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These are the Appennine mountains in Central Italy. | 0:00:02 | 0:00:06 | |
Buried underneath them | 0:00:08 | 0:00:10 | |
is one of the most sophisticated science labs in the world. | 0:00:10 | 0:00:13 | |
Last month, an international group of scientists | 0:00:16 | 0:00:19 | |
working here on a particle physics experiment | 0:00:19 | 0:00:21 | |
called OPERA made an astonishing claim. | 0:00:21 | 0:00:24 | |
They said they had detected particles that seemed to travel | 0:00:27 | 0:00:30 | |
faster than the speed of light. | 0:00:30 | 0:00:33 | |
It was a claim that contradicted | 0:00:33 | 0:00:36 | |
more than 100 years of scientific orthodoxy. | 0:00:36 | 0:00:39 | |
It has created a furore. | 0:00:39 | 0:00:41 | |
If it's true the implications are amazing. | 0:00:41 | 0:00:43 | |
They're mind-blowing. They really will turn things on their heads. | 0:00:43 | 0:00:47 | |
This is earth-shaking if true. | 0:00:47 | 0:00:48 | |
You would be able to travel back in time. | 0:00:48 | 0:00:51 | |
We have to tear up all the textbooks and start again. | 0:00:51 | 0:00:55 | |
My name's Marcus du Sautoy. | 0:00:56 | 0:00:57 | |
I'm a mathematician and as a mathematician, | 0:00:57 | 0:01:01 | |
I'm used to dealing with ideas that seem impossible in the real world. | 0:01:01 | 0:01:05 | |
For me, it's moments like this | 0:01:05 | 0:01:08 | |
when data clashes with theory that are always rather thrilling. | 0:01:08 | 0:01:12 | |
You can almost feel the shudder that passes through the entire | 0:01:12 | 0:01:15 | |
scientific community when a result as strange as this comes out. | 0:01:15 | 0:01:19 | |
Everybody's talking about it. | 0:01:19 | 0:01:21 | |
Is this the moment for a grand new theory to emerge that makes | 0:01:23 | 0:01:26 | |
sense of all the mysteries that still pervade physics? | 0:01:26 | 0:01:31 | |
Or has there just been a mistake in the measurements? | 0:01:31 | 0:01:35 | |
I'm going to explore one of the most dramatic | 0:01:35 | 0:01:37 | |
scientific announcements for a generation. | 0:01:37 | 0:01:40 | |
What does it mean and why does it matter? | 0:01:40 | 0:01:43 | |
Our story starts with light. | 0:01:52 | 0:01:54 | |
For centuries, light has fascinated us. | 0:01:55 | 0:01:59 | |
Our ancestors built monuments to capture light | 0:02:01 | 0:02:03 | |
from the sun at particular times of the year. | 0:02:03 | 0:02:07 | |
Light gives us colour. It's how we see the world. | 0:02:08 | 0:02:12 | |
Light floods the cosmos. | 0:02:15 | 0:02:17 | |
But it has always been mysterious. | 0:02:19 | 0:02:23 | |
One of the biggest mysteries about light is how fast does it travel? | 0:02:23 | 0:02:28 | |
Unravelling this question, would lead to one of the greatest | 0:02:28 | 0:02:31 | |
and most surprising leaps in the history of science. | 0:02:31 | 0:02:34 | |
Until 350 years ago, | 0:02:37 | 0:02:39 | |
many scientists argued that light didn't really travel at all. | 0:02:39 | 0:02:43 | |
It was transmitted instantaneously from source to eye. | 0:02:43 | 0:02:46 | |
But then an astronomer, making careful observations | 0:02:48 | 0:02:51 | |
of the moons of Jupiter showed it took a finite period | 0:02:51 | 0:02:55 | |
of time for light waves to reach Earth. | 0:02:55 | 0:02:59 | |
That meant light travel couldn't be instantaneous. | 0:02:59 | 0:03:02 | |
It had to have a finite speed. | 0:03:02 | 0:03:05 | |
Another puzzle remained. | 0:03:05 | 0:03:07 | |
If light was a wave, then scientists concluded it must be travelling | 0:03:07 | 0:03:11 | |
through some medium, in the same way as sound travels through air. | 0:03:11 | 0:03:16 | |
This medium was given a name - the ether. | 0:03:16 | 0:03:19 | |
It was thought that the ether was able to flow like the wind. | 0:03:24 | 0:03:29 | |
Therefore, light waves that were travelling in the same direction | 0:03:29 | 0:03:33 | |
as the ether should travel faster than those fighting against it. | 0:03:33 | 0:03:37 | |
In the 1880s, scientists tried to measure variations | 0:03:39 | 0:03:42 | |
in the speed of light travelling in different directions. | 0:03:42 | 0:03:46 | |
But to their surprise, they found no difference. | 0:03:46 | 0:03:49 | |
However you measured it, light always went at the same speed. | 0:03:49 | 0:03:54 | |
As the 20th century dawned, | 0:03:56 | 0:03:58 | |
scientists were still wrestling with the strange behaviour of light | 0:03:58 | 0:04:01 | |
and in particular, what speed it travelled at. | 0:04:01 | 0:04:06 | |
The stage was set for the arrival of a genius who would unravel | 0:04:06 | 0:04:09 | |
the mysteries of light | 0:04:09 | 0:04:11 | |
and in the process, transform our understanding of the universe. | 0:04:11 | 0:04:16 | |
In 1902, a young physicist arrived in the Swiss town of Berne. | 0:04:24 | 0:04:29 | |
He trained as a physics and maths teacher in Zurich, | 0:04:29 | 0:04:33 | |
but had been unable to find a teaching job. | 0:04:33 | 0:04:36 | |
Eventually, he found work in the Swiss patent office. | 0:04:36 | 0:04:40 | |
It was far from a lofty, academic institution, | 0:04:40 | 0:04:43 | |
but it turned out to be just the environment he needed. | 0:04:43 | 0:04:47 | |
His name was Albert Einstein. | 0:04:47 | 0:04:49 | |
An amateur scientist, someone who didn't have an academic position. | 0:04:56 | 0:05:01 | |
This patent clerk who worked on physics | 0:05:01 | 0:05:04 | |
when he wasn't doing his day job | 0:05:04 | 0:05:07 | |
was quite an unusual person to be the one | 0:05:07 | 0:05:10 | |
who revolutionised our ideas of space and time. | 0:05:10 | 0:05:13 | |
I don't know what the workload was in the patent office. | 0:05:13 | 0:05:16 | |
Maybe there weren't so much patents coming in | 0:05:16 | 0:05:19 | |
in Switzerland in those days and he had a lot of time to think. | 0:05:19 | 0:05:22 | |
Anyway, somehow or other, he was able to think | 0:05:22 | 0:05:25 | |
very long, very hard and very deep. | 0:05:25 | 0:05:27 | |
The clerk's work gave Einstein time | 0:05:27 | 0:05:30 | |
to ponder thought experiments, deceptively simple scenarios | 0:05:30 | 0:05:34 | |
that enabled him to explore the most complex of concepts. | 0:05:34 | 0:05:38 | |
Einstein was very much an individual, lone scientist | 0:05:39 | 0:05:44 | |
thinking his deep thoughts and, perhaps precisely because | 0:05:44 | 0:05:48 | |
he was working by himself, he got insights other people hadn't seen. | 0:05:48 | 0:05:52 | |
Einstein was fascinated by the mysterious behaviour of light. | 0:05:54 | 0:05:58 | |
It was a wave, yet it also had the properties of a particle, | 0:05:58 | 0:06:02 | |
what came to be known as a photon. | 0:06:02 | 0:06:04 | |
How fast did it travel, he wondered? And did it have a speed limit? | 0:06:06 | 0:06:10 | |
From the age of 16, Einstein had been pondering a thought experiment. | 0:06:10 | 0:06:14 | |
If I look into this shaving mirror and I accelerate faster and faster | 0:06:14 | 0:06:19 | |
towards the speed of light, then does my image suddenly disappear? | 0:06:19 | 0:06:25 | |
If you think about it, the photons from my face have got to travel | 0:06:25 | 0:06:28 | |
the distance from my face to the mirror and if I am going | 0:06:28 | 0:06:31 | |
at the speed of light, then those photons have to go travelling faster | 0:06:31 | 0:06:35 | |
than me. Namely, the light is travelling faster | 0:06:35 | 0:06:39 | |
than the speed of light. | 0:06:39 | 0:06:41 | |
Now, Einstein believed his image wouldn't disappear, | 0:06:41 | 0:06:44 | |
so he started to think about how to resolve this paradox. | 0:06:44 | 0:06:48 | |
In the spring of 1905, Einstein was ready | 0:06:51 | 0:06:54 | |
to launch his ideas on the world. | 0:06:54 | 0:06:57 | |
In that one year, Einstein published four papers, any one of which | 0:06:57 | 0:07:02 | |
would have been enough to create a sensation in their own right. | 0:07:02 | 0:07:05 | |
It was, arguably, one of the most sustained and extraordinary bursts | 0:07:05 | 0:07:09 | |
of scientific creativity the world has ever seen. | 0:07:09 | 0:07:12 | |
