After successful completion of the course, students are able to apply finite Lorentz transformations, to analyze Maxwell equations and their solutions in relativistic formulations, to set up and solve Euler-Lagrangian equations of motion for relativistic particles and fields, to derive Noether charges from symmetries of the Lagrangian and to derive theories resulting from spontaneous symmetry breaking and to calculate the radiation properties of moving matter.
Application and illustration of the material offered in the lecture "Electrodynamics II" using exercises and application examples.
Students are given lecture-related tasks that they calculate independently within a week and then present on the board.
The assessment is based on the number of crossed examples and the presentations of these.
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Electrodynamics I
