What question did this study set out to answer?

This research aims to connect cosmological observations with nuclear physics through a viscosity parameter.

May 22, 2026Open Access

A Unified Dissipative Framework: Linking Cosmological Viscosity to Nuclear Binding Energy via Three-Dimensional Geometric Normalization

Key Points

This research aims to connect cosmological observations with nuclear physics through a viscosity parameter.
Calibrated the optico-hydrodynamic vacuum distance metric on the Pantheon+ Type Ia supernova dataset (N=1590, z>0.01)
Evaluated goodness-of-fit using reduced chi-square values comparing against the flat Lambda-CDM model.
Achieved a reduced chi-square of 0.901, comparable to Lambda-CDM's 0.884.
Determined a characteristic vacuum viscosity coefficient of eta = 0.4182 percent.

Abstract

We present a universal dissipative framework establishing a quantitative connection between cosmological-scale observations and nuclear binding energies through a single dimensionless viscosity parameter eta. Calibrating the optico-hydrodynamic vacuum (OHV) distance metric on the Pantheon+ Type Ia supernova dataset (N = 1590, z > 0.01) yields a reduced chi-square of 0.901, statistically comparable to the flat Lambda-CDM model (0.884). The optimized parameters imply a characteristic vacuum viscosity coefficient eta = 0.4182 percent.

Read Full Paperexternally

KI fragen

Bookmark

View Full Paper