814SM - COSMOLOGIA II 2022

Section outline

• Select section General

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  General

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• Select section 1. INTRODUCTION TO THE COURSE

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  1. INTRODUCTION TO THE COURSE
• Select section 2. OBSERVATIONAL FACTS

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  2. OBSERVATIONAL FACTS
• Select section 3. BACKGROUND OF COSMOLOGY

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  3. BACKGROUND OF COSMOLOGY

  3.1 FRW metric 
  

  3.2 Relativistic cosmology
  

  3.3 Inflation
  
• Select section 4. COSMOLOGICAL PERTURBATIONS

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  4. COSMOLOGICAL PERTURBATIONS

  4.1 Newtonian theory of linear perturbations
  

  4.2 Zeldovich approximation
  

  4.3 Adhesion approximation
  

  4.4 Relativistic theory
  

  4.5 Transfer functions
  

  4.6 Statistical properties
  

  4.7 Origin of cosmological perturbations
  

  
  
• Select section 5. GRAVITATIONAL COLLAPSE AND COLLISIONLESS DYNAMICS

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  5. GRAVITATIONAL COLLAPSE AND COLLISIONLESS DYNAMICS

  5.1 Spherical collapse
  

  5.2 Similarity solution of spherical collapse
  

  5.3 Collisionless dynamics

  5.4 Gravitational collapse
  

  5.5 Cosmological N-body and hydrodynamical simulations
  

  
  
• Select section 6. PROBING THE COSMIC DENSITY FIELD

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  6. PROBING THE COSMIC DENSITY FIELD

  6.1 Large-scale mass distribution
  

  6.2 Large-scale velocity field 
  

  6.3 Clustering in real and redshift space
  

  6.4 Clustering evolution
  

  6.5 Galaxy clustering 
  
• Select section 7. GRAVITATIONAL LENSING

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  7. GRAVITATIONAL LENSING

  7.1 Lensing from point-like objects
  

  7.2 Lensing from galaxies
  

  7.3 Lensing from galaxy clusters and from the large-scale structure of the Universe
  
• Select section 8. COSMIC MICROWAVE BACKGROUND

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  8. COSMIC MICROWAVE BACKGROUND

  8.1 Brief thermal history
  

  8.2 Temperature anisotropy from recombination 
  

  8.3 Polarization anisotropy from recombination
  
• Select section 9. FORMATION AND STRUCTURE OF DM HALOS

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  9. FORMATION AND STRUCTURE OF DM HALOS

  9.1 Halo mass function
  

  9.2 Progenitor distribution and merger trees
  

  9.3 Spatial clustering and bias
  

  9.4 Internal structure of DM halos
  

  9.5 The halo model of DM clustering
  

  
  
• Select section Topic 10

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  Topic 10