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authorAaron LI <aly@aaronly.me>2017-10-21 22:13:42 +0800
committerAaron LI <aly@aaronly.me>2017-10-21 22:13:42 +0800
commit2ee32e7196f83a9350a2b83c03846f6282d7ffe9 (patch)
tree7171acc49e70b31ef796c4a58f262c0367a6972f /fg21sim/extragalactic/pointsources/radioquiet.py
parenta8a02a96a78a85ffacf52aa43c158ecc24391af3 (diff)
downloadfg21sim-2ee32e7196f83a9350a2b83c03846f6282d7ffe9.tar.bz2
clusters/halo: Rewrite turbulence acceleration & diffusion coefficient!
The previous calculation of the turbulence acceleration efficiency has significant problems, which is too low, i.e., the acceleration timescale is too large (~10 Gyr). However, it is reported that turbulent acceleration has a timescale ~100 Myr (0.1 Gyr). I believe this problem is due to the over-simplification to the formula proposed by [cassano2005]. Rewrite the turbulence acceleration and diffusion coefficient calculations, adopting the method proposed by [brunetti2016]. To this end, two new options "f_lturb" and "f_acc" are introduced to tune the results.
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