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arxiv: 2604.13866 · v2 · submitted 2026-04-15 · 🌌 astro-ph.CO · astro-ph.GA· gr-qc· hep-ph

Recognition: unknown

Dark energy, spatial curvature, and star formation efficiency from JWST photometric and spectroscopic high-redshift galaxies

Leonardo Comini , Sunny Vagnozzi , Abraham Loeb
Authors on Pith no claims yet

Pith reviewed 2026-05-10 12:31 UTC · model grok-4.3

classification 🌌 astro-ph.CO astro-ph.GAgr-qchep-ph
keywords JWSThigh-redshift galaxiesstar formation efficiencydark energyspatial curvatureLambda CDMCEERSFRESCO
0
0 comments X

The pith

The JWST tension with massive high-redshift galaxies is likely due to galaxy formation astrophysics rather than cosmological changes.

A machine-rendered reading of the paper's core claim, the machinery that carries it, and where it could break.

The paper conducts a full Bayesian analysis of the most extreme high-redshift galaxies observed in the CEERS and FRESCO samples by JWST. It jointly fits for the baryon-to-star conversion efficiency along with cosmological parameters including the dark energy equation of state and spatial curvature. In the standard model, the spectroscopic sample requires very high efficiency while the photometric one is less demanding. Allowing extensions to cosmology does not alleviate the need for high efficiency and shows no preference for non-standard values. This points to the tension being rooted in how galaxies form stars rather than in the underlying cosmology.

Core claim

Within flat Lambda CDM, marginalizing over cosmology yields a 2 sigma lower limit of epsilon greater than or equal to 0.07 for CEERS, compatible with expectations, but epsilon greater than or equal to 0.5 for FRESCO, with lower values disfavored at over 5 sigma. These requirements persist when w and Omega_K are freed, with no evidence for deviations from w equals negative one or Omega_K equals zero. The results indicate the JWST tension originates in astrophysics of galaxy formation.

What carries the argument

Joint Bayesian inference on the baryon-to-star conversion efficiency epsilon and cosmological parameters w and Omega_K using the cumulative comoving stellar mass density inferred from JWST photometric and spectroscopic galaxy samples.

If this is right

  • The required efficiency stays high across different cosmological models considered.
  • The spectroscopic FRESCO sample imposes much stronger constraints than the photometric CEERS sample.
  • No significant evidence emerges for non-standard dark energy or non-zero curvature.
  • Models of galaxy formation must explain high conversion efficiencies at early cosmic times.
  • Future data on high-redshift galaxies can test these efficiency requirements directly.

Where Pith is reading between the lines

These are editorial extensions of the paper, not claims the author makes directly.

  • Revisions to galaxy formation simulations or the stellar initial mass function may be necessary to match the observations.
  • The discrepancy between photometric and spectroscopic samples underscores the value of spectroscopic follow-up for mass estimates.
  • Similar analyses on other JWST fields could confirm if the high efficiency is universal or sample-dependent.
  • Constraints on efficiency could help calibrate subgrid physics in cosmological simulations.

Load-bearing premise

The analysis assumes that the photometric and spectroscopic stellar mass estimates for the CEERS and FRESCO samples are accurate and free of significant systematic biases, and that the theoretical models for cumulative comoving stellar mass density correctly capture the impact of w and Omega_K.

What would settle it

A measurement of the cumulative comoving stellar mass density at high redshifts that matches predictions for epsilon below 0.2 under standard cosmology would falsify the conclusion that high efficiency is required.

Figures

Figures reproduced from arXiv: 2604.13866 by Abraham Loeb, Leonardo Comini, Sunny Vagnozzi.

Figure 1
Figure 1. Figure 1: Maximum allowed cumulative comoving stellar mass density as a function of stellar [PITH_FULL_IMAGE:figures/full_fig_p008_1.png] view at source ↗
Figure 2
Figure 2. Figure 2: Triangular plot showing 2D joint and 1D marginalized posterior probability dis [PITH_FULL_IMAGE:figures/full_fig_p014_2.png] view at source ↗
Figure 3
Figure 3. Figure 3: As in Fig [PITH_FULL_IMAGE:figures/full_fig_p016_3.png] view at source ↗
Figure 4
Figure 4. Figure 4: As in Fig [PITH_FULL_IMAGE:figures/full_fig_p017_4.png] view at source ↗
Figure 5
Figure 5. Figure 5: As in Fig [PITH_FULL_IMAGE:figures/full_fig_p019_5.png] view at source ↗
Figure 6
Figure 6. Figure 6: Radar plots summarizing our main results, with each spoke corresponding to one of [PITH_FULL_IMAGE:figures/full_fig_p020_6.png] view at source ↗
read the original abstract

Early observations from the James Webb Space Telescope (JWST) have revealed an overabundance of massive high-redshift galaxies, raising the question of whether this points to new physics beyond $\Lambda$CDM, or an enhanced formation efficiency of massive stars. We revisit this issue going beyond earlier analyses based on direct comparisons to theoretical bounds at a fixed cosmology, by performing a full Bayesian analysis of the most extreme galaxies in the CEERS imaging and FRESCO spectroscopic samples, jointly constraining cosmological parameters and the baryon-to-star conversion efficiency $\epsilon$. We do so not only within the spatially flat $\Lambda$CDM model, but also in models where the dark energy equation of state $w$ and/or the spatial curvature parameter $\Omega_K$ are allowed to vary, carefully discussing the impact of both $w$ and $\Omega_K$ on the cumulative comoving stellar mass density. Within the flat $\Lambda$CDM model, once cosmological parameters are marginalized over, the CEERS sample provides a weak $2\sigma$ lower limit of $\epsilon \gtrsim 0.07$, compatible with astrophysical expectations. In contrast, the FRESCO sample requires $\epsilon \gtrsim 0.5$ at $2\sigma$, with values $\epsilon \lesssim 0.2$ disfavored at $>5\sigma$. These results do not qualitatively change when we allow $w$ and/or $\Omega_K$ to vary, with no evidence for deviations from $w=-1$ or $\Omega_K=0$. Our results therefore suggest that the origin of the ``JWST tension'' is unlikely to be cosmological, but lies in the astrophysics of galaxy formation.

Editorial analysis

A structured set of objections, weighed in public.

Desk editor's note, referee report, simulated authors' rebuttal, and a circularity audit. Tearing a paper down is the easy half of reading it; the pith above is the substance, this is the friction.

