Please see
R. Xu, D. Xu, L. Andersson, P. Amaro-Seoane, and L. Shao, Bumblebee cosmology: The FLRW solution and the CMB temperature anisotropy
for reference.
Usage:
- Write input parameters in bumblebee_input_data.txt (
$H_0, \Omega_{b0}, \Omega_{c0}, T_{\rm CMB}, n_s, \alpha, q_0$ ) - Run bumblebeecmb_1.nb (takes about 1 hr)
- Run bumblebeecmb_2.py (takes about 1 hr)
-
bumblebee_cl_data.txt is the output for
$l(l+1)C_l/2\pi$ vs.$l$