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'''Ray transfer matrix analysis''' (also known as '''ABCD matrix analysis''') is a type of [[Ray tracing (physics)|ray tracing]] technique used in the design of some [[optics|optical]] systems, particularly [[laser]]s. It involves the construction of a ''ray transfer [[matrix (math)|matrix]]'' which describes the optical system; tracing of a light path through the system can then be performed by multiplying this matrix with a [[vector space|vector]] representing the [[light ray]]. The same analysis is also used in [[accelerator physics]] to track particles through the magnet installations of a [[particle accelerator]], see [[Beam optics]].  
 
The technique that is described below uses the ''[[paraxial approximation]]'' of ray optics, which means that all rays are assumed to be at a small angle (θ) and a small distance (''x'') relative to the [[optical axis]] of the system.<ref>An exact method for tracing meridional rays is available [http://spie.org/Documents/ETOP/1991/389_1.pdf here].</ref>
 
== Definition of the ray transfer matrix ==
 
The ray tracing technique is based on two reference planes, called the ''input'' and ''output'' planes, each perpendicular to the optical axis of the system. Without loss of generality, we will define the optical axis so that it coincides with the ''z''-axis of a fixed coordinate system. A light ray enters the system when the ray crosses the input plane at a distance ''x''<sub>1</sub> from the optical axis while traveling in a direction that makes an angle θ<sub>1</sub> with the optical axis. Some distance further along, the ray crosses the output plane, this time at a distance ''x''<sub>2</sub> from the optical axis and making an angle θ<sub>2</sub>.  ''n''<sub>1</sub> and ''n''<sub>2</sub> are the [[index of refraction|indices of refraction]] of the medium in the input and output plane, respectively.
 
These quantities are related by the expression
 
:<math> {x_2 \choose \theta_2} = \begin{pmatrix} A & B \\ C & D \end{pmatrix}{x_1 \choose \theta_1}, </math>
 
where
 
:<math>A = {x_2 \over x_1 } \bigg|_{\theta_1 = 0} \qquad B = {x_2 \over \theta_1 } \bigg|_{x_1 = 0},</math>
 
and
 
:<math>C = {\theta_2 \over x_1 } \bigg|_{\theta_1 = 0} \qquad D = {\theta_2 \over \theta_1 } \bigg|_{x_1 = 0}.</math>
 
This relates the ''ray vectors'' at the input and output planes by the ''ray transfer matrix'' (RTM) '''M''', which represents the optical system between the two reference planes.  A [[thermodynamics]] argument based on the [[blackbody]] radiation can be used to show that the [[determinant]] of a RTM is the ratio of the indices of refraction:
 
:<math>\det(\mathbf{M}) = AD - BC = {  n_1  \over  n_2 }.  </math>
 
As a result, if the input and output planes are located within the same medium, or within two different media which happen to have identical indices of refraction, then the determinant of '''M''' is simply equal to 1.
 
A similar technique can be used to analyze [[electrical circuits]].  ''See'' [[Two-port network]]s.
 
== Some examples ==
 
* For example, if there is free space between the two planes, the ray transfer matrix is given by:
 
:<math> \mathbf{S} = \begin{pmatrix} 1 & d \\ 0 & 1 \end{pmatrix} </math>,
 
where ''d'' is the separation distance (measured along the optical axis) between the two reference planes. The ray transfer equation thus becomes:
 
:<math> {x_2 \choose \theta_2} = \mathbf{S}{x_1 \choose \theta_1} </math>,
 
and this relates the parameters of the two rays as:
 
:<math> \begin{matrix} x_2 & = & x_1 + d\theta_1 \\
\theta_2 & = & \theta_1 \end{matrix} </math>
 
* Another simple example is that of a [[thin lens]]. Its RTM is given by:
 
:<math> \mathbf{L} = \begin{pmatrix} 1 & 0 \\ \frac{-1}{f} & 1 \end{pmatrix} </math>,
 
where ''f'' is the [[focal length]] of the lens. To describe combinations of optical components, ray transfer matrices may be multiplied together to obtain an overall RTM for the compound optical system. For the example of free space of length ''d'' followed by a lens of focal length ''f'':
 
:<math>\mathbf{L}\mathbf{S} = \begin{pmatrix} 1 & 0 \\ \frac{-1}{f} & 1\end{pmatrix}
\begin{pmatrix} 1 & d \\ 0 & 1 \end{pmatrix}
= \begin{pmatrix} 1 & d \\ \frac{-1}{f} & 1-\frac{d}{f} \end{pmatrix} </math>.
 