One of those papers transformed our understanding of light. | 0:07:13 | 0:07:17 | |
And here it is, all 31 pages of it. | 0:07:22 | 0:07:25 | |
It's an astonishing paper in many different ways, not least | 0:07:25 | 0:07:28 | |
because if I look at one of the papers I have published, | 0:07:28 | 0:07:31 | |
then, at the end, I reference 39 other papers that I rely on. | 0:07:31 | 0:07:36 | |
In Einstein's paper there are no references at all. | 0:07:36 | 0:07:40 | |
It contains a set of scientific laws that define not just our world, | 0:07:42 | 0:07:47 | |
but also our entire universe. | 0:07:47 | 0:07:50 | |
At the centre of these is the statement that the speed of light, | 0:07:50 | 0:07:54 | |
when it travels through a vacuum, is absolute. | 0:07:54 | 0:07:58 | |
Nothing can travel faster. | 0:07:58 | 0:08:00 | |
It was an incredibly audacious piece of reasoning. | 0:08:02 | 0:08:05 | |
Einstein realised that the way we looked at the universe was wrong, | 0:08:05 | 0:08:09 | |
particularly our intuitive sense of how time and space worked. | 0:08:09 | 0:08:14 | |
We can see how, by doing a thought experiment of our own | 0:08:14 | 0:08:18 | |
with the help of the 12.12 to Ashford. | 0:08:18 | 0:08:22 | |
If I shine this torch while standing still on the platform, | 0:08:23 | 0:08:26 | |
then the beam of light from the torch | 0:08:26 | 0:08:29 | |
is going to be going at the speed of light. | 0:08:29 | 0:08:31 | |
That's straightforward. | 0:08:31 | 0:08:33 | |
But what happens to the same beam of light went I'm on a moving train? | 0:08:35 | 0:08:39 | |
Now, I've just asked the conductor how fast the train is going. | 0:08:42 | 0:08:46 | |
He says it's going at 140 miles an hour. | 0:08:46 | 0:08:49 | |
This is the same torch I had on the platform. | 0:08:49 | 0:08:53 | |
If I switch it on, the question is, | 0:08:53 | 0:08:55 | |
for somebody standing outside in the field, | 0:08:55 | 0:08:57 | |
how fast do they think the light is travelling? | 0:08:57 | 0:09:00 | |
Because logic would suggest that the light is travelling | 0:09:00 | 0:09:03 | |
at the speed of light from the torch, but then I need to add on | 0:09:03 | 0:09:06 | |
the 140 miles an hour that the train is going. | 0:09:06 | 0:09:09 | |
But Einstein said no. The speed of light is a constant. | 0:09:09 | 0:09:13 | |
It doesn't matter where you are in the universe, how you measure it, | 0:09:13 | 0:09:16 | |
on a train to Ashford or on a spaceship | 0:09:16 | 0:09:18 | |
travelling across the universe or standing still outside, | 0:09:18 | 0:09:22 | |
the speed of light is the same. | 0:09:22 | 0:09:24 | |
Einstein's brilliance was to realise | 0:09:25 | 0:09:28 | |
that if the speed of light was the same regardless | 0:09:28 | 0:09:30 | |
of where you measured it from, then something else had to give. | 0:09:30 | 0:09:35 | |
He concluded that it was time that was changing. | 0:09:36 | 0:09:40 | |
Time was not a constant. | 0:09:40 | 0:09:41 | |
Instead it changed depending on how quickly you were moving. | 0:09:41 | 0:09:46 | |
The faster you travel, the slower time passes. | 0:09:47 | 0:09:51 | |
Einstein's view of the universe was seen as radical at the time | 0:09:51 | 0:09:56 | |
and it's still hard to grasp. | 0:09:56 | 0:09:59 | |
But over the years, countless experiments have proved him right. | 0:09:59 | 0:10:04 | |
These theories have a practical impact in the real world, | 0:10:04 | 0:10:07 | |
an example being the GPS or Global Positioning System. | 0:10:07 | 0:10:12 | |
'US Naval Observatory Master Clock. | 0:10:14 | 0:10:17 | |
'At the tone, Mountain Daylight Time | 0:10:17 | 0:10:19 | |
'18 hours, 48 minutes, 5 seconds.' | 0:10:19 | 0:10:22 | |
BEEP | 0:10:22 | 0:10:23 | |
GPS uses a network of satellites orbiting | 0:10:25 | 0:10:28 | |
at speeds of 14,000 kilometres per hour | 0:10:28 | 0:10:32 | |
to accurately pinpoint locations all over the globe. | 0:10:32 | 0:10:35 | |
To ensure precision, it's vital that the time kept by the satellites | 0:10:35 | 0:10:41 | |
is the same as the time kept by the receivers on the ground. | 0:10:41 | 0:10:45 | |
But the satellites travel so fast that, compared to the receivers | 0:10:45 | 0:10:51 | |
on earth, time runs slower by seven microseconds a day. | 0:10:51 | 0:10:56 | |
If we didn't use Einstein's theories and take this into account, | 0:10:56 | 0:11:00 | |
the accuracy of our GPS systems would drift | 0:11:00 | 0:11:02 | |
by more than two kilometres a day. | 0:11:02 | 0:11:05 | |
Einstein didn't stop there. | 0:11:07 | 0:11:09 | |
He theorised that not only did light travel at a constant speed, | 0:11:09 | 0:11:13 | |
but that speed was also the speed limit of the universe. | 0:11:13 | 0:11:18 | |
Nothing can travel faster. | 0:11:18 | 0:11:20 | |
That's because of the relationship between mass and energy. | 0:11:22 | 0:11:26 | |
Einstein said that mass and energy were two sides of the same coin. | 0:11:26 | 0:11:31 | |
That means that if the amount of energy an object has increases, | 0:11:31 | 0:11:36 | |
then so does its mass. | 0:11:36 | 0:11:38 | |
Crucially, increasing an object's speed increases its energy. | 0:11:38 | 0:11:43 | |
The faster I travel on this train, the more mass I gain. | 0:11:47 | 0:11:51 | |
For example, if I was travelling at 90% of the speed of light, | 0:11:51 | 0:11:55 | |
then my mass would be twice that as if I was stationary. | 0:11:55 | 0:11:59 | |
The more I accelerate, the more my mass increases | 0:11:59 | 0:12:03 | |
and the more energy I'm going to need to make me accelerate. | 0:12:03 | 0:12:06 | |
Until, when I reach the speed of light, | 0:12:06 | 0:12:08 | |
the equations force my mass to be infinite. | 0:12:08 | 0:12:12 | |
I'm going to need an infinite amount of energy to get there. | 0:12:12 | 0:12:15 | |
But no-one can possess infinite energy however hard they tried. | 0:12:15 | 0:12:19 | |
That's why, according to Einstein, it's impossible | 0:12:19 | 0:12:22 | |
to cross the speed of light barrier. | 0:12:22 | 0:12:25 | |
From a thought experiment, | 0:12:25 | 0:12:28 | |
Einstein was able to radically alter our view of the world. | 0:12:28 | 0:12:31 | |
He concluded that the speed of light is constant | 0:12:33 | 0:12:36 | |
and that nothing with mass can travel faster than the speed. | 0:12:36 | 0:12:40 | |
These concepts are at the heart of our modern understanding | 0:12:41 | 0:12:45 | |
of the universe. | 0:12:45 | 0:12:47 | |
The results picked up by the OPERA team in Italy were so shocking | 0:12:47 | 0:12:51 | |
because they raise serious questions not just about Einstein's theory, | 0:12:51 | 0:12:55 | |
but all the evidence that's been gathered to support it. | 0:12:55 | 0:12:59 | |
That said, in some ways, we shouldn't be so shocked | 0:12:59 | 0:13:02 | |
by the results because the OPERA scientists were studying | 0:13:02 | 0:13:05 | |
one of the strangest and least understood particles there is - | 0:13:05 | 0:13:09 | |
the neutrino. | 0:13:09 | 0:13:11 | |
And if there was one particle that was going to break the rules, | 0:13:11 | 0:13:14 | |
it was this one. | 0:13:14 | 0:13:15 | |
The neutrino's been the bad boy of physics, | 0:13:16 | 0:13:20 | |
basically, putting physicists out of their comfort zone. | 0:13:20 | 0:13:23 | |
I think that's the best way to put it. | 0:13:23 | 0:13:25 | |
A lot of unusual things have been revealed by the neutrino, | 0:13:25 | 0:13:28 | |
so maybe we shouldn't be surprised by this novelty. | 0:13:28 | 0:13:31 | |
There are 16 types of fundamental particles that are the smallest | 0:13:33 | 0:13:37 | |
and simplest building blocks in the universe. | 0:13:37 | 0:13:40 | |
Together, they explain the world and what holds it together. | 0:13:40 | 0:13:44 | |
Three of those elementary particles are neutrinos. | 0:13:45 | 0:13:48 | |
Their assistance was first predicted in 1930 | 0:13:48 | 0:13:52 | |
by Austrian physicist Wolfgang Pauli. | 0:13:52 | 0:13:56 | |
But Pauli didn't think it would ever be possible to find one, | 0:13:56 | 0:14:00 | |
because their properties make them incredibly difficult to spot. | 0:14:00 | 0:14:04 | |
