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authorAaron LI <aly@aaronly.me>2017-10-30 14:01:43 +0800
committerAaron LI <aly@aaronly.me>2017-10-30 14:01:43 +0800
commit0e22ac44e5893da2d66e61682bd340a8e6cc8cff (patch)
tree48ab79272dbd25fefd8031422b452a3dd5d3898b /fg21sim
parentd41ceb35e8f4598b0e0fb0e5a0c0bf06a11e53a0 (diff)
downloadfg21sim-0e22ac44e5893da2d66e61682bd340a8e6cc8cff.tar.bz2
clusters/halo: Tune default parameters
Diffstat (limited to 'fg21sim')
-rw-r--r--fg21sim/configs/20-extragalactic.conf.spec8
1 files changed, 4 insertions, 4 deletions
diff --git a/fg21sim/configs/20-extragalactic.conf.spec b/fg21sim/configs/20-extragalactic.conf.spec
index 664ce0e..aef5151 100644
--- a/fg21sim/configs/20-extragalactic.conf.spec
+++ b/fg21sim/configs/20-extragalactic.conf.spec
@@ -20,7 +20,7 @@
# The model of the fitting function for halo mass distribution
# For all models and more details:
# https://hmf.readthedocs.io/en/latest/_autosummary/hmf.fitting_functions.html
- model = option("smt", "jenkins", "ps", default="smt")
+ model = option("smt", "jenkins", "ps", default="ps")
# The minimum (inclusive) and maximum (exclusive!) halo mass (dark
# matter only) within which to calculate the halo mass distribution.
@@ -117,7 +117,7 @@
# Mass ratio of the main and sub clusters, below which is regarded as
# a major merger event.
- ratio_major = float(default=3.0, min=1.0, max=10.0)
+ ratio_major = float(default=5.0, min=1.0, max=10.0)
# Whether to use the maximum merger event (i.e., biggest mass of the
# sub cluster) within the above ``tau_merger`` timescale to simulate the
@@ -169,11 +169,11 @@
# Ratio of the total energy injected into cosmic-ray electrons during
# the cluster life to its total thermal energy.
- eta_e = float(default=0.003, min=0.001, max=0.1)
+ eta_e = float(default=0.001, min=0.001, max=0.1)
# Electron injection, which is assumed to have a constant injection
# rate and a power-law spectrum.
- injection_index = float(default=2.4, min=2.1, max=3.5)
+ injection_index = float(default=2.3, min=2.1, max=3.5)
# Minimum and maximum Lorentz factor (i.e., energy) of the relativistic
# electron spectrum.