
Browse content similar to A Night with the Stars. Check below for episodes and series from the same categories and more!
| Line | From | To | |
|---|---|---|---|
Where's the reception? Oh, OK... | 0:00:02 | 0:00:03 | |
So nobody knows what this lecture is going to be about... | 0:00:03 | 0:00:06 | |
I know what it's about. It'll be about science, and he'll be promoting that heresy of his. | 0:00:06 | 0:00:11 | |
I hope he's going to unveil a death ray. I don't know. | 0:00:11 | 0:00:14 | |
I'm going to make one, at least one unsuspecting celebrity, do sums. | 0:00:16 | 0:00:20 | |
-I really am so out of my depth... -LAUGHTER | 0:00:20 | 0:00:23 | |
This is the worst thing that's happened to me as an adult. | 0:00:23 | 0:00:26 | |
The only thing I do know is that I've been roped in to go up | 0:00:26 | 0:00:29 | |
on stage - with Simon Pegg, no less - waving a rope about. | 0:00:29 | 0:00:34 | |
I can see why you've got no hair. | 0:00:34 | 0:00:36 | |
LAUGHTER | 0:00:36 | 0:00:37 | |
I'm so thrilled to have been asked, to be honest. | 0:00:39 | 0:00:42 | |
I never do clever things. | 0:00:42 | 0:00:44 | |
There's a real buzz in this room, and it just makes me feel proud to be a scientist in this day and age. | 0:00:44 | 0:00:50 | |
Perhaps tonight is my chance | 0:00:50 | 0:00:53 | |
to realise what it's all about, and have a big sort of Damascene moment. | 0:00:53 | 0:00:57 | |
I'd like to ask Professor Brian Cox about his hair - it's a shared interest. | 0:00:57 | 0:01:02 | |
-I hope he blows some stuff up. -Whoa... Ow! | 0:01:02 | 0:01:06 | |
I'm hoping it's going to start simple, for people like me, | 0:01:06 | 0:01:09 | |
and then get slowly more complicated. | 0:01:09 | 0:01:13 | |
Because otherwise, if my brain starts swelling inside my skull | 0:01:13 | 0:01:17 | |
it's just going to pop and I'll distract people. | 0:01:17 | 0:01:19 | |
Thank you. | 0:01:44 | 0:01:45 | |
Welcome to the Royal Institution of Great Britain, established | 0:01:46 | 0:01:50 | |
in 1799 as "an institution for diffusing knowledge", | 0:01:50 | 0:01:54 | |
and perhaps the most iconic lecture theatre in science. | 0:01:54 | 0:01:59 | |
Thomas Huxley championed Charles Darwin's theory of evolution here, | 0:01:59 | 0:02:04 | |
Michael Faraday pioneered our understanding of electricity and magnetism here, | 0:02:04 | 0:02:08 | |
and on this stage he demonstrated the first electric motor. | 0:02:08 | 0:02:13 | |
And the great scientist and lecturer Sir Humphry Davy, | 0:02:13 | 0:02:16 | |
who was also the first director of the Royal Institution | 0:02:16 | 0:02:19 | |
and one of my heroes, spoke here many times. | 0:02:19 | 0:02:22 | |
And he gave the best explanation of the absolute need to do science that I know of - | 0:02:22 | 0:02:28 | |
"Nothing is so fatal to the progress of the human mind | 0:02:28 | 0:02:31 | |
"as to suppose that our views of science are ultimate; | 0:02:31 | 0:02:34 | |
"that there are no mysteries in nature; | 0:02:34 | 0:02:36 | |
"that our triumphs are complete, | 0:02:36 | 0:02:38 | |
"and that there are no new worlds to conquer." | 0:02:38 | 0:02:41 | |
Well, tonight I want to talk about one of the great mysteries, | 0:02:41 | 0:02:45 | |
pillars of our understanding of nature - | 0:02:45 | 0:02:47 | |
the scientific theory that underpins much of the technology | 0:02:47 | 0:02:51 | |
we take for granted in the 21st century, | 0:02:51 | 0:02:53 | |
yet retains its reputation for obscure difficulty and bizarre predictions. | 0:02:53 | 0:02:59 | |
Now, by the time I've finished, I hope that | 0:02:59 | 0:03:01 | |
while your view of reality might have shifted a little, | 0:03:01 | 0:03:05 | |
you'll understand a bit more about how the universe works. | 0:03:05 | 0:03:08 | |
Now, let's start with the contents of this box. | 0:03:08 | 0:03:13 | |
This is a rough diamond. It's worth well over £1 million. | 0:03:15 | 0:03:22 | |
It costs so much because it's rare, and because it's beautiful. | 0:03:22 | 0:03:27 | |
But there's a different kind of beauty here, a more profound | 0:03:27 | 0:03:30 | |
kind of beauty - less superficial, but perhaps far more instructive. | 0:03:30 | 0:03:36 | |
A diamond is one of the hardest known substances - | 0:03:36 | 0:03:39 | |
which is why diamonds are widely used industrially - | 0:03:39 | 0:03:41 | |
but light can stream through it relatively unimpeded. | 0:03:41 | 0:03:46 | |
So there's beauty in a question, which is, | 0:03:46 | 0:03:49 | |
how can something be so ethereal, and yet be | 0:03:49 | 0:03:52 | |
so hard that it can drill through solid rock? | 0:03:52 | 0:03:55 | |
Well, to answer that we need to know about the | 0:03:55 | 0:03:58 | |
structure of the diamond - indeed the structure of all matter itself. | 0:03:58 | 0:04:02 | |
And the best theory we have to describe matter, is quantum theory. | 0:04:02 | 0:04:08 | |
Now, I understand why quantum theory can seem a bit odd. | 0:04:08 | 0:04:12 | |
It makes odd statements. | 0:04:12 | 0:04:13 | |
It says, for example, that things can be many places at once - | 0:04:13 | 0:04:17 | |
in fact, technically it says things can be in an infinite number of places at once. | 0:04:17 | 0:04:22 | |
It says that subatomic building blocks of our bodies | 0:04:22 | 0:04:25 | |
are constantly shifting in response to events that happened at the edge | 0:04:25 | 0:04:30 | |
of the known universe - a billion light years somewhere over there. | 0:04:30 | 0:04:34 | |
Now, this is all true, but that isn't a licence to talk utter drivel. | 0:04:34 | 0:04:40 | |
LAUGHTER | 0:04:40 | 0:04:42 | |
See, quantum theory might SEEM weird and mysterious, but it describes the | 0:04:42 | 0:04:46 | |
world with higher precision than the laws of physics laid down by Newton, | 0:04:46 | 0:04:50 | |
and it's one of the foundations of our modern understanding of nature. | 0:04:50 | 0:04:54 | |
It doesn't, therefore, allow mystical healing, | 0:04:54 | 0:04:57 | |
or ESP or any other manifestation of New Age woo-woo | 0:04:57 | 0:05:01 | |
into the pantheon of the possible. | 0:05:01 | 0:05:03 | |
Always remember, quantum theory is physics, and physics is | 0:05:03 | 0:05:07 | |
usually done by people without star signs tattooed on their bottom. | 0:05:07 | 0:05:11 | |
What makes quantum theory a good scientific theory? | 0:05:11 | 0:05:15 | |
Well, it makes predictions that can be tested against experiment, | 0:05:15 | 0:05:19 | |
and when we test those predictions we find that they agree with observation. | 0:05:19 | 0:05:24 | |
This means quantum theory is not wrong - it's a survivor, | 0:05:24 | 0:05:29 | |
if you like, because it's been put to the test over and over again, | 0:05:29 | 0:05:32 | |
and consistently been found to make correct predictions. | 0:05:32 | 0:05:35 | |
If this changes, then we'll search for a new theory - | 0:05:35 | 0:05:38 | |
there are NO absolute truths in science. | 0:05:38 | 0:05:40 | |
This is how we make scientific progress, and this is how | 0:05:40 | 0:05:43 | |
everything in the world that you take for granted was delivered. | 0:05:43 | 0:05:47 | |
So, remember that however odd it might seem, tonight | 0:05:47 | 0:05:52 | |
I'm going to show you, hopefully, that quantum theory works. | 0:05:52 | 0:05:56 | |
So, I want to explain quantum theory to you in the simplest way that I can. | 0:05:56 | 0:06:01 | |
Ultimately, I'll show you how it gives us insight into the | 0:06:01 | 0:06:03 | |
fundamental building blocks of the universe, and explains the existence | 0:06:03 | 0:06:07 | |
of some of the most spectacular phenomena out there in deep space. | 0:06:07 | 0:06:12 | |
And I'm going to do this now because if I don't point wistfully at the sky at least once, | 0:06:12 | 0:06:16 | |
some of my viewers will get annoyed, so there you go. | 0:06:16 | 0:06:19 | |
That's the only mountain-top pose I'm going to pull... | 0:06:19 | 0:06:23 | |
-LAUGHTER -..so, to begin... | 0:06:23 | 0:06:25 | |
No helicopters tonight. | 0:06:29 | 0:06:31 | |
To begin, let's zoom into the heart of this diamond. | 0:06:31 | 0:06:36 | |
What I've got here is a sequence of actual photographs of, well, | 0:06:36 | 0:06:39 | |
initially the surface of a diamond, but these photographs | 0:06:39 | 0:06:42 | |
have been taken by a series of increasingly powerful microscopes. | 0:06:42 | 0:06:47 | |
So as we zoom in you see that at first you're seeing a more | 0:06:47 | 0:06:49 | |
detailed picture of the structure of the surface of the diamond. | 0:06:49 | 0:06:53 | |
But as we go right in, you see that a regular pattern, | 0:06:53 | 0:06:55 | |
a regular structure emerges, | 0:06:55 | 0:06:58 | |
so this is an electron microscope photograph of diamond. | 0:06:58 | 0:07:02 | |
And what you're looking at here actually are carbon atoms, | 0:07:02 | 0:07:05 | |
individual atoms. | 0:07:05 | 0:07:07 | |
You see that they appear to be in a kind of a dumbbell shape, and there's a space | 0:07:07 | 0:07:11 | |
