Paper Citation Record · LEDGER

Early dark energy is not excluded by current large-scale structure data

As of 20 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 25 inbound Pith citation observations for arXiv:2009.10740.

A citation records a reference. It does not transfer a finding from one paper to another.

pith.paper-citation-record.v1
2009.10740 v1

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measured 25 of 25 inbound itemization

Pith citing papers itemized under the disclosed page cap.

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Pith citing papers

Observation 6df0290a-67c6-4b3a-905e-86f7e4721946 · inbound

In the Realm of the Hubble tension $-$ a Review of Solutions cites this paper.

In the Realm of the Hubble tension $-$ a Review of Solutions Early dark energy is not excluded by current large-scale structure data

Reference 103

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The Hubble Tension and Early Dark Energy cites this paper.

The Hubble Tension and Early Dark Energy Early dark energy is not excluded by current large-scale structure data

Reference 144

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Illustrating the consequences of a misuse of $\sigma_8$ in cosmology cites this paper.

Illustrating the consequences of a misuse of $\sigma_8$ in cosmology Early dark energy is not excluded by current large-scale structure data

Reference 211

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$\Lambda$CDM and early dark energy in latent space: a data-driven parametrization of the CMB temperature power spectrum cites this paper.

$\Lambda$CDM and early dark energy in latent space: a data-driven parametrization of the CMB temperature power spectrum Early dark energy is not excluded by current large-scale structure data

Reference 7

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Impact of ACT DR6 and DESI DR2 for Early Dark Energy and the Hubble tension cites this paper.

Impact of ACT DR6 and DESI DR2 for Early Dark Energy and the Hubble tension Early dark energy is not excluded by current large-scale structure data

Reference 86

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Observation f999dd99-1b68-48ef-8aed-dbc005448082 · inbound

Bayesian and frequentist perspectives agree on dynamical dark energy cites this paper.

Bayesian and frequentist perspectives agree on dynamical dark energy Early dark energy is not excluded by current large-scale structure data

Reference 16

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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 Early dark energy is not excluded by current large-scale structure data

Reference 130

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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 Early dark energy is not excluded by current large-scale structure data

Reference 35

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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 Early dark energy is not excluded by current large-scale structure data

Reference 49

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Model-independent late-universe measurements of $H_0$ and $\Omega_K$ with the parametrization based on cosmic age-improved inverse distance ladder cites this paper.

Model-independent late-universe measurements of $H_0$ and $\Omega_K$ with the parametrization based on cosmic age-improved inverse distance ladder Early dark energy is not excluded by current large-scale structure data

Reference 23

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Disentangling cosmic distance tensions with early and late dark energy cites this paper.

Disentangling cosmic distance tensions with early and late dark energy Early dark energy is not excluded by current large-scale structure data

Reference 110

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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 Early dark energy is not excluded by current large-scale structure data

Reference 170

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Observation b7c28fab-6419-437a-978f-ac3643ac8a1c · inbound

A barotropic alternative to Early Dark Energy for alleviating the $H_0$ tension cites this paper.

A barotropic alternative to Early Dark Energy for alleviating the $H_0$ tension Early dark energy is not excluded by current large-scale structure data

Reference 33

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Observation 5878e6f3-fe6b-43ec-a9bc-e542e64b5c4a · inbound

Multi-tracers, multi-surveys: a joint Fisher analysis of DESI+PFS cites this paper.

Multi-tracers, multi-surveys: a joint Fisher analysis of DESI+PFS Early dark energy is not excluded by current large-scale structure data

Reference 15

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Observation 4e041dbc-895e-44de-9d97-a961219da58c · inbound

Multi-tracers, multi-surveys: a joint Fisher analysis of DESI+PFS cites this paper.

Multi-tracers, multi-surveys: a joint Fisher analysis of DESI+PFS Early dark energy is not excluded by current large-scale structure data

Reference 15

Resolution: verified exact; arxiv_id, observed 2026-05-11T22:01:13.833063Z

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Observation 269ffbc7-93d7-4265-8bd9-6141dd0b25c2 · 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 Early dark energy is not excluded by current large-scale structure data

Reference 84

Resolution: verified exact; arxiv_id, observed 2026-05-12T00:36:16.613830Z

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Observation 908f5e0d-93da-4660-9737-bfc547f68d35 · inbound

Inflation driven by repulsive-like primordial black holes cites this paper.

Inflation driven by repulsive-like primordial black holes Early dark energy is not excluded by current large-scale structure data

Reference 105

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Observation 2ea90a14-fff9-4bf6-a968-4c08b0666aaa · inbound

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

Unifying Early and Late Dark Energy: Dynamical Requirements and Obstructions Early dark energy is not excluded by current large-scale structure data

Reference 56

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The Hubble tension: A decade review cites this paper.

The Hubble tension: A decade review Early dark energy is not excluded by current large-scale structure data

Reference 276

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Observation 26db4e05-681b-47b4-be38-fd5b5bec090c · inbound

The Hubble tension: A decade review cites this paper.

The Hubble tension: A decade review Early dark energy is not excluded by current large-scale structure data

Reference 276

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Observation f952d0db-1f9b-4cb5-a14e-763df9e69ae3 · 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 Early dark energy is not excluded by current large-scale structure data

Reference 76

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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 Early dark energy is not excluded by current large-scale structure data

Reference 61

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Observation 033bc5c6-4a39-49ac-8730-1f6dd451790b · 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 Early dark energy is not excluded by current large-scale structure data

Reference 87

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Observation 378b4895-7b95-4911-bb3b-a261339f9bc9 · inbound

Hubble tension: the shape wall cites this paper.

Hubble tension: the shape wall Early dark energy is not excluded by current large-scale structure data

Reference 81

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Observation 10837b9b-85b3-45f0-b0d6-5f100aa8df2f · inbound

Hubble tension: a short review of theoretical explanations cites this paper.

Hubble tension: a short review of theoretical explanations Early dark energy is not excluded by current large-scale structure data

Reference 163

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