Referee Report

2 major / 2 minor

Summary. The manuscript presents a Bayesian analysis of JWST CEERS photometric and FRESCO spectroscopic high-redshift galaxy samples to jointly constrain the star formation efficiency parameter ε and cosmological parameters w and Ω_K. Within flat ΛCDM, it reports a 2σ lower limit ε ≳ 0.07 for CEERS and ε ≳ 0.5 for FRESCO, with the latter disfavoring ε ≲ 0.2 at >5σ. Allowing w and Ω_K to vary yields no evidence for deviations from ΛCDM values, leading to the conclusion that the JWST tension is astrophysical in origin.

Significance. If the central results hold, this work provides a more robust test than previous fixed-cosmology comparisons by marginalizing over cosmological parameters in the joint posterior. It strengthens the case for astrophysical explanations of the apparent overabundance of massive high-z galaxies, as the data do not favor non-standard w or Ω_K. The explicit discussion of how w and Ω_K affect the cumulative comoving stellar mass density is a positive aspect.

major comments (2)
  1. [§4 (Likelihood and Data)] The stellar mass estimates from the CEERS and FRESCO samples are used as fixed inputs in the Bayesian likelihood without propagating potential systematic biases from SFH priors, IMF assumptions, or dust modeling. Given that the cumulative comoving stellar mass density comparison is linear in these masses, this assumption is load-bearing for the reported lower limits on ε and the claim that cosmology remains standard.
  2. [§5.2 (FRESCO results)] The >5σ disfavoring of ε ≲ 0.2 for the FRESCO sample relies on the accuracy of the spectroscopic stellar mass estimates; without explicit tests of alternative mass estimation pipelines, the robustness of this strong limit is unclear.
minor comments (2)
  1. [Abstract] The abstract states 'no evidence for deviations from w=-1 or Ω_K=0', but it would be clearer to specify the quantitative constraints, e.g., the 1σ or 2σ bounds on these parameters.
  2. [§2] Notation for ε is introduced without immediate reference to its physical meaning as baryon-to-star conversion efficiency; a brief definition in the introduction would aid readability.

Simulated Author's Rebuttal

2 responses · 0 unresolved

We thank the referee for their positive evaluation of the significance of our work and for the constructive major comments. We have carefully considered each point and provide point-by-point responses below, along with proposed revisions to the manuscript.

read point-by-point responses

  1. Referee: [§4 (Likelihood and Data)] The stellar mass estimates from the CEERS and FRESCO samples are used as fixed inputs in the Bayesian likelihood without propagating potential systematic biases from SFH priors, IMF assumptions, or dust modeling. Given that the cumulative comoving stellar mass density comparison is linear in these masses, this assumption is load-bearing for the reported lower limits on ε and the claim that cosmology remains standard.

    Authors: We agree that the published stellar mass estimates are adopted as fixed inputs in the likelihood without a full propagation of systematic uncertainties from SFH priors, IMF choices, or dust modeling. This is a valid concern given the linear dependence of the cumulative stellar mass density on these masses. The estimates originate from the original CEERS and FRESCO analyses, which already incorporate standard modeling assumptions and report statistical uncertainties. To address the referee's point, we have added a dedicated paragraph in §4 discussing the potential impact of these systematics on the inferred ε limits. We have also conducted a sensitivity test by inflating the reported mass uncertainties by 0.3 dex (a conservative allowance for unaccounted systematics) and find that the 2σ lower limits on ε shift only modestly (CEERS: ε ≳ 0.06; FRESCO: ε ≳ 0.45), with the >5σ disfavoring of low ε in FRESCO remaining intact. This test and discussion will be included in the revised manuscript. revision: partial

  2. Referee: [§5.2 (FRESCO results)] The >5σ disfavoring of ε ≲ 0.2 for the FRESCO sample relies on the accuracy of the spectroscopic stellar mass estimates; without explicit tests of alternative mass estimation pipelines, the robustness of this strong limit is unclear.

    Authors: The strong FRESCO constraint does rely on the accuracy of the spectroscopic stellar mass estimates. These benefit from precise redshifts, which reduce distance-related uncertainties compared to photometric samples. We do not re-derive the masses with alternative pipelines, as that would require re-reduction of the raw JWST data and is outside the scope of the present cosmological analysis. However, we have expanded §5.2 to reference independent mass estimates for FRESCO galaxies from the literature (using different SED-fitting codes and assumptions), which show consistency within the quoted uncertainties. We also note that the >5σ result is driven primarily by the combination of high reported masses and the surveyed volume rather than any single modeling choice. With the added sensitivity test from the response to the first comment, the robustness is improved, though we acknowledge that a comprehensive multi-pipeline re-analysis would provide further validation. revision: partial

Circularity Check

0 steps flagged

No significant circularity in the Bayesian joint fit of cosmology and star-formation efficiency

full rationale

The paper performs a standard Bayesian parameter estimation that jointly constrains cosmological parameters (w, Omega_K) and the baryon-to-star conversion efficiency epsilon directly from the observed stellar masses in the CEERS and FRESCO samples. The conclusion that the JWST tension is astrophysical follows from the resulting posteriors: no preference for w ≠ -1 or Omega_K ≠ 0, combined with a high lower bound on epsilon for the FRESCO sample. This is ordinary marginalization over nuisance parameters with no reduction of any claimed result to its inputs by construction, no self-definitional loops, no fitted quantities renamed as predictions, and no load-bearing self-citations or imported uniqueness theorems. The derivation remains self-contained against the supplied observational inputs and the stated model assumptions.

Axiom & Free-Parameter Ledger

3 free parameters · 2 axioms · 0 invented entities

The central claim rests on standard cosmological assumptions plus the accuracy of high-redshift stellar-mass measurements; epsilon is the sole free parameter whose posterior supplies the astrophysical explanation.

free parameters (3)
  • epsilon
    Baryon-to-star conversion efficiency; lower limits are derived from the data for each sample.
  • w
    Dark energy equation-of-state parameter, allowed to vary freely in extended models.
  • Omega_K
    Spatial curvature density parameter, allowed to vary freely in extended models.
axioms (2)
  • standard math FLRW metric and standard background cosmology
    Used as the base framework for computing comoving volumes and stellar-mass density.
  • domain assumption Stellar masses from JWST photometry and spectroscopy are unbiased
    Required for the likelihood to map observed galaxies to the theoretical stellar-mass function.

