2016-03-27 12:56:54 +03:00
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import numpy as np
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2016-03-27 13:16:37 +03:00
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from qpms_c import *
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2016-03-27 12:56:54 +03:00
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ň = np.newaxis
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2016-07-18 13:03:33 +03:00
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import scipy
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2016-03-27 12:56:54 +03:00
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from scipy.constants import epsilon_0 as ε_0, c, pi as π, e, hbar as ℏ, mu_0 as μ_0
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eV = e
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2017-03-17 07:19:57 +02:00
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from scipy.special import lpmn, lpmv, sph_jn, sph_yn, poch, gammaln
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2016-03-27 12:56:54 +03:00
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from scipy.misc import factorial
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import math
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import cmath
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2016-07-12 03:20:53 +03:00
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import quaternion, spherical_functions as sf # because of the Wigner matrices
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2016-07-18 15:58:55 +03:00
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import sys, time
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2016-12-04 22:27:03 +02:00
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2017-05-08 20:13:34 +03:00
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"""
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2016-12-04 22:27:03 +02:00
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'''
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Try to import numba. Its pre-0.28.0 versions can not handle functions
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containing utf8 identifiers, so we keep track about that.
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'''
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try:
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import numba
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use_jit = True
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if numba.__version__ >= '0.28.0':
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use_jit_utf8 = True
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else:
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use_jit_utf8 = False
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except ImportError:
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use_jit = False
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use_jit_utf8 = False
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'''
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Accordingly, we define our own jit decorator that handles
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different versions of numba or does nothing if numba is not
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present. Note that functions that include unicode identifiers
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2016-12-15 16:15:01 +02:00
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must be decorated with #@ujit
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2016-12-04 22:27:03 +02:00
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'''
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2016-12-06 18:20:23 +02:00
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#def dummywrap(f):
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# return f
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def jit(f):
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if use_jit:
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return numba.jit(f)
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else:
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return f
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def ujit(f):
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if use_jit_utf8:
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return numba.jit(f)
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else:
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2016-12-04 22:27:03 +02:00
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return f
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2017-05-08 20:13:34 +03:00
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"""
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2016-03-27 12:56:54 +03:00
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# Coordinate transforms for arrays of "arbitrary" shape
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2016-12-15 16:15:01 +02:00
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#@ujit
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2016-03-27 12:56:54 +03:00
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def cart2sph(cart,axis=-1):
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if (cart.shape[axis] != 3):
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raise ValueError("The converted array has to have dimension 3"
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" along the given axis")
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[x, y, z] = np.split(cart,3,axis=axis)
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r = np.linalg.norm(cart,axis=axis,keepdims=True)
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r_zero = np.logical_not(r)
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θ = np.arccos(z/(r+r_zero))
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φ = np.arctan2(y,x) # arctan2 handles zeroes correctly itself
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return np.concatenate((r,θ,φ),axis=axis)
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2016-12-15 16:15:01 +02:00
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#@ujit
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2016-03-27 12:56:54 +03:00
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def sph2cart(sph, axis=-1):
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if (sph.shape[axis] != 3):
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raise ValueError("The converted array has to have dimension 3"
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" along the given axis")
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[r,θ,φ] = np.split(sph,3,axis=axis)
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sinθ = np.sin(θ)
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x = r * sinθ * np.cos(φ)
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y = r * sinθ * np.sin(φ)
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z = r * np.cos(θ)
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return np.concatenate((x,y,z),axis=axis)
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2016-12-15 16:15:01 +02:00
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#@ujit
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2016-03-27 12:56:54 +03:00
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def sph_loccart2cart(loccart, sph, axis=-1):
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"""
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Transformation of vector specified in local orthogonal coordinates
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(tangential to spherical coordinates – basis r̂,θ̂,φ̂) to global cartesian
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coordinates (basis x̂,ŷ,ẑ)
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SLOW FOR SMALL ARRAYS
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Parameters
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----------
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loccart: ... TODO
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the transformed vector in the local orthogonal coordinates
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sph: ... TODO
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the point (in spherical coordinates) at which the locally
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orthogonal basis is evaluated
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Returns
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-------
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output: ... TODO
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The coordinates of the vector in global cartesian coordinates
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"""
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if (loccart.shape[axis] != 3):
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raise ValueError("The converted array has to have dimension 3"
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" along the given axis")
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[r,θ,φ] = np.split(sph,3,axis=axis)
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sinθ = np.sin(θ)
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cosθ = np.cos(θ)
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sinφ = np.sin(φ)
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cosφ = np.cos(φ)
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#x = r * sinθ * cosφ
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#y = r * sinθ * sinφ
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#z = r * cosθ
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r̂x = sinθ * cosφ
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r̂y = sinθ * sinφ
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r̂z = cosθ
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θ̂x = cosθ * cosφ
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θ̂y = cosθ * sinφ
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θ̂z = -sinθ
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φ̂x = -sinφ
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φ̂y = cosφ
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φ̂z = np.zeros(φ̂y.shape)
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r̂ = np.concatenate((r̂x,r̂y,r̂z),axis=axis)
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θ̂ = np.concatenate((θ̂x,θ̂y,θ̂z),axis=axis)
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φ̂ = np.concatenate((φ̂x,φ̂y,φ̂z),axis=axis)
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[inr̂,inθ̂,inφ̂] = np.split(loccart,3,axis=axis)
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out=inr̂*r̂+inθ̂*θ̂+inφ̂*φ̂
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return out
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2016-12-15 16:15:01 +02:00
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#@ujit
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2016-03-27 12:56:54 +03:00
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def sph_loccart_basis(sph, sphaxis=-1, cartaxis=None):
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"""
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Returns the local cartesian basis in terms of global cartesian basis.
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sphaxis refers to the original dimensions
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TODO doc
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"""
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if(cartaxis is None):
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cartaxis = sph.ndim # default to last axis
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[r,θ,φ] = np.split(sph,3,axis=sphaxis)
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sinθ = np.sin(θ)
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cosθ = np.cos(θ)
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sinφ = np.sin(φ)
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cosφ = np.cos(φ)
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#x = r * sinθ * cosφ
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#y = r * sinθ * sinφ
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#z = r * cosθ
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r̂x = sinθ * cosφ
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r̂y = sinθ * sinφ
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r̂z = cosθ
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θ̂x = cosθ * cosφ
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θ̂y = cosθ * sinφ
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θ̂z = -sinθ
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φ̂x = -sinφ
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φ̂y = cosφ
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φ̂z = np.zeros(φ̂y.shape)
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#r̂ = np.concatenate((r̂x,r̂y,r̂z),axis=axis)
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#θ̂ = np.concatenate((θ̂x,θ̂y,θ̂z),axis=axis)
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#φ̂ = np.concatenate((φ̂x,φ̂y,φ̂z),axis=axis)
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x = np.expand_dims(np.concatenate((r̂x,θ̂x,φ̂x), axis=sphaxis),axis=cartaxis)
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y = np.expand_dims(np.concatenate((r̂y,θ̂y,φ̂y), axis=sphaxis),axis=cartaxis)
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z = np.expand_dims(np.concatenate((r̂z,θ̂z,φ̂z), axis=sphaxis),axis=cartaxis)
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out = np.concatenate((x,y,z),axis=cartaxis)
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return out
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2017-05-08 20:20:57 +03:00
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#@jit
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def nelem2lMax(nelem):
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"""
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Auxiliary inverse function to nelem(lMax) = (lMax + 2) * lMax. Returns 0 if
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it nelem does not come from positive integer lMax.
