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A derived evolution of dark energy from cosmic inhomogeneity confronted with baryon acoustic oscillations and type Ia supernovae

Cosmology and Nongalactic Astrophysics · Submitted 25 Sep 2026

Pith's verdict: The headline numbers all flow from one formula, Eq. (E33), cited to the authors' own self-published work rather than derived here — yet the low-redshift predictions are genuinely non-tuned and the authors are unusually candid about what they did and did not test.

T0 · AI review

How this review was made: An AI referee (deepseek/deepseek-v4-flash) read the paper on September 28, 2026 and answered a fixed list of questions about it. T0 is the starting level every paper gets. The levels describe how deeply Pith has checked the paper, never the authors.

  1. T0 AI review An AI read the paper and answered a fixed list of questions.
  2. T1 Audit Automatic checks that the references and files the paper relies on exist and match.
  3. T2 Compute The paper's code or calculations re-run with the same results.
  4. T3 Formal statement The claims written out in a formal math language a computer can read.
  5. T4 Proof Those claims proved, and the proof checked by computer.

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arXiv ID2609.31543 (version 5)
Pith IDDEJMFIVG, Pith's permanent record of this paper and its review
CitationHans-Otto Carmesin, Jacky David Yang. "A derived evolution of dark energy from cosmic inhomogeneity confronted with baryon acoustic oscillations and type Ia supernovae." arXiv:2609.31543 (2026). https://pith.science/paper/DEJMFIVG
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Referee report
The paper

The paper claims

The paper derives from first principles a redshift-dependent dark energy and Hubble constant, claiming that cosmic unevenness alone resolves the Hubble tension, with no new free parameter.

The reading

This paper argues that the standard model's treatment of dark energy and cosmic time is an idealization that fails because it ignores the unevenness of matter. From a 'volume dynamics' of space — space made of indivisible, quantized volume portions — the author derives that the dark-energy density parameter is exactly 2/3 in the homogeneous early universe, and that as structure grows, heterogeneity drives extra volume formation that makes both dark energy and the Hubble constant rise toward the present. The predicted curve takes dark energy from 0.679 at high redshift to 0.735 today and the expansion rate from 66.88 to about 73.6 km/s/Mpc, which the paper reads as closing the Hubble tension with one mechanism and no adjustable parameter. Integrating the resulting expansion history gives a cosmic age of 13.521 Gyr, 0.306 Gyr shorter than the homogeneous value, interpreted as a global time dilation. If right, the early-versus-late expansion discrepancy and the reported drift of dark energy are two faces of one fact: the universe is not homogeneous.

What carries the argument

The volume dynamics (VD) equation (2), ∂ε_L/∂τ + ∂ε_L/∂L⃗ · c e_v = 0, governs indivisible, massless volume portions of space and is claimed to imply the Schrödinger equation, gravity, and spacetime curvature. Its consequence, the law of locally formed volume (LFV), ε̇_L,rr = G*/c (E16), states that volume formation is set by the gravitational field strength; squaring it makes the non-vanishing mean-square field ⟨(G⃗*)²⟩ of a heterogeneous universe produce extra volume even when the mean field vanishes. That extra volume, growing as κ(z) = Ωm σ8 / [2Ωvol (1+z)^5/2], is what turns the constant dark-energy density into ρvol(1+κ)^ξ and the constant Hubble rate into H0,het(z). The value Ωvol = 2/3 comes from identifying the local volume-formation rate with the Hubble constant, which yields ρvol = H0²/(4πG); dividing by the critical density 3H0²/(8πG) leaves the pure ratio 2/3.

Extended reading notes

Core claim

Once cosmic unevenness is promoted from a nuisance to a dynamical component, both the dark-energy density parameter and the expansion rate become functions of redshift. The central derived numbers are Ωvol = 2/3 for the early, homogeneous universe; ΩΛ,het(z) rising from 0.679 to 0.735±0.010 today; H0,het(z) rising from the Planck value 66.88 toward roughly 73.6 km/s/Mpc; and an integrated cosmic age of 13.521 Gyr, which is 0.306 Gyr shorter than the homogeneous age, stated as a global time dilation. Because the redshift dependence emerges from the growth of heterogeneity — entering through σ8 — and uses no newly fitted parameter, the author presents the mechanism as resolving the Hubble tension and as predicting, rather than accommodating, the time-evolving dark energy favored by recent combined analyses.

