A Night with the Stars


A Night with the Stars

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Transcript


LineFromTo

Where's the reception? Oh, OK...

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So nobody knows what this lecture is going to be about...

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I know what it's about. It'll be about science, and he'll be promoting that heresy of his.

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I hope he's going to unveil a death ray. I don't know.

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I'm going to make one, at least one unsuspecting celebrity, do sums.

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-I really am so out of my depth...

-LAUGHTER

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This is the worst thing that's happened to me as an adult.

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The only thing I do know is that I've been roped in to go up

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on stage - with Simon Pegg, no less - waving a rope about.

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I can see why you've got no hair.

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LAUGHTER

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I'm so thrilled to have been asked, to be honest.

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I never do clever things.

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There's a real buzz in this room, and it just makes me feel proud to be a scientist in this day and age.

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Perhaps tonight is my chance

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to realise what it's all about, and have a big sort of Damascene moment.

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I'd like to ask Professor Brian Cox about his hair - it's a shared interest.

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-I hope he blows some stuff up.

-Whoa... Ow!

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I'm hoping it's going to start simple, for people like me,

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and then get slowly more complicated.

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Because otherwise, if my brain starts swelling inside my skull

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it's just going to pop and I'll distract people.

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Thank you.

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Welcome to the Royal Institution of Great Britain, established

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in 1799 as "an institution for diffusing knowledge",

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and perhaps the most iconic lecture theatre in science.

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Thomas Huxley championed Charles Darwin's theory of evolution here,

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Michael Faraday pioneered our understanding of electricity and magnetism here,

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and on this stage he demonstrated the first electric motor.

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And the great scientist and lecturer Sir Humphry Davy,

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who was also the first director of the Royal Institution

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and one of my heroes, spoke here many times.

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And he gave the best explanation of the absolute need to do science that I know of -

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"Nothing is so fatal to the progress of the human mind

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"as to suppose that our views of science are ultimate;

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"that there are no mysteries in nature;

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"that our triumphs are complete,

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"and that there are no new worlds to conquer."

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Well, tonight I want to talk about one of the great mysteries,

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pillars of our understanding of nature -

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the scientific theory that underpins much of the technology

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we take for granted in the 21st century,

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yet retains its reputation for obscure difficulty and bizarre predictions.

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Now, by the time I've finished, I hope that

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while your view of reality might have shifted a little,

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you'll understand a bit more about how the universe works.

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Now, let's start with the contents of this box.

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This is a rough diamond. It's worth well over £1 million.

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It costs so much because it's rare, and because it's beautiful.

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But there's a different kind of beauty here, a more profound

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kind of beauty - less superficial, but perhaps far more instructive.

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A diamond is one of the hardest known substances -

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which is why diamonds are widely used industrially -

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but light can stream through it relatively unimpeded.

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So there's beauty in a question, which is,

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how can something be so ethereal, and yet be

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so hard that it can drill through solid rock?

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Well, to answer that we need to know about the

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structure of the diamond - indeed the structure of all matter itself.

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And the best theory we have to describe matter, is quantum theory.

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Now, I understand why quantum theory can seem a bit odd.

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It makes odd statements.

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It says, for example, that things can be many places at once -

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in fact, technically it says things can be in an infinite number of places at once.

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It says that subatomic building blocks of our bodies

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are constantly shifting in response to events that happened at the edge

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of the known universe - a billion light years somewhere over there.

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Now, this is all true, but that isn't a licence to talk utter drivel.

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LAUGHTER

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See, quantum theory might SEEM weird and mysterious, but it describes the

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world with higher precision than the laws of physics laid down by Newton,

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and it's one of the foundations of our modern understanding of nature.

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It doesn't, therefore, allow mystical healing,

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or ESP or any other manifestation of New Age woo-woo

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into the pantheon of the possible.

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Always remember, quantum theory is physics, and physics is

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usually done by people without star signs tattooed on their bottom.

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What makes quantum theory a good scientific theory?

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Well, it makes predictions that can be tested against experiment,

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and when we test those predictions we find that they agree with observation.

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This means quantum theory is not wrong - it's a survivor,

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if you like, because it's been put to the test over and over again,

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and consistently been found to make correct predictions.

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If this changes, then we'll search for a new theory -

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there are NO absolute truths in science.

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This is how we make scientific progress, and this is how

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everything in the world that you take for granted was delivered.

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So, remember that however odd it might seem, tonight

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I'm going to show you, hopefully, that quantum theory works.

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So, I want to explain quantum theory to you in the simplest way that I can.

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Ultimately, I'll show you how it gives us insight into the

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fundamental building blocks of the universe, and explains the existence

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of some of the most spectacular phenomena out there in deep space.

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And I'm going to do this now because if I don't point wistfully at the sky at least once,

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some of my viewers will get annoyed, so there you go.

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That's the only mountain-top pose I'm going to pull...

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-LAUGHTER

-..so, to begin...

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No helicopters tonight.

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To begin, let's zoom into the heart of this diamond.

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What I've got here is a sequence of actual photographs of, well,

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initially the surface of a diamond, but these photographs

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have been taken by a series of increasingly powerful microscopes.

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So as we zoom in you see that at first you're seeing a more

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detailed picture of the structure of the surface of the diamond.

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But as we go right in, you see that a regular pattern,

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a regular structure emerges,

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so this is an electron microscope photograph of diamond.

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And what you're looking at here actually are carbon atoms,

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individual atoms.

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You see that they appear to be in a kind of a dumbbell shape, and there's a space

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and another pair, because you're looking at a two-dimensional image.

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But if you take that to three dimensions

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and look at this - this is the structure of diamond,

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and what you can see is carbon atoms surrounded by four other

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carbon atoms, in a regular, beautiful crystalline structure.

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Now, in this diamond, this over- a-million-pound piece of diamond,

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there are something like 3 million billion billion atoms,

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and they are laid out in precisely this beautifully simple way.

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I should say, actually, this diamond is as it was when it was found,

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so this hasn't been cut. It was found in South Africa well over 100 years ago,

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and it's 3 billion years old.

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And that structure, its diamond shape -

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that's how it naturally appeared, because its structure

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is like this, it's built out of carbon atoms exactly like that.

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Carbon atoms can't be packed any more tightly together than this.

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That's what makes diamonds so tough, and allows them

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to cut through virtually anything.

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Which makes what I'm about to say quite remarkable.

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See, the atoms that make up this diamond -

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and pretty much everything else for that matter - are virtually empty.

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Now, what do I mean by that? Well, what is an atom?

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Well, about 100 years ago now, in the greatest city

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known to civilization - which is Manchester! -

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APPLAUSE

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..Ernest Rutherford discovered that the atom consists of an atomic nucleus,

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which is made of particles called protons and neutrons tightly packed together,

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and a third kind of particle,

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called electrons, orbit somewhere or exist somewhere around the outside.

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The nucleus protons are positively charged,

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the neutrons are neutral, so it has a positive charge.

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The electrons somewhere out here have a negative charge,

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and as Faraday would have talked about on this very stage

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just under 200 years ago, there is a force that holds

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the electron to the nucleus,

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because they're both electrically charged.

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So that's kind of a sketch, a schematic view of the atom.

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We've known that now for around a hundred years.

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Protons, neutrons and electrons.

