Today: Reminders/Assignments | |
Longair, Ch. 5-6 | |
- Getting into Theory/GR (Ch. 5+) | |
- Hogg papers | |
Unless noted, all figs and eqs from Longair. | |
Mini-Exgal-TAC on Friday | ||
Any questions at this stage? | ||
Try not to discuss with each other too much in advance, that will happen Friday | ||
Register an account on MAST? | ||
WIRO over spring break: | ||
Camera on and working, clusters selected | ||
I’ll go 1-3 nights – who else? | ||
Discuss logistics | ||
No class on Wed. March 26 | ||
Next Friday in place of our usual astro-ph preprint discussion. | |
12 proposals, everyone has two primary proposals to lead the discussion about, plus two secondary proposals. | |
Everyone must read all proposals and note strengths and weaknesses, and assign a preliminary grade (1=best, 5=worst), in accordance with guidelines. | |
I’ll chair the meeting and evaluate performance. I expect this will be a challenging but very educational experience. |
Section 5.1, the “Cosmological Principle” | ||
Isotropic, homogenous, uniform expansion | ||
Can write relativistic equations in different forms (famous names cited here…) | ||
Weyl’s postulate: “The particles of the substratum (representing the nebulae) lie in space-time on a bundle of geodesics diverging from a porint in the (finite or infinite) past.” |
Section 5.1, the “Cosmological Principle” | ||
Geodesics are “world-lines” of galaxies and do not intersect except at a singular point in the past. Weyl’s idea predates Hubble’s law. | ||
Fundamental observers on each world line, each with standard clock measuring cosmic time from that singular point. | ||
“We are not located at any special location in the universe.” |
Sections 5.1-5.4 cover underpinnings of GR (curved spaces, space-time metrics) and in particular the Robertson-Walker metric that we will need to describe the universe. | |
Read and follow these sections, but we don’t have the lecture time to go into much detail with the perspective of observational astronomers in a mixed galaxies/cosmology course. |
Section 5.5 covers observables. We’re going to jump to the chase momentarily and walk through Hogg (2000), which integrates this material with world models (Chapter 7, and a Sandage review article I will probably assign soon.) |
Chapter 6 introduces General Relativity, which I won’t go over in class. Again, read through it. I expect to cover chapter 7 following spring break. | |
WIRO and an observing manual are the “homework” over spring break…I hope! |