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-rw-r--r--fg21sim/extragalactic/clusters/halo.py33
-rw-r--r--fg21sim/extragalactic/clusters/solver.py15
2 files changed, 27 insertions, 21 deletions
diff --git a/fg21sim/extragalactic/clusters/halo.py b/fg21sim/extragalactic/clusters/halo.py
index 75789b6..ce4bcaf 100644
--- a/fg21sim/extragalactic/clusters/halo.py
+++ b/fg21sim/extragalactic/clusters/halo.py
@@ -182,7 +182,7 @@ class RadioHalo:
Returns
-------
- electron_spec : `~numpy.ndarray`
+ electron_spec : float 1D `~numpy.ndarray`
The solved electron spectrum at ``zend``.
Unit: [cm^-3]
"""
@@ -196,8 +196,7 @@ class RadioHalo:
tstop = COSMO.age(zend)
if n0_e is None:
# Accumulated constantly injected electrons until ``tstart``.
- n_inj = np.array([self.fp_injection(gm)
- for gm in self.gamma])
+ n_inj = self.fp_injection(self.gamma)
n0_e = n_inj * tstart
self.electron_spec = self.fpsolver.solve(u0=n0_e, tstart=tstart,
@@ -218,8 +217,8 @@ class RadioHalo:
Parameters
----------
- gamma : float
- Lorentz factor of electrons
+ gamma : float, or float 1D `~numpy.ndarray`
+ Lorentz factors of electrons
t : None
Currently a constant injection rate is assumed, therefore
this parameter is not used. Keep it for the consistency
@@ -227,8 +226,8 @@ class RadioHalo:
Returns
-------
- Qe : float
- Current electron injection rate at specified energy (gamma).
+ Qe : float, or float 1D `~numpy.ndarray`
+ Current electron injection rate at specified energies (gamma).
Unit: [cm^-3 Gyr^-1]
References
@@ -251,16 +250,16 @@ class RadioHalo:
Parameters
----------
- gamma : float
- The Lorentz factor of electrons
+ gamma : float, or float 1D `~numpy.ndarray`
+ The Lorentz factors of electrons
t : float
Current (cosmic) time when solving the equation
Unit: [Gyr]
Returns
-------
- diffusion : float
- Diffusion coefficient
+ diffusion : float, or float 1D `~numpy.ndarray`
+ Diffusion coefficients
Unit: [Gyr^-1]
References
@@ -283,8 +282,8 @@ class RadioHalo:
Returns
-------
- advection : float
- Advection coefficient, describing the energy loss/gain rate.
+ advection : float, or float 1D `~numpy.ndarray`
+ Advection coefficients, describing the energy loss/gain rates.
Unit: [Gyr^-1]
"""
advection = (abs(self._loss_ion(gamma, t)) +
@@ -394,16 +393,16 @@ class RadioHalo:
Parameters
----------
- gamma : float
- The Lorentz factor of electrons
+ gamma : float, or float 1D `~numpy.ndarray`
+ The Lorentz factors of electrons
t : float
The cosmic time/age
Unit: [Gyr]
Returns
-------
- loss : float
- The energy loss rate
+ loss : float, or float 1D `~numpy.ndarray`
+ The energy loss rates
Unit: [Gyr^-1]
References
diff --git a/fg21sim/extragalactic/clusters/solver.py b/fg21sim/extragalactic/clusters/solver.py
index dea7f3f..d7660b0 100644
--- a/fg21sim/extragalactic/clusters/solver.py
+++ b/fg21sim/extragalactic/clusters/solver.py
@@ -104,6 +104,13 @@ class FokkerPlanckSolver:
NOTE
----
+ All above functions should accept two parameters: ``(x, t)``,
+ where ``x`` is an 1D float `~numpy.ndarray` representing the adopted
+ logarithmic grid points along the spatial/energy axis, ``t`` is the
+ time of each solving step.
+
+ NOTE
+ ----
The diffusion coefficients (i.e., calculated by ``f_diffusion()``)
should be *positive* (i.e., C(x) > 0), otherwise unstable or wrong
results may occur, due to the current numerical scheme/algorithm
@@ -281,9 +288,9 @@ class FokkerPlanckSolver:
dx_phalf = self.dx_phalf
dx_mhalf = self.dx_mhalf
dt = self.tstep
- B = np.array([self.f_advection(x_, tc) for x_ in x])
- C = np.array([self.f_diffusion(x_, tc) for x_ in x])
- Q = np.array([self.f_injection(x_, tc) for x_ in x])
+ B = self.f_advection(x, tc)
+ C = self.f_diffusion(x, tc)
+ Q = self.f_injection(x, tc)
#
B_phalf = self.X_phalf(B)
B_mhalf = self.X_mhalf(B)
@@ -307,7 +314,7 @@ class FokkerPlanckSolver:
b[-1] = 1 + (dt/dx[-1]) * (C_mhalf[-1]/dx_mhalf[-1])*Wplus_mhalf[-1]
# Escape from the system
if self.f_escape is not None:
- T = np.array([self.f_escape(x_, tc) for x_ in x])
+ T = self.f_escape(x, tc)
b += dt / T
# Right-hand side
r = dt * Q + uc