This preprint presents a framework explaining cosmological stability using vacuum relaxation processes, indicating potential implications for our understanding of the Universe.
Key Points
The aim is to explain the apparent stability of cosmological parameters despite the dynamic evolution of the Universe.
Developed a unified framework incorporating vacuum relaxation processes
Analyzed the emergence of late-time stability from quantum vacuum behavior
Maintained consistency with general relativity and ΛCDM models
Demonstrated that the quantum vacuum approaches a quasi-stationary state
Explained robustness of expansion dynamics and temporal scales
Outlined observable consequences for empirical testing