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Five days ago, hundreds of the world's brainiest people | 0:00:08 | 0:00:12 | |
descended on a hotel in Chicago. | 0:00:12 | 0:00:15 | |
Good morning, ladies and gentlemen. | 0:00:19 | 0:00:21 | |
They have come to hear news from particle physicists | 0:00:21 | 0:00:24 | |
working at CERN. | 0:00:24 | 0:00:26 | |
Last year, researchers there had started running | 0:00:27 | 0:00:30 | |
the Large Hadron Collider at the highest energy ever... | 0:00:30 | 0:00:34 | |
..and a rumour quickly emerged. | 0:00:36 | 0:00:38 | |
They were on the brink of a huge discovery. | 0:00:38 | 0:00:42 | |
We started hearing these mysterious noises | 0:00:42 | 0:00:45 | |
about something going on at CERN. | 0:00:45 | 0:00:48 | |
This may be what I have been spending an entire lifetime | 0:00:48 | 0:00:51 | |
waiting for. | 0:00:51 | 0:00:53 | |
A strange bump on a graph suggested that they might have discovered | 0:00:53 | 0:00:57 | |
a brand-new particle... | 0:00:57 | 0:00:59 | |
..that could revolutionise physics... | 0:01:00 | 0:01:03 | |
Right here, right now at CERN, in 2016, | 0:01:04 | 0:01:07 | |
is THE most exciting time and place in the history of science. | 0:01:07 | 0:01:10 | |
If you want, really, to change the conditions of humanity, | 0:01:10 | 0:01:15 | |
then you need breakthroughs. | 0:01:15 | 0:01:18 | |
..and could change our understanding of how everything works. | 0:01:18 | 0:01:23 | |
The discovery of a new particle may mean a complete rethinking | 0:01:23 | 0:01:27 | |
of the conceptual basis of the physics world. | 0:01:27 | 0:01:31 | |
For the last eight months, | 0:01:31 | 0:01:34 | |
it looked like the universe was about to be turned upside down... | 0:01:34 | 0:01:38 | |
..and Horizon has been inside CERN following the story. | 0:01:40 | 0:01:44 | |
I doubt that it will be named after me, | 0:01:44 | 0:01:47 | |
but I can think of it like this, that it might be! | 0:01:47 | 0:01:51 | |
There was a short circuit on a circuit-breaker developed | 0:01:53 | 0:01:56 | |
which arced and damaged the nearby equipment. | 0:01:56 | 0:02:00 | |
Two teams of physicists... | 0:02:01 | 0:02:03 | |
..one massive machine... | 0:02:05 | 0:02:07 | |
and a dream. | 0:02:07 | 0:02:09 | |
Was the bump was just a glitch in the data, | 0:02:09 | 0:02:12 | |
or the biggest physics discovery in over a century? | 0:02:12 | 0:02:15 | |
A Nobel prize is possible. | 0:02:15 | 0:02:18 | |
Bonjour. Bienvenue a CERN. | 0:02:47 | 0:02:49 | |
This is the European Organization for Nuclear Research - CERN. | 0:02:51 | 0:02:57 | |
CERN is home to half of the world's particle physicists... | 0:03:00 | 0:03:03 | |
..and the biggest particle-hunting machine that has ever been built. | 0:03:05 | 0:03:09 | |
The Large Hadron Collider, or LHC. | 0:03:11 | 0:03:14 | |
Inside this pipe, two beams of protons | 0:03:16 | 0:03:20 | |
are sent hurtling around a 27km loop | 0:03:20 | 0:03:23 | |
before being smashed together | 0:03:23 | 0:03:25 | |
to create subatomic particles. | 0:03:25 | 0:03:28 | |
In November 2015, researchers here got | 0:03:31 | 0:03:34 | |
a tantalising glimpse of what they thought might be | 0:03:34 | 0:03:38 | |
a brand-new particle. | 0:03:38 | 0:03:39 | |
A particle that could transform our understanding | 0:03:41 | 0:03:44 | |
of how the universe works. | 0:03:44 | 0:03:46 | |
Now they're trying to find it. | 0:03:50 | 0:03:52 | |
The Large Hadron Collider has been hunting for particles since 2009... | 0:04:00 | 0:04:06 | |
..and it's the job of British physicist Mike Lamont | 0:04:08 | 0:04:12 | |
to keep it running. | 0:04:12 | 0:04:13 | |
Today, it's having one of its off days. | 0:04:17 | 0:04:20 | |
This is not a cock-up. | 0:04:22 | 0:04:24 | |
We stop because, | 0:04:24 | 0:04:26 | |
as you can see, | 0:04:26 | 0:04:27 | |
there's a huge amount of stuff down here - | 0:04:27 | 0:04:30 | |
big systems, cooling, ventilation, | 0:04:30 | 0:04:32 | |
cryogenics, etc, | 0:04:32 | 0:04:34 | |
and this stuff needs a bit of periodic tender loving care. | 0:04:34 | 0:04:38 | |
With over 4,000 miles of cabling and 100,000 processor cores, | 0:04:38 | 0:04:43 | |
the LHC is one of the most complicated machines in the world. | 0:04:43 | 0:04:48 | |
She is not a simple beast to operate, | 0:04:48 | 0:04:51 | |
and a lot of time we spend wrestling it under control. | 0:04:51 | 0:04:55 | |
We need very powerful magnets to bend the beam around in a circle, | 0:04:55 | 0:05:00 | |
so basically, these are superconducting magnets, | 0:05:00 | 0:05:03 | |
they're cooled with superfluid helium at 1.9K. | 0:05:03 | 0:05:07 | |
The fact that this actually works at all | 0:05:07 | 0:05:09 | |
is a real testament to an awful lot of hard work, modern technology, | 0:05:09 | 0:05:14 | |
planning, precision on a completely remarkable scale. | 0:05:14 | 0:05:19 | |
With the hunt on for a potential new particle, | 0:05:19 | 0:05:23 | |
Mike and his team are trying to run the LHC | 0:05:23 | 0:05:26 | |
at its highest ever energy, | 0:05:26 | 0:05:28 | |
and it's making their job more challenging than usual. | 0:05:28 | 0:05:32 | |
We had a very interesting month, | 0:05:33 | 0:05:35 | |
with a number of fairly major technical problems, | 0:05:35 | 0:05:38 | |
including the famous weasel, | 0:05:38 | 0:05:40 | |
which took us out for about six days, | 0:05:40 | 0:05:42 | |
but from now on, after this maintenance period, | 0:05:42 | 0:05:45 | |
it's pedal to the metal for two or three months. | 0:05:45 | 0:05:48 | |
To try and find new particles, | 0:05:54 | 0:05:56 | |
the LHC does something that was once completely out of our grasp. | 0:05:56 | 0:06:01 | |
It recreates the conditions that existed just after the Big Bang. | 0:06:03 | 0:06:09 | |
The Big Bang was an explosion that happened | 0:06:10 | 0:06:14 | |
at the beginning of the universe, when all matter was created. | 0:06:14 | 0:06:17 | |
So, this is the year zero, and if we draw a line... | 0:06:17 | 0:06:20 | |
From this point, the universe expanded, | 0:06:20 | 0:06:23 | |
getting cooler, its energy dispersing. | 0:06:23 | 0:06:27 | |
..to where we are in the universe now, where humans exist, | 0:06:27 | 0:06:30 | |
that's 14 billion years. | 0:06:30 | 0:06:32 | |
We know that when the universe was 9 billion years old, | 0:06:34 | 0:06:38 | |
the sun was formed, | 0:06:38 | 0:06:39 | |
and over 8 billion years before that, | 0:06:39 | 0:06:42 | |
the first stars were born, | 0:06:42 | 0:06:45 | |
but the LHC is able to look even further back in time | 0:06:45 | 0:06:49 | |
to when all that existed were the fundamental building blocks | 0:06:49 | 0:06:53 | |
of the universe - particles. | 0:06:53 | 0:06:55 | |
So, in a way, the Large Hadron Collider | 0:06:55 | 0:06:58 | |
is like a time machine, | 0:06:58 | 0:07:00 | |
trying to create the conditions that happened | 0:07:00 | 0:07:03 | |
just in the few millionths of a second after the Big Bang | 0:07:03 | 0:07:06 | |
to see what particles existed when the energy density | 0:07:06 | 0:07:10 | |
of the universe was really, really high. | 0:07:10 | 0:07:13 | |
To do this, the LHC makes use of | 0:07:13 | 0:07:16 | |
one the most famous scientific discoveries ever made. | 0:07:16 | 0:07:20 | |
What we're doing is using the very high energy of the protons | 0:07:22 | 0:07:26 | |
in the collision using Einstein's equation E = mc2... | 0:07:26 | 0:07:32 | |
..which tells us that mass and energy are equivalent, | 0:07:34 | 0:07:39 | |
so we have protons and they're going round and round the LHC, | 0:07:39 | 0:07:43 | |
and we have one set of protons going round this way | 0:07:43 | 0:07:45 | |
