Seven hints that early-time new physics alone is not sufficient to solve the Hubble tension | Paper Citation Record

Observation 70451903-597f-47d1-80e6-da61e1f106d2 · inbound

Upper limits on dark energy-dark matter interaction from DESI DR2 in a field-theoretic analysis cites this paper.

Upper limits on dark energy-dark matter interaction from DESI DR2 in a field-theoretic analysis Seven hints that early-time new physics alone is not sufficient to solve the Hubble tension

Reference 32

Resolution: unresolved; no resolver link, observed 2026-08-12T18:58:29.406841Z

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Observation 7b7ba839-a30d-464e-b81e-b0ea12a5b48f · inbound

Bridge the Cosmological Tensions with Thawing Gravity cites this paper.

Bridge the Cosmological Tensions with Thawing Gravity Seven hints that early-time new physics alone is not sufficient to solve the Hubble tension

Reference 48

Resolution: unresolved; no resolver link, observed 2026-08-12T18:17:21.613521Z

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Observation 15975d8c-a58a-43e8-8b02-8483d92ce639 · inbound

Late Time Phenomena in $f(T,\mathcal{T})$ Gravity Framework: Role of $H_0$ Priors cites this paper.

Late Time Phenomena in $f(T,\mathcal{T})$ Gravity Framework: Role of $H_0$ Priors Seven hints that early-time new physics alone is not sufficient to solve the Hubble tension

Reference 61

Resolution: unresolved; no resolver link, observed 2026-08-12T18:51:10.384857Z

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Observation 8f7bc130-4e31-41d2-bf73-63b5260b776a · inbound

Exploring cosmological imprints of phantom crossing with dynamical dark energy in Horndeski gravity cites this paper.

Exploring cosmological imprints of phantom crossing with dynamical dark energy in Horndeski gravity Seven hints that early-time new physics alone is not sufficient to solve the Hubble tension

Reference 13

Resolution: unresolved; no resolver link, observed 2026-08-12T04:57:06.674747Z

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Observation a8dd0e55-9d34-4d54-85d4-091019418243 · inbound

Modified gravity/Dynamical Dark Energy vs $\Lambda$CDM: is the game over? cites this paper.

Modified gravity/Dynamical Dark Energy vs $\Lambda$CDM: is the game over? Seven hints that early-time new physics alone is not sufficient to solve the Hubble tension

Reference 15

Resolution: unresolved; no resolver link, observed 2026-08-11T17:09:38.153119Z

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Observation d77141c4-02c6-43e4-8a4d-955a9596315b · inbound

DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics? cites this paper.

DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics? Seven hints that early-time new physics alone is not sufficient to solve the Hubble tension

Reference 54

Resolution: unresolved; no resolver link, observed 2026-08-11T13:41:23.762185Z

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Observation f18c6c6a-b3e9-4768-82c3-6fa1ff56e9e3 · inbound

Impact of DESI BAO Data on Inflationary Parameters: stability against late-time new physics cites this paper.

Impact of DESI BAO Data on Inflationary Parameters: stability against late-time new physics Seven hints that early-time new physics alone is not sufficient to solve the Hubble tension

Reference 31

Resolution: unresolved; no resolver link, observed 2026-08-11T12:25:17.417795Z

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Observation be3e30e7-8482-4f7c-bca6-32db28ccca99 · inbound

Effect of Peak Absolute Magnitude of Type Ia Supernovae and Sound Horizon Values on Hubble Tension using DESI results cites this paper.

Effect of Peak Absolute Magnitude of Type Ia Supernovae and Sound Horizon Values on Hubble Tension using DESI results Seven hints that early-time new physics alone is not sufficient to solve the Hubble tension

Reference 27

Resolution: unresolved; no resolver link, observed 2026-08-11T00:53:46.916904Z

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Observation 3183f2e5-5946-4899-8a8c-2e17677ff305 · inbound

Prospects for measuring neutrino mass with 21-cm forest cites this paper.

