TL;DR
This paper explores the evolution of the universe post-electroweak symmetry breaking, focusing on a multi-phase transition scenario leading to an inert phase with dark matter candidates.
Contribution
It investigates the possibility of a sequence of phase transitions instead of a single transition from symmetric to inert phase.
Findings
Potential for multiple phase transitions in the universe's evolution.
Identification of scalar dark particles as dark matter candidates.
Implications for the universe's thermal history and dark matter formation.
Abstract
We consider evolution of the Universe after EWSB leading to the present inert phase, containing a SM-like Higgs boson and scalar dark particles, among them a Dark Matter candidate. We address the question, if there is a possibility to have a sequence of the phase transitions instead of a single one leading directly from EW symmetric phase to the inert one.
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