NARRATOR: They built the largest, most complex machine in history,
to probe the deepest mysteries of the early universe,
as it was at the beginning of time.
MAN: The Large Hadron Collider is allowing us to see right back
to ten to the minus 12 seconds after the Big Bang.
NARRATOR: Within two massive detectors,
in conditions harsher even than outer space,
tiny particles smash together at nearly the speed of light...
unleashing incredible energy.
MAN: Trying to figure out
what happens in the collision of two protons at very high energy
is like analyzing what happens
in the high-speed collision of two garbage trucks.
NARRATOR: Within that spray of debris, physicists search
for a tiny bundle of energy, a subatomic particle...
proof of an invisible energy field that fills all of space.
It just may be
the most important feature of our universe.
Without it...
There are no atoms,
there's no chemistry, there's no life.
NARRATOR: 50 years of effort, $10 billion,
and thousands of researchers around the world.
For them, the stakes have never been higher.
MAN: It's practically
my whole professional life that's led to this point.
NARRATOR: It's the moment of truth when science flips the switch
on the Big Bang Machine.
MAN: One, zero...
NARRATOR: Right now, on NOVA.
Major funding for NOVA is provided by the following:
Supporting NOVA and promoting public understanding of science.
And by the Corporation for Public Broadcasting.
And by contributions to your PBS station from:
Additional funding is provided by Millicent Bell through:
One of the world's most-wanted fugitives
has finally been captured.
Done!
NARRATOR: The announcement came
at the end of a high-speed, high-stakes chase.
A mystery.
300 people were hot on the trail.
Decades worth of work.
NARRATOR: It was a truly international effort
that drew to its dramatic conclusion here.
MAN: It's a historic milestone today.
NARRATOR: On the border of France and Switzerland,
300 feet below ground.
But this wasn't a search for some outlaw
or criminal mastermind.
It was a hunt for something far more elusive...
An unstable bundle of energy far smaller than an atom
that winks out of existence
in a trillion trillionth of a second.
It's evidence of a force that fills all of space,
completely invisible, and yet without it,
life, earth, the universe we know could not exist.
Finding this elusive particle marks the end of a quest
that required constructing the largest, most complex machine
the world has ever seen.
A quest that consumed nearly half a century,
billions of dollars,
and asked thousands of scientists across the globe
to invest years, even decades of their careers
with no guarantee of success.
I got a job to do this in 1993.
It's eleventh year now.
About ten years, me.
Yeah, and about five years for me.
20 years, something like that.
Since 1994, I guess.
It's practically my whole professional life
that's led to this point.
NARRATOR: The discovery has been hailed
as one of the greatest scientific victories of all time
and has already won the Nobel Prize.
It's an enormous triumph.
This was my generation's Manhattan Project,
and I wanted to be on the inside looking out.
It's been extremely exciting.
NARRATOR: But what is this mysterious quarry?
What does it actually do?
And why was finding it so important?
That story begins at the very beginning of time,
when the universe came into being in a massive explosion
called the Big Bang.
So here we have the Big Bang.
NARRATOR: Billions of years ago.
Deserves a little bit of color, I think.
And then the timeline of the universe.
This is where we are.
This now the age of the universe,
like 13.7 billion years after the Big Bang.
And so working backwards, we had the dinosaurs.
So here's a dinosaur.
Then life itself, first DNA was about four billion years ago.
NARRATOR: Before DNA, there was the earth.
Before that, the first stars.
Before them, just atoms.
While atoms were once thought to consist
of just three basic particles--
neutrons, protons and electrons--
physicists now know some of these are made
of even more fundamental stuff--
the basic building blocks of our universe.
JON BUTTERWORTH: The big question then is
where did those building blocks come from?
The answer to all that lies in the first second.
NARRATOR: In the first instant of existence,
when the universe was unimaginably hot,
the cosmos was filled with identical bundles of energy
moving at the speed of light,
all indistinguishable from one another.
But then something changed.
Distinct types of particles emerged
with different properties, like electric charge...
and mass, what we experience as weight.
