The Cosmic Linear Anisotropy Solving System (CLASS) III: Comparision with CAMB for LambdaCDM

By Julien Lesgourgues. 2011

144 citations recorded by the source corpus.

By confronting the two independent Boltzmann codes CLASS and CAMB, we establish that for concordance cosmology and for a given recombination history, lensed CMB and matter power spectra can be computed by current codes with an accuracy of 0.01%. We list a few tiny changes in CAMB which are necessary in order to reach such a level. Using the common limit of the two codes as a set of reference spectra, we derive precision settings corresponding to fixed levels of error in the computation of a CMB likelihood. We find that for a given precision level, CLASS is about 2.5 times faster than CAMB for computing the lensed CMB spectra of a LambdaCDM model. The nature of the main improvements in CLASS (which may each contribute to these performances) is discussed in companion papers.

Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics

View Paper: https://www.semanticscholar.org/paper/99b1eeb3e43009a2fce7ce35eb25a9391460ef95

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In Astronomy and Astrophysics

  1. L. Hernquist
  2. P. Hopkins
  3. Christopher J. Conselice
  4. Volker Springel
  5. Simon D. M. White
  6. A. Cimatti
  7. Robert Nichol
  8. Will J. Percival

In Nuclear and High Energy Physics

  1. Will J. Percival
  2. M. Viel
  3. Julien Lesgourgues
  4. Michele Moresco
  5. Thomas D. Kitching
  6. Martin Kunz
  7. E. Majerotto
  8. Ofer Lahav

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