and we have another set of protons | 0:07:45 | 0:07:47 | |
which are going around in the opposite direction, | 0:07:47 | 0:07:49 | |
getting faster and faster, closer to the speed of light, | 0:07:49 | 0:07:52 | |
and more and more energetic. | 0:07:52 | 0:07:54 | |
Then we get one proton beam | 0:07:54 | 0:07:56 | |
and the other proton beam | 0:07:56 | 0:07:59 | |
going at the highest energies, | 0:07:59 | 0:08:01 | |
and then we smash them together. | 0:08:01 | 0:08:03 | |
At the moment of collision, | 0:08:06 | 0:08:08 | |
the energy is converted into mass | 0:08:08 | 0:08:10 | |
in the form of thousands of particles. | 0:08:10 | 0:08:12 | |
Although most will be ones we already know about, | 0:08:15 | 0:08:17 | |
the hope is that undiscovered particles might also be created | 0:08:17 | 0:08:22 | |
that could help explain some of the mysteries | 0:08:22 | 0:08:25 | |
of how the universe was formed. | 0:08:25 | 0:08:28 | |
SHE BLOWS | 0:08:33 | 0:08:35 | |
But creating particles is just the beginning. | 0:08:36 | 0:08:40 | |
Detecting them requires | 0:08:41 | 0:08:42 | |
some of the most sophisticated machines in the world. | 0:08:42 | 0:08:46 | |
I come into the cavern hundreds of times in a year | 0:08:46 | 0:08:50 | |
and every time I walk in, | 0:08:50 | 0:08:51 | |
my jaw still drops a little bit when I see ATLAS. | 0:08:51 | 0:08:54 | |
We built this thing. We REALLY built this thing. | 0:08:54 | 0:08:57 | |
Dave Charlton runs the snappily named | 0:08:57 | 0:09:00 | |
A Toroidal Large Hadron Collider Apparatus, known as ATLAS. | 0:09:00 | 0:09:05 | |
It's the largest particle detector on the LHC circuit. | 0:09:05 | 0:09:09 | |
The collisions take place right in the centre of the experiment, | 0:09:09 | 0:09:13 | |
about 30 metres away from where we're standing. | 0:09:13 | 0:09:16 | |
ATLAS has seven different detecting systems | 0:09:16 | 0:09:19 | |
arranged in layers around the collision point. | 0:09:19 | 0:09:22 | |
They're poised to capture evidence of the particles | 0:09:22 | 0:09:25 | |
that have been produced. | 0:09:25 | 0:09:28 | |
Dave hopes that ATLAS will lead the hunt for the potential new particle, | 0:09:29 | 0:09:34 | |
but he's not the only one | 0:09:34 | 0:09:36 | |
with a giant particle detector at his disposal. | 0:09:36 | 0:09:40 | |
There's another massive detector on the LHC circuit - | 0:09:43 | 0:09:47 | |
the Compact Muon Solenoid. | 0:09:47 | 0:09:50 | |
CMS. | 0:09:50 | 0:09:52 | |
It's run by Italian physicist Tiziano Camporesi. | 0:09:54 | 0:09:58 | |
The croissant has become something almost associated to me | 0:10:03 | 0:10:06 | |
because I've grown into the habit of bringing croissants every morning | 0:10:06 | 0:10:10 | |
to the crew which is working at the experiment. | 0:10:10 | 0:10:13 | |
So now, if I show up without croissants, | 0:10:13 | 0:10:15 | |
they are disappointed. | 0:10:15 | 0:10:17 | |
No, actually, I like this... I like this habit. | 0:10:17 | 0:10:21 | |
You know, when you have a ritual, | 0:10:21 | 0:10:23 | |
you don't want to change it because it will bring bad luck. | 0:10:23 | 0:10:27 | |
Tiziano's machine, CMS, is very similar to Dave's. | 0:10:31 | 0:10:35 | |
CMS is big. It's a 14,000-tonne object... | 0:10:36 | 0:10:42 | |
..which basically is five storeys high | 0:10:44 | 0:10:47 | |
and something like 26 metres long. | 0:10:47 | 0:10:50 | |
But ATLAS is slightly bigger. | 0:10:50 | 0:10:52 | |
Look at the size of it. As you can see, | 0:10:52 | 0:10:55 | |
it's really a huge experiment. | 0:10:55 | 0:10:56 | |
25 metres high, 45 metres long. | 0:10:56 | 0:10:58 | |
These detectors are purposefully designed | 0:10:58 | 0:11:02 | |
to do the same thing in two different ways. | 0:11:02 | 0:11:05 | |
You could see it as an oversized camera, | 0:11:07 | 0:11:09 | |
something like a 100-megapixel camera. | 0:11:09 | 0:11:12 | |
Nowadays, a digital camera might be 25 megapixels, 25 million channels, | 0:11:12 | 0:11:16 | |
but we're able to read out our 100 million channels | 0:11:16 | 0:11:20 | |
40 million times a second. | 0:11:20 | 0:11:22 | |
The idea is that new particles | 0:11:24 | 0:11:26 | |
will be seen by both detectors independently. | 0:11:26 | 0:11:29 | |
It can help ensure their findings are valid, | 0:11:29 | 0:11:32 | |
but that doesn't stop both teams | 0:11:32 | 0:11:35 | |
wanting to be first to make a discovery. | 0:11:35 | 0:11:38 | |
We understand that there is some healthy competition | 0:11:39 | 0:11:43 | |
between us and ATLAS, so we are convinced that CMS is better. | 0:11:43 | 0:11:46 | |
HE CHUCKLES | 0:11:46 | 0:11:48 | |
There IS a rivalry between the experiments. | 0:11:48 | 0:11:51 | |
We don't want to lose. | 0:11:51 | 0:11:53 | |
If CMS and ATLAS detect a new particle, | 0:11:59 | 0:12:04 | |
it could be the most important physics discovery in over 100 years. | 0:12:04 | 0:12:09 | |
Ah, you've made it! Come on in. We can talk about some physics. | 0:12:11 | 0:12:15 | |
It's going to be fun. | 0:12:15 | 0:12:17 | |
By the beginning of the 20th century, | 0:12:19 | 0:12:22 | |
particle physicists like Professor Jim Gates | 0:12:22 | 0:12:25 | |
had ascertained that milk, bowls, glasses - | 0:12:25 | 0:12:29 | |
in fact, everything we see around us - | 0:12:29 | 0:12:32 | |
is made from atoms... | 0:12:32 | 0:12:34 | |
..and that atoms themselves are made of even smaller subatomic particles. | 0:12:35 | 0:12:41 | |
From the 1950s, hundreds of particles were discovered... | 0:12:48 | 0:12:52 | |
There was this strange quark - | 0:12:53 | 0:12:57 | |
and this was not the order in which they were discovered - | 0:12:57 | 0:13:00 | |
and then the top quark... | 0:13:00 | 0:13:02 | |
and the most familiar particle of them all, the electron. | 0:13:02 | 0:13:05 | |
All of our electronics come from this. | 0:13:05 | 0:13:08 | |
And so we kept discovering particles - | 0:13:08 | 0:13:10 | |
neutrino, gluon... | 0:13:10 | 0:13:15 | |
But the influx of new particles did little to help explain | 0:13:15 | 0:13:19 | |
how the universe really behaved. | 0:13:19 | 0:13:21 | |
So, this is the state of knowledge about particles | 0:13:22 | 0:13:25 | |
in the 1950s, '60s and '70s. | 0:13:25 | 0:13:27 | |
It was a zoo of particles jumbled about - | 0:13:27 | 0:13:31 | |
confusion, no order. | 0:13:31 | 0:13:33 | |
It was only by studying their characteristics | 0:13:33 | 0:13:36 | |
that physicists could begin to understand | 0:13:36 | 0:13:38 | |
how these particles worked together. | 0:13:38 | 0:13:41 | |
It turned out that the electron, in fact, has another particle | 0:13:42 | 0:13:46 | |
very similar to it called the muon. | 0:13:46 | 0:13:48 | |
This family of particles was called the leptons | 0:13:49 | 0:13:53 | |
and they were soon joined by another - the quarks. | 0:13:53 | 0:13:57 | |
Quarks are really important, | 0:13:57 | 0:13:58 | |
because they are what you need to construct protons and neutrons. | 0:13:58 | 0:14:02 | |
And now, with protons, neutrons and the electron, | 0:14:02 | 0:14:05 | |
you can construct atoms. | 0:14:05 | 0:14:07 | |
From atoms, you can construct cells, molecules, compounds | 0:14:07 | 0:14:13 | |
and, ultimately, us - | 0:14:13 | 0:14:14 | |
so these guys are really, really important. | 0:14:14 | 0:14:17 | |
This group are the known as the fermions - | 0:14:19 | 0:14:22 | |
they're particles that make matter - | 0:14:22 | 0:14:24 | |
but you can't build a universe with fermions alone. | 0:14:24 | 0:14:28 | |
They're held in patterns | 0:14:31 | 0:14:32 | |
and interact through particles known as force carriers. | 0:14:32 | 0:14:36 | |
One of them is the photon, the particle of light. | 0:14:37 | 0:14:40 | |
