Syllabus -- PtyS 505B (Hubbard)

Spring semester, 2008

I. Physics of high pressure

A. T=0 equations of state

1. astrophysical limit -- ideal Fermi gas

2. corrections to the ideal Fermi gas

3. metallic hydrogen

4. experimental methods

B. T > 0 equations of state

1. Mie-Grüneisen theory

2. Debye theory

3. theories of melting

4. liquid-state theories (MC, MD, HSP, etc.)

5. experimental methods -- single and multiple shocks

II. Planetary interiors

A. spherical planets in hydrostatic equilibrium

1. polytropes

2. relation between pressure-density and mass-radius

3. Adams-Williamson equation

B. static distorted planets

1. spherical harmonic representations

2. moments of inertia

3. gravity anomalies

C. classical theories of rotating planets

1. Maclaurin and Jacobi theory (density = const.)

2. Clairaut and other perturbation theories (density not = const.)

D. tidal distortion

1. hydrostatic response

2. love numbers

E. energy sources in planets

1. gravitational binding energy

2. thermal energy

3. radioactivity

4. tidal dissipation (continued in III-C)

III. Celestial mechanics

A. 2-body problem

1. reduction to 1-body problem

2. Kepler's laws

3. orbital elements

4. effect of oblateness on an orbiting body

B. rigid-body motion

1. moment of inertia tensor

2. angular momentum of a rigid body

3. Euler's equations

4. effect of dissipation

C. tidal torques

1. angular momentum transfer and heating

2. spin-orbit coupling


There will be two midterm examinations. The first midterm is now scheduled on 26 February and the second midterm is scheduled for 3 April.The format for the midterms will be open notes, calculators/laptops permitted.

 

Approximately ten homework assignments will be made. Some of these will require numerical calculations, so some proficiency in a programming language will be needed.
 

I program in IDL and fortran, and can be of the most assistance to you in these languages. Some of the calculations may be amenable to spreadsheets such as Excel.
 

The final examination will be comprehensive, and will be in the same format as the midterms. The actual date and time of the final is negotiable.

 

Collaboration on homework assignments is permitted, but if this occurs, please indicate on your assignment who did what.


Algorithm for computing your final composite score:

composite = 0.2 X MT1 + 0.2 X MT2 + 0.25 X homework + 0.35 X final