Examination procedure
<p>Seminar</p>
Prerequisites
Students should be familiar with hydrodynamics and basic principles of astrophysics and cosmology. Knowing how to program in Fortran and/or C is very desirable. Designed for PhD but open also to Master students
Syllabus
In this course we are going to go through numerical techniques for solving the equations of hydrodynamics in an astrophysical context. We are also going to focus on gravity solvers and numerical techniques to follow radiative transfer on high performance computing facilities. Each lecture will be accompanied by a hands-on session.