Inside this labyrinth of pipes and chambers,
superheavy elements are being fused into existence.
This machine is part of an international hunt
to unlock the mysteries of this new class
of elements that typically don’t exist here
on Earth.
Pushing these element discoveries really is
pushing into models of how matter is formed
in the big bang.
How do we model matter?
And how do we model the formation of the universe?
Superheavy elements exist for a fraction of
time and are nearly impossible to catch.
But understanding them could force us to reimagine
the most iconic scientific symbol of all time:
the periodic table.
In 1869, Russian chemist, Dmitri Mendeleev,
laid the foundations for what would become
the modern periodic table.
He arranged the known elements in order of
increasing atomic weight–starting with the
lightest ones with the least protons and working
his way up.
And as he did so, a curious pattern started
to emerge.
What happened is he noticed that at regular
intervals, chemical properties were repeating
themselves.
Because of this periodicity in the chemistry,
he realized that there were elements at that
time that had not yet been discovered but
should be there.
In the following years, scientists started
isolating the elements Mendeleev predicted
from various materials.
Scandium was found in a hunk of euxenite,
gallium in a piece of zinc ore, and hafnium
in a zirconium mineral, to name a few.
The table’s design was revised and perfected
as more elements were added.
But as nuclei got heavier and heavier, finding
them became a bit more complicated.
When we refer to heavy elements, we're talking
about things that have these very large nuclei
that have a lot of protons in them.
Above uranium, nothing exists here naturally.
They have more protons in their system than
anything that we have naturally occurring.
In order to continue their quest towards a
complete periodic table, scientists couldn’t
just continue isolating elements from existing
materials.
They had to create them.
So we use what's called a particle accelerator
or specifically a cyclotron, which is a large
instrument that accelerates ions to a fraction
of the speed of light.
Cyclotrons have been used to discover heavy
elements ranging from curium to plutonium.
And most recently, Dr. Shaughnessy’s team
collaborated with a lab in Russia to complete
the periodic table’s 7th row– the home
of the superheavies.
When we make one of these new elements in
the cyclotron we really have to just add up
protons.
So for instance, if we wanted to look for
element 116, we could take something with
20 protons and we can take something with
96 protons, and if we can get those two nuclei
to completely fuse together for even a short
time that means we have an element 116, one
atom of it.
These elements are very short lived they're
not very stable, so they decay very quickly.
Some superheavy elements only exist for just
milliseconds.
So, in order to confirm they created one,
the team had to work backwards– sifting
through the data to find the signal that told
them a heavy element was actually there.
The Flerov lab in Dubna has an incredible
cyclotron that's really a work horse.
And we at Livermore have access to various
target materials.
So we provided our expertise, the Russians
provided their expertise, and together discovered
elements 114 through 118.
While efforts to discover more elements continue,
Dr. Shaughnessy and Dr. Gates have shifted
their sights to studying the ones we already
have.
We know almost nothing about these superheavies,
including whether or not we’ve put them
in the right place on the periodic table.
Right now, when an element is discovered,
we're putting it in the periodic table based
on its number, mostly for convenience.
But the periodic table, let's remember, it
was constructed to be a living document on
the chemistry of these elements.
The models predict that these heavy elements
might behave unexpectedly due to something
called relativistic effects.
We have these big massive nuclei and what’s
happening is they're accelerating their electrons
to near relativistic speeds.They're going
so fast that they're being dominated by the
theory of relativity.
What that does is it's changing the mass of
the electron and that's changing how it bonds
and its chemistry.
So when we get to this last row of the periodic
table, what we see sometimes, is that the
chemical properties down a given group may
invert or do something totally different.
We believe that we have them in the right
position, but we also don't think we've proven
that.
And so, what we did was we built FIONA to
actually prove that what we think is true,
actually is true.
Hooked up to the Lawrence Berkeley National
Lab’s 88 inch cyclotron, FIONA is one of
the newest tools designed to study superheavy
elements.
Its primary goal is to experimentally confirm
their mass numbers.
But before FIONA can measure the mass, the
team needs to create a superheavy element.
So we are in cave one at the Building 88 facility.
The beam comes from the cyclotron, which is
right through that wall, and then it travels
all the way down this line here until it reaches
our target out the other side.
This is what our targets look like, or this
is three fourths of a target.
We have just a couple of thousand atoms thick
of whatever our target material actually is.
What we're interested in is one nucleus from
the beam hitting one nucleus from the target
and completely fusing.
The problem is that doesn't happen very often.
Nuclei are very small compared to atoms, so
a nucleus is about 10,000 times smaller than
the atom itself.
When the beam comes in, what it actually sees
is mostly empty space. It actually passes through
our target, mostly.
And then very, very rarely we'll get this
head-on collision that makes that atom that
we want.
Right inside this box, that's where our elements
are made.
Now our job is to find a way to separate all
that junk that we don't want, from that one
atom that we do.
Everything travels through the Berkeley Gas-Filled
Separator - a machine equipped with giant
magnets that bend the excess atoms away from
the superheavy the team is interested in.
Then it enters stage one of FIONA.
That's all of that equipment over there.
It traps it in a small volume,
and then it sends it on to stage two of FIONA.
Magnetic fields then send the superheavy atom
into a specialized loop.
And, it’s the specific path it takes within
that loop that tells the team its mass.
FIONA's first scientific experiment started
in June of last year.
We were able to confirm that those new heavy
elements that we've discovered really do have
the number of neutrons and protons that we
think that they do.
But confirming that isn’t quite enough to
know for sure that we’ve put them in the
correct place on the table– we also have
to explore their chemistries.
We have atoms trapped in a cubic millimeter
of volume for a time that we pick.
We can add in different gases and we can change
the amount of time we trap things for.
We can look, "Does this gas react with this
atom?
And if so, what does it make?
We could actually learn quite a bit about
the chemistry of these new elements.
And at Dr. Shaughnessy’s lab, her team is
looking into alternative methods.
Here at Livermore we're trying to develop
a way to do aqueous chemistry of 114.
Hopefully this collection of data from both
the gas and aqueous phase will start to paint
a more complete picture.
If we do see some real shift in chemistry
we would have to rethink that last row.
What does that mean for our periodic table?
150 years after its conception, the periodic
table is reaching a turning point.
As Dr. Gates, Dr. Shaughnessy, and teams around
the world continue to unlock the mysteries
at its borders, they’re also starting to
question just how much further those borders
can be pushed.
There are people who have tried to predict
where the periodic table will end.The most
common number thrown about is around element
172, or 173.
The issue is that the probability of making
the two nuclei come together, it gets smaller
and smaller as we go up in element numbers.
So with element 118 it was a very small probability
that we would make it.
Now for 119 and 120 it's even getting lower
and lower.
In order to push out to heavier elements there's
going to have to be some real shifts in technology
compared to what we have now.
You're trying to answer a basic scientific
question.
How many elements are there in the universe,
and what are their chemical properties?
That's something that's interesting, regardless
of whether or not there's any scientific applications
for it.
If you break down an advanced piece of technology,
a new medicine, or an energy source to its
essential parts— you always end up with
the same thing: those same blocks that make
up you and me and the stars in the night sky.
It’s about the elements themselves.
The formation of these elements alone tells
us a lot about nuclear theory and how the
nucleus holds together.
We've already changed over the decades how
we think of the nucleus.
So that's where the application is right now,
is really in just our fundamental understanding
of the universe.
