쉐도잉 연습: The Uncertainty Principle: What Does It Mean, How Does It Work? - 영상으로 영어 말하기 배우기
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If you know one thing about quantum mechanics, then that's more than most people, and it's probably that it's got something to do with the uncertainty principle.
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But just exactly what does that mean and how does it work?
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That's what we'll talk about today.
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Werner Heisenberg was the first to understand that quantum mechanics sets limits to what we can know.
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Yes, even for string theorists.
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Some properties of quantum particles can't be determined precisely at the same time.
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And it's not because we're not good at measuring, it's just how nature is.
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The best known example is the position and momentum of an object.
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You can think of the momentum as the velocity multiplied with the mass.
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This isn't correct for massless particles, but for our purposes it'll be good enough.
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Let's just pretend that massless particles don't exist, it shouldn't be too hard.
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Quantum mechanics says that you can't measure both the position and momentum precisely.
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This means if you know precisely where a particle is, you don't know which direction it's going.
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And the other way around, if you know which direction it's going, you don't know where it is.
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The position of a particle is usually denoted with x and the momentum with p.
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The uncertainty in each is marked with a large delta in front of the variable.
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So delta x is the position uncertainty and delta p is the momentum uncertainty.
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Heisenberg's uncertainty principle then says that the product of those two is always larger than a constant h -bar divided by two.
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This means if one of those uncertainties gets very small, then the other one must be very large, otherwise the inequality would be violated.
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This is where the joke about Heisenberg comes from, where he gets stopped by police who tell him how fast he was driving, and Heisenberg says, great, now I'm lost.
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But what does it mean that you can't measure the position and momentum with certainty at the same time?
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Does it mean that if you come with two detectors, a lightning strike will explode one of them?
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Well, no. The uncertainty principle doesn't say that you can't measure both of those quantities.
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It shows that you can't measure both precisely.
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If you've pinned down one, then the other will have a large spread.
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This means if you repeat the experiment, the result will be all over the place.
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It's the statistical uncertainty of this series of measurements that becomes large.
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A good example of this is letting quantum particles go through a narrow opening.
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The quantum particles act like waves, so this will create an interference pattern on the screen.
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This pattern is built up of single particles.
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The particles don't all collect in one place.
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And that's because you know the particles went through the slit, so you know something about their position.
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Then you can't tell which direction they are going.
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But of course, once a single particle hits the screen, you know which direction it went.
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What the uncertainty Uncertainty principle means is therefore that if you repeat this for many particles, then the outcome has a broad distribution.
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Another example is the relation between the uncertainty in energy and time.
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Consider you have a fluorescent sticker, the kind of stuff that glows in the dark.
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You put it into light and then, for a few hours afterwards, it'll emit light of a particular color, usually it's some shade of green.
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The way this works is that the light
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which falls on the sticker kicks off an electron from its normal energy level into a higher level.
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In most materials, the higher electron levels are extremely unstable.
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The electron falls back down immediately, and in that process the photon is emitted again.
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In fluorescent materials, however, the electrons can stay there for a few hours.
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It's called a metastable state.
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And only when the electron falls down will the light be emitted again.
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As a consequence the sticker glows for some hours.
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But just exactly how long do the electrons stay in that higher energy level?
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Ah, well, you can't say exactly.
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You can only talk about the probability of it dropping down in a certain amount of time.
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And why is that?
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It's because you know something about the energy of the electron on.
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It's sitting on this meta -stable level.
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Consequently, you can't know exactly how long it stays there.
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Such is life you can't have at all.
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This is basically also how nuclear decay works, by the way.
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Finally, the uncertainty principle has its origin in the properties of waves.
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It comes about because in quantum mechanics particles can act like waves.
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What's a wave?
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A wave is something that changes periodically in space and time.
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That could be water waves, electromagnetic waves, sound waves, or even a Mexican wave when a sports game gets boring.
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Waves have a wavelength and a frequency that's inversely proportional to the wavelength.
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The frequency tells you how much change there is in a certain period of time.
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If you have a perfectly regular sound wave, then it would sound like a beep at one particular frequency.
