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Diffraction Gratings

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Diffraction Gratings & Lenses. Laser beam diffraction. A lens transforms a Fresnel ... The far-field light field is the Fourier Transform of the apertured field! ... – PowerPoint PPT presentation

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Title: Diffraction Gratings


1
Diffraction Gratings Lenses
  • Laser beam diffraction
  • A lens transforms a Fresnel diffraction
    problem to a Fraunhofer diffraction problem
  • The lens as a Fourier Transformer
  • Babinets Principle
  • Diffraction Gratings
  • Examples of Fraunhofer diffraction
  • Randomly placed identical holes X-ray
    crystallography Laser speckle Particle
    counting

2
Recall the Fraunhofer Diffraction formula
The far-field light field is the Fourier
Transform of the apertured field!
E(x,y) const if a plane wave
Aperture function
where weve dropped the subscripts, 0 and 1,
and
kx kx1/z and ky ky1/z
The ks are off-axis k-vectors.
3
Fraunhofer diffraction of a laser beam
A laser beam typically has a Gaussian radial
profile No aperture is involved.
2w1
2w0
z
What will its electric field be far away?
The Fourier transform of a Gaussian is a Gaussian.
In terms of x1 and y1
or
where
4
Angular divergence of a laser beam
The beam diverges. What will its divergence angle
be?
w1
q
2w0
z
Recall that
The half-angle will be
The divergence half-angle will be
5
Gaussian Beams
  • The Gaussian beam is the solution to the wave
    equation, or equivalently, the Fresnel integral,
    for a wave in free space with a Gaussian profile
    at z 0.

The beam has a waist at z 0, where the spot
size is w0. It then expands to w w(z) with
distance z away from the laser. The beam radius
of curvature, R(z), also increases with distance
far away.
6
Gaussian Beam Math
  • The expression for a real laser
  • beam's electric field is given by
  • w(z) is the spot size vs. distance from the
    waist,
  • R(z) is the beam radius of curvature, and
  • y(z) is a phase shift.
  • This equation is the solution to the wave
    equation when we require that the beam be well
    localized at some point (i.e., its waist).

Recall the phase factor in front of the
diffraction integrals.
7
Gaussian Beam Spot, Radius, and Phase
  • The expressions for the spot size, radius of
    curvature, and phase shift

where zR is the Rayleigh Range (the distance over
which the beam remains about the same diameter),
and it's given by
8
Gaussian Beam Collimation
  • Twice the Rayleigh range is the
  • distance over which the beam
  • remains about the same size,
  • that is, remains "collimated.
  • _____________________________________________
  • .225 cm 0.003 km 0.045 km
  • 2.25 cm 0.3 km 5 km
  • 22.5 cm 30 km 500 km
  • _____________________________________________
  • Tightly focused laser beams expand quickly.
  • Weakly focused beams expand less quickly, but
    still expand.
  • As a result, it's very difficult to shoot down a
    missile with a laser.

Collimation
Collimation Waist spot Distance
Distance size w0 l 10.6 µm
l 0.633 µm
Longer wavelengths expand faster than shorter
ones.
9
The Guoy Phase Shift
  • The phase factor yields a phase shift relative to
    the phase of a
  • plane wave when a Gaussian beam goes through a
    focus.

Phase relative to a plane wave
Recall the i in front of the Fresnel integral,
which is a result of the Guoy phase shift.
10
Laser Spatial Modes
Some particularly pretty laser modes
  • Laser beams can have any pattern, not just a
    Gaussian. And the phase shift will depend on the
    pattern. The beam shape can even change with
    distance.
  • Some beam shapes do not change with distance.
    These laser beam shapes are referred to as
    Transverse Electro-Magnetic (TEM) modes. The
    actual field can be written as an infinite series
    of them.

11
Laser Spatial Modes
  • Some Transverse Electro-Magnetic (TEM) modes

Irradiance
The 00 mode is the Gaussian beam. Higher-order
modes involve multiplication of a Gaussian by a
Hermite polynomial.
Electric field
12
Diffraction involving a lens
  • A lens has unity transmission, but it introduces
    a phase delay proportional to its thickness at a
    given point (x,y)
  • where L(x,y) is the thickness at (x,y). Compute
    L(x,y)

d
neglecting constant phase delays.
13
A lens brings the far field in to its focal
length.
  • A lens phase delay due to its thickness at the
    point (x0,y0)

If we substitute this result into the Fresnel
(not the Fraunhofer!) integral
The quadratic terms inside the exponential will
cancel provided that
Recalling the Lens-makers formula, z is the lens
focal length! For a lens that's curved on both
faces,
14
A lens brings the far field in to its focal
length.
This yields
  • If we look in a plane one focal length behind a
    lens, we are in the Fraunhofer regime, even if it
    isnt far away! So we see the Fourier Transform
    of any object immediately in front of the lens!

