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  • So, in the last video, I introduced my staircase plan for explaining spinors, which starts with the simplest explanations at the bottom and ends with the most complicated explanations at the top.

  • We're going to start at the bottom of the staircase, which is basic examples of spinors in physics.

  • In the next four or five videos, I'm going to talk about two examples of how spinors come up in physics, the polarization of light waves and quantum spin states.

  • We're going to find that both of these phenomena can be described by spinors, in the form of two-by-one columns with complex number entries.

  • Afterward, we'll see how we can visualize these spinors as flagpoles on a sphere, called the Poincaré sphere or Bloch sphere.

  • In this video, we're going to discuss all the different polarizations of light waves and their corresponding spinors, which are called Jones vectors in this specific case.

  • And in the next video, we will discuss how to rotate between these polarizations using SU2 matrices.

  • So I'm hoping you're familiar with electric and magnetic fields.

  • The electric field is a set of vectors everywhere in space that point in the direction that a positive charge will be pulled in due to electric forces.

  • The magnetic field is another set of vectors everywhere in space that tell us which direction a compass will point due to magnetic forces.

  • According to the laws of electricity and magnetism, it's possible for electric and magnetic field vectors to vibrate back and forth together in a wave, called an electromagnetic wave.

  • The light we see is an example of electromagnetic waves.

  • Usually, electromagnetic waves are traveling waves, meaning they travel through space over time.

  • The image you're seeing here is a snapshot of an electromagnetic wave at a single instant in time.

  • But as time passes by, the wave will travel forward.

  • Electromagnetic waves are transverse waves.

  • This means the direction of the wave oscillations is always perpendicular to the direction of travel.

  • So if an electromagnetic wave is traveling in the z direction, the wave can oscillate in the x-y plane perpendicular to the direction of travel, but the wave cannot oscillate in the z direction, parallel to the direction of travel.

  • The polarization of a given electromagnetic wave is the geometric orientation of the wave.

  • We only use the electric field E to define the polarization of an electromagnetic wave, so we ignore the magnetic field when talking about polarization.

  • Let's look at an electromagnetic wave propagating in the z direction.

  • Again, here we're looking at a snapshot of a traveling wave at one instant in time.

  • When the electric field oscillates up and down along the y-axis, we call this vertical polarization.

  • If we rotate this wave by a quarter turn, it is now oscillating left and right along the x-axis, and we call this horizontal polarization.

  • If we rotate the wave by another quarter turn, we end up with vertical polarization again, although with the wave shifted by a half cycle compared to the original wave.

  • Let's look more closely at a vertically polarized wave.

  • Remember, the electric field is a vector field, meaning it is represented as an arrow at every point in space and time.

  • The arrow has components in the x, y, and z directions, which we can write like this, using a linear combination of the x, y, z basis vectors.

  • We can also write this as a three-component column like this.

  • For a vertically polarized wave, the electric field only exists along the y-axis, so the x and z components of the electric field go to zero.

  • If we were to write out the y-component of the electric field for this traveling wave, it would be an amplitude A times a cosine wave.

  • That depends on both time and space.

  • Here, t is time, and z is the location along the z-axis.

  • Omega is the angular frequency, and k is the angular wave number.

  • I find traveling waves are easiest to visualize on a spacetime diagram, with time moving into the future as we move upward.

  • Let's say that we have a wave that travels in the positive z direction over time.

  • We could draw out this traveling wave as a surface in our spacetime diagram.

  • The density of the waves in the spatial direction is given by the wave number, and the density of the waves in time is given by the frequency.

  • One thing we can do to modify our traveling wave is to add an extra phi value inside the sinusoid function.

  • You can think of this as indicating the wave's starting value at the origin z equals zero when time t equals zero.

  • This starting value is called a phase, and changing the phase value will shift the wave back and forth along the axis of travel.

  • Applying a phase shift of negative pi over two to a cosine will shift the wave ahead a quarter cycle, which is equivalent to a sine wave.