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These three particles make up not only the diamond,

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but everything we can touch, every structure we can see.

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Everything is made up of these same three absolutely identical particles.

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So the richness of the natural world, everything on planet Earth,

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everything we can see beyond is described by a simple recipe

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that determines how these simple particles combine together.

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Now, clearly physicists don't call it a recipe, we call that quantum theory.

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Now, one of the first great challenges for quantum theory -

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indeed, one of the reasons it was developed at the turn of the 20th century,

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in Manchester and a few other places - was to understand precisely how these particles

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come together to create this diamond, you, me and everything else.

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And a hundred years after its discovery, it still provides

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our best understanding of the structure of matter.

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And admittedly, yes, it is still a bit strange.

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Now, one of the particularly strange things about it is the behaviour of electrons inside atoms.

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See, these imperceptibly tiny electrons spend

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the overwhelming majority of their time in far distant clouds.

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So between the nucleus and the electron there is a vast emptiness.

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If I were a nucleus, and I perched on the edge of the White Cliffs of Dover,

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then the fuzzy edge of the electron cloud would be

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somewhere in the farms of northern France.

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Looking out towards the electrons I'd see nothing but empty, interatomic space.

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So atoms are vast, and they are empty. Actually about -

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I've got to count this on my fingers -

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99.9999999999999% empty.

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That's 13 nines. So, you buy this diamond,

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and you're buying about a million quid's worth of mainly empty space, and since

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everything is made of atoms, that means you are vast and empty too.

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LAUGHTER

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Especially you... No, I can't say that, can I?

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Never say that to a stand-up comic - what am I doing?

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Anyway, if I squeezed all the space out of all the atoms in all

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the people on the planet, then you'd be able to fit the whole

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of humanity into that diamond, and that's how empty matter is.

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So, understanding why atoms are empty and yet so solid,

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why light can stream through that diamond, and yet

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it sits nicely on the predominantly empty cushion and the predominantly empty floor,

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is therefore a prerequisite to understanding the structure of everything in nature.

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Now, you might have gathered that the world inside an atom

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must be a strange place where things don't behave

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much like they appear to behave here in the macroscopic world.

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Well, there's one historic experiment

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which contains everything you need to know about the bizarre way

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that particles behave, and therefore why atoms are the way that they are.

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I'm going to need a helping hand for this,

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and I know that Sarah Millican has volunteered kindly to help me.

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-Where's Sarah?

-I'm here. Hello.

-So Sarah - would you mind...?

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Thanks, Sarah. Did you do a science degree, by the way?

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No. I've already been asked that by somebody in the audience -

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"Did you study physics?"

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No, I just sort of gave up after GCSE - is that a problem,

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-should I go back to me seat?

-LAUGHTER

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-Any other volunteers(?) No...

-Only got a C!

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So you may or may not have heard of the double slit experiment, it's something every physics student...

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-I've heard of it, but it was something different.

-Was it(?)

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-Well, we're going to...

-LAUGHTER

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Every physicist is taught this the moment they step through the doors of a university.

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It's simple, and it demonstrates the paradoxical world of quantum particles.

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So first of all we're going to do it - we're going to do it twice, or even three times.

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So I'm going to give you this bucket of sand, which is quite heavy actually.

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These are particles of sand, little bits of sand. They're probably your picture,

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I suppose, of what a particle might be, a little piece of matter.

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So what I'm going to ask you to do is just pour the sand

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onto this piece of board, which has got two slits cut in it,

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and I suppose before I do it...

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-Oh, you bugger!

-It's a bit heavy!

-It is.

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You pour it first, then I'll ask you what you think might happen.

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Yeah, let's chat for a while, while I'm holding the bucket(!)

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It weighs a ton, doesn't it? So just pour it through the slits...

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Now, what do you think is going to happen?

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So we're just pouring particles of sand over the slits.

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Just keep going...

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So there we are. That'll do, I think.

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So if I remove that... what does that remind you of?

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LAUGHTER

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I feel like smacking it - does that help?

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Pour that sand into there. So that's probably pretty much...

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-There you go, you can put it down now.

-Thank you!

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That's probably pretty much, I suppose, what you expected would happen.

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The sand has just fallen through the slits,

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and beneath each slit there's a bigger pile of sand.

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Particles fall through slits - pretty obvious.

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But...this is a picture of real data.

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So this is real experimental data,

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of electrons essentially being poured through two slits, so it's electrons

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being fired at two slits, and then there's a screen there, and so what

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you're seeing are just piles of electrons, so the white spots

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really are where electrons hit the screens -

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there's a pile, and then there's nothing,

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and then there's a pile, and then there's nothing...

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Looks nothing like that. But the experiment was the same -

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it really is electrons being poured through two slits

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onto a screen, and you get that strange pattern.

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So, let me show you this, which is a different version of the same experiment.

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Now, this is a tank of water, so there's some water in there,

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and as you can see there's just a bar that's vibrating up and down,

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-and then there's two slits.

-Yeah.

-So you can see the two slits there.

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And if you come round here... you can see the screen here.

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So there's the two slits, and these are the waves of water.

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So there's a flat wave of water hitting the two slits,

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and then coming through the slits.

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And do you see that there are waves here,

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-but here, there's kind of an area where the water's flat.

-Yeah.

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Then here there are waves,

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then here's an area where the water's flat,

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then here are waves, here's an area where the water's flat.

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So if I were to, I could sketch it actually on the blackboard.

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If I draw that...

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We've got those two slits, like that, which you can see there.

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and we've got the water wave coming through

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and you can sort of see that the waves

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when they go through the slits spread out like that.

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And I hope you can see that at the front, you're seeing

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a kind of a place where there's no waves and then some waves

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and then there's a place where there's no waves

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and then there's some waves and a place where there's no waves.

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-You see that pattern on the front.

-Yes.

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So if you were to draw kind of a detector along there,

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then you'd see that, right,

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because here you'd see nothing, no waves no electrons.

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Here you'd see the electrons, here no waves, here waves, here no waves.

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So what are we to infer about electrons?

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Have you not done your homework today, is that what it is?

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I mean this is just the experimental data... This was first done,

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by the way, in the 1920s and it was a shock when it was seen,

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but the inference is...?

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That looks like...that.

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-This could be a long game.

-It's the same pattern!

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LAUGHTER

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GCSE grade C, remember.

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This pattern here...

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What do you think...?!

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You could just tell us.

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So, the electrons are behaving more like the waves in the tank

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on the water waves and that's a classic pattern you see

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when you get waves passing through slits.

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Rather than this, which I suppose is what you might have expected

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electrons to do, because you might think of electrons as being little grains of sand.

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But actually, they don't behave like little grains of sand.

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That experiment tells us they behave more like waves and water.

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Exactly!

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LAUGHTER AND APPLAUSE

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Thank you.

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Thanks, Sarah!

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Thanks, Sarah. That's... Yeah, physics!

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Well...

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this might all be a bit confusing, as you've just seen,

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but if you remember nothing else, remember this - the double slit experiment reveals something

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fundamental about particles like the electrons inside the diamond.

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Sometimes they behave like particles,

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but sometimes experiment says that they behave like waves.

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Now there's a deep explanation for this

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and I'm going to get to that a little bit later on,

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but for now all we need to remember is that electrons behave like waves,

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and this is the key to understanding the emptiness of atoms.