Prospects for measuring neutrino mass with 21-cm forest Seven hints that early-time new physics alone is not sufficient to solve the Hubble tension

Reference 121

Resolution: unresolved; no resolver link, observed 2026-08-10T22:48:22.270075Z

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Observation 55aa8b41-6b34-4e7e-a088-a17ba9b07965 · inbound

Testing $\gamma\delta$CDM Model in the Redshift Bins cites this paper.

Testing $\gamma\delta$CDM Model in the Redshift Bins Seven hints that early-time new physics alone is not sufficient to solve the Hubble tension

Reference 49

Resolution: unresolved; no resolver link, observed 2026-08-10T20:48:20.368935Z

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Observation 9c22f156-4134-4fb8-82cf-c9c6a30a1557 · inbound

Void spin distribution as a powerful probe of $\sigma_{8}$ cites this paper.

Void spin distribution as a powerful probe of $\sigma_{8}$ Seven hints that early-time new physics alone is not sufficient to solve the Hubble tension

Reference 33

Resolution: unresolved; no resolver link, observed 2026-08-10T20:04:03.487497Z

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Observation 3f8d7ac9-88fc-49c1-93a1-1344eb0e3b3d · inbound

Sign Switching in Dark Sector Coupling Interactions as a Candidate for Resolving Cosmological Tensions cites this paper.

Sign Switching in Dark Sector Coupling Interactions as a Candidate for Resolving Cosmological Tensions Seven hints that early-time new physics alone is not sufficient to solve the Hubble tension

Reference 75

Resolution: unresolved; no resolver link, observed 2026-08-10T19:20:16.776496Z

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Observation 1faea2c7-e550-42f2-a3e2-e838a0b62f9c · inbound

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 Seven hints that early-time new physics alone is not sufficient to solve the Hubble tension

Reference 26

Resolution: unresolved; no resolver link, observed 2026-08-10T18:12:33.706829Z

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Observation 16454a25-dfdc-4324-90a8-ba7c4c06ba23 · inbound

Can the sound horizon-free measurement of $H_0$ constrain early new physics? cites this paper.

Can the sound horizon-free measurement of $H_0$ constrain early new physics? Seven hints that early-time new physics alone is not sufficient to solve the Hubble tension

Reference 101

Resolution: unresolved; no resolver link, observed 2026-08-10T05:59:55.804495Z

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Observation 6eef0521-dc55-4ea1-a085-aaeb5c17b283 · inbound

Dark energy and lensing anomaly in Planck CMB data cites this paper.

Dark energy and lensing anomaly in Planck CMB data Seven hints that early-time new physics alone is not sufficient to solve the Hubble tension

Reference 109

Resolution: unresolved; no resolver link, observed 2026-08-08T22:04:59.756372Z

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Observation 5944f95f-6a2d-4e46-8adf-302b09d13e4c · inbound

Alleviating the Hubble Tension with a Local Void and Transitions of the Absolute Magnitude cites this paper.

Alleviating the Hubble Tension with a Local Void and Transitions of the Absolute Magnitude Seven hints that early-time new physics alone is not sufficient to solve the Hubble tension

Reference 118

Resolution: unresolved; no resolver link, observed 2026-08-16T12:17:23.073851Z

Source-reported events for the cited work

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Observation f03902f7-f7ca-4530-9c43-ea15c1baddd6 · 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 Seven hints that early-time new physics alone is not sufficient to solve the Hubble tension

Reference 59

Resolution: unresolved; no resolver link, observed 2026-08-16T05:27:54.278651Z

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Observation 8bef3f66-0e33-4102-85fa-0c5be7c56d67 · inbound

The frozen vanilla model: Exploring dark sector interactions with delta effective theories cites this paper.

