Attenuation of X-rays

 


The percentage of X-ray energy absorbed by the material is due to a process known as electron ionisation , this is dependent upon the material density and atomic number. As a result the detected X-ray attenuation provides a picture of the absorbed energy on the irradiated objects. Due to the absorbed energy being relative to the atomic number, it can be used in the material discrimination process.

Generally the lower the atomic number the more transparent the material is to the X-rays. Materials composed of elements with a high atomic numbers absorb radiation more effectively causing less dark shadows in an X-ray image. Substances with low atomic numbers absorb less X-ray radiation, hence their shadowgraph appears a darker colour.

The absorption of the X-ray radiation by a material is proportional to the degree of X-ray attenuation and is dependent on the energy of the X-ray radiation and the following material parameters:

thickness;
density;
atomic number;

The attenuation or absorption, usually defined as the linear absorption coefficient, µ, is defined for a narrow well-collimated, monochromatic x-ray beam. The linear absorption coefficient is the sum of contributions of types of attenuation as listed below.
Mass attenuation coefficient is defined as the linear attenuation coefficient divided by the density of the medium. For a given incident gamma ray energy, the mass attenuation coefficient is independent of the physical and chemical state of the absorber. Thus, the mass attenuation coefficient is the same for water whether present in liquid or vapor form
 


Interactions of X-Rays with Matter

The dependence of the X-ray attenuation on the atomic number relies on mainly on three phenomena: photoelectric effect, Compton effect and pair production;

The photoelectric effect is predominant at low X-ray energies and with high atomic numbers. When a quantum of radiation strikes an atom, it may impinge on an electron within an inner shell and eject it from the atom. If the photon carries more energy than is necessary to eject the electron, it will transfer this residual energy to the ejected electron in the form of kinetic energy

 

The Compton effect occurs primarily in the absorption of high X-ray energy and low atomic numbers. The effect takes place when high X-ray energy photons collide with an electron. Both particles may be deflected at an angle to the direction of the path of the incident X-ray. The incident photon having delivered some of its energy to the electron emerges with a longer wavelength. These deflections, accompanied by a charge of wavelength are known as Compton scattering.

Pair production is the formation or materialization of two electrons, one negative and the other positive (positron), from a pulse of electromagnetic energy traveling through matter, usually in the vicinity of an atomic nucleus. Pair production is a direct conversion of radiant energy to matter. It is one of the principal ways in which high-energy gamma rays are absorbed in matter. For pair production to occur, the electromagnetic energy, in a discrete quantity called a photon, must be at least equivalent to the mass of two electrons. The mass m of a single electron is equivalent to 0.51 million electron volts (MeV) of energy E as calculated from the equation formulated by Albert Einstein, E = mc2, in which c is a constant equal to the velocity of light. To produce two electrons, therefore, the photon energy must be at least 1.02 MeV. Photon energy in excess of this amount, when pair production occurs, is converted into motion of the electron-positron pair. If pair production occurs in a track detector, such as a cloud chamber, to which a magnetic field is properly applied, the electron and the positron curve away from the point of formation in opposite directions in arcs of equal curvature. In this way pair production was first detected (1933). The positron that is formed quickly disappears by reconversion into photons in the process of annihilation with another electron in matter.


 


Two less important (In diagnostic energy levels) effects

Thomson scattering (R), also known as Rayleigh, coherent, or classical scattering, occurs when the x-ray photon interacts with the whole atom so that the photon is scattered with no change in internal energy to the scattering atom, nor to the x-ray photon. Thomson scattering is never more than a minor contributor to the absorption coefficient. The scattering occurs without the loss of energy. Scattering is mainly in the forward direction.

Photodisintegration (PD) is the process by which the x-ray photon is captured by the nucleus of the atom with the ejection of a particle from the nucleus when all the energy of the x-ray is given to the nucleus. Because of the enormously high energies involved, this process may be neglected for the energies of x-rays used in radiography.



Absorption Edges

If the mass absorption coefficient of a material is plotted against wavelength as shown in Figure Y for a monochromatic x-ray beam, mm shows sharp discontinuities at particular wavelengths.

Fig Y

 

These correspond to the ionisation energy of a K shell electron and indicate the increased probability of photoelectric absorption, however this drops sharply as the difference between the photon and electron binding energy increases. The variation of mm with photon energy E and atomic number Z for the various scattering and absorption processes is summarised in the following table and shown graphically in figure X:                            

                                 

                                Summary of Main Attenuation Mechanisms

Mechanism

Variation of mm with E

Variation of mm with Z

Energy range in tissue

Rayleigh

       µ 1 / E

        µ  Z2

1 - 30 keV

photoelectric

       µ 1 / E3

        µ  Z3

1 - 100 keV

Compton

falls gradually with E

     independent

0.5 - 5 MeV

pair production

rises slowly with E

        µ  Z2

> 5 MeV

 

The relative Importance of Attenuation processes
Only photoelectric effect and Compton effect are significant in the production of diagnostic radiographic images
 

Figure X

http://img.cryst.bbk.ac.uk/www/kelly/medicalxrays.htm


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