# Linear canonical transformation

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.

The basic properties of the transformations mentioned above, such as scaling, shift, coordinate multiplication are considered. Any linear canonical transformation is related to affine transformations in phase space, defined by time-frequency or position-momentum coordinates.

## 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(C). Then for any such matrix ${\displaystyle \left({\begin{smallmatrix}a&b\\c&d\end{smallmatrix}}\right),}$ with ad − bc = 1, the corresponding integral transform from a function ${\displaystyle x(t)}$ to ${\displaystyle X(u)}$ is defined as

 ${\displaystyle X_{(a,b,c,d)}(u)={\sqrt {\frac {1}{ib}}}\cdot e^{i\pi {\frac {d}{b}}u^{2}}\int _{-\infty }^{\infty }e^{-i2\pi {\frac {1}{b}}ut}e^{i\pi {\frac {a}{b}}t^{2}}x(t)\;dt\,,}$ when b ≠ 0, ${\displaystyle X_{(a,0,c,d)}(u)={\sqrt {d}}\cdot e^{i\pi cdu^{2}}x(du)\,,}$ when b = 0.

## Special cases

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

• Scaling, ${\displaystyle x(u)\mapsto {\sqrt {\sigma }}x(\sigma u)}$, corresponds to scaling the time and frequency dimensions inversely (as time goes faster, frequencies are higher and the time dimension shrinks):
${\displaystyle {\begin{bmatrix}1/\sigma &0\\0&\sigma \end{bmatrix}}}$
${\displaystyle {\begin{bmatrix}a&b\\c&d\end{bmatrix}}={\begin{bmatrix}0&1\\-1&0\end{bmatrix}}.}$
${\displaystyle {\begin{bmatrix}a&b\\c&d\end{bmatrix}}={\begin{bmatrix}\cos \theta &\sin \theta \\-\sin \theta &\cos \theta \end{bmatrix}}.}$
${\displaystyle {\begin{bmatrix}a&b\\c&d\end{bmatrix}}={\begin{bmatrix}1&\lambda z\\0&1\end{bmatrix}}.}$
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:
${\displaystyle {\begin{bmatrix}a&b\\c&d\end{bmatrix}}={\begin{bmatrix}0&i\\i&0\end{bmatrix}}.}$
${\displaystyle {\begin{bmatrix}a&b\\c&d\end{bmatrix}}={\begin{bmatrix}i\cos \theta &i\sin \theta \\i\sin \theta &-i\cos \theta \end{bmatrix}}.}$

## 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.

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

then

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

where

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

If ${\displaystyle W_{X(a,b,c,d)}(u,v)}$is the ${\displaystyle X_{(a,b,c,d)}(u)}$, where ${\displaystyle X_{(a,b,c,d)}(u)}$is the LCT of ${\displaystyle x(t)}$, then

${\displaystyle {\begin{cases}W_{X(a,b,c,d)}(u,v)=W_{x}(du-bv,-cu+av)\\W_{X(a,b,c,d)}(au+bv,cu+dv)=W_{x}(u,v)\end{cases}}}$

LCT is equal to the twisting operation for the WDF and the Cohen's class distribution also has the twisting operation.

We can freely use the LCT to transform the parallelogram whose center is at (0,0) to another parallelogram which has the same area and the same center

From this picture we know that the point (-1,2) transform to the point (0,1) and the point (1,2) transform to the point (4,3). As the result, we can write down the equations below

${\displaystyle {\begin{cases}-a+2b=0\\-c+2d=1\end{cases}}\,and\,{\begin{cases}a+2b=4\\c+2d=3\end{cases}}}$

we can solve the equations and get (a,b,c,d) is equal to (2,1,1,1)

## Relation

From the following picture, we summarize the LCT with other transform or properties

## 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]

In Quantum mechanics, linear canonical transformations can be identified with the linear transformations which mix the Momentum operator with the Position operator and leave invariant the Canonical commutation relations.

## 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:

${\displaystyle U_{0}(x,y)=-{\frac {j}{\lambda }}{\frac {e^{jkz}}{z}}\int _{-\infty }^{\infty }\int _{-\infty }^{\infty }e^{j{\frac {k}{2z}}[(x-x_{i})^{2}+(y-y_{i})^{2}]}U_{i}(x_{i},y_{i})\;dx_{i}\;dy_{i},}$

with

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

This is equivalent to LCT (shearing), when

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

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]

${\displaystyle U_{0}(x,y)=e^{jkn\Delta }e^{-j{\frac {k}{2f}}[x^{2}+y^{2}]}U_{i}(x,y)}$

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

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

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

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

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

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.

### Joint Free space and Spherical lens

The relation between the input and output we can use LCT to represent

${\displaystyle {\begin{bmatrix}a&b\\c&d\end{bmatrix}}={\begin{bmatrix}1&\lambda z_{2}\\0&1\end{bmatrix}}{\begin{bmatrix}1&0\\0&-1/\lambda f\end{bmatrix}}{\begin{bmatrix}1&\lambda z_{1}\\0&1\end{bmatrix}}={\begin{bmatrix}1-z_{2}/f&\lambda (z_{1}+z_{2})-\lambda z_{1}z_{2}/f\\-1/\lambda f&1-z_{1}/f\end{bmatrix}}}$

