Relativistic Astrophysics and Cosmology
From AstroBaki
Revision as of 10:14, 19 January 2017 by Aparsons (talk | contribs) (→Lecture 2: Friedmann equation; equation of state; radiation, matter, dark energy [Ch 3,4,5])
Elements of general relativity. Physics of pulsars, cosmic rays, black holes. The cosmological distance scale, elementary cosmological models, properties of galaxies and quasars. The mass density and age of the universe. Evidence for dark matter and dark energy and concepts of the early universe and of galaxy formation. Reflections on astrophysics as a probe of the extrema of physics.
Logistics
- Syllabus
- Class Repository: http://github.com/AaronParsons/astro161
- C161 on BCourses
- Main Text: Ryden, "Introduction to Cosmology" 2nd Ed. (The 1st Ed. is good, but out of date.)
Topics by Date
The Smooth Universe
Lecture 1: The Cosmological Principle; Hubble parameter H; scale factor a [Ch 1,2]
- Topics
- Cosmological Principle, intro to our universe
- Hubble's Law and Scale Factors
- Lorentz transformations
- class mechanics
- syllabus
- tools for figuring stuff out
- theoretical derivation
- order-of-magnitude estimation
- physical intuition (hands-on modeling, analogies)
- numerical simulation/programming
Lecture 2: Friedmann equation; equation of state; radiation, matter, dark energy [Ch 3,4,5]
Density parameter Omega; open, flat, closed cosmological models [Ch 6]
Time evolution of H, Omega, and a [Ch 7]
Rudiments of general relativity; the Robertson-Walker metric [Ch 8, A1]
Basic kinematic properties: distance-redshift, time-redshift, age, angular sizes [A2]