Paper Citation Record · LEDGER

Beyond LambdaCDM: How the Hubble tension challenges early universe physics

As of 13 August 2026, this Paper Citation Record lists 55 of 55 outbound references and 3 inbound Pith citation observations for arXiv:2507.08479.

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

pith.paper-citation-record.v1
2507.08479 v1

Coverage vector

measured 55 of 55 reference resolution

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Outbound references

Observation 73ac2f0b-b993-4703-8596-37cdeb8b4e99 · outbound

This paper cites Beyond LambdaCDM: How the Hubble tension challenges early universe physics.

Beyond LambdaCDM: How the Hubble tension challenges early universe physics Beyond LambdaCDM: How the Hubble tension challenges early universe physics

Reference 1

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This paper cites Interactions between photons and baryons in this fluid created perturbations in the plasma which propagated at the speed of sound.

Beyond LambdaCDM: How the Hubble tension challenges early universe physics Interactions between photons and baryons in this fluid created perturbations in the plasma which propagated at the speed of sound

Reference 2

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This paper cites The addition of the simple fluid Ω X results in essentially just Gaussian noise, as shown in Figure 6.

Beyond LambdaCDM: How the Hubble tension challenges early universe physics The addition of the simple fluid Ω X results in essentially just Gaussian noise, as shown in Figure 6

Reference 3

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This paper cites In this paper we have reviewed a number of papers that each modified the conditions in the early universe, reducing the sound horizon and raising the value of H0.

Beyond LambdaCDM: How the Hubble tension challenges early universe physics In this paper we have reviewed a number of papers that each modified the conditions in the early universe, reducing the sound horizon and raising the value of H0

Reference 4

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This paper cites The Atacama Cosmology Telescope: DR6 Constraints on Extended Cosmological Models.

Beyond LambdaCDM: How the Hubble tension challenges early universe physics The Atacama Cosmology Telescope: DR6 Constraints on Extended Cosmological Models

Reference 5

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Observation f6de4cd5-c153-4dee-9d45-b56de89ec487 · outbound

This paper cites Neutrino-Assisted Early Dark Energy is a Natural Resolution of the Hubble Tension.

Beyond LambdaCDM: How the Hubble tension challenges early universe physics Neutrino-Assisted Early Dark Energy is a Natural Resolution of the Hubble Tension

Reference 6

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This paper cites Pedro, and Marco Scalisi.

Beyond LambdaCDM: How the Hubble tension challenges early universe physics Pedro, and Marco Scalisi

Reference 7

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This paper cites Cruz, Steen Hannestad, Emil Brinch Holm, Florian Niedermann, Martin S.

Beyond LambdaCDM: How the Hubble tension challenges early universe physics Cruz, Steen Hannestad, Emil Brinch Holm, Florian Niedermann, Martin S

Reference 8

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Observation a8fe7733-968c-49ed-a8ef-49ced9da349f · outbound

This paper cites Sen, and M.

Beyond LambdaCDM: How the Hubble tension challenges early universe physics Sen, and M

Reference 9

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Observation 987daaf8-5593-4f85-8250-0b95afefaf86 · outbound

This paper cites Emergent Unparticles Dark Energy can restore cosmological concordance.

Beyond LambdaCDM: How the Hubble tension challenges early universe physics Emergent Unparticles Dark Energy can restore cosmological concordance

Reference 10

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This paper cites Early dark energy induced by non-linear electrodynamics.

Beyond LambdaCDM: How the Hubble tension challenges early universe physics Early dark energy induced by non-linear electrodynamics

Reference 11

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This paper cites Riess, et al.

Beyond LambdaCDM: How the Hubble tension challenges early universe physics Riess, et al

Reference 12

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This paper cites Feroz, M.

Beyond LambdaCDM: How the Hubble tension challenges early universe physics Feroz, M

Reference 13

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This paper cites corner.py: Scatterplot matrices in python.

Beyond LambdaCDM: How the Hubble tension challenges early universe physics corner.py: Scatterplot matrices in python

Reference 14

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This paper cites The values of θs and its uncertainty, along with a calculated DA were used in the probability of acceptance in the MCMC analysis, with constraints 0 < f < 1 and zc > 1100.