It is the carrier of the electromagnetic force - | 0:14:40 | 0:14:43 | |
so, we're going to put that up here. | 0:14:43 | 0:14:45 | |
Then there are other forces in nature beside the electromagnetism - | 0:14:45 | 0:14:49 | |
there's a weak nuclear force. | 0:14:49 | 0:14:51 | |
It has carriers - we call them the W and the Z particle. | 0:14:51 | 0:14:56 | |
This family is completed by the gluons | 0:14:58 | 0:15:01 | |
that hold matter together inside an atom, | 0:15:01 | 0:15:04 | |
and the Higgs, responsible for giving the other particles mass. | 0:15:04 | 0:15:10 | |
And now we have the modern Standard Model, | 0:15:12 | 0:15:16 | |
born around 1973, | 0:15:16 | 0:15:18 | |
where the fermions are all sitting here divided into two families | 0:15:18 | 0:15:22 | |
of quarks and leptons, | 0:15:22 | 0:15:24 | |
and these guys are the force carriers. | 0:15:24 | 0:15:26 | |
It is the best-tested, most tested piece of science | 0:15:26 | 0:15:30 | |
that has ever been constructed. | 0:15:30 | 0:15:32 | |
It literally explains tens of thousands of observational facts. | 0:15:32 | 0:15:36 | |
It is just an amazing triumph | 0:15:36 | 0:15:39 | |
that almost nobody has ever heard of, outside of physics. | 0:15:39 | 0:15:42 | |
The Standard Model has served as a map to our understanding | 0:15:43 | 0:15:47 | |
of the particles in the world around us for over 40 years... | 0:15:47 | 0:15:51 | |
..but physicists have hoped, for almost as long, | 0:15:52 | 0:15:56 | |
that it's not the end of the story - | 0:15:56 | 0:15:58 | |
that other particles will also exist | 0:15:58 | 0:16:02 | |
that could help explain | 0:16:02 | 0:16:04 | |
some of the more troublesome mysteries of the universe. | 0:16:04 | 0:16:07 | |
The problem is finding them. | 0:16:09 | 0:16:12 | |
I'm not going to disturb these guys. | 0:16:28 | 0:16:30 | |
These guys are doing serious work! | 0:16:30 | 0:16:32 | |
Fixing the chair, yeah! Fixing the chair! | 0:16:32 | 0:16:34 | |
THEY LAUGH | 0:16:34 | 0:16:36 | |
At CERN, it takes hundreds of researchers | 0:16:36 | 0:16:39 | |
writing millions of lines of computer code | 0:16:39 | 0:16:42 | |
to scour collisions for signs of new particles. | 0:16:42 | 0:16:45 | |
This thing is a raw image, | 0:16:49 | 0:16:51 | |
as they come in, basically unfiltered, | 0:16:51 | 0:16:54 | |
from the collisions which are happening 100 metres below ground, | 0:16:54 | 0:16:59 | |
under our feet. | 0:16:59 | 0:17:01 | |
What makes the job even harder is that undiscovered particles | 0:17:01 | 0:17:05 | |
will only exist at very high energies | 0:17:05 | 0:17:08 | |
like those inside the LHC - | 0:17:08 | 0:17:10 | |
and almost as soon as they're created, they decay | 0:17:10 | 0:17:14 | |
into the stable particles that we're familiar with. | 0:17:14 | 0:17:18 | |
So, I'd like to change this 60... | 0:17:18 | 0:17:20 | |
Let's say... Make it 1, or...? | 0:17:20 | 0:17:23 | |
So the teams aren't looking for the particles themselves, | 0:17:23 | 0:17:26 | |
but for the trails they leave behind. | 0:17:26 | 0:17:30 | |
This is detective work, | 0:17:30 | 0:17:31 | |
because, basically, you are seeing fragments of the disintegration, | 0:17:31 | 0:17:35 | |
you are trying to understand from the behaviour of the fragments | 0:17:35 | 0:17:39 | |
how the particle was to start with. | 0:17:39 | 0:17:41 | |
It's a task for some of the brightest minds in physics | 0:17:41 | 0:17:45 | |
working around the clock. | 0:17:45 | 0:17:46 | |
What we really like is a young brain, I have to tell you! | 0:17:48 | 0:17:51 | |
Because, I mean, these guys are amazing. | 0:17:51 | 0:17:54 | |
I lived through that, I know what it means - | 0:17:54 | 0:17:57 | |
once you become in my position, | 0:17:57 | 0:18:01 | |
the level of stress becomes a different one. | 0:18:01 | 0:18:04 | |
Towards the end of last year, | 0:18:07 | 0:18:09 | |
it looked like all the hard work would pay off. | 0:18:09 | 0:18:12 | |
28-year-old Dr Livia Soffi is an analyst for CMS. | 0:18:19 | 0:18:24 | |
She was once a European artistic roller-skating champion. | 0:18:26 | 0:18:30 | |
I really like to relax, to stay a little bit under the sun | 0:18:33 | 0:18:37 | |
without staying in the office. | 0:18:37 | 0:18:39 | |
I really like the lake, | 0:18:41 | 0:18:43 | |
because when I was younger, I used to go to the sea - | 0:18:43 | 0:18:45 | |
now we cannot go to the sea, | 0:18:45 | 0:18:47 | |
but we have the lake, it is nice, as well. | 0:18:47 | 0:18:50 | |
Then we can take an ice cream - | 0:18:50 | 0:18:52 | |
there is an Italian ice cream place close to here, | 0:18:52 | 0:18:54 | |
so it's very nice. | 0:18:54 | 0:18:55 | |
Last November, Livia found something unexpected in the data | 0:18:57 | 0:19:01 | |
coming from the CMS detector. | 0:19:01 | 0:19:03 | |
What she saw was a mysterious bump on a graph. | 0:19:05 | 0:19:09 | |
So, basically, the idea is that if you do not have anything new, | 0:19:10 | 0:19:15 | |
you will see the dashed line, | 0:19:15 | 0:19:18 | |
and if the solid line, here, the observation, | 0:19:18 | 0:19:23 | |
is inside these two bands, | 0:19:23 | 0:19:26 | |
this means that everything is quiet, | 0:19:26 | 0:19:28 | |
then the fluctuation is not interesting. | 0:19:28 | 0:19:30 | |
When the fluctuation goes outside the bands, | 0:19:30 | 0:19:35 | |
this means that your expectation and what you observe | 0:19:35 | 0:19:38 | |
are not so compatible. | 0:19:38 | 0:19:41 | |
It might not look like much, | 0:19:41 | 0:19:43 | |
but the bump indicates that, | 0:19:43 | 0:19:45 | |
at the energy of 750 giga-electronvolts, | 0:19:45 | 0:19:49 | |
the LHC is producing unexpected bursts of photons. | 0:19:49 | 0:19:54 | |
We have two possibilities. | 0:19:56 | 0:19:58 | |
Either our detector is not working - but this is not the case, | 0:19:58 | 0:20:01 | |
because we know that it is well performing - | 0:20:01 | 0:20:04 | |
or we have observed something. | 0:20:04 | 0:20:07 | |
I have never seen something like this in my life. | 0:20:09 | 0:20:12 | |
This could be evidence of a brand-new particle. | 0:20:12 | 0:20:16 | |
A particle that disappears into a pair of photons | 0:20:18 | 0:20:21 | |
almost as soon as it's created. | 0:20:21 | 0:20:23 | |
And what made the bump even more exciting | 0:20:30 | 0:20:32 | |
was that it wasn't just seen in CMS. | 0:20:32 | 0:20:35 | |
James Beacham is an analyst at the other detector, ATLAS. | 0:20:39 | 0:20:42 | |
To my mind, right here, right now at CERN, in 2016, | 0:20:45 | 0:20:48 | |
is THE most important time and place in the history of science, | 0:20:48 | 0:20:52 | |
because we have just pushed forward, as a species, | 0:20:52 | 0:20:55 | |
into an energy regime where we have never been. | 0:20:55 | 0:20:58 | |
No-one's ever looked here. | 0:20:58 | 0:20:59 | |
APPLAUSE | 0:20:59 | 0:21:01 | |
On the 15th of December, both ATLAS and CMS | 0:21:01 | 0:21:05 | |
presented their findings. | 0:21:05 | 0:21:07 | |
We, of course, observed a little bump at 750 GeV... | 0:21:08 | 0:21:14 | |
It was in this seminar that the science community learnt | 0:21:14 | 0:21:17 | |
that the mysterious bump was being seen | 0:21:17 | 0:21:20 | |
by both the CMS and ATLAS detectors. | 0:21:20 | 0:21:23 | |
It was an extremely exciting seminar that we had here at CERN, | 0:21:23 | 0:21:27 | |
and, to me, watching, you know, | 0:21:27 | 0:21:28 | |
and then, suddenly, he shows this little thing, | 0:21:28 | 0:21:30 | |
and I'm like, "This is very intriguing." | 0:21:30 | 0:21:32 | |
The implications of such a little bump, | 0:21:32 | 0:21:34 | |
if it turns into, potentially, a new particle, are super-huge. | 0:21:34 | 0:21:39 | |
