814SM - COSMOLOGIA II 2016

Section outline

• Select section General

  General

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  • Select activity Annunci

    

    Annunci Forum
• Select section 1. INTRODUCTION TO THE COURSE

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

  2. OBSERVATIONAL FACTS
• Select section 3. BACKGROUND OF COSMOLOGY 3.1 FRW metric 3.2 Relativistic cosmology 3.3 Inflation

  3. BACKGROUND OF COSMOLOGY 3.1 FRW metric 3.2 Relativistic cosmology 3.3 Inflation
• Select section 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

  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 5.1 Spherical collapse 5.2 Similarity solution of spherical collapse 5.3 Collapse of homogeneous ellipsoid 5.4 Collisionless dynamics 5.5 Gravitational collapse 5.6 N-body simulations

  5. GRAVITATIONAL COLLAPSE AND COLLISIONLESS DYNAMICS 5.1 Spherical collapse 5.2 Similarity solution of spherical collapse 5.3 Collapse of homogeneous ellipsoid 5.4 Collisionless dynamics 5.5 Gravitational collapse 5.6 N-body simulations
• Select section 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

  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 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

  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 8.1 Brief thermal history 8.2 Temperature anisotropy from recombination 8.3 Polarization anisotropy from recombination

  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 9.1 Density peaks 9.2 Halo mass function 9.3 Progenitor distribution and merger trees 9.4 Spatial clustering and bias 9.5 Internal structure of DM halos 9.6 The halo model of DM clustering

  9. FORMATION AND STRUCTURE OF DM HALOS 9.1 Density peaks 9.2 Halo mass function 9.3 Progenitor distribution and merger trees 9.4 Spatial clustering and bias 9.5 Internal structure of DM halos 9.6 The halo model of DM clustering
• Select section Topic 10

  Topic 10