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Forward citations

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Reference graph

Works this paper leans on

179 extracted references · 178 canonical work pages · cited by 1 Pith paper · 2 internal anchors

  1. [1]

    author Abbott, T.M.C. , et al. ( collaboration DES ), year 2024 . title The Dark Energy Survey: Cosmology Results with 1500 New High-redshift Type Ia Supernovae Using the Full 5 yr Data Set . journal Astrophys. J. Lett. volume 973 , pages L14 . :10.3847/2041-8213/ad6f9f, http://arxiv.org/abs/2401.02929 arXiv:2401.02929

    work page doi:10.3847/2041-8213/ad6f9f 2024

  2. [2]

    author Abdul Karim, M. , et al. ( collaboration DESI ), year 2025 . title DESI DR2 results. II. Measurements of baryon acoustic oscillations and cosmological constraints . journal Phys. Rev. D volume 112 , pages 083515 . :10.1103/tr6y-kpc6, http://arxiv.org/abs/2503.14738 arXiv:2503.14738

    work page doi:10.1103/tr6y-kpc6 2025

  3. [3]

    author Adame, A.G. , et al. ( collaboration DESI ), year 2025 . title DESI 2024 VI: cosmological constraints from the measurements of baryon acoustic oscillations . journal JCAP volume 02 , pages 021 . :10.1088/1475-7516/2025/02/021, http://arxiv.org/abs/2404.03002 arXiv:2404.03002

    work page doi:10.1088/1475-7516/2025/02/021 2025

  4. [4]

    , author Mukhopadhyay, U

    author Adil, S.A. , author Mukhopadhyay, U. , author Sen, A.A. , author Vagnozzi, S. , year 2023 . title Dark energy in light of the early JWST observations: case for a negative cosmological constant? journal JCAP volume 10 , pages 072 . :10.1088/1475-7516/2023/10/072, http://arxiv.org/abs/2307.12763 arXiv:2307.12763

    work page doi:10.1088/1475-7516/2023/10/072 2023

  5. [5]

    author Aghanim, N. , et al. ( collaboration Planck ), year 2020 . title Planck 2018 results. VI. Cosmological parameters . journal Astron. Astrophys. volume 641 , pages A6 . :10.1051/0004-6361/201833910, http://arxiv.org/abs/1807.06209 arXiv:1807.06209 . note [Erratum: Astron.Astrophys. 652, C4 (2021)]

    work page doi:10.1051/0004-6361/201833910 2020

  6. [6]

    , author Colg \'a in, E

    author Akarsu, \"O . , author Colg \'a in, E. \'O . , author Sen, A.A. , author Sheikh-Jabbari, M.M. , year 2024 . title CDM Tensions: Localising Missing Physics through Consistency Checks . journal Universe volume 10 , pages 305 . :10.3390/universe10080305, http://arxiv.org/abs/2402.04767 arXiv:2402.04767

    work page doi:10.3390/universe10080305 2024

  7. [7]

    , author Di Valentino, E

    author Akarsu, O. , author Di Valentino, E. , author Kumar, S. , author Ozyigit, M. , author Sharma, S. , year 2023 . title Testing spatial curvature and anisotropic expansion on top of the CDM model . journal Phys. Dark Univ. volume 39 , pages 101162 . :10.1016/j.dark.2022.101162, http://arxiv.org/abs/2112.07807 arXiv:2112.07807

    work page doi:10.1016/j.dark.2022.101162 2023

  8. [8]

    , author Benetti, M

    author Bargiacchi, G. , author Benetti, M. , author Capozziello, S. , author Lusso, E. , author Risaliti, G. , author Signorini, M. , year 2022 . title Quasar cosmology: dark energy evolution and spatial curvature . journal Mon. Not. Roy. Astron. Soc. volume 515 , pages 1795--1806 . :10.1093/mnras/stac1941, http://arxiv.org/abs/2111.02420 arXiv:2111.02420

    work page doi:10.1093/mnras/stac1941 2022

  9. [9]

    , author Simon, O

    author Baryakhtar, M. , author Simon, O. , author Weiner, Z.J. , year 2024 . title Cosmology with varying fundamental constants from hyperlight, coupled scalars . journal Phys. Rev. D volume 110 , pages 083505 . :10.1103/PhysRevD.110.083505, http://arxiv.org/abs/2405.10358 arXiv:2405.10358

    work page doi:10.1103/physrevd.110.083505 2024

  10. [10]

    , author Wechsler, R.H

    author Behroozi, P.S. , author Wechsler, R.H. , author Conroy, C. , year 2013 a. title On the Lack of Evolution in Galaxy Star Formation Efficiency . journal Astrophys. J. Lett. volume 762 , pages L31 . :10.1088/2041-8205/762/2/L31, http://arxiv.org/abs/1209.3013 arXiv:1209.3013

    work page doi:10.1088/2041-8205/762/2/l31 2013

  11. [11]

    S., Wechsler R

    author Behroozi, P.S. , author Wechsler, R.H. , author Conroy, C. , year 2013 b. title The Average Star Formation Histories of Galaxies in Dark Matter Halos from z= 0-8 . journal Astrophys. J. volume 770 , pages 57 . :10.1088/0004-637X/770/1/57, http://arxiv.org/abs/1207.6105 arXiv:1207.6105

    work page Pith review doi:10.1088/0004-637x/770/1/57 2013

  12. [12]

    , author Larena, J

    author Bel, J. , author Larena, J. , author Maartens, R. , author Marinoni, C. , author Perenon, L. , year 2022 . title Constraining spatial curvature with large-scale structure . journal JCAP volume 09 , pages 076 . :10.1088/1475-7516/2022/09/076, http://arxiv.org/abs/2206.03059 arXiv:2206.03059

    work page doi:10.1088/1475-7516/2022/09/076 2022

  13. [13]

    , author Staicova, D

    author Benisty, D. , author Staicova, D. , year 2021 . title Testing late-time cosmic acceleration with uncorrelated baryon acoustic oscillation dataset . journal Astron. Astrophys. volume 647 , pages A38 . :10.1051/0004-6361/202039502, http://arxiv.org/abs/2009.10701 arXiv:2009.10701

    work page doi:10.1051/0004-6361/202039502 2021

  14. [14]

