The Dark Components of the Universe Are Slowly Clarified

TL;DR

This paper discusses the gradual understanding of the Universe's dark sector, proposing a composite particle model for dark matter and predicting observable phenomena like familon detection and dark atoms.

Contribution

It introduces a composite model for dark matter involving familons and predicts new detectable phenomena related to dark medium spectroscopy.

Findings

Dark matter may consist of familon-type pseudo-Goldstone bosons.

Three generations of particles are essential in the proposed model.

Predictions include familon detection and dark atom spectroscopy.

Abstract

The dark sector of the Universe is beginning to be clarified step by step. If the dark energy is vacuum energy, then 123 orders are exactly reduced by ordinary physical processes. For many years these unexplained orders were called a crisis in physics. There was indeed a "crisis" before the introduction of the holographic principle and entropic force in physics. The vacuum energy was spent for the organization of new microstates during the entire life of the Universe, but in the initial period of its evolution the vacuum energy (78 orders) were reduced more effectively by the vacuum condensates produced by phase transitions, because the Universe lost the high symmetry during its expansion. Important problems of physics and cosmology can be solved if the quarks, leptons, and gauge bosons are composite particles. The dark matter, partially or all consisting of familon-type pseudo-Goldstone bosons with a mass of 10^{-5} - 10^{-3} eV, can be explained in the composite model. Three generations of elementary particles are absolutely necessary in this model. In addition, this model realizes three relativistic phase transitions in a medium of familons at different red shifts, forming a large-scale structure of dark matter that was "repeated" by baryons. We predict the detection of dark matter dynamics, the detection of familons as dark matter particles, and the development of spectroscopy for dark medium due to the probable presence of dark atoms in it. Other viewpoints on the dark components of the Universe are also discussed briefly.