Cosmological perturbation theory, CMB physics and their implementation in the CLASS code
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Lecture 1: General introduction to CLASS (motivations, overall structure, basic input and output, principle of the input module)
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Lecture 2: Homogeneous Cosmology and the background module
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Lecture 3: Thermal History and the thermodynamics module
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Lecture 4: Cosmological Perturbations and the perturbation module
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Lecture 5: Initial Conditions and the primordial module
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Lecture 6: Non-linear corrections and the nonlinear module. Harmonic transfer Functions and the transfer module
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Lecture 7: The spectra, lensing and output modules. Propspects and bibliography
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Focus on specialised topics in CLASS
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Lecture I: Advanced numerical numerical methods
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Lecture II: Implementation of massive neutrinos or other types of non-cold dark matter
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Lecture III: Implementation of polarisation and of spatial curvature
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Lecture IV: Implementation of non-trivial species (decaying dark matter, quintessence, ...)
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Lectures by Benjamin Audren: Parameter extraction and Monte Python
Big thanks to the organisers of this workshop and of the other CLASS Tour workshops, in particular:
Axel De La Macorra, Ivan Rodriguez,
Eiichiro Komatsu, Jochen Weller,
Dani Figueroa, Ruth Durrer,
Eugen Lim, Hiranya Peiris,
Licia Verde, Antonio Cuesta.
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