and another pair, because you're looking at a two-dimensional image. | 0:07:11 | 0:07:15 | |
But if you take that to three dimensions | 0:07:15 | 0:07:17 | |
and look at this - this is the structure of diamond, | 0:07:17 | 0:07:21 | |
and what you can see is carbon atoms surrounded by four other | 0:07:21 | 0:07:26 | |
carbon atoms, in a regular, beautiful crystalline structure. | 0:07:26 | 0:07:30 | |
Now, in this diamond, this over- a-million-pound piece of diamond, | 0:07:30 | 0:07:35 | |
there are something like 3 million billion billion atoms, | 0:07:35 | 0:07:39 | |
and they are laid out in precisely this beautifully simple way. | 0:07:39 | 0:07:45 | |
I should say, actually, this diamond is as it was when it was found, | 0:07:45 | 0:07:48 | |
so this hasn't been cut. It was found in South Africa well over 100 years ago, | 0:07:48 | 0:07:52 | |
and it's 3 billion years old. | 0:07:52 | 0:07:55 | |
And that structure, its diamond shape - | 0:07:55 | 0:07:57 | |
that's how it naturally appeared, because its structure | 0:07:57 | 0:08:01 | |
is like this, it's built out of carbon atoms exactly like that. | 0:08:01 | 0:08:05 | |
Carbon atoms can't be packed any more tightly together than this. | 0:08:05 | 0:08:09 | |
That's what makes diamonds so tough, and allows them | 0:08:09 | 0:08:12 | |
to cut through virtually anything. | 0:08:12 | 0:08:15 | |
Which makes what I'm about to say quite remarkable. | 0:08:15 | 0:08:17 | |
See, the atoms that make up this diamond - | 0:08:17 | 0:08:21 | |
and pretty much everything else for that matter - are virtually empty. | 0:08:21 | 0:08:24 | |
Now, what do I mean by that? Well, what is an atom? | 0:08:26 | 0:08:30 | |
Well, about 100 years ago now, in the greatest city | 0:08:30 | 0:08:34 | |
known to civilization - which is Manchester! - | 0:08:34 | 0:08:38 | |
APPLAUSE | 0:08:38 | 0:08:39 | |
..Ernest Rutherford discovered that the atom consists of an atomic nucleus, | 0:08:41 | 0:08:45 | |
which is made of particles called protons and neutrons tightly packed together, | 0:08:45 | 0:08:49 | |
and a third kind of particle, | 0:08:49 | 0:08:52 | |
called electrons, orbit somewhere or exist somewhere around the outside. | 0:08:52 | 0:08:57 | |
The nucleus protons are positively charged, | 0:08:57 | 0:08:59 | |
the neutrons are neutral, so it has a positive charge. | 0:08:59 | 0:09:02 | |
The electrons somewhere out here have a negative charge, | 0:09:02 | 0:09:06 | |
and as Faraday would have talked about on this very stage | 0:09:06 | 0:09:10 | |
just under 200 years ago, there is a force that holds | 0:09:10 | 0:09:12 | |
the electron to the nucleus, | 0:09:12 | 0:09:14 | |
because they're both electrically charged. | 0:09:14 | 0:09:17 | |
So that's kind of a sketch, a schematic view of the atom. | 0:09:17 | 0:09:20 | |
We've known that now for around a hundred years. | 0:09:20 | 0:09:24 | |
Protons, neutrons and electrons. | 0:09:24 | 0:09:25 | |
These three particles make up not only the diamond, | 0:09:25 | 0:09:29 | |
but everything we can touch, every structure we can see. | 0:09:29 | 0:09:33 | |
Everything is made up of these same three absolutely identical particles. | 0:09:33 | 0:09:38 | |
So the richness of the natural world, everything on planet Earth, | 0:09:38 | 0:09:41 | |
everything we can see beyond is described by a simple recipe | 0:09:41 | 0:09:45 | |
that determines how these simple particles combine together. | 0:09:45 | 0:09:49 | |
Now, clearly physicists don't call it a recipe, we call that quantum theory. | 0:09:49 | 0:09:54 | |
Now, one of the first great challenges for quantum theory - | 0:09:54 | 0:09:57 | |
indeed, one of the reasons it was developed at the turn of the 20th century, | 0:09:57 | 0:10:01 | |
in Manchester and a few other places - was to understand precisely how these particles | 0:10:01 | 0:10:06 | |
come together to create this diamond, you, me and everything else. | 0:10:06 | 0:10:10 | |
And a hundred years after its discovery, it still provides | 0:10:10 | 0:10:13 | |
our best understanding of the structure of matter. | 0:10:13 | 0:10:17 | |
And admittedly, yes, it is still a bit strange. | 0:10:17 | 0:10:20 | |
Now, one of the particularly strange things about it is the behaviour of electrons inside atoms. | 0:10:20 | 0:10:27 | |
See, these imperceptibly tiny electrons spend | 0:10:27 | 0:10:29 | |
the overwhelming majority of their time in far distant clouds. | 0:10:29 | 0:10:33 | |
So between the nucleus and the electron there is a vast emptiness. | 0:10:33 | 0:10:38 | |
If I were a nucleus, and I perched on the edge of the White Cliffs of Dover, | 0:10:38 | 0:10:42 | |
then the fuzzy edge of the electron cloud would be | 0:10:42 | 0:10:45 | |
somewhere in the farms of northern France. | 0:10:45 | 0:10:48 | |
Looking out towards the electrons I'd see nothing but empty, interatomic space. | 0:10:48 | 0:10:53 | |
So atoms are vast, and they are empty. Actually about - | 0:10:53 | 0:10:56 | |
I've got to count this on my fingers - | 0:10:56 | 0:10:58 | |
99.9999999999999% empty. | 0:10:58 | 0:11:04 | |
That's 13 nines. So, you buy this diamond, | 0:11:04 | 0:11:09 | |
and you're buying about a million quid's worth of mainly empty space, and since | 0:11:09 | 0:11:13 | |
everything is made of atoms, that means you are vast and empty too. | 0:11:13 | 0:11:19 | |
LAUGHTER | 0:11:19 | 0:11:21 | |
Especially you... No, I can't say that, can I? | 0:11:21 | 0:11:24 | |
Never say that to a stand-up comic - what am I doing? | 0:11:24 | 0:11:29 | |
Anyway, if I squeezed all the space out of all the atoms in all | 0:11:29 | 0:11:31 | |
the people on the planet, then you'd be able to fit the whole | 0:11:31 | 0:11:35 | |
of humanity into that diamond, and that's how empty matter is. | 0:11:35 | 0:11:40 | |
So, understanding why atoms are empty and yet so solid, | 0:11:40 | 0:11:44 | |
why light can stream through that diamond, and yet | 0:11:44 | 0:11:48 | |
it sits nicely on the predominantly empty cushion and the predominantly empty floor, | 0:11:48 | 0:11:52 | |
is therefore a prerequisite to understanding the structure of everything in nature. | 0:11:52 | 0:11:58 | |
Now, you might have gathered that the world inside an atom | 0:11:58 | 0:12:00 | |
must be a strange place where things don't behave | 0:12:00 | 0:12:03 | |
much like they appear to behave here in the macroscopic world. | 0:12:03 | 0:12:07 | |
Well, there's one historic experiment | 0:12:07 | 0:12:09 | |
which contains everything you need to know about the bizarre way | 0:12:09 | 0:12:12 | |
that particles behave, and therefore why atoms are the way that they are. | 0:12:12 | 0:12:17 | |
I'm going to need a helping hand for this, | 0:12:17 | 0:12:20 | |
and I know that Sarah Millican has volunteered kindly to help me. | 0:12:20 | 0:12:25 | |
-Where's Sarah? -I'm here. Hello. -So Sarah - would you mind...? | 0:12:25 | 0:12:28 | |
Thanks, Sarah. Did you do a science degree, by the way? | 0:12:38 | 0:12:42 | |
No. I've already been asked that by somebody in the audience - | 0:12:42 | 0:12:45 | |
"Did you study physics?" | 0:12:45 | 0:12:46 | |
No, I just sort of gave up after GCSE - is that a problem, | 0:12:46 | 0:12:50 | |
-should I go back to me seat? -LAUGHTER | 0:12:50 | 0:12:53 | |
-Any other volunteers(?) No... -Only got a C! | 0:12:53 | 0:12:56 | |
So you may or may not have heard of the double slit experiment, it's something every physics student... | 0:12:56 | 0:13:02 | |
-I've heard of it, but it was something different. -Was it(?) | 0:13:02 | 0:13:05 | |
-Well, we're going to... -LAUGHTER | 0:13:05 | 0:13:08 | |
Every physicist is taught this the moment they step through the doors of a university. | 0:13:08 | 0:13:13 | |
It's simple, and it demonstrates the paradoxical world of quantum particles. | 0:13:13 | 0:13:18 | |
So first of all we're going to do it - we're going to do it twice, or even three times. | 0:13:18 | 0:13:22 | |
So I'm going to give you this bucket of sand, which is quite heavy actually. | 0:13:22 | 0:13:27 | |
These are particles of sand, little bits of sand. They're probably your picture, | 0:13:27 | 0:13:32 | |
I suppose, of what a particle might be, a little piece of matter. | 0:13:32 | 0:13:37 | |
So what I'm going to ask you to do is just pour the sand | 0:13:37 | 0:13:40 | |
onto this piece of board, which has got two slits cut in it, | 0:13:40 | 0:13:42 | |
and I suppose before I do it... | 0:13:42 | 0:13:45 | |
-Oh, you bugger! -It's a bit heavy! -It is. | 0:13:45 | 0:13:47 | |
You pour it first, then I'll ask you what you think might happen. | 0:13:47 | 0:13:50 | |
Yeah, let's chat for a while, while I'm holding the bucket(!) | 0:13:50 | 0:13:54 | |
It weighs a ton, doesn't it? So just pour it through the slits... | 0:13:54 | 0:13:57 | |
Now, what do you think is going to happen? | 0:13:57 | 0:14:00 | |
So we're just pouring particles of sand over the slits. | 0:14:00 | 0:14:05 | |
Just keep going... | 0:14:05 | 0:14:07 | |
