124 |
3.1.7 Beam propagation in optical systems |
[Ref. p. 131 |
Srotated cyl.
with |
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A = |
0 1 |
||
1 0 |
and
= R−1 Scyl R = A B
C D
, B = |
0 0 |
, C = |
− cos2 θ/fx |
− sin θ cos θ/fx |
, D = |
1 0 |
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0 0 |
− sin θ cos θ/fx |
− sin2 θ/fx |
0 1 |
O |
− sin θ cos θ/fx |
− sin2 θ/fx + 1/qyy |
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Q−1 = |
− cos2 θ/fx + 1/qxx |
− sin θ cos θ/fx . |
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Therefore, the output field |
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k |
cos2 θ |
1 |
sin |
θ cos θ |
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u O (r) = exp −i |
− |
+ |
x2 − 2 |
xy + |
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2 |
fx |
qxx |
fx |
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− sin2 θ + 1 y2
fx qyy
is a general astigmatic Gaussian beam with a mixing term between the coordinates x and y.
Often, the transfer of the beam waist is required for instance for focusing of laser light. Then, the following algorithms are much more simple than the q-parameter algorithm.
In Table 3.1.20 the waist transformation for a general system is given.
The formulae (3.1.123)–(3.1.126) are further simplified using the focal length f for the thin lens only, see Table 3.1.21.
Remark : Discussion of equation (3.1.127):
The right-hand-side term of (3.1.127) containing z0 represents the modification introduced by the Gaussian beam optics to the thin-lens equation ((3.1.95), t 0) shown in Fig. 3.1.42.
In Fig. 3.1.43 the relation of the Gaussian waist transfer to the thin-lens equation of geometrical optics for di erent influences of di raction is shown.
Main modifications of the geometrical optics:
– No “image distance” is at infinity.
– |
For z = f (point P ) the image is at z = f (transfer of the object-side focal plane to the image-side |
focal plane after (3.1.130), not ∞). |
|
– |
If a target z -position is given, then two starting z-positions are possible. |
Example 3.1.17. Given for Fig. 3.1.42: z = 1179 mm, w0 = 0.22 mm, λ = 1.06 µm; it follows z = 109 mm, w0 = 0.02 mm, θ = 0.96◦ , and z0 = 1.21 mm. The second right-hand term of (3.1.127) translates the Gaussian waist image by 0.16 mm in comparison with the geometrical optical image towards the lens.
Landolt-B¨ornstein
New Series VIII/1A1
Ref. p. 131] |
3.1 Linear optics |
125 |
Table 3.1.20. Waist transformation for a general system.
Given |
Solution |
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– ABCD-matrix of the system, |
z |
= |
− |
B)(Cz + D) |
ACz2 |
||||||||||||||||||||||||||||||
– |
waist w0, |
C2z0 |
+ (Cz + D) |
0 for |
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(Az + 2 |
−2 |
C = 0 , |
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– |
wavelength λ , including z0 = π w02/λ , |
Az + B |
for |
C = 0 , |
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– |
distance z to the input plane of the system. |
− |
D |
(3.1.123) |
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Cz + A |
z0 |
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z 0 |
z0’ |
z0 |
= z0 |
= |
, |
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Optical system |
Cz + D |
C2z02 + (Cz + D)2 |
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w |
0 |
characterized by its |
’ |
w ’ |
(3.1.124) |
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0 |
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z |
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A B |
- matrix |
w0 = |
z |
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C D |
λ 0 |
, |
(3.1.125) |
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z |
z ’ |
π |
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Θ0 |
= π z0 . |
(3.1.126) |
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λ |
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Fig. 3.1.41. Waist transformation by an optical |
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system. |
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The beam parameter product is invariant: |
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Asked : Waist w0 and distance z to the output plane |
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of the system including z . |
= w0 Θ0 |
= λ/π . |
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0 |
w0 Θ0 |
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Table 3.1.21. Waist transformation by a thin lens.
