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Transcript
Experiment 3 – The Polarization of Light
1
Experiment 3
The Polarization
of Light
1 Introduction
In this experiment, we will study various polarizations of light. These
will include linearly polarized, circularly polarized, elliptically polarized and unpolarized light. The polarization of light will be described
quantitatively by the degree of polarization. We will also study the reflection of linearly polarized light from a plane surface. In these studies
we will use a photodetector and a computer to acquire the data.
2 Background - Pedrotti3, Secs. 4-8, 4-9 and 15-1 to
15-6
2.1
Types of Polarization
The electric field of a propagating transverse electromagnetic wave lies
in a plane normal to the direction of propagation. Consider a wave
propagating along ẑ. For most of this discussion, we shall consider a
wave at a particular instant in time and examine the orientation of the
electric field vector in our x − y coordinate system.
2.1.1
Polarized Light
A general expression for the E-field is:
E = x̂E0x cos(kz − ωt) + ŷE0y cos(kz − ωt + φ).
(1)
where φ is a phase shift between the x̂ and ŷ directions. If φ = 0, the
electric field oscillates along a line. This is linearly polarized light. The
angle of the polarization is determined by the relative magnitudes of
E0x and E0y . If φ = ±π/2, and E0x = E0y the electric field vector traces
Experiment 3 – The Polarization of Light
2
out a circle in the x − y plane. This describes circularly polarized light.
If φ 6= 0, ±π/2 and/or E0x 6= E0y , the light is elliptically polarized. The
electric field traces out an ellipse, that in general can have any major
to minor axis ratio and an arbitrary angle.
2.1.2 ”Unpolarized” Light
If light is monochromatic, it is polarized. It must be some form
of elliptically polarized light (where we consider linear and circular to
be limiting cases.) For light to be ”unpolarized” requires a random
phase variation between the x and y components of the field, and some
time averaging. All light is always fully polarized at any instant in
time. Unpolarized light is only possible if there are multiple frequencies
present. Our HeNe lasers may or may not be fully polarized. They tend
to lase in a few ”modes” with orthogonal polarizations, producing light
separated in frequency by ∼ 1 GHz (note this is only a part in 105 of the
optical frequency, so it still looks monochromatic). We will learn more
about lasers later in the course, but at the moment, what you need to
know is that over time (minutes to hours) the amount of light in the
two modes can drift. If it is all in one mode, the laser will be linearly
polarized. If it lases in both modes with equal intensity, it will appear
unpolarized (because any measurement we make will average over many
cycles of the difference frequency). This drift will be an impediment to
your measurements, and some of you will be fortunate and will have
much more stable lasers than others. To do experiments we will put
one polarizer in front of the laser to make it linearly polarized, but
how much light is transmitted through this polarizer will depend on
the state of the laser and may change in time!
2.2
Malus’s Law
Consider polarized light of intensity I(0) incident on an ideal linear
polarizer. Let the transmission axis of this polarizer be at an angle of θ
with respect to the initial polarization. Only light with it’s electric field
vector parallel to the axis of the polarizer will be transmitted through
the polarizer.
The intensity of the light emerging from the second polarizer is given
by Malus’ Law:
I(θ) = I(0) cos2 (θ).
(2)
To go one step further, consider the situation where light from the first
polarizer is incident on a second polarizer whose transmission axis is at
an angle of ψ with respect to the initial polarization. The intensity of
light emerging from the second polarizer is given by
I(ψ) = I(0) cos2 (θ) cos2 (θ − ψ).
(3)
Experiment 3 – The Polarization of Light
2.3
3
Degree of Polarization
The degree of polarization is basically a measure of the extent to which
the light we are studying is polarized and is given by:
V =
Imax − Imin
,
Imax + Imin
(4)
where Imin and Imax are the minimum and maximum intensities of the
light, respectively. For partially polarized light, this can also be written
as:
Ip
V =
,
(5)
Ip + Iup
where Ip is the intensity of the polarized portion and Iup is the intensity
of the unpolarized portion. Sometimes V is called the fringe visibility.
2.4
Reflection of Linearly Polarized Light
When linearly polarized light is incident on a plane surface, the amount
of light reflected, the reflectance (R), depends on the angle of incidence
and the orientation of the polarization vector relative to the scattering
plane. Note, the scattering plane is the plane containing all the ~kvectors, those for the incident, reflected and refracted waves. This is
described by the Fresnel equations:
tan (θi − θt ) 2
(6)
Rk = tan (θi + θt ) sin (θi − θt ) 2
.
