Abstract

It is shown that the non-equilibrium electrically neutral and relativistically invariant vacuum-like state with the negative energy density and positive pressure may exist at the non-zero temperature in the system of spinor particles, antiparticles, and random electromagnetic field generated by particle-particle, particle-antiparticle, and antiparticle-antiparticle transitions. At the temperature of the order of 10 -5 K, the energy density of its state corresponds to the dark energy density in absolute magnitude. The cosmological constant for such material medium turns out to be negative.

Highlights

  • Article [1] shows that the quantum theory allows building up the relativistically invariant state of matter, for which pressure p and energy density ε are related as follows p = −ε

  • At the same time particles and antiparticles are in the thermal equilibrium, but far from the chemical equilibrium state governed by the equality of their chemical potentials

  • 2c m2c2 + pF 2 1 2 ≈ 2mc2 1 + (1 2) (4 π −1)α kBTΛ. This non-equilibrium electrically neutral state exists due to the random electromagnetic field generated by spontaneous transitions between particles and antiparticles being in different quantum states

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Summary

Introduction

The cosmological constant problem is relevant in the context of the experimental confirmation of the accelerated expansion of the Universe [6] This phenomenon can be explained with the help of the General Relativity, and by the different alternative versions of the Gravity Theory (see [7] and the articles cited there), where dark energy concept isn’t introduced. Is close, at least in the order-of-magnitude, to the value of ρ (Λ) ≈(7.21 ± 0.25) ×10−30 g ⋅ cm−3 resulted from the interpretation of astrophysical data [6] that has not been solved Solving this problem seems important for the understanding of potential physical phenomena leading to the formation of such material medium

Energy-Momentum Tensor of Random Electromagnetic Field
Energy Density and Pressure of Interacting Mixture
Conclusions
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