Radioactivity
SPECIFIC OBJECTIVES
To be able to distinguish the three types of radiation; to understand the
way in which the intensity of radiation changes with
- time - radioactive decay and half-life
- distance from the source - the inverse square law
- intervening material - the absorption law
EQUIPMENT
Geiger counters; alpha, beta, and gamma radioactive sources;
cardboard, aluminum, and lead sheets; dice.
BACKGROUND
The atom is composed of a small heavy nucleus, containing protons and
neutrons, surrounded by light electrons. The protons are positively charged;
the neutrons are neutral; and the electrons are negatively charged. In
electrically neutral atoms, the number of protons in the nucleus is the same
as the number of electrons. Since the electrons determine all the chemical
properties of the substance, and since the number of electrons is determined
by the number of protons, every substance with unique chemical characteristics
(element) is distinguished by the number of protons. Changing the number of
protons in the nucleus is equivalent to changing the element.
The nucleus is positively charged since the protons have positive electric
charge and the neutrons are neutral. Why don't the protons repel each other
and fly apart? The neutrons bind the protons together with the strong
nuclear force, which is stronger than the Coulomb electrical repulsion, at
least for the smaller nuclei. Most of the lighter elements have an equal
number of protons and neutrons, but many of the heavier elements tend to
have more neutrons than protons. For example, the most common form of
uranium has 92 protons and 146 neutrons. Eventually, the neutrons are not
able to supply enough nuclear "glue" to keep larger numbers of protons from
flying apart.
Atoms with the same number of protons but different numbers of neutrons are
called isotopes. There are many more unstable isotopes than
stable ones.
More than 99.999% of the atomic nuclei in objects around you are stable,
that is, they do not decay. Some nuclei, however, are unstable. The
process of spontaneous change, and the associated emission of energetic
particles, is called radioactivity, or radioactive decay.
The three types of radiation that we will study are:
- alpha rays which are two protons and two neutrons bound tightly
to each other (a helium-4 nucleus),
- beta rays which are simply electrons, and
- gamma rays which are very high energy photons.
In alpha decay, the unstable nucleus throws off a chunk of itself. Since the
chunk contains two protons, the decay product is a different element.
In beta decay, one of the nuclear neutrons is converted into a proton, an
electron, and another particle called a neutrino which is extremely difficult
to detect. The proton remains in the nucleus and the electron is ejected as
a beta ray. Since the number of protons has increased, the decay product
is a new element.
In gamma decay, the unstable nucleus shifts from a high energy state to
a lower energy state. The difference in energy is carried away by a photon,
the same particles that make up visible light. The nuclear energy shifts
are so large, however, that the photons are much more energetic than visible
light or even X-rays. Since the number of protons in the nucleus has not
changed, the decay product is the same element, but in a more stable form.
Radioactive Decay and Half-life
Similar to a batch of popcorn, it is impossible to determine when a
particular radiaoactive atom will decay. What can be measured is how
long it takes on average for one half of a large sample of atoms to
decay. The term half-life describes this length of time; it may be
measured in any unit of time from seconds to years. For example, a
radioactive sample with a half-life of 20 minutes contains 1,000,000 atoms
at time zero. After 20 minutes, 500,000 (on average) will remain. After an
additional 20 minutes, 250,000 (on average) will remain, and so on.
The radioactive decay law is
I(t) = Io 2^(-t / T½ )
where Io is the intensity of the radiation at time zero,
I(t) is the intensity of the radiation after time t,
and T½ is the half-life of the sample.
The Inverse Square Law
In the absence of absorption (see below), the alpha, beta, and gamma rays
resulting from the decay of a sample of unstable nuclei speed away from the
sample uniformly in all directions. Imagine two mathematical spheres with
the sample at the center of both spheres and one sphere having twice the
radius of the other. All the particles that penetrate the inner sphere will
also penetrate the outer sphere (because none are absorbed). However, the
number of particles per square centimeter at the outer sphere will be lower
because the particles spread out. In fact, the intensity will be lower by
the ratio of the area of the two spheres. The inverse square law for
radiation is a result of geometry in three dimensions. The intensity is
inversely proportional to distance squared from the source:
I = A / d2
where I is the intensity of the radiation, A is a proportionality
constant, and d is the distance from the source.
The Absorption Law
Nuclear radiation is absorbed by various materials at different rates.
However, it has been determined experimentally that all radiation is absorbed
by all materials in a similar manner. The absorption law is
I(x) = Io 2^(-x / D½ )
where Io is the intensity of the radiation falling on the
material, I(x) is the intensity of the radiation transmitted through
thickness x of the absorbing material,
and D½ is the half-thickness of the material.
The half-thickness of a material is defined to be the amount of
material which will absorb one half of the incident radiation.
The Geiger Counter
consists of a metal-coated cylindrical tube filled with an inert gas like
argon and a wire running through its center. The tube and wire are held at a
large potential difference (roughly 1000 volts). Normally, the potential
difference is not enough for a spark to jump from the wire to the metal wall
of the tube. However, when an alpha, beta, or gamma ray passes through the
tube, the radiation ionizes the gas in the tube creating free electrons,
and a spark jumps easily through the ionized gas. When a voltage pulse is
detected, the Geiger counter gives an audible "click" (familiar from very
bad 1950's science fiction movies). The counter also has a needle scale for
measuring large rates of clicks, too fast for humans to count.