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Simple? I hope so. So let's clear away the water tank.

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So, we've understood that electrons exhibit wavy behaviour,

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but how does that explain the emptiness of atoms?

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Well, I need some volunteers now and I know that Simon Pegg

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and Jim Al-Khalili have kindly volunteered, so would you both like to come down?

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APPLAUSE

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Have you seen him, there?

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Hello!

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He's got an earpiece in he's watching really carefully.

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So, I've got an experiment for you both to do involving a spring

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and your wrists,

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so...

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What I'd like you to do

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is stretch the string a little bit as far away as you can.

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Now what I want you to do is start gently oscillating the spring. Very gently.

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-Both of us?

-Yeah. You'll see what happens.

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Up and down, or longitudinally?

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ALL: Ooh!

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Shall I sit back down?

0:20:260:20:28

Up and down is better. Up and down.

0:20:290:20:33

So just a bit more...

0:20:330:20:34

There you go... And a bit more.

0:20:360:20:38

There you go. So what you're doing is vibrating the spring.

0:20:380:20:42

Are you going to jump in?

0:20:420:20:44

LAUGHTER

0:20:440:20:47

It looks quite painful.

0:20:480:20:50

So what you're doing now, just gently vibrating the string,

0:20:500:20:54

you notice that it's vibrating in a very particular way.

0:20:540:20:57

Cos you're holding it still there and you're holding it still there,

0:20:570:21:00

so it's trapped - it's confined, in a sense.

0:21:000:21:03

So what you can see is there's only one bit which is moving

0:21:030:21:07

with the maximum amplitude if you like, the maximum wave

0:21:070:21:10

and it's in the middle there.

0:21:100:21:12

So that's called a standing wave. It's called a standing wave

0:21:120:21:15

because it's confined.

0:21:150:21:16

It's doing nothing, really - it's vibrating up and down.

0:21:160:21:18

It's not a wave as you might usually expect it.

0:21:180:21:22

Now, if you give it a bit more wrist action...

0:21:220:21:24

GIGGLING

0:21:240:21:26

Look at that one - now, that...

0:21:270:21:30

THAT is the next standing wave up,

0:21:300:21:33

so there is a transition from the one where we're just moving here -

0:21:330:21:37

this one's got three stationary points.

0:21:370:21:40

-I lost me stroke...

-Don't get carried away.

-Sorry, sorry.

0:21:400:21:44

Wait, wait, wait -

0:21:450:21:48

this has never happened to me before!

0:21:480:21:50

LAUGHTER AND APPLAUSE

0:21:500:21:54

There - look at that - now there's three stationary bits -

0:21:550:21:58

there's one stationary there, one stationary bit there, one stationary bit there

0:21:580:22:02

and the amplitude - the maximum amplitude is there and there.

0:22:020:22:05

Now, you can get another one going...

0:22:050:22:08

if you really try, which is the third one.

0:22:080:22:11

There it is! No!

0:22:110:22:12

CHEERING

0:22:120:22:14

Look at that.

0:22:160:22:18

Yes, yes, yes!

0:22:220:22:24

Can you see? That's got two stationary points -

0:22:240:22:27

-one there and one there. That's a brilliant...

-Oh, it's gone again!

0:22:270:22:31

I can see... Hang on... There, there, there!

0:22:310:22:34

Two stationary points... 1, 2, 3, 4 stationary points.

0:22:340:22:37

-I can see why you've got no air!

-Here it is! There it is!

0:22:370:22:40

Ah, that's better now. There's the fourth one.

0:22:440:22:46

So, you...

0:22:460:22:48

You carry on.

0:22:480:22:50

Now it feels like someone else!

0:22:500:22:52

It's back! Ah, it's gone!

0:22:520:22:54

So if I just sketch... Carry on!

0:22:570:23:00

There we go - yes!

0:23:000:23:01

-Brian, Brian, Brian, Brian!

-Yeah, yeah, yeah!

0:23:010:23:04

APPLAUSE

0:23:040:23:07

Perfect.

0:23:150:23:16

1, 2, 3, 4, 5 - all right, you can stop now.

0:23:160:23:19

Good practice for later!

0:23:210:23:23

-Thank you very much!

-Thanks.

0:23:250:23:27

APPLAUSE

0:23:270:23:28

I sketched what you saw there.

0:23:330:23:35

You saw that one very clearly which was this wave

0:23:350:23:37

where there were just two stationary points

0:23:370:23:39

which were at the ends and then you saw this one,

0:23:390:23:42

where there were three stationary points.

0:23:420:23:45

And then you saw this one where there were four stationary points

0:23:450:23:47

and actually, because you were... That's the best I've ever seen it done,

0:23:470:23:51

-there was one with about five, I think, or even six.

-(Yes!)

0:23:510:23:53

So, you saw that...

0:23:530:23:55

there were only certain waves...

0:23:550:23:58

That the spring could vibrate, certain waves it could vibrate

0:23:580:24:01

and the reason it behaved like that is because it was trapped at both ends.

0:24:010:24:06

So this is what you would call, physicists would call

0:24:060:24:10

standing waves and you saw them appear on that spring.

0:24:100:24:13

Now, what has that got to do with empty atoms?

0:24:140:24:17

Well, just as this wave was trapped between Jim and Simon,

0:24:170:24:22

electrons are trapped inside atoms.

0:24:220:24:24

The positive electric charge of the nucleus effectively traps

0:24:240:24:29

the negatively-charged electron inside an atomic-sized box.

0:24:290:24:33

And when an electron is trapped,

0:24:330:24:34

just as the spring was trapped between Jim and Simon,

0:24:340:24:37

it exhibits the same kind of wave-like behaviour as the spring.

0:24:370:24:41

So now we're getting closer to understanding what's happening inside an atom.

0:24:410:24:46

But what do standing electron waves around a nucleus actually represent?

0:24:460:24:52

Well, the clue is that Jim and Simon had to put more energy in

0:24:520:24:55

to switch from one standing wave to another.

0:24:550:24:59

So it's tempting to think of those electron standing waves

0:24:590:25:03

as waves with different energies inside an atom,

0:25:030:25:08

waves that the different energies, the electron can have, if you like

0:25:080:25:11

when it's confined around a nucleus and this turns out to be correct.

0:25:110:25:16

But, just as there were only certain standing waves on the spring,

0:25:160:25:19

inside an atom, there are only certain energies that electrons can have.

0:25:190:25:24

Now, quantum theory allows physicists to calculate the shape

0:25:240:25:26

of the waves and therefore the allowed energies the electrons can have inside the atom.

0:25:260:25:32

And when you do the calculations, you find the lowest energy 'wave',

0:25:320:25:35

if you like, so I suppose this standing wave here

0:25:350:25:40

that can fit around the nucleus

0:25:400:25:42

has a wavelength of around 3 x 10­-10 metres.

0:25:420:25:46

Now, let me just write that down, because you might not be familiar with the notation.

0:25:460:25:49

It's 1, 2, 3, 4, 5, 6, 7, 8, 9...

0:25:490:25:53

0.0000000003 of a metre which sounds

0:25:530:25:58

unimaginably small, but it's enormous compared to the size

0:25:580:26:03

of the nucleus. It's actually about a quarter of a million times larger.

