& Measurement of Radioactivity
All substance are made of atoms. These have electrons (e) around the outside, and a nucleus in the middle. The nucleus consists of protons (p) and neutrons (n), and is extremely small. (Atoms are almost entirely made of empty space!). In some types of atom, the nucleus is unstable, and will decay into a more stable atom. This radioactive decay is completely spontaneous. You can heat the substance up, or subject it to high pressure or strong magnetic fields - in fact, do whatever you like to it - and you won't affect the rate of decay in the slightest. When an unstable nucleus decays, there are three ways that it can do so. It may give out:-
· an alpha particle (we use the symbol α)
· a beta particle (symbol β)
· a gamma ray (symbol γ)
Many radioactive substances emit α particles and β particles as well as γ rays.
Alpha particles are made of 2 protons and 2 neutrons. This means that they have a charge of +2, and a mass of 4 (the mass is measured in "atomic mass units", where each proton & neutron=1). Alpha particles are relatively slow and heavy. They have a low penetrating power - you can stop them with just a sheet of paper. Because they have a large charge, alpha particles ionize other atoms strongly and have a range of only a few centimetres in air.
Alpha particles are made of 2 protons with 2 neutrons. This means that when a nucleus emits an alpha particle, it loses 2 protons and so its atomic number decreases by 2. Also, when a nucleus emits an alpha particle, its atomic mass decreases by 4 (that's 2 protons plus 2 neutrons). So Americium-241 ( an α -source used in smoke detectors), which has an atomic number of 95 and an atomic mass of 241 will decay to Neptunium-237 (which has an atomic number of 93 and an atomic mass of 237). The equation would look like this:-
Alpha-decay occurs in very heavy elements, for example, Uranium and Radium. These heavy elements have too many protons to be stable. They can become more stable by emitting an alpha particle.
Beta particles have a charge of minus 1, and a mass of about 1/2000th of a proton. This means that beta particles are the same as an electron. They are fast, and light. Beta particles have a medium penetrating power - they are stopped by a sheet of aluminium or plastics such as perspex. Beta particles ionise atoms that they pass, but not as strongly as Alpha particles do.
It appears strange that when the nucleus contains protons and neutrons, how can an electron come out of a nucleus?
To answer this, we need to know more about protons and neutrons:
Protons & neutrons are made of combinations of even smaller particles, called "quarks". Under certain conditions, a neutron can decay, to produce a proton plus an electron. The proton stays in the nucleus, whilst the electron flies off at high speed.
Beta decay occurs in very "neutron-rich" elements, for example, Strontium-90 and Iodine-130. These elements are typically created in nuclear reactors.
These elements have too few protons and too many neutrons to be stable. They can thus become more stable by emitting a beta particle.
particles have a charge of -1, and weigh only a tiny fraction of a neutron or
proton. As a result, β particles interact less readily with other atoms
than alpha particles.
Gamma rays are waves, not particles. This means that they have no mass and no charge. Gamma rays have a high penetrating power - it takes a thick sheet of metal such as lead, or concrete to reduce them significantly. Gamma rays do not directly ionise other atoms, although they may cause atoms to emit other particles which will then cause ionisation.
Gamma rays (γ) are electromagnetic waves, rather like X rays and radio waves. Thus gamma rays have no mass and no charge.
After a nucleus has emitted an α-particle or a β-particle, it may still have too much energy: we say it is in an "excited state". It can get rid of this energy by emitting a pulse of very high frequency electromagnetic radiation, called a gamma ray. Gamma rays do not pull electrons off atoms they pass, as α-particles and β-particles do. This means that they do not lose much energy as they travel, as they do not interact as much with the matter they pass. Therefore, gamma rays have a high penetrating power, and a very long range.
It's worth noting that there is no such thing as a pure γ-ray source. Gamma rays are given off by most α-emitters and β-emitters. If we want a source of pure gamma rays, we can get it by using a substance that emits both β and γ, and simply keep it in an aluminium container that stops the β-particles.
