Investigates phase transitions in the ψ-field substrate, suggesting new insights into cosmic evolution.
In this paper, within the framework of the OCEAN (FUH) model, the concept of the multiphase nature of the vacuum condensate is introduced. Based on the previously established Shlyapik threshold (Ethr = 7.76 keV), the temperature boundaries of the Ocean’s phase transitions are calculated. The existence of a high-temperature ”Lava” phase preceding the superfluid state is substantiated. This allows describing the evolution of the Universe as a process of rheological cooling and crystallization of the medium without invoking the singularity hypothesis.
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Alexander Shlyapik (2026) studied this question.
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