814SM - COSMOLOGIA II 2019

Schema della sezione

• Seleziona sezione Introduzione

  Introduzione

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  • Seleziona attività Annunci

    

    Annunci Forum
• Seleziona sezione 1. INTRODUCTION TO THE COURSE

  1. INTRODUCTION TO THE COURSE
• Seleziona sezione 2. OBSERVATIONAL FACTS

  2. OBSERVATIONAL FACTS
• Seleziona sezione 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
• Seleziona sezione 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
• Seleziona sezione 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
• Seleziona sezione 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
• Seleziona sezione 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
• Seleziona sezione 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
• Seleziona sezione 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
• Seleziona sezione Topic 10

  Topic 10