# Linear canonical transformation

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In Hamiltonian mechanics, the linear canonical transformation (LCT) is a family of integral transforms that generalizes many classical transforms. It has 4 parameters and 1 constraint, so it is a 3-dimensional family, and can be visualized as the action of the special linear group SL2(R) on the time–frequency plane (domain).

The LCT generalizes the Fourier, fractional Fourier, Laplace, Gauss–Weierstrass, Bargmann and the Fresnel transforms as particular cases. The name "linear canonical transformation" is from canonical transformation, a map that preserves the symplectic structure, as SL2(R) can also be interpreted as the symplectic group Sp2, and thus LCTs are the linear maps of the time–frequency domain which preserve the symplectic form.

## Definition

The LCT can be represented in several ways; most easily,[1] it can be parameterized by a 2×2 matrix with determinant 1, i.e., an element of the special linear group SL2(R). Then for any such matrix $\left(\begin{smallmatrix}a & b\\c & d\end{smallmatrix}\right),$ with ad − bc = 1, the corresponding integral transform from a function $x(t)$ to $X(u)$ is defined as

 $X_{(a,b,c,d)}(u) = \sqrt{-i} \cdot e^{i \pi \frac{d}{b} u^{2}} \int_{-\infty}^\infty e^{-i 2 \pi \frac{1}{b} ut}e^{i \pi \frac{a}{b} t^2} x(t) \; dt \, ,$ when b ≠ 0, $X_{(a,0,c,d)}(u) = \sqrt{d} \cdot e^{i \pi cdu^{2}} x(du) \, ,$ when b = 0.

## Special cases

Many classical transforms are special cases of the linear canonical transform:

$\begin{bmatrix} a & b \\ c & d \end{bmatrix} = \begin{bmatrix} 0 & 1 \\ -1 & 0 \end{bmatrix}.$
$\begin{bmatrix} a & b \\ c & d \end{bmatrix} = \begin{bmatrix} \cos \theta & \sin \theta \\ -\sin \theta & \cos \theta \end{bmatrix}.$
$\begin{bmatrix} a & b \\ c & d \end{bmatrix} = \begin{bmatrix} 1 & \lambda z \\ 0 & 1 \end{bmatrix}.$
where z is distance and λ is wave length.
• The Laplace transform corresponds to rotation by 90° into the complex domain, and can be represented by the matrix:
$\begin{bmatrix} a & b \\ c & d \end{bmatrix} = \begin{bmatrix} 0 & i \\ i & 0 \end{bmatrix}.$
$\begin{bmatrix} a & b \\ c & d \end{bmatrix} = \begin{bmatrix} i \cos \theta & i \sin \theta \\ i \sin \theta & -i \cos \theta \end{bmatrix}.$

## Composition

Composition of LCTs corresponds to multiplication of the corresponding matrices; this is also known as the "additivity property of the WDF".

In detail, if the LCT is denoted by OF(a,b,c,d), i.e.

$X_{(a,b,c,d)}(u) = O_F^{(a,b,c,d)}[x(t)] \,$

then

$O_F^{(a2,b2,c2,d2)} \left \{ O_F^{(a1,b1,c1,d1)}[x(t)] \right \} = O_F^{(a3,b3,c3,d3)}[x(t)] \, ,$

where

$\begin{bmatrix} a3 & b3 \\ c3 & d3 \end{bmatrix} = \begin{bmatrix} a2 & b2 \\ c2 & d2 \end{bmatrix} \begin{bmatrix} a1 & b1 \\ c1 & d1 \end{bmatrix}.$

## In optics and quantum mechanics

Paraxial optical systems implemented entirely with thin lenses and propagation through free space and/or graded index (GRIN) media, are quadratic phase systems (QPS); these were known before Moshinsky and Quesne (1974) called attention to their significance in connection with canonical transformations in quantum mechanics. The effect of any arbitrary QPS on an input wavefield can be described using the linear canonical transform, a particular case of which was developed by Segal (1963) and Bargmann (1961) in order to formalize Fock's (1928) boson calculus.[3]

## Applications

Canonical transforms are used to analyze differential equations. These include diffusion, the Schrödinger free particle, the linear potential (free-fall), and the attractive and repulsive oscillator equations. It also includes a few others such as the Fokker–Planck equation. Although this class is far from universal, the ease with which solutions and properties are found makes canonical transforms an attractive tool for problems such as these.[4]

Wave propagation through air, a lens, and between satellite dishes are discussed here. All of the computations can be reduced to 2×2 matrix algebra. This is the spirit of LCT.

