After successful completion of the course, students are able to have an understanding of the physics of particles from the cosmos, the history and evolution of the universe and new phenomena like gravitational waves.
Introduction to the standard model of particle physics; signals from outer space: discovery; the birth of high-energy physics; composition and spectra of cosmic radiation; overlap with conventional astronomy; primary and secondary cosmic rays; charged particles; photons; neutrinos; gravitational waves; hypothetical particles ("dark matter"); measurement methods of astro-particle physics: Installations on the surface of the earth, on balloons and in outer space; the earth's atmosphere serving as detector for particles; neutrino detectors in the MeV to EeV range; detectors for "dark matter"; large terrestrial installations (in the 10000 square-kilometer range on the earth's surface, as well as installations under water and in the ice of Antarctica); radio emission of highest-energy particles; installations on satellites and in space stations Physics aims of astro-particle physics: Tests of the Standard Model beyond energies that can be reached by accelerators; neutrino oscillations, measurements of properties and mass of neutrinos; search for particles which have not been discovered so far ("dark matter", supersymmetry etc.); CP-violation and antimatter; cosmology, relics of the Big Bang, the origin of the universe.
Target group and conditions of participation: Physicists, astronomers, astro-physicists and colleagues from other disciplines who are interested in astro-particle physics; basic knowledge in particle physics is useful but not required.
Target group and conditions of participation: Physicists, astronomers, astro-physicists and colleagues from other disciplines who are interested in astro-particle physics; basic knowledge in particle physics is useful but not required.