It's a very anti-social particle. It doesn't like to talk to the world. | 0:14:04 | 0:14:09 | |
Right now, you are being crossed by billions of neutrinos per second, | 0:14:09 | 0:14:12 | |
and you don't feel them because they go through you. | 0:14:12 | 0:14:15 | |
They go through the earth, through everything without interacting. | 0:14:15 | 0:14:19 | |
And still, the universe is pervaded by them. It's full of them. | 0:14:19 | 0:14:22 | |
There is a swarm of neutrinos going around, | 0:14:22 | 0:14:24 | |
many more neutrinos than particles of light and atoms | 0:14:24 | 0:14:27 | |
and anything you are used to. | 0:14:27 | 0:14:29 | |
It order to understand how neutrinos are able to travel straight | 0:14:31 | 0:14:35 | |
through matter without being noticed, | 0:14:35 | 0:14:37 | |
we need to think about what matter is made of. | 0:14:37 | 0:14:40 | |
Every physical thing in the world around us, | 0:14:40 | 0:14:42 | |
from mountains and buildings to you and me, is made of atoms. | 0:14:42 | 0:14:46 | |
And atoms are made up of a nucleus at the centre, | 0:14:46 | 0:14:51 | |
surrounded by orbiting electrons, | 0:14:51 | 0:14:54 | |
a bit like a solar system with a sun and orbiting planets. | 0:14:54 | 0:14:58 | |
The mind-boggling thing about matter is that, although it looks | 0:15:00 | 0:15:03 | |
and feels solid, it's actually mostly empty space. | 0:15:03 | 0:15:07 | |
There are vast swathes of nothingness between the tiny nucleus | 0:15:07 | 0:15:10 | |
and the orbiting electrons. | 0:15:10 | 0:15:13 | |
And the neutrino is so small without any charge, | 0:15:13 | 0:15:16 | |
that it can pass through this space very easily. | 0:15:16 | 0:15:19 | |
In fact, the neutrino's so tiny that if the atom | 0:15:19 | 0:15:23 | |
is the size of the solar system, the neutrino is the size of a golf ball. | 0:15:23 | 0:15:28 | |
These tiny particles existed in theory for a quarter of a century | 0:15:30 | 0:15:35 | |
without anyone being able to see them. | 0:15:35 | 0:15:38 | |
But then something happened to change that. | 0:15:38 | 0:15:41 | |
The nuclear bomb. | 0:15:44 | 0:15:46 | |
The power of a nuclear bomb comes from a chain reaction | 0:15:48 | 0:15:52 | |
of spitting atomic nuclei. | 0:15:52 | 0:15:55 | |
In the 1950s, a young researcher called Fred Reines | 0:15:55 | 0:15:58 | |
realised that this chain reaction would produce | 0:15:58 | 0:16:02 | |
an intense burst of neutrinos, | 0:16:02 | 0:16:04 | |
and so be the perfect place to hunt for the elusive particle. | 0:16:04 | 0:16:08 | |
But detecting neutrinos from a nuclear explosion wasn't practical. | 0:16:10 | 0:16:14 | |
So Reines turned his attention to the much more controlled | 0:16:14 | 0:16:17 | |
chain reaction in a nuclear reactor. | 0:16:17 | 0:16:19 | |
Although most neutrinos produced by the reactor passed through | 0:16:21 | 0:16:24 | |
the gaps inside atoms, so many neutrinos were produced | 0:16:24 | 0:16:29 | |
that every now and then, one would collide with an atom's nucleus. | 0:16:29 | 0:16:33 | |
When it did, a charged particle would be ejected. | 0:16:33 | 0:16:37 | |
He set up his experiment, which he called Project Poltergeist, | 0:16:37 | 0:16:41 | |
and waited for the characteristic signal of this interaction - | 0:16:41 | 0:16:45 | |
a distinctive double pulse of energy. | 0:16:45 | 0:16:47 | |
In June 1956, Reines announced that he had detected the neutrino. | 0:16:49 | 0:16:55 | |
Since that discovery, we've become a bit more adept at creating | 0:16:59 | 0:17:03 | |
and observing this most elusive of particles. | 0:17:03 | 0:17:07 | |
We've created neutrinos in man-made particle accelerators | 0:17:07 | 0:17:11 | |
like the ones in CERN in Geneva, | 0:17:11 | 0:17:13 | |
as well as detecting them naturally in cosmic rays and from the sun. | 0:17:13 | 0:17:17 | |
We now know they are essential to our existence. | 0:17:17 | 0:17:22 | |
All of the elements are made by nuclear reactions | 0:17:22 | 0:17:25 | |
that would be impossible without neutrinos. | 0:17:25 | 0:17:28 | |
We also know that despite their tiny size, | 0:17:30 | 0:17:33 | |
they do still have a small mass, which means, according to Einstein, | 0:17:33 | 0:17:38 | |
they can't travel faster than the speed of light. | 0:17:38 | 0:17:42 | |
But that theory has now been challenged by a small group | 0:17:48 | 0:17:52 | |
of scientists working in one of the most unusual science labs | 0:17:52 | 0:17:55 | |
in the world. | 0:17:55 | 0:17:57 | |
Assergi is a sleepy town nestled beneath Gran Sasso, | 0:17:57 | 0:18:01 | |
a 3,000 metre peak in the Apennines of Central Italy. | 0:18:01 | 0:18:05 | |
In the early 1980s, a new road was planned here | 0:18:05 | 0:18:08 | |
that would cut right through the mountain. | 0:18:08 | 0:18:11 | |
Italian scientists had a brilliant idea. | 0:18:11 | 0:18:14 | |
They realised that the road would give them | 0:18:14 | 0:18:18 | |
a unique opportunity to create a physics lab like no other. | 0:18:18 | 0:18:22 | |
It would give them easy access to the heart of the mountain, | 0:18:22 | 0:18:26 | |
the perfect place to build a neutrino detector. | 0:18:26 | 0:18:30 | |
Here we have 15 different experiments, | 0:18:30 | 0:18:32 | |
and there are roughly, 100 physicists per day working here. | 0:18:32 | 0:18:38 | |
Neutrinos so rarely interact with matter that it is easy | 0:18:42 | 0:18:46 | |
for an experiment to be swamped by false readings, | 0:18:46 | 0:18:49 | |
readings triggered by naturally occurring radiation | 0:18:49 | 0:18:53 | |
and charged particles such as cosmic rays hitting the experiment. | 0:18:53 | 0:18:56 | |
The only way to study neutrinos is to find some way to weed out | 0:18:59 | 0:19:04 | |
as many of these interfering particles as possible. | 0:19:04 | 0:19:08 | |
Now we are in the middle of the gallery. | 0:19:12 | 0:19:15 | |
And near here, we have the experiments. | 0:19:15 | 0:19:17 | |
On top of us, we have 1,400 metres of rock, | 0:19:17 | 0:19:22 | |
the top of Gran Sasso mountain. | 0:19:22 | 0:19:25 | |
Here, the cosmic rays are very few, because outside, | 0:19:25 | 0:19:29 | |
there are 200 per square metre per second. | 0:19:29 | 0:19:32 | |
Here, just one per square metre per hour. This is a very huge shielding. | 0:19:32 | 0:19:36 | |
Thanks to the mountain above it, | 0:19:39 | 0:19:41 | |
this vast chamber is a natural laboratory for neutrino research. | 0:19:41 | 0:19:46 | |
It was here, in 2008, that scientists began work | 0:19:46 | 0:19:50 | |
on a sophisticated experiment designed to study | 0:19:50 | 0:19:53 | |
the nature of neutrinos. | 0:19:53 | 0:19:55 | |
It was called the Oscillation Project with Emulsion Tracking Apparatus, | 0:19:55 | 0:20:00 | |
or OPERA for short. | 0:20:00 | 0:20:03 | |
At this stage, they had no idea of the impact that OPERA would have. | 0:20:03 | 0:20:08 | |
The OPERA experiment is an experiment designed to study | 0:20:08 | 0:20:12 | |
the properties of neutrinos. | 0:20:12 | 0:20:14 | |
It consists of a huge detector which is designed | 0:20:14 | 0:20:17 | |
to try and find as many of them as it can. | 0:20:17 | 0:20:19 | |
Once it's found them and counted them, | 0:20:19 | 0:20:21 | |
it wants to test their properties and enable us to know more about | 0:20:21 | 0:20:25 | |
what they're doing, what their nature is | 0:20:25 | 0:20:28 | |
and in fact, anything we can find out about them. | 0:20:28 | 0:20:31 | |
To begin with, measuring the speed of neutrinos | 0:20:32 | 0:20:35 | |
was not at the forefront of the scientists' minds. | 0:20:35 | 0:20:38 | |
They were trying to understand how the three different types | 0:20:38 | 0:20:42 | |
of neutrinos were formed and how they behaved. | 0:20:42 | 0:20:45 | |
The first step of the experiment was to create some neutrinos. | 0:20:45 | 0:20:49 | |
For this, they turned to another underground lab, | 0:20:49 | 0:20:52 | |
CERN in Switzerland. | 0:20:52 | 0:20:55 | |
CERN is most famous for the Large Hadron Collider. | 0:20:56 | 0:21:00 | |
But it was two much less-heralded particle accelerators | 0:21:00 | 0:21:04 | |
that began the OPERA experiment. | 0:21:04 | 0:21:06 | |