The frozen vanilla model: Exploring dark sector interactions with delta effective theories Seven hints that early-time new physics alone is not sufficient to solve the Hubble tension

Reference 40

Resolution: unresolved; no resolver link, observed 2026-08-16T05:19:56.201787Z

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Observation 2db1df4a-299c-4968-9115-9a6f728bdffd · inbound

Phantom matters cites this paper.

Phantom matters Seven hints that early-time new physics alone is not sufficient to solve the Hubble tension

Reference 65

Resolution: unresolved; no resolver link, observed 2026-08-15T21:15:07.436956Z

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Observation 487c2497-41a0-494a-bf3a-7fd9e485350e · inbound

Can the universe experience an AdS landscape since matter-radiation equality? cites this paper.

Can the universe experience an AdS landscape since matter-radiation equality? Seven hints that early-time new physics alone is not sufficient to solve the Hubble tension

Reference 114

Resolution: unresolved; no resolver link, observed 2026-08-07T10:52:56.641107Z

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Observation 325598b0-4506-4c5e-8cd6-16b9868c53fe · inbound

Constraints on Dark Energy Models Using Late Universe Probes cites this paper.

Constraints on Dark Energy Models Using Late Universe Probes Seven hints that early-time new physics alone is not sufficient to solve the Hubble tension

Reference 56

Resolution: unresolved; no resolver link, observed 2026-08-07T00:54:43.318362Z

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Observation 4bb647fc-dae8-4724-85d0-a9fa98d3ea9b · inbound

Decay of dark energy into dark matter in a metric $f(R)$ gravity: effective running Hubble constant cites this paper.

Decay of dark energy into dark matter in a metric $f(R)$ gravity: effective running Hubble constant Seven hints that early-time new physics alone is not sufficient to solve the Hubble tension

Reference 393

Resolution: unresolved; no resolver link, observed 2026-08-07T00:50:27.197839Z

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Observation 427975d2-4800-4117-aa1d-999d7dae519a · inbound

Dark energy era with a resolution of Hubble tension in generalized entropic cosmology cites this paper.

Dark energy era with a resolution of Hubble tension in generalized entropic cosmology Seven hints that early-time new physics alone is not sufficient to solve the Hubble tension

Reference 80

Resolution: unresolved; no resolver link, observed 2026-08-06T15:45:30.310799Z

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Observation ad3e8665-70b6-4188-879b-d00ba7195965 · inbound

How Holographic is the Dark Energy? A Spline Nodal reconstruction approach cites this paper.

How Holographic is the Dark Energy? A Spline Nodal reconstruction approach Seven hints that early-time new physics alone is not sufficient to solve the Hubble tension

Reference 19

Resolution: unresolved; no resolver link, observed 2026-08-06T12:01:08.635598Z

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Observation 60e221b5-ba91-4b97-9ecb-0fa570007382 · inbound

Resolving the Planck-DESI tension by nonminimally coupled quintessence cites this paper.

Resolving the Planck-DESI tension by nonminimally coupled quintessence Seven hints that early-time new physics alone is not sufficient to solve the Hubble tension

Reference 123

Resolution: metadata mismatch; arxiv_id, observed 2026-05-19T01:36:57.899727Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

Observation 7bb115ae-de1f-4e17-bf39-30ac827225c6 · inbound

Probing the Cosmic Distance Duality Relation via Non-Parametric Reconstruction for High Redshifts cites this paper.

Probing the Cosmic Distance Duality Relation via Non-Parametric Reconstruction for High Redshifts Seven hints that early-time new physics alone is not sufficient to solve the Hubble tension

Reference 5

Resolution: unresolved; no resolver link, observed 2026-08-15T16:14:10.084072Z

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Observation 0b47c248-90e8-429e-a095-f0f2cd534abc · 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 Seven hints that early-time new physics alone is not sufficient to solve the Hubble tension

Reference 34

Resolution: unresolved; no resolver link, observed 2026-08-04T09:59:13.108069Z

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Observation e07dd37e-925f-4b3d-8707-33e63cf1075a · inbound

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 Seven hints that early-time new physics alone is not sufficient to solve the Hubble tension

Reference 16

Resolution: unresolved; no resolver link, observed 2026-08-04T07:19:36.755191Z

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Observation de403ac2-abf9-49a6-b495-4b928389b404 · inbound

Exponential $f(R)$ cosmology with massive neutrinos as a dynamical dark energy framework cites this paper.

