Phase Wave Cosmology

We present Phase Wave Cosmology (PWC), a continuous single-fluid framework that replaces separate cold dark matter particles and dark energy vacuum fields with a mass-energy fluid medium undergoing thermodynamic phase relaxation. Using first-law thermodynamic conservation (∇_μ T^{μν} = 0), we show that an infinitely smooth (C^∞) double-hyperbolic tangent equation of state w(a) maintains true 0.0000% energy conservation violation across seven orders of magnitude in scale factor (a ∈ [10^-7, 1.0]), resolving the 10^120 quantum field theory vacuum energy problem. Integrating linear perturbations over this smooth background with fluid shear viscosity (ν_0 = 5.0 × 10^26 m^2/s) yields k^2 scale-dependent damping that reduces the top-hat window variance σ_8 by 4.12%, shifting S_8 = 0.797 ± 0.008 and resolving the 3σ weak lensing tension. Intrinsic field kinetics yields a microscopic cross-section σ/m = c_s / (3 ρ ν_0) = 0.10 cm^2/g, satisfying Bullet Cluster bounds (σ/m < 0.13 cm^2/g) without arbitrary macroscopic length scales. We define quantitative Popperian falsification criteria for Stage IV surveys (Simons Observatory, Euclid, Rubin LSST, JWST) and present a mock likelihood parameter forecast for Planck 2018 + KiDS-1000.

Authors

Publication Details

Journal
Zenodo (CERN European Organization for Nuclear Research)
Published
2026-07-28
DOI
https://doi.org/10.5281/zenodo.21642519
Primary Topic
Cosmology and Gravitation Theories
Type
preprint
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preprint

Phase Wave Cosmology

Jaden Allison
Zenodo (CERN European Organization for Nuclear Research)
Cosmology and Gravitation Theories
preprint

Phase Wave Cosmology

Jaden Allison
preprint en

Abstract

We present Phase Wave Cosmology (PWC), a continuous single-fluid framework that replaces separate cold dark matter particles and dark energy vacuum fields with a mass-energy fluid medium undergoing thermodynamic phase relaxation. Using first-law thermodynamic conservation (∇_μ T^{μν} = 0), we show that an infinitely smooth (C^∞) double-hyperbolic tangent equation of state w(a) maintains true 0.0000% energy conservation violation across seven orders of magnitude in scale factor (a ∈ [10^-7, 1.0]), resolving the 10^120 quantum field theory vacuum energy problem. Integrating linear perturbations over this smooth background with fluid shear viscosity (ν_0 = 5.0 × 10^26 m^2/s) yields k^2 scale-dependent damping that reduces the top-hat window variance σ_8 by 4.12%, shifting S_8 = 0.797 ± 0.008 and resolving the 3σ weak lensing tension. Intrinsic field kinetics yields a microscopic cross-section σ/m = c_s / (3 ρ ν_0) = 0.10 cm^2/g, satisfying Bullet Cluster bounds (σ/m < 0.13 cm^2/g) without arbitrary macroscopic length scales. We define quantitative Popperian falsification criteria for Stage IV surveys (Simons Observatory, Euclid, Rubin LSST, JWST) and present a mock likelihood parameter forecast for Planck 2018 + KiDS-1000.

Zenodo (CERN European Organization for Nuclear Research)
Life in Land
Cosmology and Gravitation Theories
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