Paper Citation Record · LEDGER

What solves the Hubble tension in phenomenological dark energy models at background level?

As of 22 August 2026, this Paper Citation Record lists 80 of 80 outbound references and 2 inbound Pith citation observations for arXiv:2505.24743.

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

pith.paper-citation-record.v1
2505.24743 v2

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Outbound references

Observation aad686e4-7993-457f-91be-981ec59e1197 · outbound

This paper cites an unresolved cited work.

What solves the Hubble tension in phenomenological dark energy models at background level? Unresolved cited work

Reference 1

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This paper cites In our case, once specific values are chosen for the additional free parameters, all models effectively possess the same free parameters as ΛCDM.

What solves the Hubble tension in phenomenological dark energy models at background level? In our case, once specific values are chosen for the additional free parameters, all models effectively possess the same free parameters as ΛCDM

Reference 2

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This paper cites Ly 𝛼-QSO+.

What solves the Hubble tension in phenomenological dark energy models at background level? Ly 𝛼-QSO+

Reference 3

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This paper cites Status Report on the Chicago-Carnegie Hubble Program (CCHP): Measurement of the Hubble Constant Using the Hubble and James Webb Space Telescopes.

What solves the Hubble tension in phenomenological dark energy models at background level? Status Report on the Chicago-Carnegie Hubble Program (CCHP): Measurement of the Hubble Constant Using the Hubble and James Webb Space Telescopes

Reference 4

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This paper cites Instead, we use 𝜎𝑢 ifA𝑒 is less than the reference value and𝜎𝑙 otherwise.

What solves the Hubble tension in phenomenological dark energy models at background level? Instead, we use 𝜎𝑢 ifA𝑒 is less than the reference value and𝜎𝑙 otherwise

Reference 5

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This paper cites Python modules used.

What solves the Hubble tension in phenomenological dark energy models at background level? Python modules used

Reference 6

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This paper cites The CosmoVerse White Paper: Addressing observational tensions in cosmology with systematics and fundamental physics.

What solves the Hubble tension in phenomenological dark energy models at background level? The CosmoVerse White Paper: Addressing observational tensions in cosmology with systematics and fundamental physics

Reference 7

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What solves the Hubble tension in phenomenological dark energy models at background level? Unresolved cited work

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This paper cites Aghanim et al., A&A 641, A6 (2020).

What solves the Hubble tension in phenomenological dark energy models at background level? Aghanim et al., A&A 641, A6 (2020)

Reference 9

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This paper cites von Marttens, L.

What solves the Hubble tension in phenomenological dark energy models at background level? von Marttens, L

Reference 10

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This paper cites Li et al., The Astrophysical Journal 976, 177 (2024).

What solves the Hubble tension in phenomenological dark energy models at background level? Li et al., The Astrophysical Journal 976, 177 (2024)

Reference 11

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This paper cites DESI DR2 Results II: Measurements of Baryon Acoustic Oscillations and Cosmological Constraints.

What solves the Hubble tension in phenomenological dark energy models at background level? DESI DR2 Results II: Measurements of Baryon Acoustic Oscillations and Cosmological Constraints

Reference 12

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This paper cites Challenging $\Lambda$CDM: 5$\sigma$ Evidence for a Dynamical Dark Energy Late-Time Transition.

What solves the Hubble tension in phenomenological dark energy models at background level? Challenging $\Lambda$CDM: 5$\sigma$ Evidence for a Dynamical Dark Energy Late-Time Transition

Reference 13

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What solves the Hubble tension in phenomenological dark energy models at background level? Li and A

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This paper cites Granda and A.

What solves the Hubble tension in phenomenological dark energy models at background level? Granda and A

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What solves the Hubble tension in phenomenological dark energy models at background level? Li and A

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This paper cites Weinberg, Rev.

What solves the Hubble tension in phenomenological dark energy models at background level? Weinberg, Rev

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What solves the Hubble tension in phenomenological dark energy models at background level? Unresolved cited work

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What solves the Hubble tension in phenomenological dark energy models at background level? Unresolved cited work

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This paper cites DESI DR2 Results I: Baryon Acoustic Oscillations from the Lyman Alpha Forest.

What solves the Hubble tension in phenomenological dark energy models at background level? DESI DR2 Results I: Baryon Acoustic Oscillations from the Lyman Alpha Forest

Reference 20

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This paper cites Vagnozzi, Phys.

What solves the Hubble tension in phenomenological dark energy models at background level? Vagnozzi, Phys

Reference 21

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This paper cites Tamayo, E.

What solves the Hubble tension in phenomenological dark energy models at background level? Tamayo, E

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What solves the Hubble tension in phenomenological dark energy models at background level? Unresolved cited work

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This paper cites Observational evidence for parametrized emergent dark energy models.