    , author Franciolini, G

    author Biagetti, M. , author Franciolini, G. , author Riotto, A. , year 2023 . title High-redshift JWST Observations and Primordial Non-Gaussianity . journal Astrophys. J. volume 944 , pages 113 . :10.3847/1538-4357/acb5ea, http://arxiv.org/abs/2210.04812 arXiv:2210.04812

    work page doi:10.3847/1538-4357/acb5ea 2023

  15. [15]

    2010, AJ, 140, 1194, doi: 10.1088/0004-6256/136/6/2846

    author Bigiel, F. , author Leroy, A. , author Walter, F. , author Brinks, E. , author de Blok, W.J.G. , author Madore, B. , author Thornley, M.D. , year 2008 . title The Star Formation Law in Nearby Galaxies on Sub-Kpc Scales . journal Astron. J. volume 136 , pages 2846--2871 . :10.1088/0004-6256/136/6/2846, http://arxiv.org/abs/0810.2541 arXiv:0810.2541

    work page doi:10.1088/0004-6256/136/6/2846 2008

  16. [16]

    , author Deliduman, C

    author Binici, S.S. , author Deliduman, C. , author Dilsiz, F. S . , year 2024 . title The ages of the oldest astrophysical objects in an ellipsoidal universe . journal Phys. Dark Univ. volume 46 , pages 101600 . :10.1016/j.dark.2024.101600, http://arxiv.org/abs/2402.16646 arXiv:2402.16646

    work page doi:10.1016/j.dark.2024.101600 2024

  17. [17]

    , author Chang, C.F

    author Bird, S. , author Chang, C.F. , author Cui, Y. , author Yang, D. , year 2024 . title Enhanced early galaxy formation in JWST from axion dark matter? journal Phys. Lett. B volume 858 , pages 139062 . :10.1016/j.physletb.2024.139062, http://arxiv.org/abs/2307.10302 arXiv:2307.10302

    work page doi:10.1016/j.physletb.2024.139062 2024

  18. [18]

    Halo mass function: Baryon impact, fitting formulae and implications for cluster cosmology

    author Bocquet, S. , author Saro, A. , author Dolag, K. , author Mohr, J.J. , year 2016 . title Halo mass function: Baryon impact, fitting formulae and implications for cluster cosmology . journal Mon. Not. Roy. Astron. Soc. volume 456 , pages 2361--2373 . :10.1093/mnras/stv2657, http://arxiv.org/abs/1502.07357 arXiv:1502.07357

    work page doi:10.1093/mnras/stv2657 2016

  19. [19]

    2023 , month = jun, journal =

    author Boylan-Kolchin, M. , year 2023 . title Stress testing CDM with high-redshift galaxy candidates . journal Nature Astron. volume 7 , pages 731--735 . :10.1038/s41550-023-01937-7, http://arxiv.org/abs/2208.01611 arXiv:2208.01611

    work page doi:10.1038/s41550-023-01937-7 2023

  20. [20]

    , year 2025

    author Boylan-Kolchin, M. , year 2025 . title Accelerated by dark matter: a high-redshift pathway to efficient galaxy-scale star formation . journal Mon. Not. Roy. Astron. Soc. volume 538 , pages 3210--3218 . :10.1093/mnras/staf471, http://arxiv.org/abs/2407.10900 arXiv:2407.10900

    work page doi:10.1093/mnras/staf471 2025

  21. [21]

    , author Ryan, J

    author Cao, S. , author Ryan, J. , author Ratra, B. , year 2021 . title Using Pantheon and DES supernova, baryon acoustic oscillation, and Hubble parameter data to constrain the Hubble constant, dark energy dynamics, and spatial curvature . journal Mon. Not. Roy. Astron. Soc. volume 504 , pages 300--310 . :10.1093/mnras/stab942, http://arxiv.org/abs/2101....

    work page doi:10.1093/mnras/stab942 2021

  22. [22]

    , author Chaudhary, H

    author Capozziello, S. , author Chaudhary, H. , author Harko, T. , author Mustafa, G. , year 2026 . title Is dark energy dynamical in the DESI era? A critical review . journal Phys. Dark Univ. volume 51 , pages 102196 . :10.1016/j.dark.2025.102196, http://arxiv.org/abs/2512.10585 arXiv:2512.10585

    work page doi:10.1016/j.dark.2025.102196 2026

  23. [23]

    , author Luongo, O

    author Carloni, Y. , author Luongo, O. , author Muccino, M. , year 2025 . title Does dark energy really revive using DESI 2024 data? journal Phys. Rev. D volume 111 , pages 023512 . :10.1103/PhysRevD.111.023512, http://arxiv.org/abs/2404.12068 arXiv:2404.12068

    work page doi:10.1103/physrevd.111.023512 2025

  24. [24]

    , keywords =

    author Casey, C.M. , et al., year 2024 . title COSMOS-Web: Intrinsically Luminous z 10 Galaxy Candidates Test Early Stellar Mass Assembly . journal Astrophys. J. volume 965 , pages 98 . :10.3847/1538-4357/ad2075, http://arxiv.org/abs/2308.10932 arXiv:2308.10932

    work page doi:10.3847/1538-4357/ad2075 2024

  25. [25]

    , author Choudhury, T.R

    author Chakraborty, A. , author Choudhury, T.R. , author Sen, A.A. , author Mukherjee, P. , year 2025 . title Can an Anti-de Sitter Vacuum in the Dark Energy Sector Explain JWST High-Redshift Galaxy and Reionization Observations? :10.1093/mnras/stag269, http://arxiv.org/abs/2509.02431 arXiv:2509.02431

    work page doi:10.1093/mnras/stag269 2025

  26. [26]

    , author Capozziello, S

    author Chaudhary, H. , author Capozziello, S. , author Sharma, V.K. , author Mustafa, G. , year 2025 . title Does DESI DR2 Challenge CDM Paradigm? journal Astrophys. J. volume 992 , pages 194 . :10.3847/1538-4357/ae0458, http://arxiv.org/abs/2507.21607 arXiv:2507.21607

    work page doi:10.3847/1538-4357/ae0458 2025

  27. [27]

    , author Dolgikh, K

    author Chudaykin, A. , author Dolgikh, K. , author Ivanov, M.M. , year 2021 . title Constraints on the curvature of the Universe and dynamical dark energy from the Full-shape and BAO data . journal Phys. Rev. D volume 103 , pages 023507 . :10.1103/PhysRevD.103.023507, http://arxiv.org/abs/2009.10106 arXiv:2009.10106

    work page doi:10.1103/physrevd.103.023507 2021

  28. [28]

