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| author | Aaron LI <aly@aaronly.me> | 2017-07-25 09:32:12 +0800 |
|---|---|---|
| committer | Aaron LI <aly@aaronly.me> | 2017-07-25 09:32:12 +0800 |
| commit | 2960ea13adf5d95b4bb2f6869d59186b2c9b2158 (patch) | |
| tree | bd21fe083064a78f63a3a445ba74bc60fd5eb66e /fg21sim/configs/20-extragalactic.conf.spec | |
| parent | e727de48313acacb55649893851674bb38fc3c72 (diff) | |
| download | fg21sim-2960ea13adf5d95b4bb2f6869d59186b2c9b2158.tar.bz2 | |
clusters/halo: Change config "eta_turb" to "beta_turb"
This configuration option "beta_turb" has different meaning as
"eta_turb" in [Cassano & Brunetti 2005], though they can both be an
indicator for the turbulence acceleration efficiency.
Rename this configuration option to make the difference more clear.
Signed-off-by: Aaron LI <aly@aaronly.me>
Diffstat (limited to 'fg21sim/configs/20-extragalactic.conf.spec')
| -rw-r--r-- | fg21sim/configs/20-extragalactic.conf.spec | 5 |
1 files changed, 2 insertions, 3 deletions
diff --git a/fg21sim/configs/20-extragalactic.conf.spec b/fg21sim/configs/20-extragalactic.conf.spec index b35507e..a48dbee 100644 --- a/fg21sim/configs/20-extragalactic.conf.spec +++ b/fg21sim/configs/20-extragalactic.conf.spec @@ -65,9 +65,8 @@ # Emission of giant radio halos from galaxy clusters [[halos]] - # Fraction of the turbulence energy in the form of magneto-sonic waves, - # which will channel into relativistic electrons. - eta_turb = float(default=0.3, min=0.0, max=1.0) + # Intensity of the turbulence acceleration. + beta_turb = float(default=0.3, min=0.1, max=2.0) # Ratio of the total energy injected into cosmic-ray electrons during # the cluster life to its total thermal energy. |