Useful gamma sources include Technetium-99m, which is used as a "tracer" in medicine. This is a combined β and γ source, and is chosen because betas are less harmful to the patient than alphas (less ionisation) and because Technetium has a short half-life (just over 6 hours), so it decays away quickly and reduces the dose to the patient. In Gamma decay, both atomic number and atomic mass remain unchanged.
some forms of electromagnetic energy, such as light and heat, can be detected by
the human senses. One of the greatest draw backs to high energy radiation is the
inability to detect it. We cannot see, feel, taste, smell, or hear the various
forms of ionizing radiation. Fortunately, ionizing radiation interacts with
matter which makes detection and measurement possible by utilizing specialized
equipment. In this section we want to introduce you to the various ways and
means of detecting and measuring ionizing radiation.
discovered radioactivity because it left marks on photographic film. However,
there are more definitive means commonly used by scientists and technicians who
study and work with radiation. The equipment utilized for the detection and
measurement of radiation commonly employs some type of substance or material
that responds to radiation. Many common methods use either an ionization process
or molecular excitation process as a basis. Remember that radiation interacts
with matter. For detection and measurement purposes the process of ionization is
the most commonly employed technique, based on the principle of charged
particles producing ion pairs by direct interaction. These charged particles may
collide with electrons, which remove them from their parent atoms, or transfer
energy to an electron by interaction of electric fields.
How do you choose a detection
considerations for choosing a particular type of detection device include the
application, the type of radiation, the energy of the radiation, and the level
of sensitivity needed. Remember from previous discussion that radiation exists
as waveforms with varying energies and may be either particulate or
electromagnetic in nature.
are three types of radiation detection devices:
o The Electroscope
Marie Curie used an electroscope to study the radioactivity or Uranium ores. The electroscope is a fairly simple device comprised of a metal rod with two thin leaves attached to one end. If the electroscope is given a negative charge, the metal leaves will separate from each other. It is this characteristic that makes the electroscope useful as a detection device. A negatively charged electroscope will discharge when ions in the air remove electrons from it, and consequently, a positively charged electroscope will discharge when it takes electrons from the air around it. The rate of discharge of the electroscope is a measure of ions in the air and can be used as a basis of measurement and detection.
THE CLOUD CHAMBER
A unique device for detection and measurement is the Cloud Chamber, invented by the British physicist Charles Wilson in 1911. The Cloud chamber makes it possible to visually see the path of ionizing radiation thus making it possible to photograph it. The cloud chamber consists of a plastic or glass container, which sits on dry ice. A dark cloth is saturated with alcohol and placed around the inside of the container near the top. A small radioactive material may be suspended from the lid of the container. In the chamber, the alcohol evaporates from the cloth and condenses as it reaches the cold region created by the dry ice at the floor of the container. Just above the floor of the chamber there is a region where the alcohol vapor does not condense unless there are seeds around, so that drops of alcohol can form. This condition is similar to that of seeding clouds with a chemical to form rain. The idea is that only seeds available in the chamber are those of ions produced by the interaction with radiation. The resulting trail of alcohol droplets can be seen against the black background in the bottom of the chamber.
These are only a few of the devices commonly utilized for purposes of detection and measurement of radioactivity and radiation. It is important to understand that when working with radioactivity/radiation, due to our inability to sense radiation, we need them to assist us in detecting the presence of radiation and we also need them to help monitor the radiation.
OTHER DETECTION DEVICES
Another common device used for detection and measurement is the ionization chamber. The Geiger counter, survey meter, and personal dosimeters work on the basis of the ionization chamber. The principle operation of an ionization chamber is that it will produce an electric current in the presence of a radioactive source. Ionization chambers consist of tubes filled with gas, such as argon. When radiation enters the tube and interacts with the gas, it removes electrons from the gas. The gas atoms become positively charged ions, and the free electrons move through the gas to a wire in the tube, setting up a current. The current is commonly amplified and sent to a recording or counting device. This in response may produce a flash of light, ticking sounds, or an analog readout. Ionization chambers are capable of measuring the amount of radiation by means of measuring the amount of current produced.
