Class cosmology documentation

  • What is class cosmology?

    CLASS is one of the standard cosmology codes for evolving perturbations in the primordial universe into CMB and other power spectra, as well as various other quantities.
    This is a very preliminary interface to the general and powerful CLASS code..

  • The Cosmic Linear Anisotropy Solving System (CLASS) is a new accurate Boltzmann code, designed to offer a more user-friendly and flexible coding environment to cosmologists.
    CLASS is very structured, easy to modify, and offers a rigorous way to control the accuracy of output quantities.
CLASS is one of the standard cosmology codes for evolving perturbations in the primordial universe into CMB and other power spectra, as well as various other quantities. This is a very preliminary interface to the general and powerful CLASS code.
The purpose of CLASS is to simulate the evolution of linear perturbations in the universe and to compute CMB and large scale structure observables.

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