A relativistic neutral scalar field is investigated on the basis of the
Schwinger-Dyson equation in the non-equilibrium thermo field dynamics. A time
evolution equation for a distribution function is obtained from a
diagonalization condition for the Schwinger-Dyson equation. An explicit
expression of the time evolution equation is calculated in the λϕ4
interaction model at the 2-loop level. The Boltzmann equation is derived for
the relativistic scalar field. We set a simple initial condition and
numerically solve the Boltzmann equation and show the time evolution of the
distribution function and the relaxation time.Comment: 23 pages, 9 figure