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The Standard Model and Beyond | |
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The Expanding Universe | |
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The Hubble Diagram | |
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Big Bang Nucleosynthesis | |
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The Cosmic Microwave Background | |
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Beyond the Standard Model | |
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Summary | |
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Exercises | |
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The Smooth, Expanding Universe | |
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General Relativity | |
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The Metric | |
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The Geodesic Equation | |
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Einstein Equations | |
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Distances | |
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Evolution of Energy | |
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Cosmic Inventory | |
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Photons | |
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Baryons | |
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Matter | |
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Neutrinos | |
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Dark Energy | |
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Epoch of Matter-Radiation Equality | |
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Summary | |
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Exercises | |
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Beyond Equilibrium | |
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Boltzmann Equation for Annihilation | |
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Big Bang Nucleosynthesis | |
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Neutron Abundance | |
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Light Element Abundances | |
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Recombination | |
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Dark Matter | |
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Summary | |
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Exercises | |
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The Boltzmann Equations | |
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The Boltzmann Equation for the Harmonic Oscillator | |
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The Collisionless Boltzmann Equation for Photons | |
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Zero-Order Equation | |
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First-Order Equation | |
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Collision Terms: Compton Scattering | |
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The Boltzmann Equation for Photons | |
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The Boltzmann Equation for Cold Dark Matter | |
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The Boltzmann Equation for Baryons | |
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Summary | |
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Exercises | |
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Einstein Equations | |
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The Perturbed Ricci Tensor and Scalar | |
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Christoffel Symbols | |
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Ricci Tensor | |
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Two Components of the Einstein Equations | |
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Tensor Perturbations | |
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Christoffel Symbols for Tensor Perturbations | |
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Ricci Tensor for Tensor Perturbations | |
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Einstein Equations for Tensor Perturbations | |
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The Decomposition Theorem | |
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From Gauge to Gauge | |
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Summary | |
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Exercises | |
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Initial Conditions | |
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The Einstein-Boltzmann Equations at Early Times | |
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The Horizon | |
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Inflation | |
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A Solution to the Horizon Problem | |
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Negative Pressure | |
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Implementation with a Scalar Field | |
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Gravity Wave Production | |
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Quantizing the Harmonic Oscillator | |
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Tensor Perturbations | |
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Scalar Perturbations | |
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Scalar Field Perturbations around a Smooth Background | |
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Super-Horizon Perturbations | |
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Spatially Flat Slicing | |
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Summary and Spectral Indices | |
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Exercises | |
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Inhomogeneities | |
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Prelude | |
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Three Stages of Evolution | |
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Method | |
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Large Scales | |
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Super-horizon Solution | |
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Through Horizon Crossing | |
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Small Scales | |
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Horizon Crossing | |
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Sub-horizon Evolution | |
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Numerical Results and Fits | |
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Growth Function | |
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Beyond Cold Dark Matter | |
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Baryons | |
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Massive Neutrinos | |
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Dark Energy | |
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Exercises | |
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Anisotropies | |
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Overview | |
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Large-Scale Anisotropies | |
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Acoustic Oscillations | |
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Tightly Coupled Limit of the Boltzmann Equations | |
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Tightly Coupled Solutions | |
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Diffusion Damping | |
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Inhomogeneities to Anisotropies | |
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Free Streaming | |
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The C[subscript l]'s | |
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The Anisotropy Spectrum Today | |
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Sachs-Wolfe Effect | |
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Small Scales | |
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Cosmological Parameters | |
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Curvature | |
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Degenerate Parameters | |
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Distinct Imprints | |
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Exercises | |
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Probes of Inhomogeneities | |
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Angular Correlations | |
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Peculiar Velocities | |
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Direct Measurements of Peculiar Velocities | |
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Redshift Space Distortions | |
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Galaxy Clusters | |
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Exercises | |
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Weak Lensing and Polarization | |
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Gravitational Distortion of Images | |
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Geodesics and Shear | |
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Ellipticity as an Estimator of Shear | |
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Weak Lensing Power Spectrum | |
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Polarization: The Quadrupole and the Q/U Decomposition | |
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Polarization from a Single Plane Wave | |
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Boltzmann Solution | |
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Polarization Power Spectra | |
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Detecting Gravity Waves | |
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Exercises | |
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Analysis | |
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The Likelihood Function | |
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Simple Example | |
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CMB Likelihood | |
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Galaxy Surveys | |
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Signal Covariance Matrix | |
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CMB Window Functions | |
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Examples of CMB Window Functions | |
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Window Functions for Galaxy Surveys | |
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Summary | |
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Estimating the Likelihood Function | |
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Karhunen-Loeve Techniques | |
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Optimal Quadratic Estimator | |
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The Fisher Matrix: Limits and Applications | |
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CMB | |
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Galaxy Surveys | |
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Forecasting | |
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Mapmaking and Inversion | |
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Systematics | |
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Foregrounds | |
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Mode Subtraction | |
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Exercises | |
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Solutions to Selected Problems | |
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Numbers | |
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Physical Constants | |
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Cosmological Constants | |
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Special Functions | |
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Legendre Polynomials | |
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Spherical Harmonics | |
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Spherical Bessel Functions | |
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Fourier Transforms | |
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Miscellaneous | |