This is completely uncharted territory. | 0:21:39 | 0:21:42 | |
The excitement quickly spread out into the physics world. | 0:21:42 | 0:21:46 | |
Within weeks, 300 papers had been written by theorists | 0:21:46 | 0:21:50 | |
trying to determine what this potential particle might be. | 0:21:50 | 0:21:55 | |
When the result was announced, | 0:21:55 | 0:21:57 | |
the whole theory group was just crazy - | 0:21:57 | 0:22:02 | |
crazy with discussion, | 0:22:02 | 0:22:03 | |
crazy to understand what it was... | 0:22:03 | 0:22:05 | |
Er... That's it! | 0:22:05 | 0:22:07 | |
This was the moment, it seemed. | 0:22:07 | 0:22:11 | |
We started hearing these mysterious noises | 0:22:11 | 0:22:14 | |
about something going on at CERN, | 0:22:14 | 0:22:17 | |
and it had a very prosaic name - the 750 GeV bump. | 0:22:17 | 0:22:22 | |
It sounds like a dance, to me. | 0:22:22 | 0:22:23 | |
I thought it was a joke - but then I began to look more carefully, | 0:22:23 | 0:22:27 | |
thinking that, "Oh, my goodness, this may be | 0:22:27 | 0:22:30 | |
"what I have been spending an entire lifetime waiting for." | 0:22:30 | 0:22:34 | |
By the beginning of this year, | 0:22:40 | 0:22:42 | |
the race was on for ATLAS and CMS to gather more collision data | 0:22:42 | 0:22:46 | |
to see if the mysterious bump would reappear, | 0:22:46 | 0:22:49 | |
or if it was simply a statistical fluctuation. | 0:22:49 | 0:22:52 | |
The fact that the two experiments | 0:22:54 | 0:22:55 | |
seem to see a hint of something in the same place is fascinating, | 0:22:55 | 0:22:59 | |
but the statistics are too low with the current data sample | 0:22:59 | 0:23:01 | |
to get too excited. | 0:23:01 | 0:23:03 | |
It's more potential excitement, at this stage, | 0:23:03 | 0:23:05 | |
for the experimentalists | 0:23:05 | 0:23:07 | |
rather than cast-iron established excitement. | 0:23:07 | 0:23:10 | |
For the bump to be confirmed as a new particle, | 0:23:12 | 0:23:15 | |
the two teams work independently, | 0:23:15 | 0:23:17 | |
both trying to collect enough data | 0:23:17 | 0:23:19 | |
to reach a level of statistical certainty known as 5-sigma. | 0:23:19 | 0:23:23 | |
I mean, to give you a feel for the scale of the statistics | 0:23:25 | 0:23:27 | |
for the Higgs discovery, | 0:23:27 | 0:23:29 | |
we had a few tens of events | 0:23:29 | 0:23:31 | |
that were identified as being signal-like Higgs events, | 0:23:31 | 0:23:34 | |
but we had looked in a million billion events. | 0:23:34 | 0:23:39 | |
So, that's the complexity of the science that we do. | 0:23:39 | 0:23:42 | |
It's really... | 0:23:42 | 0:23:43 | |
I mean, people talk about a needle in a haystack, | 0:23:43 | 0:23:46 | |
but it's a needle in a haystack of haystacks of haystacks! | 0:23:46 | 0:23:48 | |
A grain of sand in an ocean. | 0:23:48 | 0:23:50 | |
It's a huge task, | 0:23:51 | 0:23:53 | |
but with the physics world desperate for news, | 0:23:53 | 0:23:56 | |
the teams have just three months | 0:23:56 | 0:23:57 | |
to announce if they really have found a brand-new particle. | 0:23:57 | 0:24:01 | |
The big thing is our conference in Chicago. | 0:24:02 | 0:24:06 | |
The first week of August. By that time, we should have... | 0:24:06 | 0:24:10 | |
..I think at least doubled the data which we took last year. | 0:24:12 | 0:24:17 | |
As you know... | 0:24:17 | 0:24:18 | |
MUSIC: A Kind of Magic by Queen plays in background | 0:24:18 | 0:24:22 | |
This is specific to our experiment. | 0:24:22 | 0:24:25 | |
You have to realise that the guy who designed our architecture here | 0:24:25 | 0:24:31 | |
for taking data, he is a Queen fan, | 0:24:31 | 0:24:35 | |
so all of the change of states of the machines, | 0:24:35 | 0:24:39 | |
or of the experiments, are basically announced | 0:24:39 | 0:24:42 | |
by a snippet of a Queen song. | 0:24:42 | 0:24:44 | |
Everybody has become aware of the meaning and of the Queen songs! | 0:24:44 | 0:24:50 | |
"It's a kind of magic" means that you have managed to start the run. | 0:24:50 | 0:24:53 | |
The last time particle physicists were this excited, prizes were won. | 0:25:02 | 0:25:07 | |
This is the Nobel medal which I received in 2013. | 0:25:11 | 0:25:16 | |
I think it had something to do with some work I did in... | 0:25:16 | 0:25:22 | |
When was it? 1964. | 0:25:22 | 0:25:25 | |
Make way, please. | 0:25:28 | 0:25:30 | |
On the 4th of July, 2012, | 0:25:32 | 0:25:35 | |
Peter Higgs arrived at CERN for an announcement. | 0:25:35 | 0:25:38 | |
On the day itself, I found myself | 0:25:39 | 0:25:43 | |
being besieged by crowds of physicists | 0:25:43 | 0:25:46 | |
who had more or less camped out overnight | 0:25:46 | 0:25:49 | |
in the hope of getting into the lecture theatre, | 0:25:49 | 0:25:52 | |
which was really already fully booked. | 0:25:52 | 0:25:56 | |
So good morning... | 0:25:57 | 0:25:59 | |
Fabiola Gianotti, who is now Director-General of CERN, | 0:25:59 | 0:26:03 | |
was part of a team from ATLAS. | 0:26:03 | 0:26:05 | |
The atmosphere was absolutely amazing, | 0:26:07 | 0:26:10 | |
it was a big, big emotion. | 0:26:10 | 0:26:12 | |
So you can see here some beautiful events, | 0:26:12 | 0:26:15 | |
selected by our pic search. | 0:26:15 | 0:26:17 | |
We were working days and nights, | 0:26:17 | 0:26:20 | |
nourished and pushed only by adrenaline, | 0:26:20 | 0:26:23 | |
because we didn't have the time to sleep, to eat - it was fantastic. | 0:26:23 | 0:26:27 | |
So this channel has a tiny rate... | 0:26:27 | 0:26:30 | |
At this conference, CMS and ATLAS confirmed that they had found | 0:26:30 | 0:26:34 | |
a particle predicted by Peter nearly half a century earlier. | 0:26:34 | 0:26:40 | |
..extremely clean, except one big spike here, in this hadron here. | 0:26:40 | 0:26:46 | |
An excess, with a local significance of 5.0 sigma, | 0:26:46 | 0:26:50 | |
at a mass of 126.5 GeV - thank you. | 0:26:50 | 0:26:54 | |
It was 48 years from the time that the theory was formulated | 0:27:01 | 0:27:05 | |
as something which might be useful in particle physics, | 0:27:05 | 0:27:09 | |
to the discovery of the particle. | 0:27:09 | 0:27:11 | |
So it was a long wait. | 0:27:11 | 0:27:13 | |
I think we have it. Do you agree? | 0:27:15 | 0:27:18 | |
LAUGHTER AND APPLAUSE | 0:27:18 | 0:27:21 | |
Everybody cheered and got up, it was rather like the end of | 0:27:21 | 0:27:25 | |
a football match, rather than a scientific seminar. | 0:27:25 | 0:27:28 | |
Then I went into hiding again and had some lunch and escaped. | 0:27:34 | 0:27:38 | |
Fly home before anybody else tried to capture me. | 0:27:38 | 0:27:41 | |
The Higgs boson was the final piece needed | 0:27:44 | 0:27:47 | |
to complete the maths of the Standard Model. | 0:27:47 | 0:27:49 | |
But an unpredicted new particle, like the 750 GeV bump, | 0:27:53 | 0:27:57 | |
could be even more significant. | 0:27:57 | 0:27:59 | |
If the bump which has been seen recently is genuine, | 0:28:01 | 0:28:06 | |
that is opening up a new era. | 0:28:06 | 0:28:09 | |
So it's very exciting. | 0:28:09 | 0:28:10 | |
The hope was that if it really is a new particle, | 0:28:14 | 0:28:18 | |
the bump could help physicists answer some of life's big questions. | 0:28:18 | 0:28:23 | |
Like, "How stable is our universe? | 0:28:25 | 0:28:28 | |
"Does it have hidden extra dimensions?" | 0:28:28 | 0:28:31 | |
And an old bugbear - "What is the universe actually made of?" | 0:28:33 | 0:28:38 | |
In the 1930s, evidence emerged that the luminous matter, | 0:28:42 | 0:28:47 | |
the matter which forms the stars, it cannot be sufficient | 0:28:47 | 0:28:52 | |
to justify the dynamics of what we observe in the sky. | 0:28:52 | 0:28:56 | |