Exponential $f(R)$ cosmology with massive neutrinos as a dynamical dark energy framework Seven hints that early-time new physics alone is not sufficient to solve the Hubble tension

Reference 67

Resolution: unresolved; no resolver link, observed 2026-08-03T23:16:57.145708Z

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Observation 3dee41bb-c576-4b51-926e-28a9fd061ee4 · inbound

Updates on dipolar anisotropy in local measurements of the Hubble constant from Cosmicflows-4 cites this paper.

Updates on dipolar anisotropy in local measurements of the Hubble constant from Cosmicflows-4 Seven hints that early-time new physics alone is not sufficient to solve the Hubble tension

Reference 15

Resolution: verified exact; arxiv_id, observed 2026-05-17T02:51:27.706169Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

Observation 4d6cef91-5bdc-4209-b14e-2d57688a0fc3 · inbound

Towards a unified quantum field theory of dark energy and inflation: unstable de Sitter vacuum and running vacuum cites this paper.

Towards a unified quantum field theory of dark energy and inflation: unstable de Sitter vacuum and running vacuum Seven hints that early-time new physics alone is not sufficient to solve the Hubble tension

Reference 9

Resolution: unresolved; no resolver link, observed 2026-08-03T11:53:05.924353Z

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Observation 6c3c1676-3eb7-4cbd-bfa7-3b84320c6a2e · inbound

Robust Preference for Dark Sector Interactions cites this paper.

Robust Preference for Dark Sector Interactions Seven hints that early-time new physics alone is not sufficient to solve the Hubble tension

Reference 148

Resolution: unresolved; no resolver link, observed 2026-08-03T11:11:48.990482Z

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Observation 8ef36572-f0f4-4881-be88-3064af122c1d · inbound

Hubble Tension as an Effect of Horizon Entanglement Nonequilibrium cites this paper.

Hubble Tension as an Effect of Horizon Entanglement Nonequilibrium Seven hints that early-time new physics alone is not sufficient to solve the Hubble tension

Reference 9

Resolution: unresolved; no resolver link, observed 2026-08-03T08:14:17.826615Z

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Observation f8ea60a6-784f-47b8-a4c6-137141efa58f · inbound

Evidence for deviation in gravitational light deflection from general relativity at cosmological scales with KiDS-Legacy and CMB lensing cites this paper.

Evidence for deviation in gravitational light deflection from general relativity at cosmological scales with KiDS-Legacy and CMB lensing Seven hints that early-time new physics alone is not sufficient to solve the Hubble tension

Reference 22

Resolution: verified exact; arxiv_id, observed 2026-05-16T08:17:35.990287Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

Observation 45434207-139b-4f93-8896-861487d70fe7 · inbound

New constraints on cosmic anisotropy from galaxy clusters using an improved dipole fitting method cites this paper.

New constraints on cosmic anisotropy from galaxy clusters using an improved dipole fitting method Seven hints that early-time new physics alone is not sufficient to solve the Hubble tension

Reference 24

Resolution: verified exact; arxiv_id, observed 2026-05-16T02:27:10.031636Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

Observation af038df4-e256-454c-b891-4fac640e82de · 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 Seven hints that early-time new physics alone is not sufficient to solve the Hubble tension

Reference 25

Resolution: verified exact; arxiv_id, observed 2026-05-21T13:30:12.507030Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

Observation 6d4af3e0-b50f-400f-b297-53616f050723 · inbound

Measuring neutrino mass in light of ACT DR6 and DESI DR2 cites this paper.

