Interaction of Beta Radiation with Matter

The transformation of the nuclei and the electron orbitals may result in electron emission. As discussed in Section 4.4.2, the negative or positive particles (namely, electrons or positrons following the transformation of the nuclei) are called nega­tive or positive beta radiation, respectively, and they have continuous spectra. The transformation of the atomic orbital can also produce electrons, as discussed in Section 4.4.3. These electrons, such as Auger and conversion electrons, have dis­crete energy. In addition, electromagnetic radiation can produce photo, Compton, and pair electrons, as discussed in Section 5.4.

The rest mass of the beta particle is 0.51 MeV, which is much less than the rest mass of the alpha particle. Therefore, at the same energy of the radiation, the veloc­ity of the beta particle is much higher than that of the alpha particle. Because of the high velocity, the relative increase in the mass often has to be taken into account.

When beta radiation interacts with matter, the electrons in the matter may get excited or ionized, and the direction of the pathway of the beta particle may change as a result of elastic and inelastic collisions. In addition, the kinetic energy is partly or totally transmitted to the matter. When the beta particles interact with the nuclear field, Bremsstrahlung is emitted, which has a continuous spectrum. The inner Bremsstrahlung has been discussed in Section 4.4.3.

The beta particles can be scattered and absorbed, eventually losing all their energy (Table 5.4).

Table 5.4 Interaction of Beta Particles with Matter

Reacting Particles and Fields

Changes

In Radiation

In Matter

Orbital electron Nuclear field Nucleus

Bremsstrahlung, scattering, absorption

Bremsstrahlung, scattering, absorption No interaction

Excitation, ionization, chemical change

Source: Adapted from Kiss and Vertes (1979), with permission from Akademiai Kiado.

Подпись: Detected energy (keV) 400 600 800 1000 1200 600 800 1000 1200 1400 1600 Figure 5.10 Measured and simulated RBS spectra taken on oxidized SiC at scattering angles of 165° and 97°. Each sample was measured at least at two different tilt angles. For the composition, Si:O ratio of 1:2 was determined for each sample. The arrows represent the surface positions of the elements. (Thanks to Dr. E. Szilagyi, KFKI Research Institute for Particle and Nuclear Physics, Budapest, Hungary, for the spectra.) Source: Reprinted from Szilagyi et al. (2008), with permission of the American Institute of Physics.