Complex amplitude reflectance of a spherical mirror

In summary, the complex amplitude reflectance of a spherical mirror is given as ##exp[-jk(x^2+y^2)/R]##, where ##x## and ##y## are the coordinates in the plane of the mirror, and ##R## is the radius of the mirror. This is equivalent to the transmittance of a spherical mirror, ##exp[jk(x^2+y^2)/2f]##, but with a change in direction of propagation. The phase gained depends on the distance traveled from the optical axis, which can be approximated as ##\frac {\rho^2} {2R}## for small values of ##\rho## compared to ##R##.
  • #1
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Homework Statement


Prove the complex amplitude reflectance of a spherical mirror is given as exp[-jk(x2+y2)/R]


Homework Equations


Transmittance of a spherical mirror is also exp[jk(x2+y2)/2f]


The Attempt at a Solution


I have totally no idea how to go about doing this. Can I just say that the reflectance is the same as the transmittance just that the wave changes the direction of propagation?
 
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  • #2
I realize this is late but here it goes:

See how much phase you accumulate, relative to the plane wave that travels along the optical axis and bounces off a planar mirror.

If you are looking at the plane wave ##\rho = \sqrt{x^2+y^2}## away from the axis in the plane ##z=0## (mirror centre is at ##z=R## ), then to get to the mirror you need to travel additional distance ##d##. Denote ##z_0## the z at which the ray intersects with the mirror at a given ##\rho##.

$$d = z_0 = R - \sqrt{R^2 - \rho^2} = R - R\sqrt{1-(\frac \rho R)^2}$$

Assuming ##\rho## is small (we are close to the axis) compared to R, we can write
$$\sqrt{1-(\frac \rho R)^2} = 1-\frac {\rho^2} {2R^2}$$
and so
$$d = \frac {\rho^2} {2R}$$

Because we traverse that distance twice, the phase gained is ##k*2d = k \frac {\rho^2} {R}## and your complex reflectance is ##e^{ik \frac {\rho^2} {R}}##
 

Related to Complex amplitude reflectance of a spherical mirror

What is the complex amplitude reflectance of a spherical mirror?

The complex amplitude reflectance of a spherical mirror is a measure of the amount of light that is reflected off the surface of the mirror. It takes into account both the amplitude (strength) and phase (timing) of the reflected light.

How is the complex amplitude reflectance of a spherical mirror calculated?

The complex amplitude reflectance of a spherical mirror can be calculated using the Fresnel equations, which take into account the angle of incidence, the refractive index of the mirror material, and the polarization of the incident light.

What factors can affect the complex amplitude reflectance of a spherical mirror?

The complex amplitude reflectance of a spherical mirror can be affected by several factors, including the angle of incidence, the refractive index of the mirror material, and the wavelength of the incident light. The surface roughness and imperfections of the mirror can also impact the reflectance.

Why is the complex amplitude reflectance of a spherical mirror important in optical sciences?

The complex amplitude reflectance of a spherical mirror is an important parameter in optical sciences because it can help determine the performance and efficiency of optical systems. It is also used in the design and optimization of optical devices, such as telescopes and lasers.

How can the complex amplitude reflectance of a spherical mirror be measured?

The complex amplitude reflectance of a spherical mirror can be measured using various techniques such as spectrophotometry, ellipsometry, and interferometry. These methods involve measuring the intensity and polarization of the reflected light and using mathematical models to calculate the reflectance.

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