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Astronomers have long tried to understand our place as tiny specs | 0:00:07 | 0:00:12 | |
in the vastness of the universe. | 0:00:12 | 0:00:14 | |
But there is another expanse of the universe to explore, | 0:00:15 | 0:00:20 | |
a bizarre realm in which we are giants, | 0:00:20 | 0:00:23 | |
the weird world of the very small. | 0:00:23 | 0:00:26 | |
This is a journey into the heart of matter, | 0:00:29 | 0:00:32 | |
a journey down the biggest rabbit hole in history... | 0:00:32 | 0:00:35 | |
It's perfectly possible that in the high-energy end of our data, | 0:00:35 | 0:00:40 | |
right now we are occasionally making miniature black holes. | 0:00:40 | 0:00:44 | |
..a journey smaller than you can see, smaller than an atom, | 0:00:44 | 0:00:48 | |
where nothing is what it seems... | 0:00:48 | 0:00:50 | |
The more fundamental things are, | 0:00:50 | 0:00:53 | |
the nicer it is to look inside them. | 0:00:53 | 0:00:57 | |
..into a wonderland which seems far removed from reality... | 0:00:57 | 0:01:02 | |
Gravity is leaking into the extra dimensions. | 0:01:02 | 0:01:06 | |
..down to the very smallest structure of the universe. | 0:01:06 | 0:01:09 | |
We should expect space time to be not smooth as we presently imagine, | 0:01:13 | 0:01:18 | |
but more like the foam of a cappuccino. | 0:01:18 | 0:01:22 | |
The journey to find the smallest thing | 0:01:22 | 0:01:25 | |
may take us into another universe altogether. | 0:01:25 | 0:01:28 | |
But then of course, when you're down to this scale, | 0:01:29 | 0:01:33 | |
you may have the whole universe in your hand. | 0:01:33 | 0:01:35 | |
And at the bottom of the rabbit hole, | 0:01:35 | 0:01:38 | |
we may find that our universe is just one of many. | 0:01:38 | 0:01:42 | |
On top of an extinct volcano in the Canary Islands | 0:01:58 | 0:02:02 | |
a strange telescope called MAGIC stands guard. | 0:02:02 | 0:02:05 | |
It's on a ten-second stand-by | 0:02:11 | 0:02:13 | |
to respond to the most violent explosions in the cosmos. | 0:02:13 | 0:02:17 | |
With its laser-aligned panels, it is detecting the fallout | 0:02:22 | 0:02:27 | |
from cosmic rays that have travelled half way across the universe. | 0:02:27 | 0:02:31 | |
And it's helping physicists answer an eternal question. | 0:02:35 | 0:02:40 | |
Well, at the end of the day, the question comes up, why do we exist, | 0:02:40 | 0:02:45 | |
and not only we as mankind, but why does this planet exist, | 0:02:45 | 0:02:49 | |
the solar system, the universe? | 0:02:49 | 0:02:50 | |
If you want to know why the universe exists, you need to look, | 0:02:52 | 0:02:57 | |
not to the very big, but to the very small. | 0:02:57 | 0:03:00 | |
And it turns out there need to be a very small number of parameters | 0:03:00 | 0:03:06 | |
very finely adjusted for the universe to be as it is | 0:03:06 | 0:03:10 | |
and for us to sit in this universe, to be able to observe it. | 0:03:10 | 0:03:13 | |
So I think this tells why it's important to understand | 0:03:13 | 0:03:16 | |
how the laws of nature work. | 0:03:16 | 0:03:18 | |
And the strangest thing about MAGIC, | 0:03:24 | 0:03:27 | |
is that it's not really a telescope at all. | 0:03:27 | 0:03:30 | |
It's the eyepiece of the biggest microscope in the world. | 0:03:31 | 0:03:34 | |
It's just one of the incredible tools scientists have developed | 0:03:37 | 0:03:41 | |
in their ongoing search for the smallest thing in the universe. | 0:03:41 | 0:03:45 | |
Look at that! | 0:03:57 | 0:03:59 | |
The nucleus and the electrons going around the atom. | 0:03:59 | 0:04:01 | |
The exploration of the most distant, | 0:04:01 | 0:04:04 | |
unreachable territory in our universe is challenging | 0:04:04 | 0:04:07 | |
the minds of our greatest scientists. | 0:04:07 | 0:04:09 | |
-Very nice. -This is very complex, very complicated. | 0:04:09 | 0:04:13 | |
Am I getting there? Aargh! | 0:04:13 | 0:04:15 | |
As you look smaller and smaller, | 0:04:15 | 0:04:17 | |
no-one knows if there will ever be an end. | 0:04:17 | 0:04:20 | |
Well, with me you'll see the more determination to find the next layer. | 0:04:21 | 0:04:26 | |
I'm going to need a bigger collider soon. | 0:04:26 | 0:04:28 | |
So we split, even split the nucleus. | 0:04:28 | 0:04:31 | |
The hunt for the smallest thing in the universe | 0:04:32 | 0:04:35 | |
is challenging our understanding | 0:04:35 | 0:04:39 | |
of the very nature of space and time. | 0:04:39 | 0:04:42 | |
Yes. This is it. This is the smallest piece. | 0:04:44 | 0:04:49 | |
That is the smallest thing, isn't it? | 0:04:49 | 0:04:51 | |
Nice analogy! | 0:04:53 | 0:04:56 | |
The search for the smallest building blocks of the universe | 0:05:00 | 0:05:04 | |
is one of the oldest in science. | 0:05:04 | 0:05:07 | |
For almost 1,000 years, this medieval cathedral has looked over | 0:05:07 | 0:05:11 | |
the streets of Aachen in Germany, | 0:05:11 | 0:05:13 | |
an enduring monument of stone and glass. | 0:05:13 | 0:05:17 | |
But if you look really, really closely, | 0:05:18 | 0:05:21 | |
all is not what it seems. | 0:05:21 | 0:05:23 | |
Professor Joachim Mayer is a man with a unique view on the world. | 0:05:28 | 0:05:32 | |
He sees the bizarre changes that come about | 0:05:34 | 0:05:36 | |
when you view the world in terms | 0:05:36 | 0:05:39 | |
of the building blocks of stuff - | 0:05:39 | 0:05:41 | |
atoms. | 0:05:41 | 0:05:43 | |
Where you or I might see red, he sees gold. | 0:05:45 | 0:05:50 | |
There are always two parts of your brain. | 0:05:51 | 0:05:53 | |
If you look, if you come in as a human being | 0:05:53 | 0:05:55 | |
but as a scientist as well, | 0:05:55 | 0:05:57 | |
you are stunned by what people have built in these medieval times. | 0:05:57 | 0:06:02 | |
And then you ask yourself what kind of materials did they use? | 0:06:02 | 0:06:05 | |
If you look for example at these glass windows, it's very well known | 0:06:05 | 0:06:11 | |
that actually nanotechnology is used in some of the colours, for example | 0:06:11 | 0:06:17 | |
gold nanoparticles actually, produce the most durable red colour | 0:06:17 | 0:06:21 | |
which can be produced. And it's still a miracle to us | 0:06:21 | 0:06:24 | |
how in these ancient times, you know, the people found out | 0:06:24 | 0:06:29 | |
that this is the most efficient way to produce a red colour. | 0:06:29 | 0:06:32 | |
The red is just an illusion caused by the massive difference in scale | 0:06:32 | 0:06:38 | |
between the tiny clumps of gold atoms and us - | 0:06:38 | 0:06:42 | |
the giants who see red. | 0:06:42 | 0:06:44 | |
It's one of the reasons | 0:06:46 | 0:06:47 | |
scientists are obsessed with reaching the smallest scales. | 0:06:47 | 0:06:51 | |
Things don't just get smaller, they change. | 0:06:51 | 0:06:55 | |
Scientists have thought for a long time | 0:06:55 | 0:06:59 | |
what are the smallest building blocks of our matter, | 0:06:59 | 0:07:02 | |
and you can see beautiful matter around us. | 0:07:02 | 0:07:06 | |
But just how small are these building blocks? | 0:07:06 | 0:07:10 | |
If we start on the familiar scale of a human | 0:07:11 | 0:07:14 | |
and zoom in ten times closer, | 0:07:14 | 0:07:16 | |
we get to the size of a face. | 0:07:16 | 0:07:20 | |