Note that, since the multiplication of matrices is non-[[commutative]], this is not the same RTM as that for a lens followed by free space:
 
:<math> \mathbf{SL} =
\begin{pmatrix} 1 & d \\ 0 & 1 \end{pmatrix}
\begin{pmatrix} 1 & 0 \\ \frac{-1}{f} & 1\end{pmatrix}
= \begin{pmatrix} 1-\frac{d}{f} & d \\ \frac{-1}{f} & 1 \end{pmatrix} </math>.
 
Thus the matrices must be ordered appropriately, with the last matrix premultiplying the second last, and so on until the first matrix is premultiplied by the second. Other matrices can be constructed to represent interfaces with media of different [[refractive index|refractive indices]], reflection from [[mirror]]s, etc.
 
== Table of ray transfer matrices ==
'''for simple optical components'''
 
{| border="1" cellspacing="0" cellpadding="4"
|- style="background-color: #AAFFCC"
! Element
! Matrix
! Remarks
|-
| Propagation in free space or in a medium of constant refractive index
| align="center" |<math>\begin{pmatrix} 1 & d\\ 0 & 1 \end{pmatrix} </math>
| ''d'' = distance<br/>
|-
| Refraction at a flat interface
| align="center" | <math>\begin{pmatrix} 1 & 0 \\ 0 & \frac{n_1}{n_2} \end{pmatrix} </math>
| ''n''<sub>1</sub> = initial refractive index<br/>
''n''<sub>2</sub> = final refractive index.
|-
| Refraction at a curved interface
| align="center" | <math>\begin{pmatrix} 1 & 0 \\ \frac{n_1-n_2}{R \cdot n_2} & \frac{n_1}{n_2} \end{pmatrix} </math>
| ''R'' = radius of curvature, ''R'' > 0 for convex (centre of curvature after interface)<br/>
''n''<sub>1</sub> = initial refractive index<br/>
''n''<sub>2</sub> = final refractive index.
|-
| Reflection from a flat mirror
| align="center" | <math> \begin{pmatrix} 1 & 0 \\ 0 & 1 \end{pmatrix} </math>
|
|-
| Reflection from a curved mirror
| align="center" | <math> \begin{pmatrix} 1 & 0 \\ -\frac{2}{R} & 1 \end{pmatrix} </math>
| ''R'' = radius of curvature, R > 0 for concave, valid in the paraxial approximation
|-
| Thin lens
| align="center" | <math> \begin{pmatrix} 1 & 0 \\ -\frac{1}{f} & 1 \end{pmatrix} </math>
| ''f'' = focal length of lens where ''f'' > 0 for convex/positive (converging) lens.
Only valid if the focal length is much greater than the thickness of the lens.
|-
| Thick lens
| align="center" | <math>\begin{pmatrix} 1 & 0 \\ \frac{n_2-n_1}{R_2n_1} & \frac{n_2}{n_1} \end{pmatrix} \begin{pmatrix} 1 & t \\ 0 & 1 \end{pmatrix} \begin{pmatrix} 1 & 0 \\ \frac{n_1-n_2}{R_1n_2} & \frac{n_1}{n_2} \end{pmatrix}</math>
| ''n''<sub>1</sub> = refractive index outside of the lens. <br/>
''n''<sub>2</sub> = refractive index of the lens itself (inside the lens). <br/>
''R''<sub>1</sub> = Radius of curvature of First surface. <br/>
''R''<sub>2</sub> = Radius of curvature of Second surface.<br/>
''t'' = center thickness of lens.
|-  
| Single right angle prism
| align="center" | <math> \begin{pmatrix} k & \frac{d}{nk} \\ 0 & \frac{1}{k} \end{pmatrix} </math>
| ''k'' = (cos<math>\psi</math>/cos<math>\phi</math>) is the [[beam expander|beam expansion]] factor, where <math>\phi</math> is the angle of incidence, <math>\psi</math> is the angle of refraction, ''d'' = prism path length, ''n'' = refractive index of the prism material.  This matrix applies for orthogonal beam exit.
|}
 