What solves the Hubble tension in phenomenological dark energy models at background level? Observational evidence for parametrized emergent dark energy models

Reference 24

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What solves the Hubble tension in phenomenological dark energy models at background level? Unresolved cited work

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What solves the Hubble tension in phenomenological dark energy models at background level? Unresolved cited work

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What solves the Hubble tension in phenomenological dark energy models at background level? Jimenez and A

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This paper cites Interacting Dark Sectors in light of DESI DR2.

What solves the Hubble tension in phenomenological dark energy models at background level? Interacting Dark Sectors in light of DESI DR2

Reference 29

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What solves the Hubble tension in phenomenological dark energy models at background level? Unresolved cited work

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What solves the Hubble tension in phenomenological dark energy models at background level? Unresolved cited work

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What solves the Hubble tension in phenomenological dark energy models at background level? Di Valentino, A

Reference 32

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This paper cites New constraints on interacting dark energy from DESI DR2 BAO observations.

What solves the Hubble tension in phenomenological dark energy models at background level? New constraints on interacting dark energy from DESI DR2 BAO observations

Reference 33

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What solves the Hubble tension in phenomenological dark energy models at background level? Unresolved cited work

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This paper cites Stern, R.

What solves the Hubble tension in phenomenological dark energy models at background level? Stern, R

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What solves the Hubble tension in phenomenological dark energy models at background level? Moresco et al

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What solves the Hubble tension in phenomenological dark energy models at background level? Unresolved cited work

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What solves the Hubble tension in phenomenological dark energy models at background level? Moresco et al

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This paper cites Moresco, Monthly Notices of the Royal Astronomical Soci- ety: Letters 450, L16 (2015).

What solves the Hubble tension in phenomenological dark energy models at background level? Moresco, Monthly Notices of the Royal Astronomical Soci- ety: Letters 450, L16 (2015)

Reference 39

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What solves the Hubble tension in phenomenological dark energy models at background level? Chuang and Y

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This paper cites Alam et al.

What solves the Hubble tension in phenomenological dark energy models at background level? Alam et al

Reference 41

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This paper cites Anderson et al., Monthly Notices of the Royal Astronomical Society 441, 24 (2014).

What solves the Hubble tension in phenomenological dark energy models at background level? Anderson et al., Monthly Notices of the Royal Astronomical Society 441, 24 (2014)

Reference 42

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This paper cites Blake et al.

What solves the Hubble tension in phenomenological dark energy models at background level? Blake et al

Reference 43

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What solves the Hubble tension in phenomenological dark energy models at background level? Wang et al

Reference 44

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What solves the Hubble tension in phenomenological dark energy models at background level? Unresolved cited work

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What solves the Hubble tension in phenomenological dark energy models at background level? Alam et al., Phys

Reference 46

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This paper cites Gaztanaga, A.

What solves the Hubble tension in phenomenological dark energy models at background level? Gaztanaga, A

Reference 47

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What solves the Hubble tension in phenomenological dark energy models at background level? Unresolved cited work

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This paper cites Font-Ribera et al., Journal of Cosmology and Astroparticle Physics 2014, 027 (2014).

What solves the Hubble tension in phenomenological dark energy models at background level? Font-Ribera et al., Journal of Cosmology and Astroparticle Physics 2014, 027 (2014)

Reference 49

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What solves the Hubble tension in phenomenological dark energy models at background level? Unresolved cited work

Reference 50

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This paper cites et al., A&A 603, A12 (2017).

What solves the Hubble tension in phenomenological dark energy models at background level? et al., A&A 603, A12 (2017)

Reference 51

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This paper cites For similar reasons, we do not consider the DES compilation either [54].

What solves the Hubble tension in phenomenological dark energy models at background level? For similar reasons, we do not consider the DES compilation either [54]

Reference 52

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This paper cites du Mas des Bourboux et al., The Astrophysical Journal 901, 153 (2020).

What solves the Hubble tension in phenomenological dark energy models at background level? du Mas des Bourboux et al., The Astrophysical Journal 901, 153 (2020)

Reference 53

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This paper cites Adame et al.

What solves the Hubble tension in phenomenological dark energy models at background level? Adame et al

Reference 54

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T12:22:25.698031Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

Observation 358f6a88-fad2-4512-b32a-542be7115b29 · outbound

This paper cites Dynamical dark energy with AdS-dS transitions vs. Baryon Acoustic Oscillations at $z =$ 2.3-2.4.

What solves the Hubble tension in phenomenological dark energy models at background level? Dynamical dark energy with AdS-dS transitions vs. Baryon Acoustic Oscillations at $z =$ 2.3-2.4

Reference 55

Resolution: unresolved; no resolver link, observed 2026-08-07T12:22:19.023796Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 2dd1297a-4e1f-4db2-ba22-64ca9570cfd5 · outbound

This paper cites an unresolved cited work.

