From 00fccbb7e2491741f82e6603a37fe1a12af74c95 Mon Sep 17 00:00:00 2001
From: Aaron LI <aly@aaronly.me>
Date: Tue, 30 Oct 2018 21:30:30 +0800
Subject: clusters/halo: Update calculations of injection and halo radius

---
 fg21sim/extragalactic/clusters/halo.py   | 14 ++++++++++++-
 fg21sim/extragalactic/clusters/helper.py | 35 --------------------------------
 2 files changed, 13 insertions(+), 36 deletions(-)

(limited to 'fg21sim/extragalactic/clusters')

diff --git a/fg21sim/extragalactic/clusters/halo.py b/fg21sim/extragalactic/clusters/halo.py
index eac9501..baa1a36 100644
--- a/fg21sim/extragalactic/clusters/halo.py
+++ b/fg21sim/extragalactic/clusters/halo.py
@@ -234,7 +234,7 @@ class RadioHalo:
         The estimated radius for the simulated radio halo.
         Unit: [kpc]
         """
-        return helper.radius_halo(self.M_obs, self.z_obs, configs=self.configs)
+        return self.injection_radius
 
     @property
     def angular_radius(self):
@@ -362,6 +362,18 @@ class RadioHalo:
             tau = tau_max
         return tau
 
+    @property
+    @lru_cache
+    def injection_radius(self):
+        """
+        The radius of the turbulence injection regions, and then the
+        injection scale: L_turb ~= 2*R_turb.
+        Unit: [kpc]
+        """
+        rs = helper.radius_stripping(self.M_main, self.M_sub, self.z_merger,
+                                     configs=self.configs)  # [kpc]
+        return self.f_lturb * rs
+
     @property
     @lru_cache()
     def injection_rate(self):
diff --git a/fg21sim/extragalactic/clusters/helper.py b/fg21sim/extragalactic/clusters/helper.py
index ecbb866..96800e4 100644
--- a/fg21sim/extragalactic/clusters/helper.py
+++ b/fg21sim/extragalactic/clusters/helper.py
@@ -129,41 +129,6 @@ def radius_virial(mass, z=0.0):
     return R_vir * AUC.cm2kpc  # [kpc]
 
 
-def radius_halo(mass, z=0.0, configs=CONFIGS):
-    """
-    Estimate the radius of (giant) radio halo.
-
-    NOTE
-    ----
-    The halo radius is estimated to be the same as the turbulence
-    injection scale, i.e.:
-        R_halo ≅ L_turb ≅ R_vir / 3
-    where R_vir the virial radius of the merged (observed) cluster.
-
-    Reference: [vazza2011],Sec.(3.6)
-
-    Parameters
-    ----------
-    mass : float, `~numpy.ndarray`
-        Cluster virial mass.
-        Unit: [Msun]
-    z : float, `~numpy.ndarray`, optional
-        Redshift
-        Default: 0.0 (i.e., present day)
-
-    Returns
-    -------
-    R_halo : float, `~numpy.ndarray`
-        Radius of the (simulated/predicted) giant radio halo
-        Unit: [kpc]
-    """
-    # Turbulence injection scale factor
-    key = "extragalactic/halos/f_lturb"
-    f_lturb = configs.getn(key)
-    R_halo = f_lturb * radius_virial(mass=mass, z=z)  # [kpc]
-    return R_halo
-
-
 def radius_stripping(M_main, M_sub, z, configs=CONFIGS):
     """
     Calculate the stripping radius of the in-falling sub-cluster, which
-- 
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