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"""
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lMax = round(math.sqrt(1+nelem) - 1)
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if ((lMax < 1) or ((lMax + 2) * lMax != nelem)):
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return 0
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else:
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return lMax
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2016-12-15 16:15:01 +02:00
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#@jit
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2016-03-27 12:56:54 +03:00
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def lpy(nmax, z):
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"""
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Associated legendre function and its derivatative at z in the 'y-indexing'.
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(Without Condon-Shortley phase AFAIK.)
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NOT THOROUGHLY TESTED
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Parameters
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----------
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nmax: int
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The maximum order to which the Legendre functions will be evaluated..
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z: float
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The point at which the Legendre functions are evaluated.
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output: (P_y, dP_y) TODO
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y-indexed legendre polynomials and their derivatives
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"""
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pmn_plus, dpmn_plus = lpmn(nmax, nmax, z)
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pmn_minus, dpmn_minus = lpmn(-nmax, nmax, z)
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nelem = nmax * nmax + 2*nmax
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P_y = np.empty((nelem), dtype=np.float_)
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dP_y = np.empty((nelem), dtype=np.float_)
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mn_p_y, mn_n_y = get_y_mn_unsigned(nmax)
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mn_plus_mask = (mn_p_y >= 0)
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mn_minus_mask = (mn_n_y >= 0)
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#print( mn_n_y[mn_minus_mask])
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P_y[mn_p_y[mn_plus_mask]] = pmn_plus[mn_plus_mask]
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P_y[mn_n_y[mn_minus_mask]] = pmn_minus[mn_minus_mask]
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dP_y[mn_p_y[mn_plus_mask]] = dpmn_plus[mn_plus_mask]
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dP_y[mn_n_y[mn_minus_mask]] = dpmn_minus[mn_minus_mask]
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return (P_y, dP_y)
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def vswf_yr(pos_sph,nmax,J=1):
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"""
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Normalized vector spherical wavefunctions $\widetilde{M}_{mn}^{j}$,
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$\widetilde{N}_{mn}^{j}$ as in [1, (2.40)].
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Parameters
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----------
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pos_sph : np.array(dtype=float, shape=(someshape,3))
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The positions where the spherical vector waves are to be
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evaluated. The last axis corresponds to the individual
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points (r,θ,φ). The radial coordinate r is dimensionless,
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assuming that it has already been multiplied by the
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wavenumber.
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nmax : int
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The maximum order to which the VSWFs are evaluated.
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Returns
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-------
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output : np.array(dtype=complex, shape=(someshape,nmax*nmax + 2*nmax,3))
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Spherical vector wave functions evaluated at pos_sph,
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in the local basis (r̂,θ̂,φ̂). The last indices correspond
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to m, n (in the ordering given by mnindex()), and basis
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vector index, respectively.
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[1] Jonathan M. Taylor. Optical Binding Phenomena: Observations and
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Mechanisms.
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"""
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#mi, ni = mnindex(nmax)
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#nelems = nmax*nmax + 2*nmax
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## TODO Remove these two lines in production:
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#if(len(mi) != nelems):
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# raise ValueError("This is very wrong.")
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## Pre-calculate the associated Legendre function
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#Prmn, dPrmn = lpmn(nmax,nmax,)
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## Normalized funs π̃, τ̃
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#π̃ =
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pass
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from scipy.special import sph_jn, sph_yn
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2016-12-15 16:15:01 +02:00
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#@jit
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2016-03-27 12:56:54 +03:00
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def _sph_zn_1(n,z):
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return sph_jn(n,z)
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2016-12-15 16:15:01 +02:00
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#@jit
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2016-03-27 12:56:54 +03:00
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def _sph_zn_2(n,z):
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return sph_yn(n,z)
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2016-12-15 16:15:01 +02:00
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#@jit
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2016-03-27 12:56:54 +03:00
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def _sph_zn_3(n,z):
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besj=sph_jn(n,z)
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besy=sph_yn(n,z)
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return (besj[0] + 1j*besy[0],besj[1] + 1j*besy[1])
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2016-12-15 16:15:01 +02:00
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#@jit
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2016-03-27 12:56:54 +03:00
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def _sph_zn_4(n,z):
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besj=sph_jn(n,z)
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besy=sph_yn(n,z)
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return (besj[0] - 1j*besy[0],besj[1] - 1j*besy[1])
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_sph_zn = [_sph_zn_1,_sph_zn_2,_sph_zn_3,_sph_zn_4]
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# computes bessel/hankel functions for orders from 0 up to n; drops
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# the derivatives which are also included in scipy.special.sph_jn/yn
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2016-12-15 16:15:01 +02:00
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#@jit
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2016-03-27 12:56:54 +03:00
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def zJn(n, z, J=1):
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return _sph_zn[J-1](n=n,z=z)
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# The following 4 funs have to be refactored, possibly merged
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2016-06-29 14:48:09 +03:00
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# FIXME: this can be expressed simply as:
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# $$ -\frac{1}{2}\sqrt{\frac{2n+1}{4\pi}n\left(n+1\right)}(\delta_{m,1}+\delta_{m,-1}) $$
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2016-12-15 16:15:01 +02:00
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#@ujit
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2016-03-27 12:56:54 +03:00
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def π̃_zerolim(nmax): # seems OK
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"""
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lim_{θ→ 0-} π̃(cos θ)
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"""
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my, ny = get_mn_y(nmax)
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nelems = len(my)
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π̃_y = np.zeros((nelems))
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plus1mmask = (my == 1)
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minus1mmask = (my == -1)
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pluslim = -ny*(1+ny)/2
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minuslim = 0.5
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π̃_y[plus1mmask] = pluslim[plus1mmask]
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π̃_y[minus1mmask] = - minuslim
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prenorm = np.sqrt((2*ny + 1)*factorial(ny-my)/(4*π*factorial(ny+my)))
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π̃_y = prenorm * π̃_y
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return π̃_y
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2016-12-15 16:15:01 +02:00
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#@ujit
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2016-03-27 12:56:54 +03:00
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def π̃_pilim(nmax): # Taky OK, jen to možná není kompatibilní se vzorečky z mathematiky
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"""
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lim_{θ→ π+} π̃(cos θ)
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"""
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my, ny = get_mn_y(nmax)
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nelems = len(my)
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π̃_y = np.zeros((nelems))
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plus1mmask = (my == 1)
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minus1mmask = (my == -1)
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pluslim = (-1)**ny*ny*(1+ny)/2
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minuslim = 0.5*(-1)**ny
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π̃_y[plus1mmask] = pluslim[plus1mmask]
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π̃_y[minus1mmask] = minuslim[minus1mmask]
