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Phase transitions can be categorised by their [[Phase Transition#Classifications|order]]. Transitions which are first order proceed via [[False_vacuum_decay#Bubble_nucleation|bubble nucleation]] and release [[latent heat]] as the bubbles expand.
As the universe cooled after the hot Big Bang, such a phase transition would have released huge amounts of energy, both as heat and as the kinetic energy of growing bubbles. In a strongly first-order phase transition, the bubble walls may even grow at near the [[speed of light]].<ref>{{cite journal |last1=Moore |first1=Guy D. |last2=Prokopec |first2=Tomislav |title=Bubble wall velocity in a first order electroweak phase transition |journal=Phys. Rev. Lett. |date=1995 |volume=75 |pages=777-780 |doi=10.1103/PhysRevLett.75.777}}</ref> This, in turn, would lead to the production of a [[gravitational wave background|stochastic background of gravitational waves]].<ref name="witten-1984" /><ref name="hogan-gws">{{cite journal |last1=Hogan |first1=C. J. |title=Gravitational radiation from cosmological phase transitions |journal=Mon. Not.
==Examples==
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