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-rw-r--r--fg21sim/extragalactic/clusters/halo.py20
1 files changed, 10 insertions, 10 deletions
diff --git a/fg21sim/extragalactic/clusters/halo.py b/fg21sim/extragalactic/clusters/halo.py
index 160ab96..f69c1cc 100644
--- a/fg21sim/extragalactic/clusters/halo.py
+++ b/fg21sim/extragalactic/clusters/halo.py
@@ -761,17 +761,15 @@ class RadioHalo:
Advection coefficients, describing the energy loss/gain rates.
Unit: [Gyr^-1]
"""
- # Always use the properties at ``age_merger`` to derive the
- # initial electron spectrum.
if t < self.age_merger:
- # NOTE: subtract ``time_step`` to make sure ``fp_diffusion()``
- # gives no acceleration.
- t = self.age_merger - self.time_step
-
- gamma = np.asarray(gamma)
- advection = (abs(self._loss_ion(gamma, t)) +
- abs(self._loss_rad(gamma, t)) -
- (self.fp_diffusion(gamma, t) * 2 / gamma))
+ # To derive the initial electron spectrum
+ advection = (abs(self._loss_ion(gamma, self.age_merger)) +
+ abs(self._loss_rad(gamma, self.age_merger)))
+ else:
+ # Turbulence acceleration and beyond
+ advection = (abs(self._loss_ion(gamma, t)) +
+ abs(self._loss_rad(gamma, t)) -
+ (self.fp_diffusion(gamma, t) * 2 / gamma))
return advection
def _mass(self, t):
@@ -844,6 +842,7 @@ class RadioHalo:
----------
Ref.[sarazin1999],Eq.(9)
"""
+ gamma = np.asarray(gamma)
z = COSMO.redshift(t)
mass = self._mass(t)
n_th = helper.density_number_thermal(mass, z) # [cm^-3]
@@ -859,6 +858,7 @@ class RadioHalo:
----------
Ref.[sarazin1999],Eq.(6,7)
"""
+ gamma = np.asarray(gamma)
B = self._magnetic_field(t) # [uG]
z = COSMO.redshift(t)
loss = -4.32e-4 * gamma**2 * ((B/3.25)**2 + (1+z)**4)