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prenorm = np.sqrt((2*ny + 1)*factorial(ny-my)/(4*π*factorial(ny+my)))
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π̃_y = prenorm * π̃_y
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return π̃_y
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2016-06-29 14:48:09 +03:00
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# FIXME: this can be expressed simply as
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# $$ -\frac{1}{2}\sqrt{\frac{2n+1}{4\pi}n\left(n+1\right)}(\delta_{m,1}-\delta_{m,-1}) $$
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2016-12-15 16:15:01 +02:00
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#@ujit
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2016-03-27 12:56:54 +03:00
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def τ̃_zerolim(nmax):
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"""
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lim_{θ→ 0-} τ̃(cos θ)
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"""
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p0 = π̃_zerolim(nmax)
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my, ny = get_mn_y(nmax)
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minus1mmask = (my == -1)
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p0[minus1mmask] = -p0[minus1mmask]
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return p0
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2016-12-15 16:15:01 +02:00
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#@ujit
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2016-03-27 12:56:54 +03:00
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def τ̃_pilim(nmax):
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"""
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lim_{θ→ π+} τ̃(cos θ)
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"""
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t = π̃_pilim(nmax)
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my, ny = get_mn_y(nmax)
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plus1mmask = (my == 1)
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t[plus1mmask] = -t[plus1mmask]
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return t
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2016-12-15 16:15:01 +02:00
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#@ujit
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2016-03-27 12:56:54 +03:00
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def get_π̃τ̃_y1(θ,nmax):
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# TODO replace with the limit functions (below) when θ approaches
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# the extreme values at about 1e-6 distance
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"""
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(... TODO)
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"""
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if (abs(θ)<1e-6):
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return (π̃_zerolim(nmax),τ̃_zerolim(nmax))
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if (abs(θ-π)<1e-6):
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return (π̃_pilim(nmax),τ̃_pilim(nmax))
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my, ny = get_mn_y(nmax)
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nelems = len(my)
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Py, dPy = lpy(nmax, math.cos(θ))
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prenorm = np.sqrt((2*ny + 1)*factorial(ny-my)/(4*π*factorial(ny+my)))
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π̃_y = prenorm * my * Py / math.sin(θ) # bacha, možné dělení nulou
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τ̃_y = prenorm * dPy * (- math.sin(θ)) # TADY BACHA!!!!!!!!!! * (- math.sin(pos_sph[1])) ???
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return (π̃_y,τ̃_y)
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2016-12-15 16:15:01 +02:00
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#@ujit
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2016-03-27 12:56:54 +03:00
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def vswf_yr1(pos_sph,nmax,J=1):
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"""
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As vswf_yr, but evaluated only at single position (i.e. pos_sph has
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to have shape=(3))
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"""
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if (pos_sph[1].imag or pos_sph[2].imag):
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raise ValueError("The angles for the spherical wave functions can not be complex")
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kr = pos_sph[0] if pos_sph[0].imag else pos_sph[0].real # To supress the idiotic warning in scipy.special.sph_jn
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θ = pos_sph[1].real
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φ = pos_sph[2].real
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my, ny = get_mn_y(nmax)
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Py, dPy = lpy(nmax, math.cos(θ))
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nelems = nmax*nmax + 2*nmax
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# TODO Remove these two lines in production:
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if(len(Py) != nelems or len(my) != nelems):
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raise ValueError("This is very wrong.")
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prenorm = np.sqrt((2*ny + 1)*factorial(ny-my)/(4*π*factorial(ny+my)))
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if (abs(θ)<1e-6): # Ošetření limitního chování derivací Leg. fcí
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π̃_y=π̃_zerolim(nmax)
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τ̃_y=τ̃_zerolim(nmax)
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elif (abs(θ-π)<1e-6):
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π̃_y=π̃_pilim(nmax)
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τ̃_y=τ̃_pilim(nmax)
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else:
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π̃_y = prenorm * my * Py / math.sin(θ)
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τ̃_y = prenorm * dPy * (- math.sin(θ)) # TADY BACHA!!!!!!!!!! * (- math.sin(pos_sph[1])) ???
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z_n, dz_n = zJn(nmax, kr, J=J)
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z_y = z_n[ny]
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dz_y = dz_n[ny]
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eimf_y = np.exp(1j*my*φ) # zbytečné opakování my, lepší by bylo to spočítat jednou a vyindexovat
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M̃_y = np.zeros((nelems,3), dtype=np.complex_)
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M̃_y[:,1] = 1j * π̃_y * eimf_y * z_y
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M̃_y[:,2] = - τ̃_y * eimf_y * z_y
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Ñ_y = np.empty((nelems,3), dtype=np.complex_)
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Ñ_y[:,0] = (ny*(ny+1)/kr) * prenorm * Py * eimf_y * z_y
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Ñradial_fac_y = z_y / kr + dz_y
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Ñ_y[:,1] = τ̃_y * eimf_y * Ñradial_fac_y
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Ñ_y[:,2] = 1j*π̃_y * eimf_y * Ñradial_fac_y
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return(M̃_y, Ñ_y)
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#def plane_E_y(nmax):
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# """
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# The E_mn normalization factor as in [1, (3)] WITHOUT the E_0 factor,
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# y-indexed
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#
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# (... TODO)
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#
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# References
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# ----------
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# [1] Jonathan M. Taylor. Optical Binding Phenomena: Observations and
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# Mechanisms. FUCK, I MADE A MISTAKE: THIS IS FROM 7U
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# """
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# my, ny = get_mn_y(nmax)
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# return 1j**ny * np.sqrt((2*ny+1)*factorial(ny-my) /
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# (ny*(ny+1)*factorial(ny+my))
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# )
|
2016-12-15 16:15:01 +02:00
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#@ujit
|
2016-03-27 12:56:54 +03:00
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def zplane_pq_y(nmax, betap = 0):
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"""
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The z-propagating plane wave expansion coefficients as in [1, (1.12)]
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(... TODO)
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"""
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my, ny = get_mn_y(nmax)
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U_y = 4*π * 1j**ny / (ny * (ny+1))
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π̃_y = π̃_zerolim(nmax)
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τ̃_y = τ̃_zerolim(nmax)
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# fixme co je zač ten e_θ ve vzorečku? (zde neimplementováno)
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p_y = U_y*(τ̃_y*math.cos(betap) - 1j*math.sin(betap)*π̃_y)
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q_y = U_y*(π̃_y*math.cos(betap) - 1j*math.sin(betap)*τ̃_y)
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return (p_y, q_y)
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#import warnings
|
2016-12-15 16:15:01 +02:00
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#@ujit
|
2016-03-27 12:56:54 +03:00
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def plane_pq_y(nmax, kdir_cart, E_cart):
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"""
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The plane wave expansion coefficients for any direction kdir_cart
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and amplitude vector E_cart (which might be complex, depending on
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the phase and polarisation state). If E_cart and kdir_cart are
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not orthogonal, the result should correspond to the k-normal part
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of E_cart.
|
2016-07-26 00:42:16 +03:00
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The Taylor's convention on the expansion is used; therefore,
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the electric field is expressed as
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E(r) = E_cart * exp(1j * k ∙ r)
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= -1j * ∑_y ( p_y * Ñ_y(|k| * r) + q_y * M̃_y(|k| * r))
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(note the -1j factor).
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Parameters
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----------
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nmax: int
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The order of the expansion.