Given |
Solution |
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– |
Focal length f of the lens, |
1 |
1 |
1 |
2 |
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+ |
= |
+ |
z0 |
, |
(3.1.127) |
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– |
wavelength λ , |
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z [z2 + z02 |
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2 |
/λ , |
z |
z |
f |
− zf ] |
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– |
waist w0 , including z0 = π w0 |
see Fig. 3.1.42, |
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– |
distance z to the input plane of the system. |
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w0 = w0 |
f |
, |
(3.1.128) |
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0 |
0 |
z02 |
+ (z − f )2 |
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w |
w ’ |
π w |
2 |
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f |
f |
z0 |
= |
0 |
. |
(3.1.129) |
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Image point |
λ |
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of paraxial optics |
If z = f , then |
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z |
z ’ |
z |
= f |
and |
w0 = |
w0f |
. |
(3.1.130) |
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Fig. 3.1.42. Waist transformation by a thin lens. |
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z0 |
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Asked : Waist w0 and distance z to the output plane of the system and z0 .
Landolt-B¨ornstein
New Series VIII/1A1
126 |
3.1.7 Beam propagation in optical systems |
[Ref. p. 131 |
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4 |
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Geometrical optics |
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3 |
z0 /f = 3 |
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2 |
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f 1 |
z0 /f = 1 |
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P |
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|
'/ |
z0 /f = 0.5 |
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0 |
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|
z |
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z0 /f = 0.3 |
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-1 |
Geometrical optics |
z0 /f = 0.2 |
Fig. 3.1.43. Relation of the Gaussian waist transfer (full |
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-2 |
|||||||||||||||
-3 |
lines) to the thin-lens equation (dashed) of geometrical |
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-3 |
-2 |
-1 |
0 |
1 |
2 |
3 |
4 |
optics for di erent influences of di raction (wavelength λ |
|||||||
z / f |
respectively z0). |
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For Fresnel’s approximation of di raction in paraxial systems see [68Goo, 71Col, 78Loh, 94Roe]. It was generalized to the propagation of field distributions in ABCD-described systems by [70Col, 76Arn, 05Gro2, 05Hod].
In Table 3.1.22 the propagation in rotational symmetric systems and simple astigmatic systems is given.
Table 3.1.22. Propagation in rotational symmetric systems and simple astigmatic systems.
Given |
Solution |
||||||||||||
– ABCD-matrix of the optical |
Field U O(x2) in the output plane (Collins integral ): |
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system (see Tables 3.1.11 |
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U O(x2) = |
i |
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and 3.1.12), |
e− |
ikL |
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– field distribution in the in- |
λ B |
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put plane U I(x), |
∞ |
d x1 U I(x1) exp −i |
k |
2 |
2 |
. |
|||||||
– path length along the opti- |
× |
Ax1 |
− 2x1x2 + Dx2 |
(3.1.131) |
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2B |
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cal axis L. |
−∞ |
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Example 3.1.18. The waist of a Gaussian beam is given with U I(x1) = exp (−x21/w2I) in the input plane. The system consists of a thin lens with the focal length f followed by a free-space propagation by distance z. The ABCD-matrix is calculated from Fig. 3.1.34 and Table 3.1.11:
C D |
−1/f |
1 |
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A B |
= |
1 − z/f |
z . |
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∞ |
x2 |
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i |
− |
− |
k |
z |
1 |
2 |
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− |
− |
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λ z |
w2I |
2z |
f |
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U O(x2) = |
e−ikL |
d x1 exp |
1 |
exp i |
1 |
x2 |
2x1x2 + x2 . |
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−∞
Landolt-B¨ornstein
