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We outline the modifications in the numerical Boltzmann code Cosmic Linear Anisotropy Solving System (CLASS) in order to include extra inflationary fields. The functioning of the code is first described, how and where modifications are meant to be do
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5e01615619eb5bfeeb7fb771b62f54fb
http://arxiv.org/abs/2105.09747
http://arxiv.org/abs/2105.09747