There should be something else that gives a gravitational pull. | 0:28:56 | 0:29:00 | |
Physicists faced the rather disturbing realisation that | 0:29:01 | 0:29:06 | |
they don't really know what makes up most of the universe. | 0:29:06 | 0:29:09 | |
So 95% of what is around in our universe | 0:29:12 | 0:29:16 | |
is not the ordinary matter that we are used with, | 0:29:16 | 0:29:20 | |
and that the Standard Model explains. | 0:29:20 | 0:29:23 | |
This is very frustrating for particle physicists, | 0:29:24 | 0:29:27 | |
but particle physicists always look on the bright side, | 0:29:27 | 0:29:31 | |
and they see that there is an opportunity. | 0:29:31 | 0:29:33 | |
This unidentified stuff has been called "dark matter" | 0:29:37 | 0:29:42 | |
and "dark energy". | 0:29:42 | 0:29:44 | |
And the bump could bring us a step closer | 0:29:44 | 0:29:46 | |
to finding out what it actually is. | 0:29:46 | 0:29:48 | |
The 750 GeV particle cannot be the dark matter, | 0:29:55 | 0:29:59 | |
because we know that it decays very quickly into two photons, | 0:29:59 | 0:30:03 | |
meaning that if it were around in the cosmos, it would have | 0:30:03 | 0:30:07 | |
disappeared very quickly, so we know that it cannot be. | 0:30:07 | 0:30:10 | |
However, there has been speculations that the 750 | 0:30:10 | 0:30:14 | |
must be part of a bigger family. | 0:30:14 | 0:30:18 | |
Inside this family, | 0:30:18 | 0:30:19 | |
there could be one particle | 0:30:19 | 0:30:21 | |
that plays the role of the dark matter. | 0:30:21 | 0:30:24 | |
So, even if the 750 is not dark matter, | 0:30:24 | 0:30:27 | |
it could be related to the particle giving rise to the dark matter. | 0:30:27 | 0:30:30 | |
This may have a lot of implications | 0:30:30 | 0:30:32 | |
in understanding the structure of the universe, | 0:30:32 | 0:30:36 | |
understanding how this dark matter was formed | 0:30:36 | 0:30:39 | |
and understanding its role in the universe. | 0:30:39 | 0:30:43 | |
A new particle could well have a profound effect. | 0:30:46 | 0:30:49 | |
But first, they had to find it. | 0:30:50 | 0:30:53 | |
It's the middle of May at CERN. | 0:31:01 | 0:31:03 | |
And with just over two months until the important summer conference, | 0:31:04 | 0:31:08 | |
the mission to gather data continues. | 0:31:08 | 0:31:10 | |
So we are just getting ready to go to work. | 0:31:13 | 0:31:15 | |
My boyfriend is hiding. | 0:31:15 | 0:31:16 | |
SHE LAUGHS | 0:31:16 | 0:31:19 | |
You can come out. | 0:31:19 | 0:31:20 | |
If he wants to. | 0:31:21 | 0:31:23 | |
The LHC has been providing an unprecedented amount of collisions | 0:31:26 | 0:31:30 | |
for the teams on the detectors. | 0:31:30 | 0:31:32 | |
We had the longest fill in the history of the LHC. | 0:31:32 | 0:31:37 | |
And this happened over the weekend, so basically, | 0:31:37 | 0:31:40 | |
starting from Friday and then continuing through Saturday. | 0:31:40 | 0:31:45 | |
Dr Magda Chelstowska is part of the ATLAS team, | 0:31:46 | 0:31:49 | |
and it's her job to clean up and format the data as it's collected. | 0:31:49 | 0:31:53 | |
I think of myself as a person who gives birth to the data. | 0:31:56 | 0:32:01 | |
So I feel that it is my child, it is my kid. | 0:32:01 | 0:32:05 | |
Because I prepare the data and I polish it and massage it | 0:32:05 | 0:32:09 | |
and make it into something which then can go out and be on its own. | 0:32:09 | 0:32:15 | |
The race is on to see which team will be first to gather | 0:32:15 | 0:32:18 | |
enough data to find out if the bump is back. | 0:32:18 | 0:32:21 | |
When we know that we are very close to making | 0:32:21 | 0:32:25 | |
a major breakthrough in physics, | 0:32:25 | 0:32:29 | |
we of course want to do it as soon as possible, | 0:32:29 | 0:32:32 | |
because we don't want the experiment on the other side to beat us to it. | 0:32:32 | 0:32:37 | |
ATLAS and CMS are working blind, accumulating and processing the data | 0:32:40 | 0:32:44 | |
without actually being able to see what it's showing. | 0:32:44 | 0:32:48 | |
It means the two teams can't influence either their own | 0:32:50 | 0:32:53 | |
or the other's results. | 0:32:53 | 0:32:55 | |
THEY CHUCKLE | 0:32:55 | 0:32:57 | |
And with a discovery of this potential significance, for ATLAS, | 0:32:57 | 0:33:00 | |
it is up to Dr Marco Delmastro to make sure nothing is left to chance. | 0:33:00 | 0:33:05 | |
It's always difficult to see whether this excess is a new particle | 0:33:05 | 0:33:10 | |
or not, because nature is behaving in a sort of stochastical way. | 0:33:10 | 0:33:14 | |
We will be spending days and nights, basically, | 0:33:16 | 0:33:19 | |
going through all the stuff, | 0:33:19 | 0:33:21 | |
from the current that we measure inside the detector | 0:33:21 | 0:33:25 | |
to the piece of software that transforms current to energy, | 0:33:25 | 0:33:28 | |
and then tell us where the things are in the detector | 0:33:28 | 0:33:31 | |
and how they are constructed, to the very end. | 0:33:31 | 0:33:34 | |
In the back of my head, there is always a small devil | 0:33:35 | 0:33:38 | |
sitting on my shoulder, saying, | 0:33:38 | 0:33:40 | |
"Are you sure you checked everything? | 0:33:40 | 0:33:42 | |
"Are you sure that there is nothing wrong in what you're doing?" | 0:33:42 | 0:33:46 | |
That is my worry, and still is my worry, so yeah, | 0:33:47 | 0:33:51 | |
I think it is going to stay there for a while. | 0:33:51 | 0:33:54 | |
As the teams crunch the data, | 0:34:03 | 0:34:05 | |
speculation about what the new particle might be is rife. | 0:34:05 | 0:34:10 | |
Jim Gates hopes it could prove a theory known as supersymmetry. | 0:34:13 | 0:34:16 | |
He has been studying this idea for nearly 40 years. | 0:34:19 | 0:34:24 | |
For a long time, the idea of supersymmetry was pooh-poohed. | 0:34:24 | 0:34:27 | |
In fact, I remember all throughout graduate school, | 0:34:27 | 0:34:30 | |
I had colleagues working on other things that were considered | 0:34:30 | 0:34:32 | |
"good physics", and there I was in the corner, | 0:34:32 | 0:34:35 | |
the only student in my team working on this supersymmetrical stuff. | 0:34:35 | 0:34:39 | |
The idea of supersymmetry was born when physicists started | 0:34:41 | 0:34:45 | |
questioning why the Standard Model wasn't mathematically more balanced. | 0:34:45 | 0:34:50 | |
So here is the triumph of the study of the standard models. | 0:34:50 | 0:34:54 | |
And many of us who were studying physics then looked at this, | 0:34:54 | 0:34:57 | |
and we noticed that there is a lack of balance here, a lack of symmetry. | 0:34:57 | 0:35:02 | |
To make this obvious, let me put some lines on the table. | 0:35:02 | 0:35:05 | |
And you can see that there are | 0:35:08 | 0:35:11 | |
two quadrants here that are empty. | 0:35:11 | 0:35:14 | |
Physicists are very sensitive to the lack of symmetry or balance. | 0:35:14 | 0:35:18 | |
And we can ask the question, | 0:35:18 | 0:35:21 | |
"What would the world look like if it were balanced?" | 0:35:21 | 0:35:23 | |
And we ask the question with mathematics. | 0:35:23 | 0:35:26 | |
Supersymmetrists found that the Standard Model | 0:35:27 | 0:35:30 | |
could be given balance if a mirror image | 0:35:30 | 0:35:33 | |
of each of the particles also existed. | 0:35:33 | 0:35:37 | |
They were called "superpartners" or "sparticles". | 0:35:38 | 0:35:42 | |
So if the universe is supersymmetric, | 0:35:45 | 0:35:47 | |
there must be another particle | 0:35:47 | 0:35:49 | |
on this side that we call the selectron. | 0:35:49 | 0:35:52 | |
And also, that has to occur for its neutrino, | 0:35:52 | 0:35:55 | |
which we would call a sneutrino. | 0:35:55 | 0:35:58 | |
