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authorAaron LI <aly@aaronly.me>2019-01-26 15:20:38 +0800
committerAaron LI <aly@aaronly.me>2019-01-26 15:20:38 +0800
commit230c54b44958dbef49c0300d7479576c45e057c5 (patch)
treeed8977b5e27cee6e246d4418ebb176b870788030 /fg21sim/extragalactic
parent73883bf8ad77c9cfd2015b15af5af5fa73dbaf43 (diff)
downloadfg21sim-230c54b44958dbef49c0300d7479576c45e057c5.tar.bz2
clusters/halo: Use t_merger to be more explicit
Add _validate_t_merger() method to validate the given time to be an merger time.
Diffstat (limited to 'fg21sim/extragalactic')
-rw-r--r--fg21sim/extragalactic/clusters/halo.py38
1 files changed, 25 insertions, 13 deletions
diff --git a/fg21sim/extragalactic/clusters/halo.py b/fg21sim/extragalactic/clusters/halo.py
index 2b7994a..706426e 100644
--- a/fg21sim/extragalactic/clusters/halo.py
+++ b/fg21sim/extragalactic/clusters/halo.py
@@ -227,7 +227,7 @@ class RadioHalo1M:
return v_turb / cs
@lru_cache()
- def radius_turbulence(self, t):
+ def radius_turbulence(self, t_merger):
"""
The radius of the turbulence region, which is estimated as the
stripping radius ``r_s`` of the sub-cluster if ``r_s`` is larger
@@ -236,21 +236,23 @@ class RadioHalo1M:
Unit: [kpc]
"""
- z = COSMO.redshift(t)
- M_main = self.mass_main(t)
+ self._validate_t_merger(t_merger)
+ z = COSMO.redshift(t_merger)
+ M_main = self.mass_main(t_merger)
+ r_s = self.radius_stripping(t_merger)
r_c = self.f_rc * helper.radius_virial(M_main, z)
- r_s = self.radius_stripping(t)
return max([r_s, r_c])
@lru_cache()
- def radius_stripping(self, t):
+ def radius_stripping(self, t_merger):
"""
The stripping radius of the in-falling sub-cluster at time t.
Unit: [kpc]
"""
- z = COSMO.redshift(t)
- M_main = self.mass_main(t)
- M_sub = self.mass_sub(t)
+ self._validate_t_merger(t_merger)
+ z = COSMO.redshift(t_merger)
+ M_main = self.mass_main(t_merger)
+ M_sub = self.mass_sub(t_merger)
return helper.radius_stripping(M_main, M_sub, z,
f_rc=self.f_rc, beta=self.beta)
@@ -609,6 +611,14 @@ class RadioHalo1M:
"""
return self.age_merger
+ def _validate_t_merger(self, t_merger):
+ """
+ Validate that the given time ``t_merger`` is the time when the
+ merger begins, otherwise raise an error.
+ """
+ if not np.any(np.isclose(t_merger, self.age_merger)):
+ raise ValueError("Not a merger time: %s" % t_merger)
+
def mass_merged(self, t=None):
"""
The mass of the merged cluster.
@@ -655,7 +665,7 @@ class RadioHalo1M:
eta_b=eta_b, kT_out=kT_out)
@lru_cache()
- def _velocity_turb(self, t):
+ def _velocity_turb(self, t_merger):
"""
Calculate the turbulence velocity dispersion.
@@ -686,10 +696,12 @@ class RadioHalo1M:
The turbulence velocity dispersion
Unit: [km/s]
"""
- z = COSMO.redshift(t)
- M_main = self.mass_main(t)
- M_sub = self.mass_sub(t)
- R_turb = self.radius_turbulence(t) # [kpc]
+ self._validate_t_merger(t_merger)
+ z = COSMO.redshift(t_merger)
+ M_main = self.mass_main(t_merger)
+ M_sub = self.mass_sub(t_merger)
+ r_s = self.radius_stripping(t_merger) # [kpc]
+ R_turb = self.radius_turbulence(t_merger) # [kpc]
rho_gas_f = helper.calc_gas_density_profile(
M_main, z, f_rc=self.f_rc, beta=self.beta)