Now we live in a universe full of tangible stuff.
And while that monumental shift from nothing to something
must have happened almost immediately,
how it happened
was one of the biggest unanswered questions in physics.
The mysteries of existence lie within this second.
Certainly we understand the science,
we understand the physics.
Work backwards into this second,
but at some point we just run out of knowledge.
And the Large Hadron Collider is allowing us to see
right back to ten to the minus 12 seconds after the Big Bang.
Beyond that, here be dragons or dinosaurs.
(laughs)
NARRATOR: The Large Hadron Collider is a massive particle accelerator,
the largest machine in the world,
designed to simulate the universe as it was
a trillionth of a second after the Big Bang.
To solve the mystery of mass, it smashes protons together
at energy so high...
that it is capable of testing an idea first suggested in 1964
by several scientists around the world,
including a young theoretical physicist named Peter Higgs.
His mathematics suggestethat right after the Big Bang,
an invisible energy field was somehow switched on
and now fills the entire universe.
Just the way that a magnetic field affects some materials
but not others, he suggested that this new field
selectively affects some fundamental particles,
causing some of them to take on mass.
Very massive particles
like the quarks that make up protons and neutrons
interact strongly with this field.
Electrons, which form the outer shells of atoms,
interact less strongly and are very lightweight.
And still others, like photons, particles of light,
have no mass, because they don't interact with the field at all.
The theory implied that a universe without a Higgs field
might not be a very friendly place.
And that got people's attention.
If there were no Higgs mechanism,
elementary particles wouldn't have mass.
If electrons didn't have mass,
that means they would move at the speed of light.
And if electrons moved at the speed of light,
electrons do not settle down into atoms.
And if electrons do not settle down into atoms,
there e no atoms, there are no molecules,
there's no chemistry, there's no life.
Nothing.
It would look nothing like what we see today.
We wouldn't be here,
and there would be no physicists to ask these questions.
NARRATOR: When Higgs submitted his theory to a journal,
the editors based at CERN rejected it.
HIGGS: My reaction was
that they clearly hadn't understood what I was saying.
NARRATOR: Undeterred, he revised the paper,
adding a paragraph saying, in effect,
that if the field exists, we should find evidence of it
in the form of a particle that would turn up in an accelerator.
In other words, if you smash particles together
energetically, you'll make a ripple in the field.
And if you apply enough energy,
you just might be able to detect it in the form of a particle.
The second time around,
an American journal published the paper
and Peter Higgs got a lot of credit.
But in reality, the idea was cooked up independently
by a bunch of scientists:
Philip Anderson, Robert Brout, François Englert,
Gerry Guralnik, Carl R. Hagen,
Peter Higgs, Tom Kibble, Gerard 't Hooft.
Some have suggested that it really should be called this.
But since that's impossible to pronounce,
it's simply called the Higgs field.
Gradually, the theory gained support,
but without the evidence of a particle,
now called the Higgs boson, it remained unproven.
To be honest, we weren't sure that the Higgs existed.
Mr. Higgs and his collaborators were saying that there was
an invisible energy field everywhere in the universe.
So the "invisible" sounds a little odd,
and the "everywhere in the universe" also sounds
kind of far-fetched.
So that was a lot for people to swallow.
There were many people who thought
this can't be the answer.
I've heard people describe it as a trick,
a mathematical trick to make the equations work out.
NARRATOR: Finding something that's all around us
is surprisingly tricky.
Because the Higgs boson doesn't actually exist.
At least not in any form that we can easily detect.
So in 1998, scientists from around the world came together
at CERN, the Center for European Nuclear Research,
located on the border of France and Switzerland,
to build a particle accelerator that would have enough power
to create such a profound disturbance in the Higgs field
that the predicted Higgs bosons would pop into existence
and present themselves.
But easier said than done.
FABIOLA GIANOTTI: In order to find this particle,
we had to build this complex, cutting-edge accelerator.
The work is the work of thousands of people.
20 years of effort went into building these detectors.
GIANOTTI: 20 years of efforts of the international community.
