Schema della sezione

  • 3.1 FRW metric 

    3.2 Relativistic cosmology

    3.3 Inflation

  • 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


  • 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


  • 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 

  • 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

  • 8.1 Brief thermal history

    8.2 Temperature anisotropy from recombination 

    8.3 Polarization anisotropy from recombination

  • 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