== Resonator stability ==
 
RTM analysis is particularly useful when modeling the behaviour of light in [[optical resonator]]s, such as those used in lasers. At its simplest, an optical resonator consists of two identical facing mirrors of 100% [[reflectivity]] and radius of [[curvature]] ''R'', separated by some distance ''d''. For the purposes of ray tracing, this is equivalent to a series of identical thin lenses of focal length ''f''=''R''/2, each separated from the next by length ''d''. This construction is known as a ''lens equivalent duct'' or ''lens equivalent [[waveguide]]''. The RTM of each section of the waveguide is, as above,
 
:<math>\mathbf{M} =\mathbf{L}\mathbf{S} = \begin{pmatrix} 1 & d \\ \frac{-1}{f} & 1-\frac{d}{f} \end{pmatrix} </math>.
 
RTM analysis can now be used to determine the ''stability'' of the waveguide (and equivalently, the resonator). That is, it can be determined under what conditions light travelling down the waveguide will be periodically refocussed and stay within the waveguide. To do so, we can find all the "eigenrays" of the system: the input ray vector at each of the mentioned sections of the waveguide times a real or complex factor λ is equal to the output one. This gives:
 
:<math> \mathbf{M}{x_1 \choose \theta_1} = {x_2 \choose \theta_2} = \lambda {x_1 \choose \theta_1} </math>.
 
which is an [[eigenvalue]] equation:
 
:<math> \left[ \mathbf{M} - \lambda\mathbf{I} \right] {x_1 \choose \theta_1} = 0 </math>,
 
where '''I''' is the 2x2 [[identity matrix]].
 
We proceed to calculate the eigenvalues of the transfer matrix:
 
:<math>\operatorname{det}  \left[  \mathbf{M} - \lambda\mathbf{I} \right] = 0  </math>,
 
leading to the [[Characteristic polynomial#Characteristic equation|characteristic equation]]
 
:<math> \lambda^2 - \operatorname{tr}(\mathbf{M}) \lambda + \operatorname{det}( \mathbf{M}) = 0 </math>,
 
where
 
:<math>  \operatorname{tr} ( \mathbf{M} )  =    A + D  =  2 - { d \over f }  </math>
 
is the [[trace (linear algebra)|trace]] of the RTM, and
 
:<math>\operatorname{det}(\mathbf{M}) = AD - BC  = 1 </math>
 
is the [[determinant]] of the RTM. After one common substitution we have:
 
:<math> \lambda^2 - 2g \lambda + 1 = 0  </math>,
 
where
 
:<math> g \ \stackrel{\mathrm{def}}{=}\  { \operatorname{tr}(\mathbf{M}) \over 2 } = 1 - { d \over 2 f } </math>
 
is the ''stability parameter''. The eigenvalues are the solutions of the characteristic equation. From the [[Quadratic equation#Quadratic formula|quadratic formula]] we find
 
:<math> \lambda_{\pm}  =  g \pm \sqrt{g^2 - 1} \, </math>
 
Now, consider a ray after ''N'' passes through the system:
 
:<math> {x_N \choose \theta_N} = \lambda^N {x_1 \choose \theta_1} </math>.
 
If the waveguide is stable, no ray should stray arbitrarily far from the main axis, that is, λ<sup>N</sup> must not grow without limit. Suppose <math> g^2 > 1</math>. Then both eigenvalues are real. Since <math> \lambda_+ \lambda_- = 1</math>, one of them has to be bigger than 1 (in absolute value), which implies that the ray which corresponds to this eigenvector would not converge. Therefore in a stable waveguide, <math> g^2 </math> ≤ 1,  and the eigenvalues can be represented by complex numbers:
 
:<math> \lambda_{\pm} = g \pm i \sqrt{1 - g^2} = \cos(\phi) \pm i \sin(\phi) =  e^{\pm i \phi} </math>,
 
with the substitution g = cos(ϕ).
 
