pith. sign in

arxiv: astro-ph/9509018 · v1 · submitted 1995-09-05 · 🌌 astro-ph · hep-ph

Dynamics of Subcritical Bubbles in First Order Phase Transition

classification 🌌 astro-ph hep-ph
keywords bubblessubcriticalphasethermalstatetransitionamplitudederivate
0
0 comments X
read the original abstract

We derivate the Langevin and the Fokker-Planck equations for the radius of $O(3)$-symmetric subcritical bubbles as a phenomenological model to treat thermal fluctuation. The effect of thermal noise on subcritical bubbles is examined. We find that the fluctuation-dissipation relation holds and that in the high temperature phase the system settles down rapidly to the thermal equilibrium state even if it was in a nonequilibrium state initially. We then estimate the typical size of subcritical bubbles as well as the amplitude of fluctuations on that scale. We also discuss their implication to the electroweak phase transition.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.

Forward citations

Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. Subcritical bubble prehistory in weak first-order phase transition

    hep-ph 2026-05 unverdicted novelty 5.0

    In weak first-order phase transitions, subcritical bubbles reach percent-level volume fractions before critical nucleation when phases are nearly degenerate at Tn, invalidating the homogeneous-background assumption fo...