diff options
Diffstat (limited to 'fg21sim/extragalactic/clusters/emission.py')
| -rw-r--r-- | fg21sim/extragalactic/clusters/emission.py | 44 |
1 files changed, 41 insertions, 3 deletions
diff --git a/fg21sim/extragalactic/clusters/emission.py b/fg21sim/extragalactic/clusters/emission.py index 5c9e0a7..74e6ec8 100644 --- a/fg21sim/extragalactic/clusters/emission.py +++ b/fg21sim/extragalactic/clusters/emission.py @@ -17,6 +17,8 @@ import logging import numpy as np import scipy.integrate import scipy.special +from scipy import integrate +from scipy import interpolate from ...utils import COSMO from ...utils.units import (Units as AU, @@ -99,10 +101,46 @@ class SynchrotronEmission: def F(x): """ Synchrotron kernel function. + + NOTE + ---- + Use interpolation to optimize the speed, also avoid instabilities + near the lower end (e.g., x < 1e-5). + Interpolation also helps vectorize this function for easier calling. + + Parameters + ---------- + x : `~numpy.ndarray` + Points where to calculate the kernel function values. + NOTE: X values will be bounded, e.g., within [1e-5, 20] + + Returns + ------- + y : `~numpy.ndarray` + Calculated kernel function values. """ - val = x * scipy.integrate.quad(lambda t: scipy.special.kv(5/3, t), - a=x, b=np.inf)[0] - return val + # The lower and upper cuts + xmin = 1e-5 + xmax = 20.0 + # Number of samples within [xmin, xmax] + # NOTE: this kernel function is quiet smooth and slow-varying. + nsamples = 128 + # Make an interpolation + x_interp = np.logspace(np.log10(xmin), np.log10(xmax), + num=nsamples) + F_interp = [ + xp * integrate.quad(lambda t: scipy.special.kv(5/3, t), + a=xp, b=np.inf)[0] + for xp in x_interp + ] + func_interp = interpolate.interp1d(x_interp, F_interp, + kind="quadratic") + + x = np.array(x) # Make a copy! + x[x < xmin] = xmin + x[x > xmax] = xmax + y = func_interp(x) + return y def emissivity(self, nu): """ |