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But most sound signals aren't that simple.
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For example, here's me singing an A.
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This isn't just one frequency.
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You can take this sound apart and you'll find that, for one thing, I'm not a computer chip, so I don't exactly hit the A.
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But also, the way the human voice box works, it has a lot of higher harmonics.
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This breakdown of sound into all the frequencies it contains is called a spectrum.
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This doesn't only work for sound, but for every distribution of anything really.
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You can calculate a spectrum of the distribution of people in a room if you want to, and I'm sure somewhere there are businesses doing just that.
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But a more relevant example for us is light.
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If you have light of one particular wavelength, then that'd be one particular color,
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and the spectrum of this light would have one single peak at one particular frequency.
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Technically, for the spectrum to be exactly one frequency, the light wave would have to keep on waving forever.
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We never deal with that in reality.
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In reality, the light we deal with is bunched.
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It passes by within a certain window of time.
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First it wasn't there, then it was there, now it isn't there again.
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Like money on my bank account.
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Physicists call this a wave packet.
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How do you pack waves?
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Especially without getting wet?
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The curious thing about waves is that they can interfere both constructively and destructively.
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If they interfere constructively, they add up.
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If they interfere destructively, they can cancel each other out.
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If you overlay many of them in just the right way, you can do this so that outside of some region of space and time, the interference is almost completely destructive,
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and you are left with a constructive interference in just a small region.
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A wave packet is an overlay of different wavelengths and therefore an overlay of different frequencies with the correct offset.
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Such an overlay, by the way, is called a superposition.
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Sounds familiar?
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Yes, we do use superpositions in quantum mechanics.
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And this is where the word comes from.
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It comes from adding different wavelengths together.
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You superpose them.
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Okay, now here's the thing.
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As we just saw, we have two ways to describe the same wave packet.
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You can either say it's this distribution in time, wasn't there, was there, isn't there again,
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or you can say it's this distribution of frequencies with these offsets.
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They both describe the same thing, the same wave packet.
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There is a mathematical procedure to calculate one from the other.
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It's called a Fourier transformation.
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Put in a distribution in time, the Fourier transformation will give you the spectrum.
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Put in the spectrum, the Fourier transformation will give you the distribution in time.
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Here's the kicker.
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If the one distribution is sharply peaked, say you have a flash of light that's just a brief moment in time,
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then that means that it must contain a lot of different frequencies.
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The spectrum is very spread out.
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And the opposite is also true.
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If you have something with a very narrow frequency, then it must be spread out in space.
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Now you can ask, what's the relation between the spread in these two distributions, the one in time and the one in frequency?
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And would you know it, they're related to each other by an inequality that looks pretty much like the uncertainty principle.
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Whoa, but wait, this had nothing to do with quantum mechanics.
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We were just talking about spectral analysis.
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So what is going on?
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What's going on is that while this looks like the uncertainty principle, it's not.
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This is a property of waves.
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It relates a spread in time with the spread in frequency.
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To get Heisenberg's uncertainty principle, you further have to identify a frequency with an energy.
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Or if you do it in space, you have to identify the wave vector with the momentum.
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And this is where the H bar gets in.
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We learned this from no other than Albert Einstein.
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Yes, that guy again.
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He pops up more than toast in a student house.
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It's actually what he won the Nobel Prize for.
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No, seriously.
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Albert Einstein didn't win the Nobel Prize for special or general relativity.
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He wanted for putting h -bar in the right place.
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And the way he figured it out was from an observation called the photoelectric effect.
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If light shines on a metal plate, that can kick electrons out of the plate.
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One can measure this because it creates a current, so it's electric.
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This is why it's called the photoelectric effect.
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But for this to work, the frequency of the light must be above a certain threshold.
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If the frequency stays below the threshold, but you increase the brightness of the light, nothing happens.
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This was very confusing to scientists in the 19th century.
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They could understand that it takes energy above a certain threshold to kick out an electron.
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But if you think that light is a wave, then it's the brightness that measures this energy.
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So why would turning up the brightness not kick out electrons?
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Along came Einstein and he said that's because light is made of chunks of energy.
