A Cosmological Model of Thermodynamic Open Universe
G.K.Goswami, Mandwi Trivedi

TL;DR
This paper generalizes Prigogine's early universe model by including radiation, showing a vacuum instability origin for the universe, and connects it to quantum particle creation, resulting in a continuous evolution to the current universe.
Contribution
It introduces a radiation-dominated cosmological model based on vacuum instability, extending Prigogine's particle creation framework with new insights into cosmic background radiation.
Findings
Universe originates from vacuum instability, not a singularity.
Model transitions from rapid early evolution to de-sitter phase.
Results align with observed cosmic background radiation.
Abstract
In this paper we have given a generalisation of the earlier work by Prigogine et al. who have constructed a phenomenological model of entropy production via particle creation in the very early universe generated out of the vacuum rather than from a singularity, by including radiation also as the energy source and tried to develop an alternative cosmological model in which particle creation prevents the big bang. We developed Radiation dominated model of the universe which shows a general tendency that (i) it originates from instability of vacuum rather than from a singularity. (ii) Up to a characteristic time cosmological quantities like density, pressure, Hubble constant and expansion parameter vary rapidly with time. (iii) After the characteristic time these quantities settles down and the models are turned into de-sitter type model with uniform matter, radiation, creation densities…
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