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kdir_cart: (3,)-shaped real array
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The wave vector (its magnitude does not play a role).
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E_cart: (3,)-shaped complex array
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Amplitude of the plane wave
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Returns
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-------
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p_y, q_y:
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The expansion coefficients for the electric (Ñ) and magnetic
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(M̃) waves, respectively.
|
2016-03-27 12:56:54 +03:00
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"""
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if np.iscomplexobj(kdir_cart):
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warnings.warn("The direction vector for the plane wave coefficients should be real. I am discarding the imaginary part now.")
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kdir_cart = kdir_cart.real
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k_sph = cart2sph(kdir_cart)
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π̃_y, τ̃_y = get_π̃τ̃_y1(k_sph[1], nmax)
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my, ny = get_mn_y(nmax)
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U_y = 4*π * 1j**ny / (ny * (ny+1))
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θ̂ = sph_loccart2cart(np.array([0,1,0]), k_sph, axis=-1)
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φ̂ = sph_loccart2cart(np.array([0,0,1]), k_sph, axis=-1)
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p_y = np.sum( U_y[:,ň]
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* np.conj(np.exp(1j*my[:,ň]*k_sph[2]) * (
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θ̂[ň,:]*τ̃_y[:,ň] + 1j*φ̂[ň,:]*π̃_y[:,ň]))
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* E_cart[ň,:],
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axis=-1)
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q_y = np.sum( U_y[:,ň]
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* np.conj(np.exp(1j*my[:,ň]*k_sph[2]) * (
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θ̂[ň,:]*π̃_y[:,ň] + 1j*φ̂[ň,:]*τ̃_y[:,ň]))
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* E_cart[ň,:],
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axis=-1)
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return (p_y, q_y)
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# Material parameters
|
2016-12-15 16:15:01 +02:00
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#@ujit
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2016-03-27 12:56:54 +03:00
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def ε_drude(ε_inf, ω_p, γ_p, ω): # RELATIVE permittivity, of course
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return ε_inf - ω_p*ω_p/(ω*(ω+1j*γ_p))
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# In[8]:
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# Mie scattering
|
2016-12-15 16:15:01 +02:00
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#@ujit
|
2016-03-27 12:56:54 +03:00
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def mie_coefficients(a, nmax, #ω, ε_i, ε_e=1, J_ext=1, J_scat=3
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k_i, k_e, μ_i=1, μ_e=1, J_ext=1, J_scat=3):
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"""
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|
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|
FIXME test the magnetic case
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|
TODO description
|
2016-06-29 21:47:20 +03:00
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RH concerns the N ("electric") part, RV the M ("magnetic") part
|
2016-03-27 12:56:54 +03:00
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#
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Parameters
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|
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|
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----------
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a : float
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Diameter of the sphere.
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nmax : int
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To which order (inc. nmax) to compute the coefficients.
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ω : float
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Frequency of the radiation
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ε_i, ε_e, μ_i, μ_e : complex
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Relative permittivities and permeabilities of the sphere (_i)
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and the environment (_e)
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|
MAGNETIC (μ_i, μ_e != 1) CASE UNTESTED AND PROBABLY BUGGY
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J_ext, J_scat : 1, 2, 3, or 4 (must be different)
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|
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Specifies the species of the Bessel/Hankel functions in which
|
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the external incoming (J_ext) and scattered (J_scat) fields
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|
are represented. 1,2,3,4 correspond to j,y,h(1),h(2), respectively.
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|
The returned coefficients are always with respect to the decomposition
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|
of the "external incoming" wave.
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Returns
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-------
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|
|
RV == a/p, RH == b/q, TV = d/p, TH = c/q
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|
TODO
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|
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|
|
what does it return on index 0???
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|
