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The Cosmic Linear Anisotropy Solving System (CLASS) II: Approximation schemes
Boltzmann codes are used extensively by several groups for constraining cosmological parameters with Cosmic Microwave Background and Large Scale Structure data. This activity is computationally expensive, since a typical project requires from 10'000 to 100'000 Boltzmann code executions. Th...
| Autores principales: | , , |
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| Lenguaje: | eng |
| Publicado: |
2011
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| Materias: | |
| Acceso en línea: | https://dx.doi.org/10.1088/1475-7516/2011/07/034 http://cds.cern.ch/record/1345132 |