NARRATOR: From dozens of nations,
with the U.S. contributing $500 million.
It took $10 billion and ten years
to complete the Large Hadron Collider,
a massive masterpiece of engineering,
to find one of the tiniest pieces of the cosmos.
It's a very cool and expensive eye
that can look at very, very small distances
like about a billionth of a billionth of a meter.
LYN EVANS: We designed this machine
so that wherever the Higgs boson would be,
we would be able to find it.
NARRATOR: Flushing the Higgs out of hiding
begins in a modest little red bottle full of hydrogen atoms,
the smallest and most abundant element in the universe.
All the protons that we use at CERN are taken
from a bottle that size.
They start their journey here and they continue
down this orange line, and that is the linear accelerator.
NARRATOR: Trillions of hydrogen atoms stripped of their electrons
are injected into the collider.
STORR: Every 1.2 seconds...
ten to the power 14 protons are being accelerated
down that line.
NARRATOR: The protons accelerate around larger and larger loops
until they are finally directed into the main ring.
To keep the increasingly energetic particles confined,
the LHC relies on immensely powerful magnetic fields
generated by 1,232 primary superconducting magnets,
cooled to just a few degrees above absolute zero
by 120 tons of liquid helium.
After about 20 minutes of acceleration,
each bunch of protons is moving at nearly the speed of light,
with as much energy as an onrushing locomotive.
Finally the protons are carefully steered
into violent head-on collisions...
converting the huge energy into showers of exotic,
energetic particles, scattering in all directions,
many decaying into showers of even more particles,
setting the stage for the hard work of detecting the Higgs.
STEVEN WEINBERG: Trying to figure out what happens
in the collision of two protons at very high energy
is like analyzing what happens
in the high-speed collision of two garbage trucks.
Garbage is spread all over everything,
and most of it is garbage in the sense that it's not interesting.
It's old stuff that we already knew about.
And in all this garbage that's spraying out
in all directions on the highway,
you have to find the golden needle,
the rare artifact that you're looking for, the Higgs boson,
something entirely new.
NARRATOR: To the scientists at CERN,
a collection of physicists from all over the world,
the stuff produced in these powerful collisions
is anything but garbage.
Each particle has a well-understood identity,
described with great precision
in one of the most accurate theories ever devised
to explain the workings of the universe.
It's called the Standard Model,
and one of its key contributors is Frank Wilczek.
Hi, welcome.
Come on in.
A lot of what I do is really just play.
I mean, I play with the equations and ideas.
NARRATOR: All that playing won Frank a Nobel Prize
for his contribution to the Standard Model.
Well, what have we got here?
It looks like an instrument of torture for the mind.
NARRATOR: The Standard Model is essentially an understanding
of how all the known pieces of the universe fit together,
except for the mechanism of gravity,
creating a mind-boggling tapestry.
WILCZEK: This is going to be a hell of a puzzle
to figure out.
All right, now, a promising start.
We think the Standard Model contains all you need
in principle to describe how molecules behave,
all of chemistry, how stars work, all of astrophysics--
not only how things behave, but what can exist.
These are the rules of the game.
The ingredients of the Standard Model are of three basic sorts.
There's what you might broadly call matter.
That's sort of lumps of stuff
that have a certain degree of permanence.
And these are, on the one hand, quarks.
They include the building blocks of protons and neutrons
and atomic nuclei.
And leptons.
Most prominent lepton in everyday life
is certainly the electron.
So those are matter particles.
On the other side, we have what you might call force particles
or force mediators.
NARRATOR: Called "bosons,"
some of these particles are more like lumps of energy.
They transmit the forces
that bring the matter particles to life.
They include the photon,
which carries the electromagnetic force;
the gluons that carry the strong force
which holds protons and neutrons together;
and the W and Z bosons that are responsible
for the weak force governing radioactivity.
With just this small list of ingredients,
the Standard Model explains the physical properties
of the elementary building blocks of nature.
The Standard Model is just a handful of particles and forces,
and it explains every experiment ever done
by every human being in the history of science.
