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PHYS 450 Spring semester 2017
Lecture 11: Fresnel’s Theory for the Diffraction of Scalar Waves
Ron Reifenberger Birck Nanotechnology Center Purdue University
Lecture 11 1
Historical Context 1803 – Thomas Young reignites interest in wave theory of light. Increased interest in Huygens’ ideas from late 1600’s 1818 - French Academy launches a competition to explain the properties of light – Fresnel, a civil engineer, submits his wave theory Every unobstructed point on a wavefront becomes the source of a secondary spherical wavelet. The amplitude of the E-field at any point on a screen is given by the superposition of all secondary wavelets, taking into account their relative phases – Poisson, while evaluating the submissions to the French Academy competition, finds an apparent critical flaw in Fresnel’s theory. Concludes that Fresnel predicts the seemingly absurd result that a bright spot should appear directly behind a circular obstruction! – Arago experimentally verifies Fresnel’s theory and finds the Arago spot (aka Poisson spot) 1819 – enthusiasm for corpuscular theory of light begins to diminish 1882 – Kirchoff introduces more mathematical theory based on solutions to Maxwell’s wave equation 1905 – Einstein's explanation of photoeffect revives interest in the corpuscular theory of light 2
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The Generic Diffraction Problem
Viewing Screen ? Pattern in blocking screen blocks fraction of ? Fraunhofer incident EM wave ? Limit – far field b
Fresnel Limit – Illumination near field a Blocking Screen or Obstacle
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After Systematic Experiments
intensity mirrors slit shape bright fringes immediately appear, just behind screen inside edge significant light broad pattern; penetration into complicated little resemblance shadow region profile to shape of original slit 4
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What we now understand
Viewing b>100A/ Screen Fraunhofer Limit
Fresnel Limit b Far Field b<100A/ b~100A/ (gray area) b
A=Aperture Area
A
Near Field
Pattern in blocking a monochromatic screen passes only a illumination, fraction of the incident
EM wave 5
Definition Diffraction is a deviation from geometrical optics resulting from the obstruction of an optical wavefront by an obstacle or opening. We want the intensity I at an arbitrary point P located on an observation screen a distance b from the obstacle. Two Important Cases Various Openings Edges Viewing Viewing Screen Screen
P +
P + Blocking Slits or Screen Apertures The intensity at point P can be expressed in terms of two standard integrals: vvuu22 SduCv sinv cos du 6 v0022v
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Fresnel’s Approach Simplest Case: What illumination will a diverging spherical wave produce at point P located a distance b ahead of wave? . L
b+3/2 s W 3 b+2/2 s2 b+/2 The E-field amplitude at P is the sum of all Monochromatic s1 the amplitudes of all light diverging b P the emitted wavelets from a point Vo s , s , … are arc lengths from the surface W. source 1 2
Fresnel’s approach: L’ divide wavefront into zones 7
Underlying Assumptions of Huygen-Fresnel Diffraction
2‐dimensional side view L What is E-field at observation point P at a W distance b from vertex Vo of wavefront? ds • Draw sphere of radius b Spherical V +2 etc. • Draw sphere of radius b + /2 Wavefront • Intersection of b + /2 sphere with wave- V+1 b front defines 1st Fresnel zone s b 2 • Assume ALL Huygen wavelets in 1st zone P arrive at point P in phase Vo b • E-field amplitude due to ALL wavelets in a st S 1 zone is A1. b • Continue to divide incident wavefront into Viewing zones by drawing additional spheres with Screen radii b + , b + 3/2, etc. • Assume wavelets from any given zone are approximately in phase when they arrive W L at point P and radians out of phase from contribution from adjacent zones.
Arc length (and angles) measured from point Vo • Each zone has nearly the same area can be either positive (CCW) or negative (CW). • Denote the E-field from each zone as A2, A , etc. 3 8
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Using Zones in the Huygen-Fresnel Theory of Diffraction – A Few Simple Examples
I. Light through a circular aperture II. Zones & Barriers
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EXAMPLE I: What is the E-field and Intensity at point P? Adding up the contributions from the various zones
o • A2 is 180 out of phase with A1, so it tends to cancel
• A2 is slightly smaller than A1 (area is essentially equal, but distance has increased) • The amplitude from the nth zone is to a good approximation the average value of that from the n-1 and n+1 zones
• Resultant E-field amplitude Anet(at P) given to good approximation by
A1 A3 AatPAAAAnet 1234..... A5 at point P A7 11 On average,,,etc A A A A A A 232213 24 . . . . ~0 ~0 11 1 1 1 Anet=A1/2 AatPAnet 1123 AA A AA 345 A ... A6 A4 22 2 2 2 A2 1 resultant AatPAnet 1 2 dominated by A1 A2 I at P A2 at P 1 unblocked net 4
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Insert Blocking Screen AatPAnet 1 I at P A22 at P A L blocked net 1
2 . I at P A b+3/2 blocked 1 4 2 s Iunblocked at P A1 W 3 b+2/2 4 s2
s 1 s1 b+/2 at point P b P Vo
Fresnel number: N = s 2/(b) = 1 Blocking screen allows F 1 light from only 1st Note bright spot in L’ zone to pass. center of pattern 11
EXAMPLE II: How the Zones Interact with Barriers (no obstruction)
L A . W . .
