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authorAaron LI <aly@aaronly.me>2019-02-21 17:02:20 +0800
committerAaron LI <aly@aaronly.me>2019-02-21 17:02:20 +0800
commita509266bf3ebdaf85d77b30fdc77d31ced442774 (patch)
treed727df1284dbc99a7f15887c4c331c1d580cd1dc
parent27dc87774ad6f63ed4ba68201bdfe7b9b4ca2587 (diff)
downloadfg21sim-a509266bf3ebdaf85d77b30fdc77d31ced442774.tar.bz2
configs/spec: Adjust some min/max values for simplicity
-rw-r--r--fg21sim/configs/config.spec10
1 files changed, 5 insertions, 5 deletions
diff --git a/fg21sim/configs/config.spec b/fg21sim/configs/config.spec
index 556c662..0ab5843 100644
--- a/fg21sim/configs/config.spec
+++ b/fg21sim/configs/config.spec
@@ -385,27 +385,27 @@ stream = option("stderr", "stdout", "", default="stderr")
f_radius = float(default=1, min=0.1, max=10)
# The fraction of merger energy transferred into the turbulence.
- eta_turb = float(default=0.1, min=0.1, max=0.5)
+ eta_turb = float(default=0.1, min=0, max=1)
# The fraction of the thermal energy injected into the cosmic-ray
# electrons during the cluster life time.
- eta_e = float(default=0.003, min=0.001, max=0.1)
+ eta_e = float(default=0.003, min=0, max=1)
# The energy density ratio of cosmic ray to the thermal ICM.
# NOTE: Equipartition between the magnetic field and cosmic ray is
# assumed, i.e., eta_b == x_cr.
- x_cr = float(default=0.015, min=0.001, max=0.1)
+ x_cr = float(default=0.015, min=0, max=1)
# The scaling index of the diffusion coefficient (D_γγ) w.r.t. the
# mass of the cluster.
- mass_index = float(default=0, min=0, max=2)
+ mass_index = float(default=0, min=0, max=3)
# The scaling index of the halo radius (R_halo) w.r.t. the virial
# radius of the cluster.
radius_index = float(default=0, min=0, max=3)
# The spectral index of the injected primary electrons.
- injection_index = float(default=2.3, min=2.1, max=3.0)
+ injection_index = float(default=2.3, min=2, max=3)
# Minimum and maximum Lorentz factor (i.e., energy) of the relativistic
# electron spectrum.