So it's quite impressive in what it's managed to do.
It explains how stars burn.
It explains how radioactivity occurs.
It explains how chemistry works.
It explains how light works.
It's an amazing theory.
NARRATOR: The first particles were discovered in experiments
and became the foundation for the Standard Model.
But then the theorists took over
and all the particles discovered in the last 40 years
were first predicted by the mathematics
of the Standard Model and then found experimentally.
The Higgs boson, a force particle, was the last
and most challenging piece of the puzzle.
That's why finding it was such an obsession among theorists
and experimentalists alike.
In September 2008, with much fanfare...
(applause)
...the giant accelerator was switched on.
The LHC was ready to go to work.
It was an exciting time, full of high expectations.
Designing and building this machine,
it's just incredible to see it come to life.
NARRATOR: But then, just nine days after start-up...
disaster struck.
It was 11:00 in the morning,
and I got a call to come over, something looks serious.
And when I got over there, I had never seen such carnage.
NARRATOR: A short circuit burned a hole
in a giant container of liquid helium used to cool the magnets.
Six tons of helium was released into the tunnel
and more than 50 of the giant magnets were fried.
The $10 billion LHC was dead in the water.
Undaunted, engineers worked to repair the machine
and physicists continued to refine the computer programs
that would analyze the vast amount of data
that the LHC would produce
once it was running at full power.
WOMAN: Three, two, one...
(beeping)
(applause)
NARRATOR: By late 2009, after 14 months of repair work and reengineering,
the LHC was more robust than ever
and finally ready to begin the hunt in earnest.
Now, protons are whizzing both ways around the ring
at nearly the speed of light.
At the center of the two Higgs detectors, the beams cross
inside ATLAS, a massive machine the size of a cathedral
and also within its smaller cousin, CMS.
Even though the beams are microscopically small,
the vast majority of particles contained in them
whiz past each other without incident.
FRANKLIN: When you collide 100 billion protons and 100 billion protons,
most of the protons are just seeing each other
and going, "Hello," and going on.
NARRATOR: But about 800 million times every second,
pairs of protons meet head-on.
FRANKLIN: What's called a "hard collision."
When the proton breaks up so it's no longer a pron,
that's an interesting collision.
And that happens only about 20 times
out of all these billions of protons crossing.
NARRATOR: In each of these powerful collisions,
dozens of new particles flash into existence
and spray outward, their unique signatures tracked
by the huge detectors,
capturing the action 40 million times a second.
Incredibly fast, but still not able to spot the Higgs directly.
CARROLL: The Higgs is actually kind of a difficult particle to find.
It's kind of subtle in how you look for it.
As soon as you create it, it decays very, very quickly.
The lifetime of a Higgs is about one zeptosecond,
which is like ten to the minus 21 seconds.
So, in fact, you'll never even see it
in a particle accelerator.
It doesn't move that far,
enough for you to see any track left behind.
NARRATOR: And so, the only way to detect the Higgs would be by spotting
the more familiar particles
that the quickly vanishing Higgs decays into.
The math predicted
about a dozen different possible decay modes, as they're called.
But the relative likelihood of any of them
depended on the mass of the Higgs...
which was a total mystery.
It must have seemed like a cosmic joke on the theorists.
JOSEPH LYKKEN: The irony, if you like, is that
although the Higgs field that's related to the Higgs boson
gives other particles mass,
the one property of the Higgs boson that was not predicted
by Professor Higgs and his colleagues
was the mass of the Higgs boson itself.
So its mass could have been anything
from very, very light by our standards to very, very heavy.
NARRATOR: Since the Higgs could theoretically decay
in so many different ways,
the Higgs hunters had to be willing to sift
through all of the collision debris,
looking for slight increases
in the number of detectable particles,
with very specific characteristics,
into which the Higgs could possibly decay.
CARROLL: So it's not like looking for a needle in a haystack,
when at least you know that you found a needle.
It's like looking for hay in a haystack.
You're looking for a little bit more hay with certain properties
than certain other properties.