Measuring neutrino mass in light of ACT DR6 and DESI DR2 Seven hints that early-time new physics alone is not sufficient to solve the Hubble tension

Reference 8

Resolution: verified exact; arxiv_id, observed 2026-05-15T13:15:49.845667Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

Observation b96ab432-36ca-45b7-b1eb-e42a0b069c40 · 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 Seven hints that early-time new physics alone is not sufficient to solve the Hubble tension

Reference 21

Resolution: unresolved; no resolver link, observed 2026-07-15T12:01:04.317365Z

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Observation acd2a070-2319-4671-986e-de729fbc516a · inbound

Exploring the interplay of late-time dynamical dark energy and new physics before recombination cites this paper.

Exploring the interplay of late-time dynamical dark energy and new physics before recombination Seven hints that early-time new physics alone is not sufficient to solve the Hubble tension

Reference 116

Resolution: verified exact; arxiv_id, observed 2026-05-14T23:13:15.852400Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

Observation 702b101b-02a9-47bc-a1ef-0d5eee1bb035 · inbound

Do equation of state parametrizations of dark energy faithfully capture the dynamics of the late universe? cites this paper.

Do equation of state parametrizations of dark energy faithfully capture the dynamics of the late universe? Seven hints that early-time new physics alone is not sufficient to solve the Hubble tension

Reference 28

Resolution: verified exact; arxiv_id, observed 2026-05-11T11:36:01.933652Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

Observation 49fd51c0-e10f-49b4-9c5a-25d0c592bb59 · 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 Seven hints that early-time new physics alone is not sufficient to solve the Hubble tension

Reference 184

Resolution: verified exact; arxiv_id, observed 2026-05-10T13:00:24.911619Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

Observation aaad87eb-d9c7-400e-b2cf-191c38b74823 · 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 Seven hints that early-time new physics alone is not sufficient to solve the Hubble tension

Reference 52

Resolution: verified exact; arxiv_id, observed 2026-05-11T12:11:05.559298Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

Observation 7ad01af4-5a91-430c-a282-3764a8e34641 · inbound

Testing $\Lambda$CDM with ANN-Reconstructed Expansion History from Cosmic Chronometers cites this paper.

Testing $\Lambda$CDM with ANN-Reconstructed Expansion History from Cosmic Chronometers Seven hints that early-time new physics alone is not sufficient to solve the Hubble tension

Reference 19

Resolution: verified exact; arxiv_id, observed 2026-05-11T20:11:11.342629Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

Observation e81a101d-d98a-4116-8874-9561deb191e8 · 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 Seven hints that early-time new physics alone is not sufficient to solve the Hubble tension

Reference 137

Resolution: verified exact; arxiv_id, observed 2026-05-12T00:36:15.745908Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

Observation d03ba858-eb4d-4827-a6f1-0afd35ce9fc7 · inbound

Cosmological intercept tension cites this paper.

Cosmological intercept tension Seven hints that early-time new physics alone is not sufficient to solve the Hubble tension

Reference 15

Resolution: verified exact; arxiv_id, observed 2026-05-12T10:26:31.108793Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

Observation 49ab689e-d929-4eaa-ac0c-eef5af2b2ba1 · inbound

Early- and Late-Time Modifications to $\Lambda$CDM: Implications for the Hubble Tension cites this paper.

Early- and Late-Time Modifications to $\Lambda$CDM: Implications for the Hubble Tension Seven hints that early-time new physics alone is not sufficient to solve the Hubble tension

Reference 96

Resolution: verified exact; arxiv_id, observed 2026-06-30T00:14:04.979589Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

Observation 833a0fe0-220d-425a-bace-a056c1cb6957 · inbound

Running Vacuum in the expanding Universe: a unified QFT paradigm for Inflation and Dark Energy cites this paper.