|
FIXME permeabilities
|
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|
"""
|
|
|
|
|
# permittivities are relative!
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|
|
|
# cf. worknotes
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|
|
#print("a, nmax, ε_m, ε_b, ω",a, nmax, ε_m, ε_b, ω)
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|
|
|
#k_i = cmath.sqrt(ε_i*μ_i) * ω / c
|
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|
|
x_i = k_i * a
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|
|
#k_e = cmath.sqrt(ε_e*μ_e) * ω / c
|
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|
|
x_e = k_e * a
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|
|
#print("Mie: phase at radius: x_i",x_i,"x_e",x_e)
|
|
|
|
|
m = k_i/k_e#cmath.sqrt(ε_i*μ_i/(ε_e*μ_e))
|
|
|
|
|
# We "need" the absolute permeabilities for the final formula
|
|
|
|
|
# This is not the absolute wave impedance, because only their ratio
|
|
|
|
|
# ηi/ηe is important for getting the Mie coefficients.
|
|
|
|
|
η_inv_i = k_i / μ_i
|
|
|
|
|
η_inv_e = k_e / μ_e
|
|
|
|
|
#print("k_m, x_m,k_b,x_b",k_m, x_m,k_b,x_b)
|
|
|
|
|
zi, ži = zJn(nmax, x_i, J=1)
|
|
|
|
|
#Pi = (zi * x_i)
|
|
|
|
|
#Di = (zi + x_i * ži) / Pi # Vzoreček Taylor (2.9)
|
|
|
|
|
#ži = zi + x_i * ži
|
|
|
|
|
ze, že = zJn(nmax, x_e, J=J_ext)
|
|
|
|
|
#Pe = (ze * x_e)
|
|
|
|
|
#De = (ze + x_e * že) / Pe # Vzoreček Taylor (2.9)
|
|
|
|
|
#že = ze + x_e * že
|
|
|
|
|
zs, žs = zJn(nmax, x_e, J=J_scat)
|
|
|
|
|
#Ps = (zs * x_e)
|
|
|
|
|
#Ds = (zs + x_e * žs) / Ps # Vzoreček Taylor (2.9)
|
|
|
|
|
#žs = zs + x_e * zs
|
|
|
|
|
#RH = (μ_i*zi*že - μ_e*ze*ži) / (μ_i*zi*žs - μ_e*zs*ži)
|
|
|
|
|
#RV = (μ_e*m*m*zi*že - μ_i*ze*ži) / (μ_e*m*m*zi*žs - μ_i*zs*ži)
|
|
|
|
|
#TH = (μ_i*ze*žs - μ_i*zs*že) / (μ_i*zi*žs - μ_e*zs*ži)
|
|
|
|
|
#TV = (μ_i*m*ze*žs - μ_i*m*zs*že) / (μ_e*m*m*zi*žs - μ_i*zs*ži)
|
|
|
|
|
ži = zi/x_i+ži
|
|
|
|
|
žs = zs/x_e+žs
|
|
|
|
|
že = ze/x_e+že
|
|
|
|
|
RV = -((-η_inv_i * že * zi + η_inv_e * ze * ži)/(-η_inv_e * ži * zs + η_inv_i * zi * žs))
|
|
|
|
|
RH = -((-η_inv_e * že * zi + η_inv_i * ze * ži)/(-η_inv_i * ži * zs + η_inv_e * zi * žs))
|
|
|
|
|
TV = -((-η_inv_e * že * zs + η_inv_e * ze * žs)/( η_inv_e * ži * zs - η_inv_i * zi * žs))
|
|
|
|
|
TH = -(( η_inv_e * že * zs - η_inv_e * ze * žs)/(-η_inv_i * ži * zs + η_inv_e * zi * žs))
|
|
|
|
|
return (RH, RV, TH, TV)
|
|
|
|
|
|
2016-12-15 16:15:01 +02:00
|
|
|
|
#@ujit
|
2016-03-27 12:56:54 +03:00
|
|
|
|
def G_Mie_scat_precalc_cart_new(source_cart, dest_cart, RH, RV, a, nmax, k_i, k_e, μ_i=1, μ_e=1, J_ext=1, J_scat=3):
|
|
|
|
|
"""
|
|
|
|
|
Implementation according to Kristensson, page 50
|
|
|
|
|
My (Taylor's) basis functions are normalized to n*(n+1), whereas Kristensson's to 1
|
|
|
|
|
TODO: check possible -1 factors (cf. Kristensson's dagger notation)
|
|
|
|
|
"""
|
|
|
|
|
my, ny = get_mn_y(nmax)
|
|
|
|
|
nelem = len(my)
|
|
|
|
|
#source to origin
|
|
|
|
|
source_sph = cart2sph(source_cart)
|
|
|
|
|
source_sph[0] = k_e * source_sph[0]
|
|
|
|
|
dest_sph = cart2sph(dest_cart)
|
|
|
|
|
dest_sph[0] = k_e * dest_sph[0]
|
|
|
|
|
if(dest_sph[0].real >= source_sph[0].real):
|
|
|
|
|
lo_sph = source_sph
|
|
|
|
|
hi_sph = dest_sph
|
|
|
|
|
else:
|
|
|
|
|
lo_sph = dest_sph
|
|
|
|
|
hi_sph = source_sph
|
|
|
|
|
lo_sph = source_sph
|
|
|
|
|
hi_sph = dest_sph
|
|
|
|
|
|
|
|
|
|
M̃lo_y, Ñlo_y = vswf_yr1(lo_sph,nmax,J=J_scat)
|
|
|
|
|
lo_loccart_basis = sph_loccart_basis(lo_sph, sphaxis=-1, cartaxis=None)
|
|
|
|
|
M̃lo_cart_y = np.sum(M̃lo_y[:,:,ň]*lo_loccart_basis[ň,:,:],axis=-2)
|
|
|
|
|
Ñlo_cart_y = np.sum(Ñlo_y[:,:,ň]*lo_loccart_basis[ň,:,:],axis=-2)
|
|
|
|
|
|
|
|
|
|
M̃hi_y, Ñhi_y = vswf_yr1(hi_sph,nmax,J=J_scat)#J_scat
|
|
|
|
|
hi_loccart_basis = sph_loccart_basis(hi_sph, sphaxis=-1, cartaxis=None)
|
|
|
|
|
M̃hi_cart_y = np.sum(M̃hi_y[:,:,ň]*hi_loccart_basis[ň,:,:],axis=-2)
|
|
|
|
|
Ñhi_cart_y = np.sum(Ñhi_y[:,:,ň]*hi_loccart_basis[ň,:,:],axis=-2)
|
|
|
|
|
|
|
|
|
|
G_y = (RH[ny][:,ň,ň] * M̃lo_cart_y[:,:,ň].conj() * M̃hi_cart_y[:,ň,:] +
|
|
|
|
|
RV[ny][:,ň,ň] * Ñlo_cart_y[:,:,ň].conj() * Ñhi_cart_y[:,ň,:]) / (ny * (ny+1))[:,ň,ň]
|
|
|
|
|
return 1j* k_e*np.sum(G_y,axis=0)
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
# From PRL 112, 253601 (1)
|
2016-12-15 16:15:01 +02:00
|
|
|
|
#@ujit
|
2016-03-27 12:56:54 +03:00
|
|
|
|
def Grr_Delga(nmax, a, r, k, ε_m, ε_b):
|
|
|
|
|
om = k * c
|
|
|
|
|
z = (r-a)/a
|
|
|
|
|
g0 = om*cmath.sqrt(ε_b)/(6*c*π)
|
|
|
|
|
n = np.arange(1,nmax+1)
|
|
|
|
|
s = np.sum( (n+1)**2 * (ε_m-ε_b) / ((1+z)**(2*n+4) * (ε_m + ((n+1)/n)*ε_b)))
|
|
|
|
|
return (g0 + s * c**2/(4*π*om**2*ε_b*a**3))
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
# TODOs
|
|
|
|
|
# ====
|
|
|
|
|
#
|
|
|
|
|
# Rewrite the functions zJn, lpy in (at least simulated) universal manner.
|
|
|
|
|
# Then universalise the rest
|
|
|
|
|
#
|
|
|
|
|
# Implement the actual multiple scattering
|
|
|
|
|
#
|
|
|
|
|
# Test if the decomposition of plane wave works also for absorbing environment (complex k).
|
|
|
|
|
|
|
|
|
|
# From PRL 112, 253601 (1)
|
2016-12-15 16:15:01 +02:00
|
|
|
|
#@ujit
|
2016-03-27 12:56:54 +03:00
|
|
|
|
def Grr_Delga(nmax, a, r, k, ε_m, ε_b):
|
|
|
|
|
om = k * c
|
|
|
|
|
z = (r-a)/a
|
|
|
|
|
g0 = om*cmath.sqrt(ε_b)/(6*c*π)
|
|
|
|
|
n = np.arange(1,nmax+1)
|
|
|
|
|
s = np.sum( (n+1)**2 * (ε_m-ε_b) / ((1+z)**(2*n+4) * (ε_m + ((n+1)/n)*ε_b)))
|
|
|
|
|
return (g0 + s * c**2/(4*π*om**2*ε_b*a**3))
|
|
|
|
|
|
2016-12-15 16:15:01 +02:00
|
|
|
|
#@ujit
|
2016-03-27 12:56:54 +03:00
|
|
|
|
def G0_dip_1(r_cart,k):
|
|
|
|
|
"""
|
|
|
|
|
Free-space dyadic Green's function in terms of the spherical vector waves.
|
|
|
|
|
FIXME
|
|
|
|
|
"""
|
|
|
|
|
sph = cart2sph(r_cart*k)
|
|
|
|
|
pfz = 0.32573500793527994772 # 1./math.sqrt(3.*π)
|
|
|
|
|
pf = 0.23032943298089031951 # 1./math.sqrt(6.*π)
|
|
|
|
|
M1_y, N1_y = vswf_yr1(sph,nmax = 1,J=3)
|
|
|
|
|
loccart_basis = sph_loccart_basis(sph, sphaxis=-1, cartaxis=None)
|
|
|
|
|
N1_cart = np.sum(N1_y[:,:,ň]*loccart_basis[ň,:,:],axis=-2)
|
|
|
|
|
coeffs_cart = np.array([[pf,-1j*pf,0.],[0.,0.,pfz],[-pf,-1j*pf,0.]]).conj()
|
|
|
|
|
return 1j*k*np.sum(coeffs_cart[:,:,ň]*N1_cart[:,ň,:],axis=0)/2.