NARRATOR: That daunting challenge meant
building enormously complicated detectors
to track and count every bit of debris
coming out of those collisions.
FRANKLIN: And then we have to somehow,
with all of the particles that come out of this event,
we have to reconstruct them and find if there are new particles
that are happening.
NARRATOR: The mathematics predicts that the Higgs should often decay
into particles that are also maddeningly hard to detect--
like quarks, the particles that make up protons and neutrons
in the nuclei of atoms.
They looked in every possible way they can look.
In the end,
they looked for the Higgs boson decaying into photons.
NARRATOR: Out of every thousand Higgs bosons created,
a few should decay in a way that produces a pair of photons--
light particles
which can be measured very precisely in the detectors.
By knowing the energy and angle between pairs of photons,
scientists can tell if they were likely produced by a Higgs.
And by looking for unexpectedly high concentrations
of certain photons over billions of collisions,
scientists hoped to zero in on the Higgs and, as a consequence,
pinpoint its exact mass--
the one missing value in the theory.
It proved to be a statistical sifting process
of dizzying complexity.
Luckily, they had a head start.
Years of experiments in other colliders had ruled out
many possible masses for the Higgs,
measured in units called gigaelectronvolts, or GEV.
So on this line of what the mass of the Higgs might be,
we can draw on what previous experiments have...
have tried and where they've been able
to exclude it from being.
NARRATOR: A less powerful accelerator, the LEP Collider at CERN,
a predecessor of the LHC,
had already ruled out the Higgs being at the bottom end
of potential masses.
In fact they were able to say that the mass of the Higgs
is, with 95% confidence, 114 GEV or more.
So after LEP, the next major milestone in the...
in the Higgs search was limits set by another collider
in the U.S., the Tevatron.
The Tevatron was able to exclude
a range here around 160 GEV here.
NARRATOR: In 2011, CERN moved that upper boundary still lower.
DAVISON: The LHC has been able to rule out a big region
from 145, quite far up.
NARRATOR: But this last remaining energy range
was also the trickiest to search.
It's the area in which the unique signature of the Higgs
would be mostly deeply buried under the background noise
of other particles created in the collider.
MAN: If I was to bet,
I would probably put it at 130 GEV.
Probably somewhere around 120 GEV.
Somewhere between 120 and 130 GEV.
114 GEV because it's the most difficult place to look
and we haven't found it yet.
Ah, that's a good question,
because you know you are assuming that the Higgs
actually exists, which I'm-I'm starting to believe
it probably does not exist.
NARRATOR: As data piled up at the LHC,
scientists narrowed the range even further.
It seemed that they were either about to close in
on the Higgs particle or prove that it didn't exist at all.
People were beginning to worry a little bit
that we hadn't found the Higgs yet
and maybe weren't going to find it.
And that would've been a complete shock
because we know that something is doing the job of the Higgs.
You start to get a little nervous
because either it's there
or there isn't a Higgs boson at all.
NARRATOR: By the end of 2011, the window narrowed even further.
The LHC, with the new data from the whole of 2011,
is able to expand the area that it can exclude the Higgs from.
NARRATOR: The new lower limit had risen to 115 GEV,
and the new upper limit dropped to 127 GEV.
And within that range,
interesting things were showing up in the data.
DAVISON: So the really exciting thing
was that the reason the LHC experiments weren't able
to exclude anything inside this remaining window
is that in fact they see an excess of events,
the early signs of the Higgs boson, if it's there.
NARRATOR: An eess of events means that the LHC was producing
more particles of interest-- in particular, pairs of photons.
RANDALL: So, what you're looking for is called a bump
because at that particular energy,
you should see a lot more decays...
if there is a Higgs boson.
So if you see a bump, that's a clue that something's going on.
NARRATOR: Those excess photon pairs were showing up in not just one...
but in both detectors, and at practically the same mass.
CMS was seeing a spike in the number of photons
which could be the signal of a Higgs with a mass of 124 GEV.
And ATLAS was seeing a similar spike near 125.
