1997/08/18 by J. Ignatius, Ignatius, J.
Physics and Astronomy · #Astrophysics (astro-ph) #FOS: Physical sciences #High Energy Physics - Phenomenology (hep-ph) #astro-ph #hep-ph
paper · pdf · doi:10.48550/arxiv.hep-ph/9708383
6 pages, 1 figure. To appear in the Proceedings of Strong and Electroweak Matter '97, Eger, Hungary, 21-25 May 1997
arxiv created 1997/08/18 · arxiv updated 2009/11/30
The dynamical growth rate of bubbles nucleating in relativistic plasma in thermal first-order phase transitions is analyzed. The framework is a hydrodynamical model which consists of relativistic fluid and an order parameter field. The results of analytical approximations and numerical simulations coincide well.