What solves the Hubble tension in phenomenological dark energy models at background level? Unresolved cited work

Reference 56

Resolution: unresolved; raw_fallback, observed 2026-08-07T12:22:25.520158Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

Observation c34b6522-9ef4-4d38-9300-714e884242a3 · outbound

This paper cites Perlmutter et al.

What solves the Hubble tension in phenomenological dark energy models at background level? Perlmutter et al

Reference 57

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T12:22:25.361574Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

Observation 5692660b-361e-4d36-a042-1828f6f97218 · outbound

This paper cites Suzuki et al., The Astrophysical Journal 746, 85 (2012).

What solves the Hubble tension in phenomenological dark energy models at background level? Suzuki et al., The Astrophysical Journal 746, 85 (2012)

Reference 58

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T12:22:25.207026Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

Observation 843bca54-a140-48fa-bfb5-8fd1e809a6d3 · outbound

This paper cites Union Through UNITY: Cosmology with 2,000 SNe Using a Unified Bayesian Framework.

What solves the Hubble tension in phenomenological dark energy models at background level? Union Through UNITY: Cosmology with 2,000 SNe Using a Unified Bayesian Framework

Reference 59

Resolution: unresolved; no resolver link, observed 2026-08-07T12:22:19.374684Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation c8344ed3-585e-416f-8a89-5d4221c45652 · outbound

This paper cites Collaboration et al., The Astrophysical Journal Letters 973, L14 (2024).

What solves the Hubble tension in phenomenological dark energy models at background level? Collaboration et al., The Astrophysical Journal Letters 973, L14 (2024)

Reference 60

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T12:22:25.013453Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

Observation 142b89fa-99c1-44ee-8457-4f1444d53028 · outbound

This paper cites an unresolved cited work.

What solves the Hubble tension in phenomenological dark energy models at background level? Unresolved cited work

Reference 61

Resolution: unresolved; raw_fallback, observed 2026-08-07T12:22:24.850115Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

Observation dc2f4d65-8e88-42c1-8c78-44676c6d23f9 · outbound

This paper cites Code for anisotropies in the mi- crowave background (camb),.

What solves the Hubble tension in phenomenological dark energy models at background level? Code for anisotropies in the mi- crowave background (camb),

Reference 62

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T12:22:24.704044Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

Observation 9340bb32-f4ff-43a0-8d6e-b5717ae91b19 · outbound

This paper cites Chen, Q.-G.

What solves the Hubble tension in phenomenological dark energy models at background level? Chen, Q.-G

Reference 63

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T12:22:24.562277Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

Observation 5099504a-02f5-41a3-9f89-56d4c0544ab9 · outbound

This paper cites Akaike, IEEE Transactions on Automatic Control 19, 716 (1974).

What solves the Hubble tension in phenomenological dark energy models at background level? Akaike, IEEE Transactions on Automatic Control 19, 716 (1974)

Reference 64

Resolution: unresolved; no resolver link, observed 2026-08-07T12:22:19.891892Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 69f276cf-2bb7-4081-a39c-31da96eb31b3 · outbound

This paper cites Schwarz, The Annals of Statistics 6, 461 (1978).

What solves the Hubble tension in phenomenological dark energy models at background level? Schwarz, The Annals of Statistics 6, 461 (1978)

Reference 65

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T12:22:24.371925Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

Observation f3122fbb-1ade-4f7e-ba19-7c8744fe90ad · outbound

This paper cites an unresolved cited work.

What solves the Hubble tension in phenomenological dark energy models at background level? Unresolved cited work

Reference 66

Resolution: unresolved; raw_fallback, observed 2026-08-07T12:22:24.206622Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

Observation 0f047df5-73af-4d99-8ac9-d0ede5ac0644 · outbound

This paper cites Sahni, A.

What solves the Hubble tension in phenomenological dark energy models at background level? Sahni, A

Reference 67

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T12:22:24.059774Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

Observation 7cb81790-8a16-4352-9c74-ebb56d38c3c1 · outbound

This paper cites an unresolved cited work.

What solves the Hubble tension in phenomenological dark energy models at background level? Unresolved cited work

Reference 68

Resolution: unresolved; raw_fallback, observed 2026-08-07T12:22:23.924431Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

Observation e3eb00e5-dc94-4466-974f-2f028c7293ec · outbound

This paper cites an unresolved cited work.

What solves the Hubble tension in phenomenological dark energy models at background level? Unresolved cited work

Reference 69

Resolution: unresolved; raw_fallback, observed 2026-08-07T12:22:23.740518Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

Observation 97b7e046-1695-4fc7-bd55-97388d9f05fe · outbound

This paper cites How predictions of cosmological models depend on Hubble parameter data sets.