0:26:030:26:07

So that is why atoms are so big and yet so empty.

0:26:070:26:11

It's because electrons trapped around a nucleus

0:26:110:26:14

behave like waves - in this case standing waves - and there has to be

0:26:140:26:17

enough room to fit an electron wave around the atomic nucleus.

0:26:170:26:22

But that doesn't answer a very important question.

0:26:220:26:25

Now, we've shown why atoms are empty,

0:26:250:26:28

But we haven't yet explained

0:26:280:26:29

how they become so strongly bound together that they can create solid objects

0:26:290:26:34

like our beautiful million-pound diamond here.

0:26:340:26:37

Answer that, and we explain the structure of everything we see in the universe.

0:26:370:26:44

The early years of quantum theory were dominated by boy wonders,

0:26:490:26:53

people actually half my age, believe it or not.

0:26:530:26:56

So much so, that it became nicknamed "Knabenphysik",

0:26:560:27:00

which translated from German means "boy physics".

0:27:000:27:03

The key discovery was made by a man called Wolfgang Pauli.

0:27:030:27:07

Pauli published his first paper on Einstein's Theory of General Relativity when he was 18.

0:27:070:27:12

And his great contribution to quantum theory was made when he was only 24.

0:27:120:27:17

It's known as the Exclusion Principle.

0:27:170:27:20

We've seen that electrons can only exist in certain energy levels around the nucleus.

0:27:200:27:24

These energy levels, associated with the different standing waves.

0:27:240:27:29

Those energy levels correspond to standing waves that can fit in the atomic size box.

0:27:290:27:35

But the key point that Pauli realised

0:27:350:27:37

is that electrons can't all simply inhabit the lowest energy level.

0:27:370:27:42

Now, to a physicist, this should look a bit odd.

0:27:420:27:45

I mean, take this apple, for example.

0:27:450:27:48

If I lift the apple up, then I have to do work.

0:27:480:27:51

I give it energy to lift it up.

0:27:510:27:52

And if I let go, so I don't support it any more,

0:27:520:27:55

then it falls to the ground.

0:27:550:27:58

Now, the explanation of that, for a physicist,

0:27:580:28:00

is that the apple is falling into a lower-energy state.

0:28:000:28:04

Nature doesn't like to be in high-energy states.

0:28:040:28:07

It wants to cascade down into the lowest energy configuration that it can.

0:28:070:28:13

But the surprising thing is that electrons don't all live in that lowest energy level in an atom.

0:28:130:28:19

It turns out they're forbidden from doing so by an unbreakable law of nature.

0:28:190:28:24

That law is called the Pauli Exclusion Principle.

0:28:240:28:28

It's kind of like all of you sitting in these rows here.

0:28:280:28:30

You aren't allowed to all come down to the front row.

0:28:300:28:34

You can't all squash into the front seats, because there isn't room for you.

0:28:340:28:38

Electrons don't all occupy the lowest energy slots around an atom.

0:28:380:28:43

Instead, they fill each level up in order of increasing energy.

0:28:430:28:48

This might sound meaningless,

0:28:480:28:49

maybe it sounds a bit abstract.

0:28:490:28:51

But let me tell you that it isn't.

0:28:510:28:52

You see, Pauli's simple quantum rule is profoundly important.

0:28:520:28:56

In fact, it's the key to understanding chemistry.

0:28:560:29:00

But don't take my word for it. Time for another volunteer.

0:29:000:29:02

I know that James May kindly volunteered to take part in this.

0:29:020:29:07

He looks very worried, so maybe he was never asked! But anyway, James.

0:29:070:29:11

Now this is doubly amusing for me,

0:29:220:29:25

cos I know that you know exactly what's going to happen

0:29:250:29:29

because there's a canister of hydrogen gas there

0:29:290:29:31

and I know you're a keen aviator, so...

0:29:310:29:34

-You think about the story of the Hindenburg...

-Mmm!

-..while I...

0:29:340:29:37

-Which was unhappy, wasn't it?

-Oh, I get to wear the goggles?

-You might have to wear the goggles.

0:29:370:29:42

It's only a small safety thing, because it went wrong in rehearsal.

0:29:420:29:47

So what we're going to do is encourage a small chemical reaction to happen. What we're doing

0:29:470:29:52

is bubbling hydrogen through... Hydrogen gas through this, um...

0:29:520:29:55

-LAUGHTER

-..through this soap, here.

-Mmm.

0:29:550:29:59

What I'd like you to do... Actually, just wet your hands first. Just because it's a safety thing.

0:29:590:30:04

It stops your hands catching fire.

0:30:040:30:05

It actually... Perhaps roll your sleeves up a little bit.

0:30:050:30:09

You'll be all right. I'm sure you'll be fine.

0:30:090:30:11

So I'd like you to get - grab - some of that of that hydrogen in the soap bubbles.

0:30:110:30:16

Um...

0:30:170:30:19

-How's that?

-Don't look...

0:30:200:30:23

at what I'm doing.

0:30:230:30:25

What I'm going to do is I'm going to encourage a chemical reaction to happen...

0:30:250:30:33

from over here.

0:30:330:30:34

LAUGHTER

0:30:340:30:36

Whoa!

0:30:380:30:40

-Ow!

-You all right?

0:30:400:30:41

LAUGHTER AND APPLAUSE

0:30:410:30:45

LAUGHTER AND APPLAUSE DROWNS SPEECH

0:30:450:30:47

Thank you very much for putting yourself at great risk!

0:30:500:30:54

Thanks, James. That actually was a lot more fire than I was expecting! Sorry about that.

0:31:010:31:06

So what happened there?

0:31:060:31:08

What we did was we bubbled hydrogen gas into these bubbles.

0:31:080:31:12

James held them, and then I just gave them a little kick of energy

0:31:120:31:17

which encouraged them to react with oxygen in the air.

0:31:170:31:20

Now if draw the energy levels of oxygen,

0:31:200:31:23

then they look something like that.

0:31:230:31:25

They don't quite look as neat as when I drew the standing waves on the spring.

0:31:250:31:30

That's really because of the shape of the atomic box,

0:31:300:31:33

the shape of the box surrounding the oxygen nucleus.

0:31:330:31:36

Now oxygen has eight protons and eight neutrons in its nucleus,

0:31:360:31:41

which means it needs eight electrons filling up its energy levels.

0:31:410:31:45

And the electrons fill up the energy levels like that.

0:31:450:31:49

So you get three full energy levels

0:31:510:31:53

and two energy levels with a single electron in them.

0:31:530:31:57

Now that kind of makes oxygen a voracious consumer of electrons.

0:31:570:32:04

It would like, if it can -

0:32:040:32:06

it's energetically favourable for it to fill up those missing gaps.

0:32:060:32:09

Hydrogen has one proton,

0:32:090:32:13

and so it has one electron sat there in its lowest energy level.

0:32:130:32:17

Again, it has a space there. It would also like to fill that up.

0:32:170:32:21

So what happens, when I give it a little kick with this splint,

0:32:210:32:26

is that the hydrogen is encouraged to react with the with the oxygen.

0:32:260:32:31

It's energetically favourable for it to share its electron.