Now with the hunt finally closing in,
the LHC continued smashing protons,
sorting through the debris and piling up the data
for another six months.
We saw a signal growing, growing every week, every day.
NARRATOR: Until at last, on July 4, 2012, the heads of ATLAS and CMS,
Fabiola Gianotti and Joe Incandela, called a meeting.
DIETER HEUER: Two presentations from the two experiments, ATLAS and CMS.
NARRATOR: There to hear the news firsthand: Peter Higgs himself.
It was standing room only.
HEUER: Good afternoon, everybody in Melbourne.
NARRATOR: But it was also beamed live around the world.
FRANKLIN: So, of course,
everyone's heard lots of rumors at this point,
within the collaborations.
But there are these two collaborations,
the CMS collaboration and the ATLAS collaboration.
And we aren't supposed to know what they have, and I didn't.
You know, you'd heard stories, but I hadn't seen their data.
So that's kind of exciting.
So, today is a special day on a search for a certain particle.
NARRATOR: But no one was quite prepared
for the short, definitive announcement that was to come.
And I ask Joe Incandela from CMS to take the floor.
NARRATOR: This was about to become one of the defining moments
in the history of physics and science.
INCANDELA: And the energy was so incredible.
It was like a big party.
People were really excited.
And it was just then I think I started to really appreciate
where we were and that this was a major discovery.
This slide shows you one event taken just a few weeks ago.
I put the slide up and before I could say anything,
there was a gasp across the whole audience.
Now, a major result like this
from one experiment could still be wrong.
Now we go immediately to ATLAS.
Fabiola Gianotti, please.
Thank you.
But Fabiola brought the same confidence for her results.
You can already see here the compatibility between
what we observed: one big spike, here in this region here.
FRANKLIN: If you look at these plots that were shown,
first thing you want to see is
did CMS and ATLAS find the bump in the same place?
NARRATOR: And in fact they had.
GIANOTTI: An excess at a mass of 126.5 GEV.
NARRATOR: Both teams had found an excess of photons
pointing to the same mass.
FRANKLIN: And that was pretty convincing.
So you're going, "Wow," like, "we rock."
As a layman I would now say I think we have it.
You agree?
(cheers and applause)
NARRATOR: The LHC had found the Higgs particle.
HEUER: We have observed a new particle consistent with a Higgs boson.
INCANDELA: It's like running a marathon.
Suddenly you realize you crossed the finish line.
Maybe one more round of applause to all the guys
who took part in the project for more than 25 years.
LYN EVANS: It comes as a big surprise to me, I must say.
I went into that seminar expecting good results.
But I was gobsmacked, as they say.
NARRATOR: The hunt that spanned half a century was over.
The Higgs boson hid for 50 years.
But, you know, like they said with the Canadian Mounties,
"They'll get their man."
It could run, but it couldn't hide forever.
(applause)
NARRATOR: It appeared Higgs and his colleagues had been right.
The mysty of how particles gain mass had been solved.
The last piece of the Standard Model had been found.
For me it's really an incredible thing
that it's happened in my lifetime.
GIANOTTI: I had the pleasure to meet Peter Higgs
at the end of the seminar and exchange a hug.
He told me,
"Congratulations to you and your experiment
for this incredible achievement."
And of course, I replied, "Congratulations to you!
You are the first person to be congratulated."
I think it's not appropriate for me to answer
any detailed questions at this stage.
This is an occasion celebrating an experimental achievement
and I simply congratulate the people involved.
NARRATOR: Ironically, the achievement took place at the very same institute
where nearly 50 years earlier,
an editor had rejected Higgs' initial paper.
MAN: The Royal Swedish Academy of Sciences...
NARRATOR: In a fitting end to the saga,
Peter Higgs and Belgian physicist François Englert,
who had independently come up with the idea
for the Higgs field, won the 2013 Nobel Prize.
Englert's colleague, Robert Brout,
certainly would have been honored as well
had he lived to see the day.
So why is all this important?
Why does proving the existence of the Higgs field matter?