a b +s +φ P Vo a S -s
No Barrier
. . . W A L
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The Effect of a Knife Edge
L A W
a s φ P Vo S a b
W A L
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Intensity on Screen Above the Knife Edge
L A W
Integrate x I(y) over s a s Vo φ y
S a P
b
W A L
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Intensity on Screen Below the Knife Edge
L A W
Integrate a b over s φ s a P S -y Vo
x I(-y)
W A L
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Contribution from an Arbitrary Point Q on the Wavefront
=extra distance traveled L A
W The wavelet from Vo travels ds d distance b to P, Q ∆ The wavelet from an arbitrary b a s point Q travels a distance φ P d=b+Δ(s) S ab Vo before arriving at the same point P.
Need to know (s).
W L A
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Details: Generalizing the formalism
1. Define amplitude (E-field) contribution from each zone 2. Isolate terms with (s) - extra path length 3. Calculate (s) 1 ab s s2 2 ab 4. Change variables: convert s to a dimensionless parameter
2 ab vs ab 5. After considerable analytical analysis, the amplitude (E-field) contribution can be define in terms of C(v) and S(v) – Fresnel Integrals vvuu22 SduCv sinv cos du vv0022 6. From E-field amplitude, calculate time averaged irradiance at point P; additional factor of ½ 7. Introduce the Cornu Spiral: E(v) C(v) + iS(v) 8. Normalization to remove arbitrary constants 9. Relate v to y – problem specific
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The Fresnel Integrals 2. Using the phasor form for E(v ) vvuu22 SduCduvvsin cos v 2 N 1 u2 22ii u j vv00 Ev ee22 du u You can show that : v0 j0 222 E v C v i S v rectangular form uuoN u1 1 ii22 i 2 Then you can write euu e .... e u 2 2 vv22 ii u 4 u uu uu e2 u e2 .... vis contour Evcos dui sin du vv0022 3. Graphical representation: C(v ) length along v 2 i u Cornu spiral e 2 du phasor form v0 Imag 2
Intensity Ev v u E(v) . . . S(v ) What’s it mean? u 4 u2 1. Break the integral limits from 0 to v into N u 2 intervals u 2 Real
u u u 2 u ...... 4. Physical meaning u u u u u v o 1 2 3 4 E vCviSvCviSv v 22 uujujN j ,0,1,2...1 Cv Sv N 2 Intensity E v C22 v S v 18 uuuuuetco 0;12 ; 2 ; .
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The Cornu Spiral – an elegant graphical representation
v =+∞ Contributions from different +3 +1 zones S(v) +2 |E(v)| v v specifies the arc length along C(v) the Cornu spiral
-2 v =0
-1 -3 v =-∞
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Standard Geometry
Cylindrical wave encountering some arbitrary obstacle
Obstacle Viewing Plane Screen L A
y W x z slit Assume cylindrical wavefront: equivalent W to a line source L (turns a 2d problem A into 1d) a b
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Obtaining a coherent wave, diverging from a point, using a laser
objective viewing screen laser HeNe laser beam
Spatial Make sure you position filter pinhole, typically the central part of the 20 m diam. beam over the photodiode spatial filter assembly entrance slit (requires careful alignment)
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Laser stability is an issue
Laser Head No. 1373707 =633 nm 30 +10% shift 75 mins after turn on 25 +5% shift 45 mins after turn on 20 15 mins after turn on 15 Intensity (% max) (% Intensity 0 10203040506070 Time (s)
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Example I: No Obstacle
222 Ixyz,, A2 C C S S A is a constant to be determiend 2 22 2 11 11 A 22 22 2 AA221122 4 Rquire the inensity for the unblocked wave
to equal Io , the intensity of incident wave 2 Io 4A I A2 o 4
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Example II: The Knife Edge
L A W
Integrate I(y) over s x a s φ y Vo S a P
b
W A L
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Result II: Knife Edge
I 22 2 2 Ix0, z 0, y o C Cv S Sv C C S S 4 2222 Io 11 1111 Cv Cv 42 2 2 2 2 2 22 Io 11 Cv Sv 22 2 b yabv 2 a where Io is intensity of incident wave
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Use the scanning photodiode to collect data Scan photodiode . Use Data Studio software to collect data across pattern . Apply +3 V or -3 V to motor to scan Photodiode, photodiode across diffraction pattern. b entrance slit 1; . Need to measure scanning velocity. width ~0.1 mm . Position single slit (mask 1) in front of photodiode, width ~0.1 mm. Razor . Photodiode gain is typically set to 100, or a blade perhaps 10 if laser is bright.
