Chemical and kinetic equilibrations via radiative parton transport

A hot and dense partonic system can be produced in the early stage of a relativistic heavy ion collision. How it equilibrates is important for the extraction of Quark-Gluon Plasma properties. We study the chemical and kinetic equilibrations of the Quark-Gluon Plasma using a radiative transport model. Thermal and Color-Glass-Condensate motivated initial conditions are used. We observe that screened parton interactions always lead to partial pressure isotropization. Different initial pressure anisotropies result in the same asymptotic evolution. Comparison of evolutions with and without radiative processes shows that chemical equilibration interacts with kinetic equilibration and radiative processes can contribute significantly to pressure isotropization.Comment: Presented at 24th International Nuclear Physics Conference (INPC2010), Vancouver, Canada, 4-9 July 201

Parton radiative processes and pressure isotropization in relativistic heavy ion collisions

The impact of radiative processes on kinetic equilibration is studied via a radiative transport model. The 2 3 processes can significantly increase the level of thermalization. These processes lead to an approximate coupling constant scaling of the evolution of the pressure anisotropy qualitatively different from the case with only 2 -> 2 partonic processes. Furthermore, thermal and Color Glass Condensate motivated initial conditions are shown to share the same asymptotic evolution when 2 3 processes are included. This emphasizes the unique role of radiative processes in Quark-Gluon Plasma thermalization.Comment: Revised introduction and discussion on 3-body collisions, corrected Equation (3), updated acknowledgments and reference