Ay 121: Radiative Processes
Instructor: S. R. Kulkarni, 1030-1200 (Tuesday & Thursday)
In my view, success in astronomy rests upon having a sound foundation
in physics and mathematics. In this course, I will follow closely
the classic textbook "Radiative Processes in Astrophysics" by Rybicki
& Lightman.
My goal is to follow the book closely. However, I will be adding
some additional material (noted as SRK notes). In some cases, I
will provide the notes by the way of a link to a pdf file.
As an observer I find myself to refresh undergraduate physics now
and then. The classic book on E&M by Purcell has now been vastly
revised (Purcell & Morin). I am frequently reaching to it to brush
up on undergrad physics and Schaum series to brush up on those
rusty knowledge of vectors, differential geometry...
You are expected to check the on-line syllabus and do the preparatory
work ahead of the class.
There are really some very good courses on YouTube
now. I will use this spot to list interesting courses.
There is a separate class on fluids. We will be making use
of some aspects of fluid mechanics. I found the Introductory
talks on Fluid Mechanics by Professor Cimbala, PSU, to be
helpful.
Grading: Please remember that the goals in graduate school
are different from those in colleges. Here, you aim for understanding,
period. Homeworks will be posted every Friday and due midnight the
next Friday. A good teacher can catalyze understanding and an
excellent teacher can provide unique insights. I have observed that
much of learning is peer-to-peer (which is why it is profitable to
attend selective colleges). Bearing these observations in mind try
to first work out the homework on your own. If you meet a dead end
then discuss with a class mate(s). However, what you turn in must
be your own work.
Homeworks will be assigned every week and due 7 days later (COB).
The final exam will be an oral exam with questions given to the
class 2 weeks in advance. You will be asked five questions (at
random) from this set. The exam will last up to an 1 hour. Homeworks
will be given 2/3 weight with the remaining 1/3 for the final exam.
During mid-terms (the week is TBD) we will have a short (30 minute)
oral exam in lieu of a homework. It is meant to make students
familiar with the framework of oral exams.
- September 30
- Introductory talk stressed the importance of remembering basic
constants, the value of "pre-computing", and the benefits of
making order of magnitude estimates.
[SRK Notes]
- Mandel's semi-classical theory of detection
[SRK notes]
- Spectral Flux Density (Jansky, magnitude, Rayleigh)
- nu-fnu [SRK notes]
Students: I covered nu-fnu and Mandel's theory quite rapidly. Please
read through and, we can, at your request, briefl review at the next
class.
- October 2
Students: review Einstein A & B coefficients and be in a position
to derive Planck's brightness formula.
- Intensity and its moments (Ch 1.3)
- Radiative Transfer (Ch 1.4)
- Blackbody radiation (clasical & QM; Ch 1.5)
- Einstein A & B coefficients. Brightness temperature (Ch 1.6).
- Homework
- October 7
Students: Please review Maxwell's equations and also review
vector
algebra (curl, del, grad and all that)
- Poynting Vector (Ch 2.1)
- EM waves in vaccum (Ch 2.2)
- Introduction to Fourier transform, Power Spectrum (2.3)
[SRK notes]
- Homework 2
- October 14
Students: Please consult your old textbooks and become familiar
with vector potential for magnetic field. Review Poisson's equation
and Green's function.
- Radiation from moving charges. Electromagnetic potentials (Ch 2.5).
- Linenard-Wiechart potential (Ch 3.1).
- Velocity & Acceleration fields (Ch 3.2).
For the curious student:
Gauge selection
 |  Poisson's Equation
 |  History of Gauge
Choices.
- October 16
- Larmor Formula & Dipole approximation (Chapter 3.3)
- Thompson scattering (Chapter 3.4)
- Homework 3
- October 21
Students: Beware of different ways to define B-coefficients. See
notes by
R. C. Hilborn.
- Radiation Reaction (3.4)
- Classical view of line Radiation. Oscillator strength (3.5)
- Oscillator strength (quantum).
- Two-body atom with collisions (critical density).
SRK notes | 
The story of nebulium
- October 23
Students: please brush up relativity, including 4-vectors,
contravariant, covariant, summation and tensor algebra.
- 4.1 (Time dilation, length contraction, Doppler,Beaming)
- 4.2 (4-vectors; Co- and contra-variant vectors; Proper time)
"Co is low and that is all you need to know!"
- 4.3 (4-velocity, 4-wave vector)
- Homework 4
Relativistic beaming (gif
animation)
- October 28
- 4.3,4.4 (cursory review of tensors; E, B transformation))
- 4.5 (physical intution of E, B field transformation)
- 2.3 (The power spectrum of Poynting vector)
- 4.6 (E and B fields of moving charge)
SRK Internal notes
Master list for mid term exam.
- October 30
- 4.7 (Four four momentum, four acceleration, Lorentz force)
- 4.9 (Invariant Phase Volumes, Specific Intensity)
- 4.8 (Covariant Larmor Formula)
SRK-internal notes
 |  Purcell-Relativity
- November 4
In advance of the class please review first three pages of
SRK-internal notes.
I will start the class by
assuming these results.
- 4.8 (Beam pattern of Larmor emission)
- Introducing continuum processes of importance in astronomy
- 5.1 (Low-velocity Bremss)
- November 6
In advance of class, please review page 88 and section 4.6 of R&L.
- 5.2 (Thermal Bremss: emission)
- 5.3 (Thermal Bremss: absorption)
- 5.4 (Relativistic Bremss)
- November 7 (Makeup class)
- 8.1 (EM waves in plasma, dispersion relation and group velocity)
SRK-internal notes
What is dispersion measure?  | 
Waves in Plasma | 
The New SI system and
commentaries
- November 11
Please review QM of hydrogen atom
- 8.2 (Faraday Rotation)
- Hydrogen atom
SRK-internal notes
Homework 5
- November 13
- Zeeman splitting
- Spin-orbit coupling (fine structure)
- Hydrogen & Alkalis
SRK Internal  | 
History of Zeeman
splitting
- November 18
Please review QM of helium
- Binding energy of helium atom (successive approximations)
- Coulomb & Exchange integral
- Beginnings of L-S coupling
- Semi-forbidden transitions
SRK Internal
- November 20
- Multi-electron atoms (Central field approximation)->Periodic Table
- L-S coupling, combining valence electrons to yield terms
- Hund's rules
SRK internal  | 
Periodic Table  | 
Unix Program (2 and 3
electrons)  | 
J(0->0)
- November 25
- Selection Rules
- Hyperfine lines
- Intro to Synchrotron Radiation (Chapter 6)
SRK internal
Homework 6
Master List (Final
Exam)
- December 2
- Introduction to Compton Scattering (Chapter 7)
- December 5
- Synchrotron Emission (Chapter 6)
SRK internal