propagation#
- optika.materials.matrices.propagation(wavelength, direction, thickness, n)[source]#
Compute the propagation matrix, which propagates the electric field through a homogenous slab.
- Parameters:
wavelength (Quantity | AbstractScalar) – The wavelength of the incident light in vacuum.
direction (float | AbstractScalar) – The component of the incident light’s propagation direction antiparallel to the surface normal.
thickness (Quantity | AbstractScalar) – The thickness of the material.
n (Quantity | AbstractScalar) – The complex index of refraction of the material
- Return type:
Examples
Compute the propagation matrix for \(s\)-polarized light normally incident on a layer of silicon dioxide
import astropy.units as u import named_arrays as na import optika # Define the wavelength of the incident light wavelength = 100 * u.AA # Initialize a representation of silicon dioxide sio2 = optika.chemicals.Chemical("SiO2") # Compute the propagation matrix optika.materials.matrices.propagation( wavelength=wavelength, direction=1, thickness=10 * u.nm, n=sio2.n(wavelength), )
Cartesian2dMatrixArray( x=Cartesian2dVectorArray( x=ScalarArray( ndarray=1.09465461+0.10596849j , axes=(), ), y=0, ), y=Cartesian2dVectorArray( x=0, y=ScalarArray( ndarray=0.90504869-0.08761361j , axes=(), ), ), )Notes
The propagation matrix for a homogenous slab is given by Yeh [1988] Equation 5.1-24,
(1)#\[\begin{split}U = \begin{pmatrix} e^{-i \beta} & 0 \\ 0 & e^{i \beta} \\ \end{pmatrix},\end{split}\]where
(2)#\[\beta = \frac{2 \pi}{\lambda} n h \cos \theta\]is the phase change from propagating through the material, \(n\) is the index of refraction inside the material, \(\lambda\) is the wavelength of the incident light in vacuum, \(h\) is the thickness of the material, and \(\theta\) is the angle between the surface normal and the propagation direction of the incident light.
References to
optika.materials.matrices.propagation