Magnify by ten once more, and we are looking at the iris of an eye. | 0:07:20 | 0:07:26 | |
100 times closer and we can see a human hair, | 0:07:26 | 0:07:30 | |
magnified 10,000 times. | 0:07:30 | 0:07:32 | |
Microscopes have unveiled a world | 0:07:33 | 0:07:36 | |
smaller than the wavelength of light. | 0:07:36 | 0:07:38 | |
But the ability to see individual atoms has, until recently, | 0:07:38 | 0:07:43 | |
been a dream. | 0:07:43 | 0:07:45 | |
As microscopes have got bigger and more powerful, | 0:07:51 | 0:07:54 | |
they have allowed us to peer ever smaller. | 0:07:54 | 0:07:58 | |
It was the ancient Greeks who first dreamed up the idea of atoms. | 0:08:02 | 0:08:07 | |
100 years ago, scientists proved they exist. | 0:08:10 | 0:08:14 | |
But it's only in the last ten years | 0:08:14 | 0:08:17 | |
that we've actually been able to see them. | 0:08:17 | 0:08:20 | |
And now, behind these doors, | 0:08:25 | 0:08:26 | |
Joachim Mayer has a machine that gives us the best possible view. | 0:08:26 | 0:08:30 | |
MUSIC: "Also Sprach Zarathustra" by Richard Strauss | 0:08:30 | 0:08:38 | |
It looks like a giant coffee maker! | 0:09:04 | 0:09:06 | |
So this is our new PICO instrument, | 0:09:09 | 0:09:13 | |
which has been installed about a year ago. | 0:09:13 | 0:09:16 | |
And with its special new corrector for the chromatic aberration, | 0:09:16 | 0:09:20 | |
is really a very unique machine which really offers us new possibilities. | 0:09:20 | 0:09:26 | |
I think with its new capabilities, we consider it | 0:09:26 | 0:09:30 | |
as the best electron microscope in the world. | 0:09:30 | 0:09:32 | |
Being the best electron microscope in the world, | 0:09:32 | 0:09:36 | |
PICO is very sensitive to its surroundings. | 0:09:36 | 0:09:40 | |
Even a person's body heat would disturb it, | 0:09:40 | 0:09:42 | |
so PICO has to be operated remotely. | 0:09:42 | 0:09:47 | |
And, safely isolated from humans, | 0:09:48 | 0:09:51 | |
PICO is able to unveil the secret world of the very small. | 0:09:51 | 0:09:55 | |
We start our investigations at a very small magnification, | 0:09:57 | 0:10:02 | |
which is equivalent to the highest magnification, which you can actually reach | 0:10:02 | 0:10:05 | |
with a light microscope. At this magnification, | 0:10:05 | 0:10:09 | |
the diameter of a human hair would be about that size. | 0:10:09 | 0:10:12 | |
And now we can in magnification | 0:10:12 | 0:10:15 | |
go at least a factor of 1,000 higher. | 0:10:15 | 0:10:19 | |
And now we start to see the structure, | 0:10:22 | 0:10:26 | |
actually these black dots are individual gold nanoparticles. | 0:10:26 | 0:10:30 | |
And now you can see the individual atoms | 0:10:32 | 0:10:36 | |
as they appear in this individual nanoparticle. | 0:10:36 | 0:10:39 | |
So we see individual atoms aligned in the structure. | 0:10:41 | 0:10:45 | |
It's hard to imagine just how small these dots of matter really are. | 0:10:52 | 0:10:58 | |
But consider that each of us contains | 0:10:59 | 0:11:02 | |
about seven billion, billion, billion atoms. | 0:11:02 | 0:11:06 | |
That's more than the number of stars in the entire universe. | 0:11:07 | 0:11:12 | |
PICO is, quite simply, the most powerful microscope in the world. | 0:11:19 | 0:11:24 | |
After magnifying things a billion times, we can actually see | 0:11:26 | 0:11:31 | |
the individual atoms that make up everything in the universe. | 0:11:31 | 0:11:35 | |
This is the smallest thing we can see. | 0:11:36 | 0:11:39 | |
It may well be the smallest thing we'll ever be able to see. | 0:11:39 | 0:11:43 | |
These atoms look reassuringly like what you'd expect - | 0:11:44 | 0:11:48 | |
solid round balls of stuff. | 0:11:48 | 0:11:51 | |
But this is merely an illusion. | 0:11:51 | 0:11:55 | |
If you want to find out what an atom really looks like, | 0:12:05 | 0:12:08 | |
you need a whole new way of looking. | 0:12:08 | 0:12:10 | |
Professor Andy Parker is trying to find things | 0:12:12 | 0:12:15 | |
smaller than anyone has ever found. | 0:12:15 | 0:12:18 | |
Well, the way to look inside an atom | 0:12:23 | 0:12:25 | |
is to fire something at it very fast, | 0:12:25 | 0:12:27 | |
and if you hit it hard enough it you can break it into little bits. | 0:12:27 | 0:12:31 | |
He's using the most expensive experiment | 0:12:31 | 0:12:34 | |
in the history of physics, | 0:12:34 | 0:12:36 | |
one he helped design. | 0:12:36 | 0:12:39 | |
At 17 miles long, and buried 100 metres underground, | 0:12:39 | 0:12:43 | |
it is the biggest, and most famous particle accelerator in the world - | 0:12:43 | 0:12:48 | |
the Large Hadron Collider. | 0:12:48 | 0:12:50 | |
The ring goes right over behind the apartment blocks there, | 0:12:50 | 0:12:53 | |
and then it goes five miles in that direction, | 0:12:53 | 0:12:56 | |
roughly to the horizon, | 0:12:56 | 0:12:58 | |
it comes round under the base of the mountains to here, | 0:12:58 | 0:13:01 | |
and it sweeps back round, | 0:13:01 | 0:13:04 | |
past those buildings there and back to point one. | 0:13:04 | 0:13:07 | |
But once you start looking inside an atom, nothing is what it seems. | 0:13:09 | 0:13:14 | |
People always imagine atoms as billiard balls, | 0:13:16 | 0:13:18 | |
they've seen pictures of atoms as billiard balls | 0:13:18 | 0:13:20 | |
or with a little electron going round quite a big nucleus, | 0:13:20 | 0:13:23 | |
and this is a completely false picture. | 0:13:23 | 0:13:25 | |
If you blew up an atom to the size of the Large Hadron Collider, | 0:13:25 | 0:13:28 | |
so it would be five miles in that direction... | 0:13:28 | 0:13:30 | |
..all around there on that piece of landscape... | 0:13:32 | 0:13:35 | |
..then the nucleus would be about ten centimetres across, | 0:13:36 | 0:13:39 | |
about the size of this tennis ball. | 0:13:39 | 0:13:40 | |
So all the mass, all the weight of the atom | 0:13:40 | 0:13:42 | |
is condensed into this tiny little nucleus, | 0:13:42 | 0:13:46 | |
and the whole space around it is empty, apart from these few electrons buzzing around. | 0:13:46 | 0:13:50 | |
The illusion of solidity | 0:13:58 | 0:13:59 | |
comes from the fuzzy cloud of charged electrons. | 0:13:59 | 0:14:03 | |
But on their own, | 0:14:03 | 0:14:04 | |
they weigh virtually nothing and occupy no space. | 0:14:04 | 0:14:08 | |
You need to go a 100,000 times smaller | 0:14:09 | 0:14:12 | |
to get to the nucleus - a fizzing ball of protons and neutrons. | 0:14:12 | 0:14:17 | |
The challenge here at the LHC, | 0:14:20 | 0:14:22 | |
is to look inside the protons by smashing them to pieces. | 0:14:22 | 0:14:26 | |
It's brute force and ignorance really. | 0:14:30 | 0:14:33 | |
You are taking two things, which are very, very small, | 0:14:33 | 0:14:35 | |
you don't really know what's inside them to start with, | 0:14:35 | 0:14:38 | |
and you hit them together as hard as you can | 0:14:38 | 0:14:40 | |
and they smash into tiny fragments and since you really don't know | 0:14:40 | 0:14:44 | |
what the elaborate structure is inside, it's kind of like | 0:14:44 | 0:14:46 | |
colliding two clocks together and then sweeping up the mess | 0:14:46 | 0:14:50 | |
that you get and trying to figure out how the clock works. | 0:14:50 | 0:14:53 | |
