Disciplines
Computer Sciences (25%); Physics, Astronomy (75%)
Keywords
Plasma Physics,
Fusion Energy,
Plasma Turbulence,
Computational Physics,
Gyro-Fluid Theory,
Fluid Closure
Abstract
Nuclear Fusion represents a virtually clean and unlimited energy source of the future, where net
energy is to be produced by fusing charged particles. In order for this to happen, these charged
particles are heated to temperatures that exceed those of the Sun and are confined by extremely
strong magnetic fields that are 1000 times greater than that the Earths magnetic field. These
magnetic fields force the particles to follow circular paths along the magnetic fields. An outstanding
problem of nuclear fusion and the design of future fusion reactors is the accurate prediction and
reduction of the heat flow to the adjacent reactor walls. This heat flow poses extreme challenges for
wall materials, even exceeding that of rocket launches. The current state of the art mathematical
models utilize the gyro-motion of the particles for an efficient description (gyro-kinetics) of the
turbulent dynamics . However, these models reach their limits when predicting the heat flow in the
most demanding calculations on the world`s fastest high performance computing machines. In the
LEGO project (Learning gyro-fluid closure), exact relations (closure) of the heat flow are to be
found, which are the key to a so called fluid description (gyro-fluid fluid). For example, the heat
flow can be linked to temperature differences when particle collisions are dominant. Here, these
relations are to be derived for gyro-fluid theories in collision-free and collision-dominated
conditions, but in particular also for conditions that cannot be assigned to either regime. For this
purpose, the most modern methods in analytical theory, numerical mathematics and simulations as
well as machine learning are used. This should enable the design of nuclear fusion reactors and help
to understand the ongoing dynamics therein using the much less complex gyro-fluid models.