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Physics 42200 Waves & Oscillations Spring 2013 Semester Matthew Jones Lecture 40 – Diffraction

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Page 1: Physics 42200 Waves & Oscillations...Spring 2013 Semester Matthew Jones Lecture 40 –Diffraction. FraunhoferDiffraction Fraunhoferdiffraction: • The phase varies linearly across

Physics 42200

Waves & Oscillations

Spring 2013 SemesterMatthew Jones

Lecture 40 – Diffraction

Page 2: Physics 42200 Waves & Oscillations...Spring 2013 Semester Matthew Jones Lecture 40 –Diffraction. FraunhoferDiffraction Fraunhoferdiffraction: • The phase varies linearly across

Fraunhofer Diffraction

Fraunhofer diffraction:

• The phase varies linearly

across the aperture

• The intensity of light

arriving from each part

of the aperture is equal�� �

�� = ℇ��� �� ����

Page 3: Physics 42200 Waves & Oscillations...Spring 2013 Semester Matthew Jones Lecture 40 –Diffraction. FraunhoferDiffraction Fraunhoferdiffraction: • The phase varies linearly across

Fraunhofer Diffraction

Fraunhofer diffraction:

• The phase varies linearly

across the aperture

• The intensity of light

arriving from each part

of the aperture is equal�

�� = ℇ��� ( �� �� �� ��)��

Page 4: Physics 42200 Waves & Oscillations...Spring 2013 Semester Matthew Jones Lecture 40 –Diffraction. FraunhoferDiffraction Fraunhoferdiffraction: • The phase varies linearly across

Huygens-Fresnel Principle

• Each point on a wavefront is a source of spherical

waves that are in phase with the incident wave.

• The light at any point in the direction of propagation is

the sum of all such spherical waves, taking into

account their relative phases and path lengths.

• The secondary spherical waves are preferentially

emitted in the forward direction.

Page 5: Physics 42200 Waves & Oscillations...Spring 2013 Semester Matthew Jones Lecture 40 –Diffraction. FraunhoferDiffraction Fraunhoferdiffraction: • The phase varies linearly across

Huygens-Fresnel Principle

Huygens: source of spherical wave

Problem: it must also go backwards,

but that is not observed in experiment

Solution: Kirchhoff’s scalar diffraction theory

( ) ( )θθ cos12

1 +=K

inclination factor

Intensity of the spherical wavelet

depends on direction:

( ) ( )ξωθ +−= krtr

EKE cos

θ

Page 6: Physics 42200 Waves & Oscillations...Spring 2013 Semester Matthew Jones Lecture 40 –Diffraction. FraunhoferDiffraction Fraunhoferdiffraction: • The phase varies linearly across

Propagation of Spherical Waves

• Consider a spherical wave emitted from a source � at

time � = 0.

�(�, �′) = ℇ�� cos( �! − #�)�

• These spherical waves

expand outward from ��

Page 7: Physics 42200 Waves & Oscillations...Spring 2013 Semester Matthew Jones Lecture 40 –Diffraction. FraunhoferDiffraction Fraunhoferdiffraction: • The phase varies linearly across

Propagation of Spherical Waves

• Consider a series of concentric spheres around

another point $ with radii %�, %� + '/2, %� + ',⋯�

� $%�

Page 8: Physics 42200 Waves & Oscillations...Spring 2013 Semester Matthew Jones Lecture 40 –Diffraction. FraunhoferDiffraction Fraunhoferdiffraction: • The phase varies linearly across

Propagation of Spherical Waves

• Consider a series of concentric spheres around

another point $ with radii %�, %� + '/2, %� + ',⋯�

� $Zone +,Zone +-Zone +.

