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)
218
stars
291
forks
source link
calculate the transition functions in the future (z<0) #573
I am interested in the power spectrum of neutrinos and I want to see the power spectrum in the future.
How can I make CLASS continue calculating the transition functions after z=0?
Hello,
I am interested in the power spectrum of neutrinos and I want to see the power spectrum in the future. How can I make CLASS continue calculating the transition functions after z=0?
Thanks a lot! Cheers Yunzhi