2. OBSERVATIONAL COSMOLOGY
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1 2. OBSERVATIONAL COSMOLOGY 1. OBSERVATIONAL PARAMETERS i. Introduction History of modern observational Cosmology ii. Cosmological Parameters The search for 2 (or more) numbers Hubble Parameter Deceleration Parameter Density Parameter Cosmological Constant and Dark Energy, Quintessence The Cosmological Parameters iii. The Age of the Universe Olber s Paradox How Old is our Universe Radioactive dating White Dwarf ages Globular Clusters Derivation for Cosmological Models The age problem iv. The Redshift Definition Derivation of cosmological redshift The Look Back Time v. Our Universe Supernova Project Results Hubble Key Project Results WMAP Results vi. Summary 2. THE COSMIC BACKGROUND RADIATION i. The Isotropic Background Olbers paradox Discovery of the background ii. The origin of the microwave background Recombination, Decoupling & the Surface of Last Scattering The Relic Background The physics of recombination iii. Observations of the CMB Temperature fluctuations Horizons and Fluctuations CMB Experiments
2 WMAP Polarization Measurements iv. Additional Background Light Components Backgrounds or Foregrounds? Cirrus Extragalactic Sources Contributions to the EBL from radio-x-ray wavelengths 3. STRUCTURE FORMATION IN THE UNIVERSE i. Isotropy of the Universe on the Largest Scales ii. The Growth of Structure Primordial Density Fluctuations The Jeans Length Formal Jeans Theory Jeans Mass, Silk Mass and Decoupling Growth of Perturbations in an expanding Universe iii. Structure Formation in a Dark Matter universe Dark Matter Hot Dark Matter Cold Dark Matter Structure Formation in a Dark Matter universe iv. The Power Spectrum Quantifying the power in the fluctuations The Transfer Function The Power Spectrum v. The Non-Linear Regime The Non-linear Regime The Zeldovich Approximation N-Body Simulations vi. Statistical Cosmology Quantifying Clustering The Correlation Function The Limber Equation Counts in Cells MST Genus Void Probability Functions Percolation Theory Counts in cells vii. Large Scale Surveys viii. Summary
3 4. THE COSMOLOGICAL DISTANCE SCALE i. Distance Indicators ii. Primary Distance Indicators Radar Echo Trigonometric Parallax Secular and Statistical Parallax Moving cluster Method Standard Rulers and Candles Main Sequence Fitting Spectroscopic Parallax Cepheid Variables RR Lyrae Variables iii. Secondary Distance Indicators Globular Clusters Tully Fisher Relation Faber-Jackson Relation Surface Brightness Fluctuations Brightest Cluster Members Supernova Measurements Gravitational Time Delay iv. The Distance Ladder v. The Hubble Key Project To the Hubble Flow Hubble Key Project Combination of Secondary Methods vi. Summary 5. OBSERVATIONAL TOOLS i. Cosmological Distances Proper Distance Luminosity Distance Proper Motion Distance Diameter Distance ii. The K-Correction iii. Galaxy Number Counts and Cosmology iv. Background Radiation
4 6. GALAXY NUMBER COUNTS i. Why Study Source Counts How Many Galaxies are there in the Universe? The Geometry of the Universe Population Contributions Evolution ii. Derivation Simple Euclidean Case Derivation of Source Counts Cosmology Luminosity Function Calculation of Luminosity Function K-Correction Evolution V/Vmax Test iii. Source Counts Results Integral and Differential Source Counts Number redshift Distributions Background Contributions iv. Multiwavelength Source Counts Optical Counts Morphological Evolution Near infrared Source Counts Infrared Source Counts Sub-mm Source Counts Radio Source Counts X-ray Source Counts v. Star Formation History vi. The Future vii. Summary 7. THE EVOLVING UNIVERSE i. The Star Formation History of the Universe ii. The First Galaxies Ly alpha emitters Absorption Systems The Epoch of Re-ionization iii. Galaxy Formation and Evolution AGN IR Galaxies Lyman Break Galaxies Sub-mm Galaxies iv. Galaxy Surveys and Redshift Surveys
5 8. COSMOLOGY JOURNAL PRESENTATION i. 2 OHP ii. 10 mins
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