Ast/Phys 5022 - Cosmology (Fall 2008)
Syllabus & Grading
Presentations
Schedule and Topics
Homework
Tue Sep 09: Problem Set #1 (due Sep 16)
Tue Sep 16: Problem Set #2 (due Sep 23)
Tue Sep 23: No problem set
Tue Oct 07: Problem Set #3 (due Oct 14)
Thu Oct 16: Problem Set #4 (due Oct 23)
Tue Nov 18: Problem Set #5 (due Nov 25/Dec 1)
Grades
here
Lecture Notes
Relativity
Global Geometry
Inflation
Early Universe
Cosmic Microwave Background
CMB acoustic peaks - Nov 18 PPT lecture
CMB polarization - Nov 20 PPT lecture
Structure Formation
Structure Formation - Nov 20 PPT lecture
Structure Formation - Nov 25 lecture
Resources
astro-ph: preprint archive
NASA ADS paper archive
Ned Wright's Cosmology Tutorial
Brief history of the Universe -1
Brief history of the Universe - 2
Global Cosmological Parameters
Dynamical evolution of various models:
Flat;
Lambda=0;
-ve Lambda;
+ve Lambda;
all
Expansion age of the Universe models
Particle and Event Horizons in 2 models
Supernova Cosmology Project
astro-ph/0603449, see p.28, p.54, p.57, p.58
astro-ph/0409131, "The current status of observational cosmology" see p.6
see the last picture: P(k) from
CMB and galaxy clustering
Methods of measuring the Hubble constant, H0
Sunyaev-Zeldovich Effect
Galaxy Gravitational Lenses
Water Masers (see 1st talk, p.9)
Distance Ladder
Distance Ladder - summary of methods
Cosmic Microwave Background (CMB)
Gravitational lensing time delays (see p.10,11,12)
Summary of H0 estimates, arXiv:0802.3219 (p.24)
Evolution of structure in the Universe
2dF Galaxy Redshift Survey
Two micron all sky galaxy survey
A compilation of things, by Martin White (UCB)
A popular-level version of P(k); M.Tegmark)
A few exampls of Real vs Fourier space - see p.5
astro-ph/0409131, "The current status of observational cosmology" see p.3
Formation of the Milky Way type galaxy in high resolution N-body simulation
More matter power spectra P(k)
astro-ph/0212552, see ...
astro-ph/0608632, see p.31
astro-ph/0603449, see p.24
Baryogenesis and CPT theorem
Parity Violation - an article from Los Alamos Science
CERN site
Big Bang Nucleosynthesis (BBN)
Time evolution of species density
Abundance vs. baryon/photon ratio
Helium mass fraction
BBN predictions vs. observations + CMB (see p.51,53)
He-4,D,He-3,Li-7
Observed abundance of Li-7