  • Now something that can help us represent waves is remembering Euler's formula, which tells us that we can write e to the power of the imaginary i times theta as cosine theta plus i times sine theta.

  • This is a useful property, because if we have e to the i theta and we want to add some angle phi to it, all we do is just multiply by e to the i times phi, and use the standard exponent rules to rewrite this as a single exponential with the exponents added.

  • If we then use Euler's formula to convert back to sine and cosine, we see that a phase phi has been added inside the sinusoid functions.

  • Now electromagnetic waves are described by real numbers.

  • But for convenience, we can pretend that our Ey component is actually a complex number, where the real part of this complex number is the actual electric field we observe in real life, with the imaginary part being ignored.

  • This means the full Ey component would have a real part with a cosine wave, and we can invent the fake imaginary part to be a sine wave, since we ignore it anyway.

  • Using Euler's formula, we can write this more compactly as a complex exponential.

  • This also means we can pull the phase phi out using exponent rules, and write it as a multiplicative factor, e to the i phi.

  • This allows us to write travelling waves as three separate multiplicative factors, the amplitude, times the phase, times the actual travelling wave.

  • So while the true electric field here is just the real part of this complex wave, we can write the electric field using complex exponentials for mathematical convenience.

  • As I said before, if we take this vertically polarized wave and rotate it a quarter turn, we get a horizontally polarized wave.

  • In this case, the wave only oscillates in the x direction, and so the y and z components of the field are zero.

  • Once again, the true electric field is given by a cosine, but for convenience, we can write it as a complex exponential, with the amplitude and phase written separately in front.

  • So to review, with the vertically polarized waves, the y component of the electric field is a travelling wave, and the x and z components are zero.

  • And with a horizontally polarized wave, the x component of the electric field is a travelling wave, and the y and z components are zero.

  • Now, we know from physical experiments that electromagnetic waves can be superimposed on top of each other.

  • So it's possible to add horizontally and vertically polarized waves together like this.

  • Now notice that the two polarizations each have their own amplitude and their own phase.

  • But the actual travelling wave portion is identical in both, so we can factor it out and write it outside the column like this.

  • Now here I want to state the main idea of this video.

  • When it comes to studying the polarizations of waves, all the information we need to look at is contained inside this column, the amplitudes and the phases.

  • The actual travelling wave portion of the formula can be ignored, since it's the same for all components.

  • We can even go one step further and ignore the z component altogether, since we can always choose coordinates where the z direction is the direction of wave propagation.

  • And therefore the z component of the electric field will always be zero.

  • The resulting two-by-one column of complex numbers is called a Jones vector, and it tells us everything we need to know about the polarization of a given wave.

  • Any light wave polarization can be written as a linear combination of a horizontally polarized wave and a vertically polarized wave, each with complex numbers in front denoting their respective amplitudes and phases.

  • Moving forward, I'm going to write this horizontally polarized wave of amplitude 1 using the vector capital H, and I'll write this vertically polarized wave with amplitude 1 using the vector capital V.

  • So using the idea of Jones vectors, we can create new polarizations by selecting different values for the amplitude and phase parameters.

  • For example, we can set both phases to zero, so that the horizontal and vertical polarizations are in phase with each other, and then set both amplitudes to one.

  • If we think of H as a vector along the x-axis and V as a vector along the y-axis, this new Jones vector points diagonally to the upper right.

  • This is called diagonal polarization, denoted with a capital D.

  • This is what we would get if we took a horizontally polarized wave and rotated it counterclockwise by 45 degrees.

  • Although, according to Pythagoras, the Jones vector H plus V has an amplitude of the square root of 2, so we usually divide the components by the square root of 2 to force the amplitude of D to be 1.

  • It's also possible to set the amplitude to plus 1 for H and negative 1 for V, and this We call this anti-diagonal polarization A.

