Video Transcript
In this video, we’re talking about
neutron emission. This is one way that the nucleus of
an atom can undergo radioactive decay. Whenever an atomic nucleus gives
off an uncharged particle, a neutron, that’s neutron emission. And we can get a better sense of
how this works by considering a specific example.
Say that we have an atom of iodine
represented with this symbol, capital I. Iodine has an atomic number of 53,
and we’ll say the mass number of this atom is 137. We can recall that the mass number
of an atom is equal to the number of protons it has in its nucleus plus the number
of neutrons it has. While the atomic number simply
reports the number of protons. This means if you want to solve for
the number of neutrons in an atomic nucleus, we just need to subtract the atomic
number from the mass number. 137 minus 53 is equal to 84. So that means that this particular
atom of iodine has 84 neutrons in its nucleus.
We can see then that there are
significantly more neutrons in the nucleus than there are protons. We could describe this atomic
nucleus as neutron rich and proton poor. Atomic nuclei like these are strong
candidates for neutron emission. Let’s say that our iodine atom goes
through this type of nuclear decay. It gives off a neutron. The resulting atom will still be
iodine. That is, it will have 53 protons in
its nucleus. But since it’s lost one neutron,
its mass number will no longer be 137 but 136. The neutron emitted in this process
is symbolized this way, using a lower case n. Lower case because a capital N
represents the element nitrogen. And we can see that this neutron
has an atomic number of zero because it has no protons or electric charge to it. But it has a mass number of one
because there’s one neutron in it.
So this, then, is a nuclear
equation that shows us neutron emission. And notice that both atomic number
and mass number are the same on either side of this reaction. Regarding atomic number, on the
left-hand side, we have 53. And on the right-hand side, we have
53 plus zero. And then, with respect to mass
number, we have 137 on the left and 136 plus one, or 137, on the right. So then, here’s what we can say has
happened to this atomic nucleus once it undergoes neutron emission.
Neutron emission does not change
the atomic number involved. That stays the same. It also doesn’t affect the charge
of the nucleus involved because a neutron has no electric charge. However, neutron emission does
change the mass number of an atom. It decreases it by one for every
neutron emitted.
Now, one way to represent neutron
emission or other types of radioactive decay is through a graph called a nuclear
decay graph. These graphs are typically set up
so that the number of neutrons in a nucleus is plotted against the number of protons
it has. Now, let’s say we had some
particular atomic nucleus with a specific number of protons and neutrons. And let’s say that it fit right
here on our graph. That is, it has this many protons
in its nucleus, however many that is. And it has this many neutrons,
however many that is. As we’ll see, the numbers
themselves aren’t as important as how those numbers change. And indeed, if this atomic nucleus
undergoes some sort of radioactive decay, then those numbers will change.
We know there are a number of
different radioactive decay possibilities. A nucleus could emit an alpha
particle or could emit a beta plus or a minus particle or, and we’ll assume this is
the case for us, it could emit a neutron. If that happens, if this nucleus
gives off one neutron, then that means the number of neutrons it has will go down by
one. However, because it’s only neutron
emission and nothing else is given off, the number of protons in the nucleus will
stay the same. This means that if we want to
represent this transition on our graph, we do it by drawing an arrow from where our
nucleus originally was to where it transitions to following this decay event.
As we consider the starting and
ending location of our nucleus, we can see that what we’re indicating is a loss of
one neutron while maintaining the number of protons in this nucleus. The decay event that corresponds to
this is neutron emission. Now, notice that the atomic nucleus
we have here is not the same as the one we have here. It’s true the element hasn’t
changed because the number of protons in the nucleus is the same. But because the number of neutrons
is different, what we have are atomic isotopes of one another. Now, let’s say that our resulting
isotope, this nucleus right here, also underwent neutron emission. That would mean that, once again, a
neutron is lost from the nucleus, while the number of protons in it remains the
same.
We would indicate that transition
with a line like this. And our new nucleus would be here
on our decay graph. So then, on a nuclear decay graph,
which plots the number of neutrons in the nucleus versus the number of protons. Anytime we see vertically downward
transitions like we’ve seen here, that indicates the process of neutron
emission. That’s the kind of decay that must
be going on.
Now, recall that we mentioned that
when a nucleus changes, when it undergoes radioactive decay, there are different
kinds of particles it can give off. One of those is called an alpha
particle, also known as a helium nucleus because an alpha particle has two protons
just like the nucleus of a helium atom. Because an alpha particle has two
protons and no electrons, that means it has a net or a relative charge of positive
two. This strong relative charge makes
an emitted alpha particle very likely to interact with other matter. This means that alpha particles are
unlikely to travel very far at all into a solid material because they quickly
interact with that material.
We say then that the penetration
depth of an alpha particle is very low. It’s easily blocked even by fairly
thin layers of material, such as a sheet of paper. So alpha particles don’t penetrate
into material very far. But what about something else that
might be emitted in a decay process? For example, what about a beta
particle, in particular, a beta minus particle which is an electron? Knowing that an electron is much
smaller than an alpha particle in size, we would expect it to have a better
penetration depth. One thing going against it, though,
is that the beta particle, like the alpha particle, has a net charge. This means it, too, is likely to
interact with matter rather than passing right through.