And you can't do it in a subtle way. | 0:15:02 | 0:15:04 | |
There's no screwdriver to take a proton to bits | 0:15:04 | 0:15:06 | |
and there's no plan of what's inside | 0:15:06 | 0:15:08 | |
so you have to hit them very hard, then the fragments come flying out | 0:15:08 | 0:15:12 | |
and from that we can try and work out, | 0:15:12 | 0:15:14 | |
how all the cogs and gearwheels fit back together to make a proton. | 0:15:14 | 0:15:17 | |
The debris from the proton collisions | 0:15:22 | 0:15:25 | |
is detected by a vast machine called ATLAS. | 0:15:25 | 0:15:28 | |
Everything interesting happens at the centre, | 0:15:31 | 0:15:33 | |
that's where the particles collide. | 0:15:33 | 0:15:35 | |
This engineering mock-up shows just one section of the real machine. | 0:15:40 | 0:15:45 | |
And the sensitive instrument at its very heart is the part made by Andy. | 0:15:45 | 0:15:50 | |
So I'm in the middle of the mock-up of ATLAS, | 0:15:50 | 0:15:53 | |
and this is where all the action happens. | 0:15:53 | 0:15:55 | |
The beams would come in from both ends through the centre here. | 0:15:55 | 0:15:58 | |
This would of course be filled with detectors, but the beam pipe | 0:15:58 | 0:16:01 | |
would run right through the centre and the particles, which are | 0:16:01 | 0:16:04 | |
travelling in vacuum at almost the speed of light, collide head on | 0:16:04 | 0:16:07 | |
just here, and do their stuff and then all the debris comes flying out | 0:16:07 | 0:16:12 | |
and it flies through the detector layers... | 0:16:12 | 0:16:15 | |
..and that's the debris that we use to reconstruct the collision | 0:16:17 | 0:16:20 | |
that happens right here in the middle. | 0:16:20 | 0:16:22 | |
And what you find when you smash a proton to pieces, | 0:16:24 | 0:16:28 | |
is that it too is largely empty space. | 0:16:28 | 0:16:31 | |
It is made of three tiny fundamental particles called quarks. | 0:16:32 | 0:16:37 | |
But to reach the size of a quark we have to zoom in | 0:16:38 | 0:16:42 | |
1,000 times smaller. | 0:16:42 | 0:16:44 | |
Some of the earliest machines used to probe the atom | 0:16:52 | 0:16:56 | |
were bubble chambers, that produced exquisite pictures | 0:16:56 | 0:16:58 | |
of the heart of matter. | 0:16:58 | 0:17:01 | |
What you see here is a sudden explosion of particles from nowhere | 0:17:03 | 0:17:07 | |
in the liquid of the bubble chamber and that is because | 0:17:07 | 0:17:09 | |
a neutrino has hit an atomic nucleus there and smashed it to pieces, | 0:17:09 | 0:17:13 | |
and we see the particles flying off. | 0:17:13 | 0:17:16 | |
And that's anti-matter. | 0:17:18 | 0:17:19 | |
That's matter and anti-matter being created from pure energy. | 0:17:19 | 0:17:23 | |
Very, very beautiful image. | 0:17:23 | 0:17:25 | |
So this is the map or a part of the map, of what nature can do. | 0:17:25 | 0:17:31 | |
So it's part of the map of the universe. | 0:17:32 | 0:17:34 | |
But now, after 80 years of smashing, the map is complete. | 0:17:38 | 0:17:42 | |
In the summer of 2012 scientists at the LHC, | 0:17:44 | 0:17:47 | |
announced the discovery of the famous Higgs particle. | 0:17:47 | 0:17:51 | |
It's the final piece of what's called the Standard Model - | 0:17:52 | 0:17:55 | |
a set of 17 fundamental particles | 0:17:55 | 0:17:58 | |
including quarks and electrons | 0:17:58 | 0:18:01 | |
that make up everything we know. | 0:18:01 | 0:18:03 | |
But for physicists like Andy | 0:18:12 | 0:18:14 | |
it's not the end of the story. | 0:18:14 | 0:18:17 | |
Everyone's heard about the Higgs | 0:18:17 | 0:18:19 | |
but the story goes much beyond that. | 0:18:19 | 0:18:23 | |
In fact my main interest is beyond the Higgs. | 0:18:23 | 0:18:26 | |
Like any great explorer, Andy is not satisfied | 0:18:29 | 0:18:33 | |
that this is the end of the journey. | 0:18:33 | 0:18:35 | |
There may be plenty more to discover. | 0:18:36 | 0:18:39 | |
OK so we're in the ATLAS main control room, | 0:18:39 | 0:18:42 | |
where the experiment crew, shift crew here are sitting taking data today. | 0:18:42 | 0:18:46 | |
This is live data coming from the detector - | 0:18:46 | 0:18:48 | |
collisions that are happening now. | 0:18:48 | 0:18:50 | |
Collisions are happening 40 million times every second. | 0:18:50 | 0:18:53 | |
And as the energy of the collisions increases, | 0:18:55 | 0:18:58 | |
Andy will be able to look on smaller and smaller scales, | 0:18:58 | 0:19:02 | |
even delving inside the so-called fundamental particles. | 0:19:02 | 0:19:07 | |
Fundamental particles is a myth, I think. | 0:19:09 | 0:19:12 | |
It looks at the moment | 0:19:12 | 0:19:13 | |
as if quarks and electrons are point-like particles. | 0:19:13 | 0:19:16 | |
We can't see any size to them but that is just because | 0:19:16 | 0:19:19 | |
we haven't been able to measure very short distances around them. | 0:19:19 | 0:19:22 | |
What I'd like to see is what's going on inside them. | 0:19:22 | 0:19:25 | |
So we're looking for the innards of the quarks | 0:19:25 | 0:19:27 | |
by smashing them together as hard as we can. | 0:19:27 | 0:19:29 | |
In the search for the smallest piece of the universe, | 0:19:37 | 0:19:40 | |
part of the problem may be knowing when to stop. | 0:19:40 | 0:19:43 | |
Each new layer reveals great secrets. | 0:19:44 | 0:19:48 | |
But does this search have an end? | 0:19:48 | 0:19:50 | |
Or within every small thing, | 0:19:52 | 0:19:55 | |
is there another... | 0:19:55 | 0:19:57 | |
..and another? | 0:19:58 | 0:20:00 | |
Perhaps the best known of all the fundamental particles | 0:20:18 | 0:20:21 | |
is the electron. | 0:20:21 | 0:20:23 | |
It underpins much of our modern lives, | 0:20:24 | 0:20:27 | |
from computers to street lights to televisions. | 0:20:27 | 0:20:31 | |
But for theoretical physicist professor Jeroen van den Brink, | 0:20:31 | 0:20:35 | |
the electron might not be as fundamental as we think. | 0:20:35 | 0:20:39 | |
The more fundamental things are, | 0:20:39 | 0:20:42 | |
the nicer it is to look inside them. | 0:20:42 | 0:20:45 | |
Physics it's always that something appears to be fundamental, | 0:20:46 | 0:20:51 | |
and just because we believe it's fundamental we take the next step | 0:20:51 | 0:20:54 | |
and try to look what's inside it. | 0:20:54 | 0:20:57 | |
Jeroen's idea was that, rather than smashing electrons into pieces, | 0:21:10 | 0:21:15 | |
he could find a different way to split its properties... | 0:21:15 | 0:21:20 | |
the very properties that make it so useful. | 0:21:21 | 0:21:26 | |
So the electron has three fundamental properties, | 0:21:26 | 0:21:30 | |
charge, spin and orbital and theoretically | 0:21:30 | 0:21:36 | |
it's definitely possible to split those three parts of the electron. | 0:21:36 | 0:21:42 | |
If you do the mathematics | 0:21:42 | 0:21:45 | |
there is no problem in doing that. | 0:21:45 | 0:21:47 | |
If you do the quantum mechanics, it's completely allowed. | 0:21:47 | 0:21:50 | |
So in principle you can split the electron, | 0:21:50 | 0:21:54 | |
at least you can do it on paper. | 0:21:54 | 0:21:55 | |
If you want to want to do it in practice, you need this... | 0:21:55 | 0:22:01 | |
Watch your head here. | 0:22:01 | 0:22:03 | |
..the Swiss Light Source, | 0:22:03 | 0:22:05 | |