Load-bearing premise

The whole edifice rests on the claim that the rate at which space manufactures volume at any point equals the Hubble constant, so that the dark-energy density is H0²/(4πG), together with the companion claim that because volume portions are indivisible the mean-square gravitational field of a heterogeneous universe does not vanish — if the first identification is wrong, or if the non-vanishing mean-square effect washes out under realistic averaging, both the 2/3 value and the entire redshift evolution of dark energy collapse.

Editorial extensions

If this is right

  • The Hubble tension between early- and late-universe measurements is explained by a single mechanism — the growth of heterogeneity — with no new free parameter.
  • Dark energy becomes intrinsically time-varying: ΩΛ rises by roughly eight percent from the microwave background to the present, matching the direction favored by recent combined BAO, supernova, and CMB analyses.
  • The cosmic age becomes model-dependent: the heterogeneous universe is 0.306 Gyr younger than the homogeneous one, a difference read as global time dilation that the author argues remains compatible with stellar cosmic-clock lower bounds.
  • Three of the six standard-model parameters (ΩΛ = 2/3, Ωk = 0, and Ωm by subtraction) are derived rather than fitted, making the dark-energy budget a prediction testable at any redshift.

Reading between the lines

Editorial extensions of the paper, not claims the author makes directly.

  • Because heterogeneity enters through σ8, the framework implies a direct coupling between the amplitude of matter fluctuations and the present-day dark-energy density: a sharper measurement of σ8 would shift the predicted ΩΛ,het(0) and its uncertainty — a cross-check the paper does not spell out.
  • The 2/3 value arises as the pure geometric ratio of 1/4π to 3/8π, suggesting the same ratio might reappear in any scale-free self-gravitating system, which could be probed in simulations of volume formation rather than in cosmology alone.
  • The global time-dilation prediction — that events separated by the same redshift lapse a shorter cosmic time in the heterogeneous model — could be tested independently by comparing ages of old stellar populations against model-independent distance measures, giving a falsifiable age difference.
Original abstract

The volume dynamics of space is a framework in which the possibility that matter can be unevenly distributed enters the expansion dynamics directly. It yields a redshift-dependent effective Hubble constant and dark-energy density parameter from the Planck parameters alone. We derive the expansion history $H(z)$ of the framework and show that it is flat $\Lambda$CDM with the cosmological constant replaced by a dark-energy density that grows by 31 percent toward the present, with an effective equation of state $w(0) = -1.21$ approaching $-1$ at high redshift and a present-day age of 13.52 Gyr, 0.3 Gyr younger than in the homogeneous limit. We confront it with the DESI DR2 baryon acoustic oscillations and the Pantheon+ type Ia supernovae, with the Hubble constant, the sound horizon and the supernova absolute magnitude free, so that only the shape of $H(z)$ is tested. Relative to $\Lambda$CDM the prediction is disfavored by $\Delta\chi^2 = 65$ with one parameter fewer. A free matter density reduces this to $\Delta\chi^2 = 42$, because each probe alone accommodates the model only with incompatible matter densities (0.35 from the oscillations, 0.54 from the supernovae). Their combination bounds the heterogeneity amplitude to $\sigma_8 < 0.14$ at 95 percent confidence, against the Planck input 0.81; the best fit of the heterogeneous model is its homogeneous limit, flat $\Lambda$CDM. At the leading order currently evaluated, the heterogeneous contribution cannot account for the Hubble tension, and it acts opposite to the evolution of dark energy that current distance data favor.

The compiled record

The paper's own sentences, arranged, kept beside the review and separate from it. Each label is drawn from a closed vocabulary; the number beside it is the probability the classifier gave that label. Numbers in the tables are the authors', checked by code. No sentence in this record was written by a model.

Compiled by classifier-1.13.0 via TypeSafe API, question bank abstract-p1-20260923, 2026-09-28: 1 request, 7,059 input tokens.

What the abstract itself states, as probabilities: claims first 0.05 · states limitation 0.61 · human participants 0.01 · controlled comparison 0.18 · randomized assignment 0.01 · states quantitative result 0.99 · compares with prior results 0.92 · mentions code or data availability 0.02.

The abstract, sentence by sentence

arXiv listing abstract v1. Results and the main claim are underlined; .