Beyond LambdaCDM: How the Hubble tension challenges early universe physics The values of θs and its uncertainty, along with a calculated DA were used in the probability of acceptance in the MCMC analysis, with constraints 0 < f < 1 and zc > 1100

Reference 15

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Observation a8e24222-735f-49cd-b38f-37a49890eb50 · outbound

This paper cites Canonical Hubble-Tension-Resolving Early Dark Energy Cosmologies are Inconsistent with the Lyman-$\alpha$ Forest.

Beyond LambdaCDM: How the Hubble tension challenges early universe physics Canonical Hubble-Tension-Resolving Early Dark Energy Cosmologies are Inconsistent with the Lyman-$\alpha$ Forest

Reference 16

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Observation 91bba2e7-c963-4a4a-a4be-f23807ae45a2 · outbound

This paper cites Can neutrino-assisted early dark energy models ameliorate the $H_0$ tension in a natural way?.

Beyond LambdaCDM: How the Hubble tension challenges early universe physics Can neutrino-assisted early dark energy models ameliorate the $H_0$ tension in a natural way?

Reference 17

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This paper cites COLOSSUS: A Python Toolkit for Cosmology, Large-scale Structure, and Dark Matter Halos.

Beyond LambdaCDM: How the Hubble tension challenges early universe physics COLOSSUS: A Python Toolkit for Cosmology, Large-scale Structure, and Dark Matter Halos

Reference 18

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This paper cites This is in tension with the value of H0 derived from SNIa observations, which is H0 = 73.30 ± 1.04 km s −1 Mpc−1 [37].

Beyond LambdaCDM: How the Hubble tension challenges early universe physics This is in tension with the value of H0 derived from SNIa observations, which is H0 = 73.30 ± 1.04 km s −1 Mpc−1 [37]

Reference 19

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Beyond LambdaCDM: How the Hubble tension challenges early universe physics The state of the dark energy equation of state circa 2023

Reference 20

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Observation 71b55359-9ec2-4f9b-854d-41379d1f4c94 · outbound

This paper cites Constraint on Early Dark Energy from Isotropic Cosmic Birefringence.

Beyond LambdaCDM: How the Hubble tension challenges early universe physics Constraint on Early Dark Energy from Isotropic Cosmic Birefringence

Reference 21

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This paper cites Toward early dark energy and n s=1 with P l a n c k , ACT, and SPT observations.

Beyond LambdaCDM: How the Hubble tension challenges early universe physics Toward early dark energy and n s=1 with P l a n c k , ACT, and SPT observations

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This paper cites Hogg, Dustin Lang, and Jonathan Goodman.

Beyond LambdaCDM: How the Hubble tension challenges early universe physics Hogg, Dustin Lang, and Jonathan Goodman

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This paper cites Hubble tension as a guide for refining the early Universe: Cosmologies with explicit local Lorentz and diffeomorphism violation.

Beyond LambdaCDM: How the Hubble tension challenges early universe physics Hubble tension as a guide for refining the early Universe: Cosmologies with explicit local Lorentz and diffeomorphism violation

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Beyond LambdaCDM: How the Hubble tension challenges early universe physics Harris, K

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Beyond LambdaCDM: How the Hubble tension challenges early universe physics Unresolved cited work

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This paper cites Hinshaw, D.

Beyond LambdaCDM: How the Hubble tension challenges early universe physics Hinshaw, D

Reference 27

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Beyond LambdaCDM: How the Hubble tension challenges early universe physics Hubble Tension: The Evidence of New Physics

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Beyond LambdaCDM: How the Hubble tension challenges early universe physics Unresolved cited work

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Beyond LambdaCDM: How the Hubble tension challenges early universe physics Colin Hill, and Wayne Hu

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Beyond LambdaCDM: How the Hubble tension challenges early universe physics They discussed triggers at a microscopic level, either an ultralight scalar field or a dark sector temperature

Reference 31

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Beyond LambdaCDM: How the Hubble tension challenges early universe physics Unresolved cited work

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Beyond LambdaCDM: How the Hubble tension challenges early universe physics joshspeagle/dynesty: v2.1.4, June 2024

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This paper cites The Hubble tension from the standpoint of quantum cosmology.

