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In this lecture we discuss the general problem of scattering when dealing with the radiative transfer equation, illustrating with a two-component sour...
Radiation Processes in AstronomyIn this lecture we discuss photoionization a bit further. We show how to obtain the ionization rate and discuss behaviour of (hydrogenic) cross sectio...
Radiation Processes in AstronomyThis lecture considers Compton scattering as the general case of the low-energy Thomson limit for electron scattering. We obtain the frequency-shift i...
Radiation Processes in AstronomyThis lecture goes through thermal bremsstrahlung. We start with a derivation in the classical limit, then show how we obtain emission and extinction c...
Radiation Processes in AstronomyThis short lecture wraps up the spectral line broadening part by adding some notes on the effects of macroscopic velocity fields, both in the case of...
Radiation Processes in AstronomyIn this lecture (two parts, here part II) we go through spectral line broadening, focusing mostly on microscopic broadening but discussing also (in th...
Radiation Processes in AstronomyIn this lecture (two parts, here part I) we go through spectral line broadening, focusing mostly on microscopic broadening but discussing also (in par...
Radiation Processes in AstronomyIn this lecture we go through Einstein's original paper where he (correctly) suggests the process of stimulated emission. This then also introduces hi...
Radiation Processes in AstronomyIn this lecture, part II on teh Cosmic Background Radiation, we calculate and analyze when the era of photon-baryon decoupling occurred and when our U...
Radiation Processes in AstronomyIn this application lecture, first of two on the cosmic background radiation, we use knowledge we've acquired in the course to calculate and analyze t...
Radiation Processes in AstronomyThis lecture introduces the Saha and Boltzmann relations to compute excitation and ionisation balance in (local) thermodynamic equilibrium. We also br...
Radiation Processes in AstronomyThis lecture uses semi-classical arguments to make order-of-magnitude scaling estimates for the energies and strengths (life times) of electric dipole...
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