  • This is what we would get if we took a horizontally polarized wave and rotated it clockwise by 45 degrees.

  • Once again, we normalize this by dividing by the square root of 2.

  • So we can get the D and A polarizations by adding H and V together in the right amounts.

  • In fact, we can make the wave's polarization have any angle on this circle, if we set the coefficients in front of H and V properly.

  • But there are actually more polarizations that we still haven't seen yet.

  • Let's again set both amplitudes to 1, and set the horizontal phase to be 0, and set the vertical phase to be pi over 2, which is a phase of a quarter wave cycle.

  • This polarization is more difficult to visualize, so let's bring back our column notation with the traveling wave to understand it better.

  • Let's pretend we're stuck at the position z equals 0, and the angular frequency of the wave is 1, and we're watching the wave travel around the xy plane over time.

  • What would this look like?

  • We can combine the exponentials, then use Euler's formula, and then take the real part to see that the electric field is given by a cosine, and a cosine with a phase factor of a quarter cycle, which is really the same thing as a negative sign.

  • At time equals 0, this gives the coordinates 1, 0.

  • Then at t equals pi over 2, we get the coordinates 0, negative 1.

  • Then at t equals pi, we get negative 1, 0.

  • At t equals 3 pi over 2, we get 0, 1.

  • And at t equals 2 pi, we get 1, 0 again.

  • So in this wave, the electric field vector travels around in a circle in a clockwise direction over time.

  • Bringing back the z-axis, if we take our left hand and point our thumb in the direction of wave travel along the z-axis, the electric field vector at the origin z equals 0 will follow the direction of our curled fingers.

  • Since the wave follows a circle according to our left hand, we call it left circular polarized.

  • This wave would have a helix shape in three dimensions.

  • Wikipedia user Dave3457 has made a great animation of this that he's put into the public domain.

  • We denote left circular polarized waves as capital L.

  • It's also more common to write e to the i pi over 2 as just i, which is a quarter turn in the complex plane.

  • And once again, we normalize by dividing by the square root of 2.

  • If we repeat this process from the start, but instead giving the vertical polarization a phase of negative pi over 2, we get a helix wave that corkscrews in the opposite direction, matching our right hand when the right thumb points in the direction of wave travel.

  • So we call this right circular polarized, denoted by capital R.

  • Now you'll notice in this video, I've written my traveling waves with a positive time term and a negative z term.

  • Some textbooks use the opposite sign convention, with a positive z term and a negative time term.

  • And as a result, the Jones vectors for circularly polarized waves have opposite signs on the So make sure you know which sign convention you're using when talking about circularly polarized waves.

  • So to summarize this video, we initially discovered the Jones vectors h and v, which represent horizontally and vertically polarized traveling waves.

  • We then found that writing them in different linear combinations could give us new polarizations of light.

  • Like diagonal and anti-diagonal polarizations, and the left and right circular polarizations.

  • We're going to see in the next video that these Jones vectors that represent wave polarizations are actually spinors.

  • At this point, there's no particular reason why we would decide these pairs of complex numbers are special objects that deserve the special name of spinner.

  • But in the next video, we're going to see how we can rotate these various polarizations into each other using special matrices called SU2 matrices.

  • And this will reveal a special angle doubling relationship between physical space and the space of wave polarizations.

  • We'll see that one rotation in physical space corresponds to two full rotations in the polarization space.

  • The Jones vectors that live in polarization space require two full rotations to get back to the starting point.

  • And this is exactly what we would expect from spinors.

  • In the meantime, before the next video, I'd suggest trying to draw out the shapes of various polarizations for the Jones vectors shown on the screen here.

  • If you feel confused, just use the strategy I showed earlier of taking z equals zero and omega equals one, and plugging in different time values to see how the wave moves around in the xy plane.

  • The answers are linked in the description.

So, in the last video, I introduced my staircase plan for explaining spinors, which starts with the simplest explanations at the bottom and ends with the most complicated explanations at the top.

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