolver link, observed 2026-08-06T00:10:05.153634Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation cca54afd-beec-4bf5-9b3d-5cd43335c31a · inbound

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

Resolution: unresolved; no resolver link, observed 2026-08-05T16:03:01.275034Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation e9b69504-ea39-4599-9840-d3142db4dea5 · 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 Interacting dark energy in the early 2020s: a promising solution to the $H_0$ and cosmic shear tensions

Reference 214

Resolution: unresolved; no resolver link, observed 2026-08-04T12:53:51.227565Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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

Resolution: unresolved; no resolver link, observed 2026-08-04T09:59:19.051577Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation ee5cc9ad-d0ff-4ce7-8027-89144ab958b8 · 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 Interacting dark energy in the early 2020s: a promising solution to the $H_0$ and cosmic shear tensions

Reference 83

Resolution: verified exact; arxiv_id, observed 2026-05-18T04:50:54.940749Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

Observation fab2cb71-e289-420c-9107-c6ae7fd092e8 · inbound

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

Resolution: unresolved; no resolver link, observed 2026-08-03T16:54:10.842596Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 030ee0d8-dfae-460c-aa8a-59f08168fdfe · inbound

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

Resolution: unresolved; no resolver link, observed 2026-08-03T11:41:15.284516Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 3bcafde7-cfb9-42af-9523-ae33135867e7 · inbound

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

Resolution: unresolved; no resolver link, observed 2026-08-03T11:11:48.834554Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 75dafa4d-154e-4593-9d28-a4455c76b3dc · 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 Interacting dark energy in the early 2020s: a promising solution to the $H_0$ and cosmic shear tensions

Reference 104

Resolution: verified exact; arxiv_id, observed 2026-05-16T12:17:52.401932Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

Observation a54fad92-12d1-43f4-8956-374bbe56bf24 · 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 Interacting dark energy in the early 2020s: a promising solution to the $H_0$ and cosmic shear tensions

Reference 55

Resolution: verified exact; arxiv_id, observed 2026-05-21T13:30:11.876223Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

Observation 6ea865e9-4cbb-4deb-b0bb-715ad96c303e · inbound

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

Reference 36

Resolution: unresolved; no resolver link, observed 2026-07-14T23:28:39.478335Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 301c1257-4713-4930-ae64-61987e2858b6 · 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 Interacting dark energy in the early 2020s: a promising solution to the $H_0$ and cosmic shear tensions

Reference 65

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 e5de9e9d-6d77-4bb9-bc0e-55e4c77cb8c4 · 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 Interacting dark energy in the early 2020s: a promising solution to the $H_0$ and cosmic shear tensions

Reference 35

Resolution: verified exact; arxiv_id, observed 2026-05-10T13:00:24.858697Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

Observation d8e37c89-7159-4c18-afb8-2d3265d5d2c2 · inbound

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

Reference 19

Resolution: verified exact; arxiv_id, observed 2026-07-04T22:30:10.434480Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

Observation 8b7fc899-40c5-464d-b833-b9559822fc90 · inbound

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

Reference 20

Resolution: verified exact; arxiv_id, observed 2026-05-11T18:46:06.883918Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

Observation eb4e8918-cb10-4259-b823-e8b42d47feac · inbound

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

Resolution: unresolved; no resolver link, observed 2026-07-12T18:37:05.978670Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 00904879-c40b-4100-9a06-4f268a8b8b56 · 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 Interacting dark energy in the early 2020s: a promising solution to the $H_0$ and cosmic shear tensions

Reference 23

Resolution: verified exact; arxiv_id, observed 2026-05-12T00:36:15.854483Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

Observation 95319c91-fa72-444e-819d-c553e21e322b · inbound

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

Resolution: verified exact; arxiv_id, observed 2026-05-11T16:31:06.629402Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

Observation 0156fa7b-7dec-46ee-b32d-23f655c504e8 · inbound

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

Reference 33

Resolution: verified exact; arxiv_id, observed 2026-05-11T01:45:50.860886Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

Observation 2a5d8255-a851-42ea-83d0-ecc82e864cfb · inbound

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

Reference 164

Resolution: verified exact; arxiv_id, observed 2026-07-01T16:45:51.298500Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

Observation 0b3a3127-500f-45e6-a19a-a300e519b9b5 · inbound

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

Resolution: verified exact; arxiv_id, observed 2026-07-02T10:56:52.632285Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

Observation 0a8c4403-54bb-4c02-8e6c-98be428c4e48 · inbound

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

Resolution: verified exact; arxiv_id, observed 2026-07-02T14:27:03.521594Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

Observation 69edd935-5195-4139-b763-0e4cf60e4eae · 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 Interacting dark energy in the early 2020s: a promising solution to the $H_0$ and cosmic shear tensions

Reference 22

Resolution: verified exact; arxiv_id, observed 2026-07-02T15:37:06.157661Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

Observation 5eace0d2-fdec-439f-9d1d-c6fab85978ed · 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 Interacting dark energy in the early 2020s: a promising solution to the $H_0$ and cosmic shear tensions

Reference 65

Resolution: verified exact; arxiv_id, observed 2026-07-03T07:47:45.326045Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

Observation 62951415-0c40-4dd8-a61f-17def0eebfcd · inbound

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

Resolution: verified exact; arxiv_id, observed 2026-07-01T11:15:42.274037Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

Observation bd9fc380-14f6-457d-aa43-4a4570d546f5 · 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 Interacting dark energy in the early 2020s: a promising solution to the $H_0$ and cosmic shear tensions

Reference 177

Resolution: verified exact; arxiv_id, observed 2026-07-01T11:25:45.565858Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

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.

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.

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.

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.