The Geiger counter measures the intensity (I) of radiation in units called
CPM for "counts per minute".
Cosmic Ray Background
The Earth is constantly bombarded by cosmic rays (mostly very high energy
protons) with origins outside the Solar System. When the cosmic rays
encounter the Earth's atmosphere they create "showers" of secondary
particles, some of which reach the Earth's surface. One secondary particle
with a large penetrating power is the muon which can travel through several
feet of concrete and steel. Since the basement laboratory is not an
effective shield against these particles, we account for this cosmic ray
background by counting the average number of particles that pass
through the Geiger tube when no radioactive sources are present. When
sources are present, the background count is subtracted from the measurement.
The difference is the number of particles coming solely from the radioactive
source.
PROCEDURE
Radioactive Decay and Half-life
Radioactive sources that are safe to handle generally have long
half-lives. For example, uranium-238 has a half-life of 4.5 billion years.
The exponential decay in the number of counts per minute would not be
observable in the three-hour lab period. Sources with a half-life of a
few minutes can be observed in the lab period, but are very dangerous to
handle. For this reason, we use a model of radioactive decay.
- Count the total number of dice in the container.
- If the dice represent radioactive atoms about to decay, then after
one half-life one half of the atoms will remain. After two half-lives
one quarter of the initial number will remain. Plot the theoretical
number of atoms which have not yet decayed versus the number of half-lives.
- Spill the dice on the table. Remove all the dice showing even
numbers from the experiment (they represent atoms that have decayed).
- Count and record the number of odd dice, put them back in the
container, randomize, and spill these dice on the table.
- Repeat until all the dice are gone (until all the atoms have decayed).
- Plot the experimental points on the same graph as the theoretical
curve. Notice the statistical fluctuations from theory.
The Inverse Square Law
- Plug in and turn on the larger Geiger counter with the vertical scale.
- Depress and hold the red button to read the tube voltage. Set the tube
voltage to the value marked on the counter. This may require periodic
adjustment during the experiment.
- Set the range selector to the scale that is most appropriate for your
measurement, that is, the scale with the lowest fractional error.
Re-read Lab 0 to refresh your memory.
- Set the response control to slow. The Geiger counter can average
the number of counts over a short time for quick but imprecise readings; the
needle will jump about with statistical fluctuations in the CPM. We will use
the slow response setting which requires a longer period for the counter to
average the data, but the final reading will be more precise; the needle will
not bounce erratically.
- Remove any sources from the immediate vicinity of the Geiger counter.
Take a background count by ear for three minutes. Divide by three to
get an average background CPM. This value must be subtracted from all
measurements taken with this meter.
- Place the beta source (green disk) on the vertical scale using the magnetic
mount. The radioactive sample is embedded in the green disk so that radiation
is emitted in a roughly cone-shaped pattern through the hole in the aluminum
bracket. Thus, the green disk should be on the top side of the bracket.
- Align the window of the Geiger tube so that the radiation can enter the
tube. The window should face upward and be centered on the vertical scale.
- Record the CPM at various distances. Remember to subtract the background
count. If the count drops too low for an accurate meter reading, take the
count by ear.
- Make a plot of Intensity (vertical axis) vs. 1 / distance2
(horizontal axis), taking more data where the graph appears sparse.
The Absorption Law
- Turn on the smaller Geiger counter.
- Carefully remove the red plastic window from the end of the probe.
- We will study the absorption of three types of radiation (alpha,
beta, and gamma) by three materials (cardboard, aluminum, and lead).
- Remove any sources from the immediate vicinity of the Geiger counter.
Take a background count by ear for three minutes. Divide by three to
get an average background CPM. This value must be subtracted from all
measurements taken with this meter. The background count from the previous
exercise can not be used here because the two counters have different
sensitivities.
- From the last exercise, we know that the intensity of radiation varies
with distance from the source. Therefore, to study only the effect of
absorbing material without distance dependence, be certain that the distance
between the source and the Geiger tube does not vary. A good technique is
to start with the maximum amount of material between the source and probe
so that the smallest possible distance (greatest possible intensity) can be
used, and then to remove sheets of the absorbing material. A little
experimentation will tell you the largest interesting number of sheets.
- Make a plot of Intensity (vertical axis) vs. number of sheets of
absorber (horizontal axis) for each case, 9 plots in all.
Analysis
Radioactive Decay and Half-life
- A particular isotope has a half-life of five days. A sample is known to
have contained one million atoms when it was prepared, but now only 100,000
atoms remain. How long ago was the sample prepared?
The Inverse Square Law
- Your plot of I vs. 1 / d2 should be linear for large values
of d (small values of 1 / d2), but it may level off for small
values of d (large values of 1 / d2). Explain this behavior.
Hint: Remember that the radiation is emitted through the hole in the aluminum
bracket in a cone. A diagram of the cone and the Geiger tube window may help.
The Absorption Law
- From your plots in the absorption experiment, determine the half-thickness
of each of the three materials for each of the three types of radiation.
Don't forget your two random and two systematic error sources.
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