For the muon, there's another particle called the smuon. | 0:35:59 | 0:36:02 | |
We physicists, when we make great triumphs, are so happy | 0:36:04 | 0:36:08 | |
that we get giddy, so we name things in a silly manner. | 0:36:08 | 0:36:12 | |
The idea is deceptively simple. | 0:36:12 | 0:36:15 | |
Each ordinary matter particle | 0:36:15 | 0:36:17 | |
has an undiscovered supersymmetric force partner. | 0:36:17 | 0:36:21 | |
And each force particle, | 0:36:21 | 0:36:23 | |
an undiscovered supersymmetric matter partner. | 0:36:23 | 0:36:27 | |
Once we've made this change we are looking at | 0:36:29 | 0:36:32 | |
not the Standard Model but a supersymmetric extension | 0:36:32 | 0:36:36 | |
of the Standard Model, where we get a balance on both sides - | 0:36:36 | 0:36:40 | |
there's a balance of the superpartners | 0:36:40 | 0:36:42 | |
to the ordinary matter... | 0:36:42 | 0:36:44 | |
There's a balance for the super force carriers | 0:36:44 | 0:36:46 | |
to the ordinary force carriers. | 0:36:46 | 0:36:49 | |
And this is what we've been wondering about for | 0:36:49 | 0:36:51 | |
over 30 years - | 0:36:51 | 0:36:53 | |
is it just mass or is it the universe we look at? | 0:36:53 | 0:36:56 | |
Devotees of supersymmetry believe that their theory solves | 0:36:58 | 0:37:02 | |
one of the most worrying mysteries of our universe. | 0:37:02 | 0:37:05 | |
At the smallest scales, the universe is in a constant state of flux... | 0:37:07 | 0:37:13 | |
seething with particles popping in and out of existence. | 0:37:13 | 0:37:17 | |
The best way to understand it is to try to understand | 0:37:19 | 0:37:22 | |
something about what's going on inside of a teapot. | 0:37:22 | 0:37:25 | |
We can see the water is boiling, there's bubbles coming out, | 0:37:25 | 0:37:28 | |
some are big, they explode, they disappear. | 0:37:28 | 0:37:30 | |
So if you imagine that this surface is the universe, | 0:37:30 | 0:37:33 | |
the bubbles popping in and out are actually virtual particles, | 0:37:33 | 0:37:36 | |
they're virtual electrons and photons - | 0:37:36 | 0:37:38 | |
all the particles that make up our universe, | 0:37:38 | 0:37:40 | |
they pop into existence and then they disappear. | 0:37:40 | 0:37:43 | |
This state of chaos is known as the quantum vacuum. | 0:37:48 | 0:37:52 | |
And Jim thinks that without supersymmetry, | 0:37:53 | 0:37:57 | |
it might make the universe unstable. | 0:37:57 | 0:37:59 | |
I'm going to use a set of quarters to represent our universe. | 0:38:02 | 0:38:05 | |
And...with a little bit of work I can get it to balance. | 0:38:07 | 0:38:10 | |
With the particles of the Standard Model, there's actually | 0:38:10 | 0:38:13 | |
a preponderance of one type of particle over the other. | 0:38:13 | 0:38:16 | |
And now let's follow what happens | 0:38:16 | 0:38:19 | |
if you let this preponderance work for a while. | 0:38:19 | 0:38:23 | |
It's as if you are pressing on the stack of coins, | 0:38:23 | 0:38:25 | |
but because of the preponderance | 0:38:25 | 0:38:27 | |
you are always pressing in one direction. | 0:38:27 | 0:38:29 | |
And what you find is that we are very close to being | 0:38:29 | 0:38:32 | |
in a situation where the universe might collapse. | 0:38:32 | 0:38:35 | |
Now, supersymmetry can help solve this problem. | 0:38:37 | 0:38:40 | |
So, if you have particles - all the ones we know about, | 0:38:44 | 0:38:47 | |
as well as the sparticles - they press, but they press | 0:38:47 | 0:38:51 | |
in opposite directions. | 0:38:51 | 0:38:53 | |
And our universe is a much more stable place. | 0:38:53 | 0:38:57 | |
And I know I would sleep much more quietly at night | 0:38:57 | 0:39:00 | |
knowing I live in a stable universe. | 0:39:00 | 0:39:02 | |
The problem is that in 30 years of research... | 0:39:06 | 0:39:10 | |
no sparticle has ever been found. | 0:39:10 | 0:39:12 | |
But is that finally about to change? | 0:39:13 | 0:39:15 | |
The 750 GeV bump might actually be one of these particles | 0:39:17 | 0:39:22 | |
that we've predicted by the mathematics of supersymmetry. | 0:39:22 | 0:39:25 | |
And if that's the case, it becomes the herald for supersymmetry. | 0:39:25 | 0:39:29 | |
For me it will mean several things. Emotionally it will be a great high. | 0:39:29 | 0:39:33 | |
I have been a supporter of the idea of supersymmetry | 0:39:33 | 0:39:36 | |
since I was 25 years old, first learning theoretical physics. | 0:39:36 | 0:39:41 | |
The dream was to find a magical piece of mathematics. | 0:39:42 | 0:39:47 | |
Simultaneously, an accurate description of something in nature. | 0:39:47 | 0:39:51 | |
It will be a source of intense joy. | 0:39:51 | 0:39:53 | |
With the hopes of theoretical physicists around the world | 0:40:14 | 0:40:17 | |
at stake, the pressure is on the LHC to keep providing collisions. | 0:40:17 | 0:40:23 | |
But running this machine at such high energy... | 0:40:24 | 0:40:27 | |
..is putting a huge strain on all its systems. | 0:40:28 | 0:40:31 | |
When it's running well, it runs well, | 0:40:34 | 0:40:37 | |
but there are a lot of things that can go wrong and do go wrong. | 0:40:37 | 0:40:40 | |
So it can get quite stressful. | 0:40:40 | 0:40:42 | |
Today, one of the accelerators that provides the LHC with protons, | 0:40:44 | 0:40:48 | |
the Proton Synchrotron - or PS - | 0:40:48 | 0:40:52 | |
has broken down. | 0:40:52 | 0:40:54 | |
This is one of the veritable workhorses of CERN, | 0:40:54 | 0:40:56 | |
and really is like the beating heart of the complex, | 0:40:56 | 0:41:01 | |
and at the moment the line is flat. | 0:41:01 | 0:41:03 | |
So we are in some of the oldest parts of CERN here. | 0:41:05 | 0:41:09 | |
The PS has been with us since 1959, | 0:41:09 | 0:41:11 | |
so there's some really old kit around here. | 0:41:11 | 0:41:14 | |
And...this beast here is what we call the rotating machine, | 0:41:19 | 0:41:23 | |
if you like, it's a kind of temporary energy storage system | 0:41:23 | 0:41:26 | |
which we use to power and de-power the PS machine, | 0:41:26 | 0:41:31 | |
the main bending magnets of the PS. | 0:41:31 | 0:41:33 | |
It was retired a few years ago, it was pressed back into service | 0:41:33 | 0:41:38 | |
because we've had a problem with the new version. | 0:41:38 | 0:41:41 | |
Unfortunately, last week a problem developed on this - | 0:41:41 | 0:41:45 | |
there was a short-circuit on a circuit breaker | 0:41:45 | 0:41:48 | |
developed downstairs, which arced and damaged the circuit breaker | 0:41:48 | 0:41:53 | |
and some nearby equipment. | 0:41:53 | 0:41:55 | |
Thanks to the failure of this near-50-year-old power supply, | 0:41:58 | 0:42:02 | |
the world's most expensive science experiment is just an empty pipe. | 0:42:02 | 0:42:07 | |
There's a huge experimental community on the LHC out there | 0:42:10 | 0:42:13 | |
really looking forward to getting as much data as they can this year. | 0:42:13 | 0:42:16 | |
And of course, there's a lot of pressure to get the complex | 0:42:16 | 0:42:18 | |
back up and running properly. | 0:42:18 | 0:42:20 | |
I still can't believe it says 1967 on there, actually. | 0:42:21 | 0:42:25 | |
If the LHC isn't running again soon, the worry for the experimentalists | 0:42:27 | 0:42:32 | |
is that they won't be ready for the August conference. | 0:42:32 | 0:42:35 | |
Another day that it's not coming in, | 0:42:36 | 0:42:38 | |
it's a bit frustrating. I like to wake up in the morning | 0:42:38 | 0:42:41 | |
to see how much data we took... | 0:42:41 | 0:42:43 | |
..overnight. But lately I haven't had any good mornings! | 0:42:45 | 0:42:49 | |
In the very beginning, there was a loss of 1.7 inverse picobarns | 0:42:53 | 0:42:57 | |
because of a problem. And then at the end of the run... | 0:42:57 | 0:43:00 | |
