What happened to the Cosmological QCD Phase Transition?
W-Y. P. Hwang

TL;DR
This paper explores the cosmological QCD phase transition as a first-order process, examining domain wall formation and its potential role in dark matter, suggesting it may influence our understanding of early Universe epochs.
Contribution
It models the QCD phase transition using degenerate theta-vacua and complex scalar fields, analyzing domain wall formation and their implications for dark matter and cosmological epochs.
Findings
Domain walls form during the QCD transition.
Long-lived domain walls could account for dark matter.
The transition may challenge standard radiation and matter epoch concepts.
Abstract
The scenario that some first-order phase transitions may have taken place in the early Universe offers us one of the most intriguing and fascinating questions in cosmology. Indeed, the role played by the latent "heat" or energy released in the phase transition is highly nontrivial and may lead to some surprising, important results. In this paper, we take the wisdom that the cosmological QCD phase transition, which happened at a time between 10^(-5) sec and 10^(-4) sec or at the temperature of about 150 MeV and accounts for confinement of quarks and gluons to within hadrons, would be of first order. To get the essence out of the scenario, it is sufficient to approximate the true QCD vacuum as one of degenerate theta-vacua and when necessary we try to model it effectively via a complex scalar field with spontaneous symmetry breaking. We examine how and when "pasted" or "patched" domain…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
