This course provides a comprehensive introduction to cosmic ray physics and astrophysics, covering the propagation of charged particles in turbulent magnetic fields, with diffusion as a natural implication. We will derive and utilize the transport (advection-diffusion) equation to describe cosmic ray propagation in the Galaxy and particle acceleration at shock waves. We will also outline key particle interactions and energy loss mechanisms in the Galactic and Extra-galactic environments, shaping cosmic ray spectra and producing secondary species like gamma rays, neutrinos, and antiparticles, which serve as diagnostic tools in multi-messenger astrophysics.
A detailed syllabus can be found here.
The course material will be drawn from a combination of textbooks, journal literature, and my own lecture notes. The following textbooks provide excellent topical coverage:
Lecture notes can be found here
For feedback or to report any mistakes, please use the GitHub issues
Exercise sets are available as a single booklet here
Exercises solved (✅) and work in progress (🤔):