Title: Physics 214 Lecture 4
1Applications of Interference and Diffraction
2Overview
- Circular Diffraction (foreshadowing of quantum
uncertainty) - Angular resolution (Rayleighs criterion)
- Minimum spot size
- Interferometers
- Michelson
- Applications
- Crystal X-Ray Diffraction
3Diffraction-limited Optics
- Diffraction has important implications for
optical instruments - Lens-making is a craft. Even for a perfectly
designed lens, however, the image of a point
source will be a little blurry due to
diffraction in passing through the circular
aperture of the lens. -
The image of a point source through a circular
aperture is like a single-slit diffraction
pattern. But note the difference
4Transmission of light through slits and circular
apertures
Observation screen
Slit, width a
Observation screen
Pinhole, diameter D
Image Plane
Lens, diameter D
Laser with pinholes
Circular-aperture diffraction pattern the Airy
disk. Central lobe contains 84 of power.
5Exercise 1 Expansion of a Laser beam
- In 1985, a laser beam with a wavelength of l
500 nm was fired from the earth and reflected off
the space shuttle Discovery, in orbit at a
distance of L 350 km away from the laser. - If the (circular) aperture of the laser was D
4.7 cm, what was the beam diameter d at the space
shuttle?
6Exercise 1 Expansion of a Laser beam - Solution
- In 1985, a laser beam with a wavelength of l
500 nm was fired from the earth and reflected off
the space shuttle Discovery, in orbit at a
distance of L 350 km away from the laser. - If the (circular) aperture of the laser was D
4.7 cm, what was the beam diameter d at the space
shuttle?
84 of power is in central lobe.
7Act 1 Expansion of a Laser beam
- In 1985, a laser beam with a wavelength of l
500 nm was fired from the earth and reflected off
the space shuttle Discovery, in orbit at a
distance of L 350 km away from the laser. - To make a smaller spot on the shuttle, what
should we do to the beam diameter at the source? - a. reduce it
- b. increase it
- c. cannot be made smaller
8Act 1 Expansion of a Laser beam - Solution
- In 1985, a laser beam with a wavelength of l
500 nm was fired from the earth and reflected off
the space shuttle Discovery, in orbit at a
distance of L 350 km away from the laser. - To make a smaller spot on the shuttle, what
should we do to the beam diameter at the source? - a. reduce it
- b. increase it
- c. cannot be made smaller
Counter-intuitive as this is, it is correct you
reduce beam divergence by using a bigger beam.
(Note this will work until D d)
We will see soon that this can be understood as a
consequence of the uncertainty principle Dx
Dpxgt??
9Exercise 2 Focusing of a laser beam
- There are many times you would like to focus a
laser beam to as small a spot as possible.
However, diffraction limits this. - The (circular) aperture of a laser (l 780 nm)
has Dlaser 5 mm. What is the spot-size d of the
beam after passing through a (perfect) lens with
focal length f5mm, diameter Dlens 6 mm? (Hint
light passing through lens center is
undeflected.)
Dlens
d
Dlaser
f
10Exercise 2 Focusing of a laser beam - Solution
- There are many times you would like to focus a
laser beam to as small a spot as possible.
However, diffraction limits this. - The (circular) aperture of a laser (l 780 nm)
has Dlaser 5 mm. What is the spot-size d of the
beam after passing through a (perfect) lens with
focal length f5mm, diameter Dlens 6 mm? (Hint
light passing through lens center is
undeflected.)
Dlens
d
Dlaser
f
Light at this angle will intercept the focal
plane at d/2 f qo
11Act 2 Focusing of a laser beam
- There are many times you would like to focus a
laser beam to as small a spot as possible.
However, diffraction limits this. - Which of the following will reduce the spot
size? - a. increase l
- b. decrease l
- c. increase Dlens
- d. decrease Dlens
Dlens
d
Dlaser
f
12Act 2 Focusing of a laser beam - Solution
- There are many times you would like to focus a
laser beam to as small a spot as possible.