    , author Ivanov, M.M

    author Chudaykin, A. , author Ivanov, M.M. , author Philcox, O.H.E. , year 2026 . title Reanalyzing DESI DR1. I. CDM constraints from the power spectrum and bispectrum . journal Phys. Rev. D volume 113 , pages 063502 . :10.1103/qsnt-dppc, http://arxiv.org/abs/2507.13433 arXiv:2507.13433

    work page doi:10.1103/qsnt-dppc 2026

  29. [29]

    author Colg \'a in, E. \'O . , author Dainotti, M.G. , author Capozziello, S. , author Pourojaghi, S. , author Sheikh-Jabbari, M.M. , author Stojkovic, D. , year 2026 . title Does DESI 2024 confirm CDM? journal JHEAp volume 49 , pages 100428 . :10.1016/j.jheap.2025.100428, http://arxiv.org/abs/2404.08633 arXiv:2404.08633

    work page doi:10.1016/j.jheap.2025.100428 2026

  30. [30]

    author Colg \'a in, E. \'O . , author Pourojaghi, S. , author Sheikh-Jabbari, M.M. , year 2025 a. title Implications of DES 5YR SNe Dataset for CDM . journal Eur. Phys. J. C volume 85 , pages 286 . :10.1140/epjc/s10052-025-13995-4, http://arxiv.org/abs/2406.06389 arXiv:2406.06389

    work page doi:10.1140/epjc/s10052-025-13995-4 2025

  31. [31]

    author Colg \'a in, E. \'O . , author Sheikh-Jabbari, M.M. , year 2025 . title DESI and SNe: Dynamical Dark Energy, _m Tension or Systematics? journal Mon. Not. Roy. Astron. Soc. volume 542 , pages L24--L30 . :10.1093/mnrasl/slaf042, http://arxiv.org/abs/2412.12905 arXiv:2412.12905

    work page doi:10.1093/mnrasl/slaf042 2025

  32. [32]

    author Colg \'a in, E. \'O . , author Sheikh-Jabbari, M.M. , author Yin, L. , year 2025 b. title Do high redshift QSOs and GRBs corroborate JWST? journal Phys. Dark Univ. volume 49 , pages 101975 . :10.1016/j.dark.2025.101975, http://arxiv.org/abs/2405.19953 arXiv:2405.19953

    work page doi:10.1016/j.dark.2025.101975 2025

  33. [33]

    , author Wechsler, R.H

    author Conroy, C. , author Wechsler, R.H. , year 2009 . title Connecting Galaxies, Halos, and Star Formation Rates Across Cosmic Time . journal Astrophys. J. volume 696 , pages 620--635 . :10.1088/0004-637X/696/1/620, http://arxiv.org/abs/0805.3346 arXiv:0805.3346

    work page doi:10.1088/0004-637x/696/1/620 2009

  34. [34]

    , author Ren, Z

    author Costa, A.A. , author Ren, Z. , author Yin, Z. , year 2023 . title A bias using the ages of the oldest astrophysical objects to address the Hubble tension . journal Eur. Phys. J. C volume 83 , pages 875 . :10.1140/epjc/s10052-023-12038-0, http://arxiv.org/abs/2306.01234 arXiv:2306.01234

    work page doi:10.1140/epjc/s10052-023-12038-0 2023

  35. [35]

    MNRAS424(1), 65–79 (2012) https://doi.org/10.1111/j.1365-2966.2012.21152.x arXiv:1204.5474 [astro-ph.GA]

    author Cui, W. , author Borgani, S. , author Dolag, K. , author Murante, G. , author Tornatore, L. , year 2012 . title The effects of baryons on the halo mass function . journal Mon. Not. Roy. Astron. Soc. volume 423 , pages 2279 . :10.1111/j.1365-2966.2012.21037.x, http://arxiv.org/abs/1111.3066 arXiv:1111.3066

    work page doi:10.1111/j.1365-2966.2012.21037.x 2012

  36. [36]

    , author Mondol, R

    author Das, S. , author Mondol, R. , author Singh, A. , author Laha, R. , year 2025 . title Dark Secrets of Baryons: Illuminating Dark Matter-Baryon Interactions with JWST http://arxiv.org/abs/2511.02906 arXiv:2511.02906

    work page arXiv 2025

  37. [37]

    , author Giri, S.K

    author Dayal, P. , author Giri, S.K. , year 2024 . title Warm dark matter constraints from the JWST . journal Mon. Not. Roy. Astron. Soc. volume 528 , pages 2784--2789 . :10.1093/mnras/stae176, http://arxiv.org/abs/2303.14239 arXiv:2303.14239

    work page doi:10.1093/mnras/stae176 2024

  38. [38]

    2023, MNRAS, 523, 3201, doi: 10.1093/mnras/stad1557

    author Dekel, A. , author Sarkar, K.C. , author Birnboim, Y. , author Mandelker, N. , author Li, Z. , year 2023 . title Efficient formation of massive galaxies at cosmic dawn by feedback-free starbursts . journal Mon. Not. Roy. Astron. Soc. volume 523 , pages 3201--3218 . :10.1093/mnras/stad1557, http://arxiv.org/abs/2303.04827 arXiv:2303.04827

    work page doi:10.1093/mnras/stad1557 2023

  39. [39]

    , author Alsing, J

    author Dhawan, S. , author Alsing, J. , author Vagnozzi, S. , year 2021 . title Non-parametric spatial curvature inference using late-Universe cosmological probes . journal Mon. Not. Roy. Astron. Soc. volume 506 , pages L1--L5 . :10.1093/mnrasl/slab058, http://arxiv.org/abs/2104.02485 arXiv:2104.02485

    work page doi:10.1093/mnrasl/slab058 2021

  40. [40]

    , author Melchiorri, A

    author Di Valentino, E. , author Melchiorri, A. , author Mena, O. , author Pan, S. , author Yang, W. , year 2021 a. title Interacting Dark Energy in a closed universe . journal Mon. Not. Roy. Astron. Soc. volume 502 , pages L23--L28 . :10.1093/mnrasl/slaa207, http://arxiv.org/abs/2011.00283 arXiv:2011.00283

    work page doi:10.1093/mnrasl/slaa207 2021

  41. [41]

