Public repository of the Cosmic Linear Anisotropy Solving System (master for the most recent version of the standard code; GW_CLASS to include Cosmic Gravitational Wave Background anisotropies; classnet branch for acceleration with neutral networks; ExoCLASS branch for exotic energy injection; class_matter branch for FFTlog)
I am using the class code for calculating the power spectrum of an inflation potential with a special feature like a bump or dip. Can CLASS handle this type of potential for calculating the power spectrum? (It is basically a KKLT potential with a Gaussian bump/dip.) I have attached the graph of the potential vs scalar field below.
I am using the class code for calculating the power spectrum of an inflation potential with a special feature like a bump or dip. Can CLASS handle this type of potential for calculating the power spectrum? (It is basically a KKLT potential with a Gaussian bump/dip.) I have attached the graph of the potential vs scalar field below.