a million watt light bulb. | 0:22:05 | 0:22:08 | |
This is an in vacuum undulator. | 0:22:08 | 0:22:12 | |
The Swiss Light Source is in fact the Swiss X-ray Source. | 0:22:12 | 0:22:17 | |
We have digital BPM systems. | 0:22:17 | 0:22:19 | |
Inside the ring, under the care of Dr Andreas Ludeke, | 0:22:19 | 0:22:23 | |
a beam of electrons creates the ultimate X-ray laser. | 0:22:23 | 0:22:27 | |
This is a superconducting cavity. | 0:22:27 | 0:22:30 | |
It's one of the most powerful, highly focused, narrow X-ray beams | 0:22:30 | 0:22:34 | |
in the world. | 0:22:34 | 0:22:36 | |
We have a high intense magnetic field in the middle. | 0:22:36 | 0:22:40 | |
The perfect tool for probing down to the size of an electron. | 0:22:40 | 0:22:45 | |
Jeroen's partner in electron splitting, | 0:22:45 | 0:22:47 | |
the man who devised and runs the experiment, | 0:22:47 | 0:22:50 | |
is Dr Thorsten Schmitt. | 0:22:50 | 0:22:52 | |
So here we are in the so-called optical hutch, | 0:22:54 | 0:22:56 | |
where all the crucial optical elements - | 0:22:56 | 0:23:01 | |
mirrors which are optimized for X-rays and which are used | 0:23:01 | 0:23:07 | |
for shaping the beam quality are sitting. | 0:23:07 | 0:23:10 | |
-I can see it here. -Yeah. | 0:23:10 | 0:23:12 | |
So when I come here I go to the equipment, I look at it, | 0:23:14 | 0:23:19 | |
I admire it and then I go back and sit behind a computer | 0:23:19 | 0:23:25 | |
or take my pen and paper and start to do the mathematics. | 0:23:25 | 0:23:30 | |
I do not really understand what the stuff out here is exactly doing | 0:23:30 | 0:23:34 | |
and I believe, I'm sure Thorsten does and they do the experiments. | 0:23:34 | 0:23:39 | |
We have X-rays, which are coming in and hit a sample, | 0:23:44 | 0:23:49 | |
and we will then in the end analyse the X-rays, which are re-emitted | 0:23:49 | 0:23:52 | |
or scattered off from the sample. | 0:23:52 | 0:23:56 | |
When the X-ray beam strikes, | 0:24:01 | 0:24:03 | |
the electrons split into new quasi-particles. | 0:24:03 | 0:24:07 | |
These particles, called spinons, orbitons and holons, | 0:24:09 | 0:24:14 | |
carry the properties of the electron, | 0:24:14 | 0:24:16 | |
and can travel off in different directions. | 0:24:16 | 0:24:20 | |
This is actually the picture that tells the whole story. | 0:24:23 | 0:24:26 | |
The most important part is here, this red part, | 0:24:26 | 0:24:30 | |
and what's important is that it's wavy. | 0:24:30 | 0:24:34 | |
And this waviness tells us that what happened in this experiment | 0:24:34 | 0:24:37 | |
is that the electron was split into spinons and orbitons. | 0:24:37 | 0:24:41 | |
So this is the picture | 0:24:41 | 0:24:43 | |
that is the experimental proof that the electron has been split. | 0:24:43 | 0:24:47 | |
Are you proud of that picture? | 0:24:52 | 0:24:53 | |
I'm very proud of the picture. | 0:24:53 | 0:24:56 | |
So the electron can be split into these three different particles, | 0:25:03 | 0:25:06 | |
but, really, what can you do with those particles when you have them? | 0:25:06 | 0:25:11 | |
I don't have a good answer to that. | 0:25:11 | 0:25:13 | |
It's just cool to make these, make this electron that is so | 0:25:13 | 0:25:18 | |
fundamental, that's so part... That's the first fundamental particle | 0:25:18 | 0:25:22 | |
that was discovered, to see it split into its three different parts. | 0:25:22 | 0:25:26 | |
That's what I like about the experiment. | 0:25:31 | 0:25:33 | |
The electron has, in one sense, been split in three. | 0:25:37 | 0:25:41 | |
But it's a measure of just how weird things are down here | 0:25:42 | 0:25:45 | |
that it's still considered to be fundamental. | 0:25:45 | 0:25:49 | |
Down at this scale, | 0:25:49 | 0:25:51 | |
we just have to accept that the rules become deeply strange. | 0:25:51 | 0:25:55 | |
And if we reach down even further, | 0:25:56 | 0:25:58 | |
we may have to throw out the rule book altogether. | 0:25:58 | 0:26:01 | |
Back at the LHC, far beyond the Higgs, | 0:26:12 | 0:26:16 | |
smaller than the innards of a quark, Andy Parker believes ATLAS | 0:26:16 | 0:26:20 | |
could reveal something that, at this tiny scale, shouldn't really exist. | 0:26:20 | 0:26:26 | |
So this great big building here is at the top of the ATLAS pit. | 0:26:27 | 0:26:31 | |
100 metres straight down is the detector, | 0:26:31 | 0:26:32 | |
which is operating at the moment, | 0:26:32 | 0:26:34 | |
so we're not allowed in the building for safety reasons. | 0:26:34 | 0:26:37 | |
He is hoping to make one of the most fearsome objects in the universe - | 0:26:37 | 0:26:41 | |
a black hole... | 0:26:41 | 0:26:43 | |
Si je produis des problemes pour Atlas, je suis "eeeek"! | 0:26:43 | 0:26:47 | |
..a place where gravity is so vastly strong that nothing - | 0:26:47 | 0:26:51 | |
not even light - can escape. | 0:26:51 | 0:26:53 | |
Problem is, if they open it, that could set off the pit alarms. | 0:26:53 | 0:26:58 | |
It takes the entire mass of an imploding star, | 0:27:02 | 0:27:05 | |
condensed into the space of a small town, | 0:27:05 | 0:27:08 | |
to create the extreme gravitational pull of a black hole. | 0:27:08 | 0:27:12 | |
They are normally vast, and live at the centre of galaxies. | 0:27:14 | 0:27:18 | |
And yet Andy Parker is trying conjure a micro black hole | 0:27:18 | 0:27:23 | |
right here at CERN, using just a couple of protons. | 0:27:23 | 0:27:28 | |
It's perfectly possible that in the high-energy end of our data | 0:27:28 | 0:27:31 | |
right now we are occasionally making miniature black holes. | 0:27:31 | 0:27:34 | |
The protons are colliding below us, they come together, | 0:27:37 | 0:27:40 | |
they have a lot of energy in them. And gravity cares about energy. | 0:27:40 | 0:27:43 | |
It's the same as mass as far as gravity is concerned. | 0:27:43 | 0:27:45 | |
So if you put a lot of energy in a small space, | 0:27:45 | 0:27:47 | |
as we're doing right now, | 0:27:47 | 0:27:49 | |
then you could potentially form a quantum-sized black hole. | 0:27:49 | 0:27:52 | |
A very, very tiny black hole. | 0:27:52 | 0:27:53 | |
It wouldn't be stable, it wouldn't last a long time | 0:27:53 | 0:27:56 | |
and eat the planet, it would disappear in a puff of radiation, | 0:27:56 | 0:27:59 | |
and we would see that puff of radiation in our detector. | 0:27:59 | 0:28:02 | |
The only way it would be possible to make these micro black holes, | 0:28:05 | 0:28:09 | |
at least 20,000 times smaller than a proton, | 0:28:09 | 0:28:13 | |
is if, on the level of the really, really small, we discover | 0:28:13 | 0:28:18 | |
that gravity is vastly stronger than it seems in everyday life. | 0:28:18 | 0:28:23 | |
And that would change our view of the familiar world, | 0:28:26 | 0:28:30 | |
and challenge something we all take for granted - | 0:28:30 | 0:28:33 | |
that we live in a world of three-dimensional space. | 0:28:33 | 0:28:36 | |
So this seems to be a perfectly ordinary three-dimensional world. | 0:28:38 | 0:28:41 | |
There are three ways I can go. | 0:28:41 | 0:28:42 | |
I can go forwards and backwards, side to side, up and down. | 0:28:42 | 0:28:46 | |
There can't be anything much more than that, can there? | 0:28:46 | 0:28:48 | |
So if I want to go up the tower, for example, over there, | 0:28:48 | 0:28:51 | |
