Rp. Pilla et J. Shaham, KINETICS OF ELECTRON-POSITRON PAIR PLASMAS USING AN ADAPTIVE MONTE-CARLO METHOD, The Astrophysical journal, 486(2), 1997, pp. 903-918
A new algorithm for implementing the adaptive Monte Carlo method is gi
ven. It is used to solve the Boltzmann equations that describe the tim
e evolution of a nonequilibrium electron-positron pair plasma containi
ng high-energy photons. These are coupled nonlinear integro-differenti
al equations. The collision kernels for the photons as well as pairs a
re evaluated for Compton scattering, pair annihilation and creation, b
remsstrahlung, and Coulomb collisions. They are given as multidimensio
nal integrals which are valid for all energies. For an homogeneous and
isotropic plasma with no particle escape, the equilibrium solution is
expressed analytically in terms of the initial conditions. For two sp
ecific cases, for which the photon and the pair spectra are initially
constant or have a power-law distribution within the given limits, the
time evolution of the plasma is analyzed using the new method. The fi
nal spectra are found to be in a good agreement with the analytical so
lutions. The new algorithm is faster than the Monte Carlo scheme based
on uniform sampling and more flexible than the numerical methods used
in the past, which do not involve Monte Carlo sampling. It is also fo
und to be very stable. Some astrophysical applications of this techniq
ue are discussed.