Member Panel

Your Profile

Manage Your Profile

Manage Your Publications


Useful Links

Internal Documentation

Nonlinear dynamics from the relativistic Boltzmann equation in the Friedmann-Lemaı̂tre-Robertson-Walker spacetime

Jun. 02 - 14:30 - 2016

SPEAKER: Mauricio Martinez Guerrero (Ohio State University)

ABSTRACT: The dissipative dynamics of an expanding massless gas with constant cross section in a spatially flat Friedmann-Lemaı̂tre-Robertson-Walker (FLRW) universe is studied. The mathematical problem of solving the full nonlinear relativistic Boltzmann equation is recast into an infinite set of nonlinear ordinary differential equations for the moments of the one-particle distribution function. Momentum-space resolution is determined by the number of non-hydrodynamic modes included in the moment hierarchy, i.e. by the truncation order. We show that in the FLRW spacetime the non-hydrodynamic modes decouple completely from the slowest hydrodynamic degrees of freedom. This results in the system flowing as an ideal fluid while at the same time producing entropy. The solutions to the nonlinear Boltzmann equation exhibit transient tails of the distribution function with non-trivial momentum dependence. The evolution of this tail is not correctly captured by the relaxation time approximation nor by the linearized Boltzmann equation. However, the latter probes additional high-momentum details unresolved by the relaxation time approximation. While the expansion of the FLRW spacetime is slow enough for the system to move towards (and not away from) local thermal equilibrium, it is not sufficiently slow for the system to actually ever reach complete local equilibrium. Equilibration is fastest in the relaxation time approximation, followed, in turn, by kinetic evolution with a linearized and a fully nonlinear Boltzmann collision term.

An importable CVS/ICS calendar with all of CENTRA's events is available here