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X-Ray Fluorescence Analytical Techniques - CNSTN : Centre ...

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decelerated as they penetrate the material of target, and such a high negative acceleration<br />

should produce a pulse of radiation.<br />

Figure I.5: On the left, the classical model showing the production of Bremsstrahlung.<br />

On the right, the Continuum X-ray emission spectrum.<br />

The probability of radiative energy loss (Bremsstrahlung) is roughly proportional to<br />

q 2 z 2 T/M0 2 , where q is the particle charge in units of the electron charge e, Z is the atomic<br />

number of the target material, T is the particle kinetic energy, and M0 is the rest mass of the<br />

particle. Because of the fact that protons and heavier particles have large masses, compared to<br />

the electron mass, they irradiate relatively little, e.g., the intensity of continuous X-rays<br />

generated by protons is about four orders of magnitude lower than the generated by electrons.<br />

The ratio of energy lost by Bremsstrahlung to that lost by ionization can be<br />

approximated by:<br />

2<br />

⎛ m0<br />

⎞ ZT<br />

⎜<br />

M ⎟<br />

2<br />

⎝ 0 ⎠ 1600 m0<br />

c<br />

where m0 is the rest of the electron.<br />

III.6.2 Characteristic Emission<br />

, (I.6)<br />

The purpose of X-ray fluorescence is to determine chemical elements both qualitatively<br />

and quantitatively by measuring their characteristic radiation. To do this, the chemical<br />

elements in a sample must be caused emit X-rays. As characteristic X-rays only rise in the<br />

transition of atomic shell electron to lower, vacant energy levels of the atom, a method must<br />

be applied that is suitable for releasing electrons from the innermost shell of an atom. This<br />

involves adding to the inner electrons amounts of energy that are higher than the energy<br />

bonding them to the atom.<br />

This can be done in a number ways:<br />

• Irradiation using elementary particles of sufficient energy (electrons, protons, a-particles…)<br />

that transfer the energy necessary for release to the atomic shell electrons during collision<br />

processes.<br />

• Irradiation using X- or gamma rays from radionuclides.<br />

• Irradiation using X-rays from an X-ray tube.

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