So there we are. That'll do, I think. | 0:14:09 | 0:14:12 | |
So if I remove that... what does that remind you of? | 0:14:12 | 0:14:17 | |
LAUGHTER | 0:14:17 | 0:14:19 | |
I feel like smacking it - does that help? | 0:14:19 | 0:14:22 | |
Pour that sand into there. So that's probably pretty much... | 0:14:22 | 0:14:27 | |
-There you go, you can put it down now. -Thank you! | 0:14:27 | 0:14:30 | |
That's probably pretty much, I suppose, what you expected would happen. | 0:14:30 | 0:14:34 | |
The sand has just fallen through the slits, | 0:14:34 | 0:14:36 | |
and beneath each slit there's a bigger pile of sand. | 0:14:36 | 0:14:39 | |
Particles fall through slits - pretty obvious. | 0:14:39 | 0:14:42 | |
But...this is a picture of real data. | 0:14:42 | 0:14:46 | |
So this is real experimental data, | 0:14:46 | 0:14:48 | |
of electrons essentially being poured through two slits, so it's electrons | 0:14:48 | 0:14:52 | |
being fired at two slits, and then there's a screen there, and so what | 0:14:52 | 0:14:57 | |
you're seeing are just piles of electrons, so the white spots | 0:14:57 | 0:15:00 | |
really are where electrons hit the screens - | 0:15:00 | 0:15:02 | |
there's a pile, and then there's nothing, | 0:15:02 | 0:15:04 | |
and then there's a pile, and then there's nothing... | 0:15:04 | 0:15:07 | |
Looks nothing like that. But the experiment was the same - | 0:15:07 | 0:15:10 | |
it really is electrons being poured through two slits | 0:15:10 | 0:15:14 | |
onto a screen, and you get that strange pattern. | 0:15:14 | 0:15:17 | |
So, let me show you this, which is a different version of the same experiment. | 0:15:18 | 0:15:24 | |
Now, this is a tank of water, so there's some water in there, | 0:15:24 | 0:15:29 | |
and as you can see there's just a bar that's vibrating up and down, | 0:15:29 | 0:15:33 | |
-and then there's two slits. -Yeah. -So you can see the two slits there. | 0:15:33 | 0:15:38 | |
And if you come round here... you can see the screen here. | 0:15:38 | 0:15:44 | |
So there's the two slits, and these are the waves of water. | 0:15:44 | 0:15:47 | |
So there's a flat wave of water hitting the two slits, | 0:15:47 | 0:15:50 | |
and then coming through the slits. | 0:15:50 | 0:15:52 | |
And do you see that there are waves here, | 0:15:52 | 0:15:54 | |
-but here, there's kind of an area where the water's flat. -Yeah. | 0:15:54 | 0:15:58 | |
Then here there are waves, | 0:15:58 | 0:16:00 | |
then here's an area where the water's flat, | 0:16:00 | 0:16:02 | |
then here are waves, here's an area where the water's flat. | 0:16:02 | 0:16:05 | |
So if I were to, I could sketch it actually on the blackboard. | 0:16:05 | 0:16:08 | |
If I draw that... | 0:16:08 | 0:16:10 | |
We've got those two slits, like that, which you can see there. | 0:16:14 | 0:16:17 | |
and we've got the water wave coming through | 0:16:17 | 0:16:20 | |
and you can sort of see that the waves | 0:16:20 | 0:16:22 | |
when they go through the slits spread out like that. | 0:16:22 | 0:16:25 | |
And I hope you can see that at the front, you're seeing | 0:16:25 | 0:16:30 | |
a kind of a place where there's no waves and then some waves | 0:16:30 | 0:16:33 | |
and then there's a place where there's no waves | 0:16:33 | 0:16:35 | |
and then there's some waves and a place where there's no waves. | 0:16:35 | 0:16:38 | |
-You see that pattern on the front. -Yes. | 0:16:38 | 0:16:40 | |
So if you were to draw kind of a detector along there, | 0:16:40 | 0:16:43 | |
then you'd see that, right, | 0:16:43 | 0:16:46 | |
because here you'd see nothing, no waves no electrons. | 0:16:46 | 0:16:50 | |
Here you'd see the electrons, here no waves, here waves, here no waves. | 0:16:50 | 0:16:54 | |
So what are we to infer about electrons? | 0:16:54 | 0:16:57 | |
Have you not done your homework today, is that what it is? | 0:17:00 | 0:17:03 | |
I mean this is just the experimental data... This was first done, | 0:17:03 | 0:17:06 | |
by the way, in the 1920s and it was a shock when it was seen, | 0:17:06 | 0:17:10 | |
but the inference is...? | 0:17:10 | 0:17:12 | |
That looks like...that. | 0:17:15 | 0:17:18 | |
-This could be a long game. -It's the same pattern! | 0:17:18 | 0:17:21 | |
LAUGHTER | 0:17:21 | 0:17:23 | |
GCSE grade C, remember. | 0:17:25 | 0:17:27 | |
This pattern here... | 0:17:29 | 0:17:31 | |
What do you think...?! | 0:17:31 | 0:17:34 | |
You could just tell us. | 0:17:34 | 0:17:36 | |
So, the electrons are behaving more like the waves in the tank | 0:17:38 | 0:17:43 | |
on the water waves and that's a classic pattern you see | 0:17:43 | 0:17:47 | |
when you get waves passing through slits. | 0:17:47 | 0:17:50 | |
Rather than this, which I suppose is what you might have expected | 0:17:50 | 0:17:53 | |
electrons to do, because you might think of electrons as being little grains of sand. | 0:17:53 | 0:17:57 | |
But actually, they don't behave like little grains of sand. | 0:17:57 | 0:18:00 | |
That experiment tells us they behave more like waves and water. | 0:18:00 | 0:18:04 | |
Exactly! | 0:18:04 | 0:18:05 | |
LAUGHTER AND APPLAUSE | 0:18:05 | 0:18:07 | |
Thank you. | 0:18:09 | 0:18:10 | |
Thanks, Sarah! | 0:18:17 | 0:18:19 | |
Thanks, Sarah. That's... Yeah, physics! | 0:18:19 | 0:18:23 | |
Well... | 0:18:26 | 0:18:27 | |
this might all be a bit confusing, as you've just seen, | 0:18:27 | 0:18:31 | |
but if you remember nothing else, remember this - the double slit experiment reveals something | 0:18:31 | 0:18:37 | |
fundamental about particles like the electrons inside the diamond. | 0:18:37 | 0:18:42 | |
Sometimes they behave like particles, | 0:18:42 | 0:18:45 | |
but sometimes experiment says that they behave like waves. | 0:18:45 | 0:18:50 | |
Now there's a deep explanation for this | 0:18:50 | 0:18:53 | |
and I'm going to get to that a little bit later on, | 0:18:53 | 0:18:55 | |
but for now all we need to remember is that electrons behave like waves, | 0:18:55 | 0:18:59 | |
and this is the key to understanding the emptiness of atoms. | 0:18:59 | 0:19:02 | |
Simple? I hope so. So let's clear away the water tank. | 0:19:04 | 0:19:07 | |
So, we've understood that electrons exhibit wavy behaviour, | 0:19:14 | 0:19:18 | |
but how does that explain the emptiness of atoms? | 0:19:18 | 0:19:22 | |
Well, I need some volunteers now and I know that Simon Pegg | 0:19:22 | 0:19:25 | |
and Jim Al-Khalili have kindly volunteered, so would you both like to come down? | 0:19:25 | 0:19:29 | |
APPLAUSE | 0:19:29 | 0:19:31 | |
Have you seen him, there? | 0:19:46 | 0:19:48 | |
Hello! | 0:19:48 | 0:19:49 | |
He's got an earpiece in he's watching really carefully. | 0:19:51 | 0:19:55 | |
So, I've got an experiment for you both to do involving a spring | 0:19:55 | 0:20:00 | |
and your wrists, | 0:20:00 | 0:20:03 | |
so... | 0:20:03 | 0:20:06 | |
What I'd like you to do | 0:20:06 | 0:20:07 | |
is stretch the string a little bit as far away as you can. | 0:20:07 | 0:20:13 | |
Now what I want you to do is start gently oscillating the spring. Very gently. | 0:20:13 | 0:20:18 | |
-Both of us? -Yeah. You'll see what happens. | 0:20:18 | 0:20:21 | |
Up and down, or longitudinally? | 0:20:21 | 0:20:23 | |
ALL: Ooh! | 0:20:23 | 0:20:26 | |
Shall I sit back down? | 0:20:26 | 0:20:28 | |
Up and down is better. Up and down. | 0:20:29 | 0:20:33 | |
So just a bit more... | 0:20:33 | 0:20:34 | |
There you go... And a bit more. | 0:20:36 | 0:20:38 | |
There you go. So what you're doing is vibrating the spring. | 0:20:38 | 0:20:42 | |
Are you going to jump in? | 0:20:42 | 0:20:44 | |
LAUGHTER | 0:20:44 | 0:20:47 | |
It looks quite painful. | 0:20:48 | 0:20:50 | |
So what you're doing now, just gently vibrating the string, | 0:20:50 | 0:20:54 | |
you notice that it's vibrating in a very particular way. | 0:20:54 | 0:20:57 | |
Cos you're holding it still there and you're holding it still there, | 0:20:57 | 0:21:00 | |
so it's trapped - it's confined, in a sense. | 0:21:00 | 0:21:03 | |
So what you can see is there's only one bit which is moving | 0:21:03 | 0:21:07 | |
with the maximum amplitude if you like, the maximum wave | 0:21:07 | 0:21:10 | |
and it's in the middle there. | 0:21:10 | 0:21:12 | |
So that's called a standing wave. It's called a standing wave | 0:21:12 | 0:21:15 | |
because it's confined. | 0:21:15 | 0:21:16 | |
It's doing nothing, really - it's vibrating up and down. | 0:21:16 | 0:21:18 | |
It's not a wave as you might usually expect it. | 0:21:18 | 0:21:22 | |
Now, if you give it a bit more wrist action... | 0:21:22 | 0:21:24 | |
GIGGLING | 0:21:24 | 0:21:26 | |
Look at that one - now, that... | 0:21:27 | 0:21:30 | |
THAT is the next standing wave up, | 0:21:30 | 0:21:33 | |
so there is a transition from the one where we're just moving here - | 0:21:33 | 0:21:37 | |
this one's got three stationary points. | 0:21:37 | 0:21:40 | |
-I lost me stroke... -Don't get carried away. -Sorry, sorry. | 0:21:40 | 0:21:44 | |
Wait, wait, wait - | 0:21:45 | 0:21:48 | |