I go sideways, I go forwards and I go up. | 0:28:51 | 0:28:55 | |
Seems to be the only possibilities. | 0:28:55 | 0:28:57 | |
But not necessarily. | 0:29:01 | 0:29:03 | |
If we could conjure up an extra dimension, | 0:29:04 | 0:29:07 | |
it could explain how you get super gravity at the tiny scale. | 0:29:07 | 0:29:12 | |
Because, although gravity seems strong in our everyday lives, | 0:29:13 | 0:29:17 | |
it's actually pretty feeble. | 0:29:17 | 0:29:19 | |
Gravity is a puzzle. | 0:29:30 | 0:29:32 | |
It's very, very much weaker than the other forces - | 0:29:32 | 0:29:34 | |
actually a million, million, million times weaker than the other forces. | 0:29:34 | 0:29:37 | |
It feels strong to us - right here, | 0:29:37 | 0:29:39 | |
I'm feeling uncomfortable about gravity pulling me over the edge. | 0:29:39 | 0:29:43 | |
But that's because there's a whole planet there pulling me downwards. | 0:29:43 | 0:29:46 | |
The other forces that are hard at work holding the world together, | 0:29:50 | 0:29:53 | |
including the electromagnetic force, | 0:29:53 | 0:29:56 | |
are all vastly stronger than gravity. | 0:29:56 | 0:29:58 | |
So here's a little magnet. | 0:30:01 | 0:30:03 | |
And this key, being held down | 0:30:03 | 0:30:06 | |
by all the atoms in the entire planet pulling towards the centre. | 0:30:06 | 0:30:11 | |
And this feeble little magnet can overcome | 0:30:11 | 0:30:14 | |
the gravity of the whole planet quite easily. | 0:30:14 | 0:30:17 | |
Now, why is gravity so weak? | 0:30:17 | 0:30:19 | |
Well, one possible explanation is that it's not actually weak. | 0:30:19 | 0:30:22 | |
It's just as strong as the other forces, | 0:30:22 | 0:30:24 | |
but we're missing part of it, | 0:30:24 | 0:30:26 | |
and gravity is leaking into the extra dimensions, | 0:30:26 | 0:30:29 | |
and so when we calculate the strength of gravity, | 0:30:29 | 0:30:31 | |
we're only seeing the piece that's in 3D. | 0:30:31 | 0:30:33 | |
Most of our gravity could be leaking off into the fourth dimension. | 0:30:35 | 0:30:39 | |
All we get is the leftovers. | 0:30:39 | 0:30:42 | |
This would account for the feebleness of gravity, | 0:30:43 | 0:30:47 | |
but where could this fourth dimension be hiding? | 0:30:47 | 0:30:50 | |
Well, if there is an extra dimension, it's everywhere. | 0:30:50 | 0:30:53 | |
The question is, why can't we see it? | 0:30:53 | 0:30:55 | |
All the others we can go off to infinity along these directions | 0:30:58 | 0:31:02 | |
but maybe the reason we can't see the fourth dimension is that | 0:31:02 | 0:31:05 | |
it's actually curled up. | 0:31:05 | 0:31:07 | |
If you went into it, you'd go round in a little circle | 0:31:07 | 0:31:09 | |
and come back on yourself, just like if you travelled on the surface | 0:31:09 | 0:31:12 | |
of the Earth far enough, you'd come back to where you started. | 0:31:12 | 0:31:15 | |
But this would be on a very, very small scale. | 0:31:15 | 0:31:18 | |
Hiding an extra dimension may sound tricky, | 0:31:20 | 0:31:23 | |
but it's all a matter of scale. | 0:31:23 | 0:31:26 | |
It's a very strange concept, | 0:31:27 | 0:31:29 | |
but you can see it for people who live in a flat world. | 0:31:29 | 0:31:31 | |
If we look down on the people down below, then they're | 0:31:31 | 0:31:35 | |
moving around on a surface, which is pretty much flat, and looked at | 0:31:35 | 0:31:38 | |
from this large distance up, it just looks completely flat | 0:31:38 | 0:31:41 | |
and they move about, they cannot go up and down because they can't fly. | 0:31:41 | 0:31:45 | |
From a great height, the tiny people seem to live in two dimensions. | 0:31:55 | 0:32:01 | |
But if we zoom into the same scale as the ant people, | 0:32:03 | 0:32:06 | |
you realise they can actually move up and down as well. | 0:32:06 | 0:32:10 | |
Similarly, if we could get down to a small enough scale, | 0:32:13 | 0:32:16 | |
we might find there is a fourth dimension curled up. | 0:32:16 | 0:32:20 | |
It may sound an outlandish theory, | 0:32:21 | 0:32:24 | |
but if Andy spots his baby black holes, all this would be true. | 0:32:24 | 0:32:29 | |
If we did see evidence of black holes at the LHC, that would be | 0:32:30 | 0:32:33 | |
absolutely amazing because it tells us that everything we think | 0:32:33 | 0:32:36 | |
we know about gravity, general relativity and so on, isn't right. | 0:32:36 | 0:32:40 | |
Then you would have demonstrated that the world is not | 0:32:40 | 0:32:43 | |
three-dimensional, but four-dimensional or more. | 0:32:43 | 0:32:46 | |
And you would have made a black hole in the lab. | 0:32:46 | 0:32:48 | |
So you get the Nobel Prize for making a black hole in the lab, | 0:32:48 | 0:32:50 | |
you get the Nobel Prize for proving general relativity wrong, | 0:32:50 | 0:32:53 | |
and you get the Nobel Prize | 0:32:53 | 0:32:54 | |
for demonstrating that the universe is multi-dimensional. | 0:32:54 | 0:32:57 | |
I mean, how cool is that? | 0:32:57 | 0:32:59 | |
On our journey to find the smallest thing in the universe, | 0:33:01 | 0:33:04 | |
things have indeed become deeply strange. | 0:33:04 | 0:33:07 | |
We have dived down a rabbit hole into a bizarre wonderland | 0:33:08 | 0:33:11 | |
where extra dimensions may lie curled and hidden from our view. | 0:33:11 | 0:33:16 | |
But that's just the beginning of the weirdness. | 0:33:16 | 0:33:21 | |
As we look even smaller, beyond even the reach | 0:33:21 | 0:33:24 | |
of the Large Hadron Collider, we have to rely on theory alone. | 0:33:24 | 0:33:28 | |
Professor Michael Green is a founding father | 0:33:48 | 0:33:52 | |
of one of the strangest theories in physics. | 0:33:52 | 0:33:54 | |
A theory that tells us that the universe is made of strings. | 0:33:58 | 0:34:03 | |
String theory starts off simply enough, | 0:34:09 | 0:34:12 | |
but it leads to some mind-boggling conclusions. | 0:34:12 | 0:34:15 | |
The fundamental particles, instead of being point-like objects | 0:34:19 | 0:34:22 | |
are now thought of as being string-like objects. | 0:34:22 | 0:34:25 | |
Instead of the 17 particles in the standard model, | 0:34:28 | 0:34:31 | |
everything is made from a single object - | 0:34:31 | 0:34:34 | |
an incredibly tiny loop of string. | 0:34:34 | 0:34:37 | |
The characteristic feature of a string, which makes it | 0:34:39 | 0:34:42 | |
different from a point is that it can vibrate | 0:34:42 | 0:34:45 | |
and the different modes of vibration, the different notes, if you like, | 0:34:45 | 0:34:49 | |
are seen as different kinds of particles. | 0:34:49 | 0:34:52 | |
So there's this very appealing, | 0:34:54 | 0:34:56 | |
almost poetic way in which string theory describes all the particles | 0:34:56 | 0:35:00 | |
in terms of different notes on a string. | 0:35:00 | 0:35:03 | |
It's like the music of the spheres almost. | 0:35:03 | 0:35:05 | |
It's a beautifully neat idea. | 0:35:10 | 0:35:13 | |
Each note from the vibrating string produces a different particle. | 0:35:13 | 0:35:17 | |
There are, however, one or two problems. | 0:35:20 | 0:35:23 | |
These strings are so small | 0:35:25 | 0:35:27 | |
that no-one has ever seen anything remotely stringy. | 0:35:27 | 0:35:33 | |
