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This branch was used for the KiDS-1000 beyond flat LCDM paper. We should probably merge and/or tag this version.

tilmantroester and others added 30 commits August 28, 2020 13:53
Now linear spectrum is (D^2(k,z)/D_LCDM^2(z=0)) x P_CAMB(z=0)
Added Lin_Grow function which just outputs linear growth in the Real cosmology
Added Lin_Grow to HALO class
Doubled spline points to linear_growth and increased range
…R,FR,DGP and propagated the additional parameter (model) to init functions
…in SPT and to some usages of mu in the bispectrum library BSPTN.cpp
…r linear growth splining), and in the reaction parameter initialisation function react_init
…ute_reaction. model should be specified along with massloop in the pipeline script and take values 1:GR, 2:fr, 3:dgp
…ute_reaction. model should be specified along with massloop in the pipeline script and take values 1:GR, 2:fr, 3:dgp. Default set to 2:fR.
note for Tilman on mode and model params to select gravity
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3 participants