The scientists started by generating a beam of protons | 0:21:06 | 0:21:11 | |
which they accelerated around CERN's Proton Synchrotron. | 0:21:11 | 0:21:14 | |
The proton beam was then passed into the Super Proton Synchrotron | 0:21:14 | 0:21:18 | |
to accelerate them even further. | 0:21:18 | 0:21:20 | |
The resulting high-energy beam of protons | 0:21:20 | 0:21:23 | |
was slammed into a graphite target. | 0:21:23 | 0:21:25 | |
This produced a cocktail of exotic sub-atomic particles, | 0:21:25 | 0:21:29 | |
including neutrinos, which then flew off through the Earth | 0:21:29 | 0:21:33 | |
in the direction of Gran Sasso. | 0:21:33 | 0:21:35 | |
The 730 kilometre journey took them 2.4 milliseconds. | 0:21:37 | 0:21:43 | |
They came from that direction. Geneva is in that direction. | 0:21:43 | 0:21:48 | |
Several billions of neutrinos are produced every day | 0:21:49 | 0:21:52 | |
at the CERN accelerators. | 0:21:52 | 0:21:54 | |
They go through the Earth's crust and they reach the OPERA detector. | 0:21:54 | 0:21:59 | |
Even with billions of neutrinos streaming into the laboratory, | 0:22:01 | 0:22:05 | |
detecting them still wasn't easy. | 0:22:05 | 0:22:07 | |
The key was the huge detector at the heart of the Gran Sasso lab. | 0:22:07 | 0:22:12 | |
It's made from 150,000 bricks of lead, and weighs 4,500 tonnes. | 0:22:14 | 0:22:21 | |
Lead is particularly dense, | 0:22:23 | 0:22:25 | |
which increases the chances of a neutrino encountering a nucleus. | 0:22:25 | 0:22:29 | |
As the neutrinos smashed into the lead nucleus, | 0:22:32 | 0:22:35 | |
they created charged particles, | 0:22:35 | 0:22:37 | |
which are detected as tiny flashes of light. | 0:22:37 | 0:22:40 | |
You can see that with OPERA, it's a waiting game. | 0:22:42 | 0:22:47 | |
You fire a neutrino beam and you wait, | 0:22:47 | 0:22:49 | |
and you count as many of these interactions as you can. | 0:22:49 | 0:22:52 | |
The process generated about 30 flashes of light a day, | 0:22:52 | 0:22:56 | |
and provided a chance to test more | 0:22:56 | 0:22:58 | |
than just the type of neutrino arriving. | 0:22:58 | 0:23:01 | |
The nice thing about this experiment is, although it was set up | 0:23:01 | 0:23:05 | |
to study the behaviour of neutrinos in a very fundamental sense | 0:23:05 | 0:23:08 | |
and the types of neutrinos and how they might change into each other, | 0:23:08 | 0:23:11 | |
is that you can also study more basic properties of them. | 0:23:11 | 0:23:15 | |
And what OPERA decided they could measure was the speed | 0:23:15 | 0:23:18 | |
at which neutrinos travel. | 0:23:18 | 0:23:20 | |
That's quite an easy thing to measure because you know a distance, | 0:23:20 | 0:23:24 | |
you know where neutrinos were produced, | 0:23:24 | 0:23:26 | |
you know where you're finding them and how long they took to get there | 0:23:26 | 0:23:29 | |
if you have a clock where you produced it | 0:23:29 | 0:23:32 | |
and a clock in your experiment where you've made the measurement. | 0:23:32 | 0:23:35 | |
That's speed. Speed is just the distance covered | 0:23:35 | 0:23:37 | |
in a certain amount of time. | 0:23:37 | 0:23:39 | |
Nobody had anticipated what happened | 0:23:41 | 0:23:44 | |
when they started measuring how long it took the neutrinos to arrive. | 0:23:44 | 0:23:48 | |
They seemed to arrive early. Earlier than the laws of physics allow. | 0:23:48 | 0:23:53 | |
60 billionths of a second, or 60 nanoseconds sooner | 0:23:53 | 0:23:57 | |
than a beam of light would, if it were to cover the same distance. | 0:23:57 | 0:24:00 | |
That meant that the neutrinos had travelled at just over | 0:24:00 | 0:24:04 | |
two thousands of 1% faster than the speed of light. | 0:24:04 | 0:24:08 | |
If I was on a motorway, I wouldn't expect to get into trouble | 0:24:08 | 0:24:12 | |
for exceeding the speed limit by that small amount, | 0:24:12 | 0:24:15 | |
but not in physics. | 0:24:15 | 0:24:17 | |
The thing about an absolute speed limit is that it is absolute - | 0:24:17 | 0:24:20 | |
it can't be exceeded in any circumstances, | 0:24:20 | 0:24:23 | |
by however small an amount. | 0:24:23 | 0:24:26 | |
Under our current understanding of the universe, | 0:24:26 | 0:24:28 | |
this just isn't possible. | 0:24:28 | 0:24:30 | |
The researchers themselves were pretty shocked by the results. | 0:24:33 | 0:24:37 | |
They spent many months looking for mistakes. | 0:24:37 | 0:24:40 | |
They brought in outside experts. | 0:24:40 | 0:24:42 | |
They pored over the figures hundreds of times, | 0:24:42 | 0:24:45 | |
searching for an error. | 0:24:45 | 0:24:47 | |
They even made sure they'd factored the movement | 0:24:47 | 0:24:50 | |
of the continents that changes the distance | 0:24:50 | 0:24:52 | |
between Italy and Switzerland by small amounts. | 0:24:52 | 0:24:55 | |
But they couldn't find any mistakes, so they decided to publish. | 0:24:56 | 0:25:03 | |
When the news broke, it caused a sensation. | 0:25:03 | 0:25:06 | |
The theory that nothing travels faster than the speed of light is challenged. | 0:25:09 | 0:25:13 | |
The measurements could be wrong or there's some unknown... | 0:25:13 | 0:25:16 | |
Scientists have discovered that some tiny particles | 0:25:16 | 0:25:19 | |
seem to break that rule. | 0:25:19 | 0:25:20 | |
They seem to be travelling faster than the speed of light. | 0:25:20 | 0:25:23 | |
For physicists, this is earth-shaking if true. | 0:25:23 | 0:25:26 | |
It has created a huge furore, basically because if it was true, | 0:25:26 | 0:25:32 | |
then it would be so astonishing and important. | 0:25:32 | 0:25:36 | |
If the velocity of light turned out not to be absolute, | 0:25:36 | 0:25:40 | |
we just have to tear up all the textbooks and start all over again. | 0:25:40 | 0:25:45 | |
For me, it would mean the direction | 0:25:45 | 0:25:49 | |
of my own research was wrong. | 0:25:49 | 0:25:53 | |
So...it WOULD be a revolution, but to me, | 0:25:53 | 0:25:56 | |
it would also mean that nature's just playing tricks with us. | 0:25:56 | 0:26:00 | |
On the other hand, it would be nice if it were true. | 0:26:00 | 0:26:05 | |
Ever since the paper was published, | 0:26:05 | 0:26:07 | |
the internet has been buzzing with debate. | 0:26:07 | 0:26:10 | |
There are over 100 papers that have been uploaded in the last few weeks. | 0:26:10 | 0:26:15 | |
For me, this is a great example of science in action. | 0:26:15 | 0:26:19 | |
The OPERA team found some data that they couldn't explain. | 0:26:19 | 0:26:22 | |
For months, they'd been questioning it, doubting it, repeating it, | 0:26:22 | 0:26:26 | |
and only after intense scrutiny did they eventually publish it, | 0:26:26 | 0:26:30 | |
not in some triumphalist way, but asking the scientific community | 0:26:30 | 0:26:35 | |
to see where they might have made a mistake. | 0:26:35 | 0:26:37 | |
Not surprisingly, many of the responses have been sceptical. | 0:26:40 | 0:26:43 | |
And there are good reasons for doubting the figures, | 0:26:43 | 0:26:47 | |
based on both theory and experimental data. | 0:26:47 | 0:26:50 | |
The first problem is that the finding calls into question | 0:26:51 | 0:26:55 | |
one of the fundamental principles | 0:26:55 | 0:26:57 | |
that underpins our understanding of the universe - | 0:26:57 | 0:27:00 | |
cause... | 0:27:00 | 0:27:02 | |
and effect. | 0:27:02 | 0:27:04 | |
Cause and effect is a simple, yet powerful idea. | 0:27:05 | 0:27:09 | |
One thing follows another in a logically-ordered sequence. | 0:27:09 | 0:27:13 | |
The important thing is that events stay in the same order. | 0:27:13 | 0:27:17 | |
If I drink my coffee, I drink the coffee before I put the cup down. | 0:27:17 | 0:27:21 | |
A happened before B. | 0:27:22 | 0:27:26 | |
That's important cos A might have caused B. | 0:27:26 | 0:27:28 | |
Einstein's theory respects the relationship | 0:27:32 | 0:27:34 | |
between cause and effect, because with an absolute speed limit, | 0:27:34 | 0:27:39 | |
the speed of light, time can only flow in one direction. | 0:27:39 | 0:27:43 | |
If that isn't the case, | 0:27:43 | 0:27:44 | |
then the world can quickly become a very strange place indeed. | 0:27:44 | 0:27:48 | |