Building an enormous Big Bang machine to recreate conditions
in the universe near the beginning of time
and completing the Standard Model
is a tremendous scientific achievement.
FRANKLIN: Finding the Higgs sheds light on all of particle physics
and cosmology.
It's all connected.
All our models of how the universe began, how it expanded,
everything, is, you know, affected by the Higgs field
and by how we understand the universe.
NARRATOR: Perhaps discovering the Higgs boson and the field it proves
will open new doors...
GIANOTTI: The discovery of the Higgs is just the first step.
In science you make a step forward--
you answer a question, but then other questions open up.
NARRATOR: ...into even greater mysteries that still remain
beyond the Standard Model.
INCANDELA: The Standard Model can't be the final thing.
There is something beyond the Standard Model; we know that.
Hopefully the Higgs can give us some guidance in that direction.
Yes, we do know the Standard Model works.
It works incredibly well.
But we know it's not the whole story.
And any time in the history of physics
where people thought they had the whole story they were wrong.
And so we're looking for what is the next piece,
not just in terms of one particle
but in terms of forces, in terms of understanding nature.
The number of mysteries in the Standard Model is huge,
which is fine because, as a scientist,
I'm drawn to mysteries.
NARRATOR: One mystery that the Standard Model can't answer
is perhaps the most fundamental of them all.
Why isn't our universe empty?
Because according to the mathematics
behind the Standard Model, it should be.
Science has given us a set of laws that describe the world
so accurately that we can predict the motion of a coin
tossed in the air because we understand the law of gravity.
We understand electromagnetism so well
that we can use our GPS satellites to locate your car
to within a few inches.
And we understand the nuclear force so well
that we can predict the future evolution of the sun itself.
NARRATOR: Those mathematical equations that work so well
to describe the laws of the physical world
are bound together by something that we see around us every day.
Something that characterizes our faces...
and the natural world...
even the tiniest structures like viruses and our DNA--
symmetry.
WILCZEK: In the Standard Model, symmetry rules.
The laws are dictated, really, in their form
by requiring tremendous amounts of symmetry.
That's how we found them.
NARRATOR: The equations of the Standard Model seem to predict a universe
in perfect balance, formless and without structure...
(explosion)
as it was at the very beginning.
And if it had remained that way, nothing would exist.
If the laws of science are framed in their most perfect,
most symmetrical form, then life cannot exist at all.
There'd be no mountains, rivers, valleys,
no DNA, no people, nothing.
NARRATOR: A universe created along absolutely symmetric principles
would be in perfect balance.
The Higgs field is the first clue to what broke the symmetry
of that completely uniform early universe.
The state of perfect symmetry is very similar
to the state of perfect balance.
Think of a spinning top.
It exists in a state of perfect rotational symmetry.
No matter how you rotate, everything looks the same.
NARRATOR: Even more so than the symmetry of a spinning top,
at this instant of creation,
every place in the universe would have been symmetrical,
identical to every other place.
But perfection isn't stable.
The slightest imperfection, the slightest little defect
will cause it to vrate, perturb,
and fall to a lower energy state.
Symmetry has been broken.
NARRATOR: Within a fraction of a second of the Big Bang,
physicists believe the absolute symmetry of the universe
was shattered by a tiny fluctuation.
The Higgs field appeared in all of space.
The forces split apart.
The particles of the Standard Model became distinct.
Structure emerged.
This fall from perfection was what allowed us
to come into being.
KAKU: Everything we see around us is nothing but fragments
of this original perfection.
Whenever you see a beautiful snowflake, a beautiful crystal,
or even the symmetry of stars in the universe, that's a fragment.
That's a piece of the original symmetry
at the beginning of time.
NARRATOR: Finding and studying the Higgs is a vital first step
in the quest to understand that early state
when the particles that make up what we can perceive
came into being, as well as a much greater quantity
of mysterious stuff that we know is out there
but that we can't directly detect, called dark matter.
What are these missing pieces?
When James Gates came to study at MIT,
he was determined to unlock the secrets of the early universe
and understand what happened to the unity that was once there.