But the teams are determined to find a way around the problem. | 0:43:00 | 0:43:04 | |
So, we are considering suppressing our technical stops. | 0:43:05 | 0:43:11 | |
Which basically will put us on track for our goals of achieving | 0:43:11 | 0:43:18 | |
basically something like three times the statistics | 0:43:18 | 0:43:22 | |
which we have accumulated last year... | 0:43:22 | 0:43:25 | |
in time for the summer conference in Chicago. | 0:43:25 | 0:43:29 | |
At the University of Maryland near Washington, DC, | 0:43:41 | 0:43:45 | |
Professor Raman Sundrum has great expectations | 0:43:45 | 0:43:48 | |
about what the bump might be. | 0:43:48 | 0:43:50 | |
His hope is that it could be | 0:43:52 | 0:43:53 | |
a hypothetical particle that has near mythical status. | 0:43:53 | 0:43:57 | |
A force carrier particle of gravity - | 0:44:00 | 0:44:04 | |
known as an extra-dimensional graviton. | 0:44:04 | 0:44:07 | |
The discovery of a graviton could help solve a puzzle | 0:44:09 | 0:44:13 | |
that has baffled physicists for a long, long time. | 0:44:13 | 0:44:17 | |
Gravity seems strong, it seems like it's the first force that, | 0:44:17 | 0:44:20 | |
you know, cavemen would have known about, right? | 0:44:20 | 0:44:23 | |
It's the thing that dominates most of our lives, | 0:44:23 | 0:44:25 | |
just being pulled down to the Earth. | 0:44:25 | 0:44:27 | |
But we can sort of see why physicists | 0:44:27 | 0:44:29 | |
think that gravity is in fact the weakest force. | 0:44:29 | 0:44:32 | |
And a quick way to demonstrate that is to just take a simple object, | 0:44:32 | 0:44:35 | |
like a paperclip. | 0:44:35 | 0:44:37 | |
Watch gravity act on it. | 0:44:37 | 0:44:38 | |
But we can act on this paperclip with this magnet, | 0:44:39 | 0:44:43 | |
which seems much smaller, and perhaps much weaker than the Earth. | 0:44:43 | 0:44:47 | |
The entire gravitational pull of the planet can be easily overcome... | 0:44:48 | 0:44:53 | |
..with just a small magnet. | 0:44:55 | 0:44:56 | |
If you work this out you actually find that electromagnetism is | 0:44:58 | 0:45:02 | |
by far and away stronger than the force of gravity. | 0:45:02 | 0:45:07 | |
It's basically one followed by about 30 zeros times stronger than | 0:45:07 | 0:45:11 | |
the force of gravity. | 0:45:11 | 0:45:14 | |
That's how weak gravity is to a physicist. | 0:45:14 | 0:45:16 | |
Raman believes there is one mind-blowing way | 0:45:18 | 0:45:20 | |
to explain this puzzle - | 0:45:20 | 0:45:23 | |
the existence of a tiny, invisible extra dimension in our universe. | 0:45:23 | 0:45:29 | |
We're used to living in three dimensions of space - | 0:45:31 | 0:45:34 | |
we can travel forwards and backwards, left and right, | 0:45:34 | 0:45:37 | |
and up and down. | 0:45:37 | 0:45:39 | |
If you just look at the vast expanse of the grass, | 0:45:39 | 0:45:42 | |
it looks fairly flat, | 0:45:42 | 0:45:44 | |
and so you'd say, effectively, for my purposes, it's two-dimensional. | 0:45:44 | 0:45:48 | |
But if you're small, you can go places humans can't. | 0:45:49 | 0:45:53 | |
And the grass looks rather different. | 0:45:55 | 0:45:57 | |
From the bug's point of view, the grass | 0:45:59 | 0:46:00 | |
does not look that two-dimensional. Doesn't look that flat. | 0:46:00 | 0:46:04 | |
If it really gets in there, it can go up and down these clovers, | 0:46:04 | 0:46:07 | |
or up and down a blade of grass, | 0:46:07 | 0:46:09 | |
so it's really in there with the third dimension, | 0:46:09 | 0:46:12 | |
the vertical dimension. | 0:46:12 | 0:46:13 | |
The grass looks 2D to humans because we're so big, | 0:46:13 | 0:46:17 | |
and perhaps the same applies to our apparently 3D universe. | 0:46:17 | 0:46:21 | |
It might be that for human-size creatures like us, | 0:46:23 | 0:46:26 | |
we live in something that looks effectively three-dimensional. | 0:46:26 | 0:46:30 | |
And yet, there's another dimension - | 0:46:30 | 0:46:32 | |
a very small dimension that's sort of hidden to the naked eye. | 0:46:32 | 0:46:35 | |
But if you are a microscopic, subatomic particle, | 0:46:35 | 0:46:39 | |
you might be a little bit like that bug. | 0:46:39 | 0:46:41 | |
If an invisible extra dimension exists, it could mean | 0:46:42 | 0:46:46 | |
that gravity appears weak because we're only seeing | 0:46:46 | 0:46:49 | |
part of its strength. The rest is hidden - in the extra dimension. | 0:46:49 | 0:46:54 | |
And the discovery of a graviton in the LHC | 0:46:56 | 0:47:00 | |
could help prove this extraordinary theory. | 0:47:00 | 0:47:02 | |
That's part of what the LHC is doing when it collides protons. | 0:47:06 | 0:47:09 | |
The collision is incredibly energetic and that energy provides | 0:47:09 | 0:47:14 | |
the kind of quantum mechanical magnifying glass for these particles | 0:47:14 | 0:47:20 | |
to look inside the extra dimension and report back in an indirect way. | 0:47:20 | 0:47:24 | |
If it is a graviton, then that has very great significance. | 0:47:25 | 0:47:30 | |
It's the middle of June at CERN. | 0:47:40 | 0:47:43 | |
For the last four weeks, the LHC has been running so well | 0:47:43 | 0:47:47 | |
that the team from ATLAS have finally gathered enough data | 0:47:47 | 0:47:51 | |
to see if the bump is back. | 0:47:51 | 0:47:53 | |
The machine has been working over the clock and produced | 0:47:56 | 0:47:59 | |
a lot of collisions and now we have almost as much data as we got | 0:47:59 | 0:48:04 | |
in 2015, so it's kind of exciting times because the day has arrived | 0:48:04 | 0:48:10 | |
to look at this data and to see if there's something there or not. | 0:48:10 | 0:48:15 | |
I am VERY optimistic! | 0:48:15 | 0:48:17 | |
Well, last time, I was actually quite pessimistic | 0:48:17 | 0:48:21 | |
cos I didn't think that we would get enough data at this point, | 0:48:21 | 0:48:25 | |
so now my optimism is going up and up with each day! | 0:48:25 | 0:48:30 | |
My gut feeling - I... | 0:48:30 | 0:48:33 | |
Oh, I'm really oscillating, I would say, and, erm... | 0:48:33 | 0:48:38 | |
Yeah, I still hope there is something there. | 0:48:38 | 0:48:43 | |
The results will be revealed in an ATLAS team meeting. | 0:48:47 | 0:48:51 | |
You have to stay outside. | 0:48:52 | 0:48:55 | |
The secrecy is because ATLAS have beaten CMS to it | 0:49:04 | 0:49:08 | |
and they don't want them to know their conclusions. | 0:49:08 | 0:49:11 | |
An hour later, Marco and the team are out. The results are clear. | 0:49:17 | 0:49:22 | |
750 is here, so you will expect to see a bump somewhere here. | 0:49:24 | 0:49:29 | |
The data is the data, so unless we made | 0:49:29 | 0:49:31 | |
a very bad mistake in processing the data, | 0:49:31 | 0:49:35 | |
you can see by eye that there is no evident excess there. | 0:49:35 | 0:49:39 | |
It's very flat. There is no bump there. | 0:49:39 | 0:49:42 | |
Data that we have looked at from this year, | 0:49:45 | 0:49:48 | |
we haven't seen anything yet, which is a bit disappointing, | 0:49:48 | 0:49:51 | |
to be honest, but that's actually how most of our searches turn out. | 0:49:51 | 0:49:57 | |
We don't allow ourselves to hope, but, of course, | 0:49:57 | 0:50:00 | |
we are humans and we were probably | 0:50:00 | 0:50:02 | |
unconsciously hoping for something more and we're not seeing it. | 0:50:02 | 0:50:07 | |
It might simply mean there was a fluctuation | 0:50:07 | 0:50:10 | |
of the background noise in 2015 that has gone away, | 0:50:10 | 0:50:13 | |
so it's a bit disappointing, honestly, | 0:50:13 | 0:50:16 | |
and, of course, we are not in the position | 0:50:16 | 0:50:19 | |
to draw a definitive conclusion, | 0:50:19 | 0:50:21 | |