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We now call those chunks photons.
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To kick out an electron, the energy of the photon has to be above a threshold, not the total energy of the light.
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The total energy of the light is the sum of the energy of all those photons.
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But the energy in each photon is proportional to the frequency.
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Therefore, if you want to know the total energy of the light, you take the number of photons and multiply it with their frequency,
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and now you need a constant to convert the frequency into an energy.
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That constant is Planck's constant, h.
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And the h with the bar, that's called the reduced Planck's constant and is h divided by two times pi.
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It's more commonly used in quantum mechanics because, like my uncle, it makes a lot of pi's disappear, so it's more convenient.
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Why is it called Planck's constant and not Einstein's constant?
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Good question, but I'll leave this for another video.
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Let's instead step back here and ask what all this means now.
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We've seen that what's seemingly so weird about the uncertainty principle, that there are two quantities that you can't measure precisely at the same time,
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has really nothing to do with quantum mechanics.
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It's just a property of waves.
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What quantum mechanics does for you is to make this a property of particles.
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And for that to work, you have to relate time with energy and space with momentum.
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If you're uncertain about any of this, then you're doing it right.
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We have also seen that the uncertainty principle doesn't mean you can't measure those quantities precisely in one round of an experiment,
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but that means if you repeat the experiment you get a large statistical distribution for at least one of those quantities.
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But then couldn't it be that the quantum particle actually had this property before it was measured, you just didn't know what it was?
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Rather than doing this weird thing where it's in several states at the same time until you look at it
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and poof it decides on one?
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Yes indeed.
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That's what is called a hidden variables model, and it's how Einstein thought quantum mechanics really works.
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He didn't like spooky action at a distance, and he was certain about his principles.
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Watching YouTube videos is great, especially if they're about such fun topics as quantum mechanics.
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But if you want to really understand the topic, then you have to actively engage with the material.
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A great place to do that is Brilliant, who have been sponsoring this video.
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On Brilliant, you find courses on a large variety of subjects in science and mathematics.
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The great thing about their courses is that they're all interactive with visualizations and follow -up questions, so you can check your understanding right away.
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This is why I like to look things up on Brilliant.
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It's fast, it's easy, and it tells me what I need to know.
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And they are constantly expanding their content.
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To understand better what I talked about in this video, check out for example my course about quantum mechanics.
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It gives you an introduction to interference, superpositions and entanglement, and of course the uncertainty principle.
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It begins from the very basics so you don't need to bring any background knowledge.
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And after that, you can continue maybe with their course on quantum objects or quantum computing or wherever your curiosity drives you.
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If you're interested in trying Brilliant out, use our link brilliant .org slash sabine
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and sign up for a free trial where you'll get to try out everything Brilliant has to offer for a whole week.
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The first 200 subscribers using this link will also get 20 % off the annual premium subscription.
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Thanks for watching.
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See you next week.
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이 레슨의 어휘와 말하기 포인트
이 영상에는 섀도잉할 문장 182개와 단어 2366개가 있습니다. 말하는 구간의 길이는 14:44입니다. 화자는 분당 약 161단어로, 일상 대화에 가까운 자연스러운 속도로 말합니다. 영어에서 가장 많이 쓰이는 3,000단어에 속하는 단어가 81%뿐이라 어휘가 어려운 편입니다.
이 영상의 핵심 어휘
영상에 나오는 익혀 둘 만한 단어 15개를 발음, 뜻과 함께 정리했습니다.
