Baryonic Horizon Dynamics Across z ∈ [0.01, 2.30]: Resolving Late-Time Cosmic Acceleration and the Type Ia Supernova Distance Modulus Without a Cosmological Constant (Λ)

AbstractThe observed dimming of high-redshift Type Ia supernovae (SN Ia) [1–4] and BaryonAcoustic Oscillation (BAO) expansion history [5] across z ∈ [0.01, 2.30] require, withinstandard ΛCDM cosmology, that approximately 70% of the cosmic energy budget residein an unexplained cosmological constant (Λ / Dark Energy) alongside ∼ 25% non-baryonicCold Dark Matter. Completing our three-scale cosmology trilogy [6,7], we formulate a hybridCausal State-Space Spectral Integrator (CSSI) combining a gated causal state-transitionpropagator with a 16-mode 1D spectral Fourier convolution kernel constrained by the 5Dtrans-brane restoring stress-energy tensor TEPR (z, w) [8]. By formulating the causal state-transition propagator entirely from analytical, twice-differentiable operators across Nz = 300native redshift nodes (z ∈ [0.01, 2.30]), we evaluate exact second-order variational derivativesof the bulk attenuation PDE (∂TEPR /∂w + λTEPR = 0). Whereas the unconditioned baselinecollapses with an expansion rate error of RMSE = 128.20 km/s/Mpc, the stabilized solver(incorporating the ‘/1000.0‘ Friedmann equilibrium residual divisor, 10−11 horizon massscaling, λ = 8.2390 bulk attenuation lock, and hard-wired Heaviside-linear positivity projectorP+ ) converges to RMSE = 0.03 km/s/Mpc (R2 = 1.0000) for the Hubble parameter H(z)and RMSE = 0.0001 mag (R2 = 1.0000) for the Type Ia supernova distance modulus µ(z),utilizing a strictly baryonic matter density (Ωb = 0.049, ΩDM = 0, ΩΛ = 0). Intellectual Property, Copyright & Commercial Licensing Notice: © 2026 Sudhir Raj, Researcher (Equilibrium-Research.org), Equilibrium-Research.org Group, Headington, England. Manuscript text and figures may be distributed for non-commercial academic review and scientific citation with full attribution to the author and https://equilibrium-research.org. The underlying thermodynamically-constrained variational operator architecture, sequential bespoke-footprint conditioning pipeline, 1000.0 equilibrium residual conditioning divisor, hard-wired Heaviside-linear positivity projector, and pre-calibrated spectral operator state tensors described herein are the subject of United Kingdom Patent Application No. GB2625201.5 (Patent Pending). Nothing in this academic publication grants any implied or express license under any patent rights. All commercial implementation and Field-of-Use licensing rights are strictly reserved. Commercial licensing inquiries: [email protected]

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Publication Details

Journal
Zenodo (CERN European Organization for Nuclear Research)
Published
2026-10-26
DOI
https://doi.org/10.5281/zenodo.23670224
Primary Topic
Cosmology and Gravitation Theories
Type
preprint
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preprint

Baryonic Horizon Dynamics Across z ∈ [0.01, 2.30]: Resolving Late-Time Cosmic Acceleration and the Type Ia Supernova Distance Modulus Without a Cosmological Constant (Λ)

Sudhir Raj
Zenodo (CERN European Organization for Nuclear Research)
Cosmology and Gravitation Theories
preprint

Baryonic Horizon Dynamics Across z ∈ [0.01, 2.30]: Resolving Late-Time Cosmic Acceleration and the Type Ia Supernova Distance Modulus Without a Cosmological Constant (Λ)

Sudhir Raj
preprint en

Abstract

AbstractThe observed dimming of high-redshift Type Ia supernovae (SN Ia) [1–4] and BaryonAcoustic Oscillation (BAO) expansion history [5] across z ∈ [0.01, 2.30] require, withinstandard ΛCDM cosmology, that approximately 70% of the cosmic energy budget residein an unexplained cosmological constant (Λ / Dark Energy) alongside ∼ 25% non-baryonicCold Dark Matter. Completing our three-scale cosmology trilogy [6,7], we formulate a hybridCausal State-Space Spectral Integrator (CSSI) combining a gated causal state-transitionpropagator with a 16-mode 1D spectral Fourier convolution kernel constrained by the 5Dtrans-brane restoring stress-energy tensor TEPR (z, w) [8]. By formulating the causal state-transition propagator entirely from analytical, twice-differentiable operators across Nz = 300native redshift nodes (z ∈ [0.01, 2.30]), we evaluate exact second-order variational derivativesof the bulk attenuation PDE (∂TEPR /∂w + λTEPR = 0). Whereas the unconditioned baselinecollapses with an expansion rate error of RMSE = 128.20 km/s/Mpc, the stabilized solver(incorporating the ‘/1000.0‘ Friedmann equilibrium residual divisor, 10−11 horizon massscaling, λ = 8.2390 bulk attenuation lock, and hard-wired Heaviside-linear positivity projectorP+ ) converges to RMSE = 0.03 km/s/Mpc (R2 = 1.0000) for the Hubble parameter H(z)and RMSE = 0.0001 mag (R2 = 1.0000) for the Type Ia supernova distance modulus µ(z),utilizing a strictly baryonic matter density (Ωb = 0.049, ΩDM = 0, ΩΛ = 0). Intellectual Property, Copyright & Commercial Licensing Notice: © 2026 Sudhir Raj, Researcher (Equilibrium-Research.org), Equilibrium-Research.org Group, Headington, England. Manuscript text and figures may be distributed for non-commercial academic review and scientific citation with full attribution to the author and https://equilibrium-research.org. The underlying thermodynamically-constrained variational operator architecture, sequential bespoke-footprint conditioning pipeline, 1000.0 equilibrium residual conditioning divisor, hard-wired Heaviside-linear positivity projector, and pre-calibrated spectral operator state tensors described herein are the subject of United Kingdom Patent Application No. GB2625201.5 (Patent Pending). Nothing in this academic publication grants any implied or express license under any patent rights. All commercial implementation and Field-of-Use licensing rights are strictly reserved. Commercial licensing inquiries: [email protected]

Zenodo (CERN European Organization for Nuclear Research)
Equilibrium Research (GB)
Cosmology and Gravitation Theories
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