Here's an example of what might happen. | 0:27:48 | 0:27:51 | |
I'm going to send a text to my friend | 0:27:53 | 0:27:55 | |
with the winning lottery ticket numbers which were just announced. | 0:27:55 | 0:27:59 | |
The lottery numbers were... | 0:27:59 | 0:28:04 | |
2, 3, 5, 7, 11, and 13. | 0:28:04 | 0:28:11 | |
Press "send". | 0:28:11 | 0:28:13 | |
Now, let's suppose my friend and I have both got phones | 0:28:13 | 0:28:16 | |
that can send messages faster than the speed of light. | 0:28:16 | 0:28:19 | |
For this to work my friend has got to be moving relative to me, | 0:28:19 | 0:28:23 | |
so let's suppose that she's on a spaceship. | 0:28:23 | 0:28:25 | |
It's a spaceship that travels close to the speed of light. | 0:28:25 | 0:28:30 | |
This means that if I send a message that can travel faster | 0:28:30 | 0:28:34 | |
than the speed of light, | 0:28:34 | 0:28:36 | |
then, as far as she's concerned, it would arrive | 0:28:36 | 0:28:39 | |
before it had been sent. | 0:28:39 | 0:28:41 | |
Then, it's possible for me to send her a text | 0:28:43 | 0:28:47 | |
and for her to reply so that I get the reply before | 0:28:47 | 0:28:50 | |
I've even sent the original text, which is pretty weird. | 0:28:50 | 0:28:54 | |
Things get even weirder | 0:28:55 | 0:28:57 | |
if you start to think whether I can actually act on my friend's text. | 0:28:57 | 0:29:01 | |
I could now change my lottery numbers to the winning numbers | 0:29:01 | 0:29:04 | |
and become a millionaire. | 0:29:04 | 0:29:06 | |
I can change my past, which just doesn't make sense. | 0:29:06 | 0:29:11 | |
With the order of events all scrambled up, we find ourselves | 0:29:11 | 0:29:16 | |
in a universe more traditionally inhabited by science fiction. | 0:29:16 | 0:29:20 | |
If something can travel faster than the speed of light, | 0:29:20 | 0:29:23 | |
then, in principle, time travel is possible. | 0:29:23 | 0:29:28 | |
You'd venture into that forbidden region where you are influencing | 0:29:28 | 0:29:32 | |
things that you shouldn't, according to Einstein. | 0:29:32 | 0:29:34 | |
This causes paradoxes because you can go back in time | 0:29:34 | 0:29:37 | |
and kill your grandmother before you were born, all this nonsense. | 0:29:37 | 0:29:41 | |
For physicists, a consistent theory of the universe in which | 0:29:42 | 0:29:46 | |
we can travel back in time to win the lottery or kill | 0:29:46 | 0:29:49 | |
our grandmother is almost impossible to imagine. | 0:29:49 | 0:29:52 | |
It makes you wonder, | 0:29:54 | 0:29:55 | |
are the speeding neutrinos playing some sort of joke on us? | 0:29:55 | 0:30:01 | |
A barman says, "Sorry, we don't serve neutrinos." | 0:30:01 | 0:30:04 | |
A neutrino walks into a bar. | 0:30:04 | 0:30:07 | |
In other words, neutrinos that travel faster | 0:30:09 | 0:30:12 | |
than the speed of light imply all sorts of ideas | 0:30:12 | 0:30:15 | |
that don't tally with our everyday experience of the universe. | 0:30:15 | 0:30:20 | |
Another reason why many scientists are sceptical | 0:30:20 | 0:30:23 | |
that neutrinos really can break the light barrier | 0:30:23 | 0:30:26 | |
is because it contradicts previous results. | 0:30:26 | 0:30:29 | |
This is not the first time that the speed of neutrinos | 0:30:29 | 0:30:33 | |
has been measured. | 0:30:33 | 0:30:35 | |
In fact, there's one particularly famous observation | 0:30:35 | 0:30:39 | |
that was made back in the 1980s. | 0:30:39 | 0:30:41 | |
The reason you probably haven't heard about it | 0:30:41 | 0:30:44 | |
is because the results were in perfect accord | 0:30:44 | 0:30:46 | |
with Einstein's theories, so no news headlines and no TV programmes. | 0:30:46 | 0:30:51 | |
The action began on February 23rd, 1987. | 0:31:02 | 0:31:07 | |
Astronomers realised that a star on the fringes | 0:31:14 | 0:31:16 | |
of the Tarantula Nebula in the Large Magellanic Cloud had exploded. | 0:31:16 | 0:31:21 | |
It's called a supernova, one of the most violent | 0:31:21 | 0:31:25 | |
and destructive events in the universe. | 0:31:25 | 0:31:28 | |
We observed it in 1987. It actually happened over 100,000 years ago | 0:31:30 | 0:31:36 | |
and it took the light from that supernova, | 0:31:36 | 0:31:39 | |
the energy from that supernova, over 100,000 years to reach us. | 0:31:39 | 0:31:43 | |
This star exploding threw out enormous amounts of energy. | 0:31:47 | 0:31:51 | |
Most of it was in neutrinos, some of it was in light. | 0:31:51 | 0:31:54 | |
The light from the supernova and the neutrinos from the supernova | 0:31:54 | 0:31:58 | |
reached us almost at exactly the same time. | 0:31:58 | 0:32:02 | |
Scientists calculated that the neutrinos travelled | 0:32:09 | 0:32:13 | |
just a tiny bit slower than the speed of light, | 0:32:13 | 0:32:16 | |
just as you'd expect if Einstein was right. | 0:32:16 | 0:32:19 | |
Had the neutrinos from the supernova | 0:32:22 | 0:32:24 | |
travelled at the speed that the OPERA scientists recorded, | 0:32:24 | 0:32:27 | |
in other words, a little bit faster than the speed of light, | 0:32:27 | 0:32:30 | |
then they would have arrived here | 0:32:30 | 0:32:33 | |
four years before the light from the supernova. | 0:32:33 | 0:32:36 | |
That didn't happen. | 0:32:36 | 0:32:38 | |
Given this rock-solid verification of Einstein's theory, | 0:32:40 | 0:32:43 | |
it's not surprising that when the OPERA results were published | 0:32:43 | 0:32:46 | |
this year, suggesting that neutrinos travelled faster than light, | 0:32:46 | 0:32:50 | |
most people thought that, somewhere along the line, | 0:32:50 | 0:32:53 | |
they must have made a mistake. | 0:32:53 | 0:32:55 | |
When I first heard the result, I was...sceptical | 0:32:57 | 0:33:02 | |
and I think that most of my colleagues were very sceptical also. | 0:33:02 | 0:33:07 | |
I heard about this result in the coffee bar at CERN | 0:33:07 | 0:33:11 | |
about two weeks before it came out and I laughed. | 0:33:11 | 0:33:14 | |
I was like "Ah, well, they've got something wrong, haven't they?!" | 0:33:14 | 0:33:17 | |
Data error seems plausible when you consider the details | 0:33:17 | 0:33:21 | |
of what they were measuring. | 0:33:21 | 0:33:23 | |
Remember, those neutrinos arrived 60 billionths of a second, | 0:33:23 | 0:33:27 | |
that's 60 nanoseconds, early. | 0:33:27 | 0:33:29 | |
It's not the sort of measurement where a standard stopwatch | 0:33:29 | 0:33:32 | |
would be much use. | 0:33:32 | 0:33:33 | |
It's worth considering the astonishing nature | 0:33:39 | 0:33:43 | |
of the measurements we're talking about. | 0:33:43 | 0:33:46 | |
The world of athletics provides a good comparison, | 0:33:46 | 0:33:48 | |
a high precision sport relying on super accurate measurements. | 0:33:48 | 0:33:53 | |
In a 100 metre sprint the race is often so close | 0:33:55 | 0:33:58 | |
that it results in a photo-finish. | 0:33:58 | 0:34:01 | |
The winning athletes may be separated from the rest by just | 0:34:03 | 0:34:06 | |
100th of a second. A gap of 100th of a second in time | 0:34:06 | 0:34:10 | |
translates into roughly ten centimetres in distance. | 0:34:10 | 0:34:14 | |
Now, compare that to the neutrinos' journey from Switzerland to Italy. | 0:34:17 | 0:34:22 | |
The neutrinos that arrived in Gran Sasso | 0:34:22 | 0:34:25 | |
did so just 60 billionths of a second ahead of schedule. | 0:34:25 | 0:34:29 | |
If a 100 metre sprint were to be won by 60 billionths of a second, | 0:34:30 | 0:34:36 | |
then that would mean the winner would have been just under | 0:34:36 | 0:34:39 | |
1,000th of a millimetre ahead of the field. | 0:34:39 | 0:34:42 | |
So the OPERA team were attempting to measure time | 0:34:49 | 0:34:53 | |
over almost inconceivably small periods. | 0:34:53 | 0:34:55 | |
Even the tiniest error could have huge implications. | 0:35:01 | 0:35:05 | |
The scientists themselves have admitted that there are inaccuracies | 0:35:08 | 0:35:12 | |
with their measurement. | 0:35:12 | 0:35:13 | |
Firstly, they could have got the distance between CERN | 0:35:13 | 0:35:17 | |
and Gran Sasso wrong, but only by about 20 centimetres. | 0:35:17 | 0:35:22 | |