For measuring radioactivity, three types of devices are available:
1. Gas-filled tube counters e.g. the Geiger Muller Counter
2. Scintillation Counters
3. Semi-conductor Detectors
1. The Geiger Counter: A potential difference just below that required to produce a discharge is applied to the tube (1000 V). Any atoms of the gas struck by the γ-rays entering the tube are ionized, causing a discharge. Discharges are monitored and counted by electronic circuitry and the output is reported as counts/sec or Rontgens/hr or mR/hr.
2. Scintillation Counters: Crystals of certain substances e.g. cesium fluoride, cadmium tungstate, anthracine and sodium iodide emit small flashes of light when bombarded by γ-rays. The most commonly used phosphor in scintillation counters is NaI with a minute quantity of thallium added. In the instrument, the crystal is positioned against a photocell which in turn is linked to a recording unit. The number of flashes produced per unit time is proportional to the intensity of radiation. Small portable scintillation counters are available.
3. Semi-Conductor Detectors: A semi-conductor is a substance whose electrical conductivity is between that of a metal and an insulator. It is noted that Ge(Li) semi-conductors ate excellent detectors of γ-rays with a resolution ten times higher than NaI (Th) scintillometers. The main disadvantage of these is a lower efficiency for higher energy x-rays. Besides, Ge(Li) semi-conductors need to be cooled by liquid nitrogenand are hence cumbersome and not suitable as field instruments.
Besides the above there are instruments known as γ-ray spectrometers, which can distinguish different energy peaks and hence make it possible to identify the source of radiation.
A Geiger counter will record "counts per minute", but this doesn't tell us what the radioactive substance is actually doing, merely what is reaching the detector. It also tells us nothing about the amount of damage being done to you. Thus we need several different units in order to measure radioactivity.
Units of Measuring Radioactivity:
There are three measurement units for radioactivity: the Becquerel measures radioactivity, the Gray measures the absorbed dose and the Sievert measures the biological effects.
This is a very small unit, and multiples are often used:
1 MBq = 1 mega Becquerel = 1,000,000 Bq
1 GBq = 1 giga Becquerel = 1,000,000,000 Bq
1 TBq = 1 tera Becquerel = 1,000,000,000,000 Bq
The radioactivity of an environment, a material or a foodstuff is given in Becquerels per kilogram or per liter.
1 Gy = 1 joule per kilogram
Sub-multiples are often used:
1 mGy = 1 milligray = 0.001 Gy
1 μGy = 1 microgray = 0.000001 Gy
1 nGy = 1 nanogray = 0.000000001 Gy
Contrary to the Becquerel, the sievert is a very large unit, and we often use sub-multiples:
1 mSv = 1 millisievert = 0.001 Sv
1 µSv = 1 microsievert = 0.000001 Sv
· To measure the harm done to you, we need to remember that α particles ionise very strongly, and cause 20 times more cell damage than the same dose of β particles, γ rays or X-rays. We measure the "dose equivalent" in sieverts (Sv).
· A dose of 1 gray of β-particles, γ-rays or X-rays will give you a dose equivalent of 1 sievert. A dose of 1 gray of α-particles will give you a dose equivalent of 20 sieverts
Some of the
principle safety precautions commonly used in working with
radioactivity/radiation are time, distance, and shielding. Recall our earlier
discussion of the dentist wanting to photograph your teeth. Have you ever
wondered why the dentist lays a heavy apron across your chest? The dentist is
practicing a means of protection from exposure. In that, they are using distance
and shielding from the source of radiation. The concepts of these three
principles are fairly simple. The first principle is time. The less time you
spend around a radioactive material the less exposure you will receive. The
second principle states that the greater the distance away from a radioactive
source the lesser your exposure to the radiation. Lastly, if you can protect
yourself with some type of material to act as a shielding device you will also
reduce your overall exposure.
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Department of Geology
Aligarh Muslim University, Aligarh - 202 002 (India)