0:32:310:32:35

So the oxygen shares with the hydrogen,

0:32:350:32:36

the hydrogen shares with the oxygen.

0:32:360:32:38

There are two gaps, so you get two hydrogens which would like to react.

0:32:380:32:43

In doing so, the rearrangement of those electrons in the energy levels

0:32:430:32:47

is such a great giver of energy that you saw a flash.

0:32:470:32:50

All that flash that you saw, the little explosion, was energy being released

0:32:500:32:55

when the electrons in the hydrogen and the oxygen reconfigure -

0:32:550:33:00

just like the apple reconfigured itself

0:33:000:33:02

by dropping to the ground to get into the lowest energy state.

0:33:020:33:06

Two hydrogens, one oxygen. What does that make?

0:33:060:33:10

MAN: Water.

0:33:100:33:11

-ALL: Water!

-Right!

0:33:110:33:14

H2O.

0:33:140:33:17

So that is essentially the reason why we get chemistry.

0:33:170:33:22

Without Pauli's Exclusion Principle,

0:33:220:33:24

all the electrons would crowd down into the lowest energy level and there'd be no chemistry.

0:33:240:33:30

Which is worse than it sounds...

0:33:300:33:32

LAUGHTER

0:33:320:33:34

..because without chemistry, we'd have no magnificent structures in the universe,

0:33:370:33:42

like water, diamonds, or indeed, any of you.

0:33:420:33:47

Now, there's another consequence of the exclusion principle

0:33:470:33:51

that wasn't proved until 1967,

0:33:510:33:53

just one year before I was born.

0:33:530:33:55

Pauli's principle says that identical electrons

0:33:550:33:59

can't occupy the same energy level.

0:33:590:34:01

This is an absolute requirement.

0:34:010:34:03

So it also means that electrons will avoid each other at all costs.

0:34:030:34:07

And that, it was proved, is the actual reason

0:34:070:34:11

that I don't fall through the empty atoms that make up the floor.

0:34:110:34:15

That's ultimately what gives the illusion of solidity to the empty world of atoms.

0:34:150:34:21

And if you think a little bit more deeply about it,

0:34:210:34:24

then this throws up a bewildering conclusion, and it's this.

0:34:240:34:27

The Pauli Exclusion Principle applies to EVERY electron in the universe.

0:34:270:34:33

Not just every electron in a single atom, or a single molecule.

0:34:330:34:36

And this leads to a bizarre conclusion.

0:34:360:34:39

The particles that make up this diamond

0:34:390:34:41

are in communication with particles everywhere.

0:34:410:34:43

Inside all of you,

0:34:450:34:46

and inside the atoms in the furthest corners of the universe.

0:34:460:34:50

Let me explain that a little bit more. The Pauli Exclusion Principle

0:34:500:34:54

says no identical electrons can be in precisely the same energy level.

0:34:540:34:58

What if you have more than one atom?

0:34:580:35:00

For example, in this diamond

0:35:000:35:03

there are 3 million billion billion carbon atoms.

0:35:030:35:07

So this is a diamond-size box of carbon atoms.

0:35:070:35:10

And the Pauli Exclusion Principle still applies.

0:35:100:35:14

So all the energy levels

0:35:140:35:16

in all those 3 million billion billion atoms

0:35:160:35:18

have to be slightly different in order to ensure that

0:35:180:35:21

none of the electrons sit in precisely the same energy level.

0:35:210:35:25

Pauli's principle holds fast. But it doesn't stop with the diamond.

0:35:250:35:30

See, you can think of the whole universe as a vast box of atoms,

0:35:300:35:35

with countless numbers of energy levels

0:35:350:35:38

all filled by countless numbers of electrons.

0:35:380:35:42

So here's the amazing thing - the exclusion principle still applies,

0:35:420:35:46

so none of the electrons in the universe can sit in precisely

0:35:460:35:50

the same energy level.

0:35:500:35:52

But that must mean something very odd.

0:35:520:35:54

See, let me take this diamond, and let me just

0:35:540:35:57

heat it up a little bit between my hands.

0:35:570:35:59

Just gently warming it up,

0:35:590:36:01

putting a bit of energy into it, so I'm shifting the electrons around,

0:36:010:36:04

some of the electrons are jumping into different energy levels.

0:36:040:36:08

But this shift in the configuration of the electrons

0:36:080:36:11

inside the diamond has consequences, because the sum total

0:36:110:36:14

of all the electrons in the universe must respect Pauli.

0:36:140:36:19

Therefore, every electron, around every atom

0:36:190:36:22

in the universe, must be shifting as I heat the diamond up,

0:36:220:36:26

to make sure that none of them end up in the same energy level.

0:36:260:36:30

When I heat this diamond up, all the electrons across the universe

0:36:300:36:34

instantly but imperceptibly change their energy levels.

0:36:340:36:38

So everything is connected to everything else.

0:36:380:36:43

At the beginning, I promised I'd explain everything in the universe,

0:36:500:36:54

which I have in some way, but also I said that I'd give you

0:36:540:36:58

a deeper explanation of that wavy behaviour of the subatomic world.

0:36:580:37:03

So here it is. In my view, this is the deepest explanation we have,

0:37:030:37:06

and it's down to the Nobel Prize-winning physicist

0:37:060:37:09

Richard Feynman who, his colleague Freeman Dyson once described

0:37:090:37:12

as half genius, half buffoon but he subsequently, after having

0:37:120:37:15

worked with him for a while, changed that to all genius, all buffoon.

0:37:150:37:19

Let's go back to the double slit experiment, but now,

0:37:190:37:22

instead of just showing you the pattern...

0:37:220:37:24

This is Richard Feynman.

0:37:240:37:26

Instead of just showing you the pattern,

0:37:260:37:28

I want to show you how that pattern builds up.

0:37:280:37:30

Remember, we're firing electrons at two slits,

0:37:300:37:32

almost pouring them through two slits

0:37:320:37:34

and seeing what happened when they were detected on the other side.

0:37:340:37:38

Well, this is one electron at a time being fired through the slits

0:37:380:37:43

and hitting the screen, and building up in a pile.

0:37:430:37:46

Only when the one electron has gone through, was another one fired

0:37:460:37:49

and this is real data, again, a real movie of that happening

0:37:490:37:54

and you see the interference pattern.

0:37:540:37:56

Electrons, no electrons, electrons, no electrons.

0:37:560:37:59

The wavy-type interference pattern building up.

0:37:590:38:03

What could be happening there?

0:38:030:38:05

So, here it is again. Just electrons

0:38:050:38:07

and you see that what emerges is that wave-like behaviour.

0:38:070:38:10

So, you might have thought, "Well, I kind of understand

0:38:100:38:13

"what's going on with the double slits, there's loads of electrons

0:38:130:38:16

"piling through the slits and somehow there's some interference

0:38:160:38:19

"just like a big water wave and you build up the interference pattern."

0:38:190:38:23

Well, no, because this is one electron at a time,

0:38:230:38:27

so, what could possibly be happening?

0:38:270:38:29

Well, Feynman was a wonderfully intuitive, logical physicist.

0:38:290:38:34

No ordinary genius, he was often described as.

0:38:340:38:37

And he said this.

0:38:370:38:40

Here are the slits.

0:38:400:38:43

Here's the screen.

0:38:430:38:45

The electrons starts off here. What happens?

