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VLE 3 Wave optics

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Newton rings

Newton rings are generated by interference at thin layers.

Lens

Plate

Multiple reflection occur at the boundaries of lens and plate. These beams interfere. The distance between lens ant plate generate a optical path difference between the partial beams.

→ Usage of lens characterisation

41

Prof. M. Schmidt

Institute of Photonic Technologies, Univ. Erlangen, Germany

Lens characterization with monochromatic light

Error free lens

Lens with errors

source: http://wwwex.physik.uni-ulm.de, 07.10.09

The distance between two rings is equal to the height difference (between plane glass plate surface and lens surface) of /2.

The ring diameter decreases with high distance to the lens centre because the gradient of the distance change is rising.

42

Prof. M. Schmidt

Institute of Photonic Technologies, Univ. Erlangen, Germany

Calculation of the Newton rings

Path of the light ray through air gap inclusive 180° Phase shift caused by reflection:

s 2d

2

Condition for destructive interference is that the optical path is an odd multiple of the half wavelength:

s

2k 1

 

 

 

 

 

2

 

 

 

 

 

 

 

 

 

 

 

 

Combine and cross out

2d k

For r²:

 

 

r 2

d 2R d

Because d << R: r 2

2dR

 

So:

 

 

d

 

r 2

 

 

 

 

2R

 

 

 

 

 

Lens

Glass plate

source: www.fkg-wuerzburg.de, 07.10.09

Position of the k-th dark stripe is seen from the centre:

rk k R

43

Prof. M. Schmidt

Institute of Photonic Technologies, Univ. Erlangen, Germany

Michelson interferometer (1)

Layout:

Moveable mirror

 

 

HeNe laser= 633 nm

Probe beam

Beam-

splitter Fixed reference mirror

Reference beam

Interfering beams

→ Application: high-precision measurement of displacements/ distances

44

Prof. M. Schmidt

Institute of Photonic Technologies, Univ. Erlangen, Germany

Michelson interferometer (2)

Initial state:

Reference beam

= 633 nm

→ Amplification

Probe beam

Displacement of the movable mirror by /4 → Increase of the optical path by /2

Reference beam

/2

→ Cancellation

Probe beam

→ Alternation between „bright“ and „dark“ with a mirror displacement of /4 (= 158 nm)

45

Prof. M. Schmidt

Institute of Photonic Technologies, Univ. Erlangen, Germany

Michelson Interferometer (3)

Error sources of the Michelson-Interferometer:

The wavelength of the laser is the central measuring tool

→ Unknown change of the wavelength causes errors

Influences of the wavelength by: laser stability, temperature, humidity,… → Measurement of the surrounding condition necessary

Mirrors are very sensitive for tilting (reflected beam sees the double tilting angle)

→ Alternative: Retro reflector

source: www.newport.com

46

Prof. M. Schmidt

Institute of Photonic Technologies, Univ. Erlangen, Germany

Michelson Interferometer (4)

Forward-backward-counting:

Tilting of the reference mirror

Measuring mirror

The interference fringes move to left or right in dependence of the tilting of the reference mirror. With the right detector setup the direction can be found:

Refrence mirror

Interference fringes

 

 

 

on detector:

 

 

Detector 2

 

Detector 1

 

 

 

 

 

 

 

 

 

47

Prof. M. Schmidt

Institute of Photonic Technologies, Univ. Erlangen, Germany

Further interferometer types (1)

Sagnac-Interferometer

source: Demtröder, Experimantalphysik 2

If the interferometer is resting I1 and I2 have the same optical path (s1 = s2). Is it rotating, the mirrors will move while the light is going around. Therefore the distance s1 for I1 is a little bit longer than the distance s2 for I2 .

The generated phase shift is proportional to the angular velocity .

The fringe shift N = t/ is

 

4 A

with A – area of the

N

square

c

 

 

Application:

Measurement of the rotation of the earth (Michelson-Gale-experiment 1925)

Laser-Gyroscope

48

Prof. M. Schmidt

Institute of Photonic Technologies, Univ. Erlangen, Germany

Further interferometer types (2)

Mach-Zehnder-Interferometer

By change of the refractive index and with this the optical path in on arm of the interferometer a phase shift is generated. The phase shiftcan be calculated with the following equation:

n L

With this the refractive index e.g. of gases can be calculated, or the change of the refractive index can be calculated with a precision of up to 10-8.

source: Demtröder, Experimantalphysik 2

49

Prof. M. Schmidt

Institute of Photonic Technologies, Univ. Erlangen, Germany

6. Fresnel-Huygens-Principle

50

Prof. M. Schmidt

Institute of Photonic Technologies, Univ. Erlangen, Germany