Instructor: Marc Kamionkowski
Bridge Annex 120
x2563
[email protected]
.
TAs: Walter Max-Moerbeck
Robinson 053
x6350
[email protected]
and
Yacine Ali-Hamoud
Robinson 053
[email protected]
The purpose of this class will be to learn about the various physical processes that produce the radiation (radio, IR, optical, UV, x-ray, gamma-ray) that we see from a variety of astrophysical sources.
Class times: Tuesdays and Thursdays. 1-2:30pm, Robinson 105
Class structure: The class will follow very
closely the textbook by Rybicki
and Lightman, with some additions from elsewhere.
Prerequisites: This is a class on astrophysical applications of electrodynamics, special relativity, quantum mechanics (atomic physics), and some very basic optics, and it is assumed that you have studied these subjects at the advanced undergraduate level. In particular, you should be familiar and have some facility with special relativity (Lorentz transformations), Maxwell's equations, electromagnetic waves, statistical mechanics (Maxwell-Boltzman, Fermi-Dirac, and Bose-Einstein distributions), quantum mechnics including the hydrogen atom and perturbation theory. If any of these subjects are not familiar to you, please see the instructor or a TA for suggestions on background reading.
Homework: There will be problem sets assigned almost weekly. It is imperative that you do these problem sets. This class is meant to provide you with valuable tools that can be applied in all areas of astronomy (and physics). Moreover, since class time is limited, there will be some topics that you work out on your own in the problem sets. Iwill try to find problem sets that involve application of the subjects studied in class, and I will try to avoid problems that involve excessive and pointless algebra. You should first try to do all of the problems by yourself. If you run into trouble, you may consult with classmates and attempt to work out the problems together. However, when you have figured out the solution, you should go your separate ways and then each write up the solutions from scratch.
Problem sets are due in class; there will be no extensions granted, and there will be no credit given for late homeworks. In return for being diligent about turning in problem sets on time, solutions will be handed out the day the problem sets are due.
Grade: 50% homework, 50% final exam. The final exam will be closed book and closed notes. To help you study, the test problems will be picked from a list of Rybicki and Lightman problems that will be provided well before the test.
Required Text: Radiative Processes for Astrophysics by Rybicki and Lightman
Additional Suggested Text: Interpreting Astronomical Spectra by Emerson
Some other related and possibly useful books (on reserve
in the astronomy library):
The
Physics of Astrophysics, Vol 1: Radiation by Frank Shu
(lectures notes on the subject)
Molecules
and Radiation, by Seinfeld (about molecules)
Spectroscopy
of astrophysical plasmas, ed by Dalgarno and Layzer
(a collection of review articles on astrophysical spectroscopy;
in particular, a good article on x-ray spectroscopy by McCray)
Astrophysics
of gaseous nebula, Donald E. Osterbrock
Classical
electrodynamics, John David Jackson (EM text)
The
classical theory of fields, L.D. Landau,
(EM text)
Galactic
and extragalactic radio astronomy,
Principles
of modern physics, Robert B. Leighton
Radio
astrophysics: nonthermal processes... ,A.G. Pacholczyk
Stellar
atmospheres, Dimitri Mihalas
Theory
of stellar spectra, V.V. Sobolev
Relevant Library Web Pages:
Caltech Library Services webpage
Ay121 course reserves
Syllabus
Here is a list of problems from which the final-exam problems will be chosen.
Homework 1, due in class, 11 October 2007