Depending on one's viewpoint, the size of these strings | 0:35:35 | 0:35:39 | |
can vary an awful lot, | 0:35:39 | 0:35:41 | |
from scales, which are sort of | 0:35:41 | 0:35:44 | |
a millionth of a millionth of the size of a nucleus, | 0:35:44 | 0:35:47 | |
to scales, which are much, much smaller than that. | 0:35:47 | 0:35:50 | |
If string theory turned out to be true, | 0:35:53 | 0:35:56 | |
then a string would be the smallest thing in the universe. | 0:35:56 | 0:35:59 | |
The trouble is, once we get this small, the whole notion of small | 0:35:59 | 0:36:03 | |
and big may get turned completely upside down. | 0:36:03 | 0:36:06 | |
Supposing these are quarks and electrons, photons, the particles | 0:36:08 | 0:36:12 | |
that constitute the standard model. Now we've got a problem because | 0:36:12 | 0:36:18 | |
if you believe that they're made of something smaller, that's fine. | 0:36:18 | 0:36:22 | |
You'll find something smaller inside. | 0:36:22 | 0:36:25 | |
But if you believe in a theory like string theory, | 0:36:25 | 0:36:28 | |
then the notion of smallness no longer means the same. | 0:36:28 | 0:36:31 | |
Ah, I haven't actually reached it. It's even smaller than that. | 0:36:31 | 0:36:35 | |
And there's an even smaller one than that. | 0:36:35 | 0:36:37 | |
I have a little speck here, so that must be the smallest thing. | 0:36:37 | 0:36:43 | |
But then of course when you're down to this scale, | 0:36:43 | 0:36:46 | |
you may have the whole universe in your hand, | 0:36:46 | 0:36:49 | |
because the, the universe itself started | 0:36:49 | 0:36:51 | |
from something this scale and expanded into everything we know. | 0:36:51 | 0:36:54 | |
So this thing, which you think is the smallest constituent, | 0:36:57 | 0:37:00 | |
may in fact be the thing that contains all of us. | 0:37:00 | 0:37:02 | |
So the notion, the difference between... | 0:37:02 | 0:37:05 | |
Oops, I hadn't even got there. | 0:37:05 | 0:37:06 | |
I dropped it, I dropped the little universe. | 0:37:06 | 0:37:09 | |
The notion that this is the smallest constituent is paradoxically | 0:37:09 | 0:37:14 | |
not at odds with the statement that it may also be the whole universe. | 0:37:14 | 0:37:18 | |
String theory is underpinned by some fiendishly complex maths. | 0:37:25 | 0:37:30 | |
But to make it work out, | 0:37:30 | 0:37:31 | |
the theory invokes not just one new dimension, | 0:37:31 | 0:37:35 | |
but says that we live in 11 dimensional hyperspace. | 0:37:35 | 0:37:39 | |
If you could describe exactly how these extra dimensions | 0:37:42 | 0:37:44 | |
are curled up, you'd be able to describe the exact nature | 0:37:44 | 0:37:49 | |
of everything in the universe. | 0:37:49 | 0:37:51 | |
The trouble is, there's more than one way to curl them up. | 0:37:57 | 0:38:02 | |
So the equations of string theory | 0:38:08 | 0:38:09 | |
have very large numbers of solutions, a humungously large number, | 0:38:09 | 0:38:13 | |
any one of which might describe a possible universe | 0:38:13 | 0:38:16 | |
with its own laws of physics, | 0:38:16 | 0:38:18 | |
its own kinds of particles and its own kinds of forces. | 0:38:18 | 0:38:21 | |
This whole body of solutions of string theory has been called | 0:38:21 | 0:38:25 | |
the landscape string theory. | 0:38:25 | 0:38:27 | |
Each peak in the landscape represents a different solution - | 0:38:32 | 0:38:36 | |
a different possible universe. | 0:38:36 | 0:38:37 | |
With each one just as likely to exist as the next. | 0:38:41 | 0:38:44 | |
Most of these solutions would describe universes | 0:38:45 | 0:38:48 | |
which are completely absurd. | 0:38:48 | 0:38:50 | |
The typical ones would be the ones, which came into being and either | 0:38:50 | 0:38:56 | |
ceased to exist after a very, very short time or exploded in such a way | 0:38:56 | 0:39:01 | |
that matter exploded apart and never formed galaxies in the first place. | 0:39:01 | 0:39:06 | |
The fact that our universe has existed for long enough | 0:39:06 | 0:39:10 | |
for galaxies to form and evolve and planets to form and for life to form | 0:39:10 | 0:39:16 | |
and us to exist tells us that we are living in a very untypical universe. | 0:39:16 | 0:39:22 | |
If they could find the right solution - the right one | 0:39:26 | 0:39:30 | |
out of 1 followed by 500 zeros, | 0:39:30 | 0:39:33 | |
we'd have a neat explanation for everything in our universe. | 0:39:33 | 0:39:37 | |
So the fascinating thing is the multiverse idea | 0:39:39 | 0:39:42 | |
has been around for some time in astrophysics, | 0:39:42 | 0:39:44 | |
but they didn't have a theoretical way of understanding it. | 0:39:44 | 0:39:47 | |
And then along came string theory and then the two got wedded. | 0:39:47 | 0:39:51 | |
Whichever way you look - whether up to the largest scale | 0:39:58 | 0:40:02 | |
or down to the very smallest, our universe may not be alone. | 0:40:02 | 0:40:06 | |
But for now, string theory remains a theory, | 0:40:08 | 0:40:12 | |
with no experimental evidence | 0:40:12 | 0:40:14 | |
for any of its mind-boggling predictions. | 0:40:14 | 0:40:17 | |
As we look down in scale, things get increasingly cloudy. | 0:40:19 | 0:40:23 | |
To stand a chance of seeing strings, we'd need a particle accelerator | 0:40:25 | 0:40:29 | |
a million, billion times bigger than the LHC. | 0:40:29 | 0:40:33 | |
Is this, then, the end of the line for the explorers | 0:40:35 | 0:40:38 | |
searching for the smallest thing in the universe? | 0:40:38 | 0:40:41 | |
It turns out there could well be a bottom of the rabbit hole - | 0:40:49 | 0:40:55 | |
an ultimate limit of how small we can go. | 0:40:55 | 0:40:57 | |
And there may be a way to reach this ultimate destination - | 0:40:59 | 0:41:03 | |
it's just a rather roundabout route to get there. | 0:41:03 | 0:41:06 | |
Dr Giovanni Amelino-Camelia is a theoretical physicist, | 0:41:17 | 0:41:22 | |
who 12 years ago came up with an idea that could lead us | 0:41:22 | 0:41:26 | |
to the ultimate destination at the bottom of the rabbit hole. | 0:41:26 | 0:41:30 | |
An idea that may lead us to question the very fabric of the universe - | 0:41:34 | 0:41:38 | |
the three dimensions of space and one of time, known as space-time. | 0:41:38 | 0:41:42 | |
Space time to an ordinary person is space time. | 0:41:45 | 0:41:50 | |
What is space time? There is no answer. | 0:41:50 | 0:41:52 | |
To us, space time is, er... Do you understand what I'm trying to say? | 0:41:52 | 0:41:59 | |
The challenge is that I don't have anything to work with | 0:41:59 | 0:42:02 | |
because the person who listen to me thinks know space time very well, | 0:42:02 | 0:42:06 | |
but then if I asked what is space time, he would have no answer. | 0:42:06 | 0:42:10 | |
Space time, they think they know very well what it is. | 0:42:12 | 0:42:14 | |
"For God's sake, space time! You know!" | 0:42:14 | 0:42:17 | |
But "you know" is all they can say. | 0:42:17 | 0:42:20 | |
So your audience is the worst, | 0:42:20 | 0:42:23 | |
because they think they know a lot about this subject. | 0:42:23 | 0:42:27 | |
But then they know nothing, completely nothing. | 0:42:27 | 0:42:30 | |
You see what I'm trying to say? It's very tricky. | 0:42:32 | 0:42:36 | |
If we have any notion of space-time, it is that it is smooth. | 0:42:37 | 0:42:42 | |
