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Syllabus for High-Energy Astroparticle Physics (2024/2025)

  1. November 25, 2024

    • Introduction to High-Energy Astroparticle Physics
    • Overview of the field and key questions
    • Course logistics and structure
  2. November 26, 2024

    • Synchrotron power and electron energy loss timescales
    • Cooling break: definition and significance
    • Relativistic beaming: concepts and observational implications
    • Synchrotron spectrum and critical frequency
    • Synchrotron emission from electron populations
  3. November 27, 2024

    • Basics of Compton scattering
    • Inverse Compton (IC) scattering and energy transfer
    • Single-particle power radiated in IC scattering
    • Key properties of the Klein-Nishina cross-section
    • Kinetic equation for electron evolution: modeling radiation processes
  4. November 28, 2024

    • Gamma-ray absorption: threshold energy and cross-section
    • Interaction timescale for hadronic interactions
    • Pion production in proton-proton collisions
    • Pion emissivity and gamma-ray spectrum derivation
  5. November 29, 2024

    • The 𝜋⁰ gamma-ray spectrum and the pion bump
    • Diffuse Galactic gamma-ray emission: observations and theory
    • Photo-pion production: energy thresholds and relevance for UHECRs (Ultra-High-Energy Cosmic Rays)
    • Pair production processes and their astrophysical implications
  6. December 2, 2024

    • Multi-messenger relations: connecting cosmic rays, neutrinos, and gamma rays
    • The Waxman-Bahcall limit for neutrino flux
    • Introduction to the cosmic ray transport equation
    • Cosmic-ray diffusion as a random walk: the mean free path
  7. December 3, 2024

    • Diffusion equation: solutions and limitations in cosmic ray propagation
    • Transport equation for primary nuclei: formulation and solutions
    • The cosmic ray composition and the grammage pillar
  8. December 4, 2024

    • Transport equation for secondary nuclei: applications and implications
    • Secondary-to-primary ratio: insights into cosmic ray physics
    • Transport equation for unstable secondary nuclei and observational significance
    • The SN paradigm
  9. December 5, 2024

    • Charged particle motion in a turbulent magnetic field: the QLT approach
    • Pitch angle diffusion
    • The Kolmogorov turbulence power spectrum
  10. December, 6, 2024

    • The resonant scattering
    • The diffusion coefficient in space
    • Implications on the Galactic mean free path
  11. December 16, 2024 🚀

    • Diffusion equation in pitch angle
    • Diffusion equation in space
    • Cosmic ray diffusive flux and anisotropy
  12. December 17, 2024

    • General conditions for particle acceleration
    • The Hillas criterion and plausible Galactic cosmic ray sources
    • Generalities of Stochastic Acceleration
    • Second order Fermi acceleration
  13. December 18, 2024

    • The Formation of Shock Waves
    • Interstellar Shock Waves
    • The Rankine-Hugoniot jump conditions
    • Compression ratio
  14. December 19, 2024

    • Dynamical Evolution of Supernova Remnants
    • Free expansion phase
    • Sedov-Taylor phase
    • Historical Supernovae in the Milky Way
  15. December 20, 2024