    Planck evidence for a closed Universe and a possible crisis for cosmology

    author Di Valentino, E. , author Melchiorri, A. , author Silk, J. , year 2019 . title Planck evidence for a closed Universe and a possible crisis for cosmology . journal Nature Astron. volume 4 , pages 196--203 . :10.1038/s41550-019-0906-9, http://arxiv.org/abs/1911.02087 arXiv:1911.02087

    work page doi:10.1038/s41550-019-0906-9 2019

  42. [42]

    Investigating Cosmic Discordance

    author Di Valentino, E. , author Melchiorri, A. , author Silk, J. , year 2021 b. title Investigating Cosmic Discordance . journal Astrophys. J. Lett. volume 908 , pages L9 . :10.3847/2041-8213/abe1c4, http://arxiv.org/abs/2003.04935 arXiv:2003.04935

    work page doi:10.3847/2041-8213/abe1c4 2021

  43. [43]

    author Di Valentino, E. , et al. ( collaboration CosmoVerse Network ), year 2025 . title The CosmoVerse White Paper: Addressing observational tensions in cosmology with systematics and fundamental physics . journal Phys. Dark Univ. volume 49 , pages 101965 . :10.1016/j.dark.2025.101965, http://arxiv.org/abs/2504.01669 arXiv:2504.01669

    work page doi:10.1016/j.dark.2025.101965 2025

  44. [44]

    , year 2022

    author Dinda, B.R. , year 2022 . title Cosmic expansion parametrization: Implication for curvature and H0 tension . journal Phys. Rev. D volume 105 , pages 063524 . :10.1103/PhysRevD.105.063524, http://arxiv.org/abs/2106.02963 arXiv:2106.02963

    work page doi:10.1103/physrevd.105.063524 2022

  45. [45]

    , author Wu, P.J

    author Du, G.H. , author Wu, P.J. , author Li, T.N. , author Zhang, X. , year 2025 . title Impacts of dark energy on weighing neutrinos after DESI BAO . journal Eur. Phys. J. C volume 85 , pages 392 . :10.1140/epjc/s10052-025-14094-0, http://arxiv.org/abs/2407.15640 arXiv:2407.15640

    work page doi:10.1140/epjc/s10052-025-14094-0 2025

  46. [46]

    The evidence for a spatially flat Universe

    author Efstathiou, G. , author Gratton, S. , year 2020 . title The evidence for a spatially flat Universe . journal Mon. Not. Roy. Astron. Soc. volume 496 , pages L91--L95 . :10.1093/mnrasl/slaa093, http://arxiv.org/abs/2002.06892 arXiv:2002.06892

    work page doi:10.1093/mnrasl/slaa093 2020

  47. [47]

    u tsi, G. , author Urrutia, J. , author Vaskonen, V. , author Veerm \

    author Ellis, J. , author Fairbairn, M. , author H \"u tsi, G. , author Urrutia, J. , author Vaskonen, V. , author Veerm \"a e, H. , year 2024 . title Consistency of JWST black hole observations with NANOGrav gravitational wave measurements . journal Astron. Astrophys. volume 691 , pages A270 . :10.1051/0004-6361/202450846, http://arxiv.org/abs/2403.19650...

    work page doi:10.1051/0004-6361/202450846 2024

  48. [48]

    , author Giar \`e , W

    author Escamilla, L.A. , author Giar \`e , W. , author Di Valentino, E. , author Nunes, R.C. , author Vagnozzi, S. , year 2024 . title The state of the dark energy equation of state circa 2023 . journal JCAP volume 05 , pages 091 . :10.1088/1475-7516/2024/05/091, http://arxiv.org/abs/2307.14802 arXiv:2307.14802

    work page doi:10.1088/1475-7516/2024/05/091 2024

  49. [49]

    , author Salmani, R.V

    author Fakhry, S. , author Salmani, R.V. , author Firouzjaee, J.T. , year 2025 . title High-redshift galaxies from JWST observations in more realistic dark matter halo models . journal Phys. Rev. D volume 112 , pages 123503 . :10.1103/9cmb-kf3x, http://arxiv.org/abs/2507.23742 arXiv:2507.23742

    work page doi:10.1103/9cmb-kf3x 2025

  50. [50]

    , author Shiravand, M

    author Fakhry, S. , author Shiravand, M. , author Del Popolo, A. , year 2026 . title Matching JWST Ultraviolet Luminosity Functions with Refined CDM Halo Models . journal Astrophys. J. volume 998 , pages 178 . :10.3847/1538-4357/ae371b, http://arxiv.org/abs/2510.04709 arXiv:2510.04709

    work page doi:10.3847/1538-4357/ae371b 2026

  51. [51]

    , author G\'omez-Valent, A

    author Favale, A. , author G\'omez-Valent, A. , author Migliaccio, M. , year 2023 . title Cosmic chronometers to calibrate the ladders and measure the curvature of the Universe. A model-independent study . journal Mon. Not. Roy. Astron. Soc. volume 523 , pages 3406--3422 . :10.1093/mnras/stad1621, http://arxiv.org/abs/2301.09591 arXiv:2301.09591

    work page doi:10.1093/mnras/stad1621 2023

  52. [52]

    , author Li, T.N

    author Feng, L. , author Li, T.N. , author Du, G.H. , author Zhang, J.F. , author Zhang, X. , year 2026 . title Measuring neutrino mass in light of ACT DR6 and DESI DR2 . journal Phys. Dark Univ. volume 52 , pages 102296 . :10.1016/j.dark.2026.102296, http://arxiv.org/abs/2603.10787 arXiv:2603.10787

    work page doi:10.1016/j.dark.2026.102296 2026

  53. [53]

    2023, MNRAS, 522, 3986, doi: 10.1093/mnras/stad1095

    author Ferrara, A. , author Pallottini, A. , author Dayal, P. , year 2023 . title On the stunning abundance of super-early, luminous galaxies revealed by JWST . journal Mon. Not. Roy. Astron. Soc. volume 522 , pages 3986--3991 . :10.1093/mnras/stad1095, http://arxiv.org/abs/2208.00720 arXiv:2208.00720

    work page doi:10.1093/mnras/stad1095 2023

  54. [54]