For <math> g^2 < 1 </math> let <math> r_+ </math> and <math> r_- </math> be the eigenvectors with respect to the eigenvalues <math> \lambda_+ </math> and <math> \lambda_- </math> respectively, which span all the vector space because they are orthogonal, the latter due to <math>\lambda_+</math> ≠ <math>\lambda_- </math>. The input vector can therefore be written as
 
:<math> c_+ r_+ + c_- r_-  </math>,
 
for some constants <math> c_+ </math> and <math> c_- </math>.
 
After ''N'' waveguide sectors, the output reads
 
:<math> \mathbf{M}^N (c_+ r_+ + c_- r_-) = \lambda_+^N c_+ r_+ + \lambda_-^N c_- r_- = e^{i N \phi} c_+ r_+ + e^{- i N \phi} c_- r_- </math>,
 
what represents a periodic function.
 
== Ray transfer matrices for Gaussian beams ==
 
The matrix formalism is also useful to describe [[Gaussian beam]]s. If we have a Gaussian beam of wavelength <math>\lambda_0</math>, radius of curvature ''R'', beam spot size ''w'' and refractive index ''n'', it is possible to define a [[complex beam parameter]] ''q'' by:
 
:<math> \frac{1}{q} = \frac{1}{R} - \frac{i\lambda_0}{\pi n w^2} </math>.
 
This beam can be propagated through an optical system with a given ray transfer matrix by using the equation:
 
:<math> {q_2 \choose 1} = k \begin{pmatrix} A & B \\ C & D \end{pmatrix} {q_1 \choose 1} </math>,
 
where ''k'' is a normalisation constant chosen to keep the second component of the ray vector equal to 1. Using [[matrix multiplication]], this equation expands as
 
:<math> q_2 = k(Aq_1 + B) \,</math>
 
and
 
:<math> 1 =  k(Cq_1 + D) \,  </math>
 
Dividing the first equation by the second eliminates the normalisation constant:
 
:<math> q_2 =\frac{Aq_1+B}{Cq_1+D}</math>,
 
It is often convenient to express this last equation in reciprocal form:
 
:<math>  { 1 \over q_2 }    = {  C + D/q_1  \over  A + B/q_1 } .  </math>
 
== See also ==
* [[Transfer-matrix method (optics)]]
* [[Two-port network]]
* [[Linear canonical transformation]]
 
== References ==
{{reflist}}
{{refbegin}}
*:{{cite book | title = Fundamentals of Photonics | author = [[Bahaa E. A. Saleh]] and Malvin Carl Teich | publisher = John Wiley & Sons | location = New York |  year = 1991 }} Section 1.4, pp.&nbsp;26 – 36.
 
*:{{cite book
|title= Introduction to matrix methods in optics
|last1= Gerrard |first1= Anthony
|last2= Burch |first2 = James M.
|year=1994
|publisher=Courier Dover
|location=
|isbn= 9780486680446
|pages=
|url=http://books.google.de/books?id=naUSNojPwOgC
}}
 
*:{{cite book | title = Tunable Laser Optics | author = [[F. J. Duarte]] | publisher = Elsevier-Academic | location = New York |  year = 2003 }} Chapter 6.
 
{{refend}}
 
== External links ==
* [http://physics.tamuk.edu/~suson/html/4323/thick.html#Matrix Thick lenses (Matrix methods)]
* [http://www.photonics.byu.edu/ABCD_Matrix_tut.phtml ABCD Matrices Tutorial]  Provides an example for a system matrix of an entire system.
* [http://www.photonics.byu.edu/ABCD_Calc.phtml ABCD Calculator]  An interactive calculator to help solve ABCD matrices.
* [http://play.google.com/store/apps/details?id=com.dmt195.simple.abcd.optical.designer Simple Optical Designer (Android App)] An application to explore optical systems using the ABCD matrix method.
 