0:38:450:38:48

Well, obviously, the particle - electron - must go through a slit

0:38:480:38:51

and it must appear somewhere on the screen,

0:38:510:38:54

but it needs to be able to interfere with itself -

0:38:540:38:57

there've got to be regions on the screen where there are no electrons,

0:38:570:39:01

it's prevented from landing there,

0:39:010:39:02

so it must, at least, go through the other slit, as well,

0:39:020:39:06

and get to that point, and there must be some mechanism

0:39:060:39:09

for these paths interfering with each other, but why stop there?

0:39:090:39:14

See, that wouldn't be particularly logical.

0:39:140:39:16

Why only let it go through two paths?

0:39:160:39:18

Why not let it go through that path or maybe

0:39:180:39:21

some sort of path like that, or maybe like or maybe, indeed,

0:39:210:39:26

off here, out of this lecture theatre

0:39:260:39:29

and then maybe through Jonathan's head on its way...

0:39:290:39:33

I've got to say through Paul's foot, haven't I? Cos I just have to.

0:39:330:39:36

Paul Foot. I don't know - what a rubbish thing to say.

0:39:360:39:40

But, anyway, it could go through you, through Jonathan,

0:39:400:39:43

off up Oxford Street, up to Newcastle

0:39:430:39:46

indeed on to the Andromeda Galaxy

0:39:460:39:48

and back again, and land at this point on the screen.

0:39:480:39:51

Why not?

0:39:510:39:54

Why not allow the particle to travel along every possible path it can,

0:39:540:39:57

from one point to the other? And that is indeed what happens,

0:39:570:40:02

in the sense that's the way Feynman's theory works.

0:40:020:40:06

In principle, it's not too difficult.

0:40:060:40:08

You just have to calculate some quantity

0:40:080:40:10

associated with each path and find some mathematical machinery

0:40:100:40:14

from adding all those things up, and seeing whether or not they all

0:40:140:40:18

interfere together and disappear or appear when they land on the screen.

0:40:180:40:22

There is a formula that does that

0:40:220:40:24

and this is all I really need to say.

0:40:240:40:27

Let me turn it around. There it is.

0:40:270:40:30

Thank you and good... No, no, I won't say that!

0:40:300:40:32

This is called the Feynman path integral,

0:40:320:40:35

and this just says,

0:40:350:40:36

sum up over all the paths and calculate something

0:40:360:40:40

that will tell you the probability

0:40:400:40:42

of an electron going from one place to another.

0:40:420:40:44

Now, that might look a tremendous mess,

0:40:440:40:47

or it might look very simple and illuminating -

0:40:470:40:50

I suppose it depends on your point of view.

0:40:500:40:52

Probably a tremendous mess, granted.

0:40:520:40:55

But this formula is just a little machine,

0:40:550:40:57

I think that's a good way to think about it.

0:40:570:40:59

It that takes all the possible paths a particle can have,

0:40:590:41:02

it adds them up and it spits out the probability

0:41:020:41:05

that it'll end up at some particular place.

0:41:050:41:08

And that includes the particles that make up the diamond.

0:41:080:41:13

Now, for the moment, it's sat on its little cushion there.

0:41:130:41:17

Let me put it back in its box.

0:41:170:41:19

Now, Feynman's version of quantum theory tells us

0:41:210:41:24

something rather shocking.

0:41:240:41:26

This diamond is made up of atoms,

0:41:260:41:28

and the atoms are behaving according to quantum theory -

0:41:280:41:31

according to Feynman's equation.

0:41:310:41:33

In other words, they are all currently exploring the universe,

0:41:330:41:36

hopping around everywhere, exploring every possible path they can.

0:41:360:41:41

And that means this diamond is doing the same thing,

0:41:410:41:43

because it's made of atoms.

0:41:430:41:46

That means there is a finite chance that it will not

0:41:460:41:48

be inside this box at a later time - you can see where I'm going -

0:41:480:41:54

but it'll jump, completely out of its own accord,

0:41:540:41:59

without me touching it...and that's what I'm going to tell the judge!

0:41:590:42:03

But what's remarkable, is that I can calculate what the chance is

0:42:050:42:09

by using a simplified version of Feynman's formula.

0:42:090:42:15

And this is it.

0:42:150:42:17

See, just by doing a bit of maths, you can work that, simplify it,

0:42:170:42:21

and turn it into this...

0:42:210:42:23

which is an expression for the time you would have to wait,

0:42:230:42:27

on the average, to have a reasonable chance of it hopping

0:42:270:42:30

out of its box, and it goes like this.

0:42:300:42:34

OK, so, that is the distance we want it to hop,

0:42:370:42:42

that is the size of the box,

0:42:420:42:44

that's the mass of the diamond

0:42:440:42:46

and that's something called Planck's constant.

0:42:460:42:48

I'm going to need another volunteer here

0:42:480:42:50

because I'm going to actually do the maths

0:42:500:42:53

because I want to show you that you can do the sum quite simply

0:42:530:42:55

and I believe that Jonathan has kindly agreed

0:42:550:42:58

to do some sums, so, thank you.

0:42:580:43:01

-How's your maths?

-Well, you know, you know that's easy for me.

0:43:120:43:17

I do. That's why I asked you, actually.

0:43:170:43:20

We're going to do it,

0:43:200:43:21

so x - that's the distance we want the diamond to jump.

0:43:210:43:24

So let's say the box is about 5cm.

0:43:240:43:27

Let's say 6cm for x

0:43:270:43:31

and the mass of the diamond is 290-something carats -

0:43:310:43:36

-it's about 60g.

-Roughly, yes.

-An expert on diamonds, are you?

0:43:360:43:41

So, first of all, we just have to multiply those 3 numbers together.

0:43:410:43:45

6cm x 5cm x 60g.

0:43:450:43:48

Yeah. 6 x 5 x 6.

0:43:480:43:49

So 30 x 60. You just said 6!

0:43:490:43:53

60. 60g.

0:43:530:43:54

OK, 30 x 6 = 1,800.

0:43:540:43:57

Is that right? 60?

0:43:570:43:59

-It's heavy.

-It is. The BBC used to pay me in these.

0:43:590:44:03

LAUGHTER AND APPLAUSE

0:44:030:44:07

-I better take it back. I'm going to get...

-HE LAUGHS NERVOUSLY

0:44:120:44:17

-Then, though we get to this.

-Over the thing.

0:44:170:44:19

6.6 x 10­-34 kgm­2/s.

0:44:190:44:27

That is Planck's constant -

0:44:270:44:29

this is a fundamental constant of nature.

0:44:290:44:32

It's intrinsic to the way the universe is put together.

0:44:320:44:35

It's like the speed of light, like the strength of gravity.

0:44:350:44:39

It is THE fundamental THING -

0:44:390:44:40

constant, if you like - that sets the scale for quantum phenomena.

0:44:400:44:43

So, there's a slight issue here

0:44:430:44:46

because you see... You'll have noticed it.

0:44:460:44:48

The unit's are kilograms metres squared per second

0:44:480:44:50

and we calculated the 1,800 in cm and grams.

0:44:500:44:53

Which, by the way, I'm amazed I got that right!