What solves the Hubble tension in phenomenological dark energy models at background level? How predictions of cosmological models depend on Hubble parameter data sets

Reference 70

Resolution: unresolved; no resolver link, observed 2026-08-07T12:22:20.516212Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 258d3013-9740-4d86-ac0d-b19d39452016 · outbound

This paper cites an unresolved cited work.

What solves the Hubble tension in phenomenological dark energy models at background level? Unresolved cited work

Reference 71

Resolution: unresolved; no resolver link, observed 2026-08-07T12:22:20.634030Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 70e549cc-49f3-441a-a130-12d265941cd3 · outbound

This paper cites pandas-dev/pandas: Pandas,.

What solves the Hubble tension in phenomenological dark energy models at background level? pandas-dev/pandas: Pandas,

Reference 72

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T12:22:23.556842Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

Observation 207581f1-6ad4-4687-8cc9-955c6077e8c9 · outbound

This paper cites Virtanen et al., Nature Methods 17, 261 (2020).

What solves the Hubble tension in phenomenological dark energy models at background level? Virtanen et al., Nature Methods 17, 261 (2020)

Reference 73

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T12:22:23.366645Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

Observation c29ce3fd-215e-43fa-b800-8c40653e1d03 · outbound

This paper cites Foreman-Mackey, D.

What solves the Hubble tension in phenomenological dark energy models at background level? Foreman-Mackey, D

Reference 74

Resolution: unresolved; no resolver link, observed 2026-08-07T12:22:21.024444Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 39257727-e522-47f6-a335-456b5e81d010 · outbound

This paper cites lmfit/lmfit-py: 1.2.2,.

What solves the Hubble tension in phenomenological dark energy models at background level? lmfit/lmfit-py: 1.2.2,

Reference 75

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T12:22:23.141981Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

Observation 7b4f80b3-d8f7-4c58-b4e1-38ef1723f415 · outbound

This paper cites Abril-Pla et al., PeerJ Computer Science 9, e1516 (2023).

What solves the Hubble tension in phenomenological dark energy models at background level? Abril-Pla et al., PeerJ Computer Science 9, e1516 (2023)

Reference 76

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T12:22:22.956864Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

Observation 3ab34140-77ae-48d7-a98a-9a1c58eb276f · outbound

This paper cites an unresolved cited work.

What solves the Hubble tension in phenomenological dark energy models at background level? Unresolved cited work

Reference 77

Resolution: unresolved; no resolver link, observed 2026-08-07T12:22:21.393535Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 28987390-a6fa-4189-a452-c202b3bd179c · outbound

This paper cites Foreman-Mackey, The Journal of Open Source Software 1, 24 (2016).

What solves the Hubble tension in phenomenological dark energy models at background level? Foreman-Mackey, The Journal of Open Source Software 1, 24 (2016)

Reference 78

Resolution: unresolved; no resolver link, observed 2026-08-07T12:22:21.557120Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation b02f8820-2edb-45f2-8f60-b14de36a679f · outbound

This paper cites an unresolved cited work.

What solves the Hubble tension in phenomenological dark energy models at background level? Unresolved cited work

Reference 79

Resolution: unresolved; no resolver link, observed 2026-08-07T12:22:21.685178Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 4fac0795-f344-4b0b-9398-57df02cf551a · outbound

This paper cites an unresolved cited work.

What solves the Hubble tension in phenomenological dark energy models at background level? Unresolved cited work

Reference 80

Resolution: unresolved; no resolver link, observed 2026-08-07T12:22:21.787388Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Pith citing papers

Observation b669e32d-b12e-4593-8888-e4ca33e3b78f · inbound

Challenging $\Lambda$CDM: 5$\sigma$ Evidence for a Dynamical Dark Energy Late-Time Transition cites this paper.

Challenging $\Lambda$CDM: 5$\sigma$ Evidence for a Dynamical Dark Energy Late-Time Transition What solves the Hubble tension in phenomenological dark energy models at background level?

Reference 61

Resolution: unresolved; no resolver link, observed 2026-08-16T05:27:54.288803Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 1efe3b65-95a2-4cc8-9579-1a394e1498a8 · inbound

QCD CP-violation scenario for a revised cosmological dynamics: analysis of the binned Pantheon Sample of Super Novae Ia cites this paper.

QCD CP-violation scenario for a revised cosmological dynamics: analysis of the binned Pantheon Sample of Super Novae Ia What solves the Hubble tension in phenomenological dark energy models at background level?

Reference 18

Resolution: unresolved; no resolver link, observed 2026-08-01T11:25:06.226043Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.