[[Category:Geometrical optics]]
[[Category:Accelerator physics]]

Revision as of 20:01, 2 February 2014

Ray transfer matrix analysis (also known as ABCD matrix analysis) is a type of ray tracing technique used in the design of some optical systems, particularly lasers. It involves the construction of a ray transfer matrix which describes the optical system; tracing of a light path through the system can then be performed by multiplying this matrix with a vector representing the light ray. The same analysis is also used in accelerator physics to track particles through the magnet installations of a particle accelerator, see Beam optics.

The technique that is described below uses the paraxial approximation of ray optics, which means that all rays are assumed to be at a small angle (θ) and a small distance (x) relative to the optical axis of the system.[1]

Definition of the ray transfer matrix

The ray tracing technique is based on two reference planes, called the input and output planes, each perpendicular to the optical axis of the system. Without loss of generality, we will define the optical axis so that it coincides with the z-axis of a fixed coordinate system. A light ray enters the system when the ray crosses the input plane at a distance x1 from the optical axis while traveling in a direction that makes an angle θ1 with the optical axis. Some distance further along, the ray crosses the output plane, this time at a distance x2 from the optical axis and making an angle θ2. n1 and n2 are the indices of refraction of the medium in the input and output plane, respectively.

These quantities are related by the expression

(x2θ2)=(ABCD)(x1θ1),

where

A=x2x1|θ1=0B=x2θ1|x1=0,

and

C=θ2x1|θ1=0D=θ2θ1|x1=0.

This relates the ray vectors at the input and output planes by the ray transfer matrix (RTM) M, which represents the optical system between the two reference planes. A thermodynamics argument based on the blackbody radiation can be used to show that the determinant of a RTM is the ratio of the indices of refraction:

det(M)=ADBC=n1n2.

As a result, if the input and output planes are located within the same medium, or within two different media which happen to have identical indices of refraction, then the determinant of M is simply equal to 1.

A similar technique can be used to analyze electrical circuits. See Two-port networks.

Some examples

  • For example, if there is free space between the two planes, the ray transfer matrix is given by:
S=(1d01),

where d is the separation distance (measured along the optical axis) between the two reference planes. The ray transfer equation thus becomes:

(x2θ2)=S(x1θ1),

and this relates the parameters of the two rays as:

x2=x1+dθ1θ2=θ1
  • Another simple example is that of a thin lens. Its RTM is given by:
L=(101f1),

where f is the focal length of the lens. To describe combinations of optical components, ray transfer matrices may be multiplied together to obtain an overall RTM for the compound optical system. For the example of free space of length d followed by a lens of focal length f:

LS=(101f1)(1d01)=(1d1f1df).

Note that, since the multiplication of matrices is non-commutative, this is not the same RTM as that for a lens followed by free space:

SL=(1d01)(101f1)=(1dfd1f1).

Thus the matrices must be ordered appropriately, with the last matrix premultiplying the second last, and so on until the first matrix is premultiplied by the second. Other matrices can be constructed to represent interfaces with media of different refractive indices, reflection from mirrors, etc.

Table of ray transfer matrices

for simple optical components

Element Matrix Remarks
Propagation in free space or in a medium of constant refractive index (1d01) d = distance
Refraction at a flat interface (100n1n2) n1 = initial refractive index

n2 = final refractive index.

Refraction at a curved interface (10n1n2Rn2n1n2) R = radius of curvature, R > 0 for convex (centre of curvature after interface)

n1 = initial refractive index
n2 = final refractive index.

Reflection from a flat mirror (1001)
Reflection from a curved mirror (102R1) R = radius of curvature, R > 0 for concave, valid in the paraxial approximation
Thin lens (101f1) f = focal length of lens where f > 0 for convex/positive (converging) lens.

Only valid if the focal length is much greater than the thickness of the lens.