|
|
|
|
|
|
|
|
|
|
# Free-space dyadic Green's functions from RMP 70, 2, 447 =: [1]
|
|
|
|
|
# (The numerical value is correct only at the regular part, i.e. r != 0)
|
2016-12-15 16:15:01 +02:00
|
|
|
|
#@ujit
|
2016-03-27 12:56:54 +03:00
|
|
|
|
def _P(z):
|
|
|
|
|
return (1-1/z+1/(z*z))
|
2016-12-15 16:15:01 +02:00
|
|
|
|
#@ujit
|
2016-03-27 12:56:54 +03:00
|
|
|
|
def _Q(z):
|
|
|
|
|
return (-1+3/z-3/(z*z))
|
|
|
|
|
|
|
|
|
|
# [1, (9)] FIXME The sign here is most likely wrong!!!
|
2016-12-15 16:15:01 +02:00
|
|
|
|
#@ujit
|
2016-03-27 12:56:54 +03:00
|
|
|
|
def G0_analytical(r #cartesian!
|
|
|
|
|
, k):
|
|
|
|
|
I=np.identity(3)
|
|
|
|
|
rn = sph_loccart2cart(np.array([1.,0.,0.]), cart2sph(r), axis=-1)
|
|
|
|
|
rnxrn = rn[...,:,ň] * rn[...,ň,:]
|
|
|
|
|
r = np.linalg.norm(r, axis=-1)
|
|
|
|
|
#print(_P(1j*k*r).shape,_Q(1j*k*r).shape, rnxrn.shape, I.shape)
|
|
|
|
|
return ((-np.exp(1j*k*r)/(4*π*r))[...,ň,ň] *
|
|
|
|
|
(_P(1j*k*r)[...,ň,ň]*I
|
|
|
|
|
+_Q(1j*k*r)[...,ň,ň]*rnxrn
|
|
|
|
|
))
|
|
|
|
|
|
|
|
|
|
# [1, (11)]
|
2016-12-15 16:15:01 +02:00
|
|
|
|
#@ujit
|
2016-03-27 12:56:54 +03:00
|
|
|
|
def G0L_analytical(r, k):
|
|
|
|
|
I=np.identity(3)
|
|
|
|
|
rn = sph_loccart2cart(np.array([1.,0.,0.]), cart2sph(r), axis=-1)
|
|
|
|
|
rnxrn = rn[...,:,ň] * rn[...,ň,:]
|
|
|
|
|
r = np.linalg.norm(r, axis=-1)
|
|
|
|
|
return (I-3*rnxrn)/(4*π*k*k*r**3)[...,ň,ň]
|
|
|
|
|
|
|
|
|
|
# [1,(10)]
|
2016-12-15 16:15:01 +02:00
|
|
|
|
#@jit
|
2016-03-27 12:56:54 +03:00
|
|
|
|
def G0T_analytical(r, k):
|
|
|
|
|
return G0_analytical(r,k) - G0L_analytical(r,k)
|
|
|
|
|
|
2016-12-15 16:15:01 +02:00
|
|
|
|
#@ujit
|
2016-03-27 12:56:54 +03:00
|
|
|
|
def G0_sum_1_slow(source_cart, dest_cart, k, nmax):
|
|
|
|
|
my, ny = get_mn_y(nmax)
|
|
|
|
|
nelem = len(my)
|
|
|
|
|
RH = np.full((nelem),1)
|
|
|
|
|
RV = RH
|
|
|
|
|
return G_Mie_scat_precalc_cart(source_cart, dest_cart, RH, RV, a=0.001, nmax=nmax, k_i=1, k_e=k, μ_i=1, μ_e=1, J_ext=1, J_scat=3)
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
2016-07-12 03:20:53 +03:00
|
|
|
|
# Transformations of spherical bases
|
2016-12-15 16:15:01 +02:00
|
|
|
|
#@jit
|
2016-07-12 03:20:53 +03:00
|
|
|
|
def WignerD_mm(l, quat):
|
|
|
|
|
"""
|
|
|
|
|
Calculates Wigner D matrix (as an numpy (2*l+1,2*l+1)-shaped array)
|
|
|
|
|
for order l, and a rotation given by quaternion quat.
|
|
|
|
|
|
|
|
|
|
This represents the rotation of spherical vector basis
|
|
|
|
|
TODO doc
|
|
|
|
|
"""
|
|
|
|
|
|
|
|
|
|
indices = np.array([ [l,i,j] for i in range(-l,l+1) for j in range(-l,l+1)])
|
|
|
|
|
Delems = sf.Wigner_D_element(quat, indices).reshape(2*l+1,2*l+1)
|
|
|
|
|
return Delems
|
|
|
|
|
|
2016-12-15 16:15:01 +02:00
|
|
|
|
#@jit
|
2016-07-12 03:20:53 +03:00
|
|
|
|
def WignerD_mm_fromvector(l, vect):
|
|
|
|
|
"""
|
|
|
|
|
TODO doc
|
|
|
|
|
"""
|
|
|
|
|
return WignerD_mm(l, quaternion.from_rotation_vector(vect))
|
|
|
|
|
|
|
|
|
|
|
2016-12-15 16:15:01 +02:00
|
|
|
|
#@jit
|
2016-07-12 03:20:53 +03:00
|
|
|
|
def WignerD_yy(lmax, quat):
|
|
|
|
|
"""
|
|
|
|
|
TODO doc
|
|
|
|
|
"""
|
|
|
|
|
my, ny = get_mn_y(lmax)
|
|
|
|
|
Delems = np.zeros((len(my),len(my)),dtype=complex)
|
|
|
|
|
b_in = 0
|
|
|
|
|
e_in = None
|
|
|
|
|
for l in range(1,lmax+1):
|
|
|
|
|
e_in = b_in + 2*l+1
|
|
|
|
|
Delems[b_in:e_in,b_in:e_in] = WignerD_mm(l, quat)
|
|
|
|
|
b_in = e_in
|
|
|
|
|
return Delems
|
|
|
|
|
|
2016-12-15 16:15:01 +02:00
|
|
|
|
#@jit
|
2016-07-12 03:20:53 +03:00
|
|
|
|
def WignerD_yy_fromvector(lmax, vect):
|
|
|
|
|
"""
|
|
|
|
|
TODO doc
|
|
|
|
|
"""
|
|
|
|
|
return WignerD_yy(lmax, quaternion.from_rotation_vector(vect))
|
|
|
|
|
|
2016-07-19 16:24:02 +03:00
|
|
|
|
|
2016-12-15 16:15:01 +02:00
|
|
|
|
#@jit
|
2016-07-12 03:20:53 +03:00
|
|
|
|
def xflip_yy(lmax):
|
|
|
|
|
"""
|
|
|
|
|
TODO doc
|
2016-07-19 16:24:02 +03:00
