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June 4, 20260 citationsOpen Access

Quantitative Predictions for the z > 15 Frontier within the Optico-Hydrodynamic Vacuum (OHV) Framework

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SPSergey Yurevich Paygachkin

Key Points

  • This work aims to provide predictions for surface brightness scaling of distant galaxies based on the OHV framework.
  • Formulated predictions derived from the OHV framework using Type Ia supernova data.
  • Proposed observational program using JWST data from JADES, CEERS, and COSMOS-Web.
  • Measured alpha in surface brightness scaling through controlled galaxy sample selection.
  • Predicted surface brightness scales as SB ~ (1+z)^{-1}, diverging from standard SB ~ (1+z)^{-4} predictions.
  • At z = 15, the expected ratio of OHV to Lambda-CDM surface brightness is approximately 4096.
  • Empirical support is indicated if alpha ~ 1 from JWST data, with strong refutation at alpha ~ 4.

Abstract

The Optico-Hydrodynamic Vacuum (OHV) framework proposes that cosmological redshift arises from continuous energy dissipation of photons in a static viscous vacuum substrate, parameterized by a single dimensionless viscosity coefficient eta ~ 0. 004182 derived from Pantheon+ Type Ia supernova data. This memorandum presents a testable prediction for the James Webb Space Telescope (JWST): the surface brightness of distant galaxies should scale as SB ~ (1+z) ^-1, rather than SB ~ (1+z) ^-4 as predicted by Tolman dimming in standard Lambda-CDM cosmology. The prediction follows rigorously from the definition of surface brightness SB = F/Omega combined with the OHV photon dissipation law E (D) = Eₑmit * exp (-D/RH). At z = 15, the predicted ratio of OHV to LCDM surface brightness is (1+z) ³ ~ 4096 for galaxies of identical intrinsic luminosity. The document proposes a specific observational program using publicly available JWST data (JADES, CEERS, COSMOS-Web) to measure the exponent alpha in SB ~ (1+z) ^-alpha via controlled galaxy sample selection. The prediction is falsifiable: if JWST data yield alpha ~ 4, the OHV surface-brightness law is refuted; if alpha ~ 1, it receives strong empirical support. This prediction was formulated prior to definitive JWST surface-brightness measurements at z > 10.

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Cite This Study

Sergey Yurevich Paygachkin (2026) studied this question.

synapsesocial.com/papers/6a211670d499ed480b16f604https://doi.org/10.5281/zenodo.20510107
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