Beyond LambdaCDM: How the Hubble tension challenges early universe physics The Hubble tension from the standpoint of quantum cosmology

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Beyond LambdaCDM: How the Hubble tension challenges early universe physics What It Takes to Solve the Hubble Tension through Modifications of Cosmological Recombination

Reference 35

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Beyond LambdaCDM: How the Hubble tension challenges early universe physics Ruchika, Carvalho, and Jailson Alcaniz

Reference 36

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This paper cites Figure 1 is a simple illustration of various physical models briefly reviewed in Section 1.

Beyond LambdaCDM: How the Hubble tension challenges early universe physics Figure 1 is a simple illustration of various physical models briefly reviewed in Section 1

Reference 37

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Beyond LambdaCDM: How the Hubble tension challenges early universe physics CAMB: Code for Anisotropies in the Microwave Background

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Beyond LambdaCDM: How the Hubble tension challenges early universe physics New Early Dark Energy as a solution to the $H_0$ and $S_8$ tensions

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Beyond LambdaCDM: How the Hubble tension challenges early universe physics Odintsov, V

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This paper cites Odintsov, Diego S´ aez-Chill´ on G´ omez, and German S.

Beyond LambdaCDM: How the Hubble tension challenges early universe physics Odintsov, Diego S´ aez-Chill´ on G´ omez, and German S

Reference 41

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Beyond LambdaCDM: How the Hubble tension challenges early universe physics Planck 2018 results

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Beyond LambdaCDM: How the Hubble tension challenges early universe physics The Ups and Downs of Early Dark Energy solutions to the Hubble tension: a review of models, hints and constraints circa 2023

Reference 43

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Beyond LambdaCDM: How the Hubble tension challenges early universe physics Smith, and Tanvi Karwal

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Beyond LambdaCDM: How the Hubble tension challenges early universe physics Riess, Wenlong Yuan, Lucas M

Reference 45

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Beyond LambdaCDM: How the Hubble tension challenges early universe physics Nested Sampling

Reference 46

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Beyond LambdaCDM: How the Hubble tension challenges early universe physics Nested sampling for general Bayesian computation

Reference 47

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Beyond LambdaCDM: How the Hubble tension challenges early universe physics Unresolved cited work

Reference 48

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This paper cites Impact of big bang nucleosynthesis on the H0 tension.

Beyond LambdaCDM: How the Hubble tension challenges early universe physics Impact of big bang nucleosynthesis on the H0 tension

Reference 49

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Beyond LambdaCDM: How the Hubble tension challenges early universe physics Unresolved cited work

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This paper cites Seven Hints That Early-Time New Physics Alone Is Not Sufficient to Solve the Hubble Tension.

Beyond LambdaCDM: How the Hubble tension challenges early universe physics Seven Hints That Early-Time New Physics Alone Is Not Sufficient to Solve the Hubble Tension

Reference 51

Resolution: verified fuzzy; raw_fallback, observed 2026-08-06T18:27:02.541014Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

Observation 2e96f37b-1b3f-4ed5-af95-b2a369dd7cf1 · outbound

This paper cites Oliphant, et al.

Beyond LambdaCDM: How the Hubble tension challenges early universe physics Oliphant, et al

Reference 52

Resolution: verified fuzzy; raw_fallback, observed 2026-08-06T18:27:02.388885Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

Observation 1d1649c0-0666-4deb-986a-d84ff2ede0d7 · outbound

This paper cites Does the fraction of dark matter diminish with early dark energy?.

Beyond LambdaCDM: How the Hubble tension challenges early universe physics Does the fraction of dark matter diminish with early dark energy?

Reference 53

Resolution: unresolved; no resolver link, observed 2026-08-06T18:27:00.674274Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation cd955db5-103f-4387-a36b-3beb01713c1b · outbound

This paper cites Testing dark energy after pre-recombination early dark energy.

Beyond LambdaCDM: How the Hubble tension challenges early universe physics Testing dark energy after pre-recombination early dark energy

Reference 54

Resolution: verified fuzzy; raw_fallback, observed 2026-08-06T18:27:02.193288Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

Observation e2a14ad6-a62e-4b9c-9f84-f638e6adbe4c · outbound

This paper cites Shape of CMB lensing in the early dark energy cosmology.

Beyond LambdaCDM: How the Hubble tension challenges early universe physics Shape of CMB lensing in the early dark energy cosmology

Reference 55

Resolution: verified exact; local_arxiv, observed 2026-08-06T18:27:01.049828Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

Pith citing papers

Observation 73ac2f0b-b993-4703-8596-37cdeb8b4e99 · inbound