New Series VIII/1A1
Ref. p. 131] |
3.1 Linear optics |
127 |
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The result is an output Gaussian intensity distribution with the waist radius |
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w O = |
w I |
, |
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1 + |
w2 |
2 |
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π I |
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λ f |
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π w O w I |
2 |
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the waist position z = zwaist = f |
, and z O = |
π w2O/λ . |
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λ f |
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For inclusion of displacements and misalignments in Collins Integral see [96Tov]. |
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3.1.7.4.2 Three-dimensional propagation |
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In Table 3.1.23 the propagation in in general astigmatic systems is given. |
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Table 3.1.23. Propagation in general astigmatic systems. |
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Given |
Solution |
|||||||||||||||||||
– S : matrix of |
the optical sys- |
Field U O(r2) in the output plane (Collins integral ): |
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tem, see Table 3.1.15 and |
− |
i exp(−i kL) |
||||||||||||||||||
(3.1.99) with |
U O(r2) = |
d r1U I (r1) |
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λ |
√ |
det B |
||||||||||||||||||
A B |
k |
|||||||||||||||||||
S = C D |
, |
× exp −i |
r1 B−1 A r1 − 2 r1 B−1 r2 + r2 D B−1 r2 |
(3.1.132) |
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2 |
||||||||||||||||||||
– field distribution in the input |
with det B the determinant and B−1 the inverse of the matrix B . |
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plane: U I(r1) , where r1 is the |
Examples in [70Col, 05Gro2, 05Hod]. |
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position vector in the input |
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plane. |
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Classical cases of optical system design are given in [99Bor, 80Hof, 86Haf]. [82Wag, 95Gae] use the calculation of the field distribution in the image by a stop and wave aberrations in the exit pupil.
The analog is modeled for Gaussian beams on the exit pupil in the following references:
–focused Gaussian beams with aberrations and stops: see [69Cam, 71Sch],
–obscuration of a rotationally symmetrical Gaussian beam including longitudinal focal shift: see [82Car, 86Sta],
–extended systematic discussion of di raction with stops, obscuration, and aberrations: see [86Mah, 01Mah],
–spherical aberration: see [98Pu].
Landolt-B¨ornstein
New Series VIII/1A1
128 |
3.1.7 Beam propagation in optical systems |
[Ref. p. 131 |
The calculation of the excitation coe cient of an eigenmode in a waveguide (output mode) by the incident mode (input mode) at the surface of the waveguide is described in Table 3.1.24.
This task occurs
–if a laser beam is formed by an optical system and coupled afterwards into an optical fiber,
–if a laser beam of a master oscillator is to be coupled into a power amplifier,
–in the case of waveguide-waveguide coupling especially fiber-fiber coupling or coupling between semiconductor lasers.
Solutions are available in commercial optical design programs.
Table 3.1.24. Definitions for waveguide coupling.
Given |
Solution |
||||
– |
Incident beam (emitted by a laser |
Coupling coe cient (power relation): |
|||
(and) transformed by an optical system): |
O IO O IO |
||||
Einput (x, y) . |
η = |
. |
(3.1.133) |
||
– |
Waveguide with an eigenmode field the |
N I N O |
|||
coupling to which is asked: Eoutput (x, y) . |
Overlap integral : |
||||
Plane of mode |
O IO = |
∞ |
∞ |
(3.1.134) |
|||
x |
d x |
d y E I(x, y) E O(x, y) . |
|||||
matching |
|||||||
−∞ |
−∞ |
||||||
Einput ( x) |
Eoutput ( x) |
Normalization: |
|||||
z |
∞ |
∞ |
|||||
N I = |
d x |
d y E I(x, y) E I (x, y) . |
(3.1.135) |
||||
Waveguide |
−∞ |
−∞ |
|||||
Fig. 3.1.44. Mode matching. |
Normalization: |
||||||
Asked: Part of power transmitted into the waveguide (fiber, laser, integrated optical waveguide).
∞ |
∞ |
|
N O = |
d x d y E O(x, y) E O(x, y) . |
(3.1.136) |
−∞ |
−∞ |
E ective antireflection layers are assumed to be on the waveguide.
For the case that a Gaussian output waist of a source waveguide and a Gaussian input waist of a receiver waveguide are separated by air, the coupling of both waveguides is generally treated in [64Kog]. Higher-order modes are also included. The approximation of small misalignments (o set and tilt) is given in Table 3.1.25, large o sets and tilts are treated in [64Kog, 91Wu].
Landolt-B¨ornstein
New Series VIII/1A1