Right now we assume in 21cmFAST that the photon temperature, T_gamma, is identical to the CMB temperature. It would be great to relax this assumption and have the ability to simulate extra radio background in v4 (e.g. https://arxiv.org/pdf/2411.08134, where this work has been implemented in v3).
Right now we assume in
21cmFASTthat the photon temperature,T_gamma, is identical to the CMB temperature. It would be great to relax this assumption and have the ability to simulate extra radio background in v4 (e.g. https://arxiv.org/pdf/2411.08134, where this work has been implemented in v3).