this has never happened to me before! | 0:21:48 | 0:21:50 | |
LAUGHTER AND APPLAUSE | 0:21:50 | 0:21:54 | |
There - look at that - now there's three stationary bits - | 0:21:55 | 0:21:58 | |
there's one stationary there, one stationary bit there, one stationary bit there | 0:21:58 | 0:22:02 | |
and the amplitude - the maximum amplitude is there and there. | 0:22:02 | 0:22:05 | |
Now, you can get another one going... | 0:22:05 | 0:22:08 | |
if you really try, which is the third one. | 0:22:08 | 0:22:11 | |
There it is! No! | 0:22:11 | 0:22:12 | |
CHEERING | 0:22:12 | 0:22:14 | |
Look at that. | 0:22:16 | 0:22:18 | |
Yes, yes, yes! | 0:22:22 | 0:22:24 | |
Can you see? That's got two stationary points - | 0:22:24 | 0:22:27 | |
-one there and one there. That's a brilliant... -Oh, it's gone again! | 0:22:27 | 0:22:31 | |
I can see... Hang on... There, there, there! | 0:22:31 | 0:22:34 | |
Two stationary points... 1, 2, 3, 4 stationary points. | 0:22:34 | 0:22:37 | |
-I can see why you've got no air! -Here it is! There it is! | 0:22:37 | 0:22:40 | |
Ah, that's better now. There's the fourth one. | 0:22:44 | 0:22:46 | |
So, you... | 0:22:46 | 0:22:48 | |
You carry on. | 0:22:48 | 0:22:50 | |
Now it feels like someone else! | 0:22:50 | 0:22:52 | |
It's back! Ah, it's gone! | 0:22:52 | 0:22:54 | |
So if I just sketch... Carry on! | 0:22:57 | 0:23:00 | |
There we go - yes! | 0:23:00 | 0:23:01 | |
-Brian, Brian, Brian, Brian! -Yeah, yeah, yeah! | 0:23:01 | 0:23:04 | |
APPLAUSE | 0:23:04 | 0:23:07 | |
Perfect. | 0:23:15 | 0:23:16 | |
1, 2, 3, 4, 5 - all right, you can stop now. | 0:23:16 | 0:23:19 | |
Good practice for later! | 0:23:21 | 0:23:23 | |
-Thank you very much! -Thanks. | 0:23:25 | 0:23:27 | |
APPLAUSE | 0:23:27 | 0:23:28 | |
I sketched what you saw there. | 0:23:33 | 0:23:35 | |
You saw that one very clearly which was this wave | 0:23:35 | 0:23:37 | |
where there were just two stationary points | 0:23:37 | 0:23:39 | |
which were at the ends and then you saw this one, | 0:23:39 | 0:23:42 | |
where there were three stationary points. | 0:23:42 | 0:23:45 | |
And then you saw this one where there were four stationary points | 0:23:45 | 0:23:47 | |
and actually, because you were... That's the best I've ever seen it done, | 0:23:47 | 0:23:51 | |
-there was one with about five, I think, or even six. -(Yes!) | 0:23:51 | 0:23:53 | |
So, you saw that... | 0:23:53 | 0:23:55 | |
there were only certain waves... | 0:23:55 | 0:23:58 | |
That the spring could vibrate, certain waves it could vibrate | 0:23:58 | 0:24:01 | |
and the reason it behaved like that is because it was trapped at both ends. | 0:24:01 | 0:24:06 | |
So this is what you would call, physicists would call | 0:24:06 | 0:24:10 | |
standing waves and you saw them appear on that spring. | 0:24:10 | 0:24:13 | |
Now, what has that got to do with empty atoms? | 0:24:14 | 0:24:17 | |
Well, just as this wave was trapped between Jim and Simon, | 0:24:17 | 0:24:22 | |
electrons are trapped inside atoms. | 0:24:22 | 0:24:24 | |
The positive electric charge of the nucleus effectively traps | 0:24:24 | 0:24:29 | |
the negatively-charged electron inside an atomic-sized box. | 0:24:29 | 0:24:33 | |
And when an electron is trapped, | 0:24:33 | 0:24:34 | |
just as the spring was trapped between Jim and Simon, | 0:24:34 | 0:24:37 | |
it exhibits the same kind of wave-like behaviour as the spring. | 0:24:37 | 0:24:41 | |
So now we're getting closer to understanding what's happening inside an atom. | 0:24:41 | 0:24:46 | |
But what do standing electron waves around a nucleus actually represent? | 0:24:46 | 0:24:52 | |
Well, the clue is that Jim and Simon had to put more energy in | 0:24:52 | 0:24:55 | |
to switch from one standing wave to another. | 0:24:55 | 0:24:59 | |
So it's tempting to think of those electron standing waves | 0:24:59 | 0:25:03 | |
as waves with different energies inside an atom, | 0:25:03 | 0:25:08 | |
waves that the different energies, the electron can have, if you like | 0:25:08 | 0:25:11 | |
when it's confined around a nucleus and this turns out to be correct. | 0:25:11 | 0:25:16 | |
But, just as there were only certain standing waves on the spring, | 0:25:16 | 0:25:19 | |
inside an atom, there are only certain energies that electrons can have. | 0:25:19 | 0:25:24 | |
Now, quantum theory allows physicists to calculate the shape | 0:25:24 | 0:25:26 | |
of the waves and therefore the allowed energies the electrons can have inside the atom. | 0:25:26 | 0:25:32 | |
And when you do the calculations, you find the lowest energy 'wave', | 0:25:32 | 0:25:35 | |
if you like, so I suppose this standing wave here | 0:25:35 | 0:25:40 | |
that can fit around the nucleus | 0:25:40 | 0:25:42 | |
has a wavelength of around 3 x 10-10 metres. | 0:25:42 | 0:25:46 | |
Now, let me just write that down, because you might not be familiar with the notation. | 0:25:46 | 0:25:49 | |
It's 1, 2, 3, 4, 5, 6, 7, 8, 9... | 0:25:49 | 0:25:53 | |
0.0000000003 of a metre which sounds | 0:25:53 | 0:25:58 | |
unimaginably small, but it's enormous compared to the size | 0:25:58 | 0:26:03 | |
of the nucleus. It's actually about a quarter of a million times larger. | 0:26:03 | 0:26:07 | |
So that is why atoms are so big and yet so empty. | 0:26:07 | 0:26:11 | |
It's because electrons trapped around a nucleus | 0:26:11 | 0:26:14 | |
behave like waves - in this case standing waves - and there has to be | 0:26:14 | 0:26:17 | |
enough room to fit an electron wave around the atomic nucleus. | 0:26:17 | 0:26:22 | |
But that doesn't answer a very important question. | 0:26:22 | 0:26:25 | |
Now, we've shown why atoms are empty, | 0:26:25 | 0:26:28 | |
But we haven't yet explained | 0:26:28 | 0:26:29 | |
how they become so strongly bound together that they can create solid objects | 0:26:29 | 0:26:34 | |
like our beautiful million-pound diamond here. | 0:26:34 | 0:26:37 | |
Answer that, and we explain the structure of everything we see in the universe. | 0:26:37 | 0:26:44 | |
The early years of quantum theory were dominated by boy wonders, | 0:26:49 | 0:26:53 | |
people actually half my age, believe it or not. | 0:26:53 | 0:26:56 | |
So much so, that it became nicknamed "Knabenphysik", | 0:26:56 | 0:27:00 | |
which translated from German means "boy physics". | 0:27:00 | 0:27:03 | |
The key discovery was made by a man called Wolfgang Pauli. | 0:27:03 | 0:27:07 | |
Pauli published his first paper on Einstein's Theory of General Relativity when he was 18. | 0:27:07 | 0:27:12 | |
And his great contribution to quantum theory was made when he was only 24. | 0:27:12 | 0:27:17 | |
It's known as the Exclusion Principle. | 0:27:17 | 0:27:20 | |
We've seen that electrons can only exist in certain energy levels around the nucleus. | 0:27:20 | 0:27:24 | |
These energy levels, associated with the different standing waves. | 0:27:24 | 0:27:29 | |
Those energy levels correspond to standing waves that can fit in the atomic size box. | 0:27:29 | 0:27:35 | |
But the key point that Pauli realised | 0:27:35 | 0:27:37 | |
is that electrons can't all simply inhabit the lowest energy level. | 0:27:37 | 0:27:42 | |
Now, to a physicist, this should look a bit odd. | 0:27:42 | 0:27:45 | |
I mean, take this apple, for example. | 0:27:45 | 0:27:48 | |
If I lift the apple up, then I have to do work. | 0:27:48 | 0:27:51 | |
I give it energy to lift it up. | 0:27:51 | 0:27:52 | |
And if I let go, so I don't support it any more, | 0:27:52 | 0:27:55 | |
then it falls to the ground. | 0:27:55 | 0:27:58 | |
Now, the explanation of that, for a physicist, | 0:27:58 | 0:28:00 | |
is that the apple is falling into a lower-energy state. | 0:28:00 | 0:28:04 | |
Nature doesn't like to be in high-energy states. | 0:28:04 | 0:28:07 | |
It wants to cascade down into the lowest energy configuration that it can. | 0:28:07 | 0:28:13 | |
But the surprising thing is that electrons don't all live in that lowest energy level in an atom. | 0:28:13 | 0:28:19 | |
It turns out they're forbidden from doing so by an unbreakable law of nature. | 0:28:19 | 0:28:24 | |
That law is called the Pauli Exclusion Principle. | 0:28:24 | 0:28:28 | |
It's kind of like all of you sitting in these rows here. | 0:28:28 | 0:28:30 | |
You aren't allowed to all come down to the front row. | 0:28:30 | 0:28:34 | |
You can't all squash into the front seats, because there isn't room for you. | 0:28:34 | 0:28:38 | |
Electrons don't all occupy the lowest energy slots around an atom. | 0:28:38 | 0:28:43 | |
Instead, they fill each level up in order of increasing energy. | 0:28:43 | 0:28:48 | |
This might sound meaningless, | 0:28:48 | 0:28:49 | |
maybe it sounds a bit abstract. | 0:28:49 | 0:28:51 | |
But let me tell you that it isn't. | 0:28:51 | 0:28:52 | |
You see, Pauli's simple quantum rule is profoundly important. | 0:28:52 | 0:28:56 | |
In fact, it's the key to understanding chemistry. | 0:28:56 | 0:29:00 | |
But don't take my word for it. Time for another volunteer. | 0:29:00 | 0:29:02 | |