but, yeah, it could have been a more exciting day. | 0:50:21 | 0:50:25 | |
The only hope for the bump | 0:50:26 | 0:50:28 | |
is that it's been found by the other team, CMS. | 0:50:28 | 0:50:32 | |
They don't know about the ATLAS results and, three days later, | 0:50:34 | 0:50:39 | |
they're ready to look at their data. | 0:50:39 | 0:50:42 | |
I am very excited. | 0:50:44 | 0:50:47 | |
At least in my life, working life, | 0:50:47 | 0:50:49 | |
it's the most exciting moment. | 0:50:49 | 0:50:51 | |
So now we're going to open the reports. | 0:50:57 | 0:51:01 | |
And there's nothing. | 0:51:02 | 0:51:05 | |
So, no bump. | 0:51:06 | 0:51:08 | |
Nothing is there. | 0:51:10 | 0:51:11 | |
We just see something that is compatible with the expectations. | 0:51:11 | 0:51:16 | |
There was just... There have been many times in the past. | 0:51:17 | 0:51:20 | |
It will happen in the future. | 0:51:20 | 0:51:22 | |
Too bad. Of course, you are hopeful that somebody finds something | 0:51:22 | 0:51:25 | |
cos that's basically why we do the job, | 0:51:25 | 0:51:28 | |
but it basically tells everybody now that we don't need to be excited | 0:51:28 | 0:51:32 | |
because the fluctuation we saw for the moment is gone | 0:51:32 | 0:51:36 | |
and now we have to wait for the rest of the data. | 0:51:36 | 0:51:41 | |
So, I'm looking at it and, er... | 0:51:43 | 0:51:47 | |
And... | 0:51:49 | 0:51:51 | |
there is nothing. | 0:51:51 | 0:51:54 | |
The results are shared with the rest of the team at the weekly meeting. | 0:51:57 | 0:52:01 | |
Can you hear me? | 0:52:04 | 0:52:06 | |
The 750 bump now doesn't look very healthy, put it like this. | 0:52:07 | 0:52:14 | |
So, I'm going to report on the status of the analysis. | 0:52:14 | 0:52:21 | |
I would give it 95% probability that it was fluctuation | 0:52:23 | 0:52:30 | |
and in fact we always said that and we tried to keep very cool about it. | 0:52:30 | 0:52:35 | |
Obviously, I would have preferred that nature had surprised us | 0:52:35 | 0:52:40 | |
because it was a real surprise, this 750 thing. | 0:52:40 | 0:52:44 | |
On the other hand, if this thing had been real, it would have really | 0:52:44 | 0:52:47 | |
meant a complete change of the way we interpret nature, | 0:52:47 | 0:52:53 | |
so it has always been in the back of my mind | 0:52:53 | 0:52:56 | |
that this thing could be a fluctuation. | 0:52:56 | 0:53:00 | |
We got permission to look at data over the weekend | 0:53:00 | 0:53:04 | |
and now if we look at data, | 0:53:04 | 0:53:05 | |
what we can see is the observed 750 is not confirmed. | 0:53:05 | 0:53:11 | |
But in the next months, we'll get four times more statistics | 0:53:11 | 0:53:14 | |
so by that time, one will be able to tell for sure. | 0:53:14 | 0:53:19 | |
It's the 5th of August. | 0:53:48 | 0:53:50 | |
Tiziano and Dave are in Chicago for the conference. | 0:53:50 | 0:53:54 | |
The time has come for them to share the results of their hunt | 0:54:02 | 0:54:05 | |
for the 750 GEV bump with the rest of the physics world. | 0:54:05 | 0:54:10 | |
It's a great pleasure to be here today to talk about the first half | 0:54:15 | 0:54:18 | |
of the highlights from the LHC and the way we've organised this... | 0:54:18 | 0:54:22 | |
Further data has confirmed what the teams feared. | 0:54:22 | 0:54:25 | |
But then, as you will have heard, | 0:54:25 | 0:54:27 | |
we were looking at the 2016 data | 0:54:27 | 0:54:29 | |
and I'm afraid to say in the 2016 data, | 0:54:29 | 0:54:31 | |
there is no clustering around the 730-750 GEV region | 0:54:31 | 0:54:36 | |
and so there's about four times more data and so, from this, | 0:54:36 | 0:54:39 | |
we have to conclude that the 2015 excess | 0:54:39 | 0:54:41 | |
was most likely a statistical fluctuation. | 0:54:41 | 0:54:44 | |
The dream of the 750 GEV bump is over. | 0:54:44 | 0:54:48 | |
It would have been a revolution. | 0:54:50 | 0:54:51 | |
Yep, we would have broken the Standard Model of particle physics. | 0:54:51 | 0:54:55 | |
It would have sent a lot of theories back to the drawing board. | 0:54:55 | 0:54:59 | |
The bump was just a fluctuation in the data. | 0:55:01 | 0:55:05 | |
That it was seen by both detectors was a highly unlikely coincidence. | 0:55:05 | 0:55:10 | |
The bump was a cruel statistical fluke. | 0:55:10 | 0:55:14 | |
It's simply the kind of thing which can happen because basically | 0:55:14 | 0:55:20 | |
when we're dealing with statistics, it's like, | 0:55:20 | 0:55:22 | |
you know, flipping a coin five to ten times, | 0:55:22 | 0:55:26 | |
you can always get heads. | 0:55:26 | 0:55:27 | |
And the disappointing news | 0:55:29 | 0:55:31 | |
quickly reaches the rest of the physics world. | 0:55:31 | 0:55:34 | |
We'd have vastly preferred that it WAS there because it would have | 0:55:36 | 0:55:40 | |
definitely heralded a much richer particle physics | 0:55:40 | 0:55:44 | |
that would play out, guaranteed, in the next few years. | 0:55:44 | 0:55:47 | |
Scientists are human and so we have feelings just like everyone else. | 0:55:47 | 0:55:51 | |
I guess, in my case, I would say disappointment | 0:55:51 | 0:55:54 | |
but not discouragement, and so we have to look a little bit harder. | 0:55:54 | 0:55:58 | |
The 750 GEV bump didn't live up to anyone's hopes. | 0:56:01 | 0:56:05 | |
But the quest to understand the mysteries | 0:56:08 | 0:56:11 | |
of the particle world are far from over. | 0:56:11 | 0:56:13 | |
Back at CERN, the hunt for particles goes on | 0:56:18 | 0:56:21 | |
and they're certainly not giving up. | 0:56:21 | 0:56:24 | |
We are clever beings. | 0:56:27 | 0:56:29 | |
Human beings are clever beings, so our intrinsic wish | 0:56:29 | 0:56:34 | |
and our intrinsic duty and right | 0:56:34 | 0:56:36 | |
is really to be intelligent, clever beings. | 0:56:36 | 0:56:40 | |
Today, the LHC is operating at the highest capacity it's ever achieved. | 0:56:40 | 0:56:46 | |
The machine is performing exceptionally well at the moment. | 0:56:48 | 0:56:52 | |
We really are somewhere where we didn't expect to be. | 0:56:52 | 0:56:55 | |
Things aren't breaking down very often and we're sitting there | 0:56:55 | 0:56:58 | |
for 24 hours at a time with stable beams continually producing | 0:56:58 | 0:57:03 | |
these high rates of collisions to the experiments | 0:57:03 | 0:57:06 | |
and nothing's going wrong. | 0:57:06 | 0:57:08 | |
These bottles have come from ATLAS and CMS. We had a small celebration. | 0:57:08 | 0:57:12 | |
We actually reached design luminosity a couple of weeks ago. | 0:57:12 | 0:57:15 | |
This was actually a quite profound achievement for the LHC. | 0:57:15 | 0:57:19 | |
The Large Hadron Collider is the most ambitious | 0:57:19 | 0:57:22 | |
scientific experiment ever undertaken. | 0:57:22 | 0:57:25 | |
For now, it's holding on to its secrets, | 0:57:25 | 0:57:28 | |
but the teams working there | 0:57:28 | 0:57:30 | |
still hope that they will be the ones to unlock them. | 0:57:30 | 0:57:34 | |
One day. Oh, there's a huge amount more in the LHC. | 0:57:34 | 0:57:38 | |
We've barely started the journey at this point, clearly. | 0:57:38 | 0:57:41 | |
We have another 20 years of data-taking | 0:57:41 | 0:57:44 | |
and we will have huge, huge data samples | 0:57:44 | 0:57:47 | |
and lots of sensitivity to new particles if they're there. | 0:57:47 | 0:57:51 | |
I'm excited about the future. | 0:57:51 | 0:57:53 | |
The one thing where I would not be ready to bet | 0:57:53 | 0:57:56 | |
is whether the discovery's going to happen in the next six months, | 0:57:56 | 0:57:59 | |
the next three years or the next ten years. | 0:57:59 | 0:58:02 | |
It all depends on how kind nature is going to be with us. | 0:58:02 | 0:58:06 |