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Argonne PowerPoint Presentation - Spallation Neutron Source

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<strong>Spallation</strong>-Evaporation<br />

Production of <strong>Neutron</strong>s<br />

Original<br />

Nucleus<br />

Excited<br />

Nucleus<br />

Residual<br />

Radioactive<br />

Nucleus<br />

Ep<br />

Proton<br />

~10 –20 sec<br />

> 1 sec<br />

~<br />

‘<br />

‘<br />

‘<br />

e<br />

γ<br />

‘<br />

‘<br />

‘<br />

‘<br />

‘<br />

γ<br />

Recoiling particles<br />

remaining in nucleus<br />

‘<br />

‘<br />

e<br />

‘<br />

γ<br />

Emerging “Cascade” Particles<br />

(high energy, ~ E < Ep) (n, p. π, …)<br />

(These may collide with other<br />

nuclei with effects similar to<br />

that of the original proton<br />

collision.)<br />

Evaporating Particles<br />

(Low energy, E ~ 1–10 MeV);<br />

(n, p, d, t, … (mostly n)<br />

and γ rays and electrons.)<br />

Electrons (usually e + )<br />

and gamma rays due to<br />

radioactive decay.<br />

19

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