0:44:530:44:56

So, first of all, we better another 10­-2 and a 10­-2 and a 10­-3 on,

0:44:560:45:01

-so it's 10­-7.

-Yeah.

0:45:010:45:04

So all you've got to do is divide that by that.

0:45:050:45:08

-All of that with that?

-Divide that by that roughly.

0:45:080:45:11

Roughly I don't even know if I can do...

0:45:110:45:15

That, for me... That's a kilogram? I don't even know. I do pounds!

0:45:200:45:25

-No, I've done the unit conversion for you - you've just got to divide.

-Where's the unit conversion?

0:45:250:45:30

1,800 x 10­-7 x 6.6 x 10...

0:45:300:45:33

I have no idea what you're doing and why you would want to do this to me!

0:45:330:45:36

Help him out, Jim.

0:45:360:45:38

Well you've got 10­-34 downstairs. Bring it upstairs

0:45:380:45:40

-and it becomes 10­34.

-Where do I put it? Up here?

0:45:400:45:43

Yeah, put it next to the 10...

0:45:430:45:46

-So then you've got 34 - 7.

-OK 34-7?

-Yeah.

-Yes, OK.

0:45:460:45:50

So that's 10­27.

0:45:500:45:52

-You've got about 10­3.

-I really... I'm so out of my depth.

0:45:520:45:57

This is the worst thing that's happened to me as an adult.

0:45:580:46:01

-You've got 10­27.

-OK.

0:46:020:46:04

Just for any children watching, I should say,

0:46:040:46:10

34 - 7 = 27

0:46:100:46:12

So you've got 10­27 and then we've got 6 and we've got 1,800,

0:46:120:46:16

so we've got to divide those things so we get about a 3 and another 100.

0:46:160:46:22

If you say so!

0:46:220:46:24

3 x 10­29...ish.

0:46:240:46:27

Once again, I am none the wiser. LAUGHTER

0:46:270:46:31

Why couldn't I have done James May's job where you just set fire to me?

0:46:310:46:36

And everyone went "Oooh!" And he's so happy he did that

0:46:360:46:41

and I'm now sweating.

0:46:410:46:44

-We're done.

-We've done it?

-Yeah, you see, this is what that number is you calculated.

0:46:440:46:49

See, we just put in the numbers divided by Planck's constant? What this number is

0:46:490:46:53

is the number of seconds you would have to wait on the average to have

0:46:530:46:57

a reasonable chance of the diamond hopping out of the box on its own.

0:46:570:47:00

I could have told you that's not going to happen without any of this.

0:47:000:47:03

LAUGHTER

0:47:030:47:05

I didn't need the sums. The diamond is safe in the box,

0:47:050:47:08

unless it's turned into a dead cat. That's the theory, isn't it?

0:47:080:47:11

I'll tell you what this is. Do you know roughly what that is?

0:47:110:47:14

-A nine?

-3 x 10­29?

-Why would I know? I'm an idiot!

0:47:140:47:18

-In years?

-That's about...

-Well, I'll tell you what it is. It is 600 billion times

0:47:180:47:23

the current age of the universe.

0:47:230:47:26

I don't know what to do. I'm just going to keep smiling at you.

0:47:260:47:29

-LAUGHTER Thank you for sharing that.

-Thank you.

0:47:290:47:33

Thanks.

0:47:350:47:38

Thanks, Jon.

0:47:430:47:45

The point of that... The point of that is to show that quantum theory doesn't just

0:47:460:47:52

apply to the inconceivably small world of the atom.

0:47:520:47:55

The same rules apply to you, to me, and the diamond.

0:47:550:47:59

It's just that for objects out here in the familiar world,

0:47:590:48:03

like the diamond, we don't usually see quantum effects.

0:48:030:48:06

The reason for that is the smallness of Planck's constant. We had quite a big number here,

0:48:060:48:11

but we had to divide it by an extremely small number in order

0:48:110:48:15

to work out the time we'd have to wait and that's why that's big.

0:48:150:48:19

See, if that was one or something like that, then we wouldn't have had to wait many seconds -

0:48:190:48:23

about 1,800 seconds or something like that, for the diamond to hop out of the box.

0:48:230:48:27

So it's Planck's constant, this fundamental constant of nature

0:48:270:48:30

that means that quantum theory is rather unfamiliar

0:48:300:48:34

because it applies to small things, because Planck's constant is small.

0:48:340:48:39

Now you could theoretically make the diamond jump sooner.

0:48:390:48:43

Look again at this equation.

0:48:430:48:45

One way to do it, as I've said, would be to make Planck's constant very big,

0:48:450:48:49

but you can't do that. It's a fundamental constant of nature. What you could do, though,

0:48:490:48:53

is you could shrink the size of the box, this delta x here.

0:48:530:48:57

If I made the box smaller and smaller and smaller,

0:48:570:49:01

I'd make the time I had to wait for it to jump out of the box smaller and smaller and smaller.

0:49:010:49:07

So this equation says that the more we know the position

0:49:070:49:11

of something, the position of this diamond in the box, let's say,

0:49:110:49:15

then the more likely it is for the diamond to jump out of the box.

0:49:150:49:19

Now this is known as Heisenberg's Uncertainty Principle -

0:49:190:49:23

the more you try to pin down a particle's position by trapping it

0:49:230:49:27

in a smaller and smaller box, the more likely it is to jump around.

0:49:270:49:31

You might have come across Heisenberg's Uncertainty Principle.

0:49:310:49:35

It's one of the most famously misunderstood

0:49:350:49:37

and misrepresented parts of quantum theory.

0:49:370:49:40

It says, precisely, that the more precisely you know

0:49:400:49:44

a particle's position, the less certain you can be of its momentum.

0:49:440:49:49

And you can see that it emerged... I derived it from a fundamental equation.

0:49:490:49:54

It's not complete nonsense. I didn't make it up.

0:49:540:49:57

It's often misrepresented by what I would call "mischievous hippies"

0:49:570:50:01

to mean that physicists are rubbish at their job

0:50:010:50:04

or that the equipment is no good and we're unable to measure

0:50:040:50:07

two things about a particle with any accuracy.

0:50:070:50:10

But Heisenberg's Uncertainty Principle is a consequence

0:50:100:50:13

of the laws of quantum theory. It emerges

0:50:130:50:15

from Feynman's equation. It has nothing to do with any of that wishy-washy, drivelly nonsense.

0:50:150:50:21

In that spirit, I want to show you that rather than restricting our knowledge of the natural world,

0:50:210:50:26

Heisenberg can actually widen it.

0:50:260:50:30

In fact, this rule about the unimaginably small particles

0:50:300:50:34

can explain some of the most massive and spectacular objects in the universe.

0:50:340:50:39

I'm going to end

0:50:420:50:44

by explaining how everything I've told you this evening

0:50:440:50:47

predicts the existence of diamonds bigger than this -

0:50:470:50:51

in fact, bigger than this lecture theatre.

0:50:510:50:53

In fact, diamonds as big as a planet and as massive as a star.

0:50:530:50:59

Now to understand how this can be, we need to understand something

0:50:590:51:03

about the life cycles of the stars themselves.

0:51:030:51:06

Stars are big clumps of matter collapsing under their own gravity.