| 단어 | 발음 | 뜻 |
|---|---|---|
| frequency 명사 | /ˈfɹiːkwənsi/ | 빈도 |
| uncertainty 명사 | /ʌnˈsɜːtənti/ | 불확실 |
| particle 명사 | /ˈpɑɹtək(ə)l/ | 입자, 립자 |
| principle 명사 | /ˈpɹɪn.sɪ.pəl/ | 원리, 원칙 |
| mechanic 명사 | /mɪˈkænɪk/ | 정비공, 기계공 |
| momentum 명사 | /ˌmə(ʊ)ˈmɛntəm/ | 운동량 |
| spectrum 명사 | /ˈspɛktɹəm/ | 스펙트럼, 분광 |
| electron 명사 | /ɪˈlɛk.tɹɑn/ | 전자 |
| quantity 명사 | /ˈkwɑn(t)ɪti/ | 양, 량 |
| threshold 명사 | /ˈθɹɛʃ(h)oʊld/ | 문턱, 문지방 |
| interference 명사 | /ˌɪntəɹˈfɪɹɪns/ | 간섭 |
| packet 명사 | /ˈpæk.ɪt/ | 패킷, 소포 |
| experiment 명사 | /ɪkˈspɛɹ.ə.mənt/ | 실험 |
| transformation 명사 | /ˌtɹæns.fɔɹˈmeɪ.ʃən/ | 변형, 변환 |
| delta 명사 | /ˈdɛltə/ | 델타 |
영상에 나오는 구동사
| 단어 | 발음 | 뜻 |
|---|---|---|
| fall down 동사 | /fɔl ˈdaʊn/ | 떨어지다 |
주의할 발음
화자는 can't, don't, isn't 같은 축약형과 약화된 형태를 51번 사용합니다. 들리는 대로 짧게 발음하세요.
- “th” 소리: threshold /ˈθɹɛʃ(h)oʊld/, mathematics /mæθ(.ə)ˈmæt.ɪks/, mathematical /ˌmæθ(.ə)ˈmæt.ɪ.kəl/, wavelength /ˈweɪvˌlɛŋ(k)θ/, theorist /ˈθiːəɹəst/
- “sh”와 “zh” 소리: threshold /ˈθɹɛʃ(h)oʊld/, transformation /ˌtɹæns.fɔɹˈmeɪ.ʃən/, relation /ɹɪˈleɪʃ(ə)n/, flash /flæʃ/, shine /ʃaɪn/
- 긴 단어 — 강세 위치에 주의: uncertainty /ʌnˈsɜːtənti/, momentum /ˌmə(ʊ)ˈmɛntəm/, interference /ˌɪntəɹˈfɪɹɪns/, experiment /ɪkˈspɛɹ.ə.mənt/, transformation /ˌtɹæns.fɔɹˈmeɪ.ʃən/
이 영상으로 연습하는 방법
- 먼저 말하지 않고 영상을 끝까지 듣고 모르는 단어를 적어 둡니다.
- 0.75배속으로 한 문장씩 섀도잉을 시작하고, 익숙해지면 보통 속도로 돌아갑니다.
- 자신의 목소리를 녹음해 원본과 비교하고, frequency, uncertainty, particle 같은 단어에 특히 주의합니다.
이 영상의 문법
화자가 가장 많이 쓰는 문형을 영상 속 실제 표현과 함께 정리했습니다.
| 문형 | 영상 속 표현 |
|---|---|
| 수동태 be + 과거분사 — 누가 하는지보다 무슨 일이 일어나는지에 초점 | can't be determined · is usually denoted · is marked |
| 현재완료 have/has + 과거분사 — 과거의 일이 지금도 관련이 있을 때 | you've pinned · We've seen · have also seen |
쉐도잉이란? 영어 실력을 빠르게 키우는 과학적 방법
쉐도잉(Shadowing)은 원래 전문 통역사 훈련을 위해 개발된 언어 학습 기법으로, 다언어 학자인 Dr. Alexander Arguelles에 의해 대중화된 방법입니다. 핵심 원리는 간단하지만 매우 강력합니다: 원어민의 영어를 들으면서 1~2초의 짧은 지연으로 즉시 소리 내어 따라 말하는 것——마치 '그림자(shadow)'처럼 화자를 따라가는 것입니다. 문법 공부나 수동적인 청취와 달리, 쉐도잉은 뇌와 입 근육이 동시에 실시간으로 영어를 처리하고 재현하도록 훈련합니다. 연구에 따르면 이 방법은 발음 정확도, 억양, 리듬, 연음, 청취력, 말하기 유창성을 크게 향상시킵니다. IELTS 스피킹 준비와 자연스러운 영어 소통을 원하는 분들에게 특히 효과적입니다.