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5.3. Mass Measurements 89<br />

Figure 5.7: Aston’s mass spectrometer.<br />

short-lived isotopes, (9) an issue of great importance to understand the production<br />

of elements in stars (see Chapter 19.)<br />

Mass spectroscopy works well for nuclei, but it is difficult (or impossible) to<br />

apply to most particles. In the mass spectrometer, all ions start with a very small<br />

(thermal) velocity and are accelerated in the same field. Their relative masses<br />

can therefore be determined very accurately. However, particles are produced in<br />

reactions, and their initial velocities are not accurately known. Moreover, some of<br />

the particles are neutral and cannot be deflected. Different approaches are necessary,<br />

and they are based on Eqs. (1.2) and (1.7):<br />

p = mγv<br />

(1.2)<br />

(1.7)<br />

E 2 = p 2 c 2 + m 2 c 4<br />

γ =<br />

1<br />

(1 − (v/c) 2 . (1.6)<br />

) 1/2<br />

These relations show that the mass of a particle can be computed if momentum<br />

and energy or momentum and velocity are known. Many techniques are based on<br />

this fact, and the arrangement shown in Fig. 5.8 provides an example. A magnet<br />

selects particles with momentum p. Two scintillation counters, S1 and S2, record<br />

the passage of a particle. The time delay between pulses S2 and S1 can be measured<br />

and, with the distance between S1 and S2 known, the velocity can be computed.<br />

Together, momentum and velocity give the mass.<br />

The method just discussed fails if the particle is neutral or if its life-time is so<br />

9 These techniques have been brought to a fine point by H.-J. Kluge and collaborators, see K.<br />

Blaum, Phys. Rep. 425, 1 (2006).

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