I know that James May kindly volunteered to take part in this. | 0:29:02 | 0:29:07 | |
He looks very worried, so maybe he was never asked! But anyway, James. | 0:29:07 | 0:29:11 | |
Now this is doubly amusing for me, | 0:29:22 | 0:29:25 | |
cos I know that you know exactly what's going to happen | 0:29:25 | 0:29:29 | |
because there's a canister of hydrogen gas there | 0:29:29 | 0:29:31 | |
and I know you're a keen aviator, so... | 0:29:31 | 0:29:34 | |
-You think about the story of the Hindenburg... -Mmm! -..while I... | 0:29:34 | 0:29:37 | |
-Which was unhappy, wasn't it? -Oh, I get to wear the goggles? -You might have to wear the goggles. | 0:29:37 | 0:29:42 | |
It's only a small safety thing, because it went wrong in rehearsal. | 0:29:42 | 0:29:47 | |
So what we're going to do is encourage a small chemical reaction to happen. What we're doing | 0:29:47 | 0:29:52 | |
is bubbling hydrogen through... Hydrogen gas through this, um... | 0:29:52 | 0:29:55 | |
-LAUGHTER -..through this soap, here. -Mmm. | 0:29:55 | 0:29:59 | |
What I'd like you to do... Actually, just wet your hands first. Just because it's a safety thing. | 0:29:59 | 0:30:04 | |
It stops your hands catching fire. | 0:30:04 | 0:30:05 | |
It actually... Perhaps roll your sleeves up a little bit. | 0:30:05 | 0:30:09 | |
You'll be all right. I'm sure you'll be fine. | 0:30:09 | 0:30:11 | |
So I'd like you to get - grab - some of that of that hydrogen in the soap bubbles. | 0:30:11 | 0:30:16 | |
Um... | 0:30:17 | 0:30:19 | |
-How's that? -Don't look... | 0:30:20 | 0:30:23 | |
at what I'm doing. | 0:30:23 | 0:30:25 | |
What I'm going to do is I'm going to encourage a chemical reaction to happen... | 0:30:25 | 0:30:33 | |
from over here. | 0:30:33 | 0:30:34 | |
LAUGHTER | 0:30:34 | 0:30:36 | |
Whoa! | 0:30:38 | 0:30:40 | |
-Ow! -You all right? | 0:30:40 | 0:30:41 | |
LAUGHTER AND APPLAUSE | 0:30:41 | 0:30:45 | |
LAUGHTER AND APPLAUSE DROWNS SPEECH | 0:30:45 | 0:30:47 | |
Thank you very much for putting yourself at great risk! | 0:30:50 | 0:30:54 | |
Thanks, James. That actually was a lot more fire than I was expecting! Sorry about that. | 0:31:01 | 0:31:06 | |
So what happened there? | 0:31:06 | 0:31:08 | |
What we did was we bubbled hydrogen gas into these bubbles. | 0:31:08 | 0:31:12 | |
James held them, and then I just gave them a little kick of energy | 0:31:12 | 0:31:17 | |
which encouraged them to react with oxygen in the air. | 0:31:17 | 0:31:20 | |
Now if draw the energy levels of oxygen, | 0:31:20 | 0:31:23 | |
then they look something like that. | 0:31:23 | 0:31:25 | |
They don't quite look as neat as when I drew the standing waves on the spring. | 0:31:25 | 0:31:30 | |
That's really because of the shape of the atomic box, | 0:31:30 | 0:31:33 | |
the shape of the box surrounding the oxygen nucleus. | 0:31:33 | 0:31:36 | |
Now oxygen has eight protons and eight neutrons in its nucleus, | 0:31:36 | 0:31:41 | |
which means it needs eight electrons filling up its energy levels. | 0:31:41 | 0:31:45 | |
And the electrons fill up the energy levels like that. | 0:31:45 | 0:31:49 | |
So you get three full energy levels | 0:31:51 | 0:31:53 | |
and two energy levels with a single electron in them. | 0:31:53 | 0:31:57 | |
Now that kind of makes oxygen a voracious consumer of electrons. | 0:31:57 | 0:32:04 | |
It would like, if it can - | 0:32:04 | 0:32:06 | |
it's energetically favourable for it to fill up those missing gaps. | 0:32:06 | 0:32:09 | |
Hydrogen has one proton, | 0:32:09 | 0:32:13 | |
and so it has one electron sat there in its lowest energy level. | 0:32:13 | 0:32:17 | |
Again, it has a space there. It would also like to fill that up. | 0:32:17 | 0:32:21 | |
So what happens, when I give it a little kick with this splint, | 0:32:21 | 0:32:26 | |
is that the hydrogen is encouraged to react with the with the oxygen. | 0:32:26 | 0:32:31 | |
It's energetically favourable for it to share its electron. | 0:32:31 | 0:32:35 | |
So the oxygen shares with the hydrogen, | 0:32:35 | 0:32:36 | |
the hydrogen shares with the oxygen. | 0:32:36 | 0:32:38 | |
There are two gaps, so you get two hydrogens which would like to react. | 0:32:38 | 0:32:43 | |
In doing so, the rearrangement of those electrons in the energy levels | 0:32:43 | 0:32:47 | |
is such a great giver of energy that you saw a flash. | 0:32:47 | 0:32:50 | |
All that flash that you saw, the little explosion, was energy being released | 0:32:50 | 0:32:55 | |
when the electrons in the hydrogen and the oxygen reconfigure - | 0:32:55 | 0:33:00 | |
just like the apple reconfigured itself | 0:33:00 | 0:33:02 | |
by dropping to the ground to get into the lowest energy state. | 0:33:02 | 0:33:06 | |
Two hydrogens, one oxygen. What does that make? | 0:33:06 | 0:33:10 | |
MAN: Water. | 0:33:10 | 0:33:11 | |
-ALL: Water! -Right! | 0:33:11 | 0:33:14 | |
H2O. | 0:33:14 | 0:33:17 | |
So that is essentially the reason why we get chemistry. | 0:33:17 | 0:33:22 | |
Without Pauli's Exclusion Principle, | 0:33:22 | 0:33:24 | |
all the electrons would crowd down into the lowest energy level and there'd be no chemistry. | 0:33:24 | 0:33:30 | |
Which is worse than it sounds... | 0:33:30 | 0:33:32 | |
LAUGHTER | 0:33:32 | 0:33:34 | |
..because without chemistry, we'd have no magnificent structures in the universe, | 0:33:37 | 0:33:42 | |
like water, diamonds, or indeed, any of you. | 0:33:42 | 0:33:47 | |
Now, there's another consequence of the exclusion principle | 0:33:47 | 0:33:51 | |
that wasn't proved until 1967, | 0:33:51 | 0:33:53 | |
just one year before I was born. | 0:33:53 | 0:33:55 | |
Pauli's principle says that identical electrons | 0:33:55 | 0:33:59 | |
can't occupy the same energy level. | 0:33:59 | 0:34:01 | |
This is an absolute requirement. | 0:34:01 | 0:34:03 | |
So it also means that electrons will avoid each other at all costs. | 0:34:03 | 0:34:07 | |
And that, it was proved, is the actual reason | 0:34:07 | 0:34:11 | |
that I don't fall through the empty atoms that make up the floor. | 0:34:11 | 0:34:15 | |
That's ultimately what gives the illusion of solidity to the empty world of atoms. | 0:34:15 | 0:34:21 | |
And if you think a little bit more deeply about it, | 0:34:21 | 0:34:24 | |
then this throws up a bewildering conclusion, and it's this. | 0:34:24 | 0:34:27 | |
The Pauli Exclusion Principle applies to EVERY electron in the universe. | 0:34:27 | 0:34:33 | |
Not just every electron in a single atom, or a single molecule. | 0:34:33 | 0:34:36 | |
And this leads to a bizarre conclusion. | 0:34:36 | 0:34:39 | |
The particles that make up this diamond | 0:34:39 | 0:34:41 | |
are in communication with particles everywhere. | 0:34:41 | 0:34:43 | |
Inside all of you, | 0:34:45 | 0:34:46 | |
and inside the atoms in the furthest corners of the universe. | 0:34:46 | 0:34:50 | |
Let me explain that a little bit more. The Pauli Exclusion Principle | 0:34:50 | 0:34:54 | |
says no identical electrons can be in precisely the same energy level. | 0:34:54 | 0:34:58 | |
What if you have more than one atom? | 0:34:58 | 0:35:00 | |
For example, in this diamond | 0:35:00 | 0:35:03 | |
there are 3 million billion billion carbon atoms. | 0:35:03 | 0:35:07 | |
So this is a diamond-size box of carbon atoms. | 0:35:07 | 0:35:10 | |
And the Pauli Exclusion Principle still applies. | 0:35:10 | 0:35:14 | |
So all the energy levels | 0:35:14 | 0:35:16 | |
in all those 3 million billion billion atoms | 0:35:16 | 0:35:18 | |
have to be slightly different in order to ensure that | 0:35:18 | 0:35:21 | |
none of the electrons sit in precisely the same energy level. | 0:35:21 | 0:35:25 | |
Pauli's principle holds fast. But it doesn't stop with the diamond. | 0:35:25 | 0:35:30 | |
See, you can think of the whole universe as a vast box of atoms, | 0:35:30 | 0:35:35 | |
with countless numbers of energy levels | 0:35:35 | 0:35:38 | |
all filled by countless numbers of electrons. | 0:35:38 | 0:35:42 | |
So here's the amazing thing - the exclusion principle still applies, | 0:35:42 | 0:35:46 | |
so none of the electrons in the universe can sit in precisely | 0:35:46 | 0:35:50 | |
the same energy level. | 0:35:50 | 0:35:52 | |
But that must mean something very odd. | 0:35:52 | 0:35:54 | |
See, let me take this diamond, and let me just | 0:35:54 | 0:35:57 | |
heat it up a little bit between my hands. | 0:35:57 | 0:35:59 | |
Just gently warming it up, | 0:35:59 | 0:36:01 | |
putting a bit of energy into it, so I'm shifting the electrons around, | 0:36:01 | 0:36:04 | |
some of the electrons are jumping into different energy levels. | 0:36:04 | 0:36:08 | |
But this shift in the configuration of the electrons | 0:36:08 | 0:36:11 | |
inside the diamond has consequences, because the sum total | 0:36:11 | 0:36:14 | |
of all the electrons in the universe must respect Pauli. | 0:36:14 | 0:36:19 | |
Therefore, every electron, around every atom | 0:36:19 | 0:36:22 | |
in the universe, must be shifting as I heat the diamond up, | 0:36:22 | 0:36:26 | |
