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Physics
Astrophysics and Cosmology
Cosmology
1. Foundations of Modern Cosmology
2. The Expanding Universe
3. The Standard Model of Cosmology
4. The Cosmic Microwave Background
5. Contents of the Universe
6. Structure Formation and Evolution
7. Observational Cosmology
8. Frontiers and Open Questions
Structure Formation and Evolution
Gravitational Instability Theory
Linear Perturbation Theory
Jeans Instability
Growth Rate Equations
Transfer Functions
Nonlinear Evolution
Spherical Collapse Model
Virial Theorem
Halo Formation
Initial Conditions
Primordial Fluctuations
Quantum Origin
Inflation-Generated Perturbations
Power Spectrum Shape
Gaussian Random Fields
Statistical Properties
Phase Correlations
Non-Gaussianity
Primordial Non-Gaussianity
Secondary Non-Gaussianity
Observational Constraints
Hierarchical Structure Formation
Bottom-Up Scenario
Small Structures First
Merging and Accretion
Dark Matter Halo Formation
Halo Mass Function
Halo Bias
Halo Profiles
NFW Profile
Einasto Profile
Baryonic Physics
Gas Cooling
Star Formation
Stellar Feedback
AGN Feedback
Large-Scale Structure
Galaxy Formation
Disk Galaxy Formation
Elliptical Galaxy Formation
Morphology-Density Relation
Galaxy Clustering
Two-Point Correlation Function
Redshift-Space Distortions
Bias Parameters
Groups and Clusters
Halo Occupation Distribution
Cluster Mass Function
Cluster Scaling Relations
Cosmic Web
Filamentary Structure
Void Properties
Topology Measurements
Computational Methods
N-Body Simulations
Dark Matter Only
Particle-Mesh Methods
Tree Algorithms
Resolution Limits
Hydrodynamical Simulations
SPH Methods
Grid-Based Methods
Subgrid Physics
Semi-Analytic Models
Merger Trees
Baryonic Physics Modeling
Galaxy Properties Prediction
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7. Observational Cosmology