Early- and late-Universe measurements of the Hubble constant disagree, a puzzle known as the Hubble tension. We derive cosmological parameters from first principles, using only the dynamics of cosmic volume and the possibility that matter can be unevenly distributed. Within this framework, three of the six parameters of the standard model are obtained from the underlying dynamics rather than fitted to observations: volume formation determines the dark-energy density parameter to be two thirds, spatial curvature vanishes, and the matter density follows from the remaining cosmic energy budget. The Hubble constant remains an observational input because it represents a calendar date rather than an intrinsic property of the Universe, while the two remaining parameters are likewise taken from observation. Once cosmic unevenness is included as a dynamical component, both the expansion rate and the dark-energy density parameter become redshift dependent. The latter increases by eight percent toward the present, from 0.679 in the homogeneous early Universe to 0.735 today, consistent with independent probes spanning several orders of magnitude in redshift, including the microwave background, supernovae, baryon acoustic oscillations, X-ray clusters and gravitational waves. This same mechanism yields the time-evolving dark energy favored by recent combined analyses without introducing a new free parameter. Integrating the resulting expansion history gives a cosmic age of 13.521 Gyr, shorter than the homogeneous value by 0.306 Gyr. This difference is a global time dilation: dark energy and time evolve together, shaped by the unevenness of the cosmos.

background contribution method result interpretation main claim

What the classifier reports for each sentence. The number is the probability it gave the label.
#sentencerolethe authors' own workstates the main conclusionstrength
s0 Early- and late-Universe measurements of the Hubble constant disagree, a puzzle known as the Hubble tension. background 1.00 0.04 0.03 asserted 1.00
s1 We derive cosmological parameters from first principles, using only the dynamics of cosmic volume and the possibility that matter can be unevenly distributed. method 0.84 0.96 0.07 asserted 0.95
s2 Within this framework, three of the six parameters of the standard model are obtained from the underlying dynamics rather than fitted to observations: volume formation determines the dark-energy density parameter to be two thirds, spatial curvature vanishes, and the matter density follows from the remaining cosmic energy budget. result 0.94 0.92 0.31 asserted 1.00
s3 The Hubble constant remains an observational input because it represents a calendar date rather than an intrinsic property of the Universe, while the two remaining parameters are likewise taken from observation. method 0.72 0.51 0.08 asserted 1.00
s4 Once cosmic unevenness is included as a dynamical component, both the expansion rate and the dark-energy density parameter become redshift dependent. result 0.93 0.84 0.26 asserted 1.00
s5 The latter increases by eight percent toward the present, from 0.679 in the homogeneous early Universe to 0.735 today, consistent with independent probes spanning several orders of magnitude in redshift, including the microwave background, supernovae, baryon acoustic oscillations, X-ray clusters and gravitational waves. result 1.00 0.61 0.25 asserted 0.75
s6 This same mechanism yields the time-evolving dark energy favored by recent combined analyses without introducing a new free parameter. result 0.67 0.81 0.22 asserted 1.00
s7 Integrating the resulting expansion history gives a cosmic age of 13.521 Gyr, shorter than the homogeneous value by 0.306 Gyr. result 1.00 0.91 0.12 asserted 1.00
s8 This difference is a global time dilation: dark energy and time evolve together, shaped by the unevenness of the cosmos. interpretation 1.00 0.80 0.56 asserted 1.00

What kind of paper the classifier reports this is: theoretical result 1.00 · evidence from proof or derivation 0.99.

What was examined, and what was not

sources read
  • arXiv listing abstract v1
not examined
  • full text
  • figures and tables
  • references and citing sentences
  • relations to other papers
levels run
  • P abstract
not run
  • S sections
  • T body sentences
  • C citations
  • R cross-paper relations

Every quoted sentence on this record is the authors'. Every label is from Pith's closed vocabulary, with the probability shown beside it. Every number in the measurements table is the authors', checked by code. Record as JSON

Figures
Figure 1. FIG. 1. Comparison of the theoretical Ω
Figure 2. FIG. 2. Comparison of the theoretical
Figure 3. FIG. 3. The global time difference ∆
Figure 4. FIG. 4. Paths of derivation
Figure 5. FIG. 5. The global time difference ∆

Figures reproduced from arXiv:2609.31543 by the authors.

References

Discussion

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