to make sure that none of them end up in the same energy level. | 0:36:26 | 0:36:30 | |
When I heat this diamond up, all the electrons across the universe | 0:36:30 | 0:36:34 | |
instantly but imperceptibly change their energy levels. | 0:36:34 | 0:36:38 | |
So everything is connected to everything else. | 0:36:38 | 0:36:43 | |
At the beginning, I promised I'd explain everything in the universe, | 0:36:50 | 0:36:54 | |
which I have in some way, but also I said that I'd give you | 0:36:54 | 0:36:58 | |
a deeper explanation of that wavy behaviour of the subatomic world. | 0:36:58 | 0:37:03 | |
So here it is. In my view, this is the deepest explanation we have, | 0:37:03 | 0:37:06 | |
and it's down to the Nobel Prize-winning physicist | 0:37:06 | 0:37:09 | |
Richard Feynman who, his colleague Freeman Dyson once described | 0:37:09 | 0:37:12 | |
as half genius, half buffoon but he subsequently, after having | 0:37:12 | 0:37:15 | |
worked with him for a while, changed that to all genius, all buffoon. | 0:37:15 | 0:37:19 | |
Let's go back to the double slit experiment, but now, | 0:37:19 | 0:37:22 | |
instead of just showing you the pattern... | 0:37:22 | 0:37:24 | |
This is Richard Feynman. | 0:37:24 | 0:37:26 | |
Instead of just showing you the pattern, | 0:37:26 | 0:37:28 | |
I want to show you how that pattern builds up. | 0:37:28 | 0:37:30 | |
Remember, we're firing electrons at two slits, | 0:37:30 | 0:37:32 | |
almost pouring them through two slits | 0:37:32 | 0:37:34 | |
and seeing what happened when they were detected on the other side. | 0:37:34 | 0:37:38 | |
Well, this is one electron at a time being fired through the slits | 0:37:38 | 0:37:43 | |
and hitting the screen, and building up in a pile. | 0:37:43 | 0:37:46 | |
Only when the one electron has gone through, was another one fired | 0:37:46 | 0:37:49 | |
and this is real data, again, a real movie of that happening | 0:37:49 | 0:37:54 | |
and you see the interference pattern. | 0:37:54 | 0:37:56 | |
Electrons, no electrons, electrons, no electrons. | 0:37:56 | 0:37:59 | |
The wavy-type interference pattern building up. | 0:37:59 | 0:38:03 | |
What could be happening there? | 0:38:03 | 0:38:05 | |
So, here it is again. Just electrons | 0:38:05 | 0:38:07 | |
and you see that what emerges is that wave-like behaviour. | 0:38:07 | 0:38:10 | |
So, you might have thought, "Well, I kind of understand | 0:38:10 | 0:38:13 | |
"what's going on with the double slits, there's loads of electrons | 0:38:13 | 0:38:16 | |
"piling through the slits and somehow there's some interference | 0:38:16 | 0:38:19 | |
"just like a big water wave and you build up the interference pattern." | 0:38:19 | 0:38:23 | |
Well, no, because this is one electron at a time, | 0:38:23 | 0:38:27 | |
so, what could possibly be happening? | 0:38:27 | 0:38:29 | |
Well, Feynman was a wonderfully intuitive, logical physicist. | 0:38:29 | 0:38:34 | |
No ordinary genius, he was often described as. | 0:38:34 | 0:38:37 | |
And he said this. | 0:38:37 | 0:38:40 | |
Here are the slits. | 0:38:40 | 0:38:43 | |
Here's the screen. | 0:38:43 | 0:38:45 | |
The electrons starts off here. What happens? | 0:38:45 | 0:38:48 | |
Well, obviously, the particle - electron - must go through a slit | 0:38:48 | 0:38:51 | |
and it must appear somewhere on the screen, | 0:38:51 | 0:38:54 | |
but it needs to be able to interfere with itself - | 0:38:54 | 0:38:57 | |
there've got to be regions on the screen where there are no electrons, | 0:38:57 | 0:39:01 | |
it's prevented from landing there, | 0:39:01 | 0:39:02 | |
so it must, at least, go through the other slit, as well, | 0:39:02 | 0:39:06 | |
and get to that point, and there must be some mechanism | 0:39:06 | 0:39:09 | |
for these paths interfering with each other, but why stop there? | 0:39:09 | 0:39:14 | |
See, that wouldn't be particularly logical. | 0:39:14 | 0:39:16 | |
Why only let it go through two paths? | 0:39:16 | 0:39:18 | |
Why not let it go through that path or maybe | 0:39:18 | 0:39:21 | |
some sort of path like that, or maybe like or maybe, indeed, | 0:39:21 | 0:39:26 | |
off here, out of this lecture theatre | 0:39:26 | 0:39:29 | |
and then maybe through Jonathan's head on its way... | 0:39:29 | 0:39:33 | |
I've got to say through Paul's foot, haven't I? Cos I just have to. | 0:39:33 | 0:39:36 | |
Paul Foot. I don't know - what a rubbish thing to say. | 0:39:36 | 0:39:40 | |
But, anyway, it could go through you, through Jonathan, | 0:39:40 | 0:39:43 | |
off up Oxford Street, up to Newcastle | 0:39:43 | 0:39:46 | |
indeed on to the Andromeda Galaxy | 0:39:46 | 0:39:48 | |
and back again, and land at this point on the screen. | 0:39:48 | 0:39:51 | |
Why not? | 0:39:51 | 0:39:54 | |
Why not allow the particle to travel along every possible path it can, | 0:39:54 | 0:39:57 | |
from one point to the other? And that is indeed what happens, | 0:39:57 | 0:40:02 | |
in the sense that's the way Feynman's theory works. | 0:40:02 | 0:40:06 | |
In principle, it's not too difficult. | 0:40:06 | 0:40:08 | |
You just have to calculate some quantity | 0:40:08 | 0:40:10 | |
associated with each path and find some mathematical machinery | 0:40:10 | 0:40:14 | |
from adding all those things up, and seeing whether or not they all | 0:40:14 | 0:40:18 | |
interfere together and disappear or appear when they land on the screen. | 0:40:18 | 0:40:22 | |
There is a formula that does that | 0:40:22 | 0:40:24 | |
and this is all I really need to say. | 0:40:24 | 0:40:27 | |
Let me turn it around. There it is. | 0:40:27 | 0:40:30 | |
Thank you and good... No, no, I won't say that! | 0:40:30 | 0:40:32 | |
This is called the Feynman path integral, | 0:40:32 | 0:40:35 | |
and this just says, | 0:40:35 | 0:40:36 | |
sum up over all the paths and calculate something | 0:40:36 | 0:40:40 | |
that will tell you the probability | 0:40:40 | 0:40:42 | |
of an electron going from one place to another. | 0:40:42 | 0:40:44 | |
Now, that might look a tremendous mess, | 0:40:44 | 0:40:47 | |
or it might look very simple and illuminating - | 0:40:47 | 0:40:50 | |
I suppose it depends on your point of view. | 0:40:50 | 0:40:52 | |
Probably a tremendous mess, granted. | 0:40:52 | 0:40:55 | |
But this formula is just a little machine, | 0:40:55 | 0:40:57 | |
I think that's a good way to think about it. | 0:40:57 | 0:40:59 | |
It that takes all the possible paths a particle can have, | 0:40:59 | 0:41:02 | |
it adds them up and it spits out the probability | 0:41:02 | 0:41:05 | |
that it'll end up at some particular place. | 0:41:05 | 0:41:08 | |
And that includes the particles that make up the diamond. | 0:41:08 | 0:41:13 | |
Now, for the moment, it's sat on its little cushion there. | 0:41:13 | 0:41:17 | |
Let me put it back in its box. | 0:41:17 | 0:41:19 | |
Now, Feynman's version of quantum theory tells us | 0:41:21 | 0:41:24 | |
something rather shocking. | 0:41:24 | 0:41:26 | |
This diamond is made up of atoms, | 0:41:26 | 0:41:28 | |
and the atoms are behaving according to quantum theory - | 0:41:28 | 0:41:31 | |
according to Feynman's equation. | 0:41:31 | 0:41:33 | |
In other words, they are all currently exploring the universe, | 0:41:33 | 0:41:36 | |
hopping around everywhere, exploring every possible path they can. | 0:41:36 | 0:41:41 | |
And that means this diamond is doing the same thing, | 0:41:41 | 0:41:43 | |
because it's made of atoms. | 0:41:43 | 0:41:46 | |
That means there is a finite chance that it will not | 0:41:46 | 0:41:48 | |
be inside this box at a later time - you can see where I'm going - | 0:41:48 | 0:41:54 | |
but it'll jump, completely out of its own accord, | 0:41:54 | 0:41:59 | |
without me touching it...and that's what I'm going to tell the judge! | 0:41:59 | 0:42:03 | |
But what's remarkable, is that I can calculate what the chance is | 0:42:05 | 0:42:09 | |
by using a simplified version of Feynman's formula. | 0:42:09 | 0:42:15 | |
And this is it. | 0:42:15 | 0:42:17 | |
See, just by doing a bit of maths, you can work that, simplify it, | 0:42:17 | 0:42:21 | |
and turn it into this... | 0:42:21 | 0:42:23 | |
which is an expression for the time you would have to wait, | 0:42:23 | 0:42:27 | |
on the average, to have a reasonable chance of it hopping | 0:42:27 | 0:42:30 | |
out of its box, and it goes like this. | 0:42:30 | 0:42:34 | |
OK, so, that is the distance we want it to hop, | 0:42:37 | 0:42:42 | |
that is the size of the box, | 0:42:42 | 0:42:44 | |
that's the mass of the diamond | 0:42:44 | 0:42:46 | |
and that's something called Planck's constant. | 0:42:46 | 0:42:48 | |
I'm going to need another volunteer here | 0:42:48 | 0:42:50 | |
because I'm going to actually do the maths | 0:42:50 | 0:42:53 | |
because I want to show you that you can do the sum quite simply | 0:42:53 | 0:42:55 | |
and I believe that Jonathan has kindly agreed | 0:42:55 | 0:42:58 | |
to do some sums, so, thank you. | 0:42:58 | 0:43:01 | |