It is also difficult to pin down the exact moment the neutrinos hit | 0:35:22 | 0:35:26 | |
the target at Gran Sasso. | 0:35:26 | 0:35:29 | |
But by far the biggest uncertainty comes from recording exactly | 0:35:29 | 0:35:33 | |
when the neutrinos left CERN. | 0:35:33 | 0:35:34 | |
Yet, even adding together all the potential errors identified so far, | 0:35:34 | 0:35:39 | |
it only gives you around ten nanoseconds. | 0:35:39 | 0:35:43 | |
That still doesn't come close to explaining why the neutrinos | 0:35:43 | 0:35:47 | |
arrived 60 nanoseconds early. | 0:35:47 | 0:35:50 | |
But some of the physicists who have been poring over the results | 0:35:54 | 0:35:58 | |
reckon that a much larger inaccuracy could be lurking | 0:35:58 | 0:36:02 | |
deep in the detail of when exactly the neutrinos started their journey. | 0:36:02 | 0:36:05 | |
So what they do is measure this kind of pulse of the protons at CERN | 0:36:09 | 0:36:16 | |
and these things leave with some kind of shape. | 0:36:16 | 0:36:20 | |
Then, in OPERA, they sit there waiting. | 0:36:20 | 0:36:23 | |
There are billions of protons at CERN producing lots of neutrinos. | 0:36:23 | 0:36:27 | |
Very few of those neutrinos actually interact in the OPERA detector, | 0:36:27 | 0:36:32 | |
so you sit there and wait and you get a bang. There's one, bang. | 0:36:32 | 0:36:35 | |
There's another one. | 0:36:35 | 0:36:36 | |
Over time you build up a shape of the arrival time of the neutrinos | 0:36:36 | 0:36:40 | |
and you fit the two together. You fit the proton pulse shape | 0:36:40 | 0:36:43 | |
and you fit the neutrino arrival shape. | 0:36:43 | 0:36:45 | |
But the neutrino arrival shape is made up of many fewer events | 0:36:45 | 0:36:49 | |
than the proton one. | 0:36:49 | 0:36:51 | |
John Butterworth is concerned that the OPERA scientists | 0:36:54 | 0:36:57 | |
have assumed that these two shapes are the same | 0:36:57 | 0:37:00 | |
when there are good reasons why they might not be. | 0:37:00 | 0:37:04 | |
As far as I can see, they assume that the underlying shape | 0:37:04 | 0:37:08 | |
of the neutrino arrival is identical to the underlying shape | 0:37:08 | 0:37:11 | |
that they know very well, of the protons leaving. | 0:37:11 | 0:37:13 | |
It's not obvious to me that that's true | 0:37:13 | 0:37:15 | |
because the OPERA experiment, you see a very small fraction of the beam. | 0:37:15 | 0:37:21 | |
The beam is much bigger than the detector. | 0:37:21 | 0:37:23 | |
It's a kilometre across and the detector's much smaller than that. | 0:37:23 | 0:37:28 | |
Also, these protons, a lot happens to them before they become neutrinos. | 0:37:28 | 0:37:32 | |
There are various ways in which that shape | 0:37:32 | 0:37:34 | |
could be slightly different. You don't need much of a difference | 0:37:34 | 0:37:38 | |
to undermine the precision of the measurement. | 0:37:38 | 0:37:40 | |
I'm not saying this is definitely a mistake, | 0:37:40 | 0:37:43 | |
but I'm surprised that they didn't treat that more seriously | 0:37:43 | 0:37:46 | |
and I think I'd have gone, "That needs to be checked." | 0:37:46 | 0:37:49 | |
So far, dozens of suggestions have been made about potential errors | 0:37:55 | 0:38:00 | |
in the experiment, but none of them | 0:38:00 | 0:38:02 | |
have yet been proven to explain the faster than light measurement. | 0:38:02 | 0:38:07 | |
What strikes me about the paper the team have prepared | 0:38:07 | 0:38:10 | |
is just how meticulous it is. | 0:38:10 | 0:38:11 | |
This must be one of the most accurate measurements ever made. | 0:38:11 | 0:38:15 | |
So, at this stage, I think it's right to keep a sceptical, | 0:38:15 | 0:38:18 | |
but open mind. | 0:38:18 | 0:38:20 | |
There's one intriguing additional piece of evidence | 0:38:21 | 0:38:24 | |
that offers some support for the OPERA team. | 0:38:24 | 0:38:27 | |
In 2007, scientists from Fermilab, | 0:38:27 | 0:38:30 | |
the high energy physics laboratory just outside Chicago, | 0:38:30 | 0:38:34 | |
made a similar, but less precise, neutrino measurement | 0:38:34 | 0:38:38 | |
using an experiment called MINOS. | 0:38:38 | 0:38:41 | |
MINOS fired neutrino beams similar to those detected at OPERA | 0:38:41 | 0:38:45 | |
to a detector in a mine 800 kilometres away in Minnesota. | 0:38:45 | 0:38:50 | |
They measured the time between Chicago where the particles | 0:38:53 | 0:38:56 | |
are produced and the this mine in Minnesota and they get an effect | 0:38:56 | 0:39:00 | |
which goes in the same direction as what OPERA has seen, | 0:39:00 | 0:39:04 | |
so that the neutrinos are a bit faster than you'd expect. | 0:39:04 | 0:39:07 | |
The MINOS neutrinos did seem to be moving faster | 0:39:08 | 0:39:12 | |
than the speed of light. | 0:39:12 | 0:39:14 | |
However, because their equipment was less precise, | 0:39:14 | 0:39:17 | |
the MINOS scientists had to allow for a larger uncertainty | 0:39:17 | 0:39:21 | |
than the Italians. | 0:39:21 | 0:39:23 | |
And when this lack of precision was accounted for, | 0:39:23 | 0:39:25 | |
the results didn't appear to be statistically significant. | 0:39:25 | 0:39:29 | |
So nobody got really very excited about this at the time. | 0:39:32 | 0:39:35 | |
Now, this will mean, with this new result coming out, | 0:39:35 | 0:39:41 | |
that MINOS and another experiment in Japan, which is called T2K, | 0:39:41 | 0:39:46 | |
will both work very hard to get a similar measurement | 0:39:46 | 0:39:52 | |
with a similar position in the next few years. | 0:39:52 | 0:39:55 | |
But it will take a few years, I think. | 0:39:55 | 0:39:58 | |
So until we've got evidence there really is an error | 0:39:59 | 0:40:02 | |
in the OPERA results, it only seems fair to explore other options. | 0:40:02 | 0:40:06 | |
This is where it becomes particularly interesting, | 0:40:06 | 0:40:09 | |
especially if you're a mathematician. | 0:40:09 | 0:40:12 | |
Because there's a whole range of other theories | 0:40:12 | 0:40:14 | |
that could explain this. | 0:40:14 | 0:40:16 | |
At stake is one of the greatest prizes of science, | 0:40:16 | 0:40:18 | |
a theory of everything. | 0:40:18 | 0:40:21 | |
The first issue is to consider whether the speed of light | 0:40:25 | 0:40:28 | |
is really the absolute barrier that Einstein described. | 0:40:28 | 0:40:33 | |
There are at least two arguments that suggest it might be possible, | 0:40:33 | 0:40:37 | |
in certain circumstances, to travel faster than the speed of light. | 0:40:37 | 0:40:41 | |
The intriguing thing is that, mathematically speaking, | 0:40:41 | 0:40:45 | |
travelling faster than the speed of light isn't quite as difficult | 0:40:45 | 0:40:48 | |
as the popular interpretation of Einstein's series suggest. | 0:40:48 | 0:40:52 | |
In fact, from a mathematical point of view, it isn't impossible at all. | 0:40:52 | 0:40:56 | |
To understand why, you need to explore the relationship | 0:40:56 | 0:41:00 | |
between physics and maths. | 0:41:00 | 0:41:03 | |
There are many examples in the history of physics | 0:41:05 | 0:41:08 | |
where maths predicts something that, at first sight, | 0:41:08 | 0:41:11 | |
seems counter-intuitive only for the maths to then to be proved right. | 0:41:11 | 0:41:15 | |
Back in the 1920s, | 0:41:18 | 0:41:20 | |
a scientist called Paul Dirac came up with equations to describe | 0:41:20 | 0:41:24 | |
what happened to electrons when they travel close to the speed of light. | 0:41:24 | 0:41:28 | |
But his equations led to a peculiar conclusion. | 0:41:30 | 0:41:33 | |
They predicted that every particle had an equivalent antiparticle | 0:41:38 | 0:41:43 | |
with an opposite electric charge. | 0:41:43 | 0:41:46 | |
These antiparticles would combine to form antimatter. | 0:41:46 | 0:41:50 | |
At the time, the idea of antimatter seemed mad, | 0:41:52 | 0:41:55 | |
but eventually, incontrovertible evidence | 0:41:55 | 0:41:58 | |
for its existence was found. | 0:41:58 | 0:42:00 | |
And we've seen something similar happen with the prediction | 0:42:02 | 0:42:06 | |
that neutrinos would exist before they'd been observed. | 0:42:06 | 0:42:11 | |