|
|
|
|
xflip = δ(m + m') δ(l - l')
|
|
|
|
|
(i.e. ones on the (m' m) antidiagonal
|
2016-07-12 03:20:53 +03:00
|
|
|
|
"""
|
|
|
|
|
my, ny = get_mn_y(lmax)
|
|
|
|
|
elems = np.zeros((len(my),len(my)),dtype=int)
|
|
|
|
|
b_in = 0
|
|
|
|
|
e_in = None
|
|
|
|
|
for l in range(1,lmax+1):
|
|
|
|
|
e_in = b_in + 2*l+1
|
|
|
|
|
elems[b_in:e_in,b_in:e_in] = np.eye(2*l+1)[::-1,:]
|
|
|
|
|
b_in = e_in
|
|
|
|
|
return elems
|
2016-08-09 14:39:45 +03:00
|
|
|
|
|
2016-12-15 16:15:01 +02:00
|
|
|
|
#@jit
|
2016-08-09 14:39:45 +03:00
|
|
|
|
def xflip_tyy(lmax):
|
|
|
|
|
fl_yy = xflip_yy(lmax)
|
|
|
|
|
return np.array([fl_yy,-fl_yy])
|
|
|
|
|
|
2016-12-15 16:15:01 +02:00
|
|
|
|
#@jit
|
2016-08-09 14:39:45 +03:00
|
|
|
|
def xflip_tyty(lmax):
|
|
|
|
|
fl_yy = xflip_yy(lmax)
|
|
|
|
|
nelem = fl_yy.shape[0]
|
|
|
|
|
fl_tyty = np.zeros((2,nelem,2,nelem),dtype=int)
|
|
|
|
|
fl_tyty[0,:,0,:] = fl_yy
|
|
|
|
|
fl_tyty[1,:,1,:] = -fl_yy
|
|
|
|
|
return fl_tyty
|
|
|
|
|
|
2016-12-15 16:15:01 +02:00
|
|
|
|
#@jit
|
2016-07-12 03:20:53 +03:00
|
|
|
|
def yflip_yy(lmax):
|
|
|
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|
"""
|
|
|
|
|
TODO doc
|
2016-07-19 16:24:02 +03:00
|
|
|
|
yflip = rot(z,pi/2) * xflip * rot(z,-pi/2)
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|
= δ(m + m') δ(l - l') * (-1)**m
|
2016-07-12 03:20:53 +03:00
|
|
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|
"""
|
|
|
|
|
my, ny = get_mn_y(lmax)
|
|
|
|
|
elems = xflip_yy(lmax)
|
|
|
|
|
elems[(my % 2)==1] = elems[(my % 2)==1] * -1 # Obvious sign of tiredness (this is correct but ugly; FIXME)
|
|
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|
return elems
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|
2016-12-15 16:15:01 +02:00
|
|
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|
#@jit
|
2016-08-09 14:39:45 +03:00
|
|
|
|
def yflip_tyy(lmax):
|
|
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|
fl_yy = yflip_yy(lmax)
|
|
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|
return np.array([fl_yy,-fl_yy])
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|
2016-12-15 16:15:01 +02:00
|
|
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|
#@jit
|
2016-08-09 14:39:45 +03:00
|
|
|
|
def yflip_tyty(lmax):
|
|
|
|
|
fl_yy = yflip_yy(lmax)
|
|
|
|
|
nelem = fl_yy.shape[0]
|
|
|
|
|
fl_tyty = np.zeros((2,nelem,2,nelem),dtype=int)
|
|
|
|
|
fl_tyty[0,:,0,:] = fl_yy
|
|
|
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|
fl_tyty[1,:,1,:] = -fl_yy
|
|
|
|
|
return fl_tyty
|
|
|
|
|
|
2016-12-15 16:15:01 +02:00
|
|
|
|
#@jit
|
2016-07-19 16:24:02 +03:00
|
|
|
|
def zflip_yy(lmax):
|
|
|
|
|
"""
|
|
|
|
|
TODO doc
|
|
|
|
|
zflip = (-1)^(l+m)
|
|
|
|
|
"""
|
|
|
|
|
my, ny = get_mn_y(lmax)
|
|
|
|
|
elems = np.zeros((len(my), len(my)), dtype=int)
|
|
|
|
|
b_in = 0
|
|
|
|
|
e_in = None
|
|
|
|
|
for l in range(1,lmax+1):
|
|
|
|
|
e_in = b_in + 2*l+1
|
|
|
|
|
elems[b_in:e_in,b_in:e_in] = np.diag([(-1)**i for i in range(e_in-b_in)])
|
|
|
|
|
b_in = e_in
|
|
|
|
|
return elems
|
|
|
|
|
|
2016-12-15 16:15:01 +02:00
|
|
|
|
#@jit
|
2016-08-09 14:39:45 +03:00
|
|
|
|
def zflip_tyy(lmax):
|
|
|
|
|
fl_yy = zflip_yy(lmax)
|
|
|
|
|
return np.array([fl_yy,-fl_yy])
|
|
|
|
|
|
2016-12-15 16:15:01 +02:00
|
|
|
|
#@jit
|
2016-08-09 14:39:45 +03:00
|
|
|
|
def zflip_tyty(lmax):
|
|
|
|
|
fl_yy = zflip_yy(lmax)
|
|
|
|
|
nelem = fl_yy.shape[0]
|
|
|
|
|
fl_tyty = np.zeros((2,nelem,2,nelem),dtype=int)
|
|
|
|
|
fl_tyty[0,:,0,:] = fl_yy
|
|
|
|
|
fl_tyty[1,:,1,:] = -fl_yy
|
|
|
|
|
return fl_tyty
|
|
|
|
|
|
2016-12-15 16:15:01 +02:00
|
|
|
|
#@jit
|
2016-07-19 16:24:02 +03:00
|
|
|
|
def parity_yy(lmax):
|
|
|
|
|
"""
|
|
|
|
|
Parity operator (flip in x,y,z)
|
|
|
|
|
parity = (-1)**l
|
|
|
|
|
"""
|
|
|
|
|
my, ny = get_mn_y(lmax)
|
|
|
|
|
return np.diag((-1)**ny)
