
- •3. What is Radioactivity?
- •1. Ionizing radiation
- •2. Radioactive Elements
- •3. The Nature of Radiation
- •4. Alpha radiation
- •5. Beta and gamma radiation
- •6. What is an isotope?
- •7. The Radioactive Series
- •8. The Energy of the Radiation
- •8.1. Description of a Radioactive Source
- •8.2. Alpha Radiation
- •8.3. Beta Radiation
- •8.4. Gamma Radiation
- •9. The Penetration of Radiation
- •10. Ionization. Excitation.
- •Control points to Charter 3
- •Science vocabulary
8. The Energy of the Radiation
In order to detect radioactivity and to evaluate the biological effect of the radiation it is important to have information about the energy as well as the type of radiation emitted. The unit used for energy is the electron volt (abbreviated eV). By definition, an electron volt is the energy attained by an electron when it is accelerated through a voltage gap of 1 volt. The product of voltage and the electron charge (given in Coulombs, C) gives the relation between electron volt and a unit of energy, the joule (J):
1 eV = 1 V · 1.6 · 10-19 C = 1.6 · 10-19 J.
The electron volt is a very small unit. The energy usually set free by disintegration varies from a few thousand electron volts (keV) to approximately 6 million electron volts (MeV).
8.1. Description of a Radioactive Source
How is a radioactive source described? The intensity of the source depends on the number of atoms that disintegrate per second (i.e. the number of becquerels). Other parameters are: type of radiation, half-life (the half-life period is the time during which the quantity of atoms of a radioactive isotope decreases twice), and energy of the radiation. All these parameters can be given by a decay scheme. For example, the radioactive isotope Cs-137, which is the most important radioactive waste product from a nuclear reactor, has the decay scheme given in Figure 3.3.
A decay scheme is another way physicists use to convey information. The scheme tells us about the types of radiation emitted, the energy involved, half-life, etc. This type of information is necessary in calculating radiation doses and risks.
FIG. 3-3.
A scheme for the disintegration of Cs-137. The state of the nucleus is given by horizontal lines. The atomic number increases left-to-right, Cs is 55 and Ba is 56. The vertical scale is the energy of the nucleus, given in MeV. The vertical distances between the lines indicate the energy difference. This energy is set free by disintegration, appearing as β-particle or γ-ray.
The decay scheme shows that Cs-137 is transformed into the stable barium isotope Ba-137. This can take place via two different routes:
In 94.6% of the disintegrations a β-particle is emitted with an energy of 0.512 MeV (106 eV), followed immediately by a γ-ray with an energy of 0.662 MeV.
In 5.4% of the disintegrations the stable barium isotope is reached directly by emitting only a β-particle, with energy of 1.174 MeV.
The decay scheme also shows that the half-life of Cs-137 is 30 years. In addition, one might guess that Cs-137 can be observed by measuring the emitted γ-rays. γ-rays are easy to detect because they are very penetrating, a quality that is described at the end of this chapter.
8.2. Alpha Radiation
The energy of α-particle, when it is emitted by a nucleus, is usually a few MeV. Some of the properties which are characteristic of α-particles are:
The α-particles from one particular radioactive source have the same energy. For example α- particles from U-238 always have a starting energy of 4.19 MeV.
When α-particle passes through a material, іt rapidly loses energy through numerous collisions with the electrons that make up the atoms and molecules. Because the collisions produce ionizations, a high density of ions is deposited in the material tracing out a linear track. The energy of the α-particle is ultimately dissipated by this large number of low energy interactions and it stops at the end of the track.
The energy deposited per unit length of the track is called the linear energy transfer (abbreviated LET). An example is given in Figure 3.4. The range of α-particle from a radioactive source is very short in animal tissue and in air the range is only a few centimeters. As can be seen from Figure 3.4 the energy loss along the track is not constant but gradually increases toward the end of the track.
The use of heavy particle beams offers potential advantages in cancer therapy. If the "Bragg peak" lands on the tumor, the tumor dose is larger than the dose to the surrounding healthy tissue. The goal is to maximize damage to the tumor while minimizing damage to healthy tissue.
FIG. 3-4.
The energy deposition along the track of α -particle.