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Physical Principles of Electron Microscopy: An Introduction to TEM ...

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The Scanning <strong>Electron</strong> Microscope 135<br />

emitting visible-light pho<strong>to</strong>ns when bombarded by charged particles such as<br />

electrons. The number <strong>of</strong> pho<strong>to</strong>ns generated by each electron depends on its<br />

kinetic energy Ek (= eVs) and is <strong>of</strong> the order 100 for Vs � 10 kV. The<br />

scintilla<strong>to</strong>r material has a high refractive index, so advantage can be taken <strong>of</strong><br />

<strong>to</strong>tal internal reflection <strong>to</strong> guide the pho<strong>to</strong>ns through a light pipe (a solid<br />

plastic or glass rod passing through a sealed port in the specimen chamber)<br />

<strong>to</strong> a pho<strong>to</strong>multiplier tube (PMT) located outside the vacuum.<br />

The PMT is a highly sensitive detec<strong>to</strong>r <strong>of</strong> visible (or ultraviolet) pho<strong>to</strong>ns<br />

and consists <strong>of</strong> a sealed glass tube containing a hard (good-quality) vacuum.<br />

The light-entrance surface is coated internally with a thin layer <strong>of</strong> a material<br />

with low work function, which acts as a pho<strong>to</strong>cathode. When pho<strong>to</strong>ns are<br />

absorbed within the pho<strong>to</strong>cathode, they supply sufficient energy <strong>to</strong> liberate<br />

conduction or valence electrons, which may escape in<strong>to</strong> the PMT vacuum as<br />

pho<strong>to</strong>electrons. These low-energy electrons are accelerated <strong>to</strong>ward the first<br />

<strong>of</strong> a series <strong>of</strong> dynode electrodes, each biased positive with respect <strong>to</strong> the<br />

pho<strong>to</strong>cathode.<br />

At the first dynode, biased at 100 � 200 V, the accelerated pho<strong>to</strong>electrons<br />

generate secondary electrons within the escape depth, just like primary<br />

electrons striking an SEM specimen. The dynodes are coated with a material<br />

with high SE yield (�) so that at least two (sometimes as many as ten)<br />

secondary electrons are emitted for each pho<strong>to</strong>electron. The secondaries are<br />

accelerated <strong>to</strong>ward a second dynode, biased at least 100 V positive with<br />

respect <strong>to</strong> the first, where each secondary produces at least two new<br />

secondaries. This process is repeated at each <strong>of</strong> the n (typically eight)<br />

dynodes, resulting in a current amplification fac<strong>to</strong>r <strong>of</strong> (�) n , typically � 10 6 for<br />

n = 8 and ��4.<br />

Figure 5-8. A typical scintilla<strong>to</strong>r/PMT (Everhart-Thornley) detec<strong>to</strong>r, employed for secondaryelectron<br />

imaging in the SEM. From Reimer (1998), courtesy <strong>of</strong> Springer-Verlag.

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