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474 Quark Models of Mesons and Baryons<br />

Table 15.1: Hadrons. The four lowest-lying multiplets of hadrons are<br />

listed. They give rise to a total of 36 particles. The rest energy is arbitrarily<br />

taken as the central energy of the multiplet.<br />

Spin-parity, Rest Energy Members of Number of<br />

J π (GeV) Type the Multiplet Members<br />

0 − 0.5 Boson πKKηη ′ 9<br />

1− 0.8 Boson ρK∗K ∗ ωφ 9<br />

1 +<br />

2<br />

1.1 Fermion NΛΣΞ 8<br />

3 +<br />

2<br />

1.4 Fermion ∆Σ∗Ξ∗Ω 10<br />

15.3 Hunting the Quark<br />

Do quarks exist? Considerable effort has been spent by many experimental groups<br />

since 1964 to find quarks in nature, but no conclusive positive evidence has yet been<br />

uncovered. Fortunately the fractional electric charges would make quark signatures<br />

in careful experiments unambiguous.<br />

In principle, quarks can be produced by high-energy protons through reactions<br />

of the type<br />

pN −→ NNqq + bosons, pN −→ Nqqq + bosons. (15.1)<br />

The thresholds of these reactions depend on the mass mq of the quarks; the magnitudes<br />

of the cross sections are determined by the forces between the hadrons and<br />

the quarks. (Since neither the forces nor the quark masses are known, the search is<br />

an uncertain affair. If quarks are not found, one never knows if it is because they<br />

do not exist, because their mass is too high, or because the production cross section<br />

is too low.)<br />

The high energies required to produce massive particles are available in the<br />

biggest accelerators, in high-energy colliding beams, and in cosmic rays. Moreover, if<br />

free quarks exist, and if the world was created in a “big bang,” it is likely that quarks<br />

were produced during a very early stage when the temperature was exceedingly high.<br />

Some of these original quarks could still be around; searches in sedimentary rocks<br />

have not found any.<br />

Quarks can be hunted at accelerators (4) and in cosmic rays. Moreover, since at<br />

least one quark must be stable, they should have accumulated in the earth’s crust,<br />

in meteorites, or in moon rocks. Quarks can be distinguished from other particles<br />

either by their fractional charge or by their mass. If the mass is studied, stability is<br />

taken as an additional criterion. If the charge is used as signature, the idea is simple.<br />

Equation (3.2) shows that the energy loss of a particle in matter is proportional to<br />

the square of its charge. A quark of charge e/3 would produce one ninth of the ionization<br />

of a singly charged particle of the same velocity. If the particle is relativistic,<br />

4 M. Banner et al., (UA2 Collaboration) Phys. Lett. 121B, 187 (1983).

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