|
|
|
|
|
|
2016-07-12 03:20:53 +03:00
|
|
|
|
# BTW parity (xyz-flip) is simply (-1)**ny
|
2016-07-12 03:40:57 +03:00
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
#----------------------------------------------------#
|
|
|
|
|
# Loading T-matrices from scuff-tmatrix output files #
|
|
|
|
|
#----------------------------------------------------#
|
|
|
|
|
|
|
|
|
|
# We don't really need this particular function anymore, but...
|
2016-12-15 16:15:01 +02:00
|
|
|
|
#@jit
|
2016-07-12 03:40:57 +03:00
|
|
|
|
def _scuffTMatrixConvert_EM_01(EM):
|
|
|
|
|
#print(EM)
|
|
|
|
|
if (EM == b'E'):
|
|
|
|
|
return 0
|
|
|
|
|
elif (EM == b'M'):
|
|
|
|
|
return 1
|
|
|
|
|
else:
|
|
|
|
|
return None
|
|
|
|
|
|
2016-12-15 16:15:01 +02:00
|
|
|
|
#@ujit
|
2016-07-12 03:40:57 +03:00
|
|
|
|
def loadScuffTMatrices(fileName):
|
|
|
|
|
"""
|
|
|
|
|
TODO doc
|
|
|
|
|
"""
|
|
|
|
|
μm = 1e-6
|
|
|
|
|
table = np.genfromtxt(fileName,
|
|
|
|
|
converters={1: _scuffTMatrixConvert_EM_01, 4: _scuffTMatrixConvert_EM_01},
|
|
|
|
|
dtype=[('freq', '<f8'), ('outc_type', '<i8'), ('outc_l', '<i8'), ('outc_m', '<i8'),
|
|
|
|
|
('inc_type', '<i8'), ('inc_l', '<i8'), ('inc_m', '<i8'), ('Treal', '<f8'), ('Timag', '<f8')]
|
|
|
|
|
)
|
|
|
|
|
lMax=np.max(table['outc_l'])
|
|
|
|
|
my,ny = get_mn_y(lMax)
|
|
|
|
|
nelem = len(ny)
|
|
|
|
|
TMatrix_sz = nelem**2 * 4 # number of rows for each frequency: nelem * nelem spherical incides, 2 * 2 E/M types
|
|
|
|
|
freqs_weirdunits = table['freq'][::TMatrix_sz].copy()
|
|
|
|
|
freqs = freqs_weirdunits * c / μm
|
|
|
|
|
# The iteration in the TMatrix file goes in this order (the last one iterates fastest, i.e. in the innermost loop):
|
|
|
|
|
# freq outc_l outc_m outc_type inc_l inc_m inc_type
|
|
|
|
|
# The l,m mapping is the same as is given by my get_mn_y function, so no need to touch that
|
|
|
|
|
TMatrices_tmp_real = table['Treal'].reshape(len(freqs), nelem, 2, nelem, 2)
|
|
|
|
|
TMatrices_tmp_imag = table['Timag'].reshape(len(freqs), nelem, 2, nelem, 2)
|
|
|
|
|
# There are two přoblems with the previous matrices. First, we want to have the
|
|
|
|
|
# type indices first, so we want a shape (len(freqs), 2, nelem, 2, nelem) as in the older code.
|
|
|
|
|
# Second, M-waves come first, so they have now 0-valued index, and E-waves have 1-valued index,
|
|
|
|
|
# which we want to be inverted.
|
2017-02-26 04:50:15 +02:00
|
|
|
|
TMatrices = np.zeros((len(freqs),2,nelem,2,nelem),dtype=complex)
|
2016-07-12 03:40:57 +03:00
|
|
|
|
for inc_type in [0,1]:
|
|
|
|
|
for outc_type in [0,1]:
|
|
|
|
|
TMatrices[:,1-outc_type,:,1-inc_type,:] = TMatrices_tmp_real[:,:,outc_type,:,inc_type]+1j*TMatrices_tmp_imag[:,:,outc_type,:,inc_type]
|
|
|
|
|
# IMPORTANT: now we are going from Reid's/Kristensson's/Jackson's/whoseever convention to Taylor's convention
|
|
|
|
|
TMatrices[:,:,:,:,:] = TMatrices[:,:,:,:,:] * np.sqrt(ny*(ny+1))[ň,ň,ň,ň,:] / np.sqrt(ny*(ny+1))[ň,ň,:,ň,ň]
|
|
|
|
|
return (TMatrices, freqs, freqs_weirdunits, lMax)
|
2016-07-14 21:13:58 +03:00
|
|
|
|
|
|
|
|
|
|
|
|
|
|
# misc tensor maniputalion
|
2016-12-15 16:15:01 +02:00
|
|
|
|
#@jit
|
2016-07-14 21:13:58 +03:00
|
|
|
|
def apply_matrix_left(matrix, tensor, axis):
|
|
|
|
|
"""
|
|
|
|
|
TODO doc
|
|
|
|
|
Apply square matrix to a given axis of a tensor, so that the result retains the shape
|
|
|
|
|
of the original tensor. The summation goes over the second index of the matrix and the
|
|
|
|
|
given tensor axis.
|
|
|
|
|
"""
|
|
|
|
|
tmp = np.tensordot(matrix, tensor, axes=(-1,axis))
|
|
|
|
|
return np.moveaxis(tmp, 0, axis)
|
|
|
|
|
|
2016-12-15 16:15:01 +02:00
|
|
|
|
#@jit
|
2016-08-09 15:40:36 +03:00
|
|
|
|
def apply_ndmatrix_left(matrix,tensor,axes):
|
|
|
|
|
"""
|
|
|
|
|
Generalized apply_matrix_left, the matrix can have more (2N) abstract dimensions,
|
|
|
|
|
like M[i,j,k,...z,i,j,k,...,z]. N axes have to be specified in a tuple, corresponding
|
|
|
|
|
to the axes 0,1,...N-1 of the matrix
|
|
|
|
|
"""
|
|
|
|
|
N = len(axes)
|
|
|
|
|
matrix = np.tensordot(matrix, tensor, axes=([-N+axn for axn in range(N)],axes))
|
|
|
|
|
matrix = np.moveaxis(matrix, range(N), axes)
|
|
|
|
|
return matrix
|
2017-05-10 11:44:04 +03:00
|
|
|
|
|
|
|
|
|
|
|
|
|
|
def symz_indexarrays(lMax, npart = 1):
|
|
|
|
|
"""
|
|
|
|
|
Returns indices that are used for separating the in-plane E ('TE' in the photonic crystal
|
|
|
|
|
jargon) and perpendicular E ('TM' in the photonic crystal jargon) modes
|
|
|
|
|
in the z-mirror symmetric systems.
|
|
|
|
|
|
|
|
|
|
Parameters
|
|
|
|
|
----------
|
|
|
|
|
lMax : int
|
|
|
|
|
The maximum degree cutoff for the T-matrix to which these indices will be applied.
|
|
|
|
|
|
|
|
|
|
npart : int
|
|
|
|
|
Number of particles (TODO better description)
|
|
|
|
|
|
|
|
|
|
Returns
|
|
|
|
|
-------
|
|
|
|
|
TEč, TMč : (npart * 2 * nelem)-shaped bool ndarray
|
|
|
|
|
Mask arrays corresponding to the 'TE' and 'TM' modes, respectively.
|
|
|
|
|
"""
|
2017-05-10 13:44:36 +03:00
|
|
|
|
my, ny = get_mn_y(lMax)
|
|
|
|
|
nelem = len(my)
|
2017-05-10 11:44:04 +03:00
|
|
|
|
ž = np.arange(2*nelem) # single particle spherical wave indices
|
|
|
|
|
tž = ž // nelem # tž == 0: electric waves, tž == 1: magnetic waves
|
|
|
|
|
mž = my[ž%nelem]
|
|
|
|
|
nž = ny[ž%nelem]
|
|
|
|
|
TEž = ž[(mž+nž+tž) % 2 == 0]
|
|
|
|
|
TMž = ž[(mž+nž+tž) % 2 == 1]
|
|
|
|
|
|
|
|
|
|
č = np.arange(npart*2*nelem) # spherical wave indices for multiple particles (e.g. in a unit cell)
|
|
|
|
|
žč = č % (2* nelem)
|
|
|
|
|
tč = tž[žč]
|
|
|
|
|
mč = mž[žč]
|
|
|
|
|
nč = nž[žč]
|
|
|
|
|
TEč = č[(mč+nč+tč) % 2 == 0]
|
|
|
|
|
TMč = č[(mč+nč+tč) % 2 == 1]
|
|
|
|
|
return (TEč, TMč)
|
|
|
|
|
|