Page 9: Physics 42200 Waves & Oscillations...Spring 2013 Semester Matthew Jones Lecture 40 –Diffraction. FraunhoferDiffraction Fraunhoferdiffraction: • The phase varies linearly across

Fresnel Zones

• Source strength per unit area in any zone is

ℇ/ ∝ ℇ��• Curvature of the surface in each zone is small

�(�, �′) = ℇ�� cos( �! − #�)

Page 10: Physics 42200 Waves & Oscillations...Spring 2013 Semester Matthew Jones Lecture 40 –Diffraction. FraunhoferDiffraction Fraunhoferdiffraction: • The phase varies linearly across

Fresnel Zones

Electric field at point $ due to secondary

waves in zone ℓ:

�� = 2ℓ(�) ℇ/% cos � − # � + % ��

Page 11: Physics 42200 Waves & Oscillations...Spring 2013 Semester Matthew Jones Lecture 40 –Diffraction. FraunhoferDiffraction Fraunhoferdiffraction: • The phase varies linearly across

3

Fresnel Zones

• How can we describe the element of area ��?

Law of cosines: %- = �- + %� + � - − 2� %� + � cos32%�% = 2�(%� + �) sin3 �3

� sin3 �3 = %�%%� + �

�3�

� sin3

�� = (26� sin3)��3

� $

%

%� + �

Page 12: Physics 42200 Waves & Oscillations...Spring 2013 Semester Matthew Jones Lecture 40 –Diffraction. FraunhoferDiffraction Fraunhoferdiffraction: • The phase varies linearly across

Fresnel Zones

Electric field at point $ due to secondary

waves in zone ℓ:

�� = 2ℓ(�) ℇ/% cos � − # � + % ��

�� = 26 �%� + � %�%

Page 13: Physics 42200 Waves & Oscillations...Spring 2013 Semester Matthew Jones Lecture 40 –Diffraction. FraunhoferDiffraction Fraunhoferdiffraction: • The phase varies linearly across

Fresnel Zones

• Total electric field due to wavelets emitted in zone ℓ:

�ℓ = 262ℓ � ℇ/�� + %�7 cos � − # � + % �%

8ℓ8ℓ9:

= −26# 2ℓ �ℇ/�� + %� sin � − # � + % 8ℓ9:

8ℓ

• But %ℓ = %� + ℓ' 2⁄ and %ℓ�, = %� + (ℓ − 1)'/2 and

#ℓ' 2⁄ = ℓ6, so

�ℓ = −1 ℓ=,2ℓ � ℇ/�'� + %� sin � − # � + %�

• Even ℓ: �ℓ < 0, odd ℓ: �ℓ > 0

Page 14: Physics 42200 Waves & Oscillations...Spring 2013 Semester Matthew Jones Lecture 40 –Diffraction. FraunhoferDiffraction Fraunhoferdiffraction: • The phase varies linearly across

Fresnel Zones

• The total electric field at point $ is the sum of all

electric fields from each zone:

� = �, + �- + �. +⋯+ �A= �, − �- + �. − �B +⋯± |�A|• Most of the adjacent zones cancel:

� = �,2 + �,

2 − �- + �.2 +⋯± �A

2• Two possibilities:

� ≈ F:- + FG

- or � ≈ F:- − FG

-• Fresnel conjectured that �A → 0 so � ≈ |�,|/2

Page 15: Physics 42200 Waves & Oscillations...Spring 2013 Semester Matthew Jones Lecture 40 –Diffraction. FraunhoferDiffraction Fraunhoferdiffraction: • The phase varies linearly across

Circular Aperture: Fresnel Diffraction

• Suppose a circular aperture

uncovers only the first Izones.

• If I is even, then the first

two zones interfere

destructively: � = 0• If I is odd, then all but the

first one cancel each other:

� = |�,|• What about points off the

central axis?

Page 16: Physics 42200 Waves & Oscillations...Spring 2013 Semester Matthew Jones Lecture 40 –Diffraction. FraunhoferDiffraction Fraunhoferdiffraction: • The phase varies linearly across

� $

• A point on the central axis:

Circular Aperture: Fresnel Diffraction

Page 17: Physics 42200 Waves & Oscillations...Spring 2013 Semester Matthew Jones Lecture 40 –Diffraction. FraunhoferDiffraction Fraunhoferdiffraction: • The phase varies linearly across

• A point that is not on the central axis:

Circular Aperture: Fresnel Diffraction

Page 18: Physics 42200 Waves & Oscillations...Spring 2013 Semester Matthew Jones Lecture 40 –Diffraction. FraunhoferDiffraction Fraunhoferdiffraction: • The phase varies linearly across