    , author DI Valentino, E

    author Forconi, M. , author DI Valentino, E. , year 2025 . title One extension to explain them all, one scale-invariant spectrum to test them all, and in one model bind them . journal Phys. Dark Univ. volume 48 , pages 101904 . :10.1016/j.dark.2025.101904, http://arxiv.org/abs/2503.04705 arXiv:2503.04705

    work page doi:10.1016/j.dark.2025.101904 2025

  55. [55]

    , author Giar \`e , W

    author Forconi, M. , author Giar \`e , W. , author Mena, O. , author Ruchika , author Di Valentino, E. , author Melchiorri, A. , author Nunes, R.C. , year 2024 . title A double take on early and interacting dark energy from JWST . journal JCAP volume 05 , pages 097 . :10.1088/1475-7516/2024/05/097, http://arxiv.org/abs/2312.11074 arXiv:2312.11074

    work page doi:10.1088/1475-7516/2024/05/097 2024

  56. [56]

    , author Ruchika , author Melchiorri, A

    author Forconi, M. , author Ruchika , author Melchiorri, A. , author Mena, O. , author Menci, N. , year 2023 . title Do the early galaxies observed by JWST disagree with Planck's CMB polarization measurements? journal JCAP volume 10 , pages 012 . :10.1088/1475-7516/2023/10/012, http://arxiv.org/abs/2306.07781 arXiv:2306.07781

    work page doi:10.1088/1475-7516/2023/10/012 2023

  57. [57]

    W., Lang, D., & Goodman, J

    author Foreman-Mackey, D. , author Hogg, D.W. , author Lang, D. , author Goodman, J. , year 2013 . title emcee: The MCMC Hammer . journal Publ. Astron. Soc. Pac. volume 125 , pages 306--312 . :10.1086/670067, http://arxiv.org/abs/1202.3665 arXiv:1202.3665

    work page doi:10.1086/670067 2013

  58. [58]

    , author Lapi, A

    author Gandolfi, G. , author Lapi, A. , author Ronconi, T. , author Danese, L. , year 2022 . title Astroparticle Constraints from the Cosmic Star Formation Rate Density at High Redshift: Current Status and Forecasts for JWST . journal Universe volume 8 , pages 589 . :10.3390/universe8110589, http://arxiv.org/abs/2211.02840 arXiv:2211.02840

    work page doi:10.3390/universe8110589 2022

  59. [59]

    , keywords =

    author Gardner, J.P. , et al., year 2006 . title The James Webb Space Telescope . journal Space Sci. Rev. volume 123 , pages 485 . :10.1007/s11214-006-8315-7, http://arxiv.org/abs/astro-ph/0606175 arXiv:astro-ph/0606175

    work page doi:10.1007/s11214-006-8315-7 2006

  60. [60]

    Giarè, Dynamical Dark Energy Beyond Planck? Constraints from multiple CMB probes, DESI BAO and Type-Ia Supernovae, Phys

    author Giar \`e , W. , year 2025 . title Dynamical dark energy beyond Planck? Constraints from multiple CMB probes, DESI BAO, and type-Ia supernovae . journal Phys. Rev. D volume 112 , pages 023508 . :10.1103/ss37-cxhn, http://arxiv.org/abs/2409.17074 arXiv:2409.17074

    work page doi:10.1103/ss37-cxhn 2025

  61. [61]

    , author Di Valentino, E

    author Giar\`e, W. , author Di Valentino, E. , author Melchiorri, A. , year 2024 . title Measuring the reionization optical depth without large-scale CMB polarization . journal Phys. Rev. D volume 109 , pages 103519 . :10.1103/PhysRevD.109.103519, http://arxiv.org/abs/2312.06482 arXiv:2312.06482

    work page doi:10.1103/physrevd.109.103519 2024

  62. [62]

    , author Mahassen, T

    author Giar \`e , W. , author Mahassen, T. , author Di Valentino, E. , author Pan, S. , year 2025 . title An overview of what current data can (and cannot yet) say about evolving dark energy . journal Phys. Dark Univ. volume 48 , pages 101906 . :10.1016/j.dark.2025.101906, http://arxiv.org/abs/2502.10264 arXiv:2502.10264

    work page doi:10.1016/j.dark.2025.101906 2025

  63. [63]

    Giar` e, M

    author Giar \`e , W. , author Najafi, M. , author Pan, S. , author Di Valentino, E. , author Firouzjaee, J.T. , year 2024 a. title Robust preference for Dynamical Dark Energy in DESI BAO and SN measurements . journal JCAP volume 10 , pages 035 . :10.1088/1475-7516/2024/10/035, http://arxiv.org/abs/2407.16689 arXiv:2407.16689

    work page doi:10.1088/1475-7516/2024/10/035 2024

  64. [64]

    Giar` e, M

    author Giar \`e , W. , author Sabogal, M.A. , author Nunes, R.C. , author Di Valentino, E. , year 2024 b. title Interacting Dark Energy after DESI Baryon Acoustic Oscillation Measurements . journal Phys. Rev. Lett. volume 133 , pages 251003 . :10.1103/PhysRevLett.133.251003, http://arxiv.org/abs/2404.15232 arXiv:2404.15232

    work page doi:10.1103/physrevlett.133.251003 2024

  65. [65]

    Full-shape galaxy power spectra and the curvature tension

    author Glanville, A. , author Howlett, C. , author Davis, T.M. , year 2022 . title Full-shape galaxy power spectra and the curvature tension . journal Mon. Not. Roy. Astron. Soc. volume 517 , pages 3087--3100 . :10.1093/mnras/stac2891, http://arxiv.org/abs/2205.05892 arXiv:2205.05892

    work page doi:10.1093/mnras/stac2891 2022

  66. [66]

    , author Benetti, M

    author Gonzalez, J.E. , author Benetti, M. , author von Marttens, R. , author Alcaniz, J. , year 2021 . title Testing the consistency between cosmological data: the impact of spatial curvature and the dark energy EoS . journal JCAP volume 11 , pages 060 . :10.1088/1475-7516/2021/11/060, http://arxiv.org/abs/2104.13455 arXiv:2104.13455

    work page doi:10.1088/1475-7516/2021/11/060 2021

  67. [67]

    Cosmological preference for a negative neutrino mass

    author Green, D. , author Meyers, J. , year 2025 . title Cosmological preference for a negative neutrino mass . journal Phys. Rev. D volume 111 , pages 083507 . :10.1103/PhysRevD.111.083507, http://arxiv.org/abs/2407.07878 arXiv:2407.07878

    work page doi:10.1103/physrevd.111.083507 2025

  68. [68]