So maths can sometimes suggest solutions that appear impossible | 0:42:11 | 0:42:14 | |
in the real world, but then turn out to be feasible after all. | 0:42:14 | 0:42:19 | |
Surprisingly enough, there are mathematical solutions | 0:42:22 | 0:42:24 | |
to Einstein's equations which do allow particles to go faster | 0:42:24 | 0:42:28 | |
than the speed of light. | 0:42:28 | 0:42:30 | |
We even have a name to describe these theoretical particles | 0:42:30 | 0:42:33 | |
that can do this. They're called tachyons. | 0:42:33 | 0:42:36 | |
Now, I have to admit that, on the surface, | 0:42:36 | 0:42:39 | |
tachyons are pretty strange. | 0:42:39 | 0:42:41 | |
Most notably, their mass is an imaginary number, | 0:42:41 | 0:42:43 | |
but however strange that sounds, it doesn't mean they couldn't exist. | 0:42:43 | 0:42:49 | |
A surprisingly large part of the universe | 0:42:49 | 0:42:51 | |
is built on imaginary numbers. | 0:42:51 | 0:42:54 | |
So what's special about tachyons? | 0:42:54 | 0:42:56 | |
How could they travel faster than the speed of light? | 0:42:56 | 0:42:59 | |
The key is this... | 0:42:59 | 0:43:00 | |
Einstein's formula forbids any particle to travel THROUGH the speed | 0:43:00 | 0:43:05 | |
of light, because as it accelerates, its mass get greater and greater. | 0:43:05 | 0:43:10 | |
But if a particle is formed when it's already travelling | 0:43:10 | 0:43:13 | |
BEYOND the speed of light, then it gets past this problem. | 0:43:13 | 0:43:17 | |
Even before these results, a few scientists have suggested | 0:43:17 | 0:43:20 | |
that neutrinos might have a tachyonic behaviour. | 0:43:20 | 0:43:23 | |
In other words, there might be a link between tachyons and neutrinos. | 0:43:23 | 0:43:28 | |
At this stage, it's too early to say whether this theory has any legs, | 0:43:28 | 0:43:32 | |
but it's still good to know from a mathematical perspective | 0:43:32 | 0:43:36 | |
that it IS possible to travel faster than the speed of light. | 0:43:36 | 0:43:40 | |
There's another reason for doubting that Einstein's speed limit | 0:43:44 | 0:43:48 | |
is quite as absolute as it appears. | 0:43:48 | 0:43:50 | |
In fact, there are certain circumstances where the idea | 0:43:50 | 0:43:53 | |
of an ultimate speed limit doesn't make any sense. | 0:43:53 | 0:43:57 | |
The exciting thing for me about controversial results like these | 0:43:59 | 0:44:03 | |
are that they shake things up. | 0:44:03 | 0:44:05 | |
They provoke lots of questions, demand new ideas. | 0:44:05 | 0:44:08 | |
In doing so, they shine a light on theoretical problems that tend | 0:44:08 | 0:44:12 | |
to get swept under the carpet. | 0:44:12 | 0:44:15 | |
Unless you study science, you could be forgiven | 0:44:16 | 0:44:19 | |
for thinking that the theories used by academics to describe | 0:44:19 | 0:44:22 | |
the universe all join up nicely, but that's not always the case. | 0:44:22 | 0:44:27 | |
Obviously, this result contradicts what you find in textbooks, | 0:44:31 | 0:44:34 | |
but if you're actually working in the frontier of physics | 0:44:34 | 0:44:38 | |
and trying to find new theories, this is not as tragic as you might think. | 0:44:38 | 0:44:43 | |
It's a crisis, but we need a crisis because there are lots of things | 0:44:43 | 0:44:46 | |
in physics, in those textbooks, which don't really make any sense. | 0:44:46 | 0:44:51 | |
Einstein's theories describe with astonishing accuracy | 0:45:05 | 0:45:08 | |
the universe we can see. | 0:45:08 | 0:45:10 | |
The planets, the stars, even the distant galaxies. | 0:45:12 | 0:45:17 | |
And here, the speed of light is indeed the ultimate speed limit. | 0:45:26 | 0:45:30 | |
But even within this familiar universe, | 0:45:32 | 0:45:34 | |
there are places Einstein's theories don't work. | 0:45:34 | 0:45:38 | |
In extreme conditions, the rules break down. | 0:45:41 | 0:45:46 | |
Physics hasn't yet developed the language to understand | 0:45:47 | 0:45:50 | |
what happens inside a black hole, for example. | 0:45:50 | 0:45:54 | |
Einstein's ultimate speed limit also causes problems | 0:45:57 | 0:46:01 | |
in trying to explain how the universe evolved | 0:46:01 | 0:46:03 | |
from the birth of everything... | 0:46:03 | 0:46:05 | |
EXPLOSION | 0:46:05 | 0:46:07 | |
..the Big Bang. | 0:46:07 | 0:46:09 | |
Physicists think that at the moment of the Big Bang, | 0:46:13 | 0:46:16 | |
everything in the universe was crammed into one tiny point, | 0:46:16 | 0:46:20 | |
smaller than an atom. | 0:46:20 | 0:46:23 | |
At the Big Bang, the universe expanded at astonishing speed. | 0:46:27 | 0:46:32 | |
As it expanded, it cooled, allowing fundamental particles, | 0:46:32 | 0:46:36 | |
then protons and neutrons, to condense out of the energetic soup. | 0:46:36 | 0:46:41 | |
All of this happened in less than a second. | 0:46:41 | 0:46:44 | |
Over the next 400,000 years, | 0:46:50 | 0:46:52 | |
the universe cooled enough to allow the first hydrogen atoms to form, | 0:46:52 | 0:46:56 | |
creating vast clouds of gas that finally began to collapse | 0:46:56 | 0:47:00 | |
into the familiar stars and galaxies | 0:47:00 | 0:47:03 | |
that make up the universe as we see it today. | 0:47:03 | 0:47:05 | |
But here's the big problem. | 0:47:16 | 0:47:18 | |
Accepted science only seems to account for what happened | 0:47:18 | 0:47:22 | |
just after the Big Bang. | 0:47:22 | 0:47:25 | |
If you want to understand what happened to our universe | 0:47:25 | 0:47:28 | |
in its very first moments, Einstein can't help you. | 0:47:28 | 0:47:30 | |
And there's a particular problem with Einstein's idea | 0:47:32 | 0:47:36 | |
of a constant cosmic speed limit, the speed of light, | 0:47:36 | 0:47:40 | |
when you apply it to the Big Bang. | 0:47:40 | 0:47:42 | |
Some physicists believe that for the universe around us | 0:47:46 | 0:47:49 | |
to be as we see it today, then that speed limit must have been | 0:47:49 | 0:47:53 | |
broken in these instants immediately after the Big Bang. | 0:47:53 | 0:47:57 | |
In cosmology, it's very difficult to explain why the Big Bang universe | 0:48:01 | 0:48:05 | |
is what it is if you have the speed limit which is very constraining | 0:48:05 | 0:48:09 | |
in the early universe. | 0:48:09 | 0:48:10 | |
You don't have enough time to produce the universe if you have this | 0:48:10 | 0:48:14 | |
speed limit which limits your range of action and ties your hands. | 0:48:14 | 0:48:18 | |
So raising the speed limit could be exactly the missing ingredient | 0:48:18 | 0:48:21 | |
for explaining the Big Bang. | 0:48:21 | 0:48:23 | |
This is a controversial theory. | 0:48:26 | 0:48:29 | |
But it does support the idea that there are extreme circumstances | 0:48:35 | 0:48:40 | |
in which the speed of light | 0:48:40 | 0:48:41 | |
is not the ultimate speed limit of the universe. | 0:48:41 | 0:48:44 | |
However, the most exciting attempt to explain | 0:48:48 | 0:48:51 | |
how neutrinos could travel faster than light | 0:48:51 | 0:48:54 | |
comes from the very frontier of theoretical physics. | 0:48:54 | 0:48:59 | |
Scientists are attempting to create a unified theory of everything. | 0:48:59 | 0:49:04 | |
At the moment, there are two sets of theories that explain the universe. | 0:49:04 | 0:49:09 | |
Einstein's theories which explain the world of the large, | 0:49:09 | 0:49:12 | |
the things we can see in the universe. | 0:49:12 | 0:49:15 | |
And a second theory, called quantum mechanics, describes the world | 0:49:15 | 0:49:19 | |
of the small, like subatomic particles. | 0:49:19 | 0:49:22 | |
And they just don't join up. | 0:49:24 | 0:49:26 | |
The dilemma we faced at the beginning of this century is that the two main | 0:49:26 | 0:49:29 | |
pillars of the last century's physics seem to be mutually incompatible. | 0:49:29 | 0:49:34 | |
So if something big has to give... | 0:49:35 | 0:49:38 | |
and this August, perhaps, a new scientific revolution. | 0:49:38 | 0:49:42 | |
There are, however, a number of candidates | 0:49:42 | 0:49:45 | |
for this grand unifying theory. The main one is string theory. | 0:49:45 | 0:49:49 | |
And the exciting thing that's beginning to form | 0:49:49 | 0:49:51 | |