0:51:060:51:09

As they collapse, they heat up and they set off a chain reaction

0:51:090:51:12

of nuclear fusion reactions where the nuclei of hydrogen

0:51:120:51:16

fuse together, initially to form helium, and eventually they fuse

0:51:160:51:21

to form carbon and oxygen and all the heavy elements up to and including iron.

0:51:210:51:26

That's where the heavy elements come from in the universe.

0:51:260:51:30

In this process, vast amounts of energy are released.

0:51:300:51:33

That energy creates a pressure that holds the star up

0:51:330:51:36

and prevents it from collapsing.

0:51:360:51:38

The stars don't have infinite amounts of fuel

0:51:380:51:41

and eventually those fusion reactions must cease.

0:51:410:51:44

In five billion years, this will happen to our sun.

0:51:440:51:47

It'll stop generating enough energy to prevent its own collapse

0:51:470:51:50

and so it will collapse.

0:51:500:51:53

By the end of their lives, stars like our sun have converted all the hydrogen in their cores

0:51:530:51:58

and mainly they've converted it into oxygen and carbon.

0:51:580:52:03

Now remember that those carbon atoms,

0:52:030:52:06

just like those in our diamond, are almost entirely empty space,

0:52:060:52:10

so you might expect that the space can be squashed and compressed almost out of existence

0:52:100:52:15

as the dying star collapses.

0:52:150:52:17

But as the star collapses and becomes denser,

0:52:170:52:20

its electrons get closer and closer together.

0:52:200:52:24

Finally, they're so close that they try to occupy the same volume of space as each other.

0:52:240:52:30

Then Pauli's Exclusion Principle steps in,

0:52:300:52:33

because the electrons cannot occupy the same bit of space -

0:52:330:52:37

they are unable to overlap, so they try to arrange themselves

0:52:370:52:43

such that they have as much space as they possibly can.

0:52:430:52:45

And you might imagine them as being alone inside little boxes like this

0:52:450:52:49

and the boxes shrink and shrink and shrink as the star collapses.

0:52:490:52:55

But then, as the electrons become more and more confined,

0:52:550:52:58

Heisenberg's Uncertainty Principle comes into play. As the electrons' boxes get smaller and smaller,

0:52:580:53:04

their tendency to hop out of the box becomes greater and greater,

0:53:040:53:08

so you can think of it that they are frantically vibrating

0:53:080:53:11

around faster and faster inside these boxes of ever-decreasing size.

0:53:110:53:16

This quantum jiggling exerts a pressure, which stops

0:53:160:53:20

the star from collapsing any further, leaving something called

0:53:200:53:23

a white dwarf star, which is a densely-packed dead star the size of the Earth

0:53:230:53:28

but the mass of our sun, and a million times more dense than water.

0:53:280:53:33

White dwarfs are so dense that if I were to stand on their surface

0:53:330:53:37

the gravitational pull would make me weigh something like 30,000 tonnes.

0:53:370:53:43

White dwarfs are strange objects indeed.

0:53:430:53:45

But here is the final triumph, I think, of quantum theory.

0:53:450:53:49

It is the most powerful example I know of its power to predict how the natural world behaves.

0:53:490:53:55

See, it predicts the existence of these strange stars of white dwarfs.

0:53:550:54:01

But it does more than that.

0:54:010:54:03

In the 1930s, the physicist Subrahmanyan Chandrasekhar

0:54:030:54:06

used quantum theory to predict the maximum mass

0:54:060:54:09

of a lump of matter that can be held up by the exclusion pressure of electrons

0:54:090:54:14

to form a white dwarf. He just used the uncertainty principle, essentially,

0:54:140:54:18

and the exclusion principle.

0:54:180:54:20

He found that there should be no stars of this type

0:54:200:54:23

with masses greater than 1.4 times the mass of our sun.

0:54:230:54:26

Now to date, astronomers have found tens of thousands of white dwarf stars

0:54:260:54:32

and they have found that not one in the sky exceeds the maximum mass

0:54:320:54:38

calculated by Chandrasekhar using the simple laws of quantum theory.

0:54:380:54:43

And in amongst those stars, astronomers have found something that I think is quite extraordinary.

0:54:430:54:48

Now that diamond is 296 carats.

0:54:480:54:51

In the heart of this constellation, Centaurus, which is a few tens of light years away,

0:54:510:54:57

they've detected a white dwarf star with the wonderful name BPM 37093(!)

0:54:570:55:03

-LAUGHTER

-As it died and cooled, the carbon within the core crystallised.

0:55:030:55:09

So BPM 37093, which is somewhere around there, became a diamond,

0:55:090:55:18

just like this, but of ten billion trillion trillion carats.

0:55:180:55:21

LAUGHTER

0:55:210:55:23

We understand in detail why such a thing can exist.

0:55:230:55:27

That's a diamond, light years away, intimately connected to this diamond,

0:55:270:55:33

and indeed, intimately connected to everything else

0:55:330:55:35

in the universe, by the laws of quantum physics.

0:55:350:55:38

What a remarkable testament to the power of the wavy behaviour of electrons,

0:55:380:55:43

and what a spectacular demonstration of the effectiveness of quantum theory.

0:55:430:55:47

Quantum theory is a uniquely potent tool that gives us

0:55:470:55:51

our best understanding of how the inconceivably small

0:55:510:55:55

can give rise to the inconceivably large.

0:55:550:55:57

It is THE most accurate way that we currently possess

0:55:570:56:01

to understand our universe.

0:56:010:56:03

It explains how atoms are empty yet solid,

0:56:030:56:06

how the wave-like behaviour of electrons creates the hardest known substances,

0:56:060:56:11

and how the real world emerges from subatomic particles

0:56:110:56:15

that explore the universe, the entire universe, in an instant.

0:56:150:56:20

There's nothing strange, there's nothing weird, there's no woo-woo.

0:56:200:56:25

It is just beautiful physics. Thank you.

0:56:250:56:28

APPLAUSE

0:56:280:56:32

It was mind-blowing.

0:56:490:56:51

I couldn't... Some of it I could understand,

0:56:510:56:55

other parts I could not understand. It was so exciting. I loved it.

0:56:550:56:58

I love listening to him because he does makes things clear.

0:56:580:57:02

He speaks at just the right pace for me to absorb it

0:57:020:57:04

and also he's got that very winning smile, so even though

0:57:040:57:07

he does insist on telling us how soon it is that the sun's going to die out

0:57:070:57:11

and we will all die screaming and flying off into the inky void of space,

0:57:110:57:15

you don't mind it because he looks so sweet when he tells you.

0:57:150:57:18

What do you now think of quantum physics?

0:57:180:57:20

I feel like I maybe should have stuck in at school a little bit more,

0:57:200:57:24

but you know, the career that I've chosen is going well, so...

0:57:240:57:29

But I have learnt a lot - mainly "don't volunteer for things"!

0:57:290:57:34

How are your hands now?

0:57:340:57:36

My hands are fine. All it does is singe the very fine hairs on the back.

0:57:360:57:41

But I was getting a bit, you know, gorilla-ish anyway, so he's probably done me a favour.

0:57:410:57:46

It was great. I loved it. It was fantastic. It was almost exactly about everything

0:57:460:57:50

I think about all the time.

0:57:500:57:51

Subtitles by Red Bee Media Ltd

0:58:130:58:15

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0:58:150:58:17

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