-How's your maths? -Well, you know, you know that's easy for me. | 0:43:12 | 0:43:17 | |
I do. That's why I asked you, actually. | 0:43:17 | 0:43:20 | |
We're going to do it, | 0:43:20 | 0:43:21 | |
so x - that's the distance we want the diamond to jump. | 0:43:21 | 0:43:24 | |
So let's say the box is about 5cm. | 0:43:24 | 0:43:27 | |
Let's say 6cm for x | 0:43:27 | 0:43:31 | |
and the mass of the diamond is 290-something carats - | 0:43:31 | 0:43:36 | |
-it's about 60g. -Roughly, yes. -An expert on diamonds, are you? | 0:43:36 | 0:43:41 | |
So, first of all, we just have to multiply those 3 numbers together. | 0:43:41 | 0:43:45 | |
6cm x 5cm x 60g. | 0:43:45 | 0:43:48 | |
Yeah. 6 x 5 x 6. | 0:43:48 | 0:43:49 | |
So 30 x 60. You just said 6! | 0:43:49 | 0:43:53 | |
60. 60g. | 0:43:53 | 0:43:54 | |
OK, 30 x 6 = 1,800. | 0:43:54 | 0:43:57 | |
Is that right? 60? | 0:43:57 | 0:43:59 | |
-It's heavy. -It is. The BBC used to pay me in these. | 0:43:59 | 0:44:03 | |
LAUGHTER AND APPLAUSE | 0:44:03 | 0:44:07 | |
-I better take it back. I'm going to get... -HE LAUGHS NERVOUSLY | 0:44:12 | 0:44:17 | |
-Then, though we get to this. -Over the thing. | 0:44:17 | 0:44:19 | |
6.6 x 10-34 kgm2/s. | 0:44:19 | 0:44:27 | |
That is Planck's constant - | 0:44:27 | 0:44:29 | |
this is a fundamental constant of nature. | 0:44:29 | 0:44:32 | |
It's intrinsic to the way the universe is put together. | 0:44:32 | 0:44:35 | |
It's like the speed of light, like the strength of gravity. | 0:44:35 | 0:44:39 | |
It is THE fundamental THING - | 0:44:39 | 0:44:40 | |
constant, if you like - that sets the scale for quantum phenomena. | 0:44:40 | 0:44:43 | |
So, there's a slight issue here | 0:44:43 | 0:44:46 | |
because you see... You'll have noticed it. | 0:44:46 | 0:44:48 | |
The unit's are kilograms metres squared per second | 0:44:48 | 0:44:50 | |
and we calculated the 1,800 in cm and grams. | 0:44:50 | 0:44:53 | |
Which, by the way, I'm amazed I got that right! | 0:44:53 | 0:44:56 | |
So, first of all, we better another 10-2 and a 10-2 and a 10-3 on, | 0:44:56 | 0:45:01 | |
-so it's 10-7. -Yeah. | 0:45:01 | 0:45:04 | |
So all you've got to do is divide that by that. | 0:45:05 | 0:45:08 | |
-All of that with that? -Divide that by that roughly. | 0:45:08 | 0:45:11 | |
Roughly I don't even know if I can do... | 0:45:11 | 0:45:15 | |
That, for me... That's a kilogram? I don't even know. I do pounds! | 0:45:20 | 0:45:25 | |
-No, I've done the unit conversion for you - you've just got to divide. -Where's the unit conversion? | 0:45:25 | 0:45:30 | |
1,800 x 10-7 x 6.6 x 10... | 0:45:30 | 0:45:33 | |
I have no idea what you're doing and why you would want to do this to me! | 0:45:33 | 0:45:36 | |
Help him out, Jim. | 0:45:36 | 0:45:38 | |
Well you've got 10-34 downstairs. Bring it upstairs | 0:45:38 | 0:45:40 | |
-and it becomes 1034. -Where do I put it? Up here? | 0:45:40 | 0:45:43 | |
Yeah, put it next to the 10... | 0:45:43 | 0:45:46 | |
-So then you've got 34 - 7. -OK 34-7? -Yeah. -Yes, OK. | 0:45:46 | 0:45:50 | |
So that's 1027. | 0:45:50 | 0:45:52 | |
-You've got about 103. -I really... I'm so out of my depth. | 0:45:52 | 0:45:57 | |
This is the worst thing that's happened to me as an adult. | 0:45:58 | 0:46:01 | |
-You've got 1027. -OK. | 0:46:02 | 0:46:04 | |
Just for any children watching, I should say, | 0:46:04 | 0:46:10 | |
34 - 7 = 27 | 0:46:10 | 0:46:12 | |
So you've got 1027 and then we've got 6 and we've got 1,800, | 0:46:12 | 0:46:16 | |
so we've got to divide those things so we get about a 3 and another 100. | 0:46:16 | 0:46:22 | |
If you say so! | 0:46:22 | 0:46:24 | |
3 x 1029...ish. | 0:46:24 | 0:46:27 | |
Once again, I am none the wiser. LAUGHTER | 0:46:27 | 0:46:31 | |
Why couldn't I have done James May's job where you just set fire to me? | 0:46:31 | 0:46:36 | |
And everyone went "Oooh!" And he's so happy he did that | 0:46:36 | 0:46:41 | |
and I'm now sweating. | 0:46:41 | 0:46:44 | |
-We're done. -We've done it? -Yeah, you see, this is what that number is you calculated. | 0:46:44 | 0:46:49 | |
See, we just put in the numbers divided by Planck's constant? What this number is | 0:46:49 | 0:46:53 | |
is the number of seconds you would have to wait on the average to have | 0:46:53 | 0:46:57 | |
a reasonable chance of the diamond hopping out of the box on its own. | 0:46:57 | 0:47:00 | |
I could have told you that's not going to happen without any of this. | 0:47:00 | 0:47:03 | |
LAUGHTER | 0:47:03 | 0:47:05 | |
I didn't need the sums. The diamond is safe in the box, | 0:47:05 | 0:47:08 | |
unless it's turned into a dead cat. That's the theory, isn't it? | 0:47:08 | 0:47:11 | |
I'll tell you what this is. Do you know roughly what that is? | 0:47:11 | 0:47:14 | |
-A nine? -3 x 1029? -Why would I know? I'm an idiot! | 0:47:14 | 0:47:18 | |
-In years? -That's about... -Well, I'll tell you what it is. It is 600 billion times | 0:47:18 | 0:47:23 | |
the current age of the universe. | 0:47:23 | 0:47:26 | |
I don't know what to do. I'm just going to keep smiling at you. | 0:47:26 | 0:47:29 | |
-LAUGHTER Thank you for sharing that. -Thank you. | 0:47:29 | 0:47:33 | |
Thanks. | 0:47:35 | 0:47:38 | |
Thanks, Jon. | 0:47:43 | 0:47:45 | |
The point of that... The point of that is to show that quantum theory doesn't just | 0:47:46 | 0:47:52 | |
apply to the inconceivably small world of the atom. | 0:47:52 | 0:47:55 | |
The same rules apply to you, to me, and the diamond. | 0:47:55 | 0:47:59 | |
It's just that for objects out here in the familiar world, | 0:47:59 | 0:48:03 | |
like the diamond, we don't usually see quantum effects. | 0:48:03 | 0:48:06 | |
The reason for that is the smallness of Planck's constant. We had quite a big number here, | 0:48:06 | 0:48:11 | |
but we had to divide it by an extremely small number in order | 0:48:11 | 0:48:15 | |
to work out the time we'd have to wait and that's why that's big. | 0:48:15 | 0:48:19 | |
See, if that was one or something like that, then we wouldn't have had to wait many seconds - | 0:48:19 | 0:48:23 | |
about 1,800 seconds or something like that, for the diamond to hop out of the box. | 0:48:23 | 0:48:27 | |
So it's Planck's constant, this fundamental constant of nature | 0:48:27 | 0:48:30 | |
that means that quantum theory is rather unfamiliar | 0:48:30 | 0:48:34 | |
because it applies to small things, because Planck's constant is small. | 0:48:34 | 0:48:39 | |
Now you could theoretically make the diamond jump sooner. | 0:48:39 | 0:48:43 | |
Look again at this equation. | 0:48:43 | 0:48:45 | |
One way to do it, as I've said, would be to make Planck's constant very big, | 0:48:45 | 0:48:49 | |
but you can't do that. It's a fundamental constant of nature. What you could do, though, | 0:48:49 | 0:48:53 | |
is you could shrink the size of the box, this delta x here. | 0:48:53 | 0:48:57 | |
If I made the box smaller and smaller and smaller, | 0:48:57 | 0:49:01 | |
I'd make the time I had to wait for it to jump out of the box smaller and smaller and smaller. | 0:49:01 | 0:49:07 | |
So this equation says that the more we know the position | 0:49:07 | 0:49:11 | |
of something, the position of this diamond in the box, let's say, | 0:49:11 | 0:49:15 | |
then the more likely it is for the diamond to jump out of the box. | 0:49:15 | 0:49:19 | |
Now this is known as Heisenberg's Uncertainty Principle - | 0:49:19 | 0:49:23 | |
the more you try to pin down a particle's position by trapping it | 0:49:23 | 0:49:27 | |
in a smaller and smaller box, the more likely it is to jump around. | 0:49:27 | 0:49:31 | |
You might have come across Heisenberg's Uncertainty Principle. | 0:49:31 | 0:49:35 | |
It's one of the most famously misunderstood | 0:49:35 | 0:49:37 | |
and misrepresented parts of quantum theory. | 0:49:37 | 0:49:40 | |
It says, precisely, that the more precisely you know | 0:49:40 | 0:49:44 | |
a particle's position, the less certain you can be of its momentum. | 0:49:44 | 0:49:49 | |
And you can see that it emerged... I derived it from a fundamental equation. | 0:49:49 | 0:49:54 | |
It's not complete nonsense. I didn't make it up. | 0:49:54 | 0:49:57 | |
It's often misrepresented by what I would call "mischievous hippies" | 0:49:57 | 0:50:01 | |
to mean that physicists are rubbish at their job | 0:50:01 | 0:50:04 | |
or that the equipment is no good and we're unable to measure | 0:50:04 | 0:50:07 | |
two things about a particle with any accuracy. | 0:50:07 | 0:50:10 | |
But Heisenberg's Uncertainty Principle is a consequence | 0:50:10 | 0:50:13 | |
of the laws of quantum theory. It emerges | 0:50:13 | 0:50:15 | |
from Feynman's equation. It has nothing to do with any of that wishy-washy, drivelly nonsense. | 0:50:15 | 0:50:21 | |
In that spirit, I want to show you that rather than restricting our knowledge of the natural world, | 0:50:21 | 0:50:26 | |
Heisenberg can actually widen it. | 0:50:26 | 0:50:30 | |
In fact, this rule about the unimaginably small particles | 0:50:30 | 0:50:34 | |