We can move smoothly from one cafe to another, | 0:42:43 | 0:42:46 | |
can be reasonably sure how long a journey will take. | 0:42:46 | 0:42:49 | |
But maybe not if you get small enough. | 0:42:54 | 0:42:58 | |
The ultimate small destination is known as the Planck length. | 0:43:01 | 0:43:05 | |
It is the theoretical limit of how small anything can possibly be. | 0:43:07 | 0:43:11 | |
Some speculate that this could be the ultimate level. | 0:43:11 | 0:43:15 | |
I mean, this could be where the laws of nature are fundamentally written. | 0:43:15 | 0:43:20 | |
But to get to the Planck length, you have to look a hundred, | 0:43:25 | 0:43:30 | |
million, billion times smaller than a quark. | 0:43:30 | 0:43:33 | |
At this tiniest of scales, | 0:43:38 | 0:43:39 | |
we may find answers not just about the smallest lump of stuff, | 0:43:39 | 0:43:44 | |
but about the very nature of space | 0:43:44 | 0:43:48 | |
and time in which all the stuff sits. | 0:43:48 | 0:43:51 | |
What could be conceptually more fascinating than | 0:43:59 | 0:44:02 | |
learning about the structure of space time? | 0:44:02 | 0:44:04 | |
But our current theories with all their limitations suggest | 0:44:06 | 0:44:10 | |
that at this Planck scale that we're talking about, | 0:44:10 | 0:44:13 | |
we should expect space time to, to be not smooth as we imagine | 0:44:13 | 0:44:21 | |
but more like, well, more like the foam of a cappuccino | 0:44:21 | 0:44:26 | |
and actually perhaps in, in a violently dynamical way. | 0:44:26 | 0:44:33 | |
The Planck length is where the rules of the large | 0:44:37 | 0:44:41 | |
and the rules of the small collide in a heady brew | 0:44:41 | 0:44:44 | |
called quantum gravity. | 0:44:44 | 0:44:47 | |
It's a seething tempest of space and time known as space-time foam, where | 0:44:49 | 0:44:56 | |
the very fabric of space and time twist and turn in every direction. | 0:44:56 | 0:45:02 | |
It is where the two great pillars of modern physics, | 0:45:05 | 0:45:07 | |
general relativity and quantum mechanics, | 0:45:07 | 0:45:11 | |
may finally be reconciled. | 0:45:11 | 0:45:13 | |
If we could understand what is happening down here, | 0:45:15 | 0:45:18 | |
we could end up with a theory of everything. | 0:45:18 | 0:45:21 | |
We are really far, far away from, from this realm, | 0:45:24 | 0:45:28 | |
and yet some of the most conceptually striking questions | 0:45:28 | 0:45:35 | |
about what, how is the universe made, | 0:45:35 | 0:45:39 | |
what are its basic rules, appear to reside in this distant scale. | 0:45:39 | 0:45:45 | |
So it's... At one side, we have this feeling of not having | 0:45:46 | 0:45:50 | |
any access to it, and yet it appears to be the place where | 0:45:50 | 0:45:56 | |
most of the answers we are seeking are somehow hidden. | 0:45:56 | 0:46:01 | |
All roads in physics lead to the Planck length. | 0:46:06 | 0:46:09 | |
But until recently, | 0:46:09 | 0:46:11 | |
no-one had a clue how we would ever know anything about it. | 0:46:11 | 0:46:16 | |
It was a problem Giovanni was determined to solve, | 0:46:16 | 0:46:20 | |
seeking inspiration and reassurance in the cafes of Rome. | 0:46:20 | 0:46:23 | |
I never understood what triggers an idea. | 0:46:25 | 0:46:29 | |
And it's kind of reassuring to be reminded that all this is | 0:46:29 | 0:46:34 | |
all about small - important, conceptually important, | 0:46:34 | 0:46:36 | |
but small - I'm still here, the Coliseum is still there. | 0:46:36 | 0:46:39 | |
When you're stuck chasing a certain answer, | 0:46:39 | 0:46:44 | |
you often discover that all it took to find the answer | 0:46:44 | 0:46:49 | |
was to look at the same problem from a different angle. | 0:46:49 | 0:46:53 | |
MOBILE PHONE RINGS | 0:46:53 | 0:46:54 | |
From the office. | 0:46:54 | 0:46:56 | |
Pronto. | 0:46:57 | 0:46:59 | |
12 years ago, Giovanni had a flash of inspiration | 0:46:59 | 0:47:03 | |
that we could reach the unreachable. | 0:47:03 | 0:47:05 | |
Over the last decade or so, what we started to figure out is | 0:47:08 | 0:47:12 | |
that it is possible to get indirect information on the Planck scale. | 0:47:12 | 0:47:17 | |
We cannot build a microscope that show us, shows us | 0:47:18 | 0:47:22 | |
the structure of space time at the Planck scale, | 0:47:22 | 0:47:26 | |
but we can get indirect evidence about the Planck scale | 0:47:26 | 0:47:30 | |
structure of space time is made. | 0:47:30 | 0:47:33 | |
Any explorer will tell you that if the way ahead is blocked, | 0:47:33 | 0:47:37 | |
you have to set off in a new direction. | 0:47:37 | 0:47:40 | |
Instead of trying to look directly down at the smallest scale, | 0:47:43 | 0:47:47 | |
the idea is to look up at the very biggest scale possible - | 0:47:47 | 0:47:53 | |
the entire universe. | 0:47:53 | 0:47:56 | |
It's an idea that is now reality... | 0:48:07 | 0:48:10 | |
..and a trick that is now being performed by the MAGIC telescope. | 0:48:12 | 0:48:16 | |
The idea is to use the vastness of the universe | 0:48:24 | 0:48:27 | |
as a giant magnifying glass. | 0:48:27 | 0:48:30 | |
Dr Robert Wagner is using this unique instrument to peer | 0:48:44 | 0:48:48 | |
at some of the most distant and cataclysmic events in the universe. | 0:48:48 | 0:48:51 | |
Under good conditions, as we have them right now, | 0:48:54 | 0:48:57 | |
we record 200 gamma ray or cosmic ray showers per second. | 0:48:57 | 0:49:00 | |
The Earth is constantly being bombard by high-energy cosmic rays, | 0:49:03 | 0:49:08 | |
gamma rays, the most energetic form of light. | 0:49:08 | 0:49:11 | |
But Robert is looking for the most extreme of these - | 0:49:14 | 0:49:17 | |
gamma ray bursts from colliding neutron stars or exploding | 0:49:17 | 0:49:21 | |
black holes in distant galaxies. | 0:49:21 | 0:49:24 | |
Gamma ray bursts are very violent events in the universe | 0:49:26 | 0:49:30 | |
and one key characteristic of them is that we cannot predict them. | 0:49:30 | 0:49:35 | |
So they can take place at any time at any place on the sky. | 0:49:35 | 0:49:38 | |
We get the information from satellite experiments. | 0:49:38 | 0:49:41 | |
This information is transmitted in an automatic way down here, | 0:49:41 | 0:49:44 | |
it takes about ten seconds, and then the telescopes will fully | 0:49:44 | 0:49:48 | |
automatically go to those gamma ray burst locations. | 0:49:48 | 0:49:51 | |
With these light weight telescopes | 0:49:55 | 0:49:57 | |
we're able to move to any point in the sky within only 20 seconds. | 0:49:57 | 0:50:02 | |
Those bursts last anything between one and 1,000 seconds. | 0:50:08 | 0:50:12 | |
Most of the bursts are really short lived. | 0:50:12 | 0:50:14 | |
So it's of great essence to be there as fast as possible. | 0:50:14 | 0:50:19 | |
Catching these violent but fleeting events | 0:50:22 | 0:50:25 | |
takes many nights of patient observing. | 0:50:25 | 0:50:27 | |
Well, this is a place I go right after the observations, | 0:50:34 | 0:50:38 | |
and this of course gives a quite different feeling | 0:50:38 | 0:50:42 | |
from looking at screens. | 0:50:42 | 0:50:44 | |
You look at the real sky and actually the stuff | 0:50:44 | 0:50:47 | |
we are observing and hoping to detect is somewhere up there. | 0:50:47 | 0:50:50 | |