### Electromagnetic wave propagation

Assuming the system looks like as depicted in the figure, the wave travels from plane xi, yi to the plane of x and y. The Fresnel transform is used to describe electromagnetic wave propagation in air:

$U_0(x,y) = - \frac{j}{\lambda} \frac{e^{jkz}}{z} \int_{-\infty}^\infty \int_{-\infty}^{\infty} e^{j \frac{k}{2z} [ (x-x_i)^2 +(y-y_i)^2 ] } U_i(x_i,y_i) \; dx_i\; dy_i,$

with

 k = 2 π / λ : wave number; λ : wavelength; z : distance of propagation; j : imaginary unit.

This is equivalent to LCT (shearing), when

$\begin{bmatrix} a & b \\ c & d \end{bmatrix} = \begin{bmatrix} 1 & \lambda z \\ 0 & 1 \end{bmatrix}.$

When the travel distance (z) is larger, the shearing effect is larger.

### Spherical lens

With the lens as depicted in the figure, and the refractive index denoted as n, the result is:[5]

$U_0(x,y) = e^{jkn \Delta} e^{-j \frac{k}{2f} [x^2 + y ^2]} U_i(x,y)$

with f the focal length and Δ the thickness of the lens.

The distortion passing through the lens is similar to LCT, when

$\begin{bmatrix} a & b \\ c & d \end{bmatrix} = \begin{bmatrix} 1 & 0 \\ \frac{-1}{\lambda f} & 1 \end{bmatrix}.$

This is also a shearing effect: when the focal length is smaller, the shearing effect is larger.

### Spherical Mirror

The spherical mirror—e.g., a satellite dish—can be described as a LCT, with

$\begin{bmatrix} a & b \\ c & d \end{bmatrix} = \begin{bmatrix} 1 & 0 \\ \frac{-1}{\lambda R} & 1 \end{bmatrix}.$

This is very similar to lens, except focal length is replaced by the radius of the dish. Therefore, if the radius is smaller, the shearing effect is larger.

## Example

The system considered is depicted in the figure to the right: two dishes – one being the emitter and the other one the receiver – and a signal travelling between them over a distance D. First, for dish A (emitter), the LCT matrix looks like this:

$\begin{bmatrix} 1 & 0 \\ \frac{-1}{\lambda R_A} & 1 \end{bmatrix}.$

Then, for dish B (receiver), the LCT matrix similarly becomes:

$\begin{bmatrix} 1 & 0 \\ \frac{-1}{\lambda R_B} & 1 \end{bmatrix}.$

Last, for the propagation of the signal in air, the LCT matrix is:

$\begin{bmatrix} 1 & \lambda D \\ 0 & 1 \end{bmatrix}.$

Putting all three components together, the LCT of the system is:

$\begin{bmatrix} a & b \\ c & d \end{bmatrix} = \begin{bmatrix} 1 & 0 \\ \frac{-1}{\lambda R_B} & 1 \end{bmatrix} \begin{bmatrix} 1 & \lambda D \\ 0 & 1 \end{bmatrix} \begin{bmatrix} 1 & 0 \\ \frac{-1}{\lambda R_A} & 1 \end{bmatrix} = \begin{bmatrix} 1-\frac{D}{R_A} & - \lambda D \\ \frac{1}{\lambda} (R_A^{-1} + R_B^{-1} - R_A^{-1}R_B^{-1}D) & 1 - \frac{D}{R_B} \end{bmatrix} \, .$

## See also

Other time–frequency transforms
Applications

## Notes

1. ^ de Bruijn, N. G. (1973). "A theory of generalized functions, with applications to Wigner distribution and Weyl correspondence", Nieuw Arch. Wiskd., III. Ser., 21 205-280.
2. ^ P.R. Deshmukh & A.S. Gudadhe (2011) Convolution structure for two version of fractional Laplace transform. Journal of Science and Arts, 2(15):143-150. [1]
3. ^ K.B. Wolf (1979) Ch. 9:Canonical transforms.
4. ^ K.B. Wolf (1979) Ch. 9 & 10.
5. ^ Goodman, Joseph W. (2005), Introduction to Fourier optics (3rd ed.), Roberts and Company Publishers, ISBN 0-9747077-2-4, §5.1.3, pp. 100–102.

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• S.A. Collins, "Lens-system diffraction integral written in terms of matrix optics," J. Opt. Soc. Amer. 60, 1168–1177 (1970).
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