Thanks to its relatively smaller
net charge and relatively smaller size, the beta particle does have a greater
penetration depth than the average alpha particle. But it turns out that neither of
these compares with the penetration depth achieved by emitted neutrons. Neutrons are able to travel so far
into matter without interacting with it, largely because they have no electric
charge. This means they’re neither
attracted to nor repelled by any other electric charges. And recalling that atoms are mostly
empty space, a neutron is typically able to pass right on through. But when a neutron doesn’t pass
right through but instead interacts with the nucleus of an atom, something
interesting can happen.
When a neutron runs into an atomic
nucleus, and we could say is captured by it, then as a result of that capture, the
nucleus becomes heavier. And it can enter an excited
state. A nucleus in an excited state is an
unstable nucleus. That is, one prone to radioactive
decay. So here’s what this means. By emitting a neutron, which was
then captured by this nucleus, we’ve created radioactive material. This process, where a neutron is
captured by a nucleus which then becomes heavier and enters an excited state, is
called neutron activation. And the result, as we saw, is
radioactive material.
This is one reason why emitted
neutrons can be considered dangerous. They’re capable of creating
radioactive material where there was none before. Along with this, emitted neutrons
are capable of creating ions in the atoms they collide with. Not directly because a neutron has
no electric charge but indirectly through, say, colliding with an electron and
bumping it off an atom. So despite their neutral electric
charge, neutrons can actually have quite an impact on atomic nuclei and overall
atomic charge. This is one reason why in
radioactive decay scenarios that involve emitted neutrons, shielding is carefully
installed. Now that we understand a bit about
neutron emission and what causes it, let’s get a bit of practice with these ideas
through an example.
When an unstable nucleus emits
a neutron, by how much does the atomic number of the nucleus change?
Okay, so in this question, we
have an unstable nucleus. Let’s say that this is our
unstable nucleus, jiggling and shaking because it’s about to decay. We’re told that as this nucleus
decays, it gives off a neutron. And we want to know by how much
does this change the atomic number of the nucleus. Now, we can recall that given
some atomic element, let’s call it element X, that element has a certain number
of protons, sometimes symbolized Z. And it has a certain number of
protons plus neutrons, often symbolized N. Now, this number here — what
we’ve called Z, the number of protons in the nucleus — is also known as the
atomic number. It’s literally how many protons
there are in the nucleus of an X atom, whatever X is.
So then, going back over to our
unstable nucleus, we’ve drawn the neutrons in green and the protons, the
positively charged particles in blue. And in this emission process,
we’ve lost a green particle, that is a neutron. But we’ve kept all the blue
ones, the protons. Since it’s the protons that
make up the atomic number of our nucleus, that means the atomic number of this
nucleus hasn’t changed. Another way to say it is, its
change is zero. That’s because, as we saw, we
emitted a neutron. But that has no effect on the
atomic number of the nucleus. So when an unstable nucleus
goes through neutron emission, the atomic number of the nucleus does not
change.
Let’s look now at a second example
exercise.
When an unstable nucleus emits
a neutron, by how much does the mass number of the nucleus change?
So in this example, we have an
unstable atomic nucleus. We can show that here, with the
blue circles representing positively charged protons and the green circles
representing neutrally charged neutrons. And our problem statement tells
us that this nucleus is unstable and emits a neutron. So we could represent that this
way, with our nucleus giving off a green circle, a neutron. And the question is, how much
does this emission change the mass number of the nucleus?
Well, let’s remind ourselves
what the mass number of any given nucleus is. Say that we have some atomic
element. We don’t know what element it
is, so we’ll just give it the symbol X to represent that element. We know this element has some
number of protons in its nucleus. We represent that with Z, which
stands for the atomic number of the element. And if we add together the
number of protons with the number of neutrons in its nucleus, we get what’s
called its mass number. So Z, the atomic number, is the
number of protons in the nucleus. And N, the mass number, is the
number of protons plus the number of neutrons.
All this to say, if we were
interested in solving for the number of neutrons in an atom, we could subtract
Z, the atomic number, from N, the mass number. But anyway, for our purposes,
we don’t want to know about the number of neutrons in the nucleus. But rather, how much does the
mass number of the nucleus change. And this change, as we saw,
happens as a result of neutron emission.
Now, since the mass number of
any nucleus, including the unstable nucleus we have here, is equal to the number
of protons plus the number of neutrons in the nucleus. That means if we subtract away
a neutron — as a result of neutron emission, like we did here — then that mass
number will decrease by one. That’s because we’ve kept the
same number of protons, but we’ve lost a neutron. And that, then, is our answer
to this question. When an unstable nucleus emits
a neutron, its mass number decreases by one.
Now, let’s summarize what we’ve
learned about neutron emission. Starting off, we saw that neutron
emission is a form of radioactive decay, where a nucleus gives off one or more
neutrons. We saw that representing neutron
emission in a nuclear equation involves using a lower case n to represent a
neutron. And it has an atomic number of zero
and a mass number of one.
Based on this, we saw that emitting
a neutron does not change the atomic number of the emitting nucleus, but it does
change the mass number. We saw further that graphs called
nuclear decay graphs depict nuclear transitions, including neutron emission. And lastly, we saw that neutrons,
as emitted particles, can penetrate farther than alpha or beta particles. And they can create radioactive
material through a process called neutron activation.