GATES: The universe and we are intricately tied together.
This idea of unity turns out to be
one of the most powerful driving themes in physics
and it keeps getting us to look
for deeper and deeper connections.
So ultimately, perhaps, we exist
because the universe had no other choice.
NARRATOR: He looked at the Standard Model,
the matter particles and the bosons, the force particles,
that hold everything together.
He wondered if these two groups of particles
that seem so different could be related
in some profound and hidden way.
This question--
why is there a fundamental asymmetry of forces and matter--
led him to a powerful mathematical theory
called supersymmetry.
It was the asking of this "what if?" question
that drove the construction of supersymmetry,
which had an incredible resonance for me
when I was a graduate student.
I saw one more beautiful balance that we could put in nature.
NARRATOR: One of the pioneers of supersymmetry,
Jim Gates saw in the mathematics a possible hidden world
of new particles no one had suspected.
GATES: Mathematics leads us to find things we didn't know
were there before.
Supersymmetry is an example of that.
We know about ordinary matter.
The mass leads you on
to discover supermatter and superenergy.
NARRATOR: The theory gives every matter particle a force partner
and every force particle a matter partner.
These heavier supersymmetric twins are labeled sparticles.
So once you believe this math
that says there's more to existence,
then you have to wonder what these other things are.
You have to name them, at a very...
you know, at the very first step.
So in nature there is a thing called the electron.
The math says it has a superpartner
called the selectron.
Muon, it'd have to be a smuon;
photon, there'd have to be a photino;
quark, there'd have to be squarks;
Z particle, there'd have to be zino;
the W particle, there'd have to be a wino.
And that's how supersymmetry works.
NARRATOR: According to supersymmetry,
matter and forces aren't so distinct after all.
There's a grand symmetry between them
but we can currently see only e partner from each pair.
However strange it seems,
this theory has gained widespread support
from theoretical physicists.
(clanging)
Not just for the beauty of its equations
but for what it might help explain.
GATES: When supersymmetry began as a topic of discussion,
no one realized what it can do.
It turns out that studying the mathematics,
we get a firm foundation for the existence of everything.
NARRATOR: Supersymmetry could shed light on dark matter--
the missing particles that aren't included
in the Standard Model-- and even help to explain
how symmetry was broken in the first place.
WILCZEK: I very much want supersymmetry
because it's a beautiful thing by any standard
and would take our understanding of nature to a new level.
So I want that.
NARRATOR: Finding the Higgs pushed the LHC to the limit
of what it could do.
So, a few months after the Higgs announcement...
the scientists at CERN shut down the giant collider...
and began a planned two-year upgrade.
As it begins its second act,
it will smash protons even more energetically.
FRANKLIN: So when the LHC turns back on in 2015,
we will be at twice the energy we were before.
NARRATOR: The increased power will help physicists to study the Higgs
with more precision, but the real hope is that they will find
something entirely new.
Every single experimentalist is only thinking this:
Is there a massive particle we can now make with this energy,
with these energetic protons, that we haven't seen before?
NARRATOR: For the theorists, too,
it is an exciting and nerve-wracking time.
If we find supersymmetry in experiments, for me personally
it will mean that I have not wasted my entire research career
because this is the one question as a young scientist
I decided had my name on it to study.
I'm starting to get nervous.
(laughs)
You know...
So there were a lot of people who predicted
that supersymmetry was just around the corner
or something else, that as soon as LHC turned on
they'd see spectacular effects on the one hand,
or that the Higgs particle would be heavy on the other hand.
Those are all wrong.
Now it's make or break time.
NARRATOR: For the thousands of scientists who have come together
in this great quest,
pushing the frontiers of knowledge
has been a wild rollercoaster ride.
And with the Large Hadron Collider...
MULTIPLE VOICES: Three, two, one...
zero.
NARRATOR: The fun has only just begun.
The exploration continues online,
where you can watch this and ot NOVA programs.
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to explore the world's largest particle accelerator.
Also, what are gravitons, what is dark energy
and what is the smallest particle?
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