Panoramas et synthèses, n° 39-40. Numerical models for fusion

At very high temperature electrons leave the atom to which they are
attached and a gas of charged particles called a plasma is obtained.
Plasmas, because of their interaction with an electromagnetic field,
have a global and rich behaviour, much more complex than for neutral
gases. This makes their study complex and fascinating. Plasma
physics and its lighthouse application, controlled thermonuclear
fusion, thus offers new challenges to mathematicians. Two main
models are generally used to describe the dynamics of a plasma :
on the one hand the so-called kinetic models which describe the
evolution of the phase space density of the different particle species,
and on the other hand the fluid models which describe the evolution of
macroscopic quantities, like density in physical space, mean velocity
and temperature. This two types of models need to be coupled with
Maxwell's équations in order to describe the non linear interactions
with the electromagnetic field generated by the charged particles of
the plasma. This book results from notes of the lectures that were
given at CIRM in Luminy during the summer school of CEMRACS
2010. It détails for topics in the mathematical and 'numerical study
of plasmas : asymptotic preserving (AP) numerical schemes that
enable to deal consistently with two space or time scales, gyrokinetic
simulations of magnetic fusion plasmas, MHD simulations of magnetic
fusion plasmas and the mathematical study of Landau damping.