can explain some of the most massive and spectacular objects in the universe. | 0:50:34 | 0:50:39 | |
I'm going to end | 0:50:42 | 0:50:44 | |
by explaining how everything I've told you this evening | 0:50:44 | 0:50:47 | |
predicts the existence of diamonds bigger than this - | 0:50:47 | 0:50:51 | |
in fact, bigger than this lecture theatre. | 0:50:51 | 0:50:53 | |
In fact, diamonds as big as a planet and as massive as a star. | 0:50:53 | 0:50:59 | |
Now to understand how this can be, we need to understand something | 0:50:59 | 0:51:03 | |
about the life cycles of the stars themselves. | 0:51:03 | 0:51:06 | |
Stars are big clumps of matter collapsing under their own gravity. | 0:51:06 | 0:51:09 | |
As they collapse, they heat up and they set off a chain reaction | 0:51:09 | 0:51:12 | |
of nuclear fusion reactions where the nuclei of hydrogen | 0:51:12 | 0:51:16 | |
fuse together, initially to form helium, and eventually they fuse | 0:51:16 | 0:51:21 | |
to form carbon and oxygen and all the heavy elements up to and including iron. | 0:51:21 | 0:51:26 | |
That's where the heavy elements come from in the universe. | 0:51:26 | 0:51:30 | |
In this process, vast amounts of energy are released. | 0:51:30 | 0:51:33 | |
That energy creates a pressure that holds the star up | 0:51:33 | 0:51:36 | |
and prevents it from collapsing. | 0:51:36 | 0:51:38 | |
The stars don't have infinite amounts of fuel | 0:51:38 | 0:51:41 | |
and eventually those fusion reactions must cease. | 0:51:41 | 0:51:44 | |
In five billion years, this will happen to our sun. | 0:51:44 | 0:51:47 | |
It'll stop generating enough energy to prevent its own collapse | 0:51:47 | 0:51:50 | |
and so it will collapse. | 0:51:50 | 0:51:53 | |
By the end of their lives, stars like our sun have converted all the hydrogen in their cores | 0:51:53 | 0:51:58 | |
and mainly they've converted it into oxygen and carbon. | 0:51:58 | 0:52:03 | |
Now remember that those carbon atoms, | 0:52:03 | 0:52:06 | |
just like those in our diamond, are almost entirely empty space, | 0:52:06 | 0:52:10 | |
so you might expect that the space can be squashed and compressed almost out of existence | 0:52:10 | 0:52:15 | |
as the dying star collapses. | 0:52:15 | 0:52:17 | |
But as the star collapses and becomes denser, | 0:52:17 | 0:52:20 | |
its electrons get closer and closer together. | 0:52:20 | 0:52:24 | |
Finally, they're so close that they try to occupy the same volume of space as each other. | 0:52:24 | 0:52:30 | |
Then Pauli's Exclusion Principle steps in, | 0:52:30 | 0:52:33 | |
because the electrons cannot occupy the same bit of space - | 0:52:33 | 0:52:37 | |
they are unable to overlap, so they try to arrange themselves | 0:52:37 | 0:52:43 | |
such that they have as much space as they possibly can. | 0:52:43 | 0:52:45 | |
And you might imagine them as being alone inside little boxes like this | 0:52:45 | 0:52:49 | |
and the boxes shrink and shrink and shrink as the star collapses. | 0:52:49 | 0:52:55 | |
But then, as the electrons become more and more confined, | 0:52:55 | 0:52:58 | |
Heisenberg's Uncertainty Principle comes into play. As the electrons' boxes get smaller and smaller, | 0:52:58 | 0:53:04 | |
their tendency to hop out of the box becomes greater and greater, | 0:53:04 | 0:53:08 | |
so you can think of it that they are frantically vibrating | 0:53:08 | 0:53:11 | |
around faster and faster inside these boxes of ever-decreasing size. | 0:53:11 | 0:53:16 | |
This quantum jiggling exerts a pressure, which stops | 0:53:16 | 0:53:20 | |
the star from collapsing any further, leaving something called | 0:53:20 | 0:53:23 | |
a white dwarf star, which is a densely-packed dead star the size of the Earth | 0:53:23 | 0:53:28 | |
but the mass of our sun, and a million times more dense than water. | 0:53:28 | 0:53:33 | |
White dwarfs are so dense that if I were to stand on their surface | 0:53:33 | 0:53:37 | |
the gravitational pull would make me weigh something like 30,000 tonnes. | 0:53:37 | 0:53:43 | |
White dwarfs are strange objects indeed. | 0:53:43 | 0:53:45 | |
But here is the final triumph, I think, of quantum theory. | 0:53:45 | 0:53:49 | |
It is the most powerful example I know of its power to predict how the natural world behaves. | 0:53:49 | 0:53:55 | |
See, it predicts the existence of these strange stars of white dwarfs. | 0:53:55 | 0:54:01 | |
But it does more than that. | 0:54:01 | 0:54:03 | |
In the 1930s, the physicist Subrahmanyan Chandrasekhar | 0:54:03 | 0:54:06 | |
used quantum theory to predict the maximum mass | 0:54:06 | 0:54:09 | |
of a lump of matter that can be held up by the exclusion pressure of electrons | 0:54:09 | 0:54:14 | |
to form a white dwarf. He just used the uncertainty principle, essentially, | 0:54:14 | 0:54:18 | |
and the exclusion principle. | 0:54:18 | 0:54:20 | |
He found that there should be no stars of this type | 0:54:20 | 0:54:23 | |
with masses greater than 1.4 times the mass of our sun. | 0:54:23 | 0:54:26 | |
Now to date, astronomers have found tens of thousands of white dwarf stars | 0:54:26 | 0:54:32 | |
and they have found that not one in the sky exceeds the maximum mass | 0:54:32 | 0:54:38 | |
calculated by Chandrasekhar using the simple laws of quantum theory. | 0:54:38 | 0:54:43 | |
And in amongst those stars, astronomers have found something that I think is quite extraordinary. | 0:54:43 | 0:54:48 | |
Now that diamond is 296 carats. | 0:54:48 | 0:54:51 | |
In the heart of this constellation, Centaurus, which is a few tens of light years away, | 0:54:51 | 0:54:57 | |
they've detected a white dwarf star with the wonderful name BPM 37093(!) | 0:54:57 | 0:55:03 | |
-LAUGHTER -As it died and cooled, the carbon within the core crystallised. | 0:55:03 | 0:55:09 | |
So BPM 37093, which is somewhere around there, became a diamond, | 0:55:09 | 0:55:18 | |
just like this, but of ten billion trillion trillion carats. | 0:55:18 | 0:55:21 | |
LAUGHTER | 0:55:21 | 0:55:23 | |
We understand in detail why such a thing can exist. | 0:55:23 | 0:55:27 | |
That's a diamond, light years away, intimately connected to this diamond, | 0:55:27 | 0:55:33 | |
and indeed, intimately connected to everything else | 0:55:33 | 0:55:35 | |
in the universe, by the laws of quantum physics. | 0:55:35 | 0:55:38 | |
What a remarkable testament to the power of the wavy behaviour of electrons, | 0:55:38 | 0:55:43 | |
and what a spectacular demonstration of the effectiveness of quantum theory. | 0:55:43 | 0:55:47 | |
Quantum theory is a uniquely potent tool that gives us | 0:55:47 | 0:55:51 | |
our best understanding of how the inconceivably small | 0:55:51 | 0:55:55 | |
can give rise to the inconceivably large. | 0:55:55 | 0:55:57 | |
It is THE most accurate way that we currently possess | 0:55:57 | 0:56:01 | |
to understand our universe. | 0:56:01 | 0:56:03 | |
It explains how atoms are empty yet solid, | 0:56:03 | 0:56:06 | |
how the wave-like behaviour of electrons creates the hardest known substances, | 0:56:06 | 0:56:11 | |
and how the real world emerges from subatomic particles | 0:56:11 | 0:56:15 | |
that explore the universe, the entire universe, in an instant. | 0:56:15 | 0:56:20 | |
There's nothing strange, there's nothing weird, there's no woo-woo. | 0:56:20 | 0:56:25 | |
It is just beautiful physics. Thank you. | 0:56:25 | 0:56:28 | |
APPLAUSE | 0:56:28 | 0:56:32 | |
It was mind-blowing. | 0:56:49 | 0:56:51 | |
I couldn't... Some of it I could understand, | 0:56:51 | 0:56:55 | |
other parts I could not understand. It was so exciting. I loved it. | 0:56:55 | 0:56:58 | |
I love listening to him because he does makes things clear. | 0:56:58 | 0:57:02 | |
He speaks at just the right pace for me to absorb it | 0:57:02 | 0:57:04 | |
and also he's got that very winning smile, so even though | 0:57:04 | 0:57:07 | |
he does insist on telling us how soon it is that the sun's going to die out | 0:57:07 | 0:57:11 | |
and we will all die screaming and flying off into the inky void of space, | 0:57:11 | 0:57:15 | |
you don't mind it because he looks so sweet when he tells you. | 0:57:15 | 0:57:18 | |
What do you now think of quantum physics? | 0:57:18 | 0:57:20 | |
I feel like I maybe should have stuck in at school a little bit more, | 0:57:20 | 0:57:24 | |
but you know, the career that I've chosen is going well, so... | 0:57:24 | 0:57:29 | |
But I have learnt a lot - mainly "don't volunteer for things"! | 0:57:29 | 0:57:34 | |
How are your hands now? | 0:57:34 | 0:57:36 | |
My hands are fine. All it does is singe the very fine hairs on the back. | 0:57:36 | 0:57:41 | |
But I was getting a bit, you know, gorilla-ish anyway, so he's probably done me a favour. | 0:57:41 | 0:57:46 | |
It was great. I loved it. It was fantastic. It was almost exactly about everything | 0:57:46 | 0:57:50 | |
I think about all the time. | 0:57:50 | 0:57:51 | |
Subtitles by Red Bee Media Ltd | 0:58:13 | 0:58:15 | |
E-mail [email protected] | 0:58:15 | 0:58:17 |