(1) If z1 = z2 = 2f, it is reverse real image

(2) If z1 = z2 = f, it is Fourier transform+scaling

(3) if z1=z2, it is fractional Fourier transform+scaling

## Basic Properties

In this part, we show the basic properties of LCT

Operator Matrix of transform
${\displaystyle L(T)}$ ${\displaystyle {\begin{bmatrix}a&b\\c&d\end{bmatrix}}}$
${\displaystyle L(T_{1})L(T_{2})}$ ${\displaystyle T_{2}T_{1}}$
${\displaystyle L^{-1}(T)=L(T^{-1})}$ ${\displaystyle {\begin{bmatrix}d^{t}&-b^{t}\\-c^{t}&a^{t}\end{bmatrix}}}$
${\displaystyle L({\widehat {T}})=L^{*}(T^{-1})}$ ${\displaystyle {\begin{bmatrix}d^{t}&b^{t}\\c^{t}&a^{t}\end{bmatrix}}}$
${\displaystyle F}$ ${\displaystyle {\begin{bmatrix}0&I\\-I&0\end{bmatrix}}}$
${\displaystyle {\begin{cases}FL(T)F^{-1}=L^{*}(T^{t-1})\\F^{-1}L(T)F=L^{*}(T^{t-1})\end{cases}}}$ ${\displaystyle {\begin{bmatrix}d&-c\\-b&a\end{bmatrix}}}$

With the two-dimension column vector r defined as r =${\displaystyle {\begin{bmatrix}x\\y\end{bmatrix}}}$, we show some basic properties (result) for the specific input below

Input Output Remark
${\displaystyle f_{i}(r)}$ ${\displaystyle f_{o}(r)=L(T){\displaystyle f_{i}(r)},\,where\,T={\begin{bmatrix}a&b\\c&d\end{bmatrix}}}$
${\displaystyle \sum _{n}a_{n}f_{n}(r)}$ ${\displaystyle \sum _{n}a_{n}Lf_{n}(r)}$ Linearity
${\displaystyle f_{i}(r),h_{i}(r)}$ ${\displaystyle \int f_{i}(r)h_{i}^{*}(r)dr=\int f_{o}(r)h_{o}^{*}(r)dr}$ parseval's theorem
${\displaystyle f_{i}^{*}(r)}$ ${\displaystyle [L(T^{-1})f_{i}(r)]^{*}\,where\,T^{-1}={\begin{bmatrix}d^{t}&-b^{t}\\-c^{t}&a^{t}\end{bmatrix}}}$ complex conjugate
${\displaystyle \mathrm {M} ^{n}f_{i}(r)}$ ${\displaystyle (d^{t}\mathrm {M} -b^{t}D)^{n}f_{o}(r)\,\,\,\,\mathrm {M} =r}$ multiplication
${\displaystyle D^{n}f_{i}(r)}$ ${\displaystyle (-c^{t}\mathrm {M} -a^{t}D)^{n}f_{o}(r)\,\,\,\,D=(i2\pi )^{-1}\nabla ^{t}}$ derivation
${\displaystyle f_{i}(r)exp(j2\pi k^{t}r)}$ ${\displaystyle f_{o}(r-bk)exp(j2\pi k^{t}d^{t}r)exp(-i\pi k^{t}b^{t}dk)}$ modulation
${\displaystyle f_{i}(r-k)}$ ${\displaystyle f_{o}(r)exp(j2\pi k^{t}c^{t}r)exp(-i\pi k^{t}c^{t}ak)}$ shift
${\displaystyle |detW|^{-1/2}f_{i}(W^{-1}r)}$ ${\displaystyle L({\tilde {T}})f_{i}(r)\,\,where\,\,{\tilde {T}}=T{\begin{bmatrix}W&0\\0&W^{t-1}\end{bmatrix}}}$ scaling
${\displaystyle f_{i}(-r)}$ ${\displaystyle L(-T)f_{i}(r)=f_{o}(-r)}$ scaling
1 ${\displaystyle (det(A))^{-1/2}exp(i\pi r^{t}CA^{-1}r)}$
${\displaystyle exp(j\pi r^{t}L_{i}r)}$ ${\displaystyle [det(A+iL_{i})]^{-1/2}exp(-\pi r^{t}L_{o}r),\,where\,iL_{o}=(C+iDL_{i})(A+iBL_{i})^{-1}}$
${\displaystyle exp(j2\pi k^{t}r)}$ ${\displaystyle (det(A))^{-1/2}exp(i\pi r^{t}CA^{-1}r)*exp(-i\pi k^{t}A^{-1}BK)exp(i2\pi k^{t}CA^{-1}r)}$

## 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:

${\displaystyle {\begin{bmatrix}1&0\\{\frac {-1}{\lambda R_{A}}}&1\end{bmatrix}}.}$

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

${\displaystyle {\begin{bmatrix}1&0\\{\frac {-1}{\lambda R_{B}}}&1\end{bmatrix}}.}$

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

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

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

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

## Relation with Particle physics

It has been shown that it may be possible to establish a relation between some properties of the elementary Fermion in the Standard Model of Particle physics and Spin representation of linear canonical transformations. [6] In this approach, the Electric charge, Weak hypercharge and Weak isospin of the particles are expressed as linear combinations of some operators defined from the generators of the Clifford algebra associated with the spin representation of linear canonical transformations.

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. "Archived copy". Archived from the original on 2012-12-23. Retrieved 2012-08-29.CS1 maint: archived copy as title (link)
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.
6. ^ R. T. Ranaivoson, Raoelina Andriambololona, R. Hanitriarivo, R. Raboanary (2020). https://arxiv.org/abs/1804.10053

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