Running Vacuum in the expanding Universe: a unified QFT paradigm for Inflation and Dark Energy Seven hints that early-time new physics alone is not sufficient to solve the Hubble tension

Reference 88

Resolution: verified exact; arxiv_id, observed 2026-07-02T10:36:52.438688Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

Observation 23a08a71-7ca4-421f-91a5-92102d67f232 · inbound

Running Vacuum in the expanding Universe: a unified QFT paradigm for Inflation and Dark Energy cites this paper.

Running Vacuum in the expanding Universe: a unified QFT paradigm for Inflation and Dark Energy Seven hints that early-time new physics alone is not sufficient to solve the Hubble tension

Reference 88

Resolution: unresolved; no resolver link, observed 2026-07-12T15:09:17.581029Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation d7b4cb97-17fe-4b1d-ab0b-bd464bfd05c4 · 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 Seven hints that early-time new physics alone is not sufficient to solve the Hubble tension

Reference 77

Resolution: verified exact; arxiv_id, observed 2026-07-02T15:37:06.599328Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

Observation 129827e3-fa3b-4196-a050-319f5c65d981 · inbound

Geometric obstruction to resolving the Hubble tension: orthogonality of scale and shape in distance measurements cites this paper.

Geometric obstruction to resolving the Hubble tension: orthogonality of scale and shape in distance measurements Seven hints that early-time new physics alone is not sufficient to solve the Hubble tension

Reference 26

Resolution: verified exact; arxiv_id, observed 2026-07-03T15:38:34.071218Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

Observation e033a148-db9b-462c-b5e5-91d2034d8cb4 · inbound

Resolving the Hubble Tension in the Early Dark Energy Framework with JWST and DESI Data cites this paper.

Resolving the Hubble Tension in the Early Dark Energy Framework with JWST and DESI Data Seven hints that early-time new physics alone is not sufficient to solve the Hubble tension

Reference 20

Resolution: verified exact; arxiv_id, observed 2026-07-04T02:19:23.784422Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

Observation ea5b3ff7-3d96-4581-806f-6243fe2a32f5 · inbound

The Hubble tension: A decade review cites this paper.

The Hubble tension: A decade review Seven hints that early-time new physics alone is not sufficient to solve the Hubble tension

Reference 27

Resolution: verified exact; arxiv_id, observed 2026-07-04T05:19:36.224842Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

Observation 86db94b7-bb8e-489f-8d0c-e75258a3cddb · inbound

The Hubble tension: A decade review cites this paper.

The Hubble tension: A decade review Seven hints that early-time new physics alone is not sufficient to solve the Hubble tension

Reference 27

Resolution: unresolved; no resolver link, observed 2026-07-15T10:41:50.733215Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 60fb37e9-bcc6-4490-9d42-658981cdfdba · inbound

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

Cosmological Viability of Exponential Infrared $f(T)$ Gravity Seven hints that early-time new physics alone is not sufficient to solve the Hubble tension

Reference 128

Resolution: verified exact; arxiv_id, observed 2026-07-01T11:15:42.351185Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

Observation be5f104d-cafe-4522-ad0f-c4b15e5ae001 · 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 Seven hints that early-time new physics alone is not sufficient to solve the Hubble tension

Reference 166

Resolution: verified exact; arxiv_id, observed 2026-07-01T11:25:45.760789Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

Observation f32ae36d-3b38-4806-b53a-51273e0856f9 · 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 Seven hints that early-time new physics alone is not sufficient to solve the Hubble tension

Reference 31

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 a3079007-70d8-43de-b78d-39f8588a5804 · inbound

Imprint of swampland-inspired coupled early dark energy cites this paper.

Imprint of swampland-inspired coupled early dark energy Seven hints that early-time new physics alone is not sufficient to solve the Hubble tension

Reference 98

Resolution: verified exact; local_arxiv, observed 2026-07-08T15:55:04.756263Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

Observation e4e4dad9-675a-4c2b-aa7e-6dced4b1beaa · inbound

Skipping the rungs! Calibrating distance indicators through their clustering with galaxies cites this paper.

