This pathway is recommended for those particularly interested in modeling, especially numerical, of astrophysical sources or basic physical processes. The main topics for a potential thesis in this field include plasma physics (especially in the solar wind, even at the kinetic level), relativistic astrophysics, the study of compact objects (neutron stars and black holes), multi-messenger astrophysics (photons, cosmic rays, neutrinos, and gravitational waves), high-energy radiative processes, particle acceleration mechanisms, and cosmology, particularly the evolution of the first stars and first galaxies, and stellar archaeology.
The Theoretical Astrophysics pathway naturally fits within the Astrophysics curriculum, and the rules must be followed when preparing the study plan. Below are some recommendations for choosing core, supplementary/integrative, and elective astrophysical courses for this pathway.
Core Astrophysics Courses (5 courses of 6 ECTS each) Astrophysics Relativistic Astrophysics Cosmology Plasma Physics Numerical Methods for Astrophysics |
Recommended Supplementary/Integrative or Elective Courses (5 courses of 6 ECTS each) At least two electives from: First Stars and First Galaxies High Energy Astrophysics Solar and Heliospheric Physics Stellar Evolution and Nucleosynthesis Other recommended courses: Active Galactic Nuclei and Black Holes Exoplanets and Protoplanetary Disks Atmospheric Physics Physics of Galaxies Physics of the Interstellar Medium Theories of the Early Universe*
Other electives from the full list of supplementary/integrative courses, or core courses from this or other curricula, or courses from other study programs.
Notes: *Theoretical physics course, best taken after: Elementary Particle Physics, Theoretical Physics |
For further information on research areas related to the Theoretical Astrophysics pathway and for thesis requests, please refer to the following groups:
Last
update
03.03.2025