However, diffraction limits this. - Which of the following will reduce the spot
size? - a. increase l
- b. decrease l
- c. increase Dlens
- d. decrease Dlens
Dlens
d
Dlaser
f
13Angular Resolution
- Diffraction also limits our ability to resolve
(i.e., distinguish) two point sources. Consider
two point sources (e.g., stars) with angular
separation a viewed through a circular aperture
or lens of diameter D.
Rayleighs Criterion define the images to be
resolved if a ³ ac , where
At ac the central max of one image falls on the
first minimum of the second image
14Exercise 3 Angular resolution
- Car headlights in the distance
- What is the maximum distance L you can be from an
oncoming car at night, and still distinguish its
two headlights, which are separated by a distance
d 1.5 m? Assume that your pupils have a
diameter D 2 mm at night, and that the
wavelength of light is l 550 nm.
15Exercise 3 Solution
- Car headlights in the distance
- What is the maximum distance L you can be from an
oncoming car at night, and still distinguish its
two headlights, which are separated by a distance
d 1.5 m? Assume that your pupils have a
diameter D 2 mm at night, and that the
wavelength of light is l 550 nm.
Rayleighs Criterion
16Act 3 Resolving Stars
Halleys Comet
1. Assuming diffraction-limited optics (best
possible), what is the minimum angular separation
of two stars that can be resolved by a D 5 m
reflecting telescope using light of l 500
nm? a. 0.1 mrad b. 1 mrad c. 10 mrad
2. If the two points are not quite resolved
at screen 1, will they be resolved at screen 2?
17Act 3 Resolving Stars - Solution
Halleys Comet
1. Assuming diffraction-limited optics (best
possible), what is the minimum angular separation
of two stars that can be resolved by a D 5 m
reflecting telescope using light of l 500
nm? a. 0.1 mrad b. 1 mrad c. 10 mrad
The real limit of earth-bound telescopes is about
an order of magnitude larger due to atmospheric
effects (\ the Hubble).
2. If the two points are not quite resolved
at screen 1, will they be resolved at screen 2?
NO! Only the angle counts.
18Example Problem Camera resolution (Discussion
next week)
A modern-day digital camera basically looks
something like this
- If the distance between adjacent pixels is less
than the minimum resolvable separation due to
diffraction, then the image can look blurry.
- The f-number of a lens is defined as f/D. To
minimize diffraction, you want a small f-number,
i.e., a large aperture.
http//www.cambridgeincolour.com/tutorials/diffrac
tion-photography.htm
- This assumes a perfect lens. In practice,
lens aberrations limit the resolution if D is too
big.
19Optical Interferometers
- Interference arises when there are two (or more)
ways for something to happen, e.g., two slits for
the light to get from the source to the screen. - I 4I1 cos2(?/2), with ? 2p d/l, and
path-length difference d. - An interferometer is a device using mirrors and
beam splitters (half light is transmitted, half
is reflected) to give two separate paths from
source to detector. - Two common types
- Mach-Zehnder Michelson
-
beam- splitter
mirror
20Michelson Interferometer
- Michelson interferometer works by varying the
relative phase of the light waves for the two
paths light can take - One possibility is to vary the lengths L1 or L2
- Makes possible very accurate measurements of
displacements -
mirror
Total Path length L1
Path-length difference d L2 - L1
2I1
2I1
Total Path length L2
4I1
2I1
mirror
2I1
I1
I1
beam- splitter
I 4I1 cos2(?/2), with ? 2p d/l
21ACT 4
d
- Consider the following Michelson interferometer.
Assume that for the setup shown, all the light
(with l 500 nm) comes out the bottom port. - 1. How much does the top mirror need to be
moved so that none of the light comes out the
bottom port?
2. Where does the light then go? a. down b.
up c. left d. right
22ACT 4 - Solution
d
- Consider the following Michelson interferometer.
Assume that for the setup shown, all the light
(with l 500 nm) comes out the bottom port. - 1. How much does the top mirror need to be
moved so that none of the light comes out the
bottom port?
We need to go from complete constructive to
complete destructive interference ? ?f 180 ? ?
l/2 Howeverwhen we move the mirror by d, we
change ? by 2d. Therefore, d ?/2 l/4 500/4
125 nm.