E(x,y)
F t(x,y) E(x,y)
t(x,y)
A lens in this configuration is said to be a
Fourier-transforming lens.
15
Focusing a laser beam
Lens
A laser beam typically has a Gaussian radial
profile
2w1
f
What will its electric field be one focal length
after a lens?
or
Look familiar? This is the same result for a beam
diffracting!
where
or
16
Babinets Principle
The diffraction pattern of a hole is the same as
that of its opposite!
Holes
Neglecting the center point
Anti-Holes
17
The Diffraction Grating
  • A diffraction grating is a slab
  • with a periodic modulation
  • of any sort on one of its surfaces.
  • The modulation can be in
  • transmission, reflection, or
  • the phase delay of a beam.
  • The grating is then said to be
  • a transmission grating,
  • reflection grating, or
  • phase grating, respectively.
  • Diffraction gratings diffract
  • different wavelengths into
  • different directions, thus
  • allowing us to measure spectra.

18
Diffraction Grating Mathematics
  • Begin with a sinusoidal modulation of the
    transmission
  • where a is the grating spacing. The Fraunhofer
    diffracted field is

We need the A0 term because A(x,y) cant be
negative.
Ignoring the y0-integration, the x0-integral is
just the Fourier transform
19
Diffraction orders
Because x1 depends on l, different wavelengths
are separated in the 1 (and -1) orders.
x1
No wavelength dependence in zero order.
z
The longer the wavelength, the larger its
diffraction angle in nonzero orders.
20
Diffraction Grating Math Higher Orders
  • What if the periodic modulation of the
    transmission is not sinusoidal?
  • Since it's periodic, we can use a Fourier Series
    for it

Keeping up to third order, the resulting Fourier
Transform is
A square modulation is common. It has many
orders.
21
The Grating Equation
  • An order of a diffraction grating occurs if
  • where m is an integer.
  • This equation assumed normal incidence and a
    small diffraction angle, however. We can derive
    a more general result, the grating equation, if
    we use a tilted beam, E(x,y), or if we recall
    scattering ideas

Remember that the diffracted angle can be
negative, too.
22
Diffraction-grating spectrometer resolution
How accurate is a diffraction-grating
spectrometer (a grating followed by a
lens)? Recall the grating dispersion
Two similar colors illuminate the grating.
2w1
Two nearby wavelengths will be separated by
d
d cos(qm)
f
Setting this distance equal to the focused-spot
diameter
where N grating lines illuminated d / a
or
23
Diffraction-grating spectrometer resolution
Lets plug in some numbers
l 600 nm m 1 N
(50 mm) x (2400 lines/mm) 120,000 lines
2 grating with 2400 lines/mm
For simple order-of-magnitude estimates, 4 / p
1
And the resolution depends only on the
wavelength, order, and how many lines are
illuminated!
Resolution
24
Blazed Diffraction Grating
  • By tilting the facets of the grating so the
    desired diffraction ordercoincides with the
    specular reflection from the facets, the
    gratingefficiency can be increased.

Efficient diffraction
Specular means angle of incidence equals angle of
reflection.
Input beam
Inefficient diffraction
Even though both diffracted beams satisfy the
grating equation, one is vastly more intense than
the other.
25
Fraunhofer Diffraction interesting example
  • Randomly placed identical holes yield a
    diffraction pattern whose gross features reveal
    the shape of the holes.

Hole Diffraction pattern pattern
Square holes
Round holes
26
The Fourier Transform of a randomarray of
identical tiny objects
  • Define a random array of two-dimensional
    delta-functions
  • If Hole(x,y) is the shape of an individual tiny
    hole, then a random array of identically shaped
    tiny holes is
  • The Fourier Transform of a random array of
    identically shaped tiny holes is then

Shift Theorem
Sum of rapidly varying sinusoids (looks like
noise)
Rapidly Slowly varying varying
27
X-ray Crystallography
The tendency of diffraction to expand the
smallest structure into the largest pattern is
the key to the technique of x-ray
crystallography, in which x-rays diffract off the
nuclei of crystals, and the diffraction pattern
reveals the crystal molecular structure.
28
Laser speckle is a diffraction pattern.
When a laser illuminates a rough surface, it
yields a speckle pattern. It is a diffraction
pattern from the very complex surface. Dont
try to do this Fourier Transform at home.
29
Particle detection and measurement by diffraction
30
Moon coronas are due to diffraction.
When the moon looks a bit hazy, youre seeing a
corona. Its a diffraction effect.
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