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authorAaron LI <aly@aaronly.me>2019-02-21 22:16:04 +0800
committerAaron LI <aly@aaronly.me>2019-02-21 22:16:04 +0800
commitf5a177103f37e68a7557e736e36097752cc3431e (patch)
tree1d772cb5fcaee3b1134ca9191630608ceb77877a /fg21sim/extragalactic
parent53e7aac0d1f2a59a94a43397d57d2721e8fc924f (diff)
downloadfg21sim-f5a177103f37e68a7557e736e36097752cc3431e.tar.bz2
clusters/halo: Update velocity_turb() against base turbulence
Take into account the base turbulence by using the newly added velocity_turb_base() method.
Diffstat (limited to 'fg21sim/extragalactic')
-rw-r--r--fg21sim/extragalactic/clusters/halo.py29
1 files changed, 16 insertions, 13 deletions
diff --git a/fg21sim/extragalactic/clusters/halo.py b/fg21sim/extragalactic/clusters/halo.py
index d027775..3c4ecd6 100644
--- a/fg21sim/extragalactic/clusters/halo.py
+++ b/fg21sim/extragalactic/clusters/halo.py
@@ -324,7 +324,7 @@ class RadioHalo1M:
return c_s * np.sqrt(3*self.x_turb / AC.gamma)
@lru_cache()
- def velocity_turb(self, t_merger):
+ def velocity_turb(self, t):
"""
Calculate the turbulence velocity dispersion.
@@ -338,9 +338,11 @@ class RadioHalo1M:
E_merger ≅ <ρ_gas> * v_i^2 * V_turb
V_turb = ᴨ * r_s^2 * (R_vir+r_s)
Turbulence energy:
- E_turb ≅ η_turb * E_merger ≅ 0.5 * M_turb * <v_turb^2>
+ E_turb ≅ 0.5 * M_turb * <v_turb^2>
+ ≅ 0.5 * M_turb * <v_turb_base^2> + η_turb * E_merger
=> Velocity dispersion:
- <v_turb^2> ≅ 2*η_turb * <ρ_gas> * v_i^2 * V_turb / M_turb
+ <v_turb^2> ≅ <v_turb_base^2> +
+ 2*η_turb * <ρ_gas> * v_i^2 * V_turb / M_turb
M_turb = int_0^R_turb[ ρ_gas(r)*4ᴨ*r^2 ]dr
where:
<ρ_gas>: mean gas density of the main cluster
@@ -355,12 +357,13 @@ class RadioHalo1M:
The turbulence velocity dispersion
Unit: [km/s]
"""
- self._validate_time(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_strip(t_merger) # [kpc]
- R_turb = self.radius_turb(t_merger) # [kpc]
+ self._validate_time(t)
+ z = COSMO.redshift(t)
+ M_main = self.mass_main(t)
+ M_sub = self.mass_sub(t)
+ r_s = self.radius_strip(t) # [kpc]
+ R_turb = self.radius_turb(t) # [kpc]
+ v_turb_base = self.velocity_turb_base(t) # [km/s]
rho_gas_f = helper.calc_gas_density_profile(
M_main+M_sub, z, f_rc=self.f_rc, beta=self.beta)
@@ -373,10 +376,10 @@ class RadioHalo1M:
rho_main *= AC.mu*AC.u * AUC.g2Msun * AUC.kpc2cm**3 # [Msun/kpc^3]
R_vir = helper.radius_cluster(M_main, z) # [kpc]
- V_turb = np.pi * r_s**2 * R_vir # [kpc^3]
- E_turb = self.eta_turb * rho_main * v_i**2 * V_turb
- v2_turb = 2 * E_turb / M_turb # [km^2/s^2]
- return np.sqrt(v2_turb) # [km/s]
+ volume = np.pi * r_s**2 * R_vir # [kpc^3]
+ E_add = self.eta_turb * rho_main * v_i**2 * volume
+ v2_turb = v_turb_base**2 + 2 * E_add / M_turb # [km/s]^2
+ return np.sqrt(v2_turb)
@lru_cache()
def tau_acceleration(self, t_merger):