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author | Aaron LI <aly@aaronly.me> | 2019-02-21 17:02:20 +0800 |
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committer | Aaron LI <aly@aaronly.me> | 2019-02-21 17:02:20 +0800 |
commit | a509266bf3ebdaf85d77b30fdc77d31ced442774 (patch) | |
tree | d727df1284dbc99a7f15887c4c331c1d580cd1dc | |
parent | 27dc87774ad6f63ed4ba68201bdfe7b9b4ca2587 (diff) | |
download | fg21sim-a509266bf3ebdaf85d77b30fdc77d31ced442774.tar.bz2 |
configs/spec: Adjust some min/max values for simplicity
-rw-r--r-- | fg21sim/configs/config.spec | 10 |
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. |