Speaker
Prof.
Sichun Sun
(Beijing Institute of Technology)
Description
We discuss ways to extend the Standard Model quantum chromodynamics theory (QCD) theory and realize a first-order phase transition at high temperatures above 1 GeV without running into current constraints from heavy ion colliders and early cosmology. The phase transition is from a non-perturbative effect of the QCD. It can greatly impact the early universe, including gravitational wave signals detectable for future space interferometers.
Primary author
Prof.
Sichun Sun
(Beijing Institute of Technology)