Those black holes and galaxies, they are so far very away, | 0:50:54 | 0:50:59 | |
but at the same time, when you come here, | 0:50:59 | 0:51:03 | |
you realise they are real because, you know, all the photons | 0:51:03 | 0:51:07 | |
which hit my eye right now from those stars, they are real. | 0:51:07 | 0:51:10 | |
Although Robert spends his nights looking out | 0:51:15 | 0:51:18 | |
into the far reaches of the cosmos, he is actually trying to find out | 0:51:18 | 0:51:23 | |
how the universe works on the very smallest scale. | 0:51:23 | 0:51:27 | |
Things up there are so very, very far away. | 0:51:30 | 0:51:33 | |
The farthest galaxy we are looking at is shining light at the time | 0:51:34 | 0:51:38 | |
when the universe was just half its age, | 0:51:38 | 0:51:41 | |
it takes the light 7 billion years to get to here. | 0:51:41 | 0:51:44 | |
So that's a distance which, personally, | 0:51:44 | 0:51:47 | |
I cannot imagine, myself, right? It's a very abstract number. | 0:51:47 | 0:51:52 | |
At the same time, the scales we are looking at if we want to get to | 0:51:52 | 0:51:55 | |
the shortest scales are as similar small as this distance is large. | 0:51:55 | 0:52:01 | |
So it's really hard to imagine these things on scales, | 0:52:01 | 0:52:05 | |
which we see here on Earth. | 0:52:05 | 0:52:07 | |
But Robert's not really interested in the explosions themselves. | 0:52:10 | 0:52:15 | |
They act as the biggest particle accelerator in the universe, | 0:52:15 | 0:52:20 | |
way more powerful than anything we could ever achieve here on Earth. | 0:52:20 | 0:52:23 | |
He is interested in what happens to the particles, | 0:52:26 | 0:52:29 | |
in this case, photons, while they travel towards us | 0:52:29 | 0:52:32 | |
on their 7-billion year journey | 0:52:32 | 0:52:34 | |
through what seems like smooth, empty space. | 0:52:34 | 0:52:39 | |
But any distortions in the structure of space-time at the Planck scale | 0:52:41 | 0:52:45 | |
would affect photons of different energies in different ways. | 0:52:45 | 0:52:50 | |
Essentially, it's quite comparable to cars driving on a road. | 0:53:02 | 0:53:06 | |
A big car will not feel the fine structure of the road, | 0:53:07 | 0:53:11 | |
it will just roll along and will be, you know, just as fast as normal. | 0:53:11 | 0:53:16 | |
Whereas a small car, like a model car, | 0:53:16 | 0:53:18 | |
will feel every tiny ripple in the structure of the street. | 0:53:18 | 0:53:23 | |
The large car would be the low-energy photon, | 0:53:35 | 0:53:37 | |
because there is nearly no interaction with the structure | 0:53:37 | 0:53:40 | |
or the ripples in the road. | 0:53:40 | 0:53:42 | |
Whereas the small car would be the high-energy photon, | 0:53:42 | 0:53:45 | |
because it's smaller, there are more interactions with the road, | 0:53:45 | 0:53:49 | |
and this makes the photon travel slower. | 0:53:49 | 0:53:51 | |
The difference in speed is tiny. | 0:53:56 | 0:53:58 | |
But the length of the journey, half way across the universe, | 0:53:58 | 0:54:02 | |
could magnify the effect into something we might be able to see. | 0:54:02 | 0:54:07 | |
We just let those photons travel along the universe, | 0:54:13 | 0:54:16 | |
and of course they travel for billions of light years, | 0:54:16 | 0:54:19 | |
and only that long travel time makes this tiny effect visible to us, | 0:54:19 | 0:54:24 | |
which is to say, after such long travel, | 0:54:24 | 0:54:27 | |
we expect a few seconds' delay of photons of different energies, | 0:54:27 | 0:54:31 | |
and of course this is a delay which can easily be measured | 0:54:31 | 0:54:35 | |
with the MAGIC telescopes. | 0:54:35 | 0:54:36 | |
In 2005, just a few months after switching on the telescopes, | 0:54:44 | 0:54:49 | |
a gamma ray outburst from an active galactic nucleus tickled | 0:54:49 | 0:54:54 | |
the MAGIC mirrors, giving Robert his first tantalising glimpse | 0:54:54 | 0:54:58 | |
down to the smallest place in the universe. | 0:54:58 | 0:55:01 | |
It was the first time ever we observed such an effect, | 0:55:01 | 0:55:06 | |
or, to put it in cautious words, the hint of such an effect. | 0:55:06 | 0:55:09 | |
So clearly we were absolutely stunned. | 0:55:09 | 0:55:11 | |
Soon, we realised there is something in this data, which is extraordinary. | 0:55:16 | 0:55:20 | |
As soon as we dig deeper and deeper in the data, | 0:55:23 | 0:55:25 | |
it became apparent that photons of different energies may have | 0:55:25 | 0:55:31 | |
different arrival times at the instrument. | 0:55:31 | 0:55:33 | |
Those photons had to travel billions of light years. | 0:55:39 | 0:55:43 | |
The effect was on the order of seconds, maybe five seconds. | 0:55:43 | 0:55:47 | |
The Planck length is so small | 0:55:50 | 0:55:52 | |
that after a race of seven billion years, | 0:55:52 | 0:55:55 | |
the photons finished with a gap of just five seconds. | 0:55:55 | 0:56:00 | |
There are two possibilities here. | 0:56:00 | 0:56:03 | |
The first is that the photons rather inexplicably set off | 0:56:03 | 0:56:07 | |
five seconds apart. | 0:56:07 | 0:56:09 | |
The other explanation is more revolutionary. | 0:56:09 | 0:56:13 | |
This five-second delay could be our first glimpse of the smallest thing | 0:56:13 | 0:56:17 | |
in the universe, the first evidence of a lumpiness in space-time. | 0:56:17 | 0:56:23 | |
If true, it would shatter one of the most basic rules of physics. | 0:56:24 | 0:56:29 | |
To put it in simple terms, the speed of light is not constant. | 0:56:31 | 0:56:35 | |
It is dependent on the energy of the photon. | 0:56:35 | 0:56:38 | |
And that's revolutionary | 0:56:43 | 0:56:45 | |
because it's one of the fundamental laws of physics. | 0:56:45 | 0:56:48 | |
Einstein predicted speed of light is a constant, | 0:56:48 | 0:56:50 | |
no matter what you do, no matter where you are. | 0:56:50 | 0:56:53 | |
Under no circumstances should there be | 0:56:53 | 0:56:55 | |
a difference in the speed of light. | 0:56:55 | 0:56:57 | |
The conclusion from our measurements that this is not the case | 0:57:00 | 0:57:04 | |
would mean quite a revolution of physics. | 0:57:04 | 0:57:07 | |
The MAGIC observations provide a tantalising glimpse | 0:57:16 | 0:57:19 | |
of what awaits us at the smallest structures of space. | 0:57:19 | 0:57:22 | |
But to get there, | 0:57:26 | 0:57:28 | |
we've had to harness the entire expanse of the universe. | 0:57:28 | 0:57:32 | |
The journey to the very small is one of the most epic in science. | 0:57:38 | 0:57:42 | |
It takes us beyond the limits of what we can see... | 0:57:44 | 0:57:47 | |
..inside fundamental particles, | 0:57:50 | 0:57:52 | |
which may not be so fundamental after all... | 0:57:52 | 0:57:55 | |
..through a wonderland of extra dimensions and multiple universes... | 0:57:56 | 0:58:01 | |
..down to the smallest place in the universe, | 0:58:03 | 0:58:06 | |
a place that could change the face of physics. | 0:58:06 | 0:58:09 | |
And surely we expect a revolution in the laws of physics not | 0:58:13 | 0:58:18 | |
smaller than the one that took us from Newton's laws | 0:58:18 | 0:58:22 | |
to quantum mechanics a century ago. | 0:58:22 | 0:58:25 | |
Subtitles by Red Bee Media Ltd | 0:58:42 | 0:58:46 |