HeNe laser w. spatial filter. How to measure a? Photo: Diffraction from knife edge in Fresnel configuration. Alignment is critical. 26
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Scanning photodiode - details motion
scanning photodiode with entrance slit No. 1 Center laser beam over slit
linear displacement dc linear translator (mm)
Calibration: apply dc voltage to linear translator linear translator slope=velocity
displacement time 27
Using the Cornu Spiral to Predict Location of Max and Mins
v =+∞ Typical results (a=0.2 m, b=0.1 m, =650 nm) Label various max (k=0.1.2.3…) and mins (j=0,1,2,3….) Diffraction near straight edge k=0 Expected +3 +1 1.50 d 1 2 … +2 a 1.25 1.00 0.75 c e b 1 2 … c 0.50 j=0 e 0.25 a b v =0 0.00
-2 Irradiance Normalized -1500 -1000 -500 0 500 1000 1500 -1 -3 v =-∞ y (m) d
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Fitting Data Positive y (above edge) Above the edge 22 D 2 1 11 I yCvSv time yy v = -0.6 d 2 2 2 y
typically10 vy 0
Below the edge 22 D '12 1 1 I yCvSvyy time d 2 22 Negative y
typically010 vy (geometrical shadow)
Scaling parameter b yabv y 2 a Cv Cv vy = +0.6 Sv Sv
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Origin of the max and mins in the diffraction pattern
1st minimum defines y=0
1st maximum
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Matching the max and mins in the diffraction pattern near an edge Typical results (a=0.2 m, b=0.1 m, =650 nm) Diffraction near straight edge 1.50 1.25
Converting dimensionless vy to y (in m) 1.00 0.75 22ab ab 0.50 -1.225 vsayy ab ab 0.25 -1.871 -2.345
1 Normalized Irradiance 0.00 tan yab yab -6.0 -4.0 -2.0 0.0 2.0 4.0 6.0 v (dimensionless) b y yabv y 2 a Diffraction near straight edge 3 1.50 vkkmax 40,1,2,3... . . . .k y 2 1.25 1.00 min 7 0.75 . . . .j vjjy 40,1,2,3... 2 0.50 0.25 0.00 NormalizedIrradiance -1500 -1000 -500 0 500 1000 1500 y (m) 31
Talbert/Leeman data November 2016
1.50 Data 1.25 Max Loc. Min. Loc. 1.00 Fresnel Theory Io 0.75
0.50 Relative Intensity Relative 0.25
0.00 -500 0 500 1000 1500 2000 2500 Photodiode Displacement (microns)
Scaled photodiode voltage by 16 to match b=0.3 m heights of maxima and minima “a” adjusted to optimize fit =543.5 nm Shift data by 870 m to make origin match velocity=134.8 m/s 0.25Io 32
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Centering spatially filtered laser beam =633 nm 25 off-center 20 good on center 15 better 10 Misalignment of peaks in data means velocity 5 in forward and backward directions 0 are different. Intensity (% max) (% Intensity 0 102030405060 Time (s)
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Example III: Long, narrow single slit, width w
L Top view, looking down A W
Integrate over s I(y) Vo x that passes +s through slit a y φ -s w S a P
b
W A L 34
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Result III: Single Slit, width w
I 22 2 2 Ix0, z 0, y o Cu Cv Su Sv C C S S 4 22 I 2211 11 o Cu Cv Su Sv 42222
Io 22 2Cu Cv Su Sv 4 I 22 o Cu Cv Su Sv 2 b 2 2111 w y v a b 2 1 b w a b 2 2111 w y u a bw2 1 b a
where Io is intensity of incident wave
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Excel Utility to Fit Data
Enter four numbers
Copy/Paste these two columns
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Use single slits on Cornell Slit Film
Use these two slits to investigate Fresnel diffraction. Must center laser beam over slit.
to calculate width of slits, see Appendix S in PHYS 450 Lab Manual 37
Results - diffraction through a wide and narrow slit vs. y
Slit width=1406 μm; a=b=0.4 m; λ=632.8 nm Slit width=703 μm; a=b=0.4 m; λ=632.8 nm 16 12 Data Data 12 Theory 9 Theory
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Intensity (a.u.) Intensity 3
Intensity (a.u.) 0 -2500.0 -1250.0 0.0 1250.0 2500.0 0 -2500.0 -1250.0 0.0 1250.0 2500.0 Displacement along Viewing Screen (μm) Displacement along Viewing Screen (μm)
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Graphical Interpretation (Situation drawn for y=0)
b 2 -y 2111 w y u a bw2 1 b a b 2 2111 w y v a bw2 1 b a +y b 2 211111 w y y vua bww2211bb aa b 2 2 1 w a constant b
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Example III: Fraunhofer diffraction through single slit
Fresnel Number