in some scientists' minds is that perhaps the OPERA results | 0:49:51 | 0:49:54 | |
are the first experimental proof of it. | 0:49:54 | 0:49:57 | |
String theory is based on the idea that we only have | 0:50:00 | 0:50:03 | |
a very partial view of the universe. | 0:50:03 | 0:50:06 | |
It suggests that the fundamental particles we see in the universe | 0:50:06 | 0:50:10 | |
are all related to each other through a string. | 0:50:10 | 0:50:13 | |
In string theory, the particles are still there, | 0:50:15 | 0:50:19 | |
but they no longer occupy centre stage. | 0:50:19 | 0:50:22 | |
The fundamental object is a one-dimensional string. | 0:50:22 | 0:50:26 | |
One can think in an analogy of a violin string. | 0:50:26 | 0:50:30 | |
The string can vibrate and each mode of vibration, each note, | 0:50:30 | 0:50:34 | |
if you like, represents a different elementary particle. | 0:50:34 | 0:50:38 | |
So this note is an electron, that note a quark, | 0:50:38 | 0:50:43 | |
and yet another note could be a Higgs boson. | 0:50:43 | 0:50:46 | |
So it's a much more economical way of describing dozens | 0:50:46 | 0:50:50 | |
of elementary particles by a single string. | 0:50:50 | 0:50:53 | |
There are plenty of mathematical equations | 0:51:00 | 0:51:02 | |
that describe string theory, | 0:51:02 | 0:51:04 | |
but they lead to a rather uncomfortable conclusion. | 0:51:04 | 0:51:07 | |
The universe needs a lot more dimensions | 0:51:07 | 0:51:09 | |
than we are used to dealing with. | 0:51:09 | 0:51:11 | |
We are used to the idea of living in a three-dimensional world. | 0:51:13 | 0:51:18 | |
Forwards, backwards, up, down, left, right. | 0:51:18 | 0:51:22 | |
And time is the fourth dimension. | 0:51:22 | 0:51:24 | |
But string theory says there have to be an extra six. | 0:51:24 | 0:51:28 | |
But they'd have to be curled up to one unobservably small size, | 0:51:28 | 0:51:32 | |
or else rendered invisible in some other way, | 0:51:32 | 0:51:35 | |
if they're to describe the universe we find ourselves in. | 0:51:35 | 0:51:39 | |
Scientists have come up with wonderful language | 0:51:41 | 0:51:44 | |
to describe this multi-dimensional world. | 0:51:44 | 0:51:46 | |
The 3D universe we are familiar with is known as a membrane, | 0:51:46 | 0:51:50 | |
or "brane" for short. | 0:51:50 | 0:51:52 | |
But this is just part of something much larger, | 0:51:52 | 0:51:55 | |
which includes all the other membranes or dimensions. | 0:51:55 | 0:51:58 | |
And this all-encompassing entity is known as the bulk. | 0:51:58 | 0:52:03 | |
A one possibility is that our universe, you, me | 0:52:03 | 0:52:07 | |
and everything in it, is a three dimensional brane... | 0:52:07 | 0:52:10 | |
which lives itself in a higher dimensional bulk space time | 0:52:14 | 0:52:18 | |
which may have 10 or 11 dimensions. | 0:52:18 | 0:52:21 | |
And there can be other universes parallel to ours. | 0:52:21 | 0:52:25 | |
The analogy would be slices of bread in a loaf. | 0:52:25 | 0:52:30 | |
So the bulk is the loaf, the brane is the slice of bread. | 0:52:30 | 0:52:34 | |
And we live on the brane, and light is confined just to the brane. | 0:52:34 | 0:52:40 | |
It doesn't travel in the bulk. | 0:52:40 | 0:52:42 | |
So here, then, is one possible explanation. | 0:52:43 | 0:52:47 | |
The neutrinos left CERN travelling at just below the speed of light | 0:52:47 | 0:52:51 | |
on our brane. | 0:52:51 | 0:52:52 | |
They then took a short cut through the bulk and popped back | 0:52:52 | 0:52:56 | |
into our universe or membrane in time to be picked up at Gran Sasso. | 0:52:56 | 0:53:00 | |
If a particle were to leave the brane, | 0:53:01 | 0:53:04 | |
travel in the bulk and reappear on the brane, | 0:53:04 | 0:53:09 | |
it would create the impression to someone living on the brane | 0:53:09 | 0:53:12 | |
that it had travelled faster than light. | 0:53:12 | 0:53:14 | |
There are a couple of rather satisfying elements to this theory. | 0:53:33 | 0:53:37 | |
First, Einstein's theories still hold. | 0:53:43 | 0:53:46 | |
Light still forms the ultimate speed limit in our membrane, | 0:53:46 | 0:53:51 | |
just as Einstein said. | 0:53:51 | 0:53:53 | |
But if particles like neutrinos can travel in the bulk, | 0:54:01 | 0:54:05 | |
they can do so at a faster speed. | 0:54:05 | 0:54:07 | |
Second, it might explain why the supernova neutrinos | 0:54:23 | 0:54:27 | |
that were detected in 1987 travelled slower than the speed of light. | 0:54:27 | 0:54:32 | |
Think of it this way. | 0:54:33 | 0:54:35 | |
Most of the time, when ocean waves form, they behave | 0:54:35 | 0:54:38 | |
in a predictable way, because the energy that forms them | 0:54:38 | 0:54:41 | |
is fairly consistent. | 0:54:41 | 0:54:43 | |
But every now and then, there's a freak wave | 0:54:43 | 0:54:46 | |
formed from a particularly violent collision. | 0:54:46 | 0:54:50 | |
In the same way, neutrinos created at CERN are the products | 0:54:50 | 0:54:54 | |
of incredibly violent collisions, and this could be enough to throw | 0:54:54 | 0:54:58 | |
some of them briefly out of our membrane and into the bulk. | 0:54:58 | 0:55:02 | |
It all sounds rather elegant. | 0:55:11 | 0:55:13 | |
If this explanation is right, | 0:55:13 | 0:55:15 | |
then these faster than light neutrinos offer tantalising evidence | 0:55:15 | 0:55:19 | |
that string theory could indeed be a theory of everything. | 0:55:19 | 0:55:23 | |
But it's only fair to say that many string theorists | 0:55:23 | 0:55:25 | |
are far from convinced. | 0:55:25 | 0:55:27 | |
I've been working on the idea of extra dimensions for over 30 years. | 0:55:27 | 0:55:33 | |
So no-one would be happier than I if the experimentalists were | 0:55:33 | 0:55:37 | |
to find evidence for it. | 0:55:37 | 0:55:40 | |
However, to be frank, although I like the idea of extra dimensions, | 0:55:40 | 0:55:44 | |
this is not the way they are going to show up, in my opinion. | 0:55:44 | 0:55:48 | |
So I am not offering extra dimensions as an explanation | 0:55:48 | 0:55:53 | |
for the phenomenon that the Italian physicists are reporting. | 0:55:53 | 0:55:57 | |
So for the time being, there is no theory that convincingly explains | 0:56:02 | 0:56:07 | |
how the neutrinos appeared to break the speed of light barrier | 0:56:07 | 0:56:11 | |
travelling between Geneva and Gran Sasso. | 0:56:11 | 0:56:15 | |
All scientists have is some idea of the right place | 0:56:15 | 0:56:18 | |
to look for a theoretical explanation. | 0:56:18 | 0:56:22 | |
This could be one of those moments that turns our understanding | 0:56:22 | 0:56:25 | |
on its head yet again, lets us see further into the universe, | 0:56:25 | 0:56:29 | |
lets us understand more about how it ticks, how it sticks together, | 0:56:29 | 0:56:32 | |
how things are related inside it. | 0:56:32 | 0:56:34 | |
If it does that, if we understand more, then it is one of those | 0:56:34 | 0:56:38 | |
magical moments that you get in the history of physics | 0:56:38 | 0:56:41 | |
that just twists your understanding and brings the universe into focus. | 0:56:41 | 0:56:46 | |
If we are seeing the start of that now and we're documenting it, | 0:56:46 | 0:56:49 | |
then we're really, really privileged to be doing so. | 0:56:49 | 0:56:53 | |
At this stage, the argument is nicely poised. | 0:57:01 | 0:57:04 | |
Measurement error, or the beginnings of a seismic breakthrough | 0:57:04 | 0:57:07 | |
in our understanding of the universe? | 0:57:07 | 0:57:09 | |
Nobody knows. What's needed, of course, | 0:57:09 | 0:57:12 | |
is the thing that underpins all of science. | 0:57:12 | 0:57:15 | |
The scientific method demands replication of the results. | 0:57:15 | 0:57:19 | |
If other scientists can't repeat the findings coming from Italy, | 0:57:19 | 0:57:23 | |
we have to begin to doubt the accuracy of those measurements. | 0:57:23 | 0:57:26 | |
However, if they do repeat them, the stage is set for a major challenge | 0:57:26 | 0:57:31 | |
to Einstein and the creation of a grand unifying theory of everything. | 0:57:31 | 0:57:36 | |
Subtitles by Red Bee Media Ltd | 0:57:42 | 0:57:44 | |
E-mail [email protected] | 0:57:44 | 0:57:46 |