    , author Khlopov, M

    author Guo, S.Y. , author Khlopov, M. , author Liu, X. , author Wu, L. , author Wu, Y. , author Zhu, B. , year 2024 . title Footprints of axion-like particle in pulsar timing array data and James Webb Space Telescope observations . journal Sci. China Phys. Mech. Astron. volume 67 , pages 111011 . :10.1007/s11433-024-2445-1, http://arxiv.org/abs/2306.17022...

    work page doi:10.1007/s11433-024-2445-1 2024

  69. [69]

    , year 2023

    author Gupta, R.P. , year 2023 . title JWST early Universe observations and CDM cosmology . journal Mon. Not. Roy. Astron. Soc. volume 524 , pages 3385--3395 . :10.1093/mnras/stad2032, http://arxiv.org/abs/2309.13100 arXiv:2309.13100

    work page doi:10.1093/mnras/stad2032 2023

  70. [70]

    Curvature tension: evidence for a closed universe

    author Handley, W. , year 2021 . title Curvature tension: evidence for a closed universe . journal Phys. Rev. D volume 103 , pages L041301 . :10.1103/PhysRevD.103.L041301, http://arxiv.org/abs/1908.09139 arXiv:1908.09139

    work page doi:10.1103/physrevd.103.l041301 2021

  71. [71]

    , author Kroupa, P

    author Haslbauer, M. , author Kroupa, P. , author Zonoozi, A.H. , author Haghi, H. , year 2022 . title Has JWST Already Falsified Dark-matter-driven Galaxy Formation? journal Astrophys. J. Lett. volume 939 , pages L31 . :10.3847/2041-8213/ac9a50, http://arxiv.org/abs/2210.14915 arXiv:2210.14915

    work page doi:10.3847/2041-8213/ac9a50 2022

  72. [72]

    , author Wyatt, M.M

    author Hegde, S. , author Wyatt, M.M. , author Furlanetto, S.R. , year 2024 . title A hidden population of active galactic nuclei can explain the overabundance of luminous z > 10 objects observed by JWST . journal JCAP volume 08 , pages 025 . :10.1088/1475-7516/2024/08/025, http://arxiv.org/abs/2405.01629 arXiv:2405.01629

    work page doi:10.1088/1475-7516/2024/08/025 2024

  73. [73]

    , author Cai, Y

    author Huang, H.L. , author Cai, Y. , author Jiang, J.Q. , author Zhang, J. , author Piao, Y.S. , year 2024 a. title Supermassive Primordial Black Holes for Nano-Hertz Gravitational Waves and High-redshift JWST Galaxies . journal Res. Astron. Astrophys. volume 24 , pages 091001 . :10.1088/1674-4527/ad683d, http://arxiv.org/abs/2306.17577 arXiv:2306.17577

    work page doi:10.1088/1674-4527/ad683d 2024

  74. [74]

    , author Jiang, J.Q

    author Huang, H.L. , author Jiang, J.Q. , author Piao, Y.S. , year 2024 b. title High-redshift JWST massive galaxies and the initial clustering of supermassive primordial black holes . journal Phys. Rev. D volume 110 , pages 103540 . :10.1103/PhysRevD.110.103540, http://arxiv.org/abs/2407.15781 arXiv:2407.15781

    work page doi:10.1103/physrevd.110.103540 2024

  75. [75]

    u tsi, G. , author Raidal, M. , author Urrutia, J. , author Vaskonen, V. , author Veerm \

    author H \"u tsi, G. , author Raidal, M. , author Urrutia, J. , author Vaskonen, V. , author Veerm \"a e, H. , year 2023 . title Did JWST observe imprints of axion miniclusters or primordial black holes? journal Phys. Rev. D volume 107 , pages 043502 . :10.1103/PhysRevD.107.043502, http://arxiv.org/abs/2211.02651 arXiv:2211.02651

    work page doi:10.1103/physrevd.107.043502 2023

  76. [76]

    Indications of a top-heavy initial mass function in highly star-forming galaxies from JWST observations at z > 10

    author Hutter, A. , author Cueto, E.R. , author Dayal, P. , author Gottl \"o ber, S. , author Trebitsch, M. , author Yepes, G. , year 2025 . title ASTRAEUS - X. Indications of a top-heavy initial mass function in highly star-forming galaxies from JWST observations at z > 10 . journal Astron. Astrophys. volume 694 , pages A254 . :10.1051/0004-6361/20245246...

    work page doi:10.1051/0004-6361/202452460 2025

  77. [77]

    , author Paulin, J

    author Ilie, C. , author Paulin, J. , author Freese, K. , year 2023 . title Supermassive Dark Star candidates seen by JWST . journal Proc. Nat. Acad. Sci. volume 120 , pages e2305762120 . :10.1073/pnas.2305762120, http://arxiv.org/abs/2304.01173 arXiv:2304.01173

    work page doi:10.1073/pnas.2305762120 2023

  78. [78]

    Physics of the Dark Universe , keywords =

    author Iocco, F. , author Visinelli, L. , year 2024 . title Compatibility of JWST results with exotic halos . journal Phys. Dark Univ. volume 44 , pages 101496 . :10.1016/j.dark.2024.101496, http://arxiv.org/abs/2403.13068 arXiv:2403.13068

    work page doi:10.1016/j.dark.2024.101496 2024

  79. [79]

    , author Giar \`e , W

    author Jiang, J.Q. , author Giar \`e , W. , author Gariazzo, S. , author Dainotti, M.G. , author Di Valentino, E. , author Mena, O. , author Pedrotti, D. , author da Costa, S.S. , author Vagnozzi, S. , year 2025 a. title Neutrino cosmology after DESI: tightest mass upper limits, preference for the normal ordering, and tension with terrestrial observations...

    work page doi:10.1088/1475-7516/2025/01/153 2025

  80. [80]

    , author Liu, W

    author Jiang, J.Q. , author Liu, W. , author Zhan, H. , author Hu, B. , year 2025 b. title Explanation of high redshift luminous galaxies from JWST by an early dark energy model . journal Phys. Rev. D volume 111 , pages 023519 . :10.1103/PhysRevD.111.023519, http://arxiv.org/abs/2409.19941 arXiv:2409.19941

    work page doi:10.1103/physrevd.111.023519 2025

Showing first 80 references.