2. Where does the light then go? a. down b.
up c. left d. right
23ACT 4 - Solution
d
- Consider the following Michelson interferometer.
Assume that for the setup shown, all the light
(with l 500 nm) comes out the bottom port. - 1. How much does the top mirror need to be
moved so that none of the light comes out the
bottom port?
2. Where does the light then go? a. down b.
up c. left d. right
The light goes out the way it came in. Energy
is conserved --the light cant just disappear!
(This is still true in quantum mechanics see
later)
The Michelson interferometer is perhaps most
famous for disproving the hypothesis that EM
waves propagate through an aether this result
helped stimulate the Special Theory of Relativity
24Michelson Interferometer
- Another possibility is to vary the phase by
changing the speed of the waves in the two arms - Recall vc/n where n index of refraction
- Using l v/f, f 2pL(1/l1 1/l2) (where L
L1 L2) - Makes possible very accurate measurement of
changes in the speed of light in the two arms
mirror
Total Path length L, l1 c/(n1f)
Vary index of refraction n in one arm
Phase difference ? 2p L (f/c) (n1 n2)
2I1
2I1
Total Path length L, l2 c/(n2f)
4I1
2I1
mirror
2I1
I1
I1
beam- splitter
I 4I1 cos2(?/2), with ? 2pL(f/c) (n1 n2)
25Michelson Interferometer, cont.
- Its actually the wavelength that changes.
- However, its often easier to think/calculate in
terms of the effective length of the arms L
Ln. - Then f (2p/l)(L1 L2 ), where l c/f is
the vacuum wavelength.
26FYI Application Optical Coherence Tomography
- One mirror of the Michelson is replaced by
human tissue. The type of tissue controls the
amount of reflection, and the phase shift.
- By sending in many colors, one can learn about
the density, composition, and structure of the
tissue. - Used for medical diagnostics like a
microscope, but you dont have to excise the
sample from the body! - Used to study
- skin cancer
- cardiovascular disease (detect bad plaques)
- glaucoma and macular degeneration (incurable eye
disease) -
27FYI Application Gravity Wave Detection
- Einstein predicted that when massive objects
accelerate, they produce time-dependent
gravitational fields gravity waves that
propagate as warpings of spacetime at the speed
of light. (EM radiation from accelerating e) - The effect is very tiny E.g., estimated DL/L of
10-21 for in-spiraling binary neutron stars.
How to detect this???
28FYI Application Gravity Wave Detection
LIGO Laser Interferometric Gravitational wave
Observatory -Worlds largest interferometers
4-km -2 in Hanford, WA 1 in Livingston, LO -
gt400 scientists -Projected sensitivity 3 x 10-23
? DL 10-19 m (10-9 Ang.) -Real searches now
underway!
29ACT 5
- Consider the following Sagnac sahn-yack
interferometer. Here the two possible paths are
the clockwise and counter-clockwise circuits
around the fiber loop.
fiber loop
1. If we insert an extra piece of glass as shown,
how does the relative path length change?
2. How could we change the relative path-length
difference, and thereby change how much light
exits the bottom port?
30ACT 5
- Consider the following Sagnac sahn-yack
interferometer. Here the two possible paths are
the clockwise and counter-clockwise circuits
around the fiber loop.
fiber loop
1. If we insert an extra piece of glass as shown,
how does the relative path length change?
It doesnt! Because the interference paths
completely overlap, the Sagnac is a remarkably
stable interferometer, e.g., to temperature
fluctuations in the fiber.
2. How could we change the relative path-length
difference, and thereby change how much light
exits the bottom port?
31ACT 5
- Consider the following Sagnac sahn-yack
interferometer. Here the two possible paths are
the clockwise and counter-clockwise circuits
around the fiber loop.
fiber loop
1. If we insert an extra piece of glass as shown,
how does the relative path length change?
It doesnt! Because the interference paths
completely overlap, the Sagnac is a remarkably
stable interferometer, e.g., to temperature
fluctuations in the fiber.
