Abstract
We use a form of the fluctuation-dissipation theorem to derive formulas giving the rate of production of spin- baryons in terms of the fluctuations of either meson or quark fields. The most general formulas do not assume thermal or chemical equilibrium. When evaluated in a thermal ensemble we find equilibration times on the order of near the critical temperature in QCD.
- Received 25 September 2002
DOI:https://doi.org/10.1103/PhysRevC.68.014901
©2003 American Physical Society