(7)
R⊥ = sin (θi + θt ) One consequence of Eq. 6 is that when θi + θt = π/2, tan (θi + θt ) →
∞ and Rk → 0. This occurs when θi = θB where θB is called Brewster’s
angle and θt = β. Substituting θB and β into Eq. 6, subject to θB +β =
π/2 leads to
nt
tan θB = .
(8)
n0
At θB only light with its E-field perpendicular to the scattering plane
will be reflected. Consequently, it is possible to produce polarized light
from unpolarized light by allowing it strike an interface at Brewster’s
angle.
2.5
Birefringence and Optical Activity
Lenses and windows are often made of materials that are isotropic –
the index of refraction is independent of the direction the electric field
points, the direction of propagation or whether the light is linearly or
Experiment 3 – The Polarization of Light
4
elliptically polarized. There is a class of materials, crystals, that are
birefringent; as the name implies there two indices of refraction, depending on direction of propagation and the direction the electric field
points. The two indices are call the ordinary index (no ) and the extraordinary index (ne ). These two indices are the same for light propagating
in one particular direction. This direction identifies what is called optic
axis. What distinguishes no from ne is that no is independent of the
propagation direction. This is the case for light polarized in a direction perpendicular to the optic axis. On the other hand, ne varies as
the propagation direction varies away from the optic axis. For positive (negative) uniaxial crystals ne obtains its maximum (minimum)
value for light polarized in a direction perpendicular (parallel) to the
optic axis. Biaxial crystals are more complicated, having two optic
axes. Again, light polarized in a direction perpendicular to the plane
containing the optical axes specifies no .
The phase velocity of a wave, which depends on the index of refraction, is different for the ordinary and extraordinary waves. Thus,
birefringent materials make good wave plates and polarizers because
they can delay one orthogonal phase relative to the other and cause
two orthogonal polarizations to refract through different angles.
An optically active material is one that has two different indices of
refraction that depend on the helicity (right-hand or left-hand circular
polarization) of the wave. These materials can be exploited to rotate the
plane of polarization of a wave because they delay one helicity relative
to the other. Assuming no loss, or identical loss for both helicities, a
linearly polarized beam entering the medium will be linearly polarized
when it leaves, but with its plane of polarization rotated.
3 Experiment
You are supplied with 3 polarizers, one on a motorized rotation stage.
You will have to deal with the laser drifts, so you will need to make
stability measurements to disentangle effects due to the laser from your
measurements. Using the data acquisition system, measure the intensity stability of your laser, and then the time-dependent polarization
state of your laser.
Measure Brewster’s angle for the block of glass supplied. The polarizers’ axes are not marked, so you will need to figure out how to assure
that the polarization of the beam striking the block is parallel to the
plane of incidence.
Verify Malus’ Law for one and two polarizers. A demonstration that
mystifies many observers is that placing a polarizer in between two
crossed polarizers allows light to be transmitted that was previously
Experiment 3 – The Polarization of Light
5
blocked. Set up this system and figure out why this is so.
Go in the hallway and look at the light reflected off the floor. Is it
polarized, and if so, along what direction?
If you have or can borrow polarizing sunglasses, measure their polarization properties.
Multiple scattering of light can affect the polarization state. Waxed
paper makes a good multiple scatterer. Measure the polarization of the
light after passing through a piece of waxed paper.
Sugar molecules are chiral – they have a left-handed twist – so a
sugar solution is optically active. Measure the effect of transmitting
linearly polarized light through a cell containing corn syrup. Describe
the state of polarization after the beam has passed through the cell
twice. Use a mirror to retro-reflect the first pass back through the cell.
You will have to think about how to separate the input beam from
the retro-reblected beam so you can measure its state of polarization.
Explain why you see what you saw. Be careful not to drop the cell
or put your finger prints on the windows.
Play around with a 1/4-wave plate. Assuming the input beam is
linearly polarized, describe the state of polarization of the transmitted beam as you rotate the wave plate. What happens to the state of
polarization when a circularly polarized beam passes through the corn
syrup? Describe the state of polarization when you retro-reflect a circularly polarized beam back through the wave plate; compare the state
of polarization to that of the original input beam. Repeat the retroreflection experiment when the transmitted beam is linearly polarized.
Explain why you see what you saw.