2. How could we change the relative path-length
difference, and thereby change how much light
exits the bottom port?
Rotate the entire interferometer (in the plane
of the paper). For example, if we rotate it
clockwise, the light making the clockwise circuit
will have farther to go (the beamsplitter is
running away), while the counterclockwise path
will be shortened. It is not difficult to show
that
Monitor output intensity ? determine f ? rate of
rotation w ? laser ring gyroscope!
32Crystal diffraction How do we know the atomic
scale structure of matter around us?
- A crystal is a very large number of atoms or
molecules arranged in a periodic fashion - Acts like a grating with an extremely large
number (Avagadros number) of units that
diffract waves coherently - Every crystal has its own signature of the
spacings between atoms that act like gratings - By measuring the diffraction, we can determine
the atomic scale structure
NaCl structure
- Figure from http//www.cmmp.ucl.ac.uk/kpm/people/
keith.htm
33Crystal Diffraction (2)
- Typical distances between atoms are of order
0.1-0.3 nm.What are characteristic wavelengths
needed to study crystals? - We need waves with wavelength l10-10m
- X-rays! e-m waves with much smaller wavelength
than visible light -- i.e., for x-rays l10-10m
34Historical Note X-ray Crystallography
The Braggs made so many discoveries that Lawrence
described the first few years as like looking
for gold and finding nuggets lying around
everywhere
- showed that the sodium and chloride ions were not
bonded into molecules, but arranged in a lattice
- could distinguish different cubic lattices
- discovered the crystal structure of diamond
- Lawrence Bragg was the youngest Laureate ever
(25) to receive a Nobel Prize (shared with his
father in 1915) - now standardly used for all kinds of materials
analysis, even biological samples! - The same multi-layer interference phenomenon is
now used to make highly wavelength-specific
mirrors for lasers - (distributed Bragg feedback DBF)
35X-ray scattering Modern Example
- X-rays remain the primary methods for
establishing the atomic scale structures of
complex molecules - Example of rabbit liver carboxylesterase (one
molecule showing atomic groups and attached
large scale structures with atoms not shown)
Alternative strategies to improve theantitumor
efficacy have concentrated upon the design of
novel camptothecin analogs. To effect this, we
have determined the x-ray crystal structures of
the rabbit liver carboxylesterase Source
St. Jude Children Research Hospitalhttp//www.stj
ude.org/faculty/0,2512,407_2030_4278,00.html
36FYI Diffraction from Crystals
The structure of the crystal can be found using
almost the same law we have for optical
gratings! Bragg Law for constructive
interference 2d sinq ml d lattice spacing,
l x-ray wavelength q x-ray angle (with
respect to plane of crystal)
Each crystal has many values of d - the distances
between different planes. For a known wavelength
l the observed angles q can be used to determine
the crystal structure
37FYI Diffraction from Crystals
Why is there a factor of 2? (The grating
law is d sinq ml) Bragg Law for constructive
interference 2d sinq ml It is the same
idea applied to different cases!
In Bragg scattering from a crystal q x-ray
angle (with respect to plane of crystal) - two
terms d sin q in the path length difference
In the grating the light was at normal incidence
only one term d sin q in the path length
difference
The change in direction of the light is q
The change in direction of the x-rays is 2q
38FYI Diffraction from Crystals
- How do we know the structures of DNA, proteins
and other biological molecules? X-ray Bragg
diffraction! - The molecules are crystallized to create a
crystal in which the molecules are arranged in a
periodic lattice. By using the sharp Bragg
diffraction from many molecules, the structure of
each molecule is determined - the positions of
thousands of atoms
39FYI Thin Films!
- Why do soap bubbles appear colored? Oil films on
water? - Interference -- light reflected from the front
and back surfaces interferes. - However, light that reflects off a higher-index
layer gets an extra p phase-shift (from
Maxwells equations). - For a film of thickness d, viewed at an angle q,
the path length difference is d 2dsinq and the
phase difference between the light reflected from
the front and back surfaces is f 2pd/l p.
Destructive interference 2dsinq
ml Constructive interference 2dsinq (m1/2)l