International
Tables for Crystallography Volume C Mathematical, physical and chemical tables Edited by E. Prince © International Union of Crystallography 2006 |
International Tables for Crystallography (2006). Vol. C. ch. 7.3, pp. 644-645
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The neutron capture and the trajectories of the secondary charged particles as well as the specific gas ionization along these trajectories are presented in Figs. 7.3.3.1(a) and (b) . Since the gas ionization energy is about 30 eV per electron (42 eV for 3He and 30 eV for CH4), there are about 25 000 ion pairs (e−, He+ or e−, ) per captured neutron. Gases such as CH4 or C3H8 are added to diminish the length of the trajectories, i.e. the wall effect [see Subsection 7.3.4.2(b)].
We give in Fig. 7.3.3.1(c) the proton range of an 3He neutron-capture reaction in various gases (Fischer, Radeka & Boie, 1983). A schematic drawing of a gas monodetector, which might be mounted either in axial or in radial orientation in the neutron beam, is given in Fig. 7.3.3.1(d).
For this type of detector, the efficiency as a function of the gas pressure, or gas-detector law, is written as with P(atm) = the detector-gas pressure at 293 K, t(cm) = the gas thickness, and λ(Å) = the detected neutron wavelength. The numerical coefficient b, obtained at 293 K from the ideal gas law, the Avogadro number NA, and the gas absorption cross section σa (barns) at λ0 = 1.8 Å, is
For 3He, with σa = 5333 barns at λ0 = 1.8 Å, b = 0.07417; for 10BF3, with σa = 3837 barns at λ0= 1.8 Å, b = 0.0533. We give in Table 7.3.3.2 a few examples of gas-detector characteristics.
†Value calculated for the diameter.
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There are two modes of operation.
In the case of direct collection of charges, the 25000 electrons corresponding to one neutron capture (primary electrons) are collected by the anode in about 100–500 ns, and generate an input pulse in the charge preamplifier (see Section 7.3.4).
If the electrical field created by the high voltage applied to the anode exceeds a critical value, the electrons will be accelerated sufficiently to produce a cascade of ionizing collisions with the neutral molecules they encounter, the new electrons liberated in the process being called secondary electrons. This phenomenon, gas multiplication, occurs in the vicinity of the thin wire anode, since the field varies as 1/r. The avalanche stops when all the free electrons have been collected at the anode. With proper design, the number of secondary electrons is proportional to the number of primary electrons. For cylindrical geometries, the multiplication coefficient M can be calculated (Wolf, 1974). This type of detection mode is called the proportional mode. It is very commonly used because it gives a better signal-to-noise ratio (see Section 7.3.4).
A few critical remarks about gas detectors:
References
Convert, P. & Forsyth, J. B. (1983). Position-sensitive detection of thermal neutrons: Part 1, Introduction. Position-sensitive detection of thermal neutrons, pp. 1–90. London: Academic Press.Google ScholarFischer, J., Radeka, V. & Boie, R. A. (1983). High position resolution and accuracy in 3He two-dimensional thermal neutron PSDs. Position-sensitive detection of thermal neutrons, edited by P. Convert & J. B. Forsyth, pp. 129–140. London: Academic Press.Google Scholar
Whaling, W. (1958). The energy loss of charged particles in matter. Handbuch der Physik, Vol. 34. Corpuscles and radiation in matter II, edited by S. Flugge, pp. 193–217. Berlin: Springer-Verlag.Google Scholar
Wolf, R. S. (1974). Measurement of the gas constants for various proportional counter gas mixtures. Nucl. Instrum. Methods, 115, 461–463.Google Scholar