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Subatomic Physics

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164 Structure of <strong>Subatomic</strong> Particles<br />

6.9 Deep Inelastic Electron Scattering<br />

The Thomson model of the atom, in vogue before 1911, assumed that the positive<br />

and negative charges were distributed uniformly throughout the atom. Rutherford’s<br />

scattering experiment (1) proved that one charge is concentrated in the nucleus; this<br />

discovery profoundly affected atomic physics and founded nuclear physics. Highly<br />

inelastic electron scattering has had a similar impact on particle physics and we<br />

consequently discuss the most surprising results of these experiments here.<br />

In deep inelastic scattering, usually only the energies and momenta of the initial<br />

and final electron are observed, but not the particles produced from the target.<br />

These measurements result in what is often called inclusive cross sections. Nevertheless<br />

some kinematical information about the final hadronic state can be gleaned.<br />

Energy and momentum conservation give for the energy E ′ h and momentum p′ h of<br />

the final hadrons in the laboratory system (see Fig. 6.15)<br />

E ′ h = ν + mc2 , p ′ h = p − p′ , (6.53)<br />

where m is the mass of the struck particle. In terms of E ′ h and p′ h ,orq and ν one<br />

can define the relativistically invariant effective mass, W , of all the hadrons in the<br />

final state<br />

W 2 = E ′2<br />

h − (p ′ hc) 2 = m 2 c 4 + q 2 c 2 +2νmc 2 . (6.54)<br />

Since q2 and W 2 are relativistic scalars or invariants, Eq. (6.54) makes it clear that<br />

ν is also a Lorentz invariant, and therefore has the same value in any frame of<br />

reference. Indeed, we can write ν in terms of the target particle’s energy Eh and<br />

momentum p (32)<br />

h<br />

ν = ph · q<br />

m =<br />

�<br />

Ehq0<br />

mc2 − p �<br />

h · q<br />

, (6.55)<br />

m<br />

which makes its Lorentz invariance manifest.<br />

At different scattering angles, what energies E ′ should be selected? The answer<br />

can be obtained from elastic scattering and inelastic scattering to resonances: elastic<br />

scattering corresponds to looking at a final state with W = mc 2 ; observation of a<br />

resonance means selecting a final state with W = mresc 2 ,wheremres is the mass of<br />

the resonance. W characterizes the total mass of the hadrons in the final state here<br />

also, and the cross section d 2 σ/dE ′ dΩ for the continuum is consequently determined<br />

as a function of q 2 for a fixed value of W .<br />

Inelastic electron–proton scattering into the continuum has been studied both<br />

at medium energies (E ∼ 0.5−4 GeV) on nuclei and with high energy electrons and<br />

positrons. (45) At SLAC the primary electron energy was varied between about 4.5<br />

and 24 GeV; ν reachedvaluesashighas15GeVand|q 2 | over 20(GeV/c) 2 .Atthe<br />

45 A. Abramowicz and A.C. Caldwell, Rev Mod. Phys. 71, 1275 (1999).

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