There exist a number of PMT dynode structures,
each with their typical characteristics. Important PMT parameters are :
- Amplification
as a function of voltage
- Dark current
- Pulse rise
time
- Physical size
- Gain
stability
- Radiological
background
Gain, stability and dark current
depend on the used dynode materials and are a function of temperature. Pulse rise time
depends on the dynode structure. For fast timing applications, so called "linear
focused" PMTs are advised.
A very important factor is the
sensitivity as a function of the position on the PMT entrance window. A large variation
can cause a degradation of the energy resolution of a scintillation detector. This
variation can be caused by a change in quantum efficiency of the photocathode or a
non-uniform photoelectron collection efficiency from the cathode onto the first dynode.
The above effects can be important for both small and large diameter PMTs.
From Table
3.1 it is clear that each type of scintillator has a different emission spectrum. It
is important for a good performance that the emission spectrum of a scintillator is well
matched to the quantum efficiency curve (for definition see above) of the PMT. To detect
the fast scintillation component of BaF 2 for example, it is necessary to use a
PMT with quartz window since glass absorbs all light below 280 nm. Fig.
4.2 shows the quantum efficiency (Q.E.) of a standard PMT with a bialkali
photocathode. The emission spectrum of the most common scintillator NaI(Tl) is shown too.
It can be seen that the overlap is very good. For other scintillation materials such as
BGO, the match is less ideal.
The gain of a PMT is temperature
sensitive. The variation in gain, which depends on the photocathode and dynode material,
amounts to typically a few tenths of a percent per oC.
Due to their dynode stages, PMTs are
usually quite bulky devices although some short versions and miniature types have been
developed.
Care must be taken when PMTs are used
inside magnetic fields. Although there are PMT types that have a high magnetic field
immunity, this effect remains a problem.
The material of a PMT is
usually glass. Glass has an intrinsic amount of 40K which contributes to the radiological
background of the scintillation detector. 40K emits as well 1460 keV gamma
rays as beta particles. The face-plate of the PMT can be constructed of special low-K
glass. Furthermore, this background can be limited by using light guides absorbing the b-particles
and creating a distance between the crystal and the PMT. The above techniques are used in
so-called "low background" scintillation detectors.
Below we would like to summarize the
advantages and disadvantages of PMTs in conjunction with scintillation crystals.
For more information regarding PMTs
we refer to the PMT manufacturer's literature.
Photomultiplier
Tubes
- Advantages:
- Standard device
- Large signals
- Large active areas possible
- Fast rise times possible
- Disadvantages
- Large physical dimension
- High Voltage required
- Gain instability as function of
temperature
- Sensitive to magnetic fields
- Background radiation
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