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April 16, 2026Open Access

Two-Component Dissipative Distance Metric in a Viscous Vacuum: Resolution of JWST Brightness Anomalies and Pantheon+ Calibration

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Authors

SPSergey Paigachkin

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Overview

This research demonstrates a novel distance metric resolving brightness anomalies in galaxies and improving cosmological models.

Key Points

  • The study aims to develop a two-component distance metric to address brightness anomalies observed by JWST and improve Type Ia supernova calibration.
  • Developed a two-component distance metric within the Optico-Hydrodynamic Vacuum framework.
  • Calibrated the metric against the Pantheon+ Type Ia supernova catalog with 1701 entries.
  • Analyzed the metric's fit using chi-square comparisons to the flat Lambda-CDM model.
  • Achieved an excellent fit with chi-square/N = 0.72, outperforming the Lambda-CDM model (chi-square/N = 1.88).
  • Predicted galaxy magnitudes 2.1 - 2.5 mag brighter than the Lambda-CDM model for z > 10.
  • Explained light curve broadening of SNe Ia through vacuum-viscosity time dilation.

Cite This Study

Sergey Paigachkin (2026) studied this question.

synapsesocial.com/papers/69e07e992f7e8953b7cbf6f3https://doi.org/10.5281/zenodo.19570022
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