Thick lens (10n2n1R2n1n2n1)(1t01)(10n1n2R1n2n1n2) n1 = refractive index outside of the lens.

n2 = refractive index of the lens itself (inside the lens).
R1 = Radius of curvature of First surface.
R2 = Radius of curvature of Second surface.
t = center thickness of lens.

Single right angle prism (kdnk01k) k = (cosψ/cosϕ) is the beam expansion factor, where ϕ is the angle of incidence, ψ is the angle of refraction, d = prism path length, n = refractive index of the prism material. This matrix applies for orthogonal beam exit.

Resonator stability

RTM analysis is particularly useful when modeling the behaviour of light in optical resonators, such as those used in lasers. At its simplest, an optical resonator consists of two identical facing mirrors of 100% reflectivity and radius of curvature R, separated by some distance d. For the purposes of ray tracing, this is equivalent to a series of identical thin lenses of focal length f=R/2, each separated from the next by length d. This construction is known as a lens equivalent duct or lens equivalent waveguide. The RTM of each section of the waveguide is, as above,

M=LS=(1d1f1df).

RTM analysis can now be used to determine the stability of the waveguide (and equivalently, the resonator). That is, it can be determined under what conditions light travelling down the waveguide will be periodically refocussed and stay within the waveguide. To do so, we can find all the "eigenrays" of the system: the input ray vector at each of the mentioned sections of the waveguide times a real or complex factor λ is equal to the output one. This gives:

M(x1θ1)=(x2θ2)=λ(x1θ1).

which is an eigenvalue equation:

[MλI](x1θ1)=0,

where I is the 2x2 identity matrix.

We proceed to calculate the eigenvalues of the transfer matrix:

det[MλI]=0,

leading to the characteristic equation

λ2tr(M)λ+det(M)=0,

where

tr(M)=A+D=2df

is the trace of the RTM, and

det(M)=ADBC=1

is the determinant of the RTM. After one common substitution we have:

λ22gλ+1=0,

where

g=deftr(M)2=1d2f

is the stability parameter. The eigenvalues are the solutions of the characteristic equation. From the quadratic formula we find

λ±=g±g21

Now, consider a ray after N passes through the system:

(xNθN)=λN(x1θ1).

If the waveguide is stable, no ray should stray arbitrarily far from the main axis, that is, λN must not grow without limit. Suppose g2>1. Then both eigenvalues are real. Since λ+λ=1, one of them has to be bigger than 1 (in absolute value), which implies that the ray which corresponds to this eigenvector would not converge. Therefore in a stable waveguide, g2 ≤ 1, and the eigenvalues can be represented by complex numbers:

λ±=g±i1g2=cos(ϕ)±isin(ϕ)=e±iϕ,

with the substitution g = cos(ϕ).

For g2<1 let r+ and r be the eigenvectors with respect to the eigenvalues λ+ and λ respectively, which span all the vector space because they are orthogonal, the latter due to λ+λ. The input vector can therefore be written as

c+r++cr,

for some constants c+ and c.

After N waveguide sectors, the output reads

MN(c+r++cr)=λ+Nc+r++λNcr=eiNϕc+r++eiNϕcr,

what represents a periodic function.

Ray transfer matrices for Gaussian beams

The matrix formalism is also useful to describe Gaussian beams. If we have a Gaussian beam of wavelength λ0, radius of curvature R, beam spot size w and refractive index n, it is possible to define a complex beam parameter q by:

1q=1Riλ0πnw2.

This beam can be propagated through an optical system with a given ray transfer matrix by using the equation:

(q21)=k(ABCD)(q11),

where k is a normalisation constant chosen to keep the second component of the ray vector equal to 1. Using matrix multiplication, this equation expands as

q2=k(Aq1+B)

and

1=k(Cq1+D)

Dividing the first equation by the second eliminates the normalisation constant:

q2=Aq1+BCq1+D,

It is often convenient to express this last equation in reciprocal form:

1q2=C+D/q1A+B/q1.

See also

References

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    My blog: http://www.primaboinca.com/view_profile.php?userid=5889534 Section 1.4, pp. 26 – 36.
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Template:Refend

External links

  1. An exact method for tracing meridional rays is available here.