Circular Aperture: Fresnel Diffraction

• There will also be light and dark fringes off the

central axis

Page 19: Physics 42200 Waves & Oscillations...Spring 2013 Semester Matthew Jones Lecture 40 –Diffraction. FraunhoferDiffraction Fraunhoferdiffraction: • The phase varies linearly across

Circular Aperture: Fresnel Diffraction

Page 20: Physics 42200 Waves & Oscillations...Spring 2013 Semester Matthew Jones Lecture 40 –Diffraction. FraunhoferDiffraction Fraunhoferdiffraction: • The phase varies linearly across

Circular Obstacle: Fresnel Diffraction

• A circular obstacle will remove the middle zones, but

the remaining zones can interfere constructively and

destructively

� = �ℓ=, − �ℓ=- + �ℓ=. …± �A• As in the case of the unobstructed wave, only the

first unobstructed zone contributes:

� ≈ �ℓ=,2

• There should be a bright spot on the central axis

Page 21: Physics 42200 Waves & Oscillations...Spring 2013 Semester Matthew Jones Lecture 40 –Diffraction. FraunhoferDiffraction Fraunhoferdiffraction: • The phase varies linearly across

Poisson Bright Spot

• Poisson thought this result seemed absurd and

dismissed Fresnel’s paper

• Arago checked and found the bright spot:

Diffraction around a 1/8” ball bearing

Page 22: Physics 42200 Waves & Oscillations...Spring 2013 Semester Matthew Jones Lecture 40 –Diffraction. FraunhoferDiffraction Fraunhoferdiffraction: • The phase varies linearly across

Diffraction from an Edge

• The edge does not form a distinct shadow

Page 23: Physics 42200 Waves & Oscillations...Spring 2013 Semester Matthew Jones Lecture 40 –Diffraction. FraunhoferDiffraction Fraunhoferdiffraction: • The phase varies linearly across

Diffraction from an Edge

Page 24: Physics 42200 Waves & Oscillations...Spring 2013 Semester Matthew Jones Lecture 40 –Diffraction. FraunhoferDiffraction Fraunhoferdiffraction: • The phase varies linearly across

Fresnel Zone Plate

• Suppose we obscure only the even-numbered zones

� = �, + �- + �K +⋯+ �A• The electric field at the origin is 2I times that of the

unobstructed light

• What radii do we need to make some annular rings

that block only the even-numbered zones?

Page 25: Physics 42200 Waves & Oscillations...Spring 2013 Semester Matthew Jones Lecture 40 –Diffraction. FraunhoferDiffraction Fraunhoferdiffraction: • The phase varies linearly across

Fresnel Zone Plate

�A + %A − �� − %� = I'2�A = ��- + LA- ≈ �� + LA

-2��

%A = %�- + LA- ≈ %� + LA-2%�1

�� +1%� ≈

I'LA- =

1M

LA�� %�

�A %A

This looks like the

lens equation…

Page 26: Physics 42200 Waves & Oscillations...Spring 2013 Semester Matthew Jones Lecture 40 –Diffraction. FraunhoferDiffraction Fraunhoferdiffraction: • The phase varies linearly across

Fresnel Zone Plates

• There are also higher-order focal points:

MA = ,A M,

• Not an ideal lens– Works only for one wavelength (large chromatic aberration)

• But applicable to a wide range of wavelengths– Does not rely on weird atomic properties of transparent

materials

Page 27: Physics 42200 Waves & Oscillations...Spring 2013 Semester Matthew Jones Lecture 40 –Diffraction. FraunhoferDiffraction Fraunhoferdiffraction: • The phase varies linearly across

Fresnel Zone Plate

LA ≈ IM'• For green light, ' = 500OI• Suppose �� = %� = 10PI

– Then L, = 0.223II,L-= 0.316II,

etc…

• But this also works for x-rays:

'~0.1OI– Then L, = 3.16UI, L- = 4.47UI

• Challenges: very small spacing, but

needs to be thick enough to absorb

x-rays.