Skipping the rungs! Calibrating distance indicators through their clustering with galaxies Seven hints that early-time new physics alone is not sufficient to solve the Hubble tension

Reference 9

Resolution: verified exact; local_arxiv, observed 2026-07-08T01:44:25.985956Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

Observation 24cc2f9a-6af7-40fd-bd56-54776897cc18 · inbound

Skipping the rungs! Calibrating distance indicators through their clustering with galaxies cites this paper.

Skipping the rungs! Calibrating distance indicators through their clustering with galaxies Seven hints that early-time new physics alone is not sufficient to solve the Hubble tension

Reference 9

Resolution: unresolved; no resolver link, observed 2026-07-13T06:51:47.584044Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation c72a190d-acaf-4dbc-b0cf-4211540c4596 · inbound

Can Distance Duality Violation Save Late-time Solutions to the Hubble Tension? cites this paper.

Can Distance Duality Violation Save Late-time Solutions to the Hubble Tension? Seven hints that early-time new physics alone is not sufficient to solve the Hubble tension

Reference 44

Resolution: metadata mismatch; local_arxiv, observed 2026-07-10T03:56:44.453627Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

Observation 1e19479d-b9e0-4635-b3f1-bfd26ecc52f6 · inbound

Late-time cosmological constraints on three holographic dark energy models with DESI DR2 BAO and Type Ia supernovae cites this paper.

Late-time cosmological constraints on three holographic dark energy models with DESI DR2 BAO and Type Ia supernovae Seven hints that early-time new physics alone is not sufficient to solve the Hubble tension

Reference 24

Resolution: unresolved; no resolver link, observed 2026-07-14T16:44:02.461654Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 9c07a0ba-edca-42ca-bd75-de535cf8e378 · inbound

Evaporating cosmologically coupled black holes cites this paper.

Evaporating cosmologically coupled black holes Seven hints that early-time new physics alone is not sufficient to solve the Hubble tension

Reference 235

Resolution: unresolved; no resolver link, observed 2026-08-02T03:36:03.635596Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation c9322e40-4d1e-461f-9e6f-393952a5f167 · 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 Seven hints that early-time new physics alone is not sufficient to solve the Hubble tension

Reference 9

Resolution: unresolved; no resolver link, observed 2026-08-01T11:25:06.200455Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 07acaf7d-38d6-4354-a57f-a3431094e233 · inbound

Hubble tension: the shape wall cites this paper.

Hubble tension: the shape wall Seven hints that early-time new physics alone is not sufficient to solve the Hubble tension

Reference 14

Resolution: unresolved; no resolver link, observed 2026-08-01T08:08:30.726018Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation ea8e3b34-ecb7-43c8-89af-0e52d4cc8aea · inbound

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

Hubble tension: a short review of theoretical explanations Seven hints that early-time new physics alone is not sufficient to solve the Hubble tension

Reference 183

Resolution: unresolved; no resolver link, observed 2026-08-01T07:20:08.068931Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 401b7eba-04bc-4902-b5c6-97c3c7f364e4 · inbound

Hubble tension problem encompassed by phase-space quantum cosmology cites this paper.

Hubble tension problem encompassed by phase-space quantum cosmology Seven hints that early-time new physics alone is not sufficient to solve the Hubble tension

Reference 23

Resolution: unresolved; no resolver link, observed 2026-08-01T10:32:14.460712Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 9f48cf52-7f92-4cab-8cbb-2312a763ed98 · inbound

Adiabatic Perturbations in GW170817-Compatible Einstein-Gauss-Bonnet Inflation cites this paper.

Adiabatic Perturbations in GW170817-Compatible Einstein-Gauss-Bonnet Inflation Seven hints that early-time new physics alone is not sufficient to